View source for List of multiplanetary systems

{{Short description|List of systems with multiple planets}}
{{Further|Planetary system}}

[[File:Confirmed exoplanets by methods EPE.svg|right|thumb|350px|Number of extrasolar planet discoveries per year through 2023. Colors indicate method of detection.
{{Col-begin}}
{{Col-break}}
{{legend|#1f77b4|[[Methods of detecting exoplanets#Direct imaging|Direct imaging]]}}
{{legend|#ff7f0e|[[Gravitational microlensing]]}}
{{legend|#9467bd|[[Methods of detecting exoplanets#Pulsar timing|Pulsar timing]]}}
{{legend|#d62728|[[Doppler spectroscopy|Radial velocity]]}}
{{legend|#2ca02c|[[Methods of detecting exoplanets#Transit photometry|Transit photometry]]}}
{{col-end}}
]]

From the total of {{Extrasolar planet counts|system_count}} stars known to have [[exoplanet]]s (as of {{Extrasolar planet counts|asof|mdy}}), there are a total of {{Extrasolar planet counts|multiplanetsystem_count}} known multiplanetary systems,<ref name="Encyclopaedia">{{cite encyclopedia |title=Interactive Extra-solar Planets Catalog |url=https://exoplanet.eu/catalog/ |last=Schneider |first=Jean |date=6 December 2016 |encyclopedia=[[Extrasolar Planets Encyclopaedia]] |access-date=2016-12-06 |archive-date=2016-12-09 |archive-url=https://web.archive.org/web/20161209220644/http://exoplanet.eu/catalog/ |url-status=live }}</ref> or stars with at least two confirmed planets, beyond the [[Solar System]]. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are the [[Sun]] (the Solar System's star) and [[Kepler-90]], with 8 confirmed planets each, followed by [[TRAPPIST-1]] with 7 planets.

The {{Extrasolar planet counts|multiplanetsystem_count}} multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has at least one planet (the confirmed [[Proxima Centauri b|b]], along with the candidate [[Proxima Centauri d|d]] and the disputed [[Proxima Centauri c|c]]<ref name="Artigau2022"/>). The nearest system with four or more confirmed planets is [[Barnard Star]], with four known.<ref name="Basant2025"></ref> The farthest confirmed system with two or more planets is [[Optical Gravitational Lensing Experiment#Planets discovered|OGLE-2012-BLG-0026L]], at {{convert|13,300|ly|pc}} away.<ref>{{Cite web |first1=Jean-Philippe |last1=Beaulieu |first2=D. P. |last2=Bennett |first3=Virginie |last3=Batista |first4=A. |last4=Fukui |date=January 2016 |title=Revisiting the microlensing event OGLE 2012-BLG-0026: A solar mass star with two cold giant planets |url=https://www.researchgate.net/publication/290028818 |website=researchgate.net }}</ref>

The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. The two most important [[list of stellar properties|stellar properties]] are [[mass]] and [[metallicity]] because they determine how these [[planetary system]]s form. Systems with higher mass and metallicity tend to have more planets and more massive planets. However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close-in planets, orbiting at less than 1 [[Astronomical unit|AU]].<ref name="JMBrewer2018">{{cite journal |last1=Brewer |first1=John M. |last2=Wang |first2=Songhu |last3=Fischer |first3=Debra A. |last4=Foreman-Mackey |first4=Daniel |title=Compact multi-planet systems are more common around metal poor hosts|journal=The Astrophysical Journal |volume=867 |at=L3 |arxiv=1810.10009 |doi=10.3847/2041-8213/aae710 |date=2018-10-24 |issue=1 |bibcode=2018ApJ...867L...3B |s2cid=67832557 |doi-access=free }}</ref>

==Multiplanetary systems==
{{Dynamic list}}
<div style="float: left; margin: 5px;">
{| class="wikitable"
|-
! style="background: #eaeaea" colspan=8|Color indicates number of planets
|-
| bgcolor="#fdfdfd" width=30 style="text-align: center" |2 (x)
| bgcolor="#cddafb" width=30 style="text-align: center" |3
| bgcolor="#aaeee9" width=30 style="text-align: center" |4
| bgcolor="#90e090" width=30 style="text-align: center" |5
| bgcolor="#ccdd66" width=30 style="text-align: center" |6
| bgcolor="#e0c066" width=30 style="text-align: center" |7
| bgcolor="#f08a6c" width=30 style="text-align: center" |8
| bgcolor="#f76879" width=30 style="text-align: center" |9
|}</div>
<!------ Stars with only one planet should not be added here, but at [[List of exoplanetary host stars]] instead --->
{{clear}}
{{Multiplanetary systems list/Top}}
{{Multiplanetary systems list
  |               Star = Sun
  |      Constellation = -
  |    Right ascension = -
  |        Declination = -
  | Apparent magnitude = −26.74
  |           Distance = 0.000016
  |      Spectral type = G2V
  |               Mass = 1.000
  |             Radius = 1.000
  |        Temperature = 5778
  |        Metallicity = 0.000
  |                Age = 4.572
  |  Confirmed planets = 8
  |Unconfirmed planets = 1
  |              Notes = [[Pluto]] was considered a planet before [[IAU definition of planet|2006]]. The hypothesised [[Planet Nine]] remains unconfirmed.
}}
{{Multiplanetary systems list
  |               Star = Proxima Centauri
  |      Constellation = Centaurus
  |    Right ascension = {{RA|14|29|42.94853}}
  |        Declination = {{DEC|−62|40|46.1631}}
  | Apparent magnitude = 10.43 to 11.11<ref name="VizieRproximac">{{cite journal |bibcode=2009yCat....102025S |title=VizieR online data catalog: General catalogue of variable stars (Samus+ 2007–2013) |journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S |volume=1 |display-authors=etal |last1=Samus |first1=N. N. |last2=Durlevich |first2=O. V. |year=2009}}</ref>
  |           Distance = 4.244
  |      Spectral type = M5.5Ve<ref>{{cite journal |bibcode=1991AJ....101..662B |title=The late-M dwarfs |journal=The Astronomical Journal |volume=101 |pages=662 |last1=Bessell |first1=M. S. |year=1991 |doi=10.1086/115714|doi-access=free }}</ref>
  |               Mass = 0.1221
  |             Radius = 0.1542
  |        Temperature = 3042
  |        Metallicity = 0.21
  |                Age = 4.85
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              Notes = Closest star to the Sun and closest star to the Sun with a multiplanetary system. Planet b is potentially habitable.<ref name=ProximaESPRESSO>{{cite journal |last1=Mascareño |first1=A. Suárez |last2=Faria |first2=J. P. |last3=Figueira |first3=P. |last4=Lovis |first4=C. |last5=Damasso |first5=M. |last6=Hernández |first6=J. I. González |last7=Rebolo |first7=R. |last8=Cristiani |first8=S. |last9=Pepe |first9=F. |last10=Santos |first10=N. C. |last11=Osorio |first11=M. R. Zapatero |last12=Adibekyan |first12=V. |last13=Hojjatpanah |first13=S. |last14=Sozzetti |first14=A. |last15=Murgas |first15=F. |last16=Abreu |first16=M. |last17=Affolter |first17=M. |last18=Alibert |first18=Y. |last19=Aliverti |first19=M. |last20=Allart |first20=R. |last21=Prieto |first21=C. Allende |last22=Alves |first22=D. |last23=Amate |first23=M. |last24=Avila |first24=G. |last25=Baldini |first25=V. |last26=Bandi |first26=T. |last27=Barros |first27=S. C. C. |last28=Bianco |first28=A. |last29=Benz |first29=W. |last30=Bouchy |first30=F. |last31=Broeng |first31=C. |last32=Cabral |first32=A. |last33=Calderone |first33=G. |last34=Cirami |first34=R. |last35=Coelho |first35=J. |last36=Conconi |first36=P. |last37=Coretti |first37=I. |last38=Cumani |first38=C. |last39=Cupani |first39=G. |last40=D’Odorico |first40=V. |last41=Deiries |first41=S. |last42=Delabre |first42=B. |last43=Marcantonio |first43=P. Di |last44=Dumusque |first44=X. |last45=Ehrenreich |first45=D. |last46=Fragoso |first46=A. |last47=Genolet |first47=L. |last48=Genoni |first48=M. |last49=Santos |first49=R. Génova |last50=Hughes |first50=I. |last51=Iwert |first51=O. |last52=Kerber |first52=F. |last53=Knusdstrup |first53=J. |last54=Landoni |first54=M. |last55=Lavie |first55=B. |last56=Lillo-Box |first56=J. |last57=Lizon |first57=J. |last58=Curto |first58=G. Lo |last59=Maire |first59=C. |last60=Manescau |first60=A. |last61=Martins |first61=C. J. a. P. |last62=Mégevand |first62=D. |last63=Mehner |first63=A. |last64=Micela |first64=G. |last65=Modigliani |first65=A. |last66=Molaro |first66=P. |last67=Monteiro |first67=M. A. |last68=Monteiro |first68=M. J. P. F. G. |last69=Moschetti |first69=M. |last70=Mueller |first70=E. |last71=Nunes |first71=N. J. |last72=Oggioni |first72=L. |last73=Oliveira |first73=A. |last74=Pallé |first74=E. |last75=Pariani |first75=G. |last76=Pasquini |first76=L. |last77=Poretti |first77=E. |last78=Rasilla |first78=J. L. |last79=Redaelli |first79=E. |last80=Riva |first80=M. |last81=Tschudi |first81=S. Santana |last82=Santin |first82=P. |last83=Santos |first83=P. |last84=Segovia |first84=A. |last85=Sosnowska |first85=D. |last86=Sousa |first86=S. |last87=Spanò |first87=P. |last88=Tenegi |first88=F. |last89=Udry |first89=S. |last90=Zanutta |first90=A. |last91=Zerbi |first91=F. |title=Revisiting Proxima with ESPRESSO |journal=Astronomy & Astrophysics |date=1 July 2020 |volume=639 |pages=A77 |doi=10.1051/0004-6361/202037745 |arxiv=2005.12114 |bibcode=2020A&A...639A..77S |s2cid=218869742 |url=https://www.aanda.org/articles/aa/abs/2020/07/aa37745-20/aa37745-20.html |language=en |issn=0004-6361 |access-date=9 May 2022 |archive-date=27 June 2022 |archive-url=https://web.archive.org/web/20220627141045/https://www.aanda.org/articles/aa/abs/2020/07/aa37745-20/aa37745-20.html |url-status=live }}</ref><ref>{{cite journal |last1=Del Genio |first1=Anthony D. |last2=Way |first2=Michael J. |last3=Amundsen |first3=David S. |last4=Aleinov |first4=Igor |last5=Kelley |first5=Maxwell |last6=Kiang |first6=Nancy Y. |last7=Clune |first7=Thomas L. |title=Habitable Climate Scenarios for Proxima Centauri b with a Dynamic Ocean |journal=Astrobiology |date=January 2019 |volume=19 |issue=1 |pages=99–125 |doi=10.1089/ast.2017.1760 |pmid=30183335 |arxiv=1709.02051 |bibcode=2019AsBio..19...99D |s2cid=52165056 |url=https://www.liebertpub.com/doi/full/10.1089/ast.2017.1760 |issn=1531-1074}}</ref> Planet c initially appeared likely but has since been disputed.<ref name="Artigau2022">{{cite journal|last1=Artigau|first1=Étienne|last2=Cadieux|first2=Charles|last3=Cook|first3=Neil J.|last4=Doyon|first4=René|last5=Vandal|first5=Thomas|last6=Donati|first6=Jean-Françcois|last7=Moutou|first7=Claire|last8=Delfosse|first8=Xavier|last9=Fouqué|first9=Pascal|last10=Martioli|first10=Eder|last11=Bouchy|first11=François|last12=Parsons|first12=Jasmine|last13=Carmona|first13=Andres|last14=Dumusque|first14=Xavier|last15=Astudillo-Defru|first15=Nicola|last16=Bonfils|first16=Xavier|last17=Mignon|first17=Lucille|display-authors=5|title=Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry|journal=The Astronomical Journal|volume=164:84|issue=3|pages=18pp|arxiv=2207.13524|bibcode=2022AJ....164...84A|doi=10.3847/1538-3881/ac7ce6|doi-access=free|date=June 23, 2022|publication-date=August 8, 2022}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Barnard's Star
  |      Constellation = Ophiuchus
  |    Right ascension = {{RA|17|57|48.4985}}
  |        Declination = {{DEC|+04|41|36.1139}}
  | Apparent magnitude = 9.511
  |           Distance = 5.96
  |      Spectral type = M4.0V<ref name=Gizisz>{{cite journal|bibcode=1997AJ....113..806G|title=M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale|journal=[[The Astronomical Journal]]|volume=113|issue=2|pages=806–822|last=Gizis|first=John E. |date=February 1997|doi=10.1086/118302|arxiv=astro-ph/9611222|s2cid=16863021}}</ref>
  |               Mass = 0.162
  |             Radius = 0.187
  |        Temperature = 3195
  |        Metallicity = -0.56
  |                Age = 10
  |  Confirmed planets = 4
  |Unconfirmed planets = 0
  |              Notes = Closest single star to the Sun with a confirmed multiplanetary system.<ref name="Basant2025">{{cite journal |last1=Basant |first1=Ritvik |last2=Luque |first2=Rafael |display-authors=etal |date=March 2025 |title=Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO |journal=[[The Astrophysical Journal Letters]] |volume=982 |issue=|pages=L1 |doi=10.3847/2041-8213/adb8d5 |doi-access=free |arxiv=2503.08095}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Lalande 21185
  |      Constellation = Ursa Major
  |    Right ascension = {{RA|11|03|20.1940}}
  |        Declination = {{DEC|+35|58|11.5682}}
  | Apparent magnitude = 7.520<ref name=aaass61>{{citation | last=Oja | first=T. | title=Photoelectric photometry of stars near the north Galactic pole. II | journal=Astronomy and Astrophysics Supplement Series | volume=61 | pages=331–339 |date=August 1985 | bibcode=1985A&AS...61..331O }}</ref>
  |           Distance = 8.3044{{±|0.0007}}
  |      Spectral type = M2V
  |               Mass = 0.390
  |             Radius = 0.392{{±|0.004}}
  |        Temperature = 3601{{±|51}}
  |        Metallicity = -0.09{{±|0.16}}
  |                Age = 8.047
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              Notes = Brightest [[red dwarf]] star in the northern celestial hemisphere.<ref>{{cite web
 | url =http://www.universetoday.com/111716/14-red-dwarf-stars-to-view-with-backyard-telescopes/
 | title =14 Red Dwarf Stars to View with Backyard Telescopes
 | last =Dickinson
 | first =David
 | date =2015-12-23
 | publisher =Universe Today
 | access-date =2016-12-04
 | archive-date =2021-02-11
 | archive-url =https://web.archive.org/web/20210211185356/https://www.universetoday.com/111716/14-red-dwarf-stars-to-view-with-backyard-telescopes/
 | url-status =live
 }}</ref><ref>{{cite web
 | url =http://kencroswell.com/thebrightestreddwarf.html
 | title =The Brightest Red Dwarf
 | last =Croswell
 | first =Ken
 | date =July 2002
 | website =KenCroswell.com
 | access-date =2016-12-04
 | archive-date =2018-10-20
 | archive-url =https://web.archive.org/web/20181020223954/http://www.kencroswell.com/thebrightestreddwarf.html
 | url-status =live
 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Lacaille 9352
  |      Constellation = Piscis Austrinus
  |    Right ascension = {{RA|23|05|52.04}}
  |        Declination = {{DEC|−35|51|11.05}}
  | Apparent magnitude = 7.34
  |           Distance = 10.721
  |      Spectral type = M0.5V
  |               Mass = 0.486
  |             Radius = 0.47{{±|0.001}}
  |        Temperature = 3688{{±|86}}
  |        Metallicity = -0.06{{±|0.08}}
  |                Age = 4.57
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              Notes = The unconfirmed planet d is potentially habitable.<ref name="Jeffers Dreizler Barnes Haswell pp. 1477–1481">{{citation |arxiv=2006.16372 |title=A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887 |year=2020 |doi=10.1126/science.aaz0795 |last1=Jeffers |first1=S. V. |last2=Dreizler |first2=S. |last3=Barnes |first3=J. R. |last4=Haswell |first4=C. A. |last5=Nelson |first5=R. P. |last6=Rodríguez |first6=E. |last7=López-González |first7=M. J. |last8=Morales |first8=N. |last9=Luque |first9=R. |last10=Zechmeister |first10=M. |last11=Vogt |first11=S. S. |last12=Jenkins |first12=J. S. |last13=Pallé |first13=E. |last14=Berdi Ñas |first14=Z. M.|last15=Coleman |first15=G. A. L. |last16=Díaz |first16=M. R. |last17=Ribas |first17=I. |last18=Jones |first18=H. R. A.|last19=Butler |first19=R. P. |last20=Tinney |first20=C. G. |last21=Bailey |first21=J. |last22=Carter |first22=B. D. |last23=o'Toole |first23=S. |last24=Wittenmyer |first24=R. A. |last25=Crane |first25=J. D. |last26=Feng |first26=F. |last27=Shectman |first27=S. A. |last28=Teske |first28=J. |last29=Reiners |first29=Ansgar |last30=Amado |first30=P. J.|s2cid=220075207 |journal=Science |volume=368 |issue=6498 |pages=1477–1481 |pmid=32587019 |bibcode=2020Sci...368.1477J |display-authors=9}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Luyten's Star
  |      Constellation = Canis Minor
  |    Right ascension = {{RA|07|27|24.4991}}
  |        Declination = {{DEC|05|13|32.827}}
  | Apparent magnitude = 9.872
  |           Distance = 11.20
  |      Spectral type = M3.5V
  |               Mass = 0.26
  |             Radius = 0.35
  |        Temperature = 3150
  |        Metallicity = -0.16
  |                Age = 
  |  Confirmed planets = 2
  |Unconfirmed planets = 2
  |              Notes = Stellar activity level and rotational rate suggest an age higher than 8 billion years.<ref name="PozuelosSuárez2020">{{cite journal
 |last1=Pozuelos |first1=Francisco J.  |last2=Suárez    |first2=Juan C.
 |last3=de Elía  |first3=Gonzalo C.    |last4=Berdiñas  |first4=Zaira M.
 |last5=Bonfanti |first5=Andrea        |last6=Dugaro    |first6=Agustín
 |last7=Gillon   |first7=Michaël       |last8=Jehin     |first8=Emmanuël
 |last9=Günther  |first9=Maximilian N. |last10=van&nbsp;Grootel |first10=Valérie
 |last11=Garcia  |first11=Lionel J.    |last12=Thuillier |first12=Antoine
 |last13=Delrez  |first13=Laetitia     |last14=Rodón     |first14=Jose R.
 |display-authors=6
 |year=2020
 |title=GJ&nbsp;273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M&nbsp;dwarf at 3.75&nbsp;parsec
 |journal=Astronomy & Astrophysics
 |volume=641  |pages=A23
 |doi=10.1051/0004-6361/202038047 |arxiv=2006.09403
 |bibcode=2020A&A...641A..23P |s2cid=219721292 |quote=<span style="font-family:LatinModern;">GJ 273 is a planetary system orbiting an M&nbsp;dwarf only 3.75&nbsp;pc away, composed of two confirmed planets, GJ&nbsp;273b and GJ&nbsp;273c, and two promising candidates, GJ&nbsp;273d and GJ&nbsp;273e ... the system remained stable only for values of inclinations ranging from 90◦ to ~72◦</span>
}}
</ref> Planet b is potentially habitable.<ref name="arxiv.org_Gliese3293">{{cite journal
 |doi             = 10.1051/0004-6361/201630153
 |last1           = Astudillo-Defru
 |first1          = Nicola
 |last2           = Forveille
 |first2          = Thierry
 |last3           = Bonfils
 |first3          = Xavier
 |last4           = Ségransan
 |first4          = Damien
 |last5           = Bouchy
 |first5          = François
 |last6           = Delfosse
 |first6          = Xavier
 |last7           = Lovis
 |first7          = Christophe
 |last8           = Mayor
 |first8          = Michel
 |last9           = Murgas
 |first9          = Felipe
 |last10          = Pepe
 |first10         = Francesco
 |last11          = Santos
 |first11         = Nuno C.
 |last12          = Udry
 |first12         = Stéphane
 |last13          = Wünsche
 |first13         = Anaël
 |display-authors = 6
 |year            = 2017
 |title           = The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M&nbsp;dwarfs GJ&nbsp;3138, GJ&nbsp;3323, GJ&nbsp;273, GJ&nbsp;628, and GJ&nbsp;3293
 |journal         = Astronomy and Astrophysics
 |volume          = 602
 |at              = A88
 |arxiv           = 1703.05386
 |bibcode         = 2017A&A...602A..88A
 |s2cid           = 119418595
 |url             = https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
 |access-date     = 2022-02-25
 |archive-date    = 2022-09-28
 |archive-url     = https://web.archive.org/web/20220928032005/https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
 |url-status      = live
}}</ref>
}}
{{Multiplanetary systems list
  |               Star = YZ Ceti
  |      Constellation = Cetus
  |    Right ascension = {{RA|01|12|30.64}}
  |        Declination = {{DEC|−16|59|56.3}}
  | Apparent magnitude = 12.07
  |           Distance = 11.74
  |      Spectral type = M4.5V
  |               Mass = 0.13
  |             Radius = 0.168
  |        Temperature = 3056
  |        Metallicity = -0.26
  |                Age = 4.0
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes = Flare star.<ref name=gcvsyzceti>{{cite journal|bibcode=2009yCat....102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Gliese 1061
  |      Constellation = Horologium (constellation){{!}}Horologium
  |    Right ascension = {{RA|03|35|59.69}}
  |        Declination = {{DEC|-44|30|45.3}}
  | Apparent magnitude = 13.03
  |           Distance = 12.04
  |      Spectral type = M5.5V
  |               Mass = 0.113
  |             Radius = 
  |        Temperature = 2953
  |        Metallicity = -0.09
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Planets c and d are potentially habitable.<ref name=angladaescude2019>{{Cite journal |journal=[[Monthly Notices of the Royal Astronomical Society]]
|last1=Dreizler |first1=S.
|last2=Jeffers |first2=S. V.
|last3=Rodríguez |first3=E.
|last4=Zechmeister |first4=M.
|last5=Barnes |first5 = J.R.
|last6=Haswell |first6=C.A.
|last7=Coleman |first7=G. A. L.
|last8=Lalitha |first8=S.
|last9=Hidalgo Soto |first9=D.
|last10=Strachan |first10=J.B.P.
|last11=Hambsch |first11=F-J.
|last12=López-González |first12=M. J.
|last13=Morales |first13=N.
|last14=Rodríguez López |first14=C.
|last15=Berdiñas |first15=Z. M.
|last16=Ribas |first16=I.
|last17=Pallé |first17=E.
|last18=Reiners |first18=Ansgar
|last19=Anglada-Escudé |first19=G.
|date=2019-08-13 |title=Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061 |volume=493 |issue=1 |pages=536–550 |doi=10.1093/mnras/staa248 |doi-access=free |arxiv=1908.04717| s2cid=199551874 |language=en}}</ref>
}} 
{{Multiplanetary systems list
  |               Star = [[Teegarden's Star]]
  |      Constellation = Aries (constellation){{!}}Aries
  |    Right ascension = {{RA|02|53|00.89}}
  |        Declination = {{DEC|+16|52|53}}
  | Apparent magnitude = 15.13
  |           Distance = 12.497
  |      Spectral type = M7V
  |               Mass = 0.097
  |             Radius = 0.120
  |        Temperature = 3034
  |        Metallicity = -0.11±0.28
  |                Age = 8
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = Teegarden's Star b and Teegarden's Star c are likely Earth-mass planets that orbit in the habitable zone.<ref name="CARMENES">{{cite journal |last1=Caballero |first1=J. A. |last2=Reiners |first2=Ansgar |last3=Ribas |first3=I. |last4=Dreizler |first4=S. |last5=Zechmeister |first5=M. |display-authors=etal |date=12 June 2019 |title=The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star |journal=Astronomy & Astrophysics |volume=627 |pages=A49 |language=en |doi=10.1051/0004-6361/201935460 |arxiv=1906.07196 |issn=0004-6361 |bibcode=2019A&A...627A..49Z |s2cid=189999121 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Wolf 1061
  |      Constellation = Ophiuchus (constellation){{!}}Ophiuchus
  |    Right ascension = {{RA|16|30|18.0584}}
  |        Declination = {{DEC|-12|39|45.325}}
  | Apparent magnitude = 10.07
  |           Distance = 14.050 ± 0.002 
  |      Spectral type = M3.5V
  |               Mass = 0.294
  |             Radius = 0.307
  |        Temperature = 3342
  |        Metallicity = -0.09
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Planet c is potentially habitable.<ref name="unswpaper">{{cite journal |last1=Davison |first1=Cassy L. |last2=White |first2=Russel J. |last3=Henry |first3=Todd J. |last4=Riedel |first4=Adric R. |last5=Jao |first5=Wei-Chun |last6=Bailey III |first6=John I. |last7=Quinn |first7=Samuel N. |last8=Justin R. |first8=Cantrell |last9=John P. |first9=Subasavage |last10=Jen G. |first10=Winters  |title=A 3D Search for Companions to 12 Nearby M-Dwarfs |year=2015 |arxiv=1501.05012 |doi=10.1088/0004-6256/149/3/106 |volume=149 |issue=3 |journal=The Astronomical Journal |page=106|bibcode = 2015AJ....149..106D |s2cid=9719725 }}</ref><ref>{{cite web|author=Stuart Gary|url=http://www.abc.net.au/news/2015-12-17/nearest-habitable-zone-superearth-terrestrial-planet-wolf1061/7033824|title=Potentially habitable super-Earth discovered orbiting star 14 light years from Earth|publisher=ABC News (Australia)|date=17 December 2015|access-date=2022-05-10|archive-date=2017-06-09|archive-url=https://web.archive.org/web/20170609122527/http://www.abc.net.au/news/science/2015-12-17/nearest-habitable-zone-superearth-terrestrial-planet-wolf1061/7033824|url-status=live}}</ref><ref name=Wolf1061kane>{{citation
 | title=Characterization of the Wolf 1061 Planetary System
 | last1=Kane | first1=Stephen R. | last2=von Braun | first2=Kaspar
 | last3=Henry | first3=Gregory W. | last4=Waters | first4=Miranda A.
 | last5=Boyajian | first5=Tabetha S. | last6=Mann | first6=Andrew W.	
 | journal=The Astrophysical Journal | display-authors=1
 | volume=835 | issue=2 | id=200 | pages=9 | date=February 2017
 | doi=10.3847/1538-4357/835/2/200 | bibcode=2017ApJ...835..200K
 | arxiv=1612.09324 | s2cid=30738573 | postscript=. | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Gliese 876
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|53|16.73}}
  |        Declination = {{DEC|−14|15|49.3}}
  | Apparent magnitude = 10.17
  |           Distance = 15.25
  |      Spectral type = M4V
  |               Mass = 0.334
  |             Radius = 0.356
  |        Temperature = 3348
  |        Metallicity = 0.054
  |                Age = 4.893
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Planet b is a gas giant which orbits in the habitable zone.<ref name="Jones2005Gliese876">{{cite journal | title=Prospects for Habitable "Earths" in Known Exoplanetary Systems | last1=Jones | first1=Barrie W. | last2=Underwood | first2=David R. | last3=Sleep | first3=P. Nick | display-authors=1 | journal=The Astrophysical Journal | volume=622 | issue=2 | pages=1091–1101 | year=2005 | arxiv=astro-ph/0503178 | bibcode=2005ApJ...622.1091J | bibcode-access=free | doi=10.1086/428108 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = 82 G. Eridani
  |      Constellation = Eridanus (constellation){{!}}Eridanus
  |    Right ascension = {{RA|03|19|55.65}}
  |        Declination = {{DEC|−43|04|11.2}}
  | Apparent magnitude = 4.254
  |           Distance = 19.71
  |      Spectral type = G8V
  |               Mass = 0.70
  |             Radius = 0.92
  |        Temperature = 5401
  |        Metallicity = −0.40
  |                Age = 5.76
  |  Confirmed planets = 3
  |Unconfirmed planets = 3
  |              Notes = This star also has a dust disk<ref name="82Gdisk">{{cite journal | display-authors=1
 |last1=Wyatt |first1=M. C. |last2=Kennedy |first2=G. |last3=Sibthorpe |first3=B. |last4=Moro-Martín |first4=A. |last5=Lestrade |first5=J.-F. |last6=Ivison |first6=R. J. |last7=Matthews |first7=B. |last8=Udry |first8=S. |last9=Greaves |first9=J. S. |last10=Kalas |first10=P. |last11=Lawler |first11=S. |last12=Su |first12=K. Y. L. |last13=Rieke |first13=G. H. |last14=Booth |first14=M. |last15=Bryden |first15=G. |last16=Horner |first16=J. |last17=Kavelaars |first17=J. J. |last18=Wilner |first18=D.
 |date = 2012 | journal=[[Monthly Notices of the Royal Astronomical Society]]
 |volume=424 |issue=2 |pages=1206 |title = Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems
 |arxiv = 1206.2370 | doi=10.1111/j.1365-2966.2012.21298.x
 |doi-access=free |bibcode=2012MNRAS.424.1206W |s2cid=54056835 }}</ref> with a semi-major axis at approximately 19 AU.<ref name="Kennedy_2015">{{Cite journal | doi = 10.1093/mnras/stv511| title = Kuiper belt structure around nearby super-Earth host stars| journal = Monthly Notices of the Royal Astronomical Society| volume = 449| issue = 3| pages = 3121| year = 2015| last1 = Kennedy | first1 = G. M.| last2 = Matra | first2 = L.| last3 = Marmier | first3 = M.| last4 = Greaves | first4 = J. S.| last5 = Wyatt | first5 = M. C.| last6 = Bryden | first6 = G.| last7 = Holland | first7 = W.| last8 = Lovis | first8 = C.| last9 = Matthews | first9 = B. C.| last10 = Pepe | first10 = F.| last11 = Sibthorpe | first11 = B.| last12 = Udry | first12 = S.| doi-access = free|arxiv = 1503.02073 |bibcode = 2015MNRAS.449.3121K | s2cid = 53638901}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Gliese 581
  |      Constellation = Libra (constellation){{!}}Libra
  |    Right ascension = {{RA|15|19|26.83}}
  |        Declination = {{DEC|−07|43|20.2}}
  | Apparent magnitude = 10.56
  |           Distance = 20.56
  |      Spectral type = M3V
  |               Mass = 0.311
  |             Radius = 0.378
  |        Temperature = 3484
  |        Metallicity = −0.335
  |                Age = 4.326
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes = The disputed planet d is potentially habitable.<ref name="AstronomyNowGliese581">{{cite news |title=Reanalysis of data suggests 'habitable' planet GJ 581d really could exist |url=http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/ |date=9 March 2015 |work=[[Astronomy Now]] |access-date=27 May 2015 |archive-date=20 May 2015 |archive-url=https://web.archive.org/web/20150520175016/http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/ |url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Gliese 667 C
  |      Constellation = Scorpius
  |    Right ascension = {{RA|17|18|57.16}}
  |        Declination = {{DEC|−34|59|23.14}}
  | Apparent magnitude = 10.20
  |           Distance = 21
  |      Spectral type = M1.5V
  |               Mass = 0.31
  |             Radius = 0.42
  |        Temperature = 3700
  |        Metallicity = −0.59
  |                Age = 2.000
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              Notes = Triple star system - all exoplanets orbit around Star C. Planet c is potentially habitable, and there are more unconfirmed planets.<ref name="Anglada-Escudé-2012">{{cite journal|title=A Planetary System around the nearby M Dwarf GJ 667C with At Least One Super-Earth in Its Habitable Zone|author1=Anglada-Escudé, Guillem |author2=Arriagada, Pamela |author3=Vogt, Steven S. |author4=Rivera, Eugenio J. |author5=Butler, R. Paul |author6=Crane, Jeffrey D. |author7=Shectman, Stephen A. |author8=Thompson, Ian B. |author9=Minniti, Dante |author10=Haghighipour, Nader |author11=Carter, Brad D. |author12=Tinney, C. G. |author13=Wittenmyer, Robert A. |author14=Bailey, Jeremy A. |author15=O'Toole, Simon J. |author16=Jones, Hugh R. A. |author17=Jenkins, James S. |year=2012|journal=The Astrophysical Journal Letters|volume=751|issue=1|pages=<!-- this comment stops Citation bot adding nonexistent page number--> |at= L16|doi=10.1088/2041-8205/751/1/L16|bibcode=2012ApJ...751L..16A|arxiv=1202.0446|s2cid=16531923 }}</ref><ref name="Anglada-Escudé">{{cite journal|title=A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone |url=http://www.eso.org/public/archives/releases/sciencepapers/eso1328/eso1328a.pdf |date=2013-06-07 |author=Anglada-Escudé, Guillem |display-authors=etal |journal=[[Astronomy & Astrophysics]] |doi=10.1051/0004-6361/201321331 |access-date=2013-06-25 |arxiv=1306.6074 |bibcode=2013A&A...556A.126A |volume=556 |pages=A126 |s2cid=14559800 |url-status=dead |archive-url=https://web.archive.org/web/20130630214924/http://www.eso.org/public/archives/releases/sciencepapers/eso1328/eso1328a.pdf |archive-date=2013-06-30 }}</ref><ref>{{Cite journal |doi = 10.1088/0004-637X/780/2/124|title = Dynamical Evolution and Spin-Orbit Resonances of Potentially Habitable Exoplanets. The Case of Gj 667C|journal = The Astrophysical Journal|volume = 780|issue = 2|pages = 124|year = 2013|last1 = Makarov|first1 = Valeri V.|last2 = Berghea|first2 = Ciprian|arxiv = 1311.4831|s2cid = 118700510}}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[HD 219134]]
  |      Constellation = Cassiopeia (constellation){{!}}Cassiopeia
  |    Right ascension = {{RA|23|13|14.74}}
  |        Declination = {{DEC|57|10|03.5}}
  | Apparent magnitude = 5.57
  |           Distance = 21
  |      Spectral type = K3Vvar
  |               Mass = 0.794
  |             Radius = 0.778
  |        Temperature = 4699
  |        Metallicity = 0.11
  |                Age = 12.66
  |  Confirmed planets = 6
  |Unconfirmed planets = 
  |              Notes = Closest star to the Sun with exactly six<ref name="Vogt2015HD219134">{{cite journal |arxiv=1509.07912 |last1=Vogt |first1=Steven S. |display-authors=etal |title=Six Planets Orbiting HD 219134 |date=November 2015 |doi=10.1088/0004-637X/814/1/12 |volume=814 |issue=1 |journal=[[The Astrophysical Journal]] |page=12 |bibcode=2015ApJ...814...12V|s2cid=45438051 }}</ref> exoplanets, and closest [[K-type main sequence star]] to the Sun with a multiplanetary system. One of the oldest stars with a multiplanetary system, although it is still more metal-rich than the Sun. None of the known planets is in the habitable zone.<ref>{{cite journal |author-link= |arxiv=2112.05337 |title= An Integrative Analysis of the HD 219134 Planetary System and the Inner solar system: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria|last1= Dietrich|first1= Jeremy|last2= Apai|first2= Dániel|last3= Malhotra|first3= Renu|journal=The Astronomical Journal |year= 2022|volume=163 |issue=2 |page=88 |doi=10.3847/1538-3881/ac4166 |bibcode=2022AJ....163...88D |s2cid=245117944 |doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = 61 Virginis
  |      Constellation = Virgo (constellation){{!}}Virgo
  |    Right ascension = {{RA|13|18|24.31}}
  |        Declination = {{DEC|−18|18|40.3}}
  | Apparent magnitude = 4.74
  |           Distance = 28
  |      Spectral type = G5V
  |               Mass = 0.954
  |             Radius = 0.945
  |        Temperature = 5531
  |        Metallicity = −0.008
  |                Age = 8.960
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              Notes = Planet d remains unconfirmed,<ref name=debris61Vir>{{Cite journal | last1=Wyatt | first1=M. C. | last2=Kennedy | first2=G. | last3=Sibthorpe | first3=B. | last4=Moro-Martín | first4=A. | last5=Lestrade | first5=J.-F. | last6=Ivison | first6=R. J. | last7=Matthews | first7=B. | last8=Udry | first8=S. | last9=Greaves | first9=J. S. | last10=Kalas | first10=P. | last11=Lawler | first11=S. | last12=Su | first12=K. Y. L. | last13=Rieke | first13=G. H. | last14=Booth | first14=M. | last15=Bryden | first15=G. | last16=Horner | first16=J. | last17=Kavelaars | first17=J. J. | last18=Wilner | first18=D. | display-authors=1 | title=Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems | journal=MNRAS | date=2012 | bibcode = 2012MNRAS.424.1206W | doi = 10.1111/j.1365-2966.2012.21298.x | arxiv=1206.2370 | volume=424 | issue=2 | pages=1206–1223| doi-access=free | s2cid=54056835 }}</ref> and a 2021 study found that it was likely a false positive.<ref name=Rosenthal2021_61VirD>{{cite journal |arxiv=2105.11583|doi=10.3847/1538-4365/abe23c|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|year=2021|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973 |doi-access=free }}</ref> 61 Virginis also has a debris disk.
}}
{{Multiplanetary systems list
  |               Star = [[Gliese 433]]
  |      Constellation = Hydra (constellation){{!}}Hydra
  |    Right ascension = {{RA|11|35|26.9485}}
  |        Declination = {{DEC|-25|10|08.9}}
  | Apparent magnitude = 9.79
  |           Distance = 29.8±0.1
  |      Spectral type = M1.5V
  |               Mass = 0.48
  |             Radius = 0.48±0.01
  |        Temperature = 3550±100
  |        Metallicity = -0.02±0.05
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = An [[infrared excess]] around this star suggests a [[circumstellar disk]].<ref name=Kennedyetal2018Gliese433>{{cite journal
 | title=Kuiper belt analogues in nearby M-type planet-host systems
 | last1=Kennedy | first1=G. M. | last2=Bryden | first2=G.
 | last3=Ardila | first3=D. | last4=Eiroa | first4=C.
 | last5=Lestrade | first5=J. -F. | last6=Marshall | first6=J. P.
 | last7=Matthews | first7=B. C. | last8=Moro-Martin | first8=A.
 | last9=Wyatt | first9=M. C. | display-authors=1
 | journal=Monthly Notices of the Royal Astronomical Society
 | volume=476 | issue=4 | pages=4584–4591 | date=June 2018
 | doi=10.1093/mnras/sty492 | doi-access=free | arxiv=1803.02832
 | bibcode=2018MNRAS.476.4584K }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[Gliese 357]]
  |      Constellation = Hydra (constellation){{!}}Hydra
  |    Right ascension = {{RA|09|36|01.6373}}
  |        Declination = {{DEC|-21|39|38.878}}
  | Apparent magnitude = 10.906
  |           Distance = 30.776
  |      Spectral type = M2.5V
  |               Mass = 0.362
  |             Radius = 0.333
  |        Temperature = 3488
  |        Metallicity = -0.14
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = Planet d is a potentially habitable Super-Earth.<ref>Falconer, Rebecca, ''[https://www.axios.com/super-earth-31-light-years-away-may-support-life-d1d0298d-3c82-4f99-a4af-22774fc1ed70.html Newly uncovered super-Earth 31 light-years away may be habitable] {{Webarchive|url=https://web.archive.org/web/20191218061126/https://www.axios.com/super-earth-31-light-years-away-may-support-life-d1d0298d-3c82-4f99-a4af-22774fc1ed70.html |date=2019-12-18 }}'', Axios, August 1, 2019</ref><ref name="TESSGliese357d">{{Cite web|url=https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|title=TESS Discovers Habitable Zone Planet in GJ 357 System|last1=Reddy|first1=Francis|last2=Center|first2=NASA’s Goddard Space Flight|date=2019-07-31|website=SciTechDaily|language=en-US|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801162521/https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|url-status=live}}</ref><ref>{{Cite web|url=https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|title=Potentially habitable 'super-Earth' discovered just 31 light-years away|website=NBC News|date=31 July 2019|language=en|access-date=2019-08-01|archive-date=2019-07-31|archive-url=https://web.archive.org/web/20190731230808/https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|url-status=live}}</ref><ref>{{Cite web|url=http://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world|title=NASA's TESS Helps Find Intriguing New World|last=Garner|first=Rob|date=2019-07-30|website=NASA|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801045621/https://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world/|url-status=live}}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[L 98-59]]
  |      Constellation = Volans
  |    Right ascension = {{RA|08|18|07.62}}
  |        Declination = {{DEC|-68|18|46.8}}
  | Apparent magnitude = 11.69
  |           Distance = 34.6
  |      Spectral type = M3V
  |               Mass = 0.312
  |             Radius = 0.314
  |        Temperature = 3412
  |        Metallicity = -0.5
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 1
  |              Notes = The unconfirmed planet f orbits in the habitable zone.<ref name="Demangeon2021L98-59">{{cite journal
  |display-authors = etal
  |first1 = Oliver D. S.
  |last1 = Demangeon
  |first2 = M. R.
  |last2 = Zapatero Osorio
  |first3 = Y.
  |last3 = Alibert
  |first4 = S. C. C.
  |last4 = Barros
  |first5 = V.
  |last5 = Adibekyan
  |first6 = H. M.
  |last6 = Tabernero
  |title = A warm terrestrial planet with half the mass of Venus transiting a nearby star
  |url = https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf
  |date = July 2021
  |journal = Astronomy & Astrophysics
  |volume = 653
  |pages = 38
  |doi = 10.1051/0004-6361/202140728
  |s2cid = 236957385
  |arxiv = 2108.03323
  |bibcode = 2021A&A...653A..41D
  |access-date = 2022-03-03
  |archive-date = 2021-11-13
  |archive-url = https://web.archive.org/web/20211113184620/https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf
  |url-status = live
  }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[Gliese 414]] A
  |      Constellation = Ursa Major
  |    Right ascension = {{RA|11|11|05.88}}
  |        Declination = {{DEC|30|26|42.61}}
  | Apparent magnitude = 8.31
  |           Distance = 38.76
  |      Spectral type = K7V
  |               Mass = 0.65
  |             Radius = 0.679
  |        Temperature = 4120
  |        Metallicity = 0.24
  |                Age = 12.4
  |  Confirmed planets = 2
  |Unconfirmed planets = 0
  |              Notes = <ref>{{Cite journal |last1=Dedrick |first1=Cayla M. |last2=Fulton |first2=Benjamin J. |last3=Knutson |first3=Heather A. |last4=Howard |first4=Andrew W. |last5=Beatty |first5=Thomas G. |last6=Cargile |first6=Phillip A. |last7=Gaudi |first7=B. Scott |last8=Hirsch |first8=Lea A. |last9=Kuhn |first9=Rudolf B. |last10=Lund |first10=Michael B. |last11=James |first11=David J. |last12=Kosiarek |first12=Molly R. |last13=Pepper |first13=Joshua |last14=Petigura |first14=Erik A. |last15=Rodriguez |first15=Joseph E. |date=January 2021 |title=Two Planets Straddling the Habitable Zone of the Nearby K Dwarf Gl 414A |journal=The Astronomical Journal |language=en |volume=161 |issue=2 |pages=86 |doi=10.3847/1538-3881/abd0ef |doi-access=free |arxiv=2009.06503 |bibcode=2021AJ....161...86D |issn=1538-3881}}</ref><ref>{{Cite web |title=GJ 414 Overview |url=https://exoplanetarchive.ipac.caltech.edu/overview/GJ%20414 |access-date=January 4, 2024 |website=NASA Exoplanet Archive |archive-date=December 9, 2023 |archive-url=https://web.archive.org/web/20231209091347/https://exoplanetarchive.ipac.caltech.edu/overview/GJ%20414 |url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Gliese 806
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|20|45|04.099}}
  |        Declination = {{DEC|+44|29|56.6}}
  | Apparent magnitude = 10.79
  |           Distance = 39.3
  |      Spectral type = M1.5V
  |               Mass = 0.423
  |             Radius = 0.414
  |        Temperature = 3586
  |        Metallicity = -0.28
  |                Age = 3.0
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              
}}
{{Multiplanetary systems list
  |               Star = TRAPPIST-1
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|23|06|29.283}}
  |        Declination = {{DEC|-05|02|28.59}}
  | Apparent magnitude = 18.80
  |           Distance = 39.5
  |      Spectral type = M8V
  |               Mass = 0.089
  |             Radius = 0.114
  |        Temperature = 2550
  |        Metallicity = 0.04
  |                Age = 7.6
  |  Confirmed planets = 7
  |Unconfirmed planets =
  |              Notes = Planets d, e, f and g are potentially habitable. Only star known with exactly seven confirmed planets. All seven terrestrial planets lie within only 0.07 AU of the star.
}}
{{Multiplanetary systems list
  |               Star = 55 Cancri|Copernicus
  |      Constellation = Cancer (constellation){{!}}Cancer
  |    Right ascension = {{RA|08|52|35.81}}
  |        Declination = {{DEC|+28|19|50.9}}
  | Apparent magnitude = 5.95
  |           Distance = 40
  |      Spectral type = K0IV-V
  |               Mass = 1.026
  |             Radius = 0.887
  |        Temperature = 5217
  |        Metallicity = 0.290
  |                Age = 7.4
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = All five known planets orbit around star A (none are circumbinary or orbit around star B). Closest system with exactly five confirmed planets.
}}
{{Multiplanetary systems list
  |               Star = [[Gliese 180]]
  |      Constellation = Eridanus (constellation){{!}}Eridanus
  |    Right ascension = {{RA|04|53|49.9798}} 
  |        Declination = {{DEC|-17|46|24.294}}
  | Apparent magnitude = 10.894
  |           Distance = 40.3
  |      Spectral type = M2V<ref name=Schweitzer_et_al_2019GJ180>{{cite journal
 | title=The CARMENES search for exoplanets around M dwarfs. Different roads to radii and masses of the target stars
 | display-authors=1 | last1=Schweitzer | first1=A.
 | last2=Passegger | first2=V. M. | last3=Cifuentes | first3=C.
 | last4=Béjar | first4=Victor J. S. | last5=Cortés-Contreras | first5=M.
 | last6=Caballero | first6=José A. | last7=del Burgo | first7=Carlos
 | last8=Czesla | first8=Stefan | last9=Kürster | first9=Martin
 | last10=Montes | first10=David | last11=Zapatero-Osorio | first11=María Rosa
 | last12=Ribas | first12=Ignasi | last13=Reiners | first13=Ansgar
 | last14=Quirrenbach | first14=Andreas | last15=Amado | first15=Pedro J.
 | last16=Aceituno | first16=J. | last17=Anglada-Escudé | first17=Guillem
 | last18=Bauer | first18=Florian F. | last19=Dreizler | first19=Stefan
 | last20=Jeffers | first20=Sandra V. | last21=Guenther | first21=E. W.
 | last22=Henning | first22=Thomas K. | last23=Kaminski | first23=Adrian
 | last24=Lafarga | first24=M. | last25=Marfil | first25=E.
 | last26=Morales | first26=Juan Carlos | last27=Schmitt | first27=Jürgen H. M. M.
 | last28=Seifert | first28=Walter | last29=Solano | first29=E.
 | last30=Tabernero | first30=H. M. | last31=Zechmeister | first31=Mathias
 | journal=Astronomy & Astrophysics
 | volume=625 | id=A68 | pages=16 | date=May 2019
 | arxiv=1904.03231 | bibcode=2019A&A...625A..68S
 | doi=10.1051/0004-6361/201834965 | s2cid=102351979 }}</ref> or M3V<ref name=Stephenson1986GJ180>{{citation
 | title=Dwarf K and M stars of high proper motion found in a hemispheric survey
 | last=Stephenson | first=C. B. | postscript=.
 | journal=[[The Astronomical Journal]]
 | volume=92 | pages=139–165 | date=July 1986
 | bibcode=1986AJ.....92..139S | doi=10.1086/114146 | doi-access=free }}</ref>
  |               Mass = 0.39
  |             Radius = 0.42
  |        Temperature = 3562
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = The habitability of planets b and c is disputed.<ref>{{cite news | last=Sutherland | first=Paul | date=March 5, 2014 | title=Habitable planets common around red dwarf stars | url=http://sen.com/news/habitable-planets-common-around-red-dwarf-stars | website=Sen | publisher=Sen Corporation Ltd. | access-date=July 28, 2022 | archive-date=November 12, 2020 | archive-url=https://web.archive.org/web/20201112041601/https://www.sen.com/news/habitable-planets-common-around-red-dwarf-stars | url-status=live }}</ref><ref>{{citation
 | title=Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics
 | display-authors=1 | last1=Tuomi | first1=Mikko
 | last2=Jones | first2=Hugh R. A. | last3=Barnes | first3=John R.
 | last4=Anglada-Escudé | first4=Guillem | last5=Jenkins | first5=James S.
 | journal=Monthly Notices of the Royal Astronomical Society
 | volume=441 | issue=2 | pages=1545–1569 | year=2014
 | doi=10.1093/mnras/stu358 | doi-access=free | arxiv=1403.0430 | postscript=.
 | bibcode=2014MNRAS.441.1545T | s2cid=32965505 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 69830
  |      Constellation = Puppis
  |    Right ascension = {{RA|08|18|23.95}}
  |        Declination = {{DEC|−12|37|55.8}}
  | Apparent magnitude = 5.95
  |           Distance = 41
  |      Spectral type = K0V
  |               Mass = 0.856
  |             Radius = 0.895
  |        Temperature = 5385
  |        Metallicity = −0.045
  |                Age = 7.446
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = A debris disk exterior to the three exoplanets was detected by the [[Spitzer Space Telescope]] in 2005.<ref name="Lovis2006HD69830">{{cite journal | title=An extrasolar planetary system with three Neptune-mass planets | url=http://obswww.unige.ch/~pernier/publications-www/articles-pdf-ps/2006Natur.441..305L.pdf | last1=Lovis | first1=Christophe | last2=Mayor | first2=Michel | last3=Pepe | first3=Francesco | last4=Alibert | first4=Yann | last5=Benz | first5=Willy | last6=Bouchy | first6=François | last7=Correia | first7=Alexandre C. M. | last8=Laskar | first8=Jacques | last9=Mordasini | first9=Christoph | last10=Queloz | first10=Didier | last11=Santos | first11=Nuno C. | last12=Udry | first12=Stéphane | last13=Bertaux | first13=Jean-Loup | last14=Sivan | first14=Jean-Pierre | display-authors=1 | journal=Nature | volume=441 | issue=7091 | pages=305–309 | date=2006 | arxiv=astro-ph/0703024 | bibcode=2006Natur.441..305L | doi=10.1038/nature04828 | pmid=16710412 | s2cid=4343578 | access-date=2022-02-24 | archive-date=2016-03-03 | archive-url=https://web.archive.org/web/20160303232248/http://obswww.unige.ch/~pernier/publications-www/articles-pdf-ps/2006Natur.441..305L.pdf | url-status=dead }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 40307
  |      Constellation = Pictor
  |    Right ascension = {{RA|05|54|04.24}}
  |        Declination = {{DEC|−60|01|24.5}}
  | Apparent magnitude = 7.17
  |           Distance = 42
  |      Spectral type = K2.5V
  |               Mass = 0.752
  |             Radius = 0.716
  |        Temperature = 4977
  |        Metallicity = −0.308
  |                Age = 1.198
  |  Confirmed planets = 4
  |Unconfirmed planets = 2
  |              Notes = The existence of planets e and g are disputed.<ref name=Diaz2016HD40307>{{cite journal | title=The HARPS search for southern extra-solar planets. XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles | url=https://www.aanda.org/articles/aa/full_html/2016/01/aa26729-15/aa26729-15.html | last1=Díaz | first1=R. F. | last2=Ségransan | first2=D. | last3=Udry | first3=S. | last4=Lovis | first4=C. | last5=Pepe | first5=F. | last6=Dumusque | first6=X. | last7=Marmier | first7=M. | last8=Alonso | first8=R. | last9=Benz | first9=W. | last10=Bouchy | first10=F. | last11=Coffinet | first11=A. | last12=Collier Cameron | first12=A. | last13=Deleuil | first13=M. | last14=Figueira | first14=P. | last15=Gillon | first15=M. | last16=Lo Curto | first16=G. | last17=Mayor | first17=M. | last18=Mordasini | first18=C. | last19=Motalebi | first19=F. | last20=Moutou | first20=C. | last21=Pollacco | first21=D. | last22=Pompei | first22=E. | last23=Queloz | first23=D. | last24=Santos | first24=N. | last25=Wyttenbach | first25=A. | display-authors=1 | journal=Astronomy and Astrophysics | volume=585 | at=A134 | year=2016 | arxiv=1510.06446 | bibcode=2016A&A...585A.134D | doi=10.1051/0004-6361/201526729 | s2cid=118531921 | access-date=2022-02-24 | archive-date=2021-02-24 | archive-url=https://web.archive.org/web/20210224090311/https://www.aanda.org/articles/aa/full_html/2016/01/aa26729-15/aa26729-15.html | url-status=live }}</ref> If confirmed, planet g is potentially habitable.<ref name="tuomi12HD40307g">{{cite journal |doi=10.1051/0004-6361/201220268 |last1=Tuomi |first1=Mikko |last2=Anglada-Escudé |first2=Guillem |last3=Gerlach |first3=Enrico |last4=Jones |first4=Hugh R. A. |last5=Reiners |first5=Ansgar |last6=Rivera |first6=Eugenio J. |last7=Vogt |first7=Steven S. |last8=Butler |first8=R. Paul |title=Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307 |journal=Astronomy & Astrophysics |date=17 December 2012 |volume=549 |pages=A48 |arxiv=1211.1617 |bibcode=2013A&A...549A..48T |s2cid=7424216 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Upsilon Andromedae|Titawin
  |      Constellation = Andromeda (constellation){{!}}Andromeda
  |    Right ascension = {{RA|01|36|47.84}}
  |        Declination = {{DEC|+41|24|19.7}}
  | Apparent magnitude = 4.09
  |           Distance = 44
  |      Spectral type = F8V
  |               Mass = 1.27
  |             Radius = 1.699
  |        Temperature = 6107
  |        Metallicity = 0.086
  |                Age = 3.781
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = Nearest [[F-type main sequence]] star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after [[7 Canis Majoris]]. All exoplanets orbit around star A in the binary system.
}}
{{Multiplanetary systems list
  |               Star = 47 Ursae Majoris|Chalawan 
  |      Constellation = Ursa Major
  |    Right ascension = {{RA|10|59|27.97}}
  |        Declination = {{DEC|+40|25|48.9}}
  | Apparent magnitude = 5.10
  |           Distance = 46
  |      Spectral type = G0V
  |               Mass = 1.029
  |             Radius = 1.241
  |        Temperature = 5892
  |        Metallicity = 0.003
  |                Age = 7.434
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Planet Taphao Thong was discovered in 1996 and was one of the first exoplanets to be discovered.<ref>
{{cite journal
 | author=R. P. Butler
 | title=A Planet Orbiting 47 Ursae Majoris
 | journal=[[Astrophysical Journal Letters]]
 | volume=464 | issue=2 | date=1996
 | pages=L153–L156
 | doi=10.1086/310102
| bibcode=1996ApJ...464L.153B
 | last2=Marcy
 | first2=Geoffrey W.
| doi-access=free
 }}</ref> The planet was the first [[orbital period|long-period]] extrasolar planet discovered. The other planets were discovered later.<ref name="bayesian 47Uma">
{{cite journal
 |author=P. C. Gregory
 |author2=D. A. Fischer
 |date=2010
 |title=A Bayesian periodogram finds evidence for three planets in 47 Ursae Majoris
 |journal=[[Monthly Notices of the Royal Astronomical Society]]
 |volume=403 |issue=2 |pages=731–747
 |doi=10.1111/j.1365-2966.2009.16233.x
|doi-access=free
 |bibcode=2010MNRAS.403..731G
|arxiv = 1003.5549 |s2cid=16722873
 }}</ref>

}}
{{Multiplanetary systems list
  |               Star = [[Nu2 Lupi|Nu{{sup|2}} Lupi]]
  |      Constellation = Lupus (constellation){{!}}Lupus
  |    Right ascension = {{RA|15|21|49.57}}
  |        Declination = {{DEC|−48|19|01.1}}
  | Apparent magnitude = 5.65
  |           Distance = 47
  |      Spectral type = G2V
  |               Mass = 0.906
  |             Radius = 1.012
  |        Temperature = 5664
  |        Metallicity = -0.34
  |                Age = 10.36
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = One of the oldest stars in the solar neighbourhood.<ref name="Takeda2007Nu2Lupi">{{cite journal | title=Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog | last1=Takeda | first1=Genya |display-authors=etal  | date=2007 | arxiv=astro-ph/0607235 | bibcode=2007ApJS..168..297T | doi=10.1086/509763 | volume=168 | journal=The Astrophysical Journal Supplement Series | issue=2 | pages=297–318| s2cid=18775378 }}</ref><ref name=Sousa08Nu2Lupi>{{cite journal | author=Sousa, S. G. | title=Spectroscopic parameters for 451 stars in the HARPS GTO planet search program. Stellar [Fe/H] and the frequency of exo-Neptunes. | journal=Astronomy and Astrophysics | volume=487 | issue=1 |date=August 2008 | pages=373–381  | doi=10.1051/0004-6361:200809698 | bibcode=2008A&A...487..373S | display-authors=1 | last2=Santos | first2=N. C. | last3=Mayor | first3=M. | last4=Udry | first4=S. | last5=Casagrande | first5=L. | last6=Israelian | first6=G. | last7=Pepe | first7=F. | last8=Queloz | first8=D. | last9=Monteiro | first9=M. J. P. F. G. |arxiv = 0805.4826 | s2cid=18173201 }}</ref><ref name="Lovis2011Nu2Lupi">{{cite arXiv | title=The HARPS search for southern extra-solar planets. XXXI. Magnetic activity cycles in solar-type stars: statistics and impact on precise radial velocities | last1=Lovis | first1=C. |display-authors=etal  | date=2011 | class=astro-ph.SR | eprint=1107.5325}}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[LHS 1140]]
  |      Constellation = Cetus (constellation){{!}}Cetus
  |    Right ascension = {{RA|00|44|59.31}}
  |        Declination = {{DEC|-15|16|16.7}}
  | Apparent magnitude = 14.18
  |           Distance = 48.9
  |      Spectral type = M4.5V<ref name="NAT-20170419">{{cite journal |year=2017 |title=A temperate rocky super-Earth transiting a nearby cool star |journal=Nature |volume=544 |issue=7650 |pages=333–336 |arxiv=1704.05556 |doi=10.1038/nature22055 |pmid=28426003 |bibcode=2017Natur.544..333D |s2cid=2718408 |last1=Dittmann |first1=Jason A. |last2=Irwin |first2=Jonathan M. |last3=Charbonneau |first3=David |last4=Bonfils |first4=Xavier |last5=Astudillo-Defru |first5=Nicola |last6=Haywood |first6=Raphaëlle D. |last7=Berta-Thompson |first7=Zachory K. |last8=Newton |first8=Elisabeth R. |last9=Rodriguez |first9=Joseph E. |last10=Winters|first10=Jennifer G. |last11=Tan |first11=Thiam-Guan |last12=Almenara |first12=Jose-Manuel |last13=Bouchy |first13=François |last14=Delfosse |first14=Xavier |last15=Forveille |first15=Thierry |last16=Lovis |first16=Christophe |last17=Murgas |first17=Felipe |last18=Pepe |first18=Francesco |last19=Santos |first19=Nuno C. |last20=Udry |first20=Stephane |last21=Wünsche |first21=Anaël |last22=Esquerdo |first22=Gilbert A. |last23=Latham |first23=David W. |last24=Dressing |first24=Courtney D. |display-authors=6}}</ref>
  |               Mass = 0.179
  |             Radius = 0.2139
  |        Temperature = 3216{{±|39}}
  |        Metallicity = -0.24
  |                Age = 5
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              Notes = Planet b is a potentially habitable Super-Earth.<ref name="NYT-20170419">{{cite news |last=Overbye |first=Dennis |author-link=Dennis Overbye |title=A new exoplanet may be most promising yet in search for life |url=https://www.nytimes.com/2017/04/19/science/exoplanet-signs-of-life.html |date=19 April 2017 |work=[[New York Times]] |access-date=20 April 2017 |archive-date=11 November 2020 |archive-url=https://web.archive.org/web/20201111202355/https://www.nytimes.com/2017/04/19/science/exoplanet-signs-of-life.html |url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Gliese 163
  |      Constellation = Dorado
  |    Right ascension = {{RA|04|09|16}}
  |        Declination = {{DEC|−53|22|25}}
  | Apparent magnitude = 11.8
  |           Distance = 49
  |      Spectral type = M3.5V
  |               Mass = 0.4
  |             Radius =
  |        Temperature =
  |        Metallicity =
  |                Age = 3
  |  Confirmed planets = 5
  |Unconfirmed planets = 
  |              Notes = Planet c is possibly a potentially habitable Super-Earth but is probably too hot or massive.<ref name="PHL-20120829">{{cite web
 | last=Méndez
 | first=Abel
 | date=August 29, 2012
 | title=A Hot Potential Habitable Exoplanet around Gliese 163
 | url=http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163
 | publisher=[[University of Puerto Rico at Arecibo]] (Planetary Habitability Laboratory)
 | accessdate=September 20, 2012
 | archive-date=October 21, 2019
 | archive-url=https://web.archive.org/web/20191021202448/http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163
 | url-status=dead
 }}</ref><ref name="Space-20120920">{{cite web
 | last=Redd
 | first=Nola Taylor
 | title=Newfound Alien Planet a Top Contender to Host Life
 | url=http://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html
 | date=September 20, 2012
 | publisher=[[Space.com]]
 | accessdate=September 20, 2012
 | archive-date=December 26, 2019
 | archive-url=https://web.archive.org/web/20191226102330/https://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html
 | url-status=live
 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Mu Arae|Cervantes
  |      Constellation = Ara (constellation){{!}}Ara
  |    Right ascension = {{RA|17|44|08.70}}
  |        Declination = {{DEC|−51|50|02.6}}
  | Apparent magnitude = 5.15
  |           Distance = 51
  |      Spectral type = G3IV-V
  |               Mass = 1.077
  |             Radius = 1.246
  |        Temperature = 5704
  |        Metallicity = 0.277
  |                Age = 6.413
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Planet Quijote orbits in the [[circumstellar habitable zone]]. However, it is a [[gas giant]], so it itself is uninhabitable although a large moon orbiting around it may be [[Habitability of natural satellites|habitable]].
}}
{{Multiplanetary systems list
  |               Star = [[GJ 3929]]
  |      Constellation = Corona Borealis
  |    Right ascension = {{RA|15|58|18.8}}
  |        Declination = {{DEC|35|24|24.3}}
  | Apparent magnitude = 12.67
  |           Distance = 51.58
  |      Spectral type = M3.5V
  |               Mass = 0.313
  |             Radius = 0.32
  |        Temperature = 3384
  |        Metallicity = -0.02
  |                Age = 
  |  Confirmed planets = 2
  |Unconfirmed planets = 0
  |              Notes = <ref>{{Cite web |title=Simbad - Object view |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=G%20180-18 |access-date=2024-01-04 |website=simbad.cds.unistra.fr}}</ref><ref>{{Cite journal |last1=Beard |first1=Corey |last2=Robertson |first2=Paul |last3=Kanodia |first3=Shubham |last4=Lubin |first4=Jack |last5=Cañas |first5=Caleb I. |last6=Gupta |first6=Arvind F. |last7=Holcomb |first7=Rae |last8=Jones |first8=Sinclaire |last9=Libby-Roberts |first9=Jessica E. |last10=Lin |first10=Andrea S. J. |last11=Mahadevan |first11=Suvrath |last12=Stefánsson |first12=Guđmundur |last13=Bender |first13=Chad F. |last14=Blake |first14=Cullen H. |last15=Cochran |first15=William D. |date=2022-08-30 |title=GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion |journal=The Astrophysical Journal |volume=936 |issue=1 |pages=55 |doi=10.3847/1538-4357/ac8480 |doi-access=free |arxiv=2207.10672 |bibcode=2022ApJ...936...55B |issn=0004-637X}}</ref>
}}

{{Multiplanetary systems list
  |               Star = [[Gliese 676]] A
  |      Constellation = Ara (constellation){{!}}Ara
  |    Right ascension = {{RA|17|30|11.2042}}
  |        Declination = {{DEC|-51|38|13.116}}
  | Apparent magnitude = 9.59
  |           Distance = 53
  |      Spectral type = M0V
  |               Mass = 0.71
  |             Radius =
  |        Temperature =
  |        Metallicity = 0.23
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Held the record for widest range of masses in a planetary system in 2012.<ref name="4-planet Gj676A">{{cite journal
 |last=Anglada-Escudé
 |first=Guillem
 |author2=Tuomi, Mikko
 |date=2012
 |title=A planetary system with gas giants and super-Earths around the nearby M dwarf GJ 676A. Optimizing data analysis techniques for the detection of multi-planetary systems
 |arxiv=1206.7118
 |bibcode=2012A&A...548A..58A
 |doi=10.1051/0004-6361/201219910
 |volume=548
 |journal=Astronomy
 |pages=A58
 |s2cid=17115882
 |url=http://goedoc.uni-goettingen.de/goescholar/bitstream/handle/1/9595/aa19910-12.pdf?sequence=2
 }}{{Dead link|date=February 2024 |bot=InternetArchiveBot |fix-attempted=yes }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 7924
  |      Constellation = Cassiopeia (constellation){{!}}Cassiopeia
  |    Right ascension = {{RA|01|21|59.12}}
  |        Declination = {{DEC|+76|42|37.0}}
  | Apparent magnitude = 7.19
  |           Distance = 55
  |      Spectral type = K0V
  |               Mass = 0.832
  |             Radius = 0.78
  |        Temperature = 5177
  |        Metallicity = -0.15
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = These planets may be potentially habitable Super-Earths.<ref name="Fulton2015HD7924">{{cite journal
 | title=Three Super-Earths Orbiting HD 7924
 | last1=Fulton | first1=Benjamin J. | last2=Weiss | first2=Lauren M.
 | last3=Sinukoff | first3=Evan | last4=Isaacson | first4=Howard
 | last5=Howard | first5=Andrew W. | last6=Marcy | first6=Geoffrey W.
 | last7=Henry | first7=Gregory W. | last8=Holden | first8=Bradford P.
 | last9=Kibrick | first9=Robert I. | display-authors=1
 | journal=The Astrophysical Journal
 | volume=805 | issue=2 | pages=175 | year=2015
 | arxiv=1504.06629 | bibcode=2015ApJ...805..175F
 | doi=10.1088/0004-637X/805/2/175 | s2cid=7969255 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[Pi Mensae]]
  |      Constellation = Mensa_(constellation){{!}}Mensa
  |    Right ascension = {{RA|05|37|09.8851}}
  |        Declination = {{DEC|−80|28|08.8313}}
  | Apparent magnitude = 5.65
  |           Distance = 59.62{{±|0.07}}
  |      Spectral type = G0V
  |               Mass = 1.11
  |             Radius = 1.15
  |        Temperature = 6013
  |        Metallicity = 0.09
  |                Age = 3.4
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = Outer planet is likely a [[brown dwarf]].<ref name=Damasso2020>{{citation|arxiv=2007.06410|title=A precise architecture characterization of the π Mensae planetary system|year=2020|doi=10.1051/0004-6361/202038416|last1=Damasso|first1=M.|last2=Sozzetti|first2=A.|last3=Lovis|first3=C.|last4=Barros|first4=S. C. C.|last5=Sousa|first5=S. G.|last6=Demangeon|first6=O. D. S.|last7=Faria|first7=J. P.|last8=Lillo-Box|first8=J.|last9=Cristiani|first9=S.|last10=Pepe|first10=F.|last11=Rebolo|first11=R.|last12=Santos|first12=N. C.|last13=Zapatero Osorio|first13=M. R.|last14=González Hernández|first14=J. I.|last15=Amate|first15=M.|last16=Pasquini|first16=L.|last17=Zerbi|first17=F. M.|last18=Adibekyan|first18=V.|last19=Abreu|first19=M.|last20=Affolter|first20=M.|last21=Alibert|first21=Y.|last22=Aliverti|first22=M.|last23=Allart|first23=R.|last24=Allende Prieto|first24=C.|last25=Álvarez|first25=D.|last26=Alves|first26=D.|last27=Avila|first27=G.|last28=Baldini|first28=V.|last29=Bandy|first29=T.|last30=Benz|first30=W.|journal=Astronomy & Astrophysics|volume=642|pages=A31|bibcode=2020A&A...642A..31D|s2cid=220496034|display-authors=1}}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[Gliese 3293]]
  |      Constellation = Eridanus (constellation){{!}}Eridanus
  |    Right ascension = {{RA|04|28|35.72}}
  |        Declination = {{DEC|-25|10|08.9}}
  | Apparent magnitude = 11.96
  |           Distance = 59
  |      Spectral type = M2.5V
  |               Mass = 0.42
  |             Radius = 0.40±0.03
  |        Temperature = 3466±49
  |        Metallicity = 0.02±0.09
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Planets b and d orbit in the habitable zone.<ref name="arxiv.org_Gliese3293">{{cite journal
 |doi             = 10.1051/0004-6361/201630153
 |last1           = Astudillo-Defru
 |first1          = Nicola
 |last2           = Forveille
 |first2          = Thierry
 |last3           = Bonfils
 |first3          = Xavier
 |last4           = Ségransan
 |first4          = Damien
 |last5           = Bouchy
 |first5          = François
 |last6           = Delfosse
 |first6          = Xavier
 |last7           = Lovis
 |first7          = Christophe
 |last8           = Mayor
 |first8          = Michel
 |last9           = Murgas
 |first9          = Felipe
 |last10          = Pepe
 |first10         = Francesco
 |last11          = Santos
 |first11         = Nuno C.
 |last12          = Udry
 |first12         = Stéphane
 |last13          = Wünsche
 |first13         = Anaël
 |display-authors = 6
 |year            = 2017
 |title           = The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M&nbsp;dwarfs GJ&nbsp;3138, GJ&nbsp;3323, GJ&nbsp;273, GJ&nbsp;628, and GJ&nbsp;3293
 |journal         = Astronomy and Astrophysics
 |volume          = 602
 |at              = A88
 |arxiv           = 1703.05386
 |bibcode         = 2017A&A...602A..88A
 |s2cid           = 119418595
 |url             = https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
 |access-date     = 2022-02-25
 |archive-date    = 2022-09-28
 |archive-url     = https://web.archive.org/web/20220928032005/https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
 |url-status      = live
}}</ref>
}}
{{Multiplanetary systems list
  |               Star = LHS 1678
  |      Constellation = Caelum
  |    Right ascension = {{Ra|04|32|43}}
  |        Declination = {{Dec|-39|47|21}}
  | Apparent magnitude = 12
  |           Distance = 64.8
  |      Spectral type = M2V
  |               Mass = 0.345
  |             Radius = 0.329
  |        Temperature = 3490
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 0
  |              Notes = <ref>{{cite web | url=https://exoplanet.eu/catalog/lhs_1678_d--8971/ | title=Planet LHS 1678 D | date=2024 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[HD 104067]]
  |      Constellation = Corvus (constellation){{!}}Corvus
  |    Right ascension = {{RA|11|59|10.0}}
  |        Declination = {{DEC|-20|21|13.6}}
  | Apparent magnitude = 7.92
  |           Distance = 66.3
  |      Spectral type = K3V
  |               Mass = 0.82
  |             Radius = 0.77
  |        Temperature = 4942
  |        Metallicity = 0.11
  |                Age = 4.8
  |  Confirmed planets = 2 
  |Unconfirmed planets = 1
  |              Notes = The innermost planet, which is unconfirmed, might suffer from significant [[tidal heating]].<ref name="Kane2024">{{cite journal |last1=Kane |first1=Stephen R. |last2=Fetherolf |first2=Tara |display-authors=etal |date=March 2024 |title=A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World |journal=[[The Astronomical Journal]] |volume= 167|issue= 5|page=239 |doi= 10.3847/1538-3881/ad3820|doi-access=free |arxiv=2403.17062|bibcode=2024AJ....167..239K }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 142
  |      Constellation = Phoenix (constellation){{!}}Phoenix
  |    Right ascension = {{RA|00|06|19.0}}
  |        Declination = {{DEC|-49|04|30}}
  | Apparent magnitude = 5.70
  |           Distance = 67
  |      Spectral type = G1 IV
  |               Mass = 1.1
  |             Radius = 0.86
  |        Temperature = 6180
  |        Metallicity = 0.04
  |                Age = 5.93
  |  Confirmed planets = 3
  |Unconfirmed planets =  
}}
{{Multiplanetary systems list
  |               Star = HD 215152
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|43|21}}
  |        Declination = {{DEC|-06|24|03}}
  | Apparent magnitude = 8.13
  |           Distance = 70
  |      Spectral type = G8IV
  |               Mass = 1.019
  |             Radius = 1.080
  |        Temperature = 5646
  |        Metallicity = 0.367
  |                Age = 7.320
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = A debris disk candidate as it has an infrared excess.<ref name=apjl710_1_L26>{{citation | display-authors=1 | last1=Koerner | first1=D. W. | last2=Kim | first2=S. | last3=Trilling | first3=D. E. | last4=Larson | first4=H. | last5=Cotera | first5=A. | last6=Stapelfeldt | first6=K. R. | last7=Wahhaj | first7=Z. | last8=Fajardo-Acosta | first8=S. | last9=Padgett | first9=D. | last10=Backman | first10=D. | title=New Debris Disk Candidates Around 49 Nearby Stars | journal=The Astrophysical Journal Letters | volume=710 | issue=1 | pages=L26–L29 | date=February 2010 | doi=10.1088/2041-8205/710/1/L26 | bibcode=2010ApJ...710L..26K | s2cid=122844702 | postscript=. | url=http://openknowledge.nau.edu/449/7/Koerner_DW_etal_2010_New_debris_disk_candidates_around_49_nearby_stars%281%29.pdf | access-date=2022-02-25 | archive-date=2020-09-15 | archive-url=https://web.archive.org/web/20200915161129/http://openknowledge.nau.edu/449/7/Koerner_DW_etal_2010_New_debris_disk_candidates_around_49_nearby_stars%281%29.pdf | url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 164922
  |      Constellation = Hercules (constellation){{!}}Hercules
  |    Right ascension = {{RA|18|02|30.86}}
  |        Declination = {{DEC|+26|18|46.8}}
  | Apparent magnitude = 7.01
  |           Distance = 72
  |      Spectral type = G9V<ref name="Spectype164922">{{cite journal|arxiv=1607.00007|last1= Fulton|first1= Benjamin J.|title= Three Temperate Neptunes Orbiting Nearby Stars|last2=  Howard|first2= Andrew W.|last3=  Weiss|first3= Lauren M.|last4= Sinukoff|first4= Evan|last5=  Petigura|first5= Erik A.|last6= Isaacson|first6= Howard|last7= Hirsch|first7= Lea|last8=  Marcy|first8= Geoffrey W.|last9=  Henry|first9= Gregory W.|last10=  Grunblatt|first10= Samuel K.|last11= Huber|first11= Daniel|author12= Kaspar von Braun|last13=  Boyajian|first13= Tabetha S.|last14=  Kane|first14= Stephen R.|last15= Wittrock|first15= Justin|last16=  Horch|first16= Elliott P.|last17=  Ciardi|first17= David R.|last18=  Howell|first18= Steve B.|last19=  Wright|first19= Jason T.|last20=  Ford|first20= Eric B.|year= 2016|doi=10.3847/0004-637X/830/1/46|volume=830|issue= 1|journal=The Astrophysical Journal|page=46|bibcode = 2016ApJ...830...46F |s2cid= 36666883|doi-access= free}}</ref>
  |               Mass = 0.874
  |             Radius = 0.999
  |        Temperature = 5293
  |        Metallicity = 0.16
  |                Age = 13.4
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Oldest star with a multiplanetary system. Despite its age, it is more metal-rich than the Sun.<ref name="Spectype164922"/>
}}
{{Multiplanetary systems list
  |               Star = HD 63433
  |      Constellation = Gemini (constellation){{!}}Gemini
  |    Right ascension = {{RA|07|49|55.0}}
  |        Declination = {{DEC|+27|21|47.4}}
  | Apparent magnitude = 6.92
  |           Distance = 73
  |      Spectral type = G5V
  |               Mass = 0.99
  |             Radius = 0.912
  |        Temperature =5640
  |        Metallicity = 0.03
  |                Age = 0.4
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = HIP 57274
  |      Constellation = Ursa Major
  |    Right ascension = {{RA|11|44|41}}
  |        Declination = {{DEC|+30|57|33}}
  | Apparent magnitude = 8.96
  |           Distance = 85
  |      Spectral type = K5V
  |               Mass = 0.73
  |             Radius = 0.68
  |        Temperature = 4640
  |        Metallicity = 0.09
  |                Age = 7.87
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 39194
  |      Constellation = Mensa (constellation){{!}}Mensa
  |    Right ascension = {{RA|05|44|32}}
  |        Declination = {{DEC|-70|08|37}}
  | Apparent magnitude = 8.08
  |           Distance = 86.2
  |      Spectral type = K0V
  |               Mass =
  |             Radius =
  |        Temperature =5205
  |        Metallicity =-0.61
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = The planets have eccentric orbits.<ref name = Unger2021>{{cite journal | display-authors = 1 | last1 = Unger | first1 = N. | last2 = Ségransan | first2 = D. | last3 = Queloz | first3 = D. | last4 = Udry | first4 = S. | last5 = Lovis | first5 = C. | last6 = Mordasini | first6 = C. | last7 = Ahrer | first7 = E. | last8 = Benz | first8 = W. | last9 = Bouchy | first9 = F. | last10 = Delisle | first10 = J.-B. | last11 = Díaz | first11 = R. F. | last12 = Dumusque | first12 = X. | last13 = Lo Curto | first13 = G. | last14 = Marmier | first14 = M. | last15 = Mayor | first15 = M. | last16 = Pepe | first16 = F. | last17 = Santos | first17 = N. C. | last18 = Stalport | first18 = M. | last19 = Alonso | first19 = R. | last20 = Collier Cameron | first20 = A. | last21 = Deleuil | first21 = M. | last22 = Figueira | first22 = P. | last23 = Gillon | first23 = M. | last24 = Moutou | first24 = C. | last25 = Pollacco | first25 = D. | last26 = Pompei | first26 = E. | title = The HARPS search for southern extra-solar planets | journal = Astronomy & Astrophysics | date = October 2021 | volume = 654 | page = A104 | issn = 0004-6361 | eissn = 1432-0746 | doi = 10.1051/0004-6361/202141351 | bibcode = 2021A&A...654A.104U | arxiv = 2108.10198| doi-access = free}}</ref>
}}
{{Multiplanetary systems list
  |               Star = LP 791-18
  |      Constellation = Crater 
  |    Right ascension = {{RA|11|02|45.95}}
  |        Declination = {{DEC|-16|24|22.3}}
  | Apparent magnitude = 16.9
  |           Distance = 86.9
  |      Spectral type = M6V/M7V
  |               Mass = 0.139
  |             Radius = 0.17
  |        Temperature =2960
  |        Metallicity =-0.09
  |                Age = 0.5
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = HD 181433
  |      Constellation = Pavo (constellation){{!}}Pavo
  |    Right ascension = {{RA|19|25|09.57}}
  |        Declination = {{DEC|−66|28|07.7}}
  | Apparent magnitude = 8.38
  |           Distance = 87
  |      Spectral type = K5V
  |               Mass = 0.777
  |             Radius = 0.786
  |        Temperature = 4962
  |        Metallicity = 0.327
  |                Age = 8.974
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 134606
  |      Constellation = Apus
  |    Right ascension = {{RA|15|15|15}}
  |        Declination = {{DEC|-70|31|11}}
  | Apparent magnitude = 6.85
  |           Distance = 87
  |      Spectral type = G6IV
  |               Mass =
  |             Radius =
  |        Temperature =
  |        Metallicity =
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = The planets have moderately eccentric orbits.<ref name=Mayor2011>{{citation
 | first1=M. | last1=Mayor | first2=M. | last2=Marmier
 | first3=C. | last3=Lovis | first4=S. | last4=Udry
 | first5=D. | last5=Ségransan | first6=F. | last6=Pepe
 | first7=W. | last7=Benz | first8=J.-L. | last8=Bertaux
 | first9=F. | last9=Bouchy | first10=X. | last10=Dumusque
 | first11=G. | last11=Lo Curto | first12=C. | last12=Mordasini
 | first13=D. | last13=Queloz | first14=N. C. | last14=Santos
 | title=The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets
 | date=September 13, 2011 | arxiv=1109.2497 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 158259
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|17|25|24.0}}
  |        Declination = {{DEC|+52|47|26}}
  | Apparent magnitude = 6.46
  |           Distance = 89
  |      Spectral type = G0
  |               Mass = 1.08
  |             Radius = 1.21
  |        Temperature =
  |        Metallicity =
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets = 1
  |              Notes = A G-type star slightly more massive than the Sun.<ref name=SOPHIEHD>{{cite journal|last1=Hara|first1=N. C.|last2=Bouchy|first2=F.|last3=Stalport|first3=M.|last4=Boisse|first4=I.|last5=Rodrigues|first5=J.|last6=Delisle|first6=J. B.|last7=Santerne|first7=A.|last8=Henry|first8=G. W.|last9=Arnold|first9=L.|last10=Astudillo-Defru|first10=N.|last11=Borgniet|first11=S.|last12=Bonfils|first12=X.|last13=Bourrier|first13=V.|last14=Brugger|first14=B.|last15=Courcol|first15=B.|last16=Dalal|first16=S.|last17=Deleuil|first17=M.|last18=Delfosse|first18=X.|last19=Demangeon|first19=O.|last20=Díaz|first20=R. F.|last21=Dumusque|first21=X.|last22=Forveille|first22=T.|last23=Hébrard|first23=G.|last24=Hobson|first24=M. J.|last25=Kiefer|first25=F.|last26=Lopez|first26=T.|last27=Mignon|first27=L.|last28=Mousis|first28=O.|last29=Moutou|first29=C.|last30=Pepe|first30=F.|last31=Rey|first31=J.|last32=Santos|first32=N. C.|last33=Ségransan|first33=D.|last34=Udry|first34=S.|last35=Wilson|first35=P. A.|title=The SOPHIE search for northern extrasolar planets XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain|date=March 10, 2020|journal=Astronomy & Astrophysics|volume=636|issue=1|page=L6|doi=10.1051/0004-6361/201937254|arxiv=1911.13296|bibcode=2020A&A...636L...6H|s2cid=208512859}}</ref> Planet g remains unconfirmed.<ref name=SOPHIEHD />
}}
{{Multiplanetary systems list
  |               Star = HD 82943
  |      Constellation = Hydra (constellation){{!}}Hydra
  |    Right ascension = {{RA|09|34|50.74}}
  |        Declination = {{DEC|−12|07|46.4}}
  | Apparent magnitude = 6.54
  |           Distance = 90
  |      Spectral type = F9V Fe+0.5<ref name=aj132_1_161>{{citation | display-authors=1 | last1=Gray | first1=R. O. | last2=Corbally | first2=C. J. | last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T. | last5=Bubar | first5=E. J. | last6=McGahee | first6=C. E. | last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R. | title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample | journal=[[The Astronomical Journal]] | volume=132 | issue=1 | pages=161–170 |date=July 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | s2cid=119476992 }}</ref>
  |               Mass = 1.175
  |             Radius = 1.124
  |        Temperature = 5874
  |        Metallicity = 0.273
  |                Age = 3.080
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes = Planets b and c are in a 2:1 orbital resonance.<ref name="Lee2006">{{cite journal | title=On the 2:1 Orbital Resonance in the HD 82943 Planetary System | last1=Lee | first1=Man Hoi | last2=Butler | first2=R. Paul | last3=Fischer | first3=Debra A. | last4=Marcy | first4=Geoffrey W. | last5=Vogt | first5=Steven S. | display-authors=1 | journal=The Astrophysical Journal | date=2006 | volume=641 | issue=2 | pages=1178–1187 | arxiv=astro-ph/0512551 | bibcode=2006ApJ...641.1178L | doi=10.1086/500566 | s2cid=119432579 }}</ref> Planet b orbits in the habitable zone, but it and planet c are massive enough to be [[brown dwarf]]s. HD 82943 has an unusual [[lithium-6]] abundance.<ref name="eso0118">{{cite press release | title=The Harsh Destiny of a Planet? | date=May 9, 2001 | publisher=[[European Southern Observatory]] | location=Garching, Germany | url=http://www.eso.org/public/news/eso0118/ | access-date=December 30, 2012 | archive-date=September 21, 2020 | archive-url=https://web.archive.org/web/20200921074543/https://www.eso.org/public/news/eso0118/ | url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Gliese 3138
  |      Constellation = Cetus (constellation){{!}}Cetus
  |    Right ascension = {{RA|02|09|10.90}}
  |        Declination = {{DEC|-16|20|22.53}}
  | Apparent magnitude = 10.877
  |           Distance = 92.9
  |      Spectral type = 
  |               Mass = 0.681
  |             Radius = 
  |        Temperature = 3717{{±|49}}
  |        Metallicity = -0.30
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = GJ 9827
  |      Constellation = 	Pisces (constellation){{!}}Pisces
  |    Right ascension = {{RA|23|27|04.84}}
  |        Declination = {{DEC|−01|17|10.59}}
  | Apparent magnitude = 10.10
  |           Distance = 96.8{{±|0.2}}
  |      Spectral type = K6V
  |               Mass = 0.593
  |             Radius = 0.579
  |        Temperature = 4294{{±|52}}
  |        Metallicity = -0.26
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = Also known as K2-135. Planet b is extremely dense, with at least half of its mass being iron.<ref>{{cite journal | bibcode=2018AJ....155...72R | doi=10.3847/1538-3881/aaa292 | arxiv=1709.01957| title=A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc| journal=The Astronomical Journal| volume=155| issue=2| pages=72| year=2018| last1=Rodriguez| first1=Joseph E| last2=Vanderburg| first2=Andrew| last3=Eastman| first3=Jason D| last4=Mann| first4=Andrew W| last5=Crossfield| first5=Ian J. M| last6=Ciardi| first6=David R| last7=Latham| first7=David W| last8=Quinn| first8=Samuel N| s2cid=55459523 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = K2-239
  |      Constellation = Sextans{{!}}Sextans
  |    Right ascension = {{RA|10|42|22.63}}
  |        Declination = {{DEC|+04|26|28.86}}
  | Apparent magnitude = 14.5
  |           Distance = 101.5
  |      Spectral type = M3V
  |               Mass = 0.40
  |             Radius = 0.36
  |        Temperature = 3420
  |        Metallicity = -0.1
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[TOI 700|TOI-700]]
  |      Constellation = Dorado (constellation){{!}}Dorado
  |    Right ascension = {{RA|06|28|22.97}}
  |        Declination = {{DEC|−65|34|43.01}}
  | Apparent magnitude = 13.10
  |           Distance = 101.61 
  |      Spectral type = M2V
  |               Mass = 0.416 
  |             Radius = 0.42
  |        Temperature = 3480
  |        Metallicity = -0.07
  |                Age = 1.5
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = Planets d and e are potentially habitable.<ref name="NASA-20200106">{{cite news |last1=Andreolo |first1=Claire |last2=Cofield |first2=Calla |last3=Kazmierczak |first3=Jeanette |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.jpl.nasa.gov/news/news.php?feature=7569 |date=6 January 2020 |work=[[NASA]] |access-date=6 January 2020 |archive-date=14 April 2020 |archive-url=https://web.archive.org/web/20200414070820/https://www.jpl.nasa.gov/news/news.php?feature=7569 |url-status=live }}</ref><ref name="NASA-20200106b">{{cite news |last1=Garner |first1=Rob |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.nasa.gov/feature/goddard/2020/nasa-planet-hunter-finds-its-1st-earth-size-habitable-zone-world |date=6 January 2020 |work=[[NASA]] |access-date=6 January 2020 |archive-date=5 April 2020 |archive-url=https://web.archive.org/web/20200405004715/https://www.nasa.gov/feature/goddard/2020/nasa-planet-hunter-finds-its-1st-earth-size-habitable-zone-world |url-status=live }}</ref><ref name="SPC-20200106">{{cite news |last=Wall |first=Mike |title=NASA's TESS Planet Hunter Finds Its 1st Earth-Size World in 'Habitable Zone' |url=https://www.space.com/nasa-tess-first-earth-size-habitable-exoplanet-toi-700d.html |date=6 January 2020 |work=[[Space.com]] |access-date=6 January 2020 |archive-date=8 April 2020 |archive-url=https://web.archive.org/web/20200408031443/https://www.space.com/nasa-tess-first-earth-size-habitable-exoplanet-toi-700d.html |url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 17926
  |      Constellation = Fornax
  |    Right ascension = {{RA|02|51|56.16}}
  |        Declination = {{DEC|−30|48|53.2}}
  | Apparent magnitude = 6.38
  |           Distance = 105
  |      Spectral type = F6V
  |               Mass = 1.145
  |             Radius = 1.31
  |        Temperature = 6201
  |        Metallicity = -0.14
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = The star forms a binary with a red dwarf.<ref name=tessHR858>{{cite journal
 | title=TESS Spots a Compact System of Super-Earths around the Naked-Eye Star HR 858
 | journal=The Astrophysical Journal | volume=881 | issue=1 | pages=L19 | last1=Vanderburg | first1=Andrew | last2=Huang | first2=Chelsea X.
 | last3=Rodriguez | first3=Joseph E. | last4=Becker | first4=Juliette C.
 | last5=Ricker | first5=George R. | last6=Vanderspek | first6=Roland K.
 | last7=Latham | first7=David W. | last8=Seager | first8=Sara
 | last9=Winn | first9=Joshua N. | last10=Jenkins | first10=Jon M.
 | last11=Addison | first11=Brett | last12=Bieryla | first12=Allyson
 | last13=Briceño | first13=Cesar | last14=Bowler | first14=Brendan P.
 | last15=Burke | first15=Christopher J. | last16=Burt | first16=Jennifer A.
 | last17=Caldwell | first17=Douglas A. | last18=Clark | first18=Jake T.
 | last19=Crossfield | first19=Ian | last20=Dittmann | first20=Jason A.
 | last21=Dynes | first21=Scott | last22=Guerrero | first22=Natalia
 | last23=Horner | first23=Jonathan | last24=Kane | first24=Stephen R.
 | last25=Kielkopf | first25=John | last26=Kraus | first26=Adam L.
 | last27=Law | first27=Nicolas | last28=Mann | first28=Andrew W.
 | last29=Mengel | first29=Matthew W. | last30=Morton | first30=Timothy D.
 | display-authors=1 | year=2019
 | arxiv=1905.05193 | doi=10.3847/2041-8213/ab322d | bibcode=2019ApJ...881L..19V | s2cid=153311715 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 37124
  |      Constellation = Taurus (constellation){{!}}Taurus
  |    Right ascension = {{RA|05|37|02.49}}
  |        Declination = {{DEC|+20|43|50.8}}
  | Apparent magnitude = 7.68
  |           Distance = 110
  |      Spectral type = G4V
  |               Mass = 0.830
  |             Radius = 0.824
  |        Temperature = 5606
  |        Metallicity = −0.442
  |                Age = 3.327
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Planet c orbits at the outer edge of the habitable zone.<ref name="Vogt2005">{{cite journal | title=Five New Multicomponent Planetary Systems | last1=Vogt | first1=Steven S. | last2=Butler | first2=R. Paul | last3=Marcy | first3=Geoffrey W. | last4=Fischer | first4=Debra A. | last5=Henry | first5=Gregory W. | last6=Laughlin | first6=Greg | last7=Wright | first7=Jason T. | last8=Johnson | first8=John A. | display-authors=1 | journal=The Astrophysical Journal | volume=632 | issue=1 | pages=638–658 | year=2005 | bibcode=2005ApJ...632..638V | doi=10.1086/432901 | s2cid=16509245 | access-date=2020-12-11 | url=https://authors.library.caltech.edu/36250/1/0004-637X_632_1_638.pdf | archive-date=2018-07-22 | archive-url=https://web.archive.org/web/20180722000634/https://authors.library.caltech.edu/36250/1/0004-637X_632_1_638.pdf | url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 20781
  |      Constellation = Fornax
  |    Right ascension = {{RA|03|20|03}}
  |        Declination = {{DEC|-28|47|02}}
  | Apparent magnitude = 8.44
  |           Distance = 115
  |      Spectral type = G9.5V
  |               Mass = 0.7
  |             Radius =
  |        Temperature =5256±29
  |        Metallicity =−0.11
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |Notes= Located in binary star system.<ref name=Udry2017>{{citation|arxiv=1705.05153|title=The HARPS search for southern extra-solar planets. XLII. Eight HARPS multi-planet systems hosting 20 super-Earth and Neptune-mass companions|year=2019|doi=10.1051/0004-6361/201731173|last1=Udry|first1=S.|last2=Dumusque|first2=X.|last3=Lovis|first3=C.|last4=Segransan|first4=D.|last5=Diaz|first5=R. F.|last6=Benz|first6=W.|last7=Bouchy|first7=F.|last8=Coffinet|first8=A.|last9=Lo Curto|first9=G.|last10=Mayor|first10=M.|last11=Mordasini|first11=C.|last12=Motalebi|first12=F.|last13=Pepe|first13=F.|last14=Queloz|first14=D.|last15=Santos|first15=N. C.|last16=Wyttenbach|first16=A.|last17=Alonso|first17=R.|last18=Collier Cameron|first18=A.|last19=Deleuil|first19=M.|last20=Figueira|first20=P.|last21=Gillon|first21=M.|last22=Moutou|first22=C.|last23=Pollacco|first23=D.|last24=Pompei|first24=E.|journal=Astronomy & Astrophysics|volume=A37|page=622|bibcode=2019A&A...622A..37U|s2cid=119095511}}</ref><ref>{{cite arXiv|eprint=1109.2497|class=astro-ph|title=The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets|author=Mayor, M.|author2=Marmier, M.|author3=Lovis, C.|author4=Udry, S.|author5=Ségransan, D.|author6=Pepe, F.|author7=Benz, W.|author8=Bertaux, J.-L.|author9=Bouchy, F.|author10=Dumusque, G.|author11=Curto, Lo|author12=Mordasini, C.|author13=Queloz, D.|author14=Santos, N. C.|date=2011|display-authors=etal}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-444
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|19|01}}
  |        Declination = {{DEC|41|38|05}}
  | Apparent magnitude = 9.0
  |           Distance = 117
  |      Spectral type = K0V
  |               Mass = 0.758
  |             Radius = 0.752
  |        Temperature = 5040
  |        Metallicity = -0.55
  |                Age = 11.23
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = Nearest multiplanetary system where the planets were discovered by the [[Kepler space telescope]].
}}
{{Multiplanetary systems list
  |               Star = HD 141399
  |      Constellation = Boötes
  |    Right ascension = {{RA|15|46|54.0}}
  |        Declination = {{DEC|+46|59|11}}
  | Apparent magnitude = 7.2
  |           Distance = 118
  |      Spectral type = K0V
  |               Mass = 1.07
  |             Radius = 1.46
  |        Temperature = 5600
  |        Metallicity = 0.35
  |                Age =  
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Planet c orbits in the habitable zone.<ref name=Hebrard2016HD141399c>{{Cite journal |doi=10.1051/0004-6361/201527585 |last1=Hébrard |first1=Guillaume |last2=Arnold |first2=Luc |last3=Forveille |first3=Thierry |last4=Correia |first4=Alexandre C. M. |last5=Laskar |first5=Jacques |last6=Bonfils |first6=Xavier |last7=Boisse |first7=Isabelle |last8=Díaz |first8=Rodrigo F. |last9=Hagelberg |first9=Janis |last10=Sahlmann |first10=Johannes |last11=Santos |first11=Nuno C. |display-authors=11 |author12=Nicola Astudillo-Defru |author13=Simon Borgniet |author14=François Bouchy |author15=Vincent Bourrier |author16=Bastien Courcol |author17=Xavier Delfosse |author18=Magali Deleuil |author19=Olivier D. S. Demangeon |author20=David Ehrenreich |author21=João Gregório |author22=N. Jovanovic |author23=Olivier Labrevoir |author24=Anne-Marie Lagrange |author25=Christophe Lovis |author26=J. Lozi |author27=Claire Moutou |author28=Guillaume Montagnier |author29=Francesco Pepe |author30=Javiera Rey |author31=Alexandre Santerne |author32=Damien Ségransan |author33=Stéphane Udry |author34=Michael Vanhuysse |author35=A. Vigan |author36=Paul A. Wilson |date=2016-04-01 |title=The SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozen |url=http://adsabs.harvard.edu/abs/2016A%26A...588A.145H |journal=Astronomy and Astrophysics |volume=588 |pages=A145 |issn=0004-6361 |arxiv=1602.04622 |bibcode=2016A&A...588A.145H |s2cid=55138055 |access-date=2022-02-26 |archive-date=2019-04-10 |archive-url=https://web.archive.org/web/20190410043711/http://adsabs.harvard.edu/abs/2016A%26A...588A.145H |url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-42
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|28|53}}
  |        Declination = {{DEC|+44|37|10}}
  | Apparent magnitude = 16.12
  |           Distance = 126
  |      Spectral type = M5V<ref name="MuirheadKOI961spectype">{{cite journal| author1=Philip S. Muirhead | author2=John Asher Johnson | author3=Kevin Apps | author4=Joshua A. Carter | author5=Timothy D. Morton | author6=Daniel C. Fabrycky | author7=J. Sebastian Pineda | author8=Michael Bottom | author9=Barbara Rojas-Ayala | author10=Everett Schlawin | author11=Katherine Hamren | author12=Kevin R. Covey | author13=Justin R. Crepp | author14=Keivan G. Stassun | author15=Joshua Pepper | author16=Leslie Hebb | author17=Evan N. Kirby | author18=Andrew W. Howard | author19=Howard T. Isaacson | author20=Geoffrey W. Marcy | author21=David Levitan | author22=Tanio Diaz-Santos | author23=Lee Armus | author24=James P. Lloyd |year=2012 | title=Characterizing the Cool KOIs III. KOI-961: A Small Star with Large Proper Motion and Three Small Planets | arxiv=1201.2189 | language=en | doi=10.1088/0004-637X/747/2/144 | volume=747 | issue=2 | journal=The Astrophysical Journal | page=144 | bibcode=2012ApJ...747..144M
| s2cid=14889361}}</ref>
  |               Mass = 0.13
  |             Radius = 0.17
  |        Temperature = 3068
  |        Metallicity = -0.48
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 31527
  |      Constellation = Lepus
  |    Right ascension = {{RA|04|55|38}}
  |        Declination = {{DEC|-23|14|31}}
  | Apparent magnitude = 7.48
  |           Distance = 126
  |      Spectral type = G0V
  |               Mass =
  |             Radius =
  |        Temperature =
  |        Metallicity =
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 10180
  |      Constellation = Hydrus
  |    Right ascension = {{RA|01|37|53.58}}
  |        Declination = {{DEC|−60|30|41.5}}
  | Apparent magnitude = 7.33
  |           Distance = 127
  |      Spectral type = G1V
  |               Mass = 1.055
  |             Radius = 1.085
  |        Temperature = 5911
  |        Metallicity = 0.083
  |                Age = 4.335
  |  Confirmed planets = 6
  |Unconfirmed planets = 3
  |              Notes = Has three unconfirmed candidates. If these candidate exoplanets were confirmed,  HD 10180 would have the largest planetary system of any star.<ref name=TuomiHD10180>{{cite journal|last=Tuomi|first=Mikko|title=Evidence for 9 planets in the 10180 system|journal=Astronomy & Astrophysics|volume=543|pages=A52|date=6 April 2012|arxiv=1204.1254v1|doi=10.1051/0004-6361/201118518|bibcode = 2012A&A...543A..52T |s2cid=15876919}}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 23472
  |      Constellation = Reticulum{{!}}Reticulum
  |    Right ascension = {{RA|03|41|50.3988}}
  |        Declination = {{DEC|-62|46|01.4772}}
  | Apparent magnitude = 9.72
  |           Distance = 127.48
  |      Spectral type = K3.5V
  |               Mass = 0.67
  |             Radius = 0.71
  |        Temperature = 4684{{±|99}}
  |        Metallicity = -0.2
  |                Age = 
  |  Confirmed planets = 5
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = HR 8799
  |      Constellation = Pegasus
  |    Right ascension = {{RA|23|07|28.72}}
  |        Declination = {{DEC|+21|08|03.3}}
  | Apparent magnitude = 5.96
  |           Distance = 129
  |      Spectral type = A5V
  |               Mass = 1.472
  |             Radius = 1.339
  |        Temperature = 7429
  |        Metallicity = −0.466
  |                Age = 0.064
  |  Confirmed planets = 4
  |Unconfirmed planets = 1
  |              Notes = Only [[A-type main sequence star]] with a known multiplanetary system, and hottest and most massive single main sequence star with a multiplanetary system. All four planets are massive [[super-Jupiter]]s.
}}
{{Multiplanetary systems list
  |               Star = HD 27894
  |      Constellation = Reticulum
  |    Right ascension = {{RA|04|20|47.05}}
  |        Declination = {{DEC|−59|24|39.0}}
  | Apparent magnitude = 9.42
  |           Distance = 138
  |      Spectral type = K2V
  |               Mass = 0.8
  |             Radius =
  |        Temperature = 4875
  |        Metallicity = 0.3
  |                Age = 3.9
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = [[HD 93385]]
  |      Constellation = Vela (constellation){{!}}Vela
  |    Right ascension = {{RA|10|46|15.1160}}
  |        Declination = {{DEC|-41|27|51.7261}}
  | Apparent magnitude = 7.486
  |           Distance = 141.6
  |      Spectral type = G2V
  |               Mass = 1.07
  |             Radius = 1.17
  |        Temperature = 5823
  |        Metallicity = -0.05
  |                Age = 4.13
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[K2-3]]
  |      Constellation = Leo (constellation){{!}}Leo
  |    Right ascension = {{RA|11|29|20.3918}}
  |        Declination = {{DEC|-01|27|17.280}}
  | Apparent magnitude = 12.168
  |           Distance = 143.9{{±|0.4}}
  |      Spectral type = M0V
  |               Mass = 0.601
  |             Radius = 0.561±0.068
  |        Temperature = 3835±70
  |        Metallicity = -0.01±0.09
  |                Age = 1
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = The outermost planet orbits in the habitable zone.<ref name=ScienceNewsK2-3>{{Cite web |url=http://www.sci-news.com/astronomy/science-three-super-earths-red-dwarf-02412.html |title=Three Super-Earths Found Circling Nearby Red Dwarf |access-date=2022-02-27 |archive-date=2019-01-02 |archive-url=https://web.archive.org/web/20190102064436/http://www.sci-news.com/astronomy/science-three-super-earths-red-dwarf-02412.html |url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 34445
  |      Constellation = Orion (constellation){{!}}Orion
  |    Right ascension = {{RA|05|17|41.0}}
  |        Declination = {{DEC|+07|21|12}}
  | Apparent magnitude = 7.31
  |           Distance = 152
  |      Spectral type = G0V
  |               Mass = 1.07
  |             Radius = 1.38
  |        Temperature = 5836
  |        Metallicity = 0.14
  |                Age = 8.5
  |  Confirmed planets = 1
  |Unconfirmed planets = 5
  |              Notes = Some planets were not detected or inferred to be false positives in a later study.<ref name="Rosenthal2021_61VirD">{{cite journal |arxiv=2105.11583|doi=10.3847/1538-4365/abe23c|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|year=2021|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973 |doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 204313
  |      Constellation = Capricornus
  |    Right ascension = {{RA|21|28|12.21}}
  |        Declination = {{DEC|–21|43|34.5}}
  | Apparent magnitude = 7.99
  |           Distance = 154
  |      Spectral type = G5V
  |               Mass = 1.045
  |             Radius =
  |        Temperature = 5767
  |        Metallicity = 0.18
  |                Age = 3.38
  |  Confirmed planets = 3
  |Unconfirmed planets = 
}}
{{Multiplanetary systems list
  |               Star = HD 3167
  |      Constellation = Pisces (constellation){{!}}Pisces
  |    Right ascension = {{RA|00|34|57.5}}
  |        Declination = {{DEC|+04|22|53}}
  | Apparent magnitude = 8.97
  |           Distance = 154.4
  |      Spectral type = K0V
  |               Mass = 0.852
  |             Radius = 0.871
  |        Temperature = 5300
  |        Metallicity = 0.04
  |                Age = 10.2
  |  Confirmed planets = 4
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HIP 34269
  |      Constellation = Puppis (constellation){{!}}Puppis
  |    Right ascension = {{RA|07|06|13.98}}
  |        Declination = {{DEC|-47|35|13.87}}
  | Apparent magnitude = 10.59
  |           Distance = 154.81
  |      Spectral type = 
  |               Mass = 0.74
  |             Radius = 
  |        Temperature = 4440{{±|100}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[HD 133131]]
  |      Constellation = Libra (constellation){{!}}Libra
  |    Right ascension = {{RA|15|03|35.80651}}
  |        Declination = {{DEC|-27|50|27.5520}}
  | Apparent magnitude = 8.4
  |           Distance = 168
  |      Spectral type = G2V+G2V<ref name=TeskeHD />
  |               Mass = 0.95
  |             Radius = 
  |        Temperature = 5799±19
  |        Metallicity = -0.3
  |                Age = 6
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |Notes = 2 planets around primary, and 1 planet around secondary star.<ref name=TeskeHD>{{cite journal|bibcode=2016AJ....152..167T|doi=10.3847/0004-6256/152/6/167|arxiv=1608.06216|title=The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B|journal=The Astronomical Journal|volume=152|issue=6|pages=167|year=2016|last1=Teske|first1=Johanna K|last2=Shectman|first2=Stephen A|last3=Vogt|first3=Steve S|last4=Díaz|first4=Matías|last5=Butler|first5=R. Paul|last6=Crane|first6=Jeffrey D|last7=Thompson|first7=Ian B|last8=Arriagada|first8=Pamela|s2cid=118852162 |doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[K2-136]]
  |      Constellation = Taurus (constellation){{!}}Taurus
  |    Right ascension = {{RA|04|29|38.99}}
  |        Declination = {{DEC|+22|52|57.80}}
  | Apparent magnitude = 11.2
  |           Distance = 173
  |      Spectral type = K5V
  |               Mass = 0.71
  |             Radius = 0.71
  |        Temperature = 4364{{±|70}}
  |        Metallicity = 0.15
  |                Age = 0.7
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = HIP 14810
  |      Constellation = Aries (constellation){{!}}Aries
  |    Right ascension = {{RA|03|11|14.23}}
  |        Declination = {{DEC|+21|05|50.5}}
  | Apparent magnitude = 8.51
  |           Distance = 174
  |      Spectral type = G5V
  |               Mass = 0.989
  |             Radius = 1.024
  |        Temperature = 5485
  |        Metallicity = 0.230
  |                Age = 5.271
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 191939
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|20|08|05.75}}
  |        Declination = {{DEC|+66|51|2.1}}
  | Apparent magnitude = 8.971
  |           Distance = 175
  |      Spectral type = G9V
  |               Mass = 0.81
  |             Radius = 0.94
  |        Temperature = 5348
  |        Metallicity = -0.15
  |                Age = 8.7
  |  Confirmed planets = 6
  |Unconfirmed planets = 
  |              Notes = <ref name="Orell-Miquel2022">{{cite journal |arxiv=2211.00667|last1=Orell-Miquel |first1=J. |last2=Nowak |first2=G. |last3=Murgas |first3=F. |last4=Palle |first4=E. |last5=Morello |first5=G. |last6=Luque |first6=R. |last7=Badenas-Agusti |first7=M. |last8=Ribas |first8=I. |last9=Lafarga |first9=M. |last10=Espinoza |first10=N. |last11=Morales |first11=J. C. |last12=Zechmeister |first12=M. |last13=Alqasim |first13=A. |last14=Cochran |first14=W. D. |last15=Gandolfi |first15=D. |last16=Goffo |first16=E. |last17=Kabáth |first17=P. |last18=Korth |first18=J. |last19=Livingston |first19=J. |last20=Lam |first20=K. W. F. |last21=Muresan |first21=A. |last22=Persson |first22=C. M. |last23=Van Eylen |first23=V. |title=HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone |journal=Astronomy & Astrophysics |year=2023 |volume=669 |pages=A40 |doi=10.1051/0004-6361/202244120 |bibcode=2023A&A...669A..40O |s2cid=253197272 }}</ref>

}}
{{Multiplanetary systems list
  |               Star = HD 125612
  |      Constellation = Virgo (constellation){{!}}Virgo
  |    Right ascension = {{RA|14|20|53.51}}
  |        Declination = {{DEC|−17|28|53.5}}
  | Apparent magnitude = 8.33
  |           Distance = 177
  |      Spectral type = G3V
  |               Mass = 1.099
  |             Radius = 1.052
  |        Temperature = 5897
  |        Metallicity = 0.244
  |                Age = 2.150
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 184010
  |      Constellation = Vulpecula
  |    Right ascension = {{RA|19|31|22.0}}
  |        Declination = {{DEC|+26|37|02}}
  | Apparent magnitude = 5.9
  |           Distance = 200
  |      Spectral type = KOIII-IV
  |               Mass = 1.35
  |             Radius = 4.86
  |        Temperature = 4971
  |        Metallicity = -0.17
  |                Age = 2.76
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 109271
  |      Constellation = Virgo (constellation){{!}}Virgo
  |    Right ascension = {{RA|12|33|36.0}}
  |        Declination = {{DEC|-11|37|19}}
  | Apparent magnitude = 8.05
  |           Distance = 202
  |      Spectral type = G5
  |               Mass = 1.047
  |             Radius =
  |        Temperature = 5783
  |        Metallicity = 0.1
  |                Age = 7.3
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
}}
{{Multiplanetary systems list
  |               Star = HD 38677
  |      Constellation = Orion (constellation){{!}}Orion
  |    Right ascension = {{RA|05|47|06.0}}
  |        Declination = {{DEC|−10|37|49″}}
  | Apparent magnitude = 8.0
  |           Distance = 202
  |      Spectral type = F8V
  |               Mass = 1.21
  |             Radius = 1.26
  |        Temperature = 6196.0
  |        Metallicity =  
  |                Age = 2.01
  |  Confirmed planets = 4
  |Unconfirmed planets =  
}}
{{Multiplanetary systems list
  |               Star = [[TOI-178]]
  |      Constellation = Sculptor (constellation){{!}}Sculptor
  |    Right ascension = {{RA|00|29|12.30}}
  |        Declination = {{DEC|30|27|13.46}}
  | Apparent magnitude = 11.95
  |           Distance = 205.16
  |      Spectral type = K7V<ref name="TOI178">{{Cite journal| last1=Leleu | first1=A. | last2=Alibert | first2=Y. | last3=Hara | first3=N. C. | last4=Hooton | first4=M. J. | last5=Wilson | first5=T. G. | last6=Robutel | first6=P. | last7=Delisle | first7=J.-B. | last8=Laskar | first8=J. | last9=Hoyer | first9=S. | last10=Lovis | first10=C. | last11=Bryant | first11=E. M. | last12=Ducrot | first12=E. | last13=Cabrera | first13=J. | last14=Delrez | first14=L. | last15=Acton | first15=J. S. | last16=Adibekyan | first16=V. | last17=Allart | first17=R. | last18=Prieto | first18=Allende | last19=Alonso | first19=R. | last20=Alves | first20=D. | last21=Anderson | first21=D. R. | last22=Angerhausen | first22=D. | last23=Escudé | first23=Anglada | last24=Asquier | first24=J. | last25=Barrado | first25=D. | last26=Barros | first26=S. C. C. | last27=Baumjohann | first27=W. | last28=Bayliss | first28=D. | last29=Beck | first29=M. | last30=Beck | first30=T. | last31=Bekkelien | first31=A. | last32=Benz | first32=W. | last33=Billot | first33=N. | last34=Bonfanti | first34=A. | last35=Bonfils | first35=X. | last36=Bouchy | first36=F. | last37=Bourrier | first37=V. | last38=Boué | first38=G. | last39=Brandeker | first39=A. | last40=Broeg | first40=C. | last41=Buder | first41=M. | last42=Burdanov | first42=A. | last43=Burleigh | first43=M. R. | last44=Bárczy | first44=T. | last45=Cameron | first45=A. C. | last46=Chamberlain | first46=S. | last47=Charnoz | first47=S. | last48=Cooke | first48=B. F. | last49=Damme | first49=Corral Van | last50=Correia | first50=A. C. M. | last51=Cristiani | first51=S. | last52=Damasso | first52=M. | last53=Davies | first53=M. B. | last54=Deleuil | first54=M. | last55=Demangeon | first55=O. D. S. | last56=Demory | first56=B. -O. | last57=Marcantonio | first57=Di | last58=Persio | first58=Di | last59=Dumusque | first59=X. | last60=Ehrenreich | first60=D. | last61=Erikson | first61=A. | last62=Figueira | first62=P. | last63=Fortier | first63=A. | last64=Fossati | first64=L. | last65=Fridlund | first65=M. | last66=Futyan | first66=D. | last67=Gandolfi | first67=D. | last68=Muñoz | first68=García | last69=Garcia | first69=L. J. | last70=Gill | first70=S. | last71=Gillen | first71=E. | last72=Gillon | first72=M. | last73=Goad | first73=M. R. | last74=Hernández | first74=González | last75=I. | first75=J. | last76=Guedel | first76=M. | last77=Günther | first77=M. N. | last78=Haldemann | first78=J. | last79=Henderson | first79=B. | last80=Heng | first80=K. | last81=Hogan | first81=A. E. | last82=Isaak | first82=K. | last83=Jehin | first83=E. | last84=Jenkins | first84=J. S. | last85=Jordán | first85=A. | last86=Kiss | first86=L. | last87=Kristiansen | first87=M. H. | last88=Lam | first88=K. | last89=Lavie | first89=B. | last90=Etangs | first90=Lecavelier des | last91=Lendl | first91=M. | last92=Lillo-Box | first92=J. | last93=Curto | first93=Lo | last94=Magrin | first94=D. | last95=Martins | first95=C. J. A. P. | last96=Maxted | first96=P. F. L. | last97=McCormac | first97=J. | last98=Mehner | first98=A. | last99=Micela | first99=G. | last100=Molaro | first100=P. | last101=Moyano | first101=M. | last102=Murray | first102=C. A. | last103=Nascimbeni | first103=V. | last104=Nunes | first104=N. J. | last105=Olofsson | first105=G. | last106=Osborn | first106=H. P. | last107=Oshagh | first107=M. | last108=Ottensamer | first108=R. | last109=Pagano | first109=I. | last110=Pallé | first110=E. | last111=Pedersen | first111=P. P. | last112=Pepe | first112=F. A. | last113=Persson | first113=C. M. | last114=Peter | first114=G. | last115=Piotto | first115=G. | last116=Polenta | first116=G. | last117=Pollacco | first117=D. | last118=Poretti | first118=E. | last119=Pozuelos | first119=F. J. | last120=Queloz | first120=D. | last121=Ragazzoni | first121=R. | last122=Rando | first122=N. | last123=Ratti | first123=F. | last124=Rauer | first124=H. | last125=Raynard | first125=L. | last126=Rebolo | first126=R. | last127=Reimers | first127=C. | last128=Ribas | first128=I. | last129=Santos | first129=N. C. | last130=Scandariato | first130=G. | last131=Schneider | first131=J. | last132=Sebastian | first132=D. | last133=Sestovic | first133=M. | last134=Simon | first134=A. E. | last135=Smith | first135=A. M. S. | last136=Sousa | first136=S. G. | last137=Sozzetti | first137=A. | last138=Steller | first138=M. | last139=Mascareño | first139=Suárez | last140=Szabó | first140=Gy. M. | last141=Ségransan | first141=D. | last142=Thomas | first142=N. | last143=Thompson | first143=S. | last144=Tilbrook | first144=R. H. | last145=Triaud | first145=A. | last146=Turner | first146=O. | last147=Udry | first147=S. | last148=Grootel | first148=Van | last149=Venus | first149=H. | last150=Verrecchia | first150=F. | last151=Vines | first151=J. I. | last152=Walton | first152=N. A. | last153=West | first153=R. G. | last154=Wheatley | first154=P. J. | last155=Wolter | first155=D. | last156=Osorio | first156=Zapatero | last157=R. | first157=M. | display-authors=20 |date=2021-01-20|title=Six transiting planets and a chain of Laplace resonances in TOI-178|journal=Astronomy & Astrophysics| volume=649 | pages=A26 |language=en|arxiv=2101.09260|doi=10.1051/0004-6361/202039767| bibcode=2021A&A...649A..26L |issn=0004-6361|s2cid=231693292 }}</ref>
  |               Mass = 0.65
  |             Radius = 0.651
  |        Temperature = 4316{{±|70}}
  |        Metallicity = -0.23
  |                Age = 7.1
  |  Confirmed planets = 6
  |Unconfirmed planets = 
  |              Notes = The planets are in an [[orbital resonance]].<ref name="TOI178"/>
}}
{{Multiplanetary systems list
  |               Star = [[HD 108236]]
  |      Constellation = Centaurus
  |    Right ascension = {{RA|12|26|17.89}}
  |        Declination = {{DEC|-51|21|46.21}}
  | Apparent magnitude = 9.24
  |           Distance = 211
  |      Spectral type = G3V
  |               Mass = 0.97
  |             Radius = 0.888
  |        Temperature = 5730
  |        Metallicity = -0.3
  |                Age = 5.8
  |  Confirmed planets = 5
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-37
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|58|23.1}}
  |        Declination = {{DEC|44|31|05}}
  | Apparent magnitude = 9.77
  |           Distance = 215
  |      Spectral type = G8V
  |               Mass = 0.803
  |             Radius = 0.770
  |        Temperature = 5417
  |        Metallicity = −0.32
  |                Age = 6
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes = The existence of Kepler-37e is dubious.<ref name=Rajpaul2021>{{citation|arxiv=2107.13900|year=2021|title=A HARPS-N mass for the elusive Kepler-37d: A case study in disentangling stellar activity and planetary signals|doi=10.1093/mnras/stab2192|last1=Rajpaul|first1=V. M.|last2=Buchhave|first2=L. A.|last3=Lacedelli|first3=G.|last4=Rice|first4=K.|last5=Mortier|first5=A.|last6=Malavolta|first6=L.|last7=Aigrain|first7=S.|last8=Borsato|first8=L.|last9=Mayo|first9=A. W.|last10=Charbonneau|first10=D.|last11=Damasso|first11=M.|last12=Dumusque|first12=X.|last13=Ghedina|first13=A.|last14=Latham|first14=D. W.|last15=López-Morales|first15=M.|last16=Magazzù|first16=A.|last17=Micela|first17=G.|last18=Molinari|first18=E.|last19=Pepe|first19=F.|last20=Piotto|first20=G.|last21=Poretti|first21=E.|last22=Rowther|first22=S.|last23=Sozzetti|first23=A.|last24=Udry|first24=S.|last25=Watson|first25=C. A.|journal=Monthly Notices of the Royal Astronomical Society|volume=507|issue=2|pages=1847–1868 |doi-access=free |bibcode=2021MNRAS.507.1847R}} Kepler-37e is discussed in sections 2.2.2 & 6.4.</ref>
}}
{{Multiplanetary systems list
  |               Star = [[K2-72]]
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|18|29.2548}}
  |        Declination = {{DEC|-09|36|44.3824}}
  | Apparent magnitude = 15.04
  |           Distance = 217
  |      Spectral type = M2V
  |               Mass = 0.27
  |             Radius = 0.33
  |        Temperature = 3497
  |        Metallicity = -0.271
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = 2 planets in habitable zone
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-138]]
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|21|32.0}}
  |        Declination = {{DEC|+43|17|35}}
  | Apparent magnitude = 13.5
  |           Distance = 218.5
  |      Spectral type = M1V
  |               Mass = 0.57
  |             Radius = 0.54
  |        Temperature = 3871
  |        Metallicity =
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-233
  |      Constellation = Libra (constellation){{!}}Libra
  |    Right ascension = {{RA|15|21|55.2}}
  |        Declination = {{DEC|-20|13|54}}
  | Apparent magnitude = 10.0
  |           Distance = 221
  |      Spectral type = K3
  |               Mass = 0.80
  |             Radius = 0.74
  |        Temperature = 4950
  |        Metallicity = 0.07
  |                Age = 0.36
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = TOI-1260
  |      Constellation = Ursa Major
  |    Right ascension = {{RA|10|28|35.03}}
  |        Declination = {{DEC|+65|51|16.38}}
  | Apparent magnitude = 11.973
  |           Distance = 239.5
  |      Spectral type = 
  |               Mass = 0.66
  |             Radius = 0.672
  |        Temperature = 4227{{±|85}}
  |        Metallicity = -0.1
  |                Age = 6.7
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = LP 358-499
  |      Constellation = Taurus (constellation){{!}}Taurus
  |    Right ascension = {{RA|04|40|35.64}}
  |        Declination = {{DEC|+25|00|36.05}}
  | Apparent magnitude = 13.996
  |           Distance = 245.3
  |      Spectral type = 
  |               Mass = 0.46
  |             Radius = 
  |        Temperature = 3655{{±|80}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = Also known as K2-133
}}
{{Multiplanetary systems list
  |               Star = K2-266
  |      Constellation = Sextans{{!}}Sextans
  |    Right ascension = {{RA|10|31|44.5}}
  |        Declination = {{DEC|+00|56|15}}
  | Apparent magnitude = 
  |           Distance = 252
  |      Spectral type = K
  |               Mass = 0.69
  |             Radius = 0.7
  |        Temperature = 4285
  |        Metallicity = -0.12
  |                Age = 8.4
  |  Confirmed planets = 4
  |Unconfirmed planets = 2
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-155
  |      Constellation = Taurus (constellation){{!}}Taurus
  |    Right ascension = {{RA|04|21|52.5}}
  |        Declination = {{DEC|+21|21|13}}
  | Apparent magnitude = 12.8
  |           Distance = 267 
  |      Spectral type = K7
  |               Mass = 0.65
  |             Radius = 0.58
  |        Temperature = 4258
  |        Metallicity = -0.3
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-384
  |      Constellation = Cetus (constellation){{!}}Cetus
  |    Right ascension = {{RA|01|21|59.86}}
  |        Declination = {{DEC|00|45|04.41}}
  | Apparent magnitude = 16.12
  |           Distance = 270
  |      Spectral type = M?V
  |               Mass = 0.33
  |             Radius = 
  |        Temperature = 3623{{±|138}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 5
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[TOI-1136]]
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|12|48|44.38 }}
  |        Declination = {{DEC|+64|51|18.99}}
  | Apparent magnitude = 9.534
  |           Distance = 275.8
  |      Spectral type = 
  |               Mass = 1.022
  |             Radius = 0.968
  |        Temperature = 5770{{±|50}}
  |        Metallicity = 0.07
  |                Age = 0.7
  |  Confirmed planets = 6
  |Unconfirmed planets = 1
  |              Notes = The planets are in an orbital resonance.<ref name="Dai2023">{{cite journal |last1=Dai |first1=Fei |last2=Masuda |first2=Kento |display-authors=etal |date=February 2023 |title=TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain |journal=[[The Astronomical Journal]] |volume=165 |issue=2 |page=33 |doi=10.3847/1538-3881/aca327 |doi-access=free |arxiv=2210.09283 |bibcode=2023AJ....165...33D}}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[TOI-561]]
  |      Constellation = Sextans (constellation){{!}}Sextans
  |    Right ascension = {{RA|09|52|44.44}}
  |        Declination = {{DEC|+06|12|57.97}}
  | Apparent magnitude = 10.252
  |           Distance = 279
  |      Spectral type = G9V
  |               Mass = 0.785
  |             Radius = 0.849
  |        Temperature = 5455
  |        Metallicity = -0.33
  |                Age = 5
  |  Confirmed planets = 4
  |Unconfirmed planets = 1
}}
{{Multiplanetary systems list
  |               Star = Kepler-445
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|54|57.0}}
  |        Declination = {{DEC|+46|29|55}}
  | Apparent magnitude = 18
  |           Distance = 294
  |      Spectral type =  
  |               Mass = 0.18
  |             Radius = 0.21
  |        Temperature = 3157
  |        Metallicity = 0.19
  |                Age =  
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = [[TOI-763]]
  |      Constellation = Centaurus (constellation){{!}}Centaurus
  |    Right ascension = {{RA|12|57|52.45}}
  |        Declination = {{DEC|−39|45|27.71}}
  | Apparent magnitude = 10.156
  |           Distance = 311
  |      Spectral type = 
  |               Mass = 0.917
  |             Radius = 0.897
  |        Temperature = 5444
  |        Metallicity = 0.01
  |                Age = 6.2
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
}}
{{Multiplanetary systems list
  |               Star = [[K2-229]]
  |      Constellation = Virgo (constellation){{!}}Virgo
  |    Right ascension = {{RA|12|27|29.5848}}
  |        Declination = {{DEC|−06|43|18.7660}}
  | Apparent magnitude = 10.985
  |           Distance = 335
  |      Spectral type = K2V
  |               Mass = 0.837
  |             Radius = 0.793
  |        Temperature = 5185
  |        Metallicity = −0.06
  |                Age = 5.4
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |Notes = 
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-102]]
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|45|55.9}}
  |        Declination = {{DEC|+47|12|29}}
  | Apparent magnitude = 11.492
  |           Distance = 340
  |      Spectral type = K3V<ref name=SIMBAD_Kepler-102>{{cite simbad|title=KOI-82|access-date=20 March 2022}}</ref>
  |               Mass = 0.81
  |             Radius = 0.76 
  |        Temperature = 4809
  |        Metallicity = 0.18 
  |                Age = 1.41
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[V1298 Tauri]]
  |      Constellation = Taurus (constellation){{!}}Taurus
  |    Right ascension = {{RA|04|05|19.5912}}
  |        Declination = {{DEC|+20|09|25.5635}}
  | Apparent magnitude = 10.31
  |           Distance = 354
  |      Spectral type = K0-1.5<ref name="David_et_al_V1298Taurispectype">{{Cite journal|last1=David|first1=Trevor J.|last2=Cody|first2=Ann Marie|last3=Hedges|first3=Christina L.|last4=Mamajek|first4=Eric E.|last5=Hillenbrand|first5=Lynne A.|last6=Ciardi|first6=David R.|last7=Beichman|first7=Charles A.|last8=Petigura|first8=Erik A.|last9=Fulton|first9=Benjamin J.|last10=Isaacson|first10=Howard T.|last11=Howard|first11=Andrew W.|date=August 2019|title=A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau|journal=The Astronomical Journal|language=en|volume=158|issue=2|pages=79|doi=10.3847/1538-3881/ab290f|arxiv=1902.09670|bibcode=2019AJ....158...79D|s2cid=119003936|issn=0004-6256 |doi-access=free }}</ref>
  |               Mass = 1.101
  |             Radius = 1.345
  |        Temperature = 4970
  |        Metallicity = 
  |                Age = 0.023
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = This star is a young [[T Tauri variable]].<ref name="David et al 2">{{Cite journal|last1=David|first1=Trevor J.|last2=Petigura|first2=Erik A.|last3=Luger|first3=Rodrigo|last4=Foreman-Mackey|first4=Daniel|last5=Livingston|first5=John H.|last6=Mamajek|first6=Eric E.|last7=Hillenbrand|first7=Lynne A.|date=2019-10-29|title=Four Newborn Planets Transiting the Young Solar Analog V1298 Tau|journal=The Astrophysical Journal|volume=885|issue=1|pages=L12|arxiv=1910.04563|bibcode=2019ApJ...885L..12D|doi=10.3847/2041-8213/ab4c99|s2cid=204008446|issn=2041-8213 |doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[K2-302]]
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|20|22.7764}}
  |        Declination = {{DEC|-09|30|34.2934}}
  | Apparent magnitude = 11.98
  |           Distance = 359.3
  |      Spectral type = 
  |               Mass = 
  |             Radius = 0.25
  |        Temperature = 3297{{±|73}}
  |        Metallicity = -0.33
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-198
  |      Constellation = Virgo (constellation){{!}}Virgo
  |    Right ascension = {{RA|13|15|22.5}}
  |        Declination = {{DEC|-06|27|54}}
  | Apparent magnitude = 11.0
  |           Distance = 362
  |      Spectral type = 
  |               Mass = 0.8
  |             Radius = 0.76
  |        Temperature = 5213
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[TOI-125]]
  |      Constellation = Hydrus{{!}}Hydrus
  |    Right ascension = {{RA|01|34|22.73}}
  |        Declination = {{DEC|-66|40|32.95}}
  | Apparent magnitude = 11.02
  |           Distance = 363 
  |      Spectral type = 
  |               Mass = 0.859 
  |             Radius = 
  |        Temperature = 5320
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 2
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = HIP 41378
  |      Constellation = Cancer (constellation){{!}}Cancer
  |    Right ascension = {{RA|08|26|28.0}}
  |        Declination = {{DEC|+10|04|49}}
  | Apparent magnitude = 8.9
  |           Distance = 378
  |      Spectral type = F8
  |               Mass = 1.15
  |             Radius = 1.4
  |        Temperature = 6199
  |        Metallicity = -0.11
  |                Age = 
  |  Confirmed planets = 5
  |Unconfirmed planets = 2
  |              Notes = Planet f has an unusually low density, and might have rings or an extended atmosphere.<ref name=HIP_41378_f>{{Cite journal|last1=Akinsanmi|first1=B.|last2=Santos|first2=N. C.|last3=Faria|first3=J. P.|last4=Oshagh|first4=M.|last5=Barros|first5=S. C. C.|last6=Santerne|first6=A.|last7=Charnoz|first7=S.|date=2020-03-01|title=Can planetary rings explain the extremely low density of HIP 41378 𝑓?|url=https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|journal=Astronomy & Astrophysics|language=en|volume=635|pages=L8|doi=10.1051/0004-6361/202037618|arxiv=2002.11422|issn=0004-6361|doi-access=free|access-date=2022-03-19|archive-date=2021-10-28|archive-url=https://web.archive.org/web/20211028001745/https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|url-status=live}}</ref><ref name=santerneHIP41378f>{{cite arXiv|eprint=1911.07355|last1=Santerne|first1=A.|title=An extremely low-density and temperate giant exoplanet|last2=Malavolta|first2=L.|last3=Kosiarek|first3=M. R.|last4=Dai|first4=F.|last5=Dressing|first5=C. D.|last6=Dumusque|first6=X.|last7=Hara|first7=N. C.|last8=Lopez|first8=T. A.|last9=Mortier|first9=A.|last10=Vanderburg|first10=A.|last11=Adibekyan|first11=V.|last12=Armstrong|first12=D. J.|last13=Barrado|first13=D.|last14=Barros|first14=S. C. C.|last15=Bayliss|first15=D.|last16=Berardo|first16=D.|last17=Boisse|first17=I.|last18=Bonomo|first18=A. S.|last19=Bouchy|first19=F.|last20=Brown|first20=D. J. A.|last21=Buchhave|first21=L. A.|last22=Butler|first22=R. P.|last23=Collier Cameron|first23=A.|last24=Cosentino|first24=R.|last25=Crane|first25=J. D.|last26=Crossfield|first26=I. J. M.|last27=Damasso|first27=M.|last28=Deleuil|first28=M. R.|last29=Delgado Mena|first29=E.|last30=Demangeon|first30=O.|display-authors=29|class=astro-ph.EP|year=2019}}</ref> More planets are still suspected.<ref name="Vanderburg_HIP_41378">{{Cite journal| author = Andrew Vanderburg|display-authors=etal
| author-link =
| arxiv       =1606.08441
| title       =Five Planets Transiting a Ninth Magnitude Star
| journal     =The Astrophysical Journal
| volume      =827
| issue       =1
| pages       =L10
| language    =en
| year        =2016
| doi         =10.3847/2041-8205/827/1/L10
| bibcode     =2016ApJ...827L..10V
|s2cid=8794583
|doi-access=free
}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-446
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|49|00.0}}
  |        Declination = {{DEC|+44|55|16}}
  | Apparent magnitude = 16.5
  |           Distance = 391
  |      Spectral type = M4V
  |               Mass = 0.22
  |             Radius = 0.24
  |        Temperature = 3359
  |        Metallicity = -0.3
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = HD 33142
  |      Constellation = Lepus (constellation){{!}}Lepus
  |    Right ascension = {{RA|05|07|35.54}}
  |        Declination = {{DEC|-13|59|11.34}}
  | Apparent magnitude = 7.96
  |           Distance = 394.3
  |      Spectral type = 
  |               Mass = 1.52
  |             Radius = 
  |        Temperature = 5025{{±|24|16}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = Host star is 
a giant star with spectral type of K0III.<ref>{{Cite web |last=Martin |first=Pierre-Yves |date=2022 |title=Planet HD 33142 c |url=https://exoplanet.eu/catalog/hd_33142_c--6882/ |access-date=2024-02-03 |website=exoplanet.eu |language=en |archive-date=2024-02-03 |archive-url=https://web.archive.org/web/20240203050836/https://exoplanet.eu/catalog/hd_33142_c--6882/ |url-status=live }}</ref> 
}}
{{Multiplanetary systems list
  |               Star = WASP-132
  |      Constellation = Lupus (constellation){{!}}Lupus
  |    Right ascension = {{RA|14|30|26.2}}
  |        Declination = {{DEC|-46|09|33}}
  | Apparent magnitude = 11.938
  |           Distance = 403
  |      Spectral type = K4V
  |               Mass = 0.782
  |             Radius = 0.753
  |        Temperature = 4714
  |        Metallicity = 0.18
  |                Age = 7.2
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = K2-148
  |      Constellation = Cetus (constellation){{!}}Cetus
  |    Right ascension = {{RA|00|58|04.28}}
  |        Declination = {{DEC|-00|11|35.36}}
  | Apparent magnitude = 13.05
  |           Distance = 407
  |      Spectral type = K7V
  |               Mass = 0.65
  |             Radius = 0.63
  |        Temperature = 4079{{±|70}}
  |        Metallicity = -0.11
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = A secondary red dwarf is gravitationally bound to K2-148.<ref name=K2-148>{{Cite journal |arxiv = 1710.03239|doi = 10.3847/1538-3881/aaa9c1|title = Exoplanets around Low-mass Stars Unveiled by K2|journal = The Astronomical Journal|volume = 155|issue = 3|pages = 127|year = 2018|last1 = Hirano|first1 = Teruyuki|last2 = Dai|first2 = Fei|last3 = Gandolfi|first3 = Davide|last4 = Fukui|first4 = Akihiko|last5 = Livingston|first5 = John H.|last6 = Miyakawa|first6 = Kohei|last7 = Endl|first7 = Michael|last8 = Cochran|first8 = William D.|last9 = Alonso-Floriano|first9 = Francisco J.|last10 = Kuzuhara|first10 = Masayuki|last11 = Montes|first11 = David|last12 = Ryu|first12 = Tsuguru|last13 = Albrecht|first13 = Simon|last14 = Barragan|first14 = Oscar|last15 = Cabrera|first15 = Juan|last16 = Csizmadia|first16 = Szilard|last17 = Deeg|first17 = Hans|last18 = Eigmüller|first18 = Philipp|last19 = Erikson|first19 = Anders|last20 = Fridlund|first20 = Malcolm|last21 = Grziwa|first21 = Sascha|last22 = Guenther|first22 = Eike W.|last23 = Hatzes|first23 = Artie P.|last24 = Korth|first24 = Judith|last25 = Kudo|first25 = Tomoyuki|last26 = Kusakabe|first26 = Nobuhiko|last27 = Narita|first27 = Norio|last28 = Nespral|first28 = David|last29 = Nowak|first29 = Grzegorz|last30 = Pätzold|first30 = Martin|display-authors = 29|bibcode = 2018AJ....155..127H| s2cid=54590874 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-68
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|24|07.76}}
  |        Declination = {{DEC|+49|02|25.0}}
  | Apparent magnitude = 8.588
  |           Distance = 440
  |      Spectral type = G1V
  |               Mass = 1.079
  |             Radius = 1.243
  |        Temperature = 5793
  |        Metallicity = 0.12
  |                Age = 6.3
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes = Planet d, the outermost confirmed planet, is a Jupiter-sized planet which orbits in the habitable zone.<ref name="Gilliland2013Kepler-68">{{cite journal | title=Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants | last1=Gilliland | first1=Ronald L. | last2=Marcy | first2=Geoffrey W. | last3=Rowe | first3=Jason F. | last4=Rogers | first4=Leslie | last5=Torres | first5=Guillermo | last6=Fressin | first6=Francois | last7=Lopez | first7=Eric D. | last8=Buchhave | first8=Lars A. | last9=Christensen-Dalsgaard | first9=Jørgen | last10=Désert | first10=Jean-Michel | last11=Henze | first11=Christopher E. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Lissauer | first14=Jack J. | last15=Chaplin | first15=William J. | last16=Basu | first16=Sarbani | last17=Metcalfe | first17=Travis S. | last18=Elsworth | first18=Yvonne | last19=Handberg | first19=Rasmus | last20=Hekker | first20=Saskia | last21=Huber | first21=Daniel | last22=Karoff | first22=Christoffer | last23=Kjeldsen | first23=Hans | last24=Lund | first24=Mikkel N. | last25=Lundkvist | first25=Mia | last26=Miglio | first26=Andrea | last27=Charbonneau | first27=David | last28=Ford | first28=Eric B. | last29=Fortney | first29=Jonathan J. | last30=Haas | first30=Michael R. | display-authors=1 | journal=The Astrophysical Journal | volume=766 | issue=1 | at=40 | year=2013 | arxiv=1302.2596 | bibcode=2013ApJ...766...40G | bibcode-access=free | doi=10.1088/0004-637X/766/1/40 | doi-access=free }}</ref> Radial velocity measurements discovered an additional signal, which could be a fourth planet or a stellar companion.<ref name="Mills2019Kepler-68">{{cite journal | title=Long-period Giant Companions to Three Compact, Multiplanet Systems | last1=Mills | first1=Sean M. | last2=Howard | first2=Andrew W. | last3=Weiss | first3=Lauren M. | last4=Steffen | first4=Jason H. | last5=Isaacson | first5=Howard | last6=Fulton | first6=Benjamin J. | last7=Petigura | first7=Erik A. | last8=Kosiarek | first8=Molly R. | last9=Hirsch | first9=Lea A. | last10=Boisvert | first10=John H. | display-authors=1 | journal=The Astronomical Journal | volume=157 | issue=4 | at=145 | year=2019 | arxiv=1903.07186 | bibcode=2019AJ....157..145M | doi=10.3847/1538-3881/ab0899 | s2cid=119197547 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = HD 28109
  |      Constellation = Hydrus (constellation){{!}}Hydrus
  |    Right ascension = {{RA|04|20|57.13}}
  |        Declination = {{DEC|-68|06|09.51}}
  | Apparent magnitude = 9.38
  |           Distance = 457
  |      Spectral type = 
  |               Mass = 1.26
  |             Radius = 
  |        Temperature = 6120{{±|50}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = COROT-7
  |      Constellation = Monoceros
  |    Right ascension = {{RA|06|43|49.47}}
  |        Declination = {{DEC|−01|03|46.9}}
  | Apparent magnitude = 11.73
  |           Distance = 489
  |      Spectral type = K0V
  |               Mass = 0.93
  |             Radius = 0.87
  |        Temperature = 5275
  |        Metallicity = 0.03
  |                Age = 1.5
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = [[XO-2 (star)|XO-2]]
  |      Constellation = Lynx (constellation){{!}}Lynx
  |    Right ascension = {{RA|07|48|07.4814}}
  |        Declination = {{DEC|+50|13|03.2578}}
  | Apparent magnitude = 11.18
  |           Distance = 496±3
  |      Spectral type = K0V+K0V
  |               Mass = 
  |             Radius = 
  |        Temperature = 
  |        Metallicity = 
  |                Age = 6.3
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = Binary with each star orbited by two planets.<ref name="Desidera2014">{{cite journal | title=The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S | url=https://www.aanda.org/articles/aa/full_html/2014/07/aa24339-14/aa24339-14.html | last1=Desidera | first1=S. | last2=Bonomo | first2=A. S. | last3=Claudi | first3=R. U. | last4=Damasso | first4=M. | last5=Biazzo | first5=K. | last6=Sozzetti | first6=A. | last7=Marzari | first7=F. | last8=Benatti | first8=S. | last9=Gandolfi | first9=D. | last10=Gratton | first10=R. | last11=Lanza | first11=A. F. | last12=Nascimbeni | first12=V. | last13=Andreuzzi | first13=G. | last14=Affer | first14=L. | last15=Barbieri | first15=M. | last16=Bedin | first16=L. R. | last17=Bignamini | first17=A. | last18=Bonavita | first18=M. | last19=Borsa | first19=F. | last20=Calcidese | first20=P. | last21=Christille | first21=J. M. | last22=Cosentino | first22=R. | last23=Covino | first23=E. | last24=Esposito | first24=M. | last25=Giacobbe | first25=P. | last26=Harutyunyan | first26=A. | last27=Latham | first27=D. | last28=Lattanzi | first28=M. | last29=Leto | first29=G. | last30=Lodato | first30=G. | display-authors=1 | journal=Astronomy and Astrophysics | volume=567 | issue=6 | at=L6 | year=2014 | arxiv=1407.0251 | bibcode=2014A&A...567L...6D | doi=10.1051/0004-6361/201424339 | s2cid=118567085 | access-date=2022-06-25 | archive-date=2021-05-11 | archive-url=https://web.archive.org/web/20210511170517/https://www.aanda.org/articles/aa/full_html/2014/07/aa24339-14/aa24339-14.html | url-status=live }}</ref><ref name="Damasso et al">{{cite journal | title=A comprehensive analysis of the XO-2 stellar and planetary systems | last1=Damasso | first1=M. | last2=Biazzo | first2=K. | last3=Bonomo | first3=A. S. | last4=Desidera | first4=S. | last5=Lanza | first5=A. F. | last6=Nascimbeni | first6=V. | last7=Esposito | first7=M. | last8=Scandariato | first8=G. | last9=Sozzetti | first9=A. | last10=Cosentino | first10=R. | last11=Gratton | first11=R. | last12=Malavolta | first12=L. | last13=Rainer | first13=M. | last14=Gandolfi | first14=D. | last15=Poretti | first15=E. | last16=Zanmar Sanchez | first16=R. | last17=Ribas | first17=I. | last18=Santos | first18=N. | last19=Affer | first19=L. | last20=Andreuzzi | first20=G. | last21=Barbieri | first21=M. | last22=Bedin | first22=L. R. | last23=Benatti | first23=S. | last24=Bernagozzi | first24=A. | last25=Bertolini | first25=E. | last26=Bonavita | first26=M. | last27=Borsa | first27=F. | last28=Borsato | first28=L. | last29=Boschin | first29=W. | last30=Calcidese | first30=P. | last31=Carbognani | first31=A. | last32=Cenadelli | first32=D. | last33=Christille | first33=J. M. | last34=Claudi | first34=R. U. | last35=Covino | first35=E. | last36=Cunial | first36=A. | last37=Giacobbe | first37=P. | last38=Granata | first38=V. | last39=Harutyunyan | first39=A. | last40=Lattanzi | first40=M. G. | last41=Leto | first41=G. | last42=Libralato | first42=M. | last43=Lodato | first43=G. | last44=Lorenzi | first44=V. | last45=Mancini | first45=L. | last46=Martinez Fiorenzano | first46=A. F. | last47=Marzari | first47=F. | last48=Masiero | first48=S. | last49=Micela | first49=G. | last50=Molinari | first50=E. | last51=Molinaro | first51=M. | last52=Munari | first52=U. | last53=Murabito | first53=S. | last54=Pagano | first54=I. | last55=Pedani | first55=M. | last56=Piotto | first56=G. | last57=Rosenberg | first57=A. | last58=Silvotti | first58=R. | last59=Southworth | first59=J. | display-authors=1 | journal=Astronomy & Astrophysics | volume=575 | at=A111 | year=2015 | doi=10.1051/0004-6361/201425332 | doi-access=free | arxiv=1501.01424 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-411
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|10|25.3}}
  |        Declination = {{DEC|+49|31|24}}
  | Apparent magnitude = 12.5
  |           Distance = 499.4
  |      Spectral type = K3V
  |               Mass = 0.83
  |             Radius = 0.79
  |        Temperature = 4974
  |        Metallicity = 0.23
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-381
  |      Constellation = Sagittarius (constellation){{!}}Sagittarius
  |    Right ascension = {{RA|19|12|06.46}}
  |        Declination = {{DEC|-21|00|27.51}}
  | Apparent magnitude = 13.01
  |           Distance = 505
  |      Spectral type = K2
  |               Mass = 0.754
  |             Radius = 
  |        Temperature = 4473{{±|138}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-285
  |      Constellation = Pisces (constellation){{!}}Pisces
  |    Right ascension = {{RA|23|17|32.2}}
  |        Declination = {{DEC|+01|18|01}}
  | Apparent magnitude = 12.03
  |           Distance = 508
  |      Spectral type = K2V
  |               Mass = 0.83
  |             Radius = 0.79
  |        Temperature = 4975
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[K2-32]]
  |      Constellation = Ophiuchus (constellation){{!}}Ophiuchus
  |    Right ascension = {{RA|16|49|42.2602}}
  |        Declination = {{DEC|−19|32|34.151}}
  | Apparent magnitude = 12.31
  |           Distance = 510
  |      Spectral type = G9V
  |               Mass = 0.856
  |             Radius = 0.845
  |        Temperature = 5275
  |        Metallicity = -0.02
  |                Age = 7.9
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = The planets are likely in a 1:2:5:7 orbital resonance.<ref name="Heller2019K2-32">{{cite journal | title=Transit least-squares survey. I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance | url=https://www.aanda.org/articles/aa/full_html/2019/05/aa35276-19/aa35276-19.html | last1=Heller | first1=René | last2=Rodenbeck | first2=Kai | last3=Hippke | first3=Michael | journal=Astronomy and Astrophysics | volume=625 | at=A31 | year=2019 | arxiv=1904.00651 | bibcode=2019A&A...625A..31H | bibcode-access=free | doi=10.1051/0004-6361/201935276 | doi-access=free | access-date=2022-03-04 | archive-date=2022-01-25 | archive-url=https://web.archive.org/web/20220125190022/https://www.aanda.org/articles/aa/full_html/2019/05/aa35276-19/aa35276-19.html | url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = TOI-1246
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|16|44|27.96}}
  |        Declination = {{DEC|70|25|46.70}}
  | Apparent magnitude = 11.6
  |           Distance = 558
  |      Spectral type = 
  |               Mass = 1.12
  |             Radius = 
  |        Temperature = 5217{{±|50}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes =
}}

{{Multiplanetary systems list
  |               Star = [[K2-352]]
  |      Constellation = Cancer (constellation){{!}}Cancer
  |    Right ascension = {{RA|09|21|46.8434}}
  |        Declination = {{DEC|+18|28|10.34710}}
  | Apparent magnitude = 11.12
  |           Distance = 577
  |      Spectral type = G2V
  |               Mass = 0.98
  |             Radius = 0.95
  |        Temperature = 5791
  |        Metallicity = -0.05
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-398
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|25|52.5}}
  |        Declination = {{DEC|+40|20|38}}
  | Apparent magnitude = 
  |           Distance = 578
  |      Spectral type = K5V
  |               Mass = 0.72
  |             Radius = 0.67
  |        Temperature = 4493
  |        Metallicity = -0.046
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-186
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|54|36.6}}
  |        Declination = {{DEC|+43|57|18}}
  | Apparent magnitude = 15.29<ref name="Souto2017">{{Cite journal|arxiv=1612.01598|last1=Souto|first1=Diogo|title=Chemical Abundances of M-dwarfs from the APOGEE Survey. I. The Exoplanet Hosting Stars Kepler-138 and Kepler-186|journal=The Astrophysical Journal|volume=835|issue=2|pages=239|last2=Cunha|first2=Katia|last3= Garcia-Hernandez|first3=D. A.|last4=Zamora|first4=Olga|last5= Allende Prieto|first5=C.|last6=Smith|first6=Verne|last7=Mahadevan|first7=Suvrath|last8=Blake|first8=Cullen|last9= Johnson|first9=J. A.|last10=Jonsson|first10=Henrik|last11=Pinsonneault|first11=Marc|last12=Holtzman|first12=Jon|last13= Majewski|first13=S. R.|last14=Shetrone|first14=Matthew|last15=Teske|first15=Johanna|last16=Nidever|first16=David|last17=Schiavon|first17=Ricardo|last18=Sobeck|first18=Jennifer|last19= Garcia Perez|first19=A. E.|last20= Gomez Maqueo Chew|first20=Y.|last21=Stassun|first21=Keivan|display-authors=1|year=2017|bibcode=2017ApJ...835..239S|doi=10.3847/1538-4357/835/2/239|s2cid=73634716 |doi-access=free }}</ref>
  |           Distance = 579.23<ref name="GaiaDR2Specific4DistancesKepler-186">{{cite journal |title=Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2 |journal=The Astronomical Journal |last1=Bailer-Jones |first1=C. A. L. |last2=Rybizki |first2=J. |last3=Fouesneau |first3=M. |last4=Mantelet |first4=G. |last5=Andrae |first5=R. |display-authors=1 |volume=156 |issue=2 |pages=58 |date=August 2018 |doi=10.3847/1538-3881/aacb21 |bibcode=2018AJ....156...58B |arxiv=1804.10121|s2cid=119289017 |doi-access=free }}[http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-ref=VIZ5d5b5b10086b&-out.add=.&-source=I/347/gaia2dis&-c=298.65273597008%20%2b43.95498841816,eq=ICRS,rs=2&-out.orig=o &nbsp;Distance to Kepler 186, after taking into account light extinction] {{Webarchive|url=https://web.archive.org/web/20220511093334/http://vizier.u-strasbg.fr/viz-bin/VizieR-5?-ref=VIZ5d5b5b10086b&-out.add=.&-source=I/347/gaia2dis&-c=298.65273597008%20%2b43.95498841816,eq=ICRS,rs=2&-out.orig=o |date=2022-05-11 }}</ref>
  |      Spectral type = M1V<ref name=NASAExoplanetKepler-186f>{{cite web|url=http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-186+f|title=Kepler-186 f|work=NASA Exoplanet Archive|access-date=19 July 2016|archive-date=18 March 2022|archive-url=https://web.archive.org/web/20220318185724/https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-186+f|url-status=live}}</ref>
  |               Mass = 0.478
  |             Radius = 0.472
  |        Temperature = 3788
  |        Metallicity = -0.28
  |                Age =  
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = Planet f is the first Earth-size exoplanet discovered that orbits in the habitable zone.<ref name="SCI-20140418">{{Cite journal| doi = 10.1126/science.1249403| title = An Earth-Sized Planet in the Habitable Zone of a Cool Star| journal = [[Science (journal)|Science]]| volume = 344| issue = 6181| pages = 277–280| date = 2014-04-18| arxiv=1404.5667| last1 = Quintana | first1 = E. V.| last2 = Barclay | first2 = T.| last3 = Raymond | first3 = S. N.| last4 = Rowe | first4 = J. F.| last5 = Bolmont | first5 = E.| last6 = Caldwell | first6 = D. A.| last7 = Howell | first7 = S. B.| last8 = Kane | first8 = S. R.| last9 = Huber | first9 = D.| last10 = Crepp | first10 = J. R.| last11 = Lissauer | first11 = J. J. | author-link11=Jack J. Lissauer| last12 = Ciardi | first12 = D. R.| last13 = Coughlin | first13 = J. L.| last14 = Everett | first14 = M. E.| last15 = Henze | first15 = C. E.| last16 = Horch | first16 = E.| last17 = Isaacson | first17 = H.| last18 = Ford | first18 = E. B.| last19 = Adams | first19 = F. C.| last20 = Still | first20 = M.| last21 = Hunter | first21 = R. C.| last22 = Quarles | first22 = B.| last23 = Selsis | first23 = F.|bibcode = 2014Sci...344..277Q | pmid=24744370| s2cid = 1892595}} free version = http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf {{Webarchive|url=https://web.archive.org/web/20140418183443/http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf |date=2014-04-18 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[K2-37]]
  |      Constellation = Scorpius (constellation){{!}}Scorpius
  |    Right ascension = {{RA|16|13|48.2445}}
  |        Declination = {{DEC|-24|47|13.4279}}
  | Apparent magnitude = 12.52
  |           Distance = 590
  |      Spectral type = G3V
  |               Mass = 0.9
  |             Radius = 0.85
  |        Temperature = 5413
  |        Metallicity = -0.03
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[K2-58]]
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|15|17.2364}}
  |        Declination = {{DEC|-14|02|59.3151}}
  | Apparent magnitude = 12.13
  |           Distance = 596
  |      Spectral type = K2V
  |               Mass = 0.89
  |             Radius = 0.86
  |        Temperature = 5038
  |        Metallicity = 0.25
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[K2-138]]
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|23|15|47.77}}
  |        Declination = {{DEC|-10|50|58.91}}
  | Apparent magnitude = 12.21
  |           Distance = 597{{±|55}}
  |      Spectral type = K1V
  |               Mass = 0.93
  |             Radius = 0.86
  |        Temperature = 5378±60
  |        Metallicity = +0.16 ± 0.04
  |                Age = 2.3
  |  Confirmed planets = 6
  |Unconfirmed planets =
  |              Notes = Planet g was not fully verified, or could be two long-period planets instead.<ref name="Christiansen">{{Cite journal|first1=Jessie L. |last1=Christiansen |first2=Ian J. M. |last2=Crossfield |first3=Geert |last3=Barentsen |first4=Chris J. |last4=Lintott |first5=Thomas |last5=Barclay |first6=Brooke D. |last6=Simmons |first7=Erik |last7=Petigura |first8=Joshua E. |last8=Schlieder |first9=Courtney D. |last9=Dressing |first10=Andrew |last10=Vanderburg |first11=David R. |last11=Ciardi |first12=Campbell |last12=Allen |first13=Adam |last13=McMaster |first14=Grant |last14=Miller |first15=Martin |last15=Veldthuis |first16=Sarah |last16=Allen |first17=Zach |last17=Wolfenbarger |first18=Brian |last18=Cox |first19=Julia |last19=Zemiro |first20=Andrew W. |last20=Howard |first21=John |last21=Livingston |first22=Evan |last22=Sinukoff |first23=Timothy |last23=Catron |first24=Andrew |last24=Grey |first25=Joshua J. E. |last25=Kusch |first26=Ivan |last26=Terentev |first27=Martin |last27=Vales |first28=Martti H. |last28=Kristiansen|date=2018-01-11|title=The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists|journal=The Astronomical Journal|language=en|volume=155|issue=2|pages=57|arxiv=1801.03874|doi=10.3847/1538-3881/aa9be0|issn=1538-3881|bibcode=2018AJ....155...57C |s2cid=52971376 |doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[K2-38]]
  |      Constellation = Scorpius
  |    Right ascension = {{RA|16|00|08.06}}
  |        Declination = {{DEC|-23|11|21.33}}
  | Apparent magnitude = 11.34
  |           Distance = 630
  |      Spectral type = G3V
  |               Mass = 1.03
  |             Radius = 1.10
  |        Temperature = 5731{{±|66}}
  |        Metallicity = 0.28
  |                Age = 
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
  |              Notes = Dust disk in system
}}
{{Multiplanetary systems list
  |               Star = WASP-47
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|04|49.0}}
  |        Declination = {{DEC|-12|01|08}}
  | Apparent magnitude = 11.9
  |           Distance = 652
  |      Spectral type = G9V
  |               Mass = 1.084
  |             Radius = 1.15
  |        Temperature = 5400
  |        Metallicity = 0.18
  |                Age =  
  |  Confirmed planets = 4
  |Unconfirmed planets =  
  |              Notes = One planet is a gas giant which orbits in the habitable zone.<ref name="WASP-47habzone">{{Cite journal|last1=Becker|first1=Juliette C.|last2=Vanderburg|first2=Andrew|last3=Adams|first3=Fred C.|last4=Rappaport|first4=Saul A.|last5=Schwengeler|first5=Hans Martin|title=Wasp-47: A Hot Jupiter System with Two Additional Planets Discovered by K2|date=2015-10-12|journal=The Astrophysical Journal|language=en|volume=812|issue=2|pages=L18|doi=10.1088/2041-8205/812/2/L18|issn=2041-8213|arxiv=1508.02411|bibcode=2015ApJ...812L..18B|s2cid=14681933}}</ref><ref name="Neveu-VanMalle2016">{{cite journal | title=Hot Jupiters with relatives: Discovery of additional planets in orbit around WASP-41 and WASP-47 | url=https://www.aanda.org/articles/aa/full_html/2016/02/aa26965-15/aa26965-15.html | last1=Neveu-VanMalle | first1=M. | last2=Queloz | first2=D. | last3=Anderson | first3=D. R. | last4=Brown | first4=D. J. A. | last5=Collier Cameron | first5=A. | last6=Delrez | first6=L. | last7=Díaz | first7=R. F. | last8=Gillon | first8=M. | last9=Hellier | first9=C. | last10=Jehin | first10=E. | last11=Lister | first11=T. | last12=Pepe | first12=F. | last13=Rojo | first13=P. | last14=Ségransan | first14=D. | last15=Triaud | first15=A. H. M. J. | last16=Turner | first16=O. D. | last17=Udry | first17=S. | display-authors=1 | journal=Astronomy and Astrophysics | volume=586 | at=A93 | year=2016 | arxiv=1509.07750 | bibcode=2016A&A...586A..93N | doi=10.1051/0004-6361/201526965 | s2cid=53354547 | access-date=2022-05-08 | archive-date=2022-02-28 | archive-url=https://web.archive.org/web/20220228025245/https://www.aanda.org/articles/aa/full_html/2016/02/aa26965-15/aa26965-15.html | url-status=live }}</ref> WASP-47 is the only planetary system known to have both planets near the [[hot Jupiter]] and another planet much further out.<ref name="caltech.eduWASP-47">{{cite web|url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=WASP-47&type=PLANET_HOST|title=WASP-47|website=exoplanetarchive.ipac.caltech.edu|access-date=2022-05-08|archive-date=2022-05-08|archive-url=https://web.archive.org/web/20220508114227/https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=WASP-47&type=PLANET_HOST|url-status=live}}</ref>
}}

{{Multiplanetary systems list
  |               Star = K2-368
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|10|32.58}}
  |        Declination = {{DEC|-11|09|58.02}}
  | Apparent magnitude = 13.54
  |           Distance = 674
  |      Spectral type = K3
  |               Mass = 0.746
  |             Radius = 
  |        Temperature = 4663{{±|138}}
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = HAT-P-13
  |      Constellation = Ursa Major
  |    Right ascension = {{RA|08|39|31.81}}
  |        Declination = {{DEC|+47|21|07.3}}
  | Apparent magnitude = 10.62
  |           Distance = 698
  |      Spectral type = G4
  |               Mass = 1.22
  |             Radius = 1.56
  |        Temperature = 5638
  |        Metallicity = 0.43
  |                Age = 5
  |  Confirmed planets = 2
  |Unconfirmed planets = 1
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-19]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|21|41}}
  |        Declination = {{DEC|+37|51|06}}
  | Apparent magnitude = 15.178
  |           Distance = 717
  |      Spectral type = G
  |               Mass = 0.936
  |             Radius = 0.85
  |        Temperature = 5541
  |        Metallicity = -0.13
  |                Age = 1.9
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = System consists of a thick-envelope Super-Earth and two Neptune-mass planets.<ref name="Malavolta2017">{{cite journal | title=The Kepler-19 System: A Thick-envelope Super-Earth with Two Neptune-mass Companions Characterized Using Radial Velocities and Transit Timing Variations | last1=Malavolta | first1=Luca | last2=Borsato | first2=Luca | last3=Granata | first3=Valentina | last4=Piotto | first4=Giampaolo | last5=Lopez | first5=Eric | last6=Vanderburg | first6=Andrew | last7=Figueira | first7=Pedro | last8=Mortier | first8=Annelies | last9=Nascimbeni | first9=Valerio | last10=Affer | first10=Laura | last11=Bonomo | first11=Aldo S. | last12=Bouchy | first12=Francois | last13=Buchhave | first13=Lars A. | last14=Charbonneau | first14=David | last15=Cameron | first15=Andrew Collier | last16=Cosentino | first16=Rosario | last17=Dressing | first17=Courtney D. | last18=Dumusque | first18=Xavier | last19=Fiorenzano | first19=Aldo F. M. | last20=Harutyunyan | first20=Avet | last21=Haywood | first21=Raphaëlle D. | last22=Johnson | first22=John Asher | last23=Latham | first23=David W. | last24=Lopez-Morales | first24=Mercedes | last25=Lovis | first25=Christophe | last26=Mayor | first26=Michel | last27=Micela | first27=Giusi | last28=Molinari | first28=Emilio | last29=Motalebi | first29=Fatemeh | last30=Pepe | first30=Francesco | display-authors=1 | journal=The Astronomical Journal | volume=153 | issue=5 | at=224 | year=2017 | arxiv=1703.06885 | bibcode=2017AJ....153..224M | bibcode-access=free | doi=10.3847/1538-3881/aa6897 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-296]]
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|06|09.6}}
  |        Declination = {{DEC|+49|26|14.4}}
  | Apparent magnitude = 12.6
  |           Distance = 737.113
  |      Spectral type = K7V + M1V<ref name=Lissauer_Kepler296spectype>{{cite journal|doi=10.1088/0004-637X/784/1/44|arxiv=1402.6352|title=Validation Of Kepler's Multiple Planet Candidates. Ii. Refined Statistical Framework and Descriptions of Systems of Special Interest|journal=The Astrophysical Journal|volume=784|pages=44|year=2014|last1=Lissauer|first1=Jack J|last2=Marcy|first2=Geoffrey W|last3=Bryson|first3=Stephen T|last4=Rowe|first4=Jason F|last5=Jontof-Hutter|first5=Daniel|last6=Agol|first6=Eric|last7=Borucki|first7=William J|last8=Carter|first8=Joshua A|last9=Ford|first9=Eric B|last10=Gilliland|first10=Ronald L|last11=Kolbl|first11=Rea|last12=Star|first12=Kimberly M|last13=Steffen|first13=Jason H|last14=Torres|first14=Guillermo|issue=1|bibcode=2014ApJ...784...44L|s2cid=119108651}}</ref>
  |               Mass =
  |             Radius = 0.557
  |        Temperature = 4249
  |        Metallicity = 0.168
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = All planets orbit around the primary star.<ref name=BarclayKepler296/> Planets e and f are potentially habitable.<ref name=BarclayKepler296>{{cite journal|bibcode=2015ApJ...809....7B|doi=10.1088/0004-637X/809/1/7|arxiv=1505.01845|title=The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis|journal=The Astrophysical Journal|volume=809|pages=7|year=2015|last1=Barclay|first1=Thomas|last2=Quintana|first2=Elisa V|last3=Adams|first3=Fred C|last4=Ciardi|first4=David R|last5=Huber|first5=Daniel|last6=Foreman-Mackey|first6=Daniel|last7=Montet|first7=Benjamin T|last8=Caldwell|first8=Douglas|issue=1|s2cid=37742564}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-454
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|09|55.0}}
  |        Declination = {{DEC|+38|13|44}}
  | Apparent magnitude = 11.57 
  |           Distance = 753
  |      Spectral type = G
  |               Mass = 1.028
  |             Radius = 1.066
  |        Temperature = 5687
  |        Metallicity = 0.32
  |                Age = 5.25 
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-25]]
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|06|33.0}}
  |        Declination = {{DEC|+39|29|16}}
  | Apparent magnitude = 11
  |           Distance = 799
  |      Spectral type = F<ref name=epeKepler-25spectype>{{citation
 |first1=Jean 
 |last1=Schneider 
 |title=Star: Kepler-25 
 |url=http://exoplanet.eu/star.php?st=Kepler-25 
 |access-date=2013-12-18 
 |url-status=dead 
 |archive-url=https://web.archive.org/web/20120616125118/http://exoplanet.eu/star.php?st=Kepler-25 
 |encyclopedia=[[Extrasolar Planets Encyclopaedia]]
 |archive-date=2012-06-16 
}}</ref>
  |               Mass = 1.22
  |             Radius = 1.36
  |        Temperature = 6190
  |        Metallicity = 0.01
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Two planets were discovered by transit-timing variations,<ref name="Steffen2012Kepler-25">{{cite journal | title=Transit timing observations from Kepler - III. Confirmation of four multiple planet systems by a Fourier-domain study of anticorrelated transit timing variations | last1=Steffen | first1=Jason H. | last2=Fabrycky | first2=Daniel C. | last3=Ford | first3=Eric B. | last4=Carter | first4=Joshua A. | last5=Désert | first5=Jean-Michel | last6=Fressin | first6=Francois | last7=Holman | first7=Matthew J. | last8=Lissauer | first8=Jack J. | last9=Moorhead | first9=Althea V. | last10=Rowe | first10=Jason F. | last11=Ragozzine | first11=Darin | last12=Welsh | first12=William F. | last13=Batalha | first13=Natalie M. | last14=Borucki | first14=William J. | last15=Buchhave | first15=Lars A. | last16=Bryson | first16=Steve | last17=Caldwell | first17=Douglas A. | last18=Charbonneau | first18=David | last19=Ciardi | first19=David R. | last20=Cochran | first20=William D. | last21=Endl | first21=Michael | last22=Everett | first22=Mark E. | last23=Gautier | first23=Thomas N. | last24=Gilliland | first24=Ron L. | last25=Girouard | first25=Forrest R. | last26=Jenkins | first26=Jon M. | last27=Horch | first27=Elliott | last28=Howell | first28=Steve B. | last29=Isaacson | first29=Howard | last30=Klaus | first30=Todd C. | display-authors=1 | journal=Monthly Notices of the Royal Astronomical Society | volume=421 | issue=3 | pages=2342–2354 | year=2012 | arxiv=1201.5412 | bibcode=2012MNRAS.421.2342S | bibcode-access=free | doi=10.1111/j.1365-2966.2012.20467.x | doi-access=free }}</ref> and the third planet was discovered by follow-up radial velocity measurements.<ref name="Marcy2014">{{cite journal | title=Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets | last1=Marcy | first1=Geoffrey W. | last2=Isaacson | first2=Howard | last3=Howard | first3=Andrew W. | last4=Rowe | first4=Jason F. | last5=Jenkins | first5=Jon M. | last6=Bryson | first6=Stephen T. | last7=Latham | first7=David W. | last8=Howell | first8=Steve B. | last9=Gautier | first9=Thomas N. | last10=Batalha | first10=Natalie M. | last11=Rogers | first11=Leslie | last12=Ciardi | first12=David | last13=Fischer | first13=Debra A. | last14=Gilliland | first14=Ronald L. | last15=Kjeldsen | first15=Hans | last16=Christensen-Dalsgaard | first16=Jørgen | last17=Huber | first17=Daniel | last18=Chaplin | first18=William J. | last19=Basu | first19=Sarbani | last20=Buchhave | first20=Lars A. | last21=Quinn | first21=Samuel N. | last22=Borucki | first22=William J. | last23=Koch | first23=David G. | last24=Hunter | first24=Roger | last25=Caldwell | first25=Douglas A. | last26=Van Cleve | first26=Jeffrey | last27=Kolbl | first27=Rea | last28=Weiss | first28=Lauren M. | last29=Petigura | first29=Erik | last30=Seager | first30=Sara | display-authors=1 | journal=The Astrophysical Journal Supplement Series | volume=210 | issue=2 | at=20 | year=2014 | arxiv=1401.4195 | bibcode=2014ApJS..210...20M | bibcode-access=free | doi=10.1088/0067-0049/210/2/20 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-114
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|36|29.0}}
  |        Declination = {{DEC|+48|20|58}}
  | Apparent magnitude = 13.7
  |           Distance = 846
  |      Spectral type = K
  |               Mass = 0.71
  |             Radius = 0.65
  |        Temperature = 4450
  |        Metallicity = -0.003
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-54
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|39|06.0}}
  |        Declination = {{DEC|+43|03|23}}
  | Apparent magnitude = 16.3
  |           Distance = 886
  |      Spectral type = M
  |               Mass = 0.52
  |             Radius = 0.55
  |        Temperature = 3705
  |        Metallicity = 
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-20
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|10|47.524}}
  |        Declination = {{DEC|42|20|19.30}}
  | Apparent magnitude = 12.51
  |           Distance = 950
  |      Spectral type = G8V
  |               Mass = 0.912
  |             Radius = 0.944
  |        Temperature = 5466
  |        Metallicity = 0.02
  |                Age = 8.8
  |  Confirmed planets = 6
  |Unconfirmed planets = 
  |              Notes = Planets e and f were the first Earth-sized planets to be discovered.<ref name="Nature-20111220">{{cite journal |last=Hand |first=Eric |title=Kepler discovers first Earth-sized exoplanets |doi=10.1038/nature.2011.9688 |date=20 December 2011 |journal=[[Nature (journal)|Nature]]|s2cid=122575277 }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[K2-19]]
  |      Constellation = Virgo (constellation){{!}}Virgo
  |    Right ascension = {{RA|11|39|50.4804}}
  |        Declination = {{DEC|+00|36|12.8773}}
  | Apparent magnitude = 13.002
  |           Distance = 976
  |      Spectral type = K0V<ref name="Nespral2017">{{cite journal | title=Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations | url=https://www.aanda.org/articles/aa/full_html/2017/05/aa28639-16/aa28639-16.html | last1=Nespral | first1=D. | last2=Gandolfi | first2=D. | last3=Deeg | first3=H. J. | last4=Borsato | first4=L. | last5=Fridlund | first5=M. C. V. | last6=Barragán | first6=O. | last7=Alonso | first7=R. | last8=Grziwa | first8=S. | last9=Korth | first9=J. | last10=Albrecht | first10=S. | last11=Cabrera | first11=J. | last12=Csizmadia | first12=Sz. | last13=Nowak | first13=G. | last14=Kuutma | first14=T. | last15=Saario | first15=J. | last16=Eigmüller | first16=P. | last17=Erikson | first17=A. | last18=Guenther | first18=E. W. | last19=Hatzes | first19=A. P. | last20=Montañés Rodríguez | first20=P. | last21=Palle | first21=E. | last22=Pätzold | first22=M. | last23=Prieto-Arranz | first23=J. | last24=Rauer | first24=H. | last25=Sebastian | first25=D. | display-authors=1 | journal=Astronomy and Astrophysics | volume=601 | at=A128 | year=2017 | arxiv=1604.01265 | bibcode=2017A&A...601A.128N | doi=10.1051/0004-6361/201628639 | s2cid=55978628 | access-date=2022-03-18 | archive-date=2022-05-04 | archive-url=https://web.archive.org/web/20220504003941/https://www.aanda.org/articles/aa/full_html/2017/05/aa28639-16/aa28639-16.html | url-status=live }}</ref> or G9V<ref name="Sinukoff2016">{{cite journal | title=Eleven Multiplanet Systems From K2 Campaigns 1 and 2 and the Masses of Two Hot Super-Earths | last1=Sinukoff | first1=Evan | last2=Howard | first2=Andrew W. | last3=Petigura | first3=Erik A. | last4=Schlieder | first4=Joshua E. | last5=Crossfield | first5=Ian J. M. | last6=Ciardi | first6=David R. | last7=Fulton | first7=Benjamin J. | last8=Isaacson | first8=Howard | last9=Aller | first9=Kimberly M. | last10=Baranec | first10=Christoph | last11=Beichman | first11=Charles A. | last12=Hansen | first12=Brad M. S. | last13=Knutson | first13=Heather A. | last14=Law | first14=Nicholas M. | last15=Liu | first15=Michael C. | last16=Riddle | first16=Reed | last17=Dressing | first17=Courtney D. | display-authors=1 | journal=The Astrophysical Journal | volume=827 | issue=1 | at=78 | year=2016 | arxiv=1511.09213 | bibcode=2016ApJ...827...78S | doi=10.3847/0004-637X/827/1/78 | doi-access=free }}</ref>
  |               Mass = 0.918
  |             Radius = 0.881±0.111
  |        Temperature = 5250±70
  |        Metallicity = 0.10±0.05
  |                Age = 8
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = PSR B1257+12|Lich
  |      Constellation = Virgo (constellation){{!}}Virgo
  |    Right ascension = {{RA|13|00|03.58}}
  |        Declination = {{DEC|+12|40|56.5}}
  | Apparent magnitude = 24.31
  |           Distance = 980
  |      Spectral type = pulsar
  |               Mass = 1.444
  |             Radius = 0.000023
  |        Temperature = 28856
  |        Metallicity =
  |                Age = 0.797
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Only pulsar with a multiplanetary system, and first exoplanets and multiplanetary system to be confirmed.<ref>{{cite web |url=http://www.astro.psu.edu/users/alex/pulsar_planets.htm |title=Pulsar Planets |url-status=dead |archive-url=https://web.archive.org/web/20051230112904/http://www.astro.psu.edu/users/alex/pulsar_planets.htm |archive-date=30 December 2005  }}</ref><ref>{{cite journal|bibcode=1992Natur.355..145W|author=Wolszczan, A.|author2=Frail, D.|title=A planetary system around the millisecond pulsar PSR1257 + 12|journal=[[Nature (journal)|Nature]]|volume=355|issue=6356|pages=145–147|date=1992|doi=10.1038/355145a0|s2cid=4260368}}</ref> Star with dimmest apparent magnitude to have a multiplanetary system.
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-62]]
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|52|51.060}}
  |        Declination = {{DEC|+45|20|59.507}}
  | Apparent magnitude = 13.75<ref name = "BoruckiKepler-62"/>
  |           Distance = 990
  |      Spectral type = K2V<ref name = "BoruckiKepler-62"/>
  |               Mass = 0.69
  |             Radius = 0.64
  |        Temperature = 4925
  |        Metallicity = –0.37
  |                Age = 7
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = Planets e and f orbit in the habitable zone.<ref name = "BoruckiKepler-62">{{Cite journal | last=Borucki | first=William J. | author-link=William J. Borucki | display-authors=etal | title=Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone | journal=Science Express | date=18 April 2013 | doi=10.1126/science.1234702 | access-date=18 March 2022 | url=https://www.science.org/doi/10.1126/science.1234702 | arxiv=1304.7387 | bibcode=2013Sci...340..587B | pmid=23599262 | volume=340 | issue=6132 | pages=587–90 | hdl=1721.1/89668 | s2cid=21029755 | archive-date=2 May 2022 | archive-url=https://web.archive.org/web/20220502115940/https://www.science.org/doi/10.1126/science.1234702 | url-status=live }}</ref><ref name="NASA-20130418">{{cite web |last1=Johnson |first1=Michele |last2=Harrington |first2=J.D. |title=NASA's Kepler Discovers Its Smallest 'Habitable Zone' Planets to Date |url=http://www.nasa.gov/mission_pages/kepler/news/kepler-62-kepler-69.html |date=18 April 2013 |work=[[NASA]] |access-date=18 March 2022 |archive-date=8 May 2020 |archive-url=https://web.archive.org/web/20200508010029/https://www.nasa.gov/mission_pages/kepler/news/kepler-62-kepler-69.html |url-status=dead }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-48
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|56|33.41}}
  |        Declination = {{DEC|+40|56|56.47}}
  | Apparent magnitude = 13.04
  |           Distance = 1000
  |      Spectral type = K
  |               Mass = 0.88
  |             Radius = 0.89
  |        Temperature = 5190
  |        Metallicity = -0.216
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-100
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|25|32.6}}
  |        Declination = {{DEC|+41|59|24}}
  | Apparent magnitude =  
  |           Distance = 1011
  |      Spectral type = G1IV
  |               Mass = 1.109
  |             Radius = 1.5131
  |        Temperature = 5825
  |        Metallicity = 0.02
  |                Age = 6.5
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-49
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|29|11.0}}
  |        Declination = {{DEC|+40|35|30}}
  | Apparent magnitude = 15.5
  |           Distance = 1015
  |      Spectral type = K
  |               Mass = 0.55
  |             Radius = 0.56
  |        Temperature = 3974
  |        Metallicity = 
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-65
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|14|45.3}}
  |        Declination = {{DEC|+41|09|04.2}}
  | Apparent magnitude = 11.018
  |           Distance = 1019
  |      Spectral type = F6IV
  |               Mass = 1.199
  |             Radius = 1.399
  |        Temperature = 6211
  |        Metallicity = 0.17
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets = 
}}
{{Multiplanetary systems list
  |               Star = Kepler-52
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|19|06|57.0}}
  |        Declination = {{DEC|+49|58|33}}
  | Apparent magnitude = 15.5
  |           Distance = 1049
  |      Spectral type = K
  |               Mass = 0.58
  |             Radius = 0.56
  |        Temperature = 4075
  |        Metallicity =  
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-314
  |      Constellation = Libra (constellation){{!}}Libra
  |    Right ascension = {{RA|15|13|00.0}}
  |        Declination = {{DEC|-16|43|29}}
  | Apparent magnitude = 11.4
  |           Distance = 1059
  |      Spectral type = G8IV/V
  |               Mass = 1.05
  |             Radius = 1.71
  |        Temperature = 5430
  |        Metallicity = 0.2
  |                Age = 9.0
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = K2-219
  |      Constellation = Pisces (constellation){{!}}Pisces
  |    Right ascension = {{RA|00|51|22.9}}
  |        Declination = {{DEC|+08|52|04}}
  | Apparent magnitude = 12.09
  |           Distance = 1071
  |      Spectral type = G2
  |               Mass = 1.02
  |             Radius = 1.19
  |        Temperature = 5753{{±|50}}
  |        Metallicity = 0.13
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[K2-268]]
  |      Constellation = Cancer (constellation){{!}}Cancer
  |    Right ascension = {{RA|08|54|50.2862}}
  |        Declination = {{DEC|+11|50|53.7745}}
  | Apparent magnitude = 13.85
  |           Distance = 1079
  |      Spectral type = 
  |               Mass = 
  |             Radius = 
  |        Temperature =  
  |        Metallicity = 
  |                Age = 
  |  Confirmed planets = 5
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[K2-183]]
  |      Constellation = Cancer (constellation){{!}}Cancer
  |    Right ascension = {{RA|08|20|01.7184}}
  |        Declination = {{DEC|14|01|10.0711}}
  | Apparent magnitude = 12.85
  |           Distance = 1083
  |      Spectral type = 
  |               Mass = 
  |             Radius = 0.87
  |        Temperature = 5482{{±|50}}
  |        Metallicity = 0.09
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |Notes =
}}
{{Multiplanetary systems list
  |               Star = [[K2-187]]
  |      Constellation = Cancer (constellation){{!}}Cancer
  |    Right ascension = {{RA|08|50|05.6682}}
  |        Declination = {{DEC|23|11|33.3712}}
  | Apparent magnitude = 12.864
  |           Distance = 1090
  |      Spectral type = G?V
  |               Mass = 0.967
  |             Radius = 0.895
  |        Temperature = 5438{{±|63}}
  |        Metallicity = 0.26
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-1542
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|02|54.8}}
  |        Declination = {{DEC|+42|39|16}}
  | Apparent magnitude = 
  |           Distance = 1096
  |      Spectral type = G5V
  |               Mass = 0.94
  |             Radius = 0.99
  |        Temperature = 5564
  |        Metallicity = 0.06
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets = 1
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-26]]
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|59|46}}
  |        Declination = {{DEC|+46|34|00}}
  | Apparent magnitude = 16
  |           Distance = 1100
  |      Spectral type = M0V
  |               Mass = 0.65
  |             Radius = 0.59
  |        Temperature = 4500
  |        Metallicity = -0.21
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = Transiting exoplanets<ref name=Steffen2012>{{citation|arxiv=1201.5412|title=Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations|year=2012|doi=10.1111/j.1365-2966.2012.20467.x|last1=Steffen|first1=Jason H.|last2=Fabrycky|first2=Daniel C.|last3=Ford|first3=Eric B.|last4=Carter|first4=Joshua A.|last5=Desert|first5=Jean-Michel|last6=Fressin|first6=Francois|last7=Holman|first7=Matthew J.|last8=Lissauer|first8=Jack J.|last9=Moorhead|first9=Althea V.|last10=Rowe|first10=Jason F.|last11=Ragozzine|first11=Darin|last12=Welsh|first12=William F.|last13=Batalha|first13=Natalie M.|last14=Borucki|first14=William J.|last15=Buchhave|first15=Lars A.|last16=Bryson|first16=Steve|last17=Caldwell|first17=Douglas A.|last18=Charbonneau|first18=David|last19=Ciardi|first19=David R.|last20=Cochran|first20=William D.|last21=Endl|first21=Michael|last22=Everett|first22=Mark E.|last23=Gautier III|first23=Thomas N.|last24=Gilliland|first24=Ron L.|last25=Girouard|first25=Forrest R.|last26=Jenkins|first26=Jon M.|last27=Horch|first27=Elliott|last28=Howell|first28=Steve B.|last29=Isaacson|first29=Howard|last30=Klaus|first30=Todd C.|journal=Monthly Notices of the Royal Astronomical Society |volume=421 |issue=3 |doi-access=free |bibcode=2012MNRAS.421.2342S |s2cid=11898578|display-authors=29}}</ref> which are low-density planets below the size of [[Neptune]].<ref name=Cubillos2016>{{citation|arxiv=1611.09236|title=An overabundance of low-density Neptune-like planets|year=2016|doi=10.1093/mnras/stw3103|last1=Cubillos|first1=Patricio|last2=Erkaev|first2=Nikolai V.|last3=Juvan|first3=Ines|last4=Fossati|first4=Luca|last5=Johnstone|first5=Colin P.|last6=Lammer|first6=Helmut|last7=Lendl|first7=Monika|last8=Odert|first8=Petra|last9=Kislyakova|first9=Kristina G.|journal=Monthly Notices of the Royal Astronomical Society|volume=466|issue=2|pages=1868–1879|doi-access=free |s2cid=119408956}}</ref><ref name=Jontof2015>{{citation|arxiv=1512.02003|title=Secure TTV Mass Measurements: Ten Kepler Exoplanets between 3 and 8 M<sub>🜨</sub> with Diverse Densities and Incident Fluxes|year=2015|doi=10.3847/0004-637X/820/1/39|last1=Jontof-Hutter|first1=Daniel|last2=Ford|first2=Eric B.|last3=Rowe|first3=Jason F.|last4=Lissauer|first4=Jack J.|last5=Fabrycky|first5=Daniel C.|author6=Christa Van Laerhoven|last7=Agol|first7=Eric|last8=Deck|first8=Katherine M.|last9=Holczer|first9=Tomer|last10=Mazeh|first10=Tsevi|journal=The Astrophysical Journal |volume=820 |issue=1 |page=39 |s2cid=11322397 |doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-167
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|30|38.0}}
  |        Declination = {{DEC|+38|20|43}}
  | Apparent magnitude = 
  |           Distance = 1119 ± 6
  |      Spectral type =
  |               Mass = 0.76
  |             Radius = 0.7
  |        Temperature = 4796
  |        Metallicity = 0.052
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Planet e is the first transiting Jupiter analog discovered.<ref name="Kipping2016">{{cite journal |last1=Kipping |first1=David M. |last2=Torres |first2=Guillermo |display-authors=etal |date=April 2016 |title=A Transiting Jupiter Analog |journal=[[The Astrophysical Journal]] |volume=820 |issue=2 |pages=112 |doi=10.3847/0004-637X/820/2/112 |arxiv=1603.00042 |bibcode=2016ApJ...820..112K|s2cid=1892262 |doi-access=free }}</ref><ref name="Chachan2022">{{cite journal |last1=Chachan |first1=Yayaati |last2=Dalba |first2=Paul A. |display-authors=etal |date=February 2022 |title=Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths |journal=[[The Astrophysical Journal]] |volume=926 |issue=1 |pages=62 |doi=10.3847/1538-4357/ac3ed6 |arxiv=2112.00747 |bibcode=2022ApJ...926...62C|s2cid=244799213 |doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-81
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|34|32.9}}
  |        Declination = {{DEC|+42|49|30}}
  | Apparent magnitude = 15.56
  |           Distance = 1136
  |      Spectral type = K?V
  |               Mass = 0.648
  |             Radius = 0.578
  |        Temperature = 4391
  |        Metallicity = -0.2
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-132
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|52|56.6}}
  |        Declination = {{DEC|+41|20|35}}
  | Apparent magnitude = 
  |           Distance = 1140
  |      Spectral type = F9
  |               Mass = 0.98
  |             Radius = 1.18
  |        Temperature = 6003
  |        Metallicity = -0.053
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-80
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|44|27.0}}
  |        Declination = {{DEC|+39|58|44}}
  | Apparent magnitude = 14.804
  |           Distance = 1218
  |      Spectral type = M0V<ref name=SIMBADKepler-80>{{cite simbad|title=Kepler-80|access-date=10 January 2017}}</ref>
  |               Mass = 0.730
  |             Radius = 0.738
  |        Temperature = 4250
  |        Metallicity = -0.56
  |                Age = 
  |  Confirmed planets = 6
  |Unconfirmed planets =  
  |              Notes = Red dwarf star with six confirmed planets.<ref name="Xie2013Kepler-80">{{cite journal|last1=Xie|first1=J.-W.|year=2013|title=Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems|journal=Astrophysical Journal Supplement Series|volume=208|issue=2|pages=22|arxiv=1208.3312|bibcode=2013ApJS..208...22X|doi=10.1088/0067-0049/208/2/22|s2cid=17160267}}</ref><ref name="Shallue2017">{{cite journal|last1=Shallue|first1=C. J.|last2=Vanderburg|first2=A.|date=2017|title=Identifying Exoplanets With Deep Learning: A Five Planet Resonant Chain Around Kepler-80 And An Eighth Planet Around Kepler-90|url=https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf|journal=[[The Astrophysical Journal]]|volume=155|issue=2|pages=94|arxiv=1712.05044|bibcode=2018AJ....155...94S|doi=10.3847/1538-3881/aa9e09|s2cid=4535051|access-date=2017-12-15|doi-access=free|archive-date=2017-12-24|archive-url=https://web.archive.org/web/20171224094458/https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf|url-status=live}}</ref> Five of them are in an [[orbital resonance]].<ref name="MacDonald2016">{{Cite journal|last1=MacDonald|first1=Mariah G.|last2=Ragozzine|first2=Darin|last3=Fabrycky|first3=Daniel C.|last4=Ford|first4=Eric B.|last5=Holman|first5=Matthew J.|last6=Isaacson|first6=Howard T.|last7=Lissauer|first7=Jack J.|last8=Lopez|first8=Eric D.|last9=Mazeh|first9=Tsevi|date=2016-01-01|title=A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets|url=http://stacks.iop.org/1538-3881/152/i=4/a=105|journal=The Astronomical Journal|volume=152|issue=4|pages=105|doi=10.3847/0004-6256/152/4/105|arxiv = 1607.07540 |bibcode = 2016AJ....152..105M |s2cid=119265122 |doi-access=free }}</ref><ref name="Shallue2017" />
}}
{{Multiplanetary systems list
  |               Star = Kepler-159
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|48|16.8}}
  |        Declination = {{DEC|+40|52|08}}
  | Apparent magnitude =  
  |           Distance = 1219
  |      Spectral type = K
  |               Mass = 0.63
  |             Radius = 0.66
  |        Temperature = 4625
  |        Metallicity = -0.911
  |                Age =
  |  Confirmed planets = 2
  |Unconfirmed planets = 1 
  |              Notes = Star has a very low metallicity.
}}
{{Multiplanetary systems list
  |               Star = [[K2-299]]
  |      Constellation = Aquarius (constellation){{!}}Aquarius
  |    Right ascension = {{RA|22|05|06.5342}}
  |        Declination = {{DEC|-14|07|18.0135}}
  | Apparent magnitude = 13.12
  |           Distance = 1220
  |      Spectral type = 
  |               Mass = 
  |             Radius = 1.1
  |        Temperature = 5724{{±|72}}
  |        Metallicity = -0.22
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-88]]
  |      Constellation = Lyra (constellation){{!}}Lyra
  |    Right ascension = {{RA|19|24|35.5431}}
  |        Declination = {{DEC|+40|40|09.8098}}
  | Apparent magnitude = 13.5
  |           Distance = 1243
  |      Spectral type = G8IV
  |               Mass = 1.022
  |             Radius = 0.961
  |        Temperature = 5513{{±|67}}
  |        Metallicity = 0.37
  |                Age = 2.45
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-174
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|09|45.4}}
  |        Declination = {{DEC|+43|49:56}}
  | Apparent magnitude =  
  |           Distance = 1269
  |      Spectral type = K
  |               Mass =  
  |             Radius = 0.62 
  |        Temperature = 4880
  |        Metallicity = -0.556
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Planet d may orbit in the habitable zone.
}}
{{Multiplanetary systems list
  |               Star = Kepler-32
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|51|22.0}}
  |        Declination = {{DEC|+46|34|27}}
  | Apparent magnitude = 16
  |           Distance = 1301.1
  |      Spectral type = M1V
  |               Mass = 0.58
  |             Radius = 0.53
  |        Temperature = 3900
  |        Metallicity = 0
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets = 2
}}
{{Multiplanetary systems list
  |               Star = Kepler-83
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|48|55.8}}
  |        Declination = {{DEC|+43|39|56}}
  | Apparent magnitude = 16.51
  |           Distance = 1306
  |      Spectral type = K7V
  |               Mass = 0.664
  |             Radius = 0.539
  |        Temperature = 4164
  |        Metallicity = -0.2
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = TOI-1338
  |      Constellation = Pictor
  |    Right ascension = {{RA|06|08|31.97}}
  |        Declination = {{DEC|+59|32|28.1}}
  | Apparent magnitude = 11.72
  |           Distance = 1318
  |      Spectral type = F8 <br> M
  |               Mass = 1.127
  |             Radius = 1.331/0.309
  |        Temperature = 6160
  |        Metallicity = 0.01
  |                Age = 4.4
  |  Confirmed planets = 2
  |Unconfirmed planets = 0
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-271
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|52|00.7}}
  |        Declination = {{DEC|+44|17|03}}
  | Apparent magnitude = 
  |           Distance = 1319
  |      Spectral type = G7V
  |               Mass = 0.9
  |             Radius = 0.88
  |        Temperature = 5524
  |        Metallicity = -0.951
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Metal-poor star
}}
{{Multiplanetary systems list
  |               Star = Kepler-169
  |      Constellation =
  |    Right ascension = {{RA|19|03|60.0}}
  |        Declination = {{DEC|+40|55:10}}
  | Apparent magnitude = 12.186
  |           Distance = 1326
  |      Spectral type = K2V
  |               Mass = 0.86
  |             Radius = 0.76
  |        Temperature = 4997
  |        Metallicity = 0.238
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-451]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|38|32.61}}
  |        Declination = {{DEC|46|03|59.1}}
  | Apparent magnitude = 
  |           Distance = 1340
  |      Spectral type = [[Subdwarf B star|sdB]] <br> M
  |               Mass = 0.48+0.12
  |             Radius = 
  |        Temperature = 29564
  |        Metallicity = 
  |                Age = 6
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes = Three circumbinary planets orbit around the Kepler-451 binary pair.<ref name=Esmer2022_Kepler-451>{{citation|arxiv=2202.02118|year=2022|title=Detection of two additional circumbinary planets around Kepler-451|author1=Ekrem Murat Esmer|last2=Baştürk|first2=Özgür|author3=Selim Osman Selam|last4=Aliş|first4=Sinan|journal=Monthly Notices of the Royal Astronomical Society |volume=511 |issue=4 |pages=5207–5216 |doi=10.1093/mnras/stac357 |doi-access=free |bibcode=2022MNRAS.511.5207E }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-304
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|37|46.0}}
  |        Declination = {{DEC|+40|33|27}}
  | Apparent magnitude = 
  |           Distance = 1418
  |      Spectral type = K
  |               Mass = 0.8
  |             Radius = 0.73
  |        Temperature = 4731
  |        Metallicity = 0.523
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-18]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|52|19.06}}
  |        Declination = {{DEC|+44|44|46.76}}
  | Apparent magnitude = 13.549
  |           Distance = 1430
  |      Spectral type = G7V
  |               Mass = 0.97
  |             Radius = 1.11
  |        Temperature = 5345
  |        Metallicity = +0.19
  |                Age = 10
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-106
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|20|03|27.4}}
  |        Declination = {{DEC|+44|20|15}}
  | Apparent magnitude = 12.882
  |           Distance = 1449
  |      Spectral type = G1V
  |               Mass = 1
  |             Radius = 1.04
  |        Temperature = 5858
  |        Metallicity = -0.12
  |                Age = 4.83
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-92
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|16|21.0}}
  |        Declination = {{DEC|+41|33|47}}
  | Apparent magnitude = 11.6
  |           Distance = 1463
  |      Spectral type = G1IV
  |               Mass = 1.209
  |             Radius = 1.716
  |        Temperature = 5871
  |        Metallicity = 0.17
  |                Age = 5.52
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-450
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|41|56.8}}
  |        Declination = {{DEC|+51|00|49}}
  | Apparent magnitude = 11.684 
  |           Distance = 1487
  |      Spectral type = F  
  |               Mass = 1.19
  |             Radius = 1.64
  |        Temperature = 6152
  |        Metallicity = -0.342
  |                Age =  
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-89]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|49|20.0}}
  |        Declination = {{DEC|+41|53|28}}
  | Apparent magnitude = 12.4
  |           Distance = 1580
  |      Spectral type = F8V
  |               Mass = 1.25
  |             Radius = 1.656
  |        Temperature = 6116
  |        Metallicity = -0.01
  |                Age = 3.9
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Farthest [[F-type main sequence star]] from the Sun with a multiplanetary system. One study found hints of additional planets orbiting Kepler-89.<ref>{{Cite journal|arxiv=1310.5771|title=Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse|journal=The Astrophysical Journal|volume=778|issue=2|pages=185–200|last1=Masuda|first1=Kento|last2=Hirano|first2=Teruyuki|last3=Taruya|first3=Atsushi|last4=Nagasawa|first4=Makiko|last5=Suto|first5=Yasushi|year=2013|doi=10.1088/0004-637X/778/2/185|bibcode = 2013ApJ...778..185M |s2cid=119264400}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-1388
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|53|20.6}}
  |        Declination = {{DEC|+47|10|28}}
  | Apparent magnitude = 
  |           Distance = 1604
  |      Spectral type = 
  |               Mass = 0.63
  |             Radius = 0.61
  |        Temperature = 4098
  |        Metallicity = 0.02
  |                Age = 
  |  Confirmed planets = 4
  |Unconfirmed planets = 1
}}
{{Multiplanetary systems list
  |               Star = [[K2-282]]
  |      Constellation = Pisces (constellation){{!}}Pisces
  |    Right ascension = {{RA|00|53|43.6833}}
  |        Declination = {{DEC|07|59|43.1397}}
  | Apparent magnitude = 14.04
  |           Distance = 1638
  |      Spectral type = G?V
  |               Mass = 0.94
  |             Radius = 1
  |        Temperature = 5499{{±|109}}
  |        Metallicity = -0.23
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-107]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|48|06.8}}
  |        Declination = {{DEC|+48|12|31}}
  | Apparent magnitude = 12.7
  |           Distance = 1714
  |      Spectral type = G2V<ref name=Kepler-107spectype>{{cite journal |last1=Bonomo |first1=Aldo S. |last2=Zeng |first2=Li |last3=Damasso |first3=Mario |last4=Leinhardt |first4=Zoë M. |last5=Justesen |first5=Anders B. |last6=Lopez |first6=Eric |last7=Lund |first7=Mikkel N. |last8=Malavolta |first8=Luca |last9=Silva Aguirre |first9=Victor |last10=Buchhave |first10=Lars A. |last11=Corsaro |first11=Enrico |last12=Denman |first12=Thomas |last13=Lopez-Morales |first13=Mercedes |last14=Mills |first14=Sean M. |last15=Mortier |first15=Annelies |last16=Rice |first16=Ken |last17=Sozzetti |first17=Alessandro |last18=Vanderburg |first18=Andrew |last19=Affer |first19=Laura |last20=Arentoft |first20=Torben |last21=Benbakoura |first21=Mansour |last22=Bouchy |first22=François |last23=Christensen-Dalsgaard |first23=Jørgen |last24=Collier Cameron |first24=Andrew |last25=Cosentino |first25=Rosario |last26=Dressing |first26=Courtney D. |last27=Dumusque |first27=Xavier |last28=Figueira |first28=Pedro |last29=Fiorenzano |first29=Aldo F. M. |last30=García |first30=Rafael A. |last31=Handberg |first31=Rasmus |last32=Harutyunyan |first32=Avet |last33=Johnson |first33=John A. |last34=Kjeldsen |first34=Hans |last35=Latham |first35=David W. |last36=Lovis |first36=Christophe |last37=Lundkvist |first37=Mia S. |last38=Mathur |first38=Savita |last39=Mayor |first39=Michel |last40=Micela |first40=Giusi |last41=Molinari |first41=Emilio |last42=Motalebi |first42=Fatemeh |last43=Nascimbeni |first43=Valerio |last44=Nava |first44=Chantanelle |last45=Pepe |first45=Francesco |last46=Phillips |first46=David F. |last47=Piotto |first47=Giampaolo |last48=Poretti |first48=Ennio |last49=Sasselov |first49=Dimitar |last50=Ségransan |first50=Damien |last51=Udry |first51=Stéphane |last52=Watson |first52=Chris |title=A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system |journal=Nature Astronomy |date=May 2019 |volume=3 |issue=5 |pages=416–423 |doi=10.1038/s41550-018-0684-9 |arxiv=1902.01316 |bibcode=2019NatAs...3..416B |s2cid=89604609 }}</ref>
  |               Mass = 1.238
  |             Radius = 1.41
  |        Temperature = 5851
  |        Metallicity = -0.092
  |                Age = 4.29
  |  Confirmed planets = 4
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-1047
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|14|35.1}}
  |        Declination = {{DEC|+50|47|20}}
  | Apparent magnitude = 
  |           Distance = 1846
  |      Spectral type = G2V
  |               Mass = 1.08
  |             Radius = 1.13
  |        Temperature = 5754
  |        Metallicity = 0.29
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-55
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|00|40.0}}
  |        Declination = {{DEC|+44|01|35}}
  | Apparent magnitude = 16.3
  |           Distance = 1888
  |      Spectral type = K
  |               Mass = 0.62
  |             Radius = 0.58
  |        Temperature = 4362
  |        Metallicity = 
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = Planet c may orbit in the inner habitable zone.
}}
{{Multiplanetary systems list
  |               Star = Kepler-166
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|32|38.4}}
  |        Declination = {{DEC|+48|52|52}}
  | Apparent magnitude = 
  |           Distance = 1968
  |      Spectral type = G
  |               Mass = 0.88
  |             Radius = 0.74
  |        Temperature = 5413
  |        Metallicity = -0.286
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-11
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|48|27.62}}
  |        Declination = {{DEC|+41|54|32.9}}
  | Apparent magnitude = 13.69
  |           Distance = 2150 {{±|20}}
  |      Spectral type = G6V<ref name="Lissauer2011_Kepler-11"/>
  |               Mass = 0.954
  |             Radius = 1.102
  |        Temperature = 5681
  |        Metallicity = 0.003
  |                Age = 7.834
  |  Confirmed planets = 6
  |Unconfirmed planets =
  |              Notes = Farthest star from the Sun with exactly six exoplanets. First system discovered with six transiting planets.<ref name="Lissauer2011_Kepler-11">{{cite journal | title=A closely packed system of low-mass, low-density planets transiting Kepler-11 | last1=Lissauer | first1=Jack J. | last2=Fabrycky | first2=Daniel C. | last3=Ford | first3=Eric B. | last4=Borucki | first4=William J. | last5=Fressin | first5=Francois | last6=Marcy | first6=Geoffrey W. | last7=Orosz | first7=Jerome A. | last8=Rowe | first8=Jason F. | last9=Torres | first9=Guillermo | last10=Welsh | first10=William F. | last11=Batalha | first11=Natalie M. | last12=Bryson | first12=Stephen T. | last13=Buchhave | first13=Lars A. | last14=Caldwell | first14=Douglas A. | last15=Carter | first15=Joshua A. | last16=Charbonneau | first16=David | last17=Christiansen | first17=Jessie L. | last18=Cochran | first18=William D. | last19=Desert | first19=Jean-Michel | last20=Dunham | first20=Edward W. | last21=Fanelli | first21=Michael N. | last22=Fortney | first22=Jonathan J. | last23=Gautier III | first23=Thomas N. | last24=Geary | first24=John C. | last25=Gilliland | first25=Ronald L. | last26=Haas | first26=Michael R. | last27=Hall | first27=Jennifer R. | last28=Holman | first28=Matthew J. | last29=Koch | first29=David G. | last30=Latham | first30=David W. | s2cid=4388001 | display-authors=1 | journal=Nature | volume=470 | issue=7332 | pages=53–58 | year=2011 | arxiv=1102.0291 | bibcode=2011Natur.470...53L | doi=10.1038/nature09760 | pmid=21293371 }}</ref> The planets have low densities.<ref name="Lissauer2013_Kepler-11">{{cite journal | title=All Six Planets Known to Orbit Kepler-11 Have Low Densities | last1=Lissauer | first1=Jack J. | last2=Jontof-Hutter | first2=Daniel | last3=Rowe | first3=Jason F. | last4=Fabrycky | first4=Daniel C. | last5=Lopez | first5=Eric D. | last6=Agol | first6=Eric | last7=Marcy | first7=Geoffrey W. | last8=Deck | first8=Katherine M. | last9=Fischer | first9=Debra A. | last10=Fortney | first10=Jonathan J. | last11=Howell | first11=Steve B. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Kolbl | first14=Rea | last15=Sasselov | first15=Dimitar | last16=Short | first16=Donald R. | last17=Welsh | first17=William F. | display-authors=1 | journal=The Astrophysical Journal | volume=770 | issue=2 | at=131 | year=2013 | arxiv=1303.0227 | bibcode=2013ApJ...770..131L | bibcode-access=free | doi=10.1088/0004-637X/770/2/131 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-1254
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|19|34|59.3}}
  |        Declination = {{DEC|+45|06|26}}
  | Apparent magnitude = 
  |           Distance = 2205
  |      Spectral type = 
  |               Mass = 0.78
  |             Radius = 0.75
  |        Temperature = 4985
  |        Metallicity = -0.1
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-289
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|49|51.7}}
  |        Declination = {{DEC|+42|52|58}}
  | Apparent magnitude = 12.9
  |           Distance = 2283
  |      Spectral type = G0V
  |               Mass = 1.08
  |             Radius = 1.0
  |        Temperature = 5990
  |        Metallicity = 0.05
  |                Age = 0.65
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-85
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|23|54.0}}
  |        Declination = {{DEC|+45|17|25}}
  | Apparent magnitude = 15.0
  |           Distance = 2495
  |      Spectral type = G
  |               Mass = 0.92
  |             Radius = 0.89
  |        Temperature = 5666
  |        Metallicity = 
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-157
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|24|23.3}}
  |        Declination = {{DEC|+38|52|32}}
  | Apparent magnitude = 
  |           Distance = 2523
  |      Spectral type = G2V
  |               Mass = 1.02
  |             Radius = 1.03
  |        Temperature = 5774
  |        Metallicity = -0.108
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-342
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|24|23.3}}
  |        Declination = {{DEC|+38|52|32}}
  | Apparent magnitude = 
  |           Distance = 2549
  |      Spectral type = F
  |               Mass = 1.13
  |             Radius = 1.47
  |        Temperature = 6175
  |        Metallicity = -0.053
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-148
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|19|08.7}}
  |        Declination = {{DEC|+46|51|32}}
  | Apparent magnitude = 
  |           Distance = 2580
  |      Spectral type = K?V
  |               Mass = 0.83
  |             Radius = 0.85
  |        Temperature = 5019.0±122.0
  |        Metallicity = 0.143
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-51]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|45|55.0}}
  |        Declination = {{DEC|+49|56|16}}
  | Apparent magnitude = 15.0
  |           Distance = 2610
  |      Spectral type = G?V
  |               Mass = 1.0
  |             Radius = 0.91
  |        Temperature = 5803
  |        Metallicity = -0.079
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes = Super-puff planets with some of the lowest densities known.<ref name="Kepler-51">{{cite journal
 | title=The Featureless Transmission Spectra of Two Super-puff Planets
 | first1=Jessica E. | last1=Libby-Roberts | first2=Zachory K. | last2=Berta-Thompson
 | first3=Jean-Michel | last3=Desert | first4=Kento | last4=Masuda
 | first5=Caroline V. | last5=Morley | first6=Eric D. | last6=Lopez
 | first7=Katherine M. | last7=Deck | first8=Daniel | last8=Fabrycky
 | first9=Jonathan J. | last9=Fortney | first10=Michael R. | last10=Line
 | first11=Roberto | last11=Sanchis-Ojeda | first12=Joshua N. | last12=Winn
 | journal=The Astronomical Journal | year=2020 | volume=159 | issue=2 | page=57 | display-authors=1 | doi=10.3847/1538-3881/ab5d36 | arxiv=1910.12988 | bibcode=2020AJ....159...57L | s2cid=204950000 | doi-access=free }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-403
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|19|41.1}}
  |        Declination = {{DEC|+46|44|40}}
  | Apparent magnitude = 
  |           Distance = 2741
  |      Spectral type = F9IV-V
  |               Mass = 1.25
  |             Radius = 1.45
  |        Temperature = 6090
  |        Metallicity = -0.145
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-9
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|02|17.76}}
  |        Declination = {{DEC|+38|24|03.2}}
  | Apparent magnitude = 13.91
  |           Distance = 2754
  |      Spectral type = G2V
  |               Mass = 0.998
  |             Radius = 1.095
  |        Temperature = 5722
  |        Metallicity = 0.167
  |                Age = 3.008
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = First multiplanetary system to be discovered by the Kepler Space Telescope.<ref>{{cite web |url=http://www.universetoday.com/72104/kepler-discovers-multi-planet-system/ |title=Kepler Discovers Multi-Planet System |author=Nancy Atkinson |date=26 August 2010 |publisher=Universe Today |access-date=13 January 2011 |archive-date=24 February 2012 |archive-url=https://web.archive.org/web/20120224041800/http://www.universetoday.com/72104/kepler-discovers-multi-planet-system/ |url-status=live }}</ref><ref name="Holman2010Kepler-9">{{Cite journal | title=Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations | url=http://www.astro.ubc.ca/people/gladman/a520/Holmanetal2010.pdf | last1=Holman | first1=M. J. | last2=Fabrycky | first2=D. C. | last3=Ragozzine | first3=D. | last4=Ford | first4=E. B. | last5=Steffen | first5=J. H. | last6=Welsh | first6=W. F. | last7=Lissauer | first7=J. J. | last8=Latham | first8=D. W. | last9=Marcy | first9=G. W. | last10=Walkowicz | first10=L. M. | last11=Batalha | first11=N. M. | last12=Jenkins | first12=J. M. | last13=Rowe | first13=J. F. | last14=Cochran | first14=W. D. | last15=Fressin | first15=F. | last16=Torres | first16=G. | last17=Buchhave | first17=L. A. | last18=Sasselov | first18=D. D. | last19=Borucki | first19=W. J. | last20=Koch | first20=D. G. | last21=Basri | first21=G. | last22=Brown | first22=T. M. | last23=Caldwell | first23=D. A. | last24=Charbonneau | first24=D. | last25=Dunham | first25=E. W. | last26=Gautier | first26=T. N. | last27=Geary | first27=J. C. | last28=Gilliland | first28=R. L. | last29=Haas | first29=M. R. | last30=Howell | first30=S. B. | display-authors=1 | journal=Science | volume=330 | issue=6000 | pages=51–54 | year=2010 | bibcode=2010Sci...330...51H | doi=10.1126/science.1195778 | pmid=20798283 | s2cid=8141085 | access-date=2022-06-17 | archive-date=2022-12-07 | archive-url=https://web.archive.org/web/20221207160620/https://www.astro.ubc.ca/people/gladman/a520/Holmanetal2010.pdf | url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-23]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|36|52.0}}
  |        Declination = {{DEC|+49|28|45}}
  | Apparent magnitude = 14
  |           Distance = 2790
  |      Spectral type = G5V
  |               Mass = 1.11
  |             Radius = 1.52
  |        Temperature = 5760
  |        Metallicity = -0.09
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-46
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|17|05.0}}
  |        Declination = {{DEC|+42|36|15}}
  | Apparent magnitude = 15.3
  |           Distance = 2795
  |      Spectral type = K?V
  |               Mass = 0.902
  |             Radius = 0.94
  |        Temperature = 5155
  |        Metallicity = 0.41
  |                Age = 9.9
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-305
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|56|53.83}}
  |        Declination = {{DEC|+40|20|35.46}}
  | Apparent magnitude = 15.812
  |           Distance = 2833
  |      Spectral type = K
  |               Mass = 0.85
  |             Radius = 0.9
  |        Temperature = 4918
  |        Metallicity = -0.071
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-90
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|18|57|44.0}}
  |        Declination = {{DEC|+49|18|19}}
  | Apparent magnitude = 14.0
  |           Distance = 2840 ± 40
  |      Spectral type = F9 IV/V
  |               Mass = 1.13
  |             Radius = 1.2
  |        Temperature = 5930
  |        Metallicity = -0.17
  |                Age = 2
  |  Confirmed planets = 8
  |Unconfirmed planets = 
  |              Notes = All eight exoplanets are larger than Earth and are within 1.1 AU of the parent star. Only star apart from the Sun with at least eight planets.<ref name="NASA-20171214a">{{cite web |last1=Chou |first1=Felicia |last2=Hawkes |first2=Alison |last3=Landau |first3=Elizabeth |title=Artificial Intelligence, NASA Data Used to Discover Eighth Planet Circling Distant Star |url=https://www.jpl.nasa.gov/news/news.php?feature=7026 |date=14 December 2017 |work=[[NASA]] |access-date=15 December 2017 |archive-date=5 May 2020 |archive-url=https://web.archive.org/web/20200505042830/https://www.jpl.nasa.gov/news/news.php?feature=7026 |url-status=live }}</ref> A [[Hill sphere|Hill stability]] test shows that the system is stable.<ref name="Schmitt2014">{{cite journal|last1= Schmitt|first1=J. R.|last2= Wang|first2= J.|last3= Fischer|first3=D. A.|last4= Jek|first4=K. J.|last5= Moriarty|first5=J. C.|last6= Boyajian|first6=T. S.|last7= Schwamb|first7=M. E.|last8= Lintott|first8= C.|last9= Lynn|first9=S.|last10= Smith|first10=A. M.|last11= Parrish|first11= M.|last12= Schawinski|first12= K.|last13= Simpson|first13= R.|last14= LaCourse|first14= D.|last15= Omohundro|first15=M. R.|last16= Winarski|first16= T.|last17= Goodman|first17=S. J.|last18= Jebson|first18= T.|last19= Schwengeler|first19=H. M.|last20= Paterson|first20=D. A.|last21= Sejpka|first21= J.|last22= Terentev|first22= I.|last23= Jacobs|first23= T.|last24= Alsaadi|first24 =N.|last25= Bailey|first25=R. C.|last26= Ginman|first26= T.|last27= Granado|first27= P.|last28= Guttormsen|first28=K. V.|last29= Mallia|first29= F.|last30= Papillon|first30=A. L.|last31= Rossi|first31= F.|last32= Socolovsky|first32= M.|last33= Stiak|first33= L.|title= Planet Hunters. VI. An Independent Characterization of KOI-351 and Several Long Period Planet Candidates From the Kepler Archival Data|journal= The Astronomical Journal|volume= 148|issue= 28|date= 2014-06-26|page=28|doi= 10.1088/0004-6256/148/2/28 |arxiv= 1310.5912|bibcode=2014AJ....148...28S|s2cid=119238163}}</ref> Planet h orbits in the habitable zone.
}}
{{Multiplanetary systems list
  |               Star = Kepler-150
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|12|56.2}}
  |        Declination = {{DEC|+40|31|15}}
  | Apparent magnitude =  
  |           Distance = 2906
  |      Spectral type = G?V
  |               Mass = 0.97
  |             Radius = 0.91
  |        Temperature = 5560
  |        Metallicity = -0.136
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =  
  |              Notes = Planet f orbits in the habitable zone.
}}
{{Multiplanetary systems list
  |               Star = Kepler-82
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|31|29.61}}
  |        Declination = {{DEC|+42|57|58.09}}
  | Apparent magnitude = 15.158
  |           Distance = 2949
  |      Spectral type = G?V
  |               Mass = 0.91
  |             Radius = 0.9
  |        Temperature = 5512
  |        Metallicity = -0.014
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-154
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|19|07.3}}
  |        Declination = {{DEC|+49|53|48}}
  | Apparent magnitude = 
  |           Distance = 2985
  |      Spectral type = G3V
  |               Mass = 0.98
  |             Radius = 1.0
  |        Temperature = 5690
  |        Metallicity = -0.391
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-56]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|35|02.0}}
  |        Declination = {{DEC|+41|52|19}}
  | Apparent magnitude = 13
  |           Distance = 3060
  |      Spectral type = K?III
  |               Mass = 1.32
  |             Radius = 4.23
  |        Temperature = 4840
  |        Metallicity = 0.2
  |                Age = 3.5
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-350
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|01|41.0}}
  |        Declination = {{DEC|+39|42|22}}
  | Apparent magnitude = 13.8
  |           Distance = 3121
  |      Spectral type = F
  |               Mass = 1.03 
  |             Radius = 1.25 
  |        Temperature = 6215
  |        Metallicity = -0.308
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-603
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|37|07.4}}
  |        Declination = {{DEC|+42|17|27}}
  | Apparent magnitude = 
  |           Distance = 3134
  |      Spectral type = G2V
  |               Mass = 1.01
  |             Radius = 1.01
  |        Temperature = 5808
  |        Metallicity = 0.03
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-160
  |      Constellation = Lyra 
  |    Right ascension = {{RA|19|11|05.65}}
  |        Declination = {{DEC|+42|52|09.5}}
  | Apparent magnitude = 13.101
  |           Distance = 3140
  |      Spectral type = G2V
  |               Mass = 
  |             Radius = 1.18
  |        Temperature =5470
  |        Metallicity =-0.361
  |                Age = 
  |  Confirmed planets = 3
  |Unconfirmed planets = 1
  |              Notes = The unconfirmed planet Kepler-160e (or KOI-456.04) is a potentially habitable planet.<ref>{{Cite web|last=Patel|first=Neel V.|date=2020-06-05|title=Astronomers have found a planet like Earth orbiting a star like the sun|url=https://www.technologyreview.com/2020/06/05/1002831/kepler-160-koi-456-04-earth-sun-exoplanet-habitable/|access-date=2020-06-07|website=MIT Technology Review|language=en|archive-date=2023-05-25|archive-url=https://web.archive.org/web/20230525031722/https://www.technologyreview.com/2020/06/05/1002831/kepler-160-koi-456-04-earth-sun-exoplanet-habitable/|url-status=live}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-401
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|20|19.9}}
  |        Declination = {{DEC|+50|51|49}}
  | Apparent magnitude = 
  |           Distance = 3149
  |      Spectral type = F8V
  |               Mass = 1.17
  |             Radius = 1.29
  |        Temperature = 6117
  |        Metallicity = -0.297
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-58
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|45|26.0}}
  |        Declination = {{DEC|+39|06|55}}
  | Apparent magnitude = 15.3
  |           Distance = 3161
  |      Spectral type = G1V
  |               Mass = 1.04
  |             Radius = 1.13
  |        Temperature = 5843
  |        Metallicity = 
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-79
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|20|02|04.11}}
  |        Declination = {{DEC|+44|22|53.69}}
  | Apparent magnitude = 13.914
  |           Distance = 3329
  |      Spectral type = F
  |               Mass = 1.17
  |             Radius = 1.3
  |        Temperature = 6187
  |        Metallicity = -0.263
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}} 
{{Multiplanetary systems list
  |               Star = Kepler-60
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|15|50.70}}
  |        Declination = {{DEC|+42|15|54.04}}
  | Apparent magnitude = 13.959
  |           Distance = 3343
  |      Spectral type = G
  |               Mass = 1.04
  |             Radius = 1.26
  |        Temperature = 5915
  |        Metallicity = -0.116
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-122
  |      Constellation =
  |    Right ascension = {{RA|19|24|26.9}}
  |        Declination = {{DEC|+39|56|57}}
  | Apparent magnitude = 
  |           Distance = 3351 
  |      Spectral type = F
  |               Mass = 1.08
  |             Radius = 1.22
  |        Temperature = 6050
  |        Metallicity = -0.202
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-279
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|09|34.0}}
  |        Declination = {{DEC|+42|11|42}}
  | Apparent magnitude = 13.7
  |           Distance = 3383
  |      Spectral type = F
  |               Mass = 1.1
  |             Radius = 1.07
  |        Temperature = 6562
  |        Metallicity = -0.57
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-255
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|44|15.4}}
  |        Declination = {{DEC|+45|58|37}}
  | Apparent magnitude = 
  |           Distance = 3433
  |      Spectral type = G6V
  |               Mass = 0.90
  |             Radius = 0.86
  |        Temperature = 5573
  |        Metallicity = 0.212
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-47]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|41|11.5}}
  |        Declination = {{DEC|+46|55|13.69}}
  | Apparent magnitude = 15.178
  |           Distance = 3442
  |      Spectral type = G <br> M
  |               Mass = 1.043
  |             Radius = 0.964/0.3506
  |        Temperature = 5636(A) <br> (B is unknown)
  |        Metallicity = -0.25†(A) <br> (B is unknown)
  |                Age = 4.5
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes = Circumbinary planets, with one of the planets orbiting in the habitable zone.<ref name=discoveryKepler-47>{{Cite journal|arxiv= 1208.5489 |title= Kepler-47: A Transiting Circumbinary Multi-Planet System|journal= Science|volume= 337|issue= 6101|pages= 1511–4|last1=  Orosz|first1= Jerome A.|last2=  Welsh|first2= William F.|last3=  Carter|first3= Joshua A.|last4=  Fabrycky|first4= Daniel C.|last5=  Cochran|first5= William D.|last6= Endl|first6= Michael|last7=  Ford|first7= Eric B.|last8= Haghighipour|first8= Nader|last9=  MacQueen|first9= Phillip J.|last10= Mazeh|first10= Tsevi|last11= Sanchis-Ojeda|first11= Roberto|last12=  Short|first12= Donald R.|last13= Torres|first13= Guillermo|last14= Agol|first14= Eric|last15=  Buchhave|first15= Lars A.|last16=  Doyle|first16= Laurance R.|last17= Isaacson|first17= Howard|last18=  Lissauer|first18= Jack J.|last19=  Marcy|first19= Geoffrey W.|last20= Shporer|first20= Avi|last21= Windmiller|first21= Gur|last22= Barclay|first22= Thomas|last23=  Boss|first23= Alan P.|last24=  Clarke|first24= Bruce D.|last25= Fortney|first25= Jonathan|last26=  Geary|first26= John C.|last27=  Holman|first27= Matthew J.|last28= Huber|first28= Daniel|last29=  Jenkins|first29= Jon M.|last30= Kinemuchi|first30= Karen|display-authors= 29|year= 2012|doi= 10.1126/science.1228380 |pmid=22933522|bibcode = 2012Sci...337.1511O |s2cid= 44970411 }}</ref><ref name=NASAKepler-47>{{cite news|url=http://www.nasa.gov/mission_pages/kepler/news/kepler-47.html|title=NASA's Kepler Discovers Multiple Planets Orbiting a Pair of Stars|date=28 August 2012|publisher=[[NASA]]|website=exoplanets.nasa.gov|quote=Kepler mission has discovered multiple transiting planets orbiting two suns for the first time|access-date=2 September 2012|archive-date=31 October 2012|archive-url=https://web.archive.org/web/20121031024345/http://www.nasa.gov/mission_pages/kepler/news/kepler-47.html|url-status=dead}}</ref><ref name="ScienceDaily2012Kepler-47">{{cite journal |url=https://www.sciencedaily.com/releases/2012/08/120828190127.htm |title=NASA's Kepler discovers multiple planets orbiting a pair of stars |doi=10.1126/science.1228380 |publisher=[[Sciencedaily.com]] |date=28 August 2012 |access-date=4 November 2012 |arxiv=1208.5489 |bibcode=2012Sci...337.1511O |last1=Orosz |first1=Jerome A. |last2=Welsh |first2=William F. |last3=Carter |first3=Joshua A. |last4=Fabrycky |first4=Daniel C. |last5=Cochran |first5=William D. |last6=Endl |first6=Michael |last7=Ford |first7=Eric B. |last8=Haghighipour |first8=Nader |last9=MacQueen |first9=Phillip J. |last10=Mazeh |first10=Tsevi |last11=Sanchis-Ojeda |first11=Roberto |last12=Short |first12=Donald R. |last13=Torres |first13=Guillermo |last14=Agol |first14=Eric |last15=Buchhave |first15=Lars A. |last16=Doyle |first16=Laurance R. |last17=Isaacson |first17=Howard |last18=Lissauer |first18=Jack J. |last19=Marcy |first19=Geoffrey W. |last20=Shporer |first20=Avi |last21=Windmiller |first21=Gur |last22=Barclay |first22=Thomas |last23=Boss |first23=Alan P. |last24=Clarke |first24=Bruce D. |last25=Fortney |first25=Jonathan |last26=Geary |first26=John C. |last27=Holman |first27=Matthew J. |last28=Huber |first28=Daniel |last29=Jenkins |first29=Jon M. |last30=Kinemuchi |first30=Karen |journal=Science |volume=337 |issue=6101 |pages=1511–4 |pmid=22933522 |s2cid=44970411 |display-authors=29 |archive-date=21 September 2022 |archive-url=https://web.archive.org/web/20220921182959/https://www.sciencedaily.com/releases/2012/08/120828190127.htm |url-status=live }}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-292
  |      Constellation =
  |    Right ascension = {{RA|19|43|03.84}}
  |        Declination = {{DEC|+43|25|27.4}}
  | Apparent magnitude = 13.97
  |           Distance = 3446
  |      Spectral type = K0V
  |               Mass = 0.85
  |             Radius = 0.826
  |        Temperature = 5299
  |        Metallicity = 0.077
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-27]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|28|56.82}}
  |        Declination = {{DEC|+41|05|9.15}}
  | Apparent magnitude = 15.855
  |           Distance = 3500
  |      Spectral type = G5V
  |               Mass = 0.65
  |             Radius = 0.59
  |        Temperature = 5400
  |        Metallicity = +0.41
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets = 
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-351
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|05|48.6}}
  |        Declination = {{DEC|+42|39|28}}
  | Apparent magnitude = 
  |           Distance = 3535
  |      Spectral type = G?V
  |               Mass = 0.89
  |             Radius = 0.85
  |        Temperature = 5643
  |        Metallicity = -0.134
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-276
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|34|16}}
  |        Declination = {{DEC|+39|02|11}}
  | Apparent magnitude = 15.368
  |           Distance = 3734
  |      Spectral type = G?V
  |               Mass = 1.1
  |             Radius = 1.03
  |        Temperature = 5812
  |        Metallicity = 0.012
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-24
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|21|39.18}}
  |        Declination = {{DEC|+38|20|37.51}}
  | Apparent magnitude = 14.925
  |           Distance = 3910
  |      Spectral type = G1V
  |               Mass = 1.03
  |             Radius = 1.07
  |        Temperature = 5800
  |        Metallicity = -0.24
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-87
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|51|40.0}}
  |        Declination = {{DEC|+46|57|54}}
  | Apparent magnitude = 15
  |           Distance = 4021
  |      Spectral type = G4IV
  |               Mass = 1.1
  |             Radius = 1.82
  |        Temperature = 5600
  |        Metallicity = -0.17
  |                Age = 7.5
  |  Confirmed planets = 2
  |Unconfirmed planets = 2
  |              Notes = Farthest system from the Sun with an unconfirmed exoplanet candidate. 
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-33]]
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|16|18.61}}
  |        Declination = {{DEC|+46|00|18.8}}
  | Apparent magnitude = 13.988
  |           Distance = 4090
  |      Spectral type = G1IV
  |               Mass = 1.164
  |             Radius = 1.615
  |        Temperature = 5849
  |        Metallicity = 0.12
  |                Age = 4.27
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-282
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|58|43.0}}
  |        Declination = {{DEC|+44|47|51}}
  | Apparent magnitude = 15.2
  |           Distance = 4363
  |      Spectral type = G?V
  |               Mass = 0.97
  |             Radius = 0.89
  |        Temperature = 5876
  |        Metallicity = -0.374
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-758
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|32|20.3}}
  |        Declination = {{DEC|+41|08|08}}
  | Apparent magnitude = 
  |           Distance = 4413
  |      Spectral type =
  |               Mass = 1.16
  |             Radius = 1.42
  |        Temperature = 6228
  |        Metallicity = -0.1
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets = 
  |              Notes = Farthest system from the Sun with exactly four confirmed exoplanets.
}}
{{Multiplanetary systems list
  |               Star = Kepler-53
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|21|51.0}}
  |        Declination = {{DEC|+40|33|45}}
  | Apparent magnitude = 16
  |           Distance = 4455
  |      Spectral type = G?V
  |               Mass = 0.98
  |             Radius = 0.89
  |        Temperature = 5858
  |        Metallicity =  
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-30
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|01|08.07}}
  |        Declination = {{DEC|+38|56|50.21}}
  | Apparent magnitude = 15.403
  |           Distance = 4560
  |      Spectral type = G6V
  |               Mass = 0.99
  |             Radius = 0.95
  |        Temperature = 5498
  |        Metallicity = +0.18
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-84]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|53|00.49}}
  |        Declination = {{DEC|+40|29|45.87}}
  | Apparent magnitude = 14.764
  |           Distance = 4700
  |      Spectral type = G3IV
  |               Mass = 1
  |             Radius = 1.43
  |        Temperature = 5755
  |        Metallicity = -0.131
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-385]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|37|21.23}}
  |        Declination = {{DEC|+50|20|11.55}}
  | Apparent magnitude = 15.76
  |           Distance = 4900
  |      Spectral type = F8V
  |               Mass = 0.99
  |             Radius = 1.09
  |        Temperature = 5835
  |        Metallicity = 0.010
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets = 4
  |              Notes = 
}}
{{Multiplanetary systems list
  |               Star = [[Kepler-31]]
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|36|06.0}}
  |        Declination = {{DEC|+45|51|11}}
  | Apparent magnitude = 15.5
  |           Distance = 5429 
  |      Spectral type = F
  |               Mass = 1.21
  |             Radius = 1.22
  |        Temperature = 6340
  |        Metallicity = -0.08
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes = The three planets are in an orbital resonance.<ref name=Kepler-31resonance>{{citation|arxiv=1903.09474|title=The role of dissipative evolution for three-planet, near-resonant extrasolar systems|year=2019|doi=10.1051/0004-6361/201935259|last1=Pichierri|first1=Gabriele|last2=Batygin|first2=Konstantin|last3=Morbidelli|first3=Alessandro|journal=Astronomy & Astrophysics|volume=625|pages=A7|bibcode=2019A&A...625A...7P|s2cid=85459759}}</ref>
}}
{{Multiplanetary systems list
  |               Star = Kepler-238
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|11|35}}
  |        Declination = {{DEC|+40|38|16}}
  | Apparent magnitude = 15.084
  |           Distance = 5867
  |      Spectral type = G5IV
  |               Mass = 1.06
  |             Radius = 1.43
  |        Temperature = 5614
  |        Metallicity = 0.143
  |                Age =
  |  Confirmed planets = 5
  |Unconfirmed planets =
  |              Notes = One of the farthest systems from the Sun with a multiplanetary system, and the farthest system where exoplanets were discovered by the [[Kepler space telescope]].
}}

{{Multiplanetary systems list
  |               Star = Kepler-245
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|26|33.4}}
  |        Declination = {{DEC|+42|26|11}}
  | Apparent magnitude = 
  |           Distance =
  |      Spectral type =
  |               Mass = 0.8
  |             Radius = 0.8
  |        Temperature = 5100
  |        Metallicity = -0.028
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-218
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|41|39.1}}
  |        Declination = {{DEC|+46|15|59}}
  | Apparent magnitude = 
  |           Distance =
  |      Spectral type =
  |               Mass =  
  |             Radius = 1.06
  |        Temperature = 5502
  |        Metallicity = 0.194
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-217
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|32|09.1}}
  |        Declination = {{DEC|+46|16|39}}
  | Apparent magnitude = 
  |           Distance =
  |      Spectral type =
  |               Mass =  
  |             Radius = 1.8
  |        Temperature = 6171
  |        Metallicity = 
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-192
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|11|40.3}}
  |        Declination = {{DEC|+45|35|34}}
  | Apparent magnitude = 
  |           Distance =
  |      Spectral type =
  |               Mass =  
  |             Radius = 1.01
  |        Temperature = 5479
  |        Metallicity = -0.153
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-191
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|24|44.0}}
  |        Declination = {{DEC|+45|19|23}}
  | Apparent magnitude = 
  |           Distance =
  |      Spectral type =
  |               Mass = 0.85 
  |             Radius = 0.79
  |        Temperature = 5282
  |        Metallicity = 0.006
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-176
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|38|40.3}}
  |        Declination = {{DEC|+43|51|12}}
  | Apparent magnitude = 
  |           Distance =
  |      Spectral type =
  |               Mass = 
  |             Radius = 0.89
  |        Temperature = 5232
  |        Metallicity = 0.072
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-431
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|44|26.9}}
  |        Declination = {{DEC|+43|13|40}}
  | Apparent magnitude =  
  |           Distance =
  |      Spectral type =  
  |               Mass = 1.071
  |             Radius = 1.092
  |        Temperature = 6004
  |        Metallicity = 0.07
  |                Age =  
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-338
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|51|54.9}}
  |        Declination = {{DEC|+40|47|04}}
  | Apparent magnitude =   
  |           Distance =
  |      Spectral type =  
  |               Mass = 1.1
  |             Radius = 1.74
  |        Temperature = 5923
  |        Metallicity = -0.106
  |                Age =   
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-197
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|40|54.3}}
  |        Declination = {{DEC|+50|33|32}}
  | Apparent magnitude =   
  |           Distance =
  |      Spectral type =  
  |               Mass =  
  |             Radius = 1.12
  |        Temperature = 6004
  |        Metallicity = -0.533
  |                Age =   
  |  Confirmed planets = 4
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-247
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|14|34.2}}
  |        Declination = {{DEC|+43|02|21}}
  | Apparent magnitude =    
  |           Distance =
  |      Spectral type =  
  |               Mass = 0.884 
  |             Radius = 0.791
  |        Temperature = 5094
  |        Metallicity = 0.21
  |                Age =    
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-104
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|10|25.1}}
  |        Declination = {{DEC|+42|10|00}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =  
  |               Mass = 0.81
  |             Radius = 1.35
  |        Temperature = 5711
  |        Metallicity = -0.777 
  |                Age =  
  |  Confirmed planets = 3 
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-126
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|17|23.4}}
  |        Declination = {{DEC|+44|12|31}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =  
  |             Radius = 1.36
  |        Temperature = 6239
  |        Metallicity =  
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-127
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|00|45.6}}
  |        Declination = {{DEC|+46|01|41}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =  
  |             Radius = 1.36
  |        Temperature = 6106
  |        Metallicity = -0.154 
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-130
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|13|48.2}}
  |        Declination = {{DEC|+40|14|43}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 1.0 
  |             Radius = 1.13
  |        Temperature = 5884
  |        Metallicity = 0.02
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-164
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|11|07.4}}
  |        Declination = {{DEC|+47|37|48}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 1.11
  |             Radius = 1.15
  |        Temperature = 5888
  |        Metallicity = -0.125
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-171
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|47|05.3}}
  |        Declination = {{DEC|+41|45|20}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 
  |             Radius = 0.84
  |        Temperature = 5642
  |        Metallicity = -0.151
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-172
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|47|05.3}}
  |        Declination = {{DEC|+41|45|20}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.86
  |             Radius = 1.08 
  |        Temperature = 5526
  |        Metallicity = 0.012
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets =
}}
{{Multiplanetary systems list
  |               Star = Kepler-149
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|03|24.9}}
  |        Declination = {{DEC|+38|23|03}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =  
  |             Radius = 0.95  
  |        Temperature = 5381
  |        Metallicity = 0.147
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-142
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|40|28.5}}
  |        Declination = {{DEC|+48|28|53}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.99   
  |             Radius = 1.27  
  |        Temperature = 5790
  |        Metallicity = -0.274
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-124
  |      Constellation = Draco (constellation){{!}}Draco
  |    Right ascension = {{RA|19|07|00.7}}
  |        Declination = {{DEC|+49|03|54}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =    
  |             Radius = 0.64
  |        Temperature = 4984
  |        Metallicity = -0.535
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}

{{Multiplanetary systems list
  |               Star = Kepler-402
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|13|28.9}}
  |        Declination = {{DEC|+43|21|17}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =      
  |             Radius = 1.26 
  |        Temperature = 6090
  |        Metallicity = -0.22
  |                Age =
  |  Confirmed planets = 4
  |Unconfirmed planets = 1
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-399
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|58|00.4}}
  |        Declination = {{DEC|+40|40|15}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =      
  |             Radius = 0.68  
  |        Temperature = 5502
  |        Metallicity = -0.827
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-374
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|36|33.1}}
  |        Declination = {{DEC|+42|22|14}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.84
  |             Radius = 0.91 
  |        Temperature = 5977
  |        Metallicity = -0.441
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-372
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|25|01.5}}
  |        Declination = {{DEC|+49|15|32}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 1.15
  |             Radius = 1.14
  |        Temperature = 6509
  |        Metallicity = -0.137
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-363
  |      Constellation = Lyra
  |    Right ascension = {{RA|18|52|46.1}}
  |        Declination = {{DEC|+41|18|19}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 1.23
  |             Radius = 1.49
  |        Temperature = 5593
  |        Metallicity = 0.299
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-359
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|33|10.5}}
  |        Declination = {{DEC|+42|11|47}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 1.07
  |             Radius = 1.09
  |        Temperature = 6248
  |        Metallicity = -0.039
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-357
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|24|58.3}}
  |        Declination = {{DEC|+44|00|31}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.78
  |             Radius = 0.83
  |        Temperature = 5036
  |        Metallicity = 0.051
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-354
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|03|00.4}}
  |        Declination = {{DEC|+41|20|08}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.65 
  |             Radius = 0.67
  |        Temperature = 4648
  |        Metallicity = -0.036
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =  
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-206
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|26|32.3}}
  |        Declination = {{DEC|+41|50|02}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.94
  |             Radius = 1.19
  |        Temperature = 5764
  |        Metallicity = -0.149
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-203
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|01|23.3}}
  |        Declination = {{DEC|+41|45|43}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.98  
  |             Radius = 1.11
  |        Temperature = 5821
  |        Metallicity = -0.107
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-194
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|27|53.1}}
  |        Declination = {{DEC|+47|51|51}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =    
  |             Radius = 1.02
  |        Temperature = 6089
  |        Metallicity = -0.298
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-184
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|27|48.5}}
  |        Declination = {{DEC|+43|04|29}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =  
  |             Radius = 0.87
  |        Temperature = 5788
  |        Metallicity = -0.338
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-178
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|08|24.3}}
  |        Declination = {{DEC|+46|53|47}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass =  
  |             Radius = 1.07
  |        Temperature = 5676
  |        Metallicity = -0.188
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-336
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|20|57.0}}
  |        Declination = {{DEC|+41|19|53}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.89 
  |             Radius = 1.3
  |        Temperature = 5867
  |        Metallicity = -0.401
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-334
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|08|33.8}}
  |        Declination = {{DEC|+47|06|55}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 1.0 
  |             Radius = 1.07
  |        Temperature = 5828
  |        Metallicity = -0.074
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-332
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|06|39.1}}
  |        Declination = {{DEC|+47|24|49}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.8 
  |             Radius = 0.72
  |        Temperature = 4955
  |        Metallicity = 0.05
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-331
  |      Constellation = Lyra
  |    Right ascension = {{RA|19|27|20.2}}
  |        Declination = {{DEC|+39|18|26}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.51 
  |             Radius = 0.49
  |        Temperature = 4347
  |        Metallicity = -0.85
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-327
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|30|34.2}}
  |        Declination = {{DEC|44|05|16}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.55 
  |             Radius = 0.49 
  |        Temperature = 3799
  |        Metallicity = -0.042
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-326
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|37|18.1}}
  |        Declination = {{DEC|+46|00|08}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.98 
  |             Radius = 0.8
  |        Temperature = 5105
  |        Metallicity = 0.133
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list
  |               Star = Kepler-325
  |      Constellation = Cygnus (constellation){{!}}Cygnus
  |    Right ascension = {{RA|19|19|20.5}}
  |        Declination = {{DEC|+49|49|32}}
  | Apparent magnitude =  
  |           Distance =  
  |      Spectral type =
  |               Mass = 0.87 
  |             Radius = 1.0
  |        Temperature = 5752
  |        Metallicity = -0.171
  |                Age =
  |  Confirmed planets = 3
  |Unconfirmed planets =
  |              Notes =
}}
{{Multiplanetary systems list/Bottom}}

==Stars orbited by both planets and brown dwarfs==
These are stars orbited by objects on both sides of the ~13 [[Jupiter mass]] dividing line.

* [[54 Piscium]] (HD 3651)<ref>{{cite journal | display-authors=1 | last1=Mugrauer | first1=M. | last2=Seifahrt | first2=A. | last3=Neuhäuser | first3=R. | last4=Mazeh | first4=T. | title=HD 3651 B: the first directly imaged brown dwarf companion of an exoplanet host star | journal=Monthly Notices of the Royal Astronomical Society: Letters | volume=373 | issue=1 | pages=L31–L35 | date=2006 | doi=10.1111/j.1745-3933.2006.00237.x | doi-access=free | type=abstract | arxiv=astro-ph/0608484 | bibcode=2006MNRAS.373L..31M | s2cid=15608344 }}</ref>
* [[HD 168443]]<ref>{{cite journal
 | title=Two New Planets in Eccentric Orbits
 | last1=Marcy | first1=Geoffrey W. | last2=Butler | first2=R. Paul
 | last3=Vogt | first3=Steven S. | last4=Fischer | first4=Debra
 | last5=Liu | first5=Michael C. | display-authors=1
 | journal=The Astrophysical Journal
 | volume=520 | issue=1 | pages=239–247 | year=1999
 | arxiv=astro-ph/9904275 | bibcode=1999ApJ...520..239M
 | doi=10.1086/307451 | s2cid=16827678 }}</ref><ref>{{cite journal
 | title=Two Substellar Companions Orbiting HD 168443
 | last1=Marcy | first1=Geoffrey W. | last2=Butler | first2=R. Paul
 | last3=Vogt | first3=Steven S. | last4=Liu | first4=Michael C.
 | last5=Laughlin | first5=Gregory | last6=Apps | first6=Kevin
 | last7=Graham | first7=J. R. | last8=Lloyd | first8=J.
 | last9=Luhman | first9=Kevin L. | first10=Ray | last10=Jayawardhana
 | display-authors=1 | journal=The Astrophysical Journal
 | volume=555 | issue=1 | pages=418–425 | year=2001
 | bibcode=2001ApJ...555..418M | doi=10.1086/321445 | doi-access=free }}</ref>
* [[HD 4113]] A<ref name=Cheetham2018>{{cite journal
 | title=Direct imaging of an ultracool substellar companion to the exoplanet host star HD 4113 A
 | last1=Cheetham | first1=A. | last2=Ségransan | first2=D.
 | last3=Peretti | first3=S. | last4=Delisle | first4=J. -B.
 | last5=Hagelberg | first5=J. | last6=Beuzit | first6=J. -L.
 | last7=Forveille | first7=T. | last8=Marmier | first8=M.
 | last9=Udry | first9=S. | last10=Wildi | first10=F.
 | display-authors=1 | journal=Astronomy & Astrophysics
 | volume=614 | id=A16 | pages=19 | date=June 2018
 | arxiv=1712.05217 | bibcode=2018A&A...614A..16C 
 | doi=10.1051/0004-6361/201630136 | s2cid=119084543 }}</ref>
* [[Epsilon Indi]] A<ref>{{Citation | title=Detection of the nearest Jupiter analog in radial velocity and astrometry data | first1=Fabo | last1=Feng | first2=Guillem  | last2=Anglada-Escudé | first3=Mikko | last3=Tuomi | first4=Hugh R. A. | last4=Jones | first5=Julio | last5=Chanamé | first6=Paul R. | last6=Butler | first7=Markus | last7=Janson | journal=Monthly Notices of the Royal Astronomical Society | arxiv=1910.06804 | date=14 October 2019 | volume=490 | issue=4 | pages=5002–5016 | doi=10.1093/mnras/stz2912 | doi-access=free | bibcode=2019MNRAS.490.5002F | s2cid=204575783 }}</ref><ref>{{cite news|last=Scholz |first=Ralf-Dieter |author2=McCaughrean, Mark |date=2003-01-13 |title=Discovery of Nearest Known Brown Dwarf: Bright Southern Star Epsilon Indi Has Cool, Substellar Companion |publisher=European Southern Observatory |url=http://www.eso.org/public/outreach/press-rel/pr-2003/pr-01-03.html |access-date=2006-05-24 |url-status=dead |archive-url=https://web.archive.org/web/20071014191814/http://eso.org/public/outreach/press-rel/pr-2003/pr-01-03.html |archive-date=October 14, 2007 }}</ref><ref>{{cite journal | last=Scholz | first=R.-D. | author2=McCaughrean, M. J. | author3=Lodieu, N. | author4=Kuhlbrodt, B. | title=ε Indi B: A new benchmark T dwarf | journal=Astronomy and Astrophysics | date=February 2003 | volume=398 | issue=3 | pages=L29–L33 | bibcode=2003A&A...398L..29S | doi=10.1051/0004-6361:20021847 | arxiv=astro-ph/0212487 | s2cid=119474823 }}</ref>
* [[HD 82943]]<ref>{{cite journal | title=Catalog of Nearby Exoplanets | last1=Butler | first1=R. P. | last2=Wright | first2=J. T. | last3=Marcy | first3=G. W. | last4=Fischer | first4=D. A. | last5=Vogt | first5=S. S. | last6=Tinney | first6=C. G. | last7=Jones | first7=H. R. A. | last8=Carter | first8=B. D. | last9=Johnson | first9=J. A. | display-authors=1 | journal=The Astrophysical Journal | date=2006 | volume=646 | issue=1 | pages=505–522 | arxiv=astro-ph/0607493 | bibcode=2006ApJ...646..505B | doi=10.1086/504701 | s2cid=119067572 }}</ref>
* [[Pi Mensae]] (TOI-144)<ref>{{cite journal |last1=Feng |first1=Fabo |last2=Butler |first2=R. Paul |display-authors=etal |date=August 2022 |title=3D Selection of 167 Substellar Companions to Nearby Stars |journal=[[The Astrophysical Journal Supplement Series]] |volume=262 |issue=21 |page=21 |doi=10.3847/1538-4365/ac7e57 |arxiv=2208.12720 |bibcode=2022ApJS..262...21F|s2cid=251864022 |doi-access=free }}</ref><ref>{{cite journal | arxiv=2203.01018| doi=10.3847/1538-3881/ac5dcb| title=A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit| year=2022| last1=Hatzes| first1=Artie P.| last2=Gandolfi| first2=Davide| last3=Korth| first3=Judith| last4=Rodler| first4=Florian| last5=Sabotta| first5=Silvia| last6=Esposito| first6=Massimiliano| last7=Barragán| first7=Oscar| last8=Van Eylen| first8=Vincent| last9=Livingston| first9=John H.| last10=Serrano| first10=Luisa Maria| last11=Luque| first11=Rafael| last12=Smith| first12=Alexis M. S.| last13=Redfield| first13=Seth| last14=Persson| first14=Carina M.| last15=Pätzold| first15=Martin| last16=Palle| first16=Enric| last17=Nowak| first17=Grzegorz| last18=Osborne| first18=Hannah L. M.| last19=Narita| first19=Norio| last20=Mathur| first20=Savita| last21=Lam| first21=Kristine W. F.| last22=Kabáth| first22=Petr| last23=Johnson| first23=Marshall C.| last24=Guenther| first24=Eike W.| last25=Grziwa| first25=Sascha| last26=Goffo| first26=Elisa| last27=Fridlund| first27=Malcolm| last28=Endl| first28=Michael| last29=Deeg| first29=Hans J.| last30=Csizmadia| first30=Szilard| journal=The Astronomical Journal| volume=163| issue=5| page=223| bibcode=2022AJ....163..223H| s2cid=247218413| display-authors=1| doi-access=free}}</ref>
* [[HD 38529]]<ref>{{cite journal | title=A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529 | last1=Fischer | first1=Debra A. | last2=Marcy | first2=Geoffrey W. | last3=Butler | first3=R. Paul | last4=Vogt | first4=Steven S. | last5=Henry | first5=Gregory W. | last6=Pourbaix | first6=Dimitri | last7=Walp | first7=Bernard | last8=Misch | first8=Anthony A. | last9=Wright | first9=Jason T. | display-authors=1 | journal=The Astrophysical Journal | volume=586 | issue=2 |  pages=1394–1408 | year=2003 | bibcode=2003ApJ...586.1394F | bibcode-access=free | doi=10.1086/367889 | doi-access=free }}</ref>
* [[HD 245134]]<ref>{{Cite journal |last1=Khandelwal |first1=Akanksha |last2=Sharma |first2=Rishikesh |last3=Chakraborty |first3=Abhijit |last4=Chaturvedi |first4=Priyanka |last5=Ulmer-Moll |first5=Solène |last6=Ciardi |first6=David R. |last7=Boyle |first7=Andrew W. |last8=Baliwal |first8=Sanjay |last9=Bieryla |first9=Allyson |last10=Latham |first10=David W. |last11=Prasad |first11=Neelam J. S. S. V. |last12=Nayak |first12=Ashirbad |last13=Lendl |first13=Monika |last14=Mordasini |first14=Christoph |date=2023-04-01 |title=Discovery of a massive giant planet with extreme density around the sub-giant star TOI-4603 |url=https://www.aanda.org/articles/aa/abs/2023/04/aa45608-22/aa45608-22.html |journal=Astronomy & Astrophysics |language=en |volume=672 |pages=L7 |doi=10.1051/0004-6361/202245608 |issn=0004-6361 |doi-access=free |arxiv=2303.11841 |bibcode=2023A&A...672L...7K |access-date=2023-12-15 |archive-date=2024-02-28 |archive-url=https://web.archive.org/web/20240228142329/https://www.aanda.org/articles/aa/abs/2023/04/aa45608-22/aa45608-22.html |url-status=live }}</ref>
* [[KMT-2020-BLG-0414L]]<ref name="Zhang2024">{{cite journal |last1=Zhang |first1=Keming |last2=Zang |first2=Weicheng |last3=El-Badry |first3=Kareem |last4=Lu |first4=Jessica R. |display-authors=etal |date=September 2024 |title=An Earth-mass planet and a brown dwarf in orbit around a white dwarf |journal=[[Nature Astronomy]] |volume= 8 |issue = 12 |pages = 1575–1582 |doi=10.1038/s41550-024-02375-9 |arxiv=2409.02157 |bibcode=2024NatAs...8.1575Z}}</ref>

==See also==
{{cmn|
* [[Lists of exoplanets]]
* [[Methods of detecting exoplanets]]
* [[List of exoplanet firsts]]
* [[List of exoplanet extremes]]
* [[List of brown dwarfs]]
* [[Lists of stars]]
* [[List of nearest stars]]
* [[List of stars with proplyds]]
* [[Lists of astronomical objects]]

For links to specific lists of exoplanets see:
* [[List of exoplanets detected by microlensing]]
* [[List of exoplanets detected by radial velocity]]
* [[List of exoplanets detected by timing]]
* [[List of directly imaged exoplanets]]
* [[List of transiting exoplanets]]
* [[List of nearest terrestrial exoplanet candidates]]

Online archives:
* [[NASA Exoplanet Archive]]
}}

<!-- ==Notes==
{{Reflist|group=note}} -->

==Notes==
{{notelist}}

==References==
{{Reflist}}

{{exoplanet}}
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[[Category:Planetary systems|*List]]
[[Category:Lists of exoplanets|Multiplanetary systems]]