View source for Moons of Saturn

{{Use mdy dates|date=November 2025}}
{{Short description|Natural satellites of the planet Saturn}}
{{Featured list}}
[[File:Saturn - September 9 2007 - Annotated (50316920862).jpg|thumb|upright=2|An annotated picture of [[Saturn]]'s many moons captured by the [[Cassini–Huygens|''Cassini'']] spacecraft. Shown in the image are [[Dione (moon)|Dione]], [[Enceladus]], [[Epimetheus (moon)|Epimetheus]], [[Prometheus (moon)|Prometheus]], [[Mimas]], [[Rhea (moon)|Rhea]], [[Janus (moon)|Janus]], [[Tethys (moon)|Tethys]] and [[Titan (moon)|Titan]].]]
[[File:Saturn irregular moon orbits tilted annotated 2025.png|thumb|upright=2|Diagram showing the highly clustered orbits of Saturn's 250 known outer [[irregular moon]]s {{asof|2025|lc=y}}. Majority of these irregular moons orbit [[retrograde motion|retrograde]], or opposite to the direction of Saturn's rotation. The orbits of retrograde moons are colored red while the orbits of prograde moons are colored blue.]]

There are 274 known [[Natural satellite|moons]] of the planet [[Saturn]], the most of any planet in the [[Solar System]].<ref name="MPEC-2025-E155">{{cite web |date=11 March 2025 |title=MPEC 2025-E155 : THIRTY-THREE NEW SATURNIAN SATELLITES |url=https://minorplanetcenter.net/mpec/K25/K25EF5.html |accessdate=11 March 2025 |publisher=Minor Planet Center}}</ref> Saturn's moons are diverse in size, ranging from tiny [[moonlet]]s to [[Titan (moon)|Titan]], which is larger than the planet [[Mercury (planet)|Mercury]]. Three of these moons possess particularly notable features: Titan, Saturn's largest moon (and the second largest moon in the Solar System), has a [[Atmosphere of Titan#Composition|nitrogen-rich]], Earth-like [[Atmosphere of Titan|atmosphere]] and a landscape featuring river networks and [[lakes of Titan|hydrocarbon lakes]],<ref>{{cite web |last=Redd |first=Nola Taylor |url=https://www.space.com/15257-titan-saturn-largest-moon-facts-discovery-sdcmp.html |title=Titan: Facts About Saturn's Largest Moon |work=[[Space.com]] |date=27 March 2018 |access-date=7 October 2019 |archive-date=15 October 2017 |archive-url=https://web.archive.org/web/20171015185936/https://www.space.com/15257-titan-saturn-largest-moon-facts-discovery-sdcmp.html |url-status=live}}</ref> [[Enceladus]] emits jets of ice from its south-polar region and is covered in a deep layer of snow,<ref>{{cite web|url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Enceladus|title=Enceladus - Overview - Planets - NASA Solar System Exploration|url-status=dead|archive-url=https://web.archive.org/web/20130217190247/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Enceladus|archive-date=2013-02-17}}</ref> and [[Iapetus (moon)|Iapetus]] has contrasting black and white hemispheres as well as an [[Equatorial ridge on Iapetus|extensive ridge of equatorial mountains]] which are among [[List of tallest mountains in the Solar System|the tallest in the solar system]].

Twenty-four of the known moons are [[regular moon|regular satellites]]; they have [[prograde orbit]]s not greatly [[inclination|inclined]] to Saturn's equatorial plane (except Iapetus, which has a prograde but highly inclined orbit).<ref>{{cite web|url=http://abyss.uoregon.edu/~js/ast121/lectures/lec17.html|title=Moons|access-date=2013-02-13|archive-date=2013-04-20|archive-url=https://web.archive.org/web/20130420125226/http://abyss.uoregon.edu/~js/ast121/lectures/lec17.html|url-status=live}}</ref><ref>{{Cite web|url=https://science.nasa.gov/saturn/moons/iapetus/|title=Iapetus - NASA Science|website=science.nasa.gov|date=December 2017 |access-date=2024-01-06|archive-date=2024-01-06|archive-url=https://web.archive.org/web/20240106100409/https://science.nasa.gov/saturn/moons/iapetus/|url-status=live}}</ref><ref>{{cite web | url=https://www.nasa.gov/image-article/view-from-iapetus/#:~:text=the%20Saturn%20System.-,Iapetus%20(1%2C468%20kilometers%2C%20or%20912%20miles%20across)%20is%20the,a%20tilt%2C%20as%20seen%20here | title=The View from Iapetus - NASA | access-date=2024-01-06 | archive-date=2024-06-16 | archive-url=https://web.archive.org/web/20240616103717/https://www.nasa.gov/image-article/view-from-iapetus/#:~:text=the%20Saturn%20System.-,Iapetus%20(1%2C468%20kilometers%2C%20or%20912%20miles%20across)%20is%20the,a%20tilt%2C%20as%20seen%20here | url-status=live}}</ref> They include the seven major satellites, four small moons that exist in a [[trojan moon|trojan]] orbit with larger moons, and five that act as [[shepherd moon]]s, of which two are mutually [[Co-orbital configuration|co-orbital]]. At least two tiny moons orbit inside of Saturn's [[B Ring|B]] and [[Rings of Saturn#G Ring|G rings]]. The relatively large [[Hyperion (moon)|Hyperion]] is locked in an [[orbital resonance]] with Titan. The remaining regular moons orbit near the outer edges of the dense [[A Ring]] and the narrow [[F Ring]], and between the major moons [[Mimas]] and Enceladus. The regular satellites are traditionally named after [[Titans]] and Titanesses or other figures associated with the mythological [[Saturn (mythology)|Saturn]].

The remaining 250, with mean diameters ranging from {{cvt|2 to 213|km|mi|0}}, orbit much farther from Saturn. They are [[irregular satellite]]s, having high orbital [[inclination]]s and [[orbital eccentricity|eccentricities]] mixed between [[prograde and retrograde]]. These moons are probably captured [[minor planet]]s, or fragments from the [[impact event|collisional]] breakup of such bodies after they were captured, creating [[collisional family|collisional families]]. The irregular satellites are classified by their orbital characteristics into the prograde [[Inuit group|Inuit]] and [[Gallic group|Gallic]] groups and the large retrograde [[Norse group]], and their names are chosen from the corresponding mythologies (with the Gallic group corresponding to [[Celtic mythology]]). {{as of|2025|3|post=,}} 210 of these are unnamed (plus the designated B-ring moonlet [[S/2009 S 1]]).<ref name="NameSaturnsMoons">{{cite web |date=7 October 2019 |title=Help Name 20 Newly Discovered Moons of Saturn! |url=https://carnegiescience.edu/NameSaturnsMoons |url-status=live |archive-url=https://web.archive.org/web/20191009031345/https://carnegiescience.edu/NameSaturnsMoons |archive-date=9 October 2019 |access-date=9 October 2019 |publisher=Carnegie Science}}</ref><ref name="Carnegie2019" /> [[Phoebe (moon)|Phoebe]], the largest irregular Saturnian moon, is the sole exception to this naming system; it is part of the Norse group but named for a Greek Titaness.

The rings of Saturn are made up of objects ranging in size from microscopic to [[moonlet]]s hundreds of meters across, each in its own orbit around Saturn.<ref name="Esposito2002" /> The number of moons given above does not include these moonlets, nor hundreds of possible kilometer-sized distant moons that have been observed on single occasions.<ref name="SheppardMoons" /><ref name="Tiscareno2008" /><ref name="Ashton2021" /> Thus an absolute number of Saturnian moons cannot be given, because there is no consensus on a boundary between the countless small unnamed objects that form Saturn's ring system and the larger objects that have been named as moons. Over 150 moonlets embedded in the rings have been detected by the disturbance they create in the surrounding ring material, though this is thought to be only a small sample of the total population of such objects.<ref name=Tiscareno2008/>

==Discovery==
===Early observations===
[[File:Iapetus-2010Mar04.jpg|thumb|Saturn ([[Exposure (photography)#Overexposure and underexposure|overexposed]]) and the moons Iapetus, Titan, Dione, Hyperion, and Rhea viewed through a 12.5-inch telescope|alt=A large bright circle in the center is surrounded by small circles.]]
Before the advent of [[astrophotography|telescopic photography]], eight moons of Saturn were discovered by direct observation using [[optical telescope]]s. Saturn's largest moon, [[Titan (moon)|Titan]], was discovered in 1655 by [[Christiaan Huygens]] using a {{convert|57|mm|in|1|adj=on|sp=us}} [[objective lens]]<ref name="ap050325" /> on a [[refracting telescope]] of his own design.<ref name="Baalke" /> [[Tethys (moon)|Tethys]], [[Dione (moon)|Dione]], [[Rhea (moon)|Rhea]] and [[Iapetus (moon)|Iapetus]] (the "[[Sidera Lodoicea]]") were discovered between 1671 and 1684 by [[Giovanni Domenico Cassini]].<ref name=Helden1994/> [[Mimas]] and [[Enceladus]] were discovered in 1789 by [[William Herschel]].<ref name=Helden1994/> [[Hyperion (moon)|Hyperion]] was discovered in 1848 by [[William Cranch Bond|W. C. Bond]], [[George Phillips Bond|G. P. Bond]]<ref name=Bond1848/> and [[William Lassell]].<ref name=Lassell1848/>

The use of [[long exposure photography|long-exposure]] photographic plates made possible the discovery of additional moons. The first to be discovered in this manner, [[Phoebe (moon)|Phoebe]], was found in 1899 by [[William Henry Pickering|W. H. Pickering]].<ref name=Pickering1899/> In 1966 the tenth satellite of Saturn was discovered by [[Audouin Dollfus]], when the rings were observed edge-on near an [[equinox]].<ref name=Fountain1977/> It was later named [[Janus (moon)|Janus]]. A few years later it was realized that all observations of 1966 could only be explained if another satellite had been present and that it had an orbit similar to that of Janus.<ref name=Fountain1977/> This object is now known as [[Epimetheus (moon)|Epimetheus]], the eleventh moon of Saturn. It shares the same orbit with Janus—the only known example of [[co-orbital moon|co-orbitals]] in the Solar System.<ref name=Uralskaya1998/> In 1980, three additional Saturnian moons were discovered from the ground and later confirmed by the ''[[Voyager program|Voyager]]'' probes. They are [[trojan moon]]s of Dione ([[Helene (moon)|Helene]]) and Tethys ([[Telesto (moon)|Telesto]] and [[Calypso (moon)|Calypso]]).<ref name=Uralskaya1998/>

===Observations by spacecraft===
[[File:PIA12797-Saturn&FiveMoons-20110729-FullColor-20180730.jpg|thumb|Five moons in a Cassini image: Rhea bisected in the far-right foreground, Mimas behind it, bright Enceladus above and beyond the rings, Pandora eclipsed by the F Ring, and Janus off to the left]]

The study of the outer planets has since been revolutionized by the use of uncrewed space probes. The arrival of the ''[[Voyager program|Voyager]]'' spacecraft at Saturn in 1980–1981 resulted in the discovery of three additional moons—[[Atlas (moon)|Atlas]], [[Prometheus (moon)|Prometheus]] and [[Pandora (moon)|Pandora]]—bringing the total to 17.<ref name=Uralskaya1998/> In addition, Epimetheus was confirmed as distinct from Janus. In 1990, [[Pan (moon)|Pan]] was discovered in archival ''Voyager'' images.<ref name=Uralskaya1998/>

The ''[[Cassini–Huygens|Cassini]]'' mission,<ref name="NYT-20151218-jc">{{cite news |last=Corum |first=Jonathan |title=Mapping Saturn's Moons |url=https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html |date=December 18, 2015 |work=[[The New York Times]] |access-date=December 18, 2015 |archive-date=May 20, 2020 |archive-url=https://web.archive.org/web/20200520124847/https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html |url-status=live}}</ref> which arrived at Saturn in July 2004, initially discovered three small inner moons: [[Methone (moon)|Methone]] and [[Pallene (moon)|Pallene]] between Mimas and Enceladus, and the second trojan moon of Dione, [[Polydeuces (moon)|Polydeuces]]. It also observed three suspected but unconfirmed moons in the [[F Ring]].<ref name=Porco2005/> In {{Nowrap|November 2004}} Cassini scientists announced that the structure of [[Saturn's rings]] indicates the presence of several more moons orbiting within the rings, although only one, [[Daphnis (moon)|Daphnis]], had been visually confirmed at the time.<ref name=Britt2004/> In 2007 [[Anthe (moon)|Anthe]] was announced.<ref name=IAUC2007/> In 2008 it was reported that ''Cassini'' observations of a depletion of energetic electrons in Saturn's [[magnetosphere]] near [[Rhea (moon)|Rhea]] might be the signature of a [[Rings of Rhea|tenuous ring system]] around Saturn's second largest moon.<ref name=Jones2008/> In {{Nowrap|March 2009}}, [[Aegaeon (moon)|Aegaeon]], a moonlet within the G Ring, was announced.<ref name="IAUC2009" /> In July of the same year, [[S/2009 S 1]], the first moonlet within the B Ring, was observed.<ref name="IAUC2009b" /> In April 2014, the possible beginning of a new [[Natural satellite|moon]], within the [[Rings of Saturn#A Ring|A Ring]], was reported.<ref name="NASA-20140414a">{{cite web |last1=Platt |first1=Jane |last2=Brown |first2=Dwayne |title=NASA Cassini Images May Reveal Birth of a Saturn Moon |url=http://www.jpl.nasa.gov/news/news.php?release=2014-112 |date=14 April 2014 |work=[[NASA]] |access-date=14 April 2014 |archive-date=10 April 2019 |archive-url=https://web.archive.org/web/20190410120305/https://www.jpl.nasa.gov/news/news.php?release=2014-112 |url-status=live}}</ref> ([[:File:PIA18078-PossibleBeginning-NewMoonOfPlanetSaturn-20130415.jpg|related image]])

===Outer moons===
[[File:2019 S 1 shift-and-add demonstration.png|thumb|This image demonstrates the application of the [[shift-and-add]] technique to the detection of a faint moon of Saturn ([[S/2019 S 1]]; circled in red). While the moon is barely visible in an individual image (top panel), it can be seen better when many images of the moon are taken, stacked to the moon's motion and then added together (bottom panel)]]
Study of Saturn's moons has also been aided by advances in telescope instrumentation, primarily the introduction of digital [[charge-coupled device]]s which replaced photographic plates. For the 20th century, Phoebe stood alone among Saturn's known moons with its highly irregular orbit. Then in 2000, a team of astronomers led by [[Brett J. Gladman]] discovered twelve irregular moons of Saturn using various ground-based telescopes around the world.<ref name=Gladman2001/><ref name=Jewitt2007/> The discovery of these irregular moons revealed orbital groupings within Saturn's irregular moon population, which provided the first insights into the collisional history of Saturn's irregular moons.<ref name=Jewitt2007/>

In 2003, a team of astronomers including [[Scott Sheppard]], [[David C. Jewitt]], and [[Jan Kleyna]] began using the [[Subaru Telescope|Subaru 8.2&nbsp;m telescope]] at [[Mauna Kea Observatory]] to search for irregular moons around Saturn, and discovered [[Narvi (moon)|Narvi]].<ref name=Jewitt2007/> Because of the Subaru telescope's very large aperture size alongside its camera's large field of view, it is capable of detecting extremely faint moons, hence Sheppard's team continued using the Subaru telescope for further moon searches.<ref name=Jewitt2007/> In 2005, Sheppard's team announced the discovery of twelve more small outer moons from their Subaru observations.<ref name=Jewitt2005/><ref name=Lakdawalla2005/> Sheppard's team announced nine more irregular moons in 2006<ref name=IAUC8727/> and three more moons in 2007, when [[Tarqeq]] was announced in {{Nowrap|April 2007}}, followed by [[S/2007 S 2]] and [[S/2007 S 3]] the following month.<ref name=IAUC8836/>

No new irregular moons of Saturn were reported until 2019, when Sheppard's team identified twenty more irregular satellites of Saturn in archives of their 2004–2007 Subaru observations. This brought Saturn's moon count to 82, which resulted in Saturn overtaking Jupiter as the planet with the most known moons for the first time since 2000.<ref name="Carnegie2019">{{cite web|title=Saturn Surpasses Jupiter After The Discovery Of 20 New Moons And You Can Help Name Them!|url=https://carnegiescience.edu/news/saturn-surpasses-jupiter-after-discovery-20-new-moons-and-you-can-help-name-them|publisher=Carnegie Science|date=7 October 2019|access-date=7 October 2019|archive-date=6 June 2020|archive-url=https://web.archive.org/web/20200606203854/https://carnegiescience.edu/news/saturn-surpasses-jupiter-after-discovery-20-new-moons-and-you-can-help-name-them|url-status=live}}</ref><ref name="SheppardMoons" /> In 2019, researchers Edward Ashton, Brett Gladman, and Matthew Beaudoin conducted a survey of Saturn's Hill sphere using the 3.6-meter [[Canada–France–Hawaii Telescope]] (CFHT) and discovered about 80 new Saturnian irregular moons, which were reported to the [[Minor Planet Center]] (MPC) for announcement.<ref name="Ashton2021"/><ref name="Ashton2022"/> Follow-up observations of these new moons took place over 2019–2021, eventually leading to [[S/2019 S 1]] being announced in November 2021 and an additional 62 moons being announced from 3–16 May 2023.<ref name="UBC-20230511"/><ref name="MPEC-2023-K118"/> These discoveries brought Saturn's total number of confirmed moons up to 145, making it the first planet known to have over 100 moons.<ref name="UBC-20230511"/><ref name="NYT-20230512">{{cite news |last=O'Callaghan |first=Jonathan |title=With 62 Newly Discovered Moons, Saturn Knocks Jupiter Off Its Pedestal - If all the objects are recognized by scientific authorities, the ringed giant world will have 145 moons in its orbit. |url=https://www.nytimes.com/2023/05/12/science/saturn-moons-jupiter.html |date=12 May 2023 |work=[[The New York Times]] |url-status=live |archiveurl=https://archive.today/20230512174454/https://www.nytimes.com/2023/05/12/science/saturn-moons-jupiter.html |archivedate=12 May 2023 |accessdate=13 May 2023}}</ref> Yet another moon, [[S/2006 S 20]], was announced on 23 May 2023, bringing Saturn's total count moons to 146.<ref name="MPEC-2023-K118"/> On 11 March 2025, 128 moons of Saturn were simultaneously announced by the MPC,<ref name="MPEC-2025-E155" /> bringing the total number of confirmed moons to 274.<ref name="Ashton2025b" /><ref name="UBC2025">{{Cite news |date=11 March 2025 |title=2025 Discovery of more Saturnian Moons |url=https://phas.ubc.ca/2025-discovery-more-saturnian-moons |accessdate=12 March 2025 |work=The University of British Columbia |publisher=The University of British Columbia}}</ref><ref>{{Cite news |date=11 March 2025 |title=Saturn has 128 new moons – more than the rest of the planets combined |url=https://www.newscientist.com/article/2471071-saturn-has-128-new-moons-more-than-the-rest-of-the-planets-combined/ |accessdate=12 March 2025 |work=New Scientist |publisher=New Scientist}}</ref> These moons were found by Ashton, Gladman, Mike Alexandersen, and Jean-Marc Petit, using the CFHT in 2023, as a continuation of their survey.<ref name="Ashton2025b" /><ref name="UBC2025" /> Ashton's team also searched in CFHT images taken by a separate team consisting of Wesley Fraser, Samantha Lawler, and [[John Kavelaars]].<ref name="MPEC-2025-E155" /> Many of these moons were traced back to earlier observations from 2004 to 2021, which correspond to their discovery dates.<ref name="MPEC-2025-E155" />

All of these recently announced moons are small and faint, with diameters over {{cvt|3|km|mi|sigfig=1}} and [[apparent magnitude]]s of 25–27.<ref name="Ashton2021"/> These extremely dim moons could only be seen via the [[shift-and-add]] technique, where multiple long-exposure images are overlaid, shifted to follow the motion of Saturn in the sky, and then additively combined to bring out the signal of faint moons that follow Saturn in the sky.<ref name="Ashton2021"/> The researchers found that the Saturnian irregular moon population is more abundant at smaller sizes, suggesting that they are likely fragments from a collision that occurred a few hundred million years ago. The researchers extrapolated that the true population of Saturnian irregular moons larger than {{cvt|2.8|km|mi|sigfig=2}} in diameter amounts to {{val|150|30}}, which is approximately three times as many Jovian irregular moons down to the same size. If this size distribution applies to even smaller diameters, Saturn would therefore intrinsically have more irregular moons than Jupiter.<ref name="Ashton2021"/>

==Naming==
{{Main|Naming of moons}}
The modern names for Saturnian moons were suggested by [[John Herschel]] in 1847.<ref name=Helden1994/> He proposed to name them after mythological figures associated with the Roman god of agriculture and harvest, [[Saturn (mythology)|Saturn]] (equated to the Greek [[Cronus]]).<ref name=Helden1994/> In particular, the then known seven satellites were named after [[Titan (mythology)|Titans]], Titanesses and [[Giants (Greek mythology)|Giants]] – brothers and sisters of Cronus.<ref name=Pickering1899/> The idea was similar to [[Simon Marius]]' scheme for naming [[moons of Jupiter]] after [[:Category:Children of Zeus|children of Zeus]].<ref name=Helden>{{cite journal |last1=van Helden |first1=Albert |title=Naming the Satellites of Jupiter and Saturn |journal=The Newsletter of the Historical Astronomy Division of the American Astronomical Society |date=August 1994 |issue=32 |url=https://had.aas.org/sites/had.aas.org/files/HADN32.pdf |access-date=10 March 2023 |archive-date=7 December 2022 |archive-url=https://web.archive.org/web/20221207151902/https://had.aas.org/sites/had.aas.org/files/HADN32.pdf |url-status=live}}</ref>
<blockquote>As Saturn devoured his children, his family could not be assembled around him, so that the choice lay among his brothers and sisters, the Titans and Titanesses. The name ''Iapetus'' seemed indicated by the obscurity and remoteness of the exterior satellite, ''Titan'' by the superior size of the Huyghenian, while the three female appellations [''Rhea'', ''Dione'', and ''Tethys''] class together the three intermediate Cassinian satellites. The minute interior ones seemed appropriately characterized by a return to male appellations [''Enceladus'' and ''Mimas''] chosen from a younger and inferior (though still superhuman) brood. [''Results of the Astronomical Observations made ... at the Cape of Good Hope'', p.&nbsp;415]</blockquote>

In 1848, Lassell proposed that the eighth satellite of Saturn be named Hyperion after another Titan.<ref name=Lassell1848/><ref name=Helden/> When in the 20th century the names of Titans were exhausted, the moons were named after different characters of the [[Greco-Roman mythology]] or giants from other mythologies.<ref name=Gazetteer/> All the irregular moons (except Phoebe, discovered about a century before the others) are named after [[Inuit mythology|Inuit]], and [[Celtic mythology|Gallic]] gods, and after [[Norse mythology|Norse]] ice giants.<ref name=Grav2007/> The [[International Astronomical Union]]'s (IAU) Committee for Planetary System Nomenclature, which oversees the naming of Solar System moons, rules that Saturnian moons that are smaller than 3&nbsp;km in diameter ([[absolute magnitude#Small Solar System bodies (H)|absolute magnitude]] H<sub>V</sub>&nbsp;>&nbsp;16.5){{efn|If assuming an albedo of 0.04, H<sub>V</sub>&nbsp;{{=}}&nbsp;16.5 corresponds to a diameter of 3.3&nbsp;km. The formula for the calculation can be found in [[absolute magnitude#Small Solar System bodies (H)]].}} should only be named if it is of scientific interest.<ref name="IAU-rules">{{cite web|title=IAU Rules and Conventions|url=https://planetarynames.wr.usgs.gov/Page/Rules|work=Gazetteer of Planetary Nomenclature|publisher=USGS Astrogeology Science Center|accessdate=16 March 2025}}</ref>

Some [[asteroid]]s share [[name conflicts of solar system objects|the same names]] as moons of Saturn: [[55 Pandora]], [[106 Dione]], [[577 Rhea]], [[1809 Prometheus]], [[1810 Epimetheus]], and [[4450 Pan]]. In addition, three more asteroids would share the names of Saturnian moons until spelling differences were made permanent by the IAU: [[Calypso (moon)|Calypso]] and asteroid [[53 Kalypso]]; [[Helene (moon)|Helene]] and asteroid [[101 Helena]]; and [[Gunnlod (moon)|Gunnlod]] and asteroid [[657 Gunlöd]].

==Physical characteristics==
Saturn's satellite system is very lopsided: one moon, Titan, comprises more than 96% of the mass in orbit around the planet. The six other [[planemo]] ([[ellipsoid]]al) moons constitute roughly 4% of the mass. These seven moons are large enough to have collapsed into a relaxed, ellipsoidal shape, though only one or two, Titan and possibly<!--shape of Rhea consistent w HE, but not demonstrated to be in HE since it spun down--> [[Rhea (moon)|Rhea]], are currently in [[hydrostatic equilibrium]]. The remaining small moons, together with the rings, comprise only 0.04% of the orbiting mass.{{refn | group = lower-alpha | The mass of the rings is about 0.40 times the mass of Mimas, whereas the combined mass of Janus, Hyperion and Phoebe—the most massive of the remaining moons—is about one-third. The total mass of the rings and small moons is around {{val|5.5|e=19|u=kg}}.}}

{{image frame
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 {"value":0.04, "label": "Mimas $d"},
 {"value":0.11, "label": "Enceladus $d"},
 {"value":0.62, "label": "Tethys $d"},
 {"value":1.1, "label": "Dione $d"},
 {"value":2.3, "label": "Rhea $d"},
 {"value":134.5, "label": "Titan $d"},
 {"value":1.8, "label": "Iapetus $d"},
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{{Pie chart
|1= [ 
 {"value":0.04, "label": "Mimas $d"},
 {"value":0.11, "label": "Enceladus $d"},
 {"value":0.62, "label": "Tethys $d"},
 {"value":1.1, "label": "Dione $d"},
 {"value":2.3, "label": "Rhea $d"},
 {"value":0, "label": "[Titan omitted] $d"},
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|caption=The relative masses of Saturn's moons. Values are ×10<sup>21</sup>&nbsp;kg. With Titan in the comparison (left), Mimas and Enceladus are invisible at this scale. Even excluding Titan (right), Phoebe, Hyperion, the smaller moons and the rings are invisible.
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{| class="wikitable sortable" style="clear:left;text-align:center;"
|+ Saturn's major satellites, compared with the [[Moon]]
|-
! Name<br>
! data-sort-type="number" | Diameter<br>(km)<ref name="Thomas2010" />
! data-sort-type="number" | Mass<br>(kg)<ref name="Jacobson Antreasian et al. 2006" />
! data-sort-type="number" | Orbital radius<br>(km)<ref name=NASA/>
! data-sort-type="number" | Orbital period<br>(days)<ref name=NASA/>
|-
| '''[[Mimas]]''' || 396<br>(0.12&nbsp;''D''<sub>☾</sub>) ||data-sort-value=4.0E19| 4×10<sup>19</sup><br>(0.0005&nbsp;''M''<sub>☾</sub>) || 185,539<br>(0.48&nbsp;''a''<sub>☾</sub>) || 0.9<br>(0.03&nbsp;''T''<sub>☾</sub>)
|-
| '''[[Enceladus]]''' || 504<br>(0.14&nbsp;''D''<sub>☾</sub>) ||data-sort-value=1.1E20| 1.1×10<sup>20</sup><br>(0.002&nbsp;''M''<sub>☾</sub>) || 237,948<br>(0.62&nbsp;''a''<sub>☾</sub>) || 1.4<br>(0.05&nbsp;''T''<sub>☾</sub>)
|-
| '''[[Tethys (moon)|Tethys]]''' || 1,062<br>(0.30&nbsp;''D''<sub>☾</sub>) ||data-sort-value=6.2E20| 6.2×10<sup>20</sup><br>(0.008&nbsp;''M''<sub>☾</sub>) || 294,619<br>(0.77&nbsp;''a''<sub>☾</sub>) || 1.9<br>(0.07&nbsp;''T''<sub>☾</sub>)
|-
| '''[[Dione (moon)|Dione]]''' || 1,123<br>(0.32&nbsp;''D''<sub>☾</sub>) ||data-sort-value=1.1E21| 1.1×10<sup>21</sup><br>(0.015&nbsp;''M''<sub>☾</sub>) || 377,396<br>(0.98&nbsp;''a''<sub>☾</sub>) || 2.7<br>(0.10&nbsp;''T''<sub>☾</sub>)
|-
| '''[[Rhea (moon)|Rhea]]''' || 1,527<br>(0.44&nbsp;''D''<sub>☾</sub>) ||data-sort-value=2.3E21| 2.3×10<sup>21</sup><br>(0.03&nbsp;''M''<sub>☾</sub>) || 527,108<br>(1.37&nbsp;''a''<sub>☾</sub>) || 4.5<br>(0.20&nbsp;''T''<sub>☾</sub>)
|-
| '''[[Titan (moon)|Titan]]''' || 5,149<br>(1.48&nbsp;''D''<sub>☾</sub>)<br>(0.75&nbsp;''D''<sub>[[Mars|♂]]</sub>) ||data-sort-value=1.35E23| 1.35×10<sup>23</sup><br>(1.80&nbsp;''M''<sub>☾</sub>)<br>(0.21&nbsp;''M''<sub>[[Mars|♂]]</sub>) || 1,221,870<br>(3.18&nbsp;''a''<sub>☾</sub>) || 16<br>(0.60&nbsp;''T''<sub>☾</sub>)
|-
| '''[[Iapetus (moon)|Iapetus]]''' || 1,470<br>(0.42&nbsp;''D''<sub>☾</sub>) ||data-sort-value=1.8E21| 1.8×10<sup>21</sup><br>(0.025&nbsp;''M''<sub>☾</sub>) || 3,560,820<br>(9.26&nbsp;''a''<sub>☾</sub>) || 79<br>(2.90&nbsp;''T''<sub>☾</sub>)
|}

==Orbital groups==
[[File:Saturn's Rings PIA03550.jpg|thumb|upright=2.0|Artist conception of Saturn, its rings and major icy moons—from Mimas to Rhea]]
Although the boundaries may be somewhat vague, Saturn's moons can be divided into nine groups according to their orbital characteristics. Many of them, such as [[Pan (moon)|Pan]] and [[Daphnis (moon)|Daphnis]], orbit within Saturn's ring system and have orbital periods only slightly longer than the planet's rotation period.<ref name="Porco2007" /> The innermost moons and most regular satellites all have mean [[orbital inclination]]s ranging from less than a degree to about 1.5 degrees (except [[Iapetus (moon)|Iapetus]], which has an inclination of 7.57 degrees) and small [[orbital eccentricity|orbital eccentricities]].<ref name="SheppardMoons" /> On the other hand, irregular satellites in the outermost regions of Saturn's moon system, in particular the [[Norse group]], have orbital radii of millions of kilometers and orbital periods lasting several years. The moons of the Norse group also orbit in the opposite direction to Saturn's rotation.<ref name=Grav2007/>

===Inner moons===
====Ring moonlets====
{{multiple image |caption_align=center |align=right |width=200 |direction=vertical
|image1=PIA21056 - Daphnis Up Close.jpg
|caption1=Shepherd moon [[Daphnis (moon)|Daphnis]] creating waves in Saturn's [[Rings of Saturn#A Ring|A Ring]]
|image2=Aegaeon (2008 S1).jpg
|caption2=Sequence of ''Cassini'' images of [[Aegaeon (moon)|Aegaeon]] embedded within the bright arc of Saturn's [[Rings of Saturn#G Ring|G Ring]]}}
During late July 2009, a [[moonlet]], [[S/2009 S 1]], was discovered in the [[B Ring]], 480&nbsp;km from the outer edge of the ring, by the shadow it cast.<ref name="IAUC2009b" /> It is estimated to be 300&nbsp;m in diameter. Unlike the [[A Ring]] moonlets (see below), it does not induce a 'propeller' feature, probably due to the density of the B Ring.<ref name=2009s1/>

In 2006, four tiny moonlets were found in ''Cassini'' images of the A Ring.<ref name="Tiscareno2006" /> Before this discovery only two larger moons had been known within gaps in the A Ring: Pan and Daphnis. These are large enough to clear continuous gaps in the ring.<ref name="Tiscareno2006" /> In contrast, a moonlet is only massive enough to clear two small—about 10&nbsp;km across—partial gaps in the immediate vicinity of the moonlet itself creating a structure shaped like an airplane [[propeller]].<ref name="Sremcevic2007" /> The moonlets themselves are tiny, ranging from about 40 to 500&nbsp;meters in diameter, and are too small to be seen directly.<ref name="Tiscareno2008" />

In 2007, the discovery of 150 more moonlets revealed that they (with the exception of two that have been seen outside the [[Encke gap]]) are confined to three narrow bands in the A Ring between 126,750 and 132,000&nbsp;km from Saturn's center. Each band is about a thousand kilometers wide, which is less than 1% the width of Saturn's rings.<ref name="Tiscareno2008" /> This region is relatively free from the disturbances caused by resonances with larger satellites,<ref name="Tiscareno2008" /> although other areas of the A Ring without disturbances are apparently free of moonlets. The moonlets were probably formed from the breakup of a larger satellite.<ref name="Sremcevic2007" /> It is estimated that the A Ring contains 7,000–8,000 propellers larger than 0.8&nbsp;km in size and millions larger than 0.25&nbsp;km.<ref name="Tiscareno2008" /> In April 2014, [[NASA]] scientists reported the possible consolidation of a new moon within the A Ring, implying that Saturn's present moons may have formed in a similar process in the past when Saturn's ring system was much more massive.<ref name="NASA-20140414a"/>

Similar moonlets may reside in the [[F Ring]].<ref name="Tiscareno2008" /> There, "jets" of material may be due to collisions, initiated by perturbations from the nearby small moon Prometheus, of these moonlets with the core of the F Ring. One of the largest F Ring moonlets may be the as-yet unconfirmed object [[S/2004 S 6]]. The F Ring also contains transient "fans" which are thought to result from even smaller moonlets, about 1&nbsp;km in diameter, orbiting near the F Ring core.<ref name=Murray2008/>

One recently discovered moon, [[Aegaeon (moon)|Aegaeon]], resides within the bright arc of [[Rings of Saturn#G Ring|G Ring]] and is trapped in the 7:6 mean-motion [[orbital resonance|resonance]] with Mimas.<ref name=IAUC2009/> This means that it makes exactly seven revolutions around Saturn while Mimas makes exactly six. The moon is the largest among the population of bodies that are sources of dust in this ring.<ref name=Hedman2007/>

====Ring shepherds====
[[File:PIA12684 F Ring.png|thumb|right|Shepherd moon Prometheus disturbing Saturn's [[Rings of Saturn|F Ring]]]]
[[Shepherd moon|Shepherd satellites]] are small moons that orbit within, or just beyond, a planet's [[ring system]]. They have the effect of sculpting the rings: giving them sharp edges, and creating gaps between them. Saturn's shepherd moons are [[Pan (moon)|Pan]] ([[Rings of Saturn#Encke Gap|Encke gap]]), [[Daphnis (moon)|Daphnis]] ([[Keeler gap]]), [[Prometheus (moon)|Prometheus]] (F Ring), [[Janus (moon)|Janus]] (A Ring), and [[Epimetheus (moon)|Epimetheus]] (A Ring).<ref name=Porco2005/><ref name=IAUC2009/> [[Atlas (moon)|Atlas]] and [[Pandora (moon)|Pandora]] orbit on the outside edge of the A Ring and F Ring respectively, and were long thought to be shepherds as well, until more recent studies began to indicate otherwise. These moons likely formed as a result of accretion of the friable ring material on preexisting denser cores. The cores with sizes from one-third to one-half the present-day moons may be themselves collisional shards formed when a parental satellite of the rings disintegrated.<ref name="Porco2007" />

Janus and Epimetheus are [[co-orbital moon]]s.<ref name="Uralskaya1998" /> They are of similar size, with Janus being somewhat larger than Epimetheus.<ref name="Porco2007" /> They have orbits with less than a 100-kilometer difference in [[semi-major axis]], close enough that they would collide if they attempted to pass each other. Instead of colliding, their gravitational interaction causes them to swap orbits every four years.<ref name="Spitale Jacobson et al. 2006" />{{clear|left}}

===Inner large===
{{multiple image
| header            = Saturn's inner large moons
| caption_align     = center
| align             = right
| direction         = vertical
| image1            = Fountains of Enceladus PIA07758.jpg
| caption1          = Enceladus ejecting icy particles from its south polar plumes
| image2            = PIA18355-SaturnMoon-Tethys-20151123.jpg
| caption2          = Tethys and the rings of Saturn
| image3            = Dione and Saturn.jpg
| caption3          = Color view of Dione in front of Saturn
}}

The innermost large moons of Saturn orbit within its tenuous [[Rings of Saturn#E Ring|E Ring]], along with three smaller moons of the Alkyonides group.
*[[Mimas]] is the smallest and least massive of the inner round moons,<ref name="Jacobson Antreasian et al. 2006" /> although its mass is sufficient to alter the orbit of [[Methone (moon)|Methone]].<ref name="Spitale Jacobson et al. 2006" /> It is noticeably ovoid-shaped, having been made shorter at the poles and longer at the equator (by about 20&nbsp;km) by the effects of Saturn's gravity.<ref name=Thomas2007/> Mimas has a large [[impact crater]] one-third its diameter, [[Herschel (Mimantean crater)|Herschel]], situated on its leading hemisphere<ref name="Moore Schenk et al. 2004" /> Mimas has no known past or present geologic activity and its surface is dominated by impact craters, though it does have a water ocean 20–30&nbsp;km beneath the surface.<ref>{{Cite journal |last1=Lainey |first1=V |last2=Rambaux |first2=N |last3=Tobie |first3=G |last4=Cooper |first4=N |last5=Zhang |first5=Q |last6=Noyelles |first6=B |last7=Baillié |first7=K |date=2024-02-07 |title=A recently formed ocean inside Saturn's moon Mimas |url=https://www.nature.com/articles/s41586-023-06975-9.epdf?sharing_token=vYAG4f049M5kK2gX7OfZg9RgN0jAjWel9jnR3ZoTv0MN0ukW__TUAf43EkTwisrqQJAdNax6CY-KTbuDYP9edZjI9EdTKQHqBQ7K4elhr_eA7eCcg60b2Fa-ecxLjrdaHL789s2t1YlS3e4-7nwjkbYcddy-Gnh3L73x_IXMKpuk6IXunnHmMERXqVHjOrcX0QRIEEolq8Efgnu3Kz1-6vBxMaerFbOz8sldPmErHwqNcmCFFYGSE3pLfIeaGK87Lisfz_gHA_dN9cqMDnl_asFvF8X4cvtD9qTYp0xwrzzdoKkTp2J5UhquPn7vGF4R |journal=Nature |language=en |volume=626 |issue=7998 |pages=280–282 |doi=10.1038/s41586-023-06975-9 |pmid=38326592 |bibcode=2024Natur.626..280L |s2cid=267546453 |issn=1476-4687 |access-date=2024-02-07 |archive-date=2024-06-16 |archive-url=https://web.archive.org/web/20240616103720/https://www.nature.com/articles/s41586-023-06975-9.epdf?sharing_token=vYAG4f049M5kK2gX7OfZg9RgN0jAjWel9jnR3ZoTv0MN0ukW__TUAf43EkTwisrqQJAdNax6CY-KTbuDYP9edZjI9EdTKQHqBQ7K4elhr_eA7eCcg60b2Fa-ecxLjrdaHL789s2t1YlS3e4-7nwjkbYcddy-Gnh3L73x_IXMKpuk6IXunnHmMERXqVHjOrcX0QRIEEolq8Efgnu3Kz1-6vBxMaerFbOz8sldPmErHwqNcmCFFYGSE3pLfIeaGK87Lisfz_gHA_dN9cqMDnl_asFvF8X4cvtD9qTYp0xwrzzdoKkTp2J5UhquPn7vGF4R |url-status=live}}</ref> The only tectonic features known are a few arcuate and linear [[trough (geology)|troughs]], which probably formed when Mimas was shattered by the Herschel impact.<ref name="Moore Schenk et al. 2004" /> 
*[[Enceladus]] is one of the smallest of Saturn's moons that is spherical in shape—only Mimas is smaller<ref name=Thomas2007/>—yet is the only small Saturnian moon that is currently endogenously active, and the smallest known body in the Solar System that is geologically active today.<ref name="Porco Helfenstein et al. 2006" /> Its surface is morphologically diverse; it includes ancient heavily cratered terrain as well as younger smooth areas with few impact craters. Many plains on Enceladus are fractured and intersected by systems of [[lineament]]s.<ref name="Porco Helfenstein et al. 2006" /> The area around its south pole was found by ''Cassini'' to be unusually warm and cut by a system of fractures about 130&nbsp;km long called "tiger stripes", some of which emit [[Jet (fluid)|jets]] of [[water vapor]] and [[dust]].<ref name="Porco Helfenstein et al. 2006" /> These jets form a large [[Plume (fluid dynamics)|plume]] off its south pole, which replenishes Saturn's E ring<ref name="Porco Helfenstein et al. 2006" /> and serves as the main source of [[ion]]s in the [[magnetosphere of Saturn]].<ref name=Pontius2006/> The gas and dust are released with a rate of more than 100&nbsp;kg/s. Enceladus may have liquid water underneath the south-polar surface.<ref name="Porco Helfenstein et al. 2006" /> The source of the energy for this [[cryovolcanism]] is thought to be a 2:1 [[orbital resonance|mean-motion resonance]] with Dione.<ref name="Porco Helfenstein et al. 2006" /> The pure ice on the surface makes Enceladus one of the brightest known objects in the Solar System—its [[geometrical albedo]] is more than 140%.<ref name="Porco Helfenstein et al. 2006" />
*[[Tethys (moon)|Tethys]] is the third largest of Saturn's inner moons.<ref name="Jacobson Antreasian et al. 2006" /> Its most prominent features are a large (400&nbsp;km diameter) impact crater named [[Odysseus (crater)|Odysseus]] on its leading hemisphere and a vast canyon system named [[Ithaca Chasma]] extending at least 270° around Tethys.<ref name="Moore Schenk et al. 2004" /> The Ithaca Chasma is concentric with Odysseus, and these two features may be related. Tethys appears to have no current geological activity. A heavily cratered hilly terrain occupies the majority of its surface, while a smaller and smoother plains region lies on the hemisphere opposite to that of Odysseus.<ref name="Moore Schenk et al. 2004" /> The plains contain fewer craters and are apparently younger. A sharp boundary separates them from the cratered terrain. There is also a system of extensional troughs radiating away from Odysseus.<ref name="Moore Schenk et al. 2004" /> The density of Tethys (0.985&nbsp;g/cm<sup>3</sup>) is less than that of water, indicating that it is made mainly of water ice with only a small fraction of [[rock (geology)|rock]].<ref name="Thomas2010" />
* [[Dione (moon)|Dione]] is the second-largest inner moon of Saturn. It has a higher density than the geologically dead Rhea, the largest inner moon, but lower than that of active Enceladus.<ref name=Thomas2007/> While the majority of Dione's surface is heavily cratered old terrain, this moon is also covered with an extensive network of troughs and lineaments, indicating that in the past it had global [[tectonic]] activity.<ref name=Wagner2009/> The troughs and lineaments are especially prominent on the trailing hemisphere, where several intersecting sets of fractures form what is called "wispy terrain".<ref name=Wagner2009/> The cratered plains have a few large impact craters reaching 250&nbsp;km in diameter.<ref name="Moore Schenk et al. 2004" /> Smooth plains with low impact-crater counts are also present on a small fraction of its surface.<ref name=Schenk2009b/> They were probably tectonically resurfaced relatively later in the geological history of Dione. At two locations within smooth plains strange landforms (depressions) resembling oblong impact craters have been identified, both of which lie at the centers of radiating networks of cracks and troughs;<ref name=Schenk2009b/> these features may be cryovolcanic in origin. Dione may be geologically active even now, although on a scale much smaller than the cryovolcanism of Enceladus. This follows from Cassini magnetic measurements that show Dione is a net source of plasma in the magnetosphere of Saturn, much like Enceladus.<ref name=Schenk2009b/>

{{anchor|The Alkyonides}}

===Alkyonides===
Three small moons orbit between Mimas and Enceladus: [[Methone (moon)|Methone]], [[Anthe (moon)|Anthe]], and [[Pallene (moon)|Pallene]]. Named after the [[Alkyonides]] of Greek mythology, they are some of the smallest moons in the Saturn system. Anthe and Methone have very faint ring arcs along their orbits, whereas Pallene has a faint complete ring.<ref name=Alkyonides/> Of these three moons, only Methone has been photographed at close range, showing it to be egg-shaped with very few or no craters.<ref>{{cite web |last1=Lakdawalla |first1=Emily |author-link1=Emily Lakdawalla |title=Methone, an egg in Saturn orbit? |url=http://www.planetary.org/blogs/emily-lakdawalla/2012/05211206.html |website=Planetary Society |access-date=27 April 2019 |archive-date=27 April 2019 |archive-url=https://web.archive.org/web/20190427233242/http://www.planetary.org/blogs/emily-lakdawalla/2012/05211206.html |url-status=live}}</ref>

===Trojan moons===
{{Main|Trojan moon}}

Trojan moons are a unique feature only known from the Saturnian system. A trojan body orbits at either the leading L<sub>4</sub> or trailing L<sub>5</sub> [[Lagrange point]] of a much larger object, such as a large moon or planet. Tethys has two trojan moons, [[Telesto (moon)|Telesto]] (leading) and [[Calypso (moon)|Calypso]] (trailing), and Dione also has two, [[Helene (moon)|Helene]] (leading) and [[Polydeuces (moon)|Polydeuces]] (trailing).<ref name=Porco2005/> Helene is by far the largest trojan moon,<ref name=Thomas2007/> while Polydeuces is the smallest and has the most [[chaos (physics)|chaotic]] orbit.<ref name="Spitale Jacobson et al. 2006" /> These moons are coated with dusty material that has smoothed out their surfaces.<ref>{{Cite web|url=https://www.planetary.org/articles/2078|title=Cassini goodies: Telesto, Janus, Prometheus, Pandora, F ring|website=The Planetary Society}}</ref>

===Outer large===
{{multiple image
| header            = Saturn's outer large moons
| caption_align     = center
| align             = right
| width             = 
| direction         = vertical
| image1            = PIA08148 (Rhea-Splat).jpg
| caption1          = [[Inktomi (crater)|Inktomi]] or "The Splat", a relatively young crater with prominent butterfly-shaped [[ejecta blanket|ejecta]] on Rhea's leading hemisphere
| alt1              = A spherical body is almost fully illuminated. Its grayish surface is covered by numerous circular craters. The terminator is located near the upper-right limb. A large crater can be seen near the limb in the upper-left part of the body. Another smaller bright crater can be seen in the center. It is surrounded by a large bright patch having the shape of a five-pointed star.
| image2            = Ringside with Titan and Dione.jpg
| caption2          = Titan in front of Dione and the rings of Saturn
| image3            = PIA17193-SaturnMoon-Hyperion-20150531.jpg
| caption3          = ''Cassini'' image of [[Hyperion (moon)|Hyperion]]
| alt3              = An irregularly-shaped and heavily cratered body, pock-marked with dark pits and ridges on its tan-colored icy surface.
| image4            = Iapetus equatorial ridge.jpg
| caption4          = Equatorial ridge on [[Iapetus (moon)|Iapetus]]
| alt4              = A part of a spherical body illuminated from the above and behind. The convex limb runs from the lower-left to the upper-right corner. The black outer space is in the upper-left corner. The terminator is near the bottom. The surface of the body is covered with numerous craters. A large ridge runs in the center from the top to bottom.
}}

These moons all orbit beyond the E Ring. They are:
*[[Rhea (moon)|Rhea]] is the second-largest of Saturn's moons. It is even slightly larger than [[Oberon (moon)|Oberon]], the second-largest moon of [[Uranus (planet)|Uranus]].<ref name=Thomas2007/> In 2005, ''Cassini'' detected a depletion of electrons in the plasma wake of Rhea, which forms when the co-rotating plasma of [[Magnetosphere of Saturn|Saturn's magnetosphere]] is absorbed by the moon.<ref name=Jones2008/> The depletion was hypothesized to be caused by the presence of dust-sized particles concentrated in a few [[Rings of Rhea|faint equatorial rings]].<ref name=Jones2008/> Such a ring system would make Rhea the only moon in the Solar System known to have rings.<ref name=Jones2008/> Subsequent targeted observations of the putative ring plane from several angles by ''Cassini'''s [[Cassini–Huygens#Instruments|narrow-angle camera]] turned up no evidence of the expected ring material, leaving the origin of the plasma observations unresolved.<ref name="Tiscareno2010">{{Cite journal |last1=Tiscareno |first1=Matthew S. |last2=Burns |first2=Joseph A. |last3=Cuzzi |first3=Jeffrey N. |last4=Hedman |first4=Matthew M. |date=July 2010 |title=Cassini imaging search rules out rings around Rhea |journal=Geophysical Research Letters |language=en |volume=37 |issue=14 |pages=L14205 |arxiv=1008.1764 |bibcode=2010GeoRL..3714205T |doi=10.1029/2010GL043663 |issn=0094-8276 |s2cid=59458559}}</ref>
: Otherwise Rhea has rather a typical heavily cratered surface,<ref name="Moore Schenk et al. 2004" /> with the exceptions of a few large Dione-type fractures (wispy terrain) on the trailing hemisphere<ref name=Wagner2008/> and a very faint "line" of material at the equator that may have been deposited by material deorbiting from present or former rings.<ref name=Schenk2009/> Rhea also has two very large impact basins on its anti-Saturnian hemisphere, which are about 400 and 500&nbsp;km across.<ref name=Wagner2008/> The first, [[Tirawa (crater)|Tirawa]], is roughly comparable to the Odysseus basin on Tethys.<ref name="Moore Schenk et al. 2004" /> There is also a 48&nbsp;km-diameter impact crater called [[Inktomi (crater)|Inktomi]]<ref name=Inktomi/> at 112°W that is prominent because of an extended system of bright [[ray system|rays]],<ref name=Splat/> which may be one of the youngest craters on the inner moons of Saturn.<ref name=Wagner2008/> No evidence of any endogenic activity has been discovered on the surface of Rhea.<ref name=Wagner2008/>
*[[Titan (moon)|Titan]], at 5,149&nbsp;km diameter, is the second largest moon in the Solar System and Saturn's largest.<ref name="Zebker 2009" /><ref name="Jacobson Antreasian et al. 2006" /> Out of all the large moons, Titan is the only one with a dense (surface pressure of 1.5&nbsp;[[Atmosphere (unit)|atm]]), cold atmosphere, primarily made of [[nitrogen]] with a small fraction of [[methane]].<ref name=Porco2005c/> The dense atmosphere frequently produces bright white [[Cumulus cloud|convective clouds]], especially over the south pole region.<ref name=Porco2005c/> On 6 June 2013, scientists at the [[Instituto de Astrofísica de Andalucía|IAA-CSIC]] reported the detection of [[polycyclic aromatic hydrocarbons]] in the [[upper atmosphere]] of Titan.<ref name="IAA-20130606">{{cite news |last=López-Puertas |first=Manuel |url=http://www.iaa.es/content/pahs-titans-upper-atmosphere |title=PAH's in Titan's Upper Atmosphere |date=6 June 2013 |work=[[Spanish National Research Council|CSIC]] |access-date=6 June 2013 |archive-date=22 August 2016 |archive-url=https://web.archive.org/web/20160822010505/http://www.iaa.es/content/pahs-titans-upper-atmosphere |url-status=dead}}</ref> On 23 June 2014, NASA claimed to have strong evidence that [[nitrogen]] in the [[atmosphere of Titan]] came from materials in the [[Oort cloud]], associated with [[comets]], and not from the materials that formed Saturn in earlier times.<ref name="NASA-201450623">{{cite press release |last1=Dyches |first1=Preston |last2=Clavin |first2=Whitney |title=Titan's Building Blocks Might Pre-date Saturn |url=http://www.jpl.nasa.gov/news/news.php?release=2014-200 |date=23 June 2014 |publisher=[[Jet Propulsion Laboratory]] |access-date=28 June 2014 |archive-date=9 September 2018 |archive-url=https://web.archive.org/web/20180909162240/https://www.jpl.nasa.gov/news/news.php?release=2014-200 |url-status=live}}</ref>

: The surface of Titan, which is difficult to observe due to persistent atmospheric [[haze]], shows only a few impact craters and is probably very young.<ref name=Porco2005c/> It contains a pattern of light and dark regions, flow channels and possibly cryovolcanos.<ref name=Porco2005c/><ref name=Lopes2007/> Some dark regions are covered by [[Dune#Longitudinal (Seif) and transverse dunes|longitudinal dune]] fields shaped by tidal winds, where sand is made of frozen water or hydrocarbons.<ref name=Lorenz2006/> Titan is the only body in the Solar System beside Earth with bodies of liquid on its surface, in the form of [[Lakes of Titan|methane–ethane lakes]] in Titan's north and south polar regions.<ref name=Stofan2007/> The largest lake, [[Kraken Mare]], is larger than the [[Caspian Sea]].<ref name=KrakenMare/> Like Europa and Ganymede, it is believed that Titan has a subsurface ocean made of water mixed with [[ammonia]], which can erupt to the surface of the moon and lead to cryovolcanism.<ref name=Lopes2007/> On 2 July 2014, NASA reported the ocean inside Titan may be "as salty as the Earth's [[Dead Sea]]".<ref name="NASA-20140702">{{cite web |last1=Dyches |first1=Preston |last2=Brown |first2=Dwayne |title=Ocean on Saturn Moon Could be as Salty as the Dead Sea |url=http://www.jpl.nasa.gov/news/news.php?release=2014-217 |date=2 July 2014 |work=[[NASA]] |access-date=July 2, 2014 |archive-date=9 July 2014 |archive-url=https://web.archive.org/web/20140709165628/http://www.jpl.nasa.gov/news/news.php?release=2014-217 |url-status=live}}</ref><ref name="ICARUS-2014">{{cite journal |last1=Mitri |first1=Giuseppe |last2=Meriggiola |first2=Rachele |last3=Hayes |first3=Alex |last4=Lefevre |first4=Axel |last5=Tobie | first5=Gabriel |last6=Genova |first6=Antonio |last7=Lunine |first7=Jonathan I. |last8=Zebker |first8=Howard |title=Shape, topography, gravity anomalies and tidal deformation of Titan |date=1 July 2014 |journal=[[Icarus (journal)|Icarus]] |doi=10.1016/j.icarus.2014.03.018 |volume=236 |pages=169–177 |bibcode = 2014Icar..236..169M}}</ref>
*[[Hyperion (moon)|Hyperion]] is Titan's nearest neighbor in the Saturn system. The two moons are locked in a 4:3 [[Orbital resonance|mean-motion resonance]] with each other, meaning that while Titan makes four revolutions around Saturn, Hyperion makes exactly three.<ref name="Jacobson Antreasian et al. 2006" /> With an average diameter of about 270&nbsp;km, Hyperion is smaller and lighter than Mimas.<ref name=Thomas2007b/> It has an extremely irregular shape, and a very odd, tan-colored icy surface resembling a sponge, though its interior may be partially porous as well.<ref name=Thomas2007b/> The average density of about 0.55&nbsp;g/cm<sup>3</sup><ref name=Thomas2007b/> indicates that the porosity exceeds 40% even assuming it has a purely icy composition. The surface of Hyperion is covered with numerous impact craters—those with diameters 2–10&nbsp;km are especially abundant.<ref name=Thomas2007b/> It is the only moon besides the small [[moons of Pluto]] known to have a chaotic rotation, which means Hyperion has no well-defined poles or equator. While on short timescales the satellite approximately rotates around its long axis at a rate of 72–75° per day, on longer timescales its axis of rotation (spin vector) wanders chaotically across the sky.<ref name=Thomas2007b/> This makes the rotational behavior of Hyperion essentially unpredictable.<ref name=Thomas1995/>
*[[Iapetus (moon)|Iapetus]] is the third-largest of Saturn's moons.<ref name=Thomas2007/> Orbiting the planet at {{Nowrap|3.5 million}} km, it is by far the most distant of Saturn's large moons, and also has the largest [[Inclination|orbital inclination]], at 15.47°.<ref name=NASA/> Iapetus has long been known for its unusual two-toned surface; its leading hemisphere is pitch-black and its trailing hemisphere is almost as bright as fresh snow.<ref name=Porco2005b/> ''Cassini'' images showed that the dark material is confined to a large near-equatorial area on the leading hemisphere called [[Cassini Regio]], which extends approximately from 40°N to 40°S.<ref name=Porco2005b/> The pole regions of Iapetus are as bright as its trailing hemisphere. ''Cassini'' also discovered a 20&nbsp;km tall equatorial ridge, which spans nearly the moon's entire equator.<ref name=Porco2005b/> Otherwise both dark and bright surfaces of Iapetus are old and heavily cratered. The images revealed at least four large impact basins with diameters from 380 to 550&nbsp;km and numerous smaller impact craters.<ref name=Porco2005b/> No evidence of any endogenic activity has been discovered.<ref name=Porco2005b/>

: A clue to the origin of the dark material covering part of Iapetus's starkly [[dichroism|dichromatic]] surface may have been found in 2009, when NASA's [[Spitzer Space Telescope]] discovered a vast, nearly invisible disk around Saturn, just inside the orbit of the moon Phoebe &ndash; the [[Phoebe ring]].<ref name=Verbiscer2009/> Scientists believe that the disk originates from dust and ice particles kicked up by impacts on Phoebe. Because the disk particles, like Phoebe itself, orbit in the opposite direction to Iapetus, Iapetus collides with them as they drift in the direction of Saturn, darkening its leading hemisphere slightly.<ref name=Verbiscer2009/> Once a difference in albedo, and hence in average temperature, was established between different regions of Iapetus, a [[thermal runaway]] process of water ice [[Sublimation (chemistry)|sublimation]] from warmer regions and [[Deposition (phase transition)|deposition]] of water vapor onto colder regions ensued. Iapetus's present two-toned appearance results from the contrast between the bright, primarily ice-coated areas and regions of dark lag, the residue left behind after the loss of surface ice.<ref name = "Denk">{{Cite journal
 | last = Denk | first = T. |display-authors=etal
 | title = Iapetus: Unique Surface Properties and a Global Color Dichotomy from Cassini Imaging
 | journal = [[Science (journal)|Science]] | volume = 327| issue =5964 | pages =435–9
 | date = 2009-12-10
 | doi = 10.1126/science.1177088
 | pmid = 20007863|bibcode = 2010Sci...327..435D | s2cid = 165865}}</ref><ref name = "Spencer">{{Cite journal
 | last = Spencer | first = J. R. |author2=Denk, T.
 | title = Formation of Iapetus' Extreme Albedo Dichotomy by Exogenically Triggered Thermal Ice Migration
 | journal = [[Science (journal)|Science]] | volume = 327| issue =5964 | pages =432–5
 | date = 2009-12-10 | doi = 10.1126/science.1177132 | pmid = 20007862|bibcode = 2010Sci...327..432S | citeseerx = 10.1.1.651.4218 | s2cid = 20663944}}</ref>

===Irregular===
[[File:Saturn irregular moon orbits top-side 2025.png|thumb|upright=1.25|Orbits and positions of Saturn's 250 irregular moons as of March 2025. Prograde orbits are colored blue while retrograde orbits are colored red. Saturn's outermost regular moons, Titan, Hyperion, and Iapetus, are also shown with turquoise orbits.]]

[[Irregular moon]]s are small satellites with distant, inclined, and frequently [[retrograde and direct motion|retrograde]] orbits, believed to have been acquired by the parent planet through a capture process. They often occur as [[collisional family|collisional families]] or groups.<ref name=Jewitt2007/> The precise size and albedo of many of the irregular moons are not known because they are too small to be resolved by telescopes on Earth and in space, so their sizes are estimated from their brightness by assuming a dark surface or low albedo of around 6% (albedo of Phoebe) or less.<ref name=Gladman2001/> The irregular moons generally have featureless visible and [[near infrared]] spectra dominated by water absorption bands.<ref name=Jewitt2007/> They are typically gray (spectrally neutral) or moderately red in color—similar to [[C-type asteroid|C-type]], [[P-type asteroid|P-type]], or [[D-type asteroid]]s,<ref name=Grav2007/> though they are much less red than [[Kuiper belt]] objects.<ref name=Jewitt2007/>{{refn | group = lower-alpha | The photometric color may be used as a proxy for the chemical composition of satellites' surfaces.}}

====Inuit====
{{Main|Inuit group}}

The Inuit group includes 36<!--for a count of 274--> [[prograde orbit|prograde]] outer moons that are similar enough in their distances from the planet (190–300 radii of Saturn), their orbital inclinations (43–51°) and their colors that they can be considered a group.<ref name=Gladman2001/><ref name=Grav2007/> The Inuit group is further split into three distinct subgroups at different semi-major axes, and are named after their respective largest members. Ordered by increasing semi-major axis, these subgroups are the [[Kiviuq (moon)|Kiviuq]] subgroup (188 Saturn radii), [[Paaliaq]] (249 Saturn radii), and the [[Siarnaq]] subgroup (297 Saturn radii).<ref name="Sheppard2023"/><ref name="Ashton2025a"/><ref name="jplsats-elem"/> It is unknown whether all of these subgroups of the Inuit group share a common origin.<ref name="Ashton2025a"/>

The Kiviuq group includes 20 members, with the only named members being [[Ijiraq (moon)|Ijiraq]] and the group's largest member and namesake Kiviuq. Kiviuq has a diameter of about 17&nbsp;km and has a highly elongated shape, which may indicate it is a [[contact binary (small Solar System body)|contact binary]].<ref name="Denk2018"/> The Siarnaq group includes 15 members, with the only named members being [[Tarqeq]] and the group's namesake Siarnaq.<ref name="jplsats-elem"/> Siarnaq is the largest member of its subgroup and the entire Inuit group, with an estimated diameter of about 39&nbsp;km.<ref name="Grav2015"/> The moons of the Kiviuq and Siarnaq subgroups are tightly clustered in semi-major axis and inclination with respect to their namesake moon, which makes them distinct collisional families.<ref name="Ashton2025a"/><ref name="Ashton2025b"/> In contrast to Kiviuq and Siarnaq, Paaliaq (diameter ~25&nbsp;km) does not have an associated subgroup.<ref name="Ashton2025a"/><ref name="Sheppard2023"/>

====Gallic====
{{Main|Gallic group}}

The Gallic group includes 17<!--for a count of 274--> prograde outer moons that are similar in their orbital inclination (34–41°), their orbital eccentricity, and their color that they can be considered a group.<ref name=Gladman2001/><ref name=Grav2007/> The named members of the Gallic group are [[Albiorix (moon)|Albiorix]], [[Bebhionn (moon)|Bebhionn]], [[Erriapus]], and [[Tarvos (moon)|Tarvos]].<ref name="jplsats-elem"/> The largest of these moons is Albiorix with an estimated diameter of about 29&nbsp;km.<ref name="Grav2015"/> The Gallic group may be divided into the Albiorix subgroup, which consists of 16 moons with semi-major axes between 200–330 radii of Saturn, and the outlier moon [[S/2004 S 24]] which has a lower eccentricity and a much more distant semi-major axis of ~400 Saturn radii.<ref name="jplsats-elem" /><ref name="Ashton2025a"/> S/2004 S 24 may not be directly related to the Gallic group, although it is possible that it could have formed as a fragment of an Albiorix subgroup member that was collisionally disrupted when it was at its farthest distance from Saturn in its elliptical orbit.<ref name="Ashton2025a"/>

====Norse====
[[File:Phoebe cassini full.jpg|thumb|[[Phoebe (moon)|Phoebe]], Saturn's largest irregular moon]]
{{Main|Norse group}}

All 197<!--for a count of 274--> [[retrograde motion|retrograde]] outer moons of Saturn are broadly classified into the Norse group.<ref name="Gladman2001" /><ref name="Grav2007" /> Only 31 moons of the Norse group have been named: [[Aegir (moon)|Aegir]], [[Angrboda (moon)|Angrboda]], [[Alvaldi (moon)|Alvaldi]], [[Beli (moon)|Beli]], [[Bergelmir (moon)|Bergelmir]], [[Bestla (moon)|Bestla]], [[Eggther (moon)|Eggther]], [[Farbauti (moon)|Farbauti]], [[Fenrir (moon)|Fenrir]], [[Fornjot (moon)|Fornjot]], [[Geirrod (moon)|Geirrod]], [[Gerd (moon)|Gerd]], [[Greip (moon)|Greip]], [[Gridr (moon)|Gridr]], [[Gunnlod (moon)|Gunnlod]], [[Hati (moon)|Hati]], [[Hyrrokkin (moon)|Hyrrokkin]], [[Jarnsaxa (moon)|Jarnsaxa]], [[Kari (moon)|Kari]], [[Loge (moon)|Loge]], [[Mundilfari (moon)|Mundilfari]], [[Narvi (moon)|Narvi]], [[Phoebe (moon)|Phoebe]], [[Skathi (moon)|Skathi]], [[Skoll (moon)|Skoll]], [[Skrymir (moon)|Skrymir]], [[Surtur (moon)|Surtur]], [[Suttungr (moon)|Suttungr]], [[Thiazzi (moon)|Thiazzi]], [[Thrymr (moon)|Thrymr]], and [[Ymir (moon)|Ymir]].<ref name="jplsats-elem"/>

Although the Norse group does not show obvious clustering in orbital elements, researchers led by Edward Ashton have proposed splitting the Norse group into four different subgroups by inclination.<ref name="Ashton2025a"/> These subgroups still have a broad range of orbital semi-major axes, inclinations, and eccentricities, and may not necessarily have an impact origin.<ref name="Ashton2025a"/>

*The Phoebe subgroup consists of moons between inclinations 172.5° and 180° and is named after [[Phoebe (moon)|Phoebe]],<ref name="Ashton2025a" /> by far the largest irregular moon of Saturn with a diameter of {{val|213|1.4|u=km}}.<ref name="Jewitt2007" /> It has a retrograde orbit and rotates on its axis every 9.3 hours.<ref name="Giese2006" /> Phoebe was the first moon of Saturn to be studied in detail by ''Cassini'', in {{Nowrap|June 2004}}; during this encounter ''Cassini'' was able to map nearly 90% of the moon's surface. Phoebe has a nearly spherical shape and a relatively high density of about 1.6&nbsp;g/cm<sup>3</sup>.<ref name="Jewitt2007" /> ''Cassini'' images revealed a dark surface scarred by numerous impacts—there are about 130 craters with diameters exceeding 10&nbsp;km. Such impacts may have ejected fragments of Phoebe into orbit around Saturn—two of these may be [[S/2006 S 20]] and [[S/2006 S 9]], whose orbits are similar to Phoebe.<ref name="Sheppard2023" /><ref>{{Cite web |title=S/2006 S 20 – Tilmann Denk |url=https://tilmanndenk.de/outersaturnianmoons/s2006_s20/ |access-date=2024-01-23 |language=en-US |archive-date=2024-06-16 |archive-url=https://web.archive.org/web/20240616103718/https://tilmanndenk.de/outersaturnianmoons/s2006_s20/ |url-status=live}}</ref><ref>{{Cite web |title=S/2006 S 9 – Tilmann Denk |url=https://tilmanndenk.de/outersaturnianmoons/s2006_s9/ |access-date=2024-01-23 |language=en-US |archive-date=2023-12-24 |archive-url=https://web.archive.org/web/20231224062938/https://tilmanndenk.de/outersaturnianmoons/s2006_s9/ |url-status=live}}</ref> Spectroscopic measurement showed that the surface is made of water ice, [[carbon dioxide]], [[phyllosilicate]]s, organics and possibly iron-bearing minerals.<ref name="Jewitt2007" /> Phoebe is believed to be a captured [[Centaur (minor planet)|centaur]] that originated in the [[Kuiper belt]].<ref name="Jewitt2007" /> It also serves as a source of material for the largest known ring of Saturn, which darkens the leading hemisphere of Iapetus (see above).<ref name="Verbiscer2009" />

*The Mundilfari subgroup consists of moons between inclinations 157° and 172.5° and is the most populated of the four Norse subgroups proposed by Ashton and collaborators.<ref name="Ashton2025a"/> Named after its largest member [[Mundilfari (moon)|Mundilfari]] (diameter ~7&nbsp;km), this subgroup is dominated by tiny moons smaller than 4&nbsp;km in diameter, which suggests they were formed by a relatively recent collisional event that destroyed a progenitor moon at least 100 million years ago.<ref name="Ashton2025a"/><ref name="Ashton2025b"/> Ashton and collaborators proposed that this progenitor moon of the Mundifari subgroup would have orbited Saturn at a semi-major axis of ~19.5&nbsp;million&nbsp;km (~320 Saturn radii), inclination ~165°, and eccentricity ~0.28.<ref name="Ashton2025a"/> The collision that destroyed this progenitor moon would have to eject its fragments at a speed of at least 200&nbsp;m/s, and subsequent collisions of its fragments may further disperse their orbits to produce the broad orbital distribution of the Mundilfari group observed today.<ref name="Ashton2025a"/>

*The Kari subgroup consists of moons between inclinations 151° and 157° and appears mostly concentrated around the orbit of its namesake and largest member [[Kari (moon)|Kari]] (diameter ~6&nbsp;km) with a semi-major axis range between {{convert|0.14–0.16|AU|e6km|abbr=unit}} from Saturn.<ref name="Ashton2025a"/> This tight clustering may be a collisional family.<ref name="Ashton2025a"/> There are several other moons in the Kari subgroup's inclination range that have semi-major axes less than the aforementioned range, and thus may not be related to the proposed collisional family.<ref name="Ashton2025a"/><ref name="Ashton2025b"/>

*The remaining Norse group moons with inclinations below 151° are sparse in number and are assigned to the low-inclination subgroup by Ashton and collaborators.<ref name="Ashton2025a"/> Of the moons of the low-inclination subgroup, [[Narvi (moon)|Narvi]] and [[S/2019 S 11]] have the most similar orbits to each other, which suggests these two moons share an origin.<ref name="Ashton2025a"/>

==List==
[[File:Saturnmoonsdiagram.png|thumb|upright=4|center|Orbital diagram of the [[orbital inclination]] and orbital distances for Saturn's rings and moon system at various scales. Notable moons, moon groups, and rings are individually labeled. Open the image for full resolution.]]

===Confirmed===
The Saturnian moons are listed here by [[orbital period]] (or semi-major axis), from shortest to longest. Moons massive enough for their surfaces to have [[gravitational collapse|collapsed]] into a [[spheroid]] are highlighted in bold and marked with a blue background, while the irregular moons are listed in red, orange, green, and gray background. The orbits and mean distances of the irregular moons are strongly variable over short timescales due to frequent planetary and solar [[perturbation (astronomy)|perturbations]], so the orbital elements of irregular moons listed here are averaged over a 5,000-year [[numerical integration]] by the [[Jet Propulsion Laboratory]]. These may sometimes strongly differ from the [[osculating orbit|osculating]] orbital elements provided by other sources.<ref name="jplsats-elem"/><ref name="Jacobson2022b"/> Otherwise, recently discovered irregular moons without published proper elements are temporarily listed here with inaccurate [[Osculating orbit|osculating orbital elements]] that are ''italicized'' to distinguish them from other irregular moons with proper orbital elements. The mean orbital elements are based on a reference [[Epoch (astronomy)|epoch]] of 1 January 2000.<ref name="jplsats-elem">{{cite web|title=Planetary Satellite Mean Elements|url=https://ssd.jpl.nasa.gov/sats/elem/|publisher=Jet Propulsion Laboratory|access-date=10 November 2025|archive-date=November 16, 2025|archive-url=https://web.archive.org/web/20251116001458/https://ssd.jpl.nasa.gov/sats/elem/|url-status=live}}</ref>

<div style="float:left">
{| class="wikitable" style="margin:0; font-size:90%; text-align:left"
|-
|+ Key
|-
| style="background:#fff;" |&nbsp; ''Small regular moons (17)''
| style="background:#ccf;" | ♠ '''''Major moons''' (7)''
| style="background:#f4c2c2"| ♦ ''[[Inuit group]] (36)''
| style="background:#fdd5b1"| ♣ ''[[Gallic group]] (17)''
| style="background:#d3d3d3"| ‡ ''[[Norse group]] (197)''
|}</div>

{{Clear}}
{{sort under}}
{{sticky table start}}
{| class="wikitable sortable sort-under sticky-table-row1 sticky-table-col1" style="font-size:85%"
|-
! Label<br>{{refn|group=lower-alpha|A confirmed moon is given a permanent designation by the [[International Astronomical Union|IAU]] consisting of a name and a [[Roman numeral]].<ref name="Gazetteer" /> The eight moons that were known before 1850 are numbered in order of their distance from Saturn; the rest are numbered in the order by which they received their permanent designations. Many small moons have not yet received a permanent designation.}}
! Name
! class="unsortable" |Pronunciation
! class="unsortable" |Image
! data-sort-type="number" | [[Absolute magnitude#Solar System bodies (H)|Abs.<br>magn.]]<br />{{refn|group=lower-alpha|Absolute magnitudes of regular satellites are calculated from their mean diameters and geometric albedos given in NASA's Saturnian Satellite Fact Sheet.<ref name="NASA"/> Absolute magnitude estimates for some small inner moons are not available as they do not have measured geometric albedos. Absolute magnitudes of irregular satellites were taken from the Minor Planet Center's Natural Satellites Ephemeris Service.<ref name="MPC-NatSats"/>|name=absmag}}
! data-sort-type="number" | [[List of Solar System objects by size|Diameter]]<br>(km)<br />{{refn|group=lower-alpha|The diameters and dimensions of the small inner moons, from Pan to Helene, are taken from Thomas et al., 2020, Table 1.<ref name="Thomas2020"/> Diameters and dimensions of Mimas, Enceladus, Tethys, Dione, Rhea, Iapetus, and Phoebe are from Thomas 2010, Table 1.<ref name="Thomas2010"/> Diameters of Siarnaq and Albiorix are from Grav et al., 2015, Table 3.<ref name="Grav2015"/> The approximate sizes of all other irregular satellites are calculated from their absolute magnitudes with an assumed geometric albedo of 0.04, which is the average value for that population.<ref name="Grav2015"/> Calculations were made with NASA/JPL's Asteroid Size Estimator.<ref name="SizeEstimator"/>|name=diameter}}
! data-sort-type="number" | [[List of Solar System objects by mass|Mass]]<br>({{e|15}} kg)<br />{{refn|group=lower-alpha|Masses of the large round moons, including Hyperion, Phoebe, and Helene, were taken from Jacobson et al., 2022, Table 5.<ref name="Jacobson2022a"/> Masses of Atlas, Prometheus, Pandora, Epimetheus, and Janus were taken from Lainey et al., 2023, Table 1.<ref name="Lainey2023"/> Masses of Pan, Daphnis, Aegaeon, Methone, and Pallene were taken from Thomas et al., 2020, Table 2.<ref name="Thomas2020"/> Masses of other regular satellites were calculated by multiplying their volumes with an assumed density of 500 kg/m<sup>3</sup> (0.5&nbsp;g/cm<sup>3</sup>), while masses of irregular satellites were calculated with an assumed density of 1000 kg/m<sup>3</sup> (1.0&nbsp;g/cm<sup>3</sup>).}}
! data-sort-type="number" | [[Semi-major axis|Semi-major<br>axis]]<br>(km)<br /><ref name="jplsats-elem"/>
! data-sort-type="number" | [[Orbital period]] ([[day|d]])<br /><ref name="jplsats-elem"/>{{refn | group = lower-alpha | Negative orbital periods indicate a [[retrograde orbit]] around Saturn (opposite to the planet's rotation). Orbital periods of irregular satellites may not directly correlate with their semi-major axes due to perturbations.}}
! data-sort-type="number" | [[Orbital inclination|Inclination]]<br />([[Degree (angle)|°]])<br /><ref name="jplsats-elem"/>{{refn | group = lower-alpha |Orbital inclinations of regular satellites and Phoebe are with respect to their [[Laplace plane]]s. Orbital inclinations of irregular satellites are with respect to the ecliptic.<ref name="jplsats-elem"/>|name=inclination}}
! data-sort-type="number"| [[Orbital eccentricity|Eccentricity]]<br /><ref name="jplsats-elem"/>
! Position<br>{{refn|group=lower-alpha|The irregular moons are categorized as described in Ashton et al., 2025a. Otherwise, for the 128 newly discovered satellites not included in the paper, they are sorted into their categories based on the inclination and semi-major axis criteria stated in Ashton et al., 2025a.<ref name="Ashton2025a"/>}}
! [[Timeline of discovery of Solar System planets and their moons|Discovery<br>year]]<br /><ref name="jplsats-disc">{{cite web|title=Planetary Satellite Discovery Circumstances|url=https://ssd.jpl.nasa.gov/sats/discovery.html|publisher=Jet Propulsion Laboratory|date=23 May 2023|access-date=7 June 2023|archive-date=27 September 2021|archive-url=https://web.archive.org/web/20210927162554/https://ssd.jpl.nasa.gov/sats/discovery.html|url-status=live}}</ref>
! Year announced
! Discoverer<br /><ref name="Gazetteer" /><ref name="jplsats-disc" />
|-style="background:#fff;"
| {{sort|Q|}} || {{hid|S/2009}} <small>[[S/2009 S 1]]</small> || — || style="background:white;"| [[File:PIA11665 moonlet in B Ring cropped.jpg|frameless|upright=0.3|center]] || {{sort|98|—}} || 0.3 || {{nowrap|{{sort|0.0000071|≈&thinsp;{{val|0.0000071}}}}}} || {{sort|116900|&thinsp;{{val|116900}}}}|| {{sort|0.47150|&thinsp;{{val|0.47150}}}}|| {{sort|0|≈&thinsp;{{val|0.0}}}} || {{sort|0|≈&thinsp;{{val|0.000}}}} || outer B Ring || 2009 || 2009 || ''[[Cassini–Huygens|Cassini]]''<ref name="IAUC2009b" />
|-style="background:#fff;"
| {{sort|A|}} || ([[moonlet]]s) || — || style="background:white;"| [[File:First moonlets PIA07792 (closeup).jpg|frameless|upright=0.3|center|alt=A noisy image showing a few bright dots marked by circles]] || {{sort|99|—}} || {{sort|0.22|0.04–0.4}} || {{nowrap|{{sort|0.000017|<&thinsp;{{val|0.000017}}}}}} || {{sort|130000|≈&thinsp;{{val|130000}}}} || {{sort|0.55|≈&thinsp;{{val|0.55}}}} || {{sort|0|≈&thinsp;0.0}} || {{sort|0|≈&thinsp;0.000}} || Three 1,000&nbsp;km bands within A Ring<ref name="Tiscareno2008"/> || 2006 || — || ''[[Cassini–Huygens|Cassini]]''
|-style="background:#fff;"
| {{sort|18|XVIII}} || {{hid|Pan}} [[Pan (moon)|Pan]] || {{IPAc-en|ˈ|p|æ|n}} || style="background:black;"| [[File:Pan_by_Cassini,_March_2017.jpg|frameless|upright=0.3|center|alt=An irregularly shaped body with a prominent equatorial ridge. It is illuminated from the bottom right.]]|| 9.2 || {{sort|28.2|28.2<br>(35&thinsp;×&thinsp;28&thinsp;×&thinsp;21)}} || {{val|4.30}} || {{val|133600}} || {{sort|0.57505|+{{val|0.57505}}}} || 0.0 || 0.000 || in Encke Division || 1990 || 1990 || [[Mark Showalter|Showalter]]
|-style="background:#fff;"
| {{sort|35|XXXV}} || {{hid|Daphnis}} [[Daphnis (moon)|Daphnis]] || {{IPAc-en|ˈ|d|æ|f|n|ə|s}} || style="background:black;"| [[File:Daphnis (Saturn's Moon).jpg|frameless|upright=0.3|center|alt=A small, irregularly shaped body elongated from the bottom left to top right. It is illuminated from the bottom left.]] || {{sort|99|—}} || {{sort|7.6|7.6<br>(9.8&thinsp;×&thinsp;8.4&thinsp;×&thinsp;5.6)}}|| {{val|0.068}} || {{val|136500}} || {{sort|0.59408|+{{val|0.59408}}}} || 0.0 || 0.000 || in Keeler Gap || 2005 || 2005 || ''[[Cassini–Huygens|Cassini]]''
|-style="background:#fff;"
| {{sort|15|XV}} || {{hid|Atlas}} [[Atlas (moon)|Atlas]] || {{IPAc-en|ˈ|æ|t|l|ə|s}} || style="background:black;"| [[File:Atlas color PIA21449.png|frameless|upright=0.3|center|alt=An irregularly shaped body is fully illuminated. The body, which looks like a cone viewed from the south pole, is elongated downward.]] || 8.5 || {{sort|30.2|30.2<br>(41&thinsp;×&thinsp;35&thinsp;×&thinsp;19)}} || {{val|5.490}} || {{val|137700}} || {{sort|0.60460|+{{val|0.60460}}}} || 0.0 || 0.001 || || 1980 || 1980 || ''[[Voyager 1]]''
|-style="background:#fff;"
| {{sort|16|XVI}} || {{hid|Prometheus}} [[Prometheus (moon)|Prometheus]] || {{IPAc-en|p|r|oʊ|ˈ|m|iː|θ|i|ə|s}} || style="background:black;"| [[File:Prometheus 12-26-09a.jpg|frameless|upright=0.3|center|alt=An irregularly shaped oblong body is fully illuminated. It is elongated in the direction from the top left to bottom left. Its surface is covered by craters.]] || 6.7 || {{sort|86.2|86.2<br>(137&thinsp;×&thinsp;81&thinsp;×&thinsp;56)}} || {{val|159.72}} || {{val|139400}} || {{sort|0.61588|+{{val|0.61588}}}} || 0.0 || 0.002 || F Ring shepherd || 1980 || 1980 || ''[[Voyager 1]]''
|-style="background:#fff;"
| {{sort|17|XVII}} || {{hid|Pandora}} [[Pandora (moon)|Pandora]] || {{IPAc-en|p|æ|n|ˈ|d|ɔər|ə}} || style="background:black;"| [[File:PIA21055 - Pandora Up Close (cropped).jpg|alt=An irregularly shaped body is half illuminated from the bottom. The terminator runs from the left to right. The surface is covered by numerous craters.|center|frameless|upright=0.3]] || 6.5 || {{sort|81.4|81.4<br>(104&thinsp;×&thinsp;81&thinsp;×&thinsp;64)}} || {{val|135.7}} || {{val|141700}} || {{sort|0.63137|+{{val|0.63137}}}} || 0.0 || 0.004 || || 1980 || 1980 || ''[[Voyager 1]]''
|-style="background:#fff;"
| {{sort|11|XI}} || {{hid|Epimetheus}} [[Epimetheus (moon)|Epimetheus]] || {{IPAc-en|ɛ|p|ə|ˈ|m|iː|θ|i|ə|s}} || style="background:black;"| [[File:PIA09813 Epimetheus S. polar region.jpg|frameless|upright=0.3|center|alt=A partially-illuminated irregular body, which has a shape remotely resembling a cube. The body's surface consists of ridges and valleys and is covered by craters.]] || 5.5 || {{sort|116.2|116.2<br>(130&thinsp;×&thinsp;114&thinsp;×&thinsp;106)}} || {{val|525.607}} || {{val|151400}} || {{sort|0.69701|+{{val|0.69701}}}} || 0.3 || 0.020 || co-orbital with Janus || 1966 || 1967 || Fountain & Larson
|-style="background:#fff;"
| {{sort|10|X}} || {{hid|Janus}} [[Janus (moon)|Janus]] || {{IPAc-en|ˈ|dʒ|eɪ|n|ə|s}} || style="background:black;"| [[File:PIA12714 Janus crop.jpg|frameless|upright=0.3|alt=An irregular body, whose outline looks like an approximate circle in this image. It is illuminated from the bottom-left. The terminator runs from the top-left to bottom-right. The surface is covered by craters.]] || 4.5 || {{sort|179|179<br>(203&thinsp;×&thinsp;185&thinsp;×&thinsp;153)}} || {{val|1893.88}} || {{val|151500}} || {{sort|0.69735|+{{val|0.69735}}}} || 0.2 || 0.007 || co-orbital with Epimetheus || 1966 || 1967 || [[Audouin Dollfus|Dollfus]]
|-style="background:#fff;"
| {{sort|53|LIII}} || {{hid|Aegaeon}} [[Aegaeon (moon)|Aegaeon]] || {{IPAc-en|iː|ˈ|dʒ|iː|ɒ|n}} || style="background:black;"| [[File:N1643264379_1.jpg|frameless|upright=0.3|center|alt=Image of Aegaeon by Cassini.]] || {{sort|99|—}} || {{sort|0.66|0.66<br>(1.4&thinsp;×&thinsp;0.5&thinsp;×&thinsp;0.4)}} || {{val|0.0000782}} ||| {{val|167500}} || {{sort|0.80812|+{{val|0.80812}}}} || 0.0 || 0.000 || G Ring moonlet || 2008 || 2009 || ''[[Cassini–Huygens|Cassini]]''
|- style="background:#ccf;"
| {{sort|01|I}} || {{hid|Mimas}} ♠'''[[Mimas]]''' || {{IPAc-en|ˈ|m|aɪ|m|ə|s}} || style="background:black;"| [[File:Mimas_Cassini.jpg|frameless|upright=0.3|center|alt=A spherical body is half illuminated from the left. The terminator runs from the top to bottom in the vicinity of the right limb. A large crater with a central peak sits on the terminator slightly to the right and above the center of the body. It makes the body look like the Death Star. There are numerous smaller craters.]] || 3.2 || {{sort|396.4|396.4<br>(416&thinsp;×&thinsp;393&thinsp;×&thinsp;381)}} || {{val|37509.4}} || {{val|186000}} || {{sort|0.94242|+{{val|0.94242}}}} || 1.6 || 0.020 || &nbsp; || 1789 || 1789 || [[William Herschel|Herschel]]
|-style="background:#fff;"
| {{sort|32|XXXII}} || {{hid|Methone}} [[Methone (moon)|Methone]] || {{IPAc-en|m|ə|ˈ|θ|oʊ|n|iː}} || style="background:black;"| [[File:Methone PIA14633.jpg|frameless|upright=0.3|center|alt=A smooth, featureless ellipsoidal object illuminated from the top right, distinctly looking like an egg.]] || {{sort|99|—}} || {{sort|2.9|2.9<br>(4.0&thinsp;×&thinsp;2.6&thinsp;×&thinsp;2.4)}} || {{val|0.00392}} ||| {{val|194700}} || {{sort|1.00955|+{{val|1.00955}}}} || 0.0 || 0.002 || Alkyonides || 2004 || 2004 || ''[[Cassini–Huygens|Cassini]]''
|-style="background:#fff;"
| {{sort|49|XLIX}} || {{hid|Anthe}} [[Anthe (moon)|Anthe]] || {{IPAc-en|ˈ|æ|n|θ|iː}} || style="background:black;"| [[File:Anthe crop.jpg|frameless|upright=0.3|center|alt=A blurry ellipsoidal object in the center of the image]] || {{sort|99|—}} || 1.8 || {{sort|0.0015|≈&thinsp;{{val|0.0015}}}} ||| {{val|198100}} || {{sort|1.03890|+{{val|1.03890}}}} || 0.0 || 0.002 || Alkyonides || 2007 || 2007 || ''[[Cassini–Huygens|Cassini]]''
|-style="background:#fff;"
| {{sort|33|XXXIII}} || {{hid|Pallene}} [[Pallene (moon)|Pallene]] || {{IPAc-en|p|ə|ˈ|l|iː|n|iː}} || style="background:#bab271;"| [[File:Pallene Cassini color-crop 20101016.png|frameless|upright=0.3|center|alt=A small, half-illuminated ellipsoidal object in front of Saturn as a backdrop]] || {{sort|99|—}} || {{sort|4.44|4.44<br>(5.8&thinsp;×&thinsp;4.2&thinsp;×&thinsp;3.7)}} || {{sort|0.023|≈&thinsp;{{val|0.023}}}} ||| {{val|212300}} || {{sort|1.15606|+{{val|1.15606}}}} || 0.2 || 0.004 || Alkyonides || 2004 || 2004 || ''[[Cassini–Huygens|Cassini]]''
|- style="background:#ccf;"
| {{sort|02|II}} || {{hid|Enceladus}} ♠'''[[Enceladus]]''' || {{IPAc-en|ɛ|n|ˈ|s|ɛ|l|ə|d|ə|s}} || style="background:black;"| [[File:PIA17202 - Approaching Enceladus.jpg|frameless|upright=0.3|center]] || 2.1 || {{sort|504.2|504.2<br>(513&thinsp;×&thinsp;503&thinsp;×&thinsp;497)}} || {{val|108031.8}} || {{val|238400}} || {{sort|1.37022|+{{val|1.37022}}}} || 0.0 || 0.005 || Generates the E ring || 1789 || 1789 || [[William Herschel|Herschel]]
|- style="background:#ccf;"
| {{sort|03|III}} || {{hid|Tethys}} ♠'''[[Tethys (moon)|Tethys]]''' || {{IPAc-en|ˈ|t|iː|θ|ə|s}} || style="background:black;"| [[File:Tethys.jpg.fromcassini.jpg|center|frameless|upright=0.3]]|| 0.7 || {{sort|1062.2|1062.2<br>(1077&thinsp;×&thinsp;1057&thinsp;×&thinsp;1053)}} || {{val|617495.9}} || {{val|295000}} || {{sort|1.887802|+{{val|1.88780}}}}|| 1.1 || 0.001 || &nbsp; || 1684 || 1684 || [[Giovanni Domenico Cassini|Cassini]]
|-style="background:#fff;"
| {{sort|13|XIII}} || {{hid|Telesto}} [[Telesto (moon)|Telesto]] || {{IPAc-en|t|ə|ˈ|l|ɛ|s|t|oʊ}} || style="background:black;"| [[File:Telesto cassini closeup.jpg|frameless|upright=0.3|center|alt=An oblong object with a few large craters and a smooth surface]] || 8.7 || {{sort|24.8|24.8<br>(33&thinsp;×&thinsp;23&thinsp;×&thinsp;19)}} || {{sort|3.9|≈&thinsp;{{val|3.9}}}} || {{val|295000}} || {{sort|1.887802|+{{val|1.88780}}}}|| 1.2 || 0.001 || leading Tethys trojan ({{L4}}) || 1980 || 1980 || [[Bradford A. Smith|Smith]] et al.
|-style="background:#fff;"
| {{sort|14|XIV}} || {{hid|Calypso}} [[Calypso (moon)|Calypso]] || {{IPAc-en|k|ə|ˈ|l|ɪ|p|s|oʊ}} || style="background:black;" | [[File:Calypso N1644755236 1.jpg|frameless|upright=0.3|center|alt=An oblong body is seen in this low resolution image.]] || 9.2 || {{sort|21.4|21.4<br>(29&thinsp;×&thinsp;19&thinsp;×&thinsp;13)}} || {{sort|1.8|≈&thinsp;{{val|1.8}}}} || {{val|295000}} || {{sort|1.887803|+{{val|1.88780}}}}|| 1.5 || 0.001 || trailing Tethys trojan ({{L5}}) || 1980 || 1980 || Pascu et al.
|-style="background:#fff;"
| {{sort|12|XII}} || {{hid|Helene}} [[Helene (moon)|Helene]] || {{IPAc-en|ˈ|h|ɛ|l|ə|n|iː}} || style="background:black;" | [[File:PIA12758 Helene crop.jpg|frameless|upright=0.3|center|alt=An irregularly shaped body illuminated from the left. Its surface is covered by numerous impact craters.]] || 8.2 || {{sort|35.2|35.2<br>(45&thinsp;×&thinsp;39&thinsp;×&thinsp;27)}} || {{val|7.1}} || {{val|377600}} || {{sort|2.73692|+{{val|2.73692}}}} || 0.2 || 0.007 || leading Dione trojan ({{L4}}) || 1980 || 1980 || Laques & Lecacheux
|-style="background:#fff;"
| {{sort|34|XXXIV}} || {{hid|Polydeuces}} [[Polydeuces (moon)|Polydeuces]] || {{IPAc-en|p|ɒ|l|i|ˈ|dj|uː|s|iː|z}} || style="background:black;" | [[File:Polydeuces.jpg|frameless|upright=0.3|center|alt=A small oblong body is barely resolved in this image.]] || {{sort|99|—}} || {{sort|2.6|2.6<br>(3.5&thinsp;×&thinsp;3.1&thinsp;×&thinsp;2.7)}} || {{sort|0.0075|≈&thinsp;{{val|0.0075}}}} || {{val|377600}} || {{sort|2.73692|+{{val|2.73692}}}} || 0.2 || 0.019 || trailing Dione trojan ({{L5}}) || 2004 || 2004 || ''[[Cassini–Huygens|Cassini]]''
|- style="background:#ccf;"
| {{sort|04|IV}} || {{hid|Dione}} ♠'''[[Dione (moon)|Dione]]''' || {{IPAc-en|d|aɪ|ˈ|oʊ|n|iː}} || style="background:black;" | [[File:Dione in natural light (cropped).jpg|center|frameless|upright=0.3]]|| 0.8 || {{sort|1122.8|1122.8<br>(1128&thinsp;×&thinsp;1123&thinsp;×&thinsp;1119)}} || {{val|1095486.8}} || {{val|377700}} || {{sort|2.73692|+{{val|2.73692}}}} || 0.0 || 0.002 || &nbsp; || 1684 || 1684 || [[Giovanni Domenico Cassini|Cassini]]
|- style="background:#ccf;"
| {{sort|05|V}} || {{hid|Rhea}} ♠'''[[Rhea (moon)|Rhea]]''' || {{IPAc-en|ˈ|r|eɪ|ə}} || style="background:black;"| [[File:Rhea true color.jpg|frameless|upright=0.3|center]] || 0.1 || {{sort|1527.6|1527.6<br>{{nowrap|(1530&thinsp;×&thinsp;1526&thinsp;×&thinsp;1525)}}}} || {{val|2306485.4}} || {{val|527200}} || {{sort|4.51750|+{{val|4.51750}}}} || 0.3 || 0.001 || &nbsp; || 1672 || 1673 || [[Giovanni Domenico Cassini|Cassini]]
|- style="background:#ccf;"
| {{sort|06|VI}} || {{hid|Titan}} ♠'''[[Titan (moon)|Titan]]''' || {{IPAc-en|ˈ|t|aɪ|t|ən}} || style="background:black;"| [[File:Titan in true color.jpg|frameless|upright=0.3|center]] || –1.3 || {{sort|5149.46|5149.46<br>{{nowrap|({{val|5149}}&thinsp;×&thinsp;{{val|5149}}&thinsp;×&thinsp;{{val|5150}})}}}} || {{val|134518035.4}} || {{val|1221900}} || {{sort|15.9454|+{{val|15.9454}}}} || 0.3 || 0.029 || &nbsp; || 1655 || 1656 || [[Christiaan Huygens|Huygens]]
|-style="background:#fff;"
| {{sort|07|VII}} || {{hid|Hyperion}} [[Hyperion (moon)|Hyperion]] || {{IPAc-en|h|aɪ|ˈ|p|ɪər|i|ə|n}} || style="background:black;"| [[File:Hyperion true.jpg|frameless|upright=0.3|center|alt=An irregularly shaped oblong body is illuminated from the left. The terminator is near the right limb. The body is elongated in the top-bottom direction. The surface is punctured by numerous impact craters, which make it look like a sponge or cheese.]] || 4.8 || {{sort|270.0|270.0<br>(360&thinsp;×&thinsp;266&thinsp;×&thinsp;205)}} || {{val|5551.0}} || {{val|1481500}} || {{sort|21.2767|+{{val|21.2767}}}} || 0.6 || 0.105 || in 4:3 resonance with Titan || 1848 || 1848 || [[William Cranch Bond|Bond]] & [[William Lassell|Lassell]]
|- style="background:#ccf;"
| {{sort|08|VIII}} || {{hid|Iapetus}} ♠'''[[Iapetus (moon)|Iapetus]]''' || {{IPAc-en|aɪ|ˈ|æ|p|ə|t|ə|s}} || style="background:black;"| [[File:Iapetus.jpg|frameless|upright=0.3|center]] || 1.2 || {{sort|1468.6|1468.6<br>{{nowrap|(1491&thinsp;×&thinsp;1491&thinsp;×&thinsp;1424)}}}} || {{val|1805659.1}} || {{val|3561700}} || {{sort|79.3310|+{{val|79.3310}}}} || 7.6 || 0.028 || &nbsp; || 1671 || 1673 || [[Giovanni Domenico Cassini|Cassini]]
|- id="S/2023 S 1" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 1</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11205400}} || {{sort|442.86|+{{val|442.86}}}} || 48.8 || 0.386 || [[Inuit group]] (Kiviuq) || 2023 || 2025 || Ashton et al.
|- id="S/2019 S 1" style="background:#F4C2C2;"
| {{sort|R|}} || {{hid|S/2019A}} ♦<small>[[S/2019 S 1]]</small> || — || style="background:black;"| [[File:2019 S 1 CFHT 2019-07-02 15x205s stack.png|frameless|upright=0.3|center]] || 15.3 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|11245400}}|| {{sort|445.17|+{{val|445.17}}}} || 49.5 || 0.383 || Inuit group (Kiviuq) || 2019 || 2021 || Ashton et al.
|- id="S/2004 S 54" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2004 S 54</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11277500}} || {{sort|447.14|+{{val|447.14}}}} || 48.1 || 0.373 || Inuit group (Kiviuq) || 2004 || 2025 || Sheppard et al.
|- id="S/2004 S 55" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2004 S 55</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11294700}} || {{sort|448.16|+{{val|448.16}}}} || 48.9 || 0.260 || Inuit group (Kiviuq) || 2004 || 2025 || Sheppard et al.
|- id="S/2020 S 11" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 11</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11295600}} || {{sort|448.21|+{{val|448.21}}}} || 48.2 || 0.372 || Inuit group (Kiviuq) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 22" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 22</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11305100}} || {{sort|448.78|+{{val|448.48}}}} || 47.3 || 0.369 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al.
|- id="Kiviuq" style="background:#F4C2C2;"
| {{sort|24|XXIV}} || {{hid|Kiviuq}} ♦[[Kiviuq (moon)|Kiviuq]] || {{IPAc-en|ˈ|k|ɪ|v|i|ə|k}} || style="background:black;" | [[File:Kiviuq-CFHT.gif|frameless|upright=0.3|center]] || 12.7 || {{sort|17|≈&thinsp;{{val|17}}}}|| {{sort|3.6|≈&thinsp;{{val|3.6}}}} || {{val|11307400}}|| {{sort|448.91|+{{val|448.91}}}} || 48.0 || 0.275 || Inuit group (Kiviuq) || 2000 || 2000 || Gladman et al.
|- id="S/2023 S 2" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 2</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11309900}} || {{sort|449.05|+{{val|449.05}}}} || 45.7 || 0.339 || Inuit group (Kiviuq) || 2023 || 2025 || Ashton et al.
|- id="S/2019 S 23" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 23</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11310200}} || {{sort|449.08|+{{val|449.08}}}} || 48.7 || 0.255 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al.
|- id="S/2020 S 12" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 12</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11314500}} || {{sort|449.33|+{{val|449.33}}}} || 50.8 || 0.260 || Inuit group (Kiviuq) || 2020 || 2025 || Ashton et al.
|- id="S/2005 S 4" style="background:#F4C2C2;"
| {{sort|Zza|}} || {{hid|S/2005A}} ♦<small>[[S/2005 S 4]]</small> || — || style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|11324500}} || {{sort|449.93|+{{val|449.93}}}} || 48.0 || 0.315 || Inuit group (Kiviuq) || 2005 || 2023 || Sheppard et al.
|- id="S/2019 S 25" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 25</small> || ― || style="background:black;"| || 16.4 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11329400}} || {{sort|450.22|+{{val|450.22}}}} || 48.1 || 0.271 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al.
|- id="S/2020 S 1" style="background:#F4C2C2;"
| {{sort|S|}} || {{hid|S/2020A}} ♦<small>[[S/2020 S 1]]</small> || — || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11338600}} || {{sort|450.77|+{{val|450.77}}}} || 48.2 || 0.337 || Inuit group (Kiviuq) || 2020 || 2023 || Ashton et al.
|- id="Ijiraq" style="background:#F4C2C2;"
| {{sort|22|XXII}} || {{hid|Ijiraq}} ♦[[Ijiraq (moon)|Ijiraq]] || {{IPAc-en|ˈ|iː|ɪ|r|ɒ|k}} || style="background:black;" | [[File:Ijiraq-discovery-CFHT.gif|frameless|upright=0.3|center]] || 13.2 || {{sort|13|≈&thinsp;{{val|13}}}}|| {{sort|1.8|≈&thinsp;{{val|1.8}}}} || {{val|11344700}} || {{sort|451.12|+{{val|451.12}}}} || 49.2 || 0.293 || Inuit group (Kiviuq) || 2000 || 2000 || Gladman et al.
|- id="S/2019 S 24" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 24</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11360500}} || {{sort|452.07|+{{val|452.07}}}} || 46.7 || 0.345 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al.
|- id="S/2007 S 10" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2007 S 10</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|11364900}} || {{sort|452.36|+{{val|452.36}}}} || 45.8 || 0.367 || Inuit group (Kiviuq) || 2007 || 2025 || Sheppard et al.
|- id="S/2019 S 26" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 26</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11390900}} || {{sort|453.89|+{{val|453.89}}}} || 48.1 || 0.365 || Inuit group (Kiviuq) || 2019 || 2025 || Ashton et al.
|- id="S/2020 S 13" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 13</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11415600}} || {{sort|455.39|+{{val|455.39}}}} || 48.0 || 0.373 || Inuit group (Kiviuq) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 50" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 50</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11656500}} || {{sort|469.82|−{{val|469.82}}}} || 166.1 || 0.263 || [[Norse group]] (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 6" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 6</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|11953100}} || {{sort|487.91|+{{val|487.91}}}} || 47.4 || 0.336 || Inuit group (Kiviuq) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 7" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 7</small> || ― || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|12133700}} || {{sort|499.01|+{{val|499.01}}}} || 44.7 || 0.284 || Inuit group (Kiviuq) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 38" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 38</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|12823500}} || {{sort|546.31|−{{val|546.31}}}} || 149.2 || 0.909 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al.
|- id="Phoebe" style="background:#d3d3d3;"
| {{sort|09|IX}} || {{hid|Phoebe}} ‡[[Phoebe (moon)|Phoebe]] || {{IPAc-en|ˈ|f|iː|b|i}} || style="background:black;"| [[File:Phoebe cassini full.jpg|frameless|upright=0.3|center|alt=An approximately spherical heavily cratered body is illuminated from the bottom-right. The terminator runs near the left and top limbs. There is huge crater at the top, which affects the shape, and another slightly smaller at the bottom.]] || 6.7 || {{sort|213.0|213.0<br>(219&thinsp;×&thinsp;217&thinsp;×&thinsp;204)}} || {{val|8312.3}} || {{val|12929400}} || {{sort|550.30|{{val|−550.30}}}} || 175.2 || 0.164 || Norse group (Phoebe) || 1898 || 1899 || [[William Henry Pickering|Pickering]]
|- id="S/2023 S 9" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 9</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|13167500}} || {{sort|564.11|−{{val|564.11}}}} || 172.2 || 0.141 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2006 S 20" style="background:#d3d3d3;"
| {{sort|Zzzc|}} || {{hid|S/2006N}} ‡<small>[[S/2006 S 20]]</small> || — || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|13193700}} || {{sort|565.79|{{val|−565.79}}}} || 173.1 || 0.206 || Norse group (Phoebe) || 2006 || 2023 || Sheppard et al.
|- id="S/2004 S 56" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 56</small> || ― || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|13670200}} || {{sort|596.69|−{{val|596.69}}}} || 161.6 || 0.339 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al.
|- id="S/2023 S 8" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 8</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14018800}} || {{sort|619.69|−{{val|619.69}}}}|| 166.9 || 0.122 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 11" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 11</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14046100}} || {{sort|621.49|−{{val|621.49}}}} || 170.9 || 0.300 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2006 S 9" style="background:#d3d3d3;"
| {{sort|T|}} || {{hid|S/2006C}} ‡<small>[[S/2006 S 9]]</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14406700}} || {{sort|645.58|{{val|−645.58}}}} || 173.0 || 0.249 || Norse group (Phoebe) || 2006 || 2023 || Sheppard et al.
|- id="S/2006 S 21" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 21</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|14976500}} || {{sort|684.28|−{{val|684.28}}}} || 169.8 || 0.204 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al.
|- id="Paaliaq" style="background:#F4C2C2;"
| {{sort|20|XX}} || {{hid|Paaliaq}} ♦[[Paaliaq]] || {{IPAc-en|ˈ|p|ɑː|l|i|ɒ|k}} || style="background:black;"| [[File:Paaliaq-CFHT.gif|frameless|upright=0.3|center]] || 11.7 || {{sort|25|≈&thinsp;25<ref>{{Cite web|url=https://tilmanndenk.de/outersaturnianmoons/paaliaq/|title=Paaliaq (S/2000 S 2) – Tilmann Denk}}</ref>}}|| {{sort|14|≈&thinsp;{{val|14}}}} || {{val|14997700}} || {{sort|685.72|+{{val|685.72}}}} || 48.5 || 0.378 || Inuit group{{refn|group=lower-alpha|The moon has a similar inclination, but a significantly different semi-major axis. Therefore, it is uncertain whether it comes from the same parent body as the rest of the Inuit group.<ref name="Ashton2025a"/>}} || 2000 || 2000 || Gladman et al.
|- id="S/2006 S 22" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 22</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15109500}} || {{sort|693.41|−{{val|693.41}}}} || 172.0 || 0.246 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al.
|- id="S/2023 S 13" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 13</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15193000}} || {{sort|699.18|−{{val|699.18}}}} || 168.5 || 0.179 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 10" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 10</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15500200}} || {{sort|720.49|−{{val|720.49}}}} || 163.0 || 0.302 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="Skathi" style="background:#d3d3d3;"
| {{sort|27|XXVII}} || {{hid|Skathi}} ‡[[Skathi (moon)|Skathi]] || {{IPAc-en|ˈ|s|k|ɑː|ð|i}} || style="background:black;"| [[File:Skathi-discovery-CFHT.gif|frameless|upright=0.3|center]] || 14.3 || {{sort|8|≈&thinsp;8}} || {{sort|0.38|≈&thinsp;{{val|0.38}}}} || {{val|15575400}} || {{sort|725.73|{{val|−725.73}}}} || 151.6 || 0.281 || Norse group (low-inclination) || 2000 || 2000 || Gladman et al.
|- id="S/2023 S 12" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 12</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|15805900}} || {{sort|741.92|−{{val|741.92}}}} || 168.8 || 0.601 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2007 S 5" style="background:#d3d3d3;"
| {{sort|U|}} || {{hid|S/2007C}} ‡<small>[[S/2007 S 5]]</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|15835600}} || {{sort|744.01|{{val|−744.01}}}} || 158.4 || 0.104 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al.
|- id="S/2007 S 7" style="background:#d3d3d3;"
| {{sort|Zzb|}} || {{hid|S/2007E}} ‡<small>S/2007 S 7</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|15931600}} || {{sort|750.80|{{val|−750.80}}}} || 169.3 || 0.217 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al.
|- id="S/2007 S 2" style="background:#d3d3d3;"
| {{sort|O|}} || {{hid|S/2007A}} ‡<small>[[S/2007 S 2]]</small> || —|| style="background:black;"| || 15.6 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|15939100}} || {{sort|751.33|{{val|−751.33}}}} || 174.0 || 0.232 || Norse group (Phoebe) || 2007 || 2007 || Sheppard et al.
|- id="S/2004 S 37" style="background:#d3d3d3;"
| {{sort|K|}} || {{hid|S/2004T}} ‡<small>[[S/2004 S 37]]</small> || —|| style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|15956300}} || {{sort|752.55|{{val|−752.55}}}} || 158.2 || 0.448 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2004 S 47" style="background:#d3d3d3;"
| {{sort|Zu|}} || {{hid|S/2004Zd}} ‡<small>S/2004 S 47</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|16050700}} || {{sort|759.22|{{val|−759.22}}}} || 160.9 || 0.291 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2004 S 40" style="background:#d3d3d3;"
| {{sort|V|}} || {{hid|S/2004W}} ‡<small>S/2004 S 40</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|16075600}} || {{sort|761.00|{{val|−761.00}}}} || 169.2 || 0.297 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2020 S 14" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 14</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16186200}} || {{sort|768.86|−{{val|768.86}}}} || 161.7 || 0.313 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 27" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 27</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16267000}} || {{sort|774.63|−{{val|774.63}}}} || 162.1 || 0.420 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="Albiorix" style="background:#FDD5B1;"
| {{sort|26|XXVI}} || {{hid|Albiorix}} ♣[[Albiorix (moon)|Albiorix]] || {{IPAc-en|ˌ|æ|l|b|i|ˈ|ɒr|ɪ|k|s}} || style="background:black;"| [[File:Albiorix_WISE-W4.jpg|frameless|upright=0.3|center]] || 11.2 || 28.6 || {{sort|12|≈&thinsp;{{val|12}}}} || {{val|16329200}} || {{sort|779.07|+{{val|779.07}}}} || 36.8 || 0.482 || [[Gallic group]] || 2000 || 2000 || [[Matthew J. Holman|Holman]]
|- id="S/2019 S 2" style="background:#d3d3d3;"
| {{sort|W|}} || {{hid|S/2019B}} ‡<small>[[S/2019 S 2]]</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16560300}} || {{sort|795.67|{{val|−795.67}}}} || 173.3 || 0.279 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al.
|- id="S/2020 S 15" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2020 S 15</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16729200}} || {{sort|807.82|+{{val|807.82}}}} || 37.1 || 0.462 || Gallic group || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 14" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 14</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16853000}} || {{sort|816.86|−{{val|816.86}}}} || 171.6 || 0.497 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 16" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 16</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|16963400}} || {{sort|824.92|−{{val|824.92}}}} || 167.3 || 0.405 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 16" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 16</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17005300}} || {{sort|827.91|−{{val|827.81}}}} || 162.6 || 0.270 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="Bebhionn" style="background:#FDD5B1;"
| {{sort|37|XXXVII}} || {{hid|Bebhionn}} ♣[[Bebhionn (moon)|Bebhionn]] || {{IPAc-en|ˈ|b|eɪ|v|ɪ|n}} || style="background:black;"| [[File:Bebhionn-cassini.png|frameless|upright=0.3|center]] || 15.0 || {{sort|6|≈&thinsp;6}} || {{sort|0.18|≈&thinsp;{{val|0.18}}}} || {{val|17027300}} || {{sort|829.64|+{{val|829.64}}}} || 38.6 || 0.459 || Gallic group || 2004 || 2005 || Sheppard et al.
|- id="S/2007 S 8" style="background:#FDD5B1;"
| {{sort|Zzc|}} || {{hid|S/2007F}} ♣<small>[[S/2007 S 8]]</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17048900}} || {{sort|831.21|+{{val|831.21}}}} || 36.2 || 0.490 || Gallic group || 2007 || 2023 || Sheppard et al.
|- id="Saturn LX" style="background:#FDD5B1;"
| {{sort|60|[[Saturn LX|LX]]}} || {{hid|S/2004M}} ♣<small>[[S/2004 S 29]]</small> || —|| style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|17063900}} || {{sort|832.27|+{{val|832.27}}}} || 38.6 || 0.485 || Gallic group || 2004 || 2019 || Sheppard et al.
|- id="S/2019 S 3" style="background:#d3d3d3;"
| {{sort|X|}} || {{hid|S/2019C}} ‡<small>S/2019 S 3</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17077400}} || {{sort|833.19|{{val|−833.19}}}} || 166.9 || 0.248 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="S/2020 S 17" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 17</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17094200}} || {{sort|834.45|−{{val|834.45}}}} || 148.9 || 0.378 || Norse group (low-inclination) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 20" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 20</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17261000}} || {{sort|846.77|−{{val|846.77}}}} || 136.5 || 0.442 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al.
|- id="S/2019 S 29" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2019 S 29</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17353900}} || {{sort|853.62|+{{val|853.62}}}} || 37.7 || 0.441 || Gallic group || 2019 || 2025 || Ashton et al.
|- id="S/2023 S 18" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2023 S 18</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17381700}} || {{sort|855.65|+{{val|855.65}}}} || 36.7 || 0.448 || Gallic group || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 17" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2023 S 17</small> || ― || style="background:black;"| || 17.1 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17385300}} || {{sort|855.94|+{{val|855.94}}}} || 35.9 || 0.498 || Gallic group || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 7" style="background:#d3d3d3;"
| {{sort|Zzd|}} || {{hid|S/2020G}} ‡<small>[[S/2020 S 7]]</small> || — || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17394000}} || {{sort|856.53|{{val|−856.53}}}} || 161.4 || 0.500 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al.
|- id="S/2007 S 11" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2007 S 11</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17434400}} || {{sort|859.53|+{{val|859.53}}}} || 35.5 || 0.499 || Gallic group || 2007 || 2025 || Sheppard et al.
|- id="S/2019 S 28" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 28</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17496000}} || {{sort|864.09|−{{val|864.09}}}} || 158.4 || 0.199 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2004 S 31" style="background:#F4C2C2;"
| {{sort|I|}} || {{hid|S/2004O}} ♦<small>[[S/2004 S 31]]</small> || —|| style="background:black;"| || 15.6 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|17497100}} || {{sort|863.92|+{{val|863.92}}}} || 48.0 || 0.159 || Inuit group (Siarnaq) || 2004 || 2019 || Sheppard et al.
|- id="Erriapus" style="background:#FDD5B1;"
| {{sort|28|XXVIII}} || {{hid|Erriapus}} ♣[[Erriapus]] || {{IPAc-en|ɛ|r|i|ˈ|æ|p|ə|s}} || style="background:black;"| [[File:Erriapus-discovery-CFHT.gif|frameless|upright=0.3|center]] || 13.7 || {{sort|10|≈&thinsp;10}} || {{sort|0.95|≈&thinsp;{{val|0.95}}}} || {{val|17506900}} || {{sort|864.92|+{{val|864.92}}}} || 37.1 || 0.475 || Gallic group || 2000 || 2000 || Gladman et al.
|- id="S/2023 S 19" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 19</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17590300}} || {{sort|870.92|+{{val|870.92}}}} || 48.2 || 0.092 || Inuit group (Siarnaq) || 2023 || 2025 || Ashton et al.
|- id="Skoll" style="background:#d3d3d3;"
| {{sort|47|XLVII}} || {{hid|Skoll}} ‡[[Skoll (moon)|Skoll]] || {{IPAc-en|ˈ|s|k|ɒ|l}} || style="background:black;"| [[File:Skoll-Cassini.png|frameless|upright=0.3|center]] || 15.4 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|17623400}} || {{sort|873.57|{{val|−873.57}}}} || 159.4 || 0.463 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al.
|- id="S/2023 S 3" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 3</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17646400}} || {{sort|875.00|+{{val|875.00}}}} || 46.9 || 0.178 || Inuit group (Siarnaq) || 2023 || 2025 || Ashton et al.
|- id="S/2019 S 30" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 30</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17709900}} || {{sort|879.97|−{{val|879.97}}}} || 168.3 || 0.107 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2020 S 19" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2020 S 19</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17726700}} || {{sort|881.04|+{{val|881.04}}}} || 48.1 || 0.159 || Inuit group (Siarnaq) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 31" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2019 S 31</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17739100}} || {{sort|882.24|+{{val|882.24}}}} || 39.8 || 0.488 || Gallic group || 2019 || 2025 || Ashton et al.
|- id="Tarqeq" style="background:#F4C2C2;"
| {{sort|52|LII}} || {{hid|Tarqeq}} ♦[[Tarqeq]] || {{IPAc-en|ˈ|t|ɑːr|k|eɪ|k}} ||style="background:black;"| [[File:Tarqeq-cassini.png|frameless|upright=0.3|center]] || 14.8 || {{sort|7|≈&thinsp;7}}|| {{sort|0.18|≈&thinsp;{{val|0.18}}}} || {{val|17751000}} || {{sort|882.85|+{{val|882.85}}}} || 48.7 || 0.144 || Inuit group (Siarnaq) || 2007 || 2007 || Sheppard et al.
|- id="S/2023 S 21" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 21</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17755400}} || {{sort|883.31|−{{val|883.31}}}} || 157.3 || 0.077 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 4" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 4</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17764600}} || {{sort|884.11|−{{val|884.11}}}} || 170.0 || 0.276 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 18" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 18</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17777900}} || {{sort|885.12|−{{val|885.12}}}} || 168.9 || 0.180 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 14" style="background:#F4C2C2;"
| {{sort|Zze|}} || {{hid|S/2019N}} ♦<small>[[S/2019 S 14]]</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|17852800}} || {{sort|893.15|+{{val|890.59}}}} || 46.2 || 0.172 || Inuit group (Siarnaq) || 2019 || 2023 || Ashton et al.
|- id="S/2020 S 2" style="background:#d3d3d3;"
| {{sort|Y|}} || {{hid|S/2020B}} ‡<small>S/2020 S 2</small> || — || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17869000}} || {{sort|891.86|{{val|−891.86}}}} || 170.7 || 0.152 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al.
|- id="Siarnaq" style="background:#F4C2C2;"
| {{sort|29|XXIX}} || {{hid|Siarnaq}} ♦[[Siarnaq]] || {{IPAc-en|ˈ|s|iː|ɑːr|n|ə|k}} || style="background:black;"| [[File:Siarnaq-discovery-CFHT.gif|frameless|upright=0.3|center]] || 10.6 || 39.3 || {{sort|32|≈&thinsp;{{val|32}}}} || {{val|17881100}} || {{sort|892.68|+{{val|892.68}}}} || 47.8 || 0.308 || Inuit group (Siarnaq) || 2000 || 2000 || Gladman et al.
|- id="S/2019 S 4" style="background:#d3d3d3;"
| {{sort|Za|}} || {{hid|S/2019D}} ‡<small>S/2019 S 4</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17951900}} || {{sort|898.09|{{val|−898.09}}}} || 170.1 || 0.408 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="S/2019 S 32" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2019 S 32</small> || ― || style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|17960500}} || {{sort|898.71|+{{val|898.71}}}} || 46.2 || 0.276 || Inuit group (Siarnaq) || 2019 || 2025 || Ashton et al.
|- id="S/2020 S 20" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 20</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|17997300}} || {{sort|901.53|−{{val|901.53}}}} || 169.8 || 0.133 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2020 S 3" style="background:#F4C2C2;"
| {{sort|Z|}} || {{hid|S/2020C}} ♦<small>[[S/2020 S 3]]</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18056800}} || {{sort|905.84|+{{val|905.84}}}} || 46.0 || 0.142 || Inuit group (Siarnaq) || 2020 || 2023 || Ashton et al.
|- id="S/2004 S 41" style="background:#d3d3d3;"
| {{sort|Zb|}} || {{hid|S/2004X}} ‡<small>S/2004 S 41</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18095400}} || {{sort|908.89|{{val|−908.89}}}} || 165.7 || 0.301 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2005 S 6" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2005 S 6</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18107300}} || {{sort|909.58|+{{val|909.58}}}} || 47.7 || 0.084 || Inuit group (Siarnaq) || 2005 || 2025 || Sheppard et al.
|- id="S/2004 S 57" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 57</small> || ― || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18150500}} || {{sort|913.07|−{{val|913.07}}}} || 167.9 || 0.263 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al.
|- id="S/2019 S 6" style="background:#F4C2C2;"
| {{sort|Zn|}} || {{hid|S/2019F}} ♦<small>[[S/2019 S 6]]</small> || — || style="background:black;" | || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|18205600}} || {{sort|917.11|+{{val|917.11}}}} || 46.4 || 0.120 || Inuit group (Siarnaq)|| 2019 || 2023 || Ashton et al.
|- id="S/2006 S 24" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 24</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18210700}} || {{sort|917.56|−{{val|917.56}}}} || 165.9 || 0.352 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al.
|- id="Tarvos" style="background:#FDD5B1;"
| {{sort|21|XXI}} || {{hid|Tarvos}} ♣[[Tarvos (moon)|Tarvos]] || {{IPAc-en|ˈ|t|ɑːr|v|ə|s}} || style="background:black;"| [[File:Tarvos discovery.gif|frameless|upright=0.3|center]] || 13.1 || {{sort|15|≈&thinsp;15}} || {{sort|2.1|≈&thinsp;{{val|2.1}}}} || {{val|18216600}} || {{sort|917.98|+{{val|917.98}}}} || 37.8 || 0.522 || Gallic group || 2000 || 2000 || Gladman et al.
|- id="S/2020 S 4" style="background:#FDD5B1;"
| {{sort|Zc|}} || {{hid|S/2020D}} ♣<small>[[S/2020 S 4]]</small> || — || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18236400}} || {{sort|919.52|+{{val|919.52}}}} || 40.1 || 0.496 || Gallic group || 2020 || 2023 || Ashton et al.
|- id="S/2023 S 30" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 30</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18238300}} || {{sort|919.71|−{{val|919.71}}}} || 142.4 || 0.493 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al.
|- id="S/2004 S 42" style="background:#d3d3d3;"
| {{sort|Zf|}} || {{hid|S/2004Y}} ‡<small>S/2004 S 42</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18240700}} || {{sort|919.88|{{val|−919.88}}}} || 165.7 || 0.158 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2023 S 15" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 15</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18241300}} || {{sort|919.93|−{{val|919.93}}}} || 161.9 || 0.549 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2004 S 58" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2004 S 58</small> || ― || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|18254500}} || {{sort|920.80|+{{val|920.80}}}} || 45.7 || 0.249 || Inuit group (Siarnaq) || 2004 || 2025 || Sheppard et al.
|- id="S/2006 S 23" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2006 S 23</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18269700}} || {{sort|921.86|+{{val|921.86}}}} || 43.8 || 0.190 || Inuit group (Siarnaq) || 2006 || 2025 || Sheppard et al.
|- id="Hyrrokkin" style="background:#d3d3d3;"
| {{sort|44|XLIV}} || {{hid|Hyrrokkin}} ‡[[Hyrrokkin (moon)|Hyrrokkin]] || {{IPAc-en|h|ɪ|ˈ|r|ɒ|k|ə|n}} ||style="background:black;"| [[File:Hyrrokkin-cassini.png|frameless|upright=0.3|center]] || 14.3 || {{sort|8|≈&thinsp;8}} || {{sort|0.38|≈&thinsp;{{val|0.38}}}} || {{val|18340900}} || {{sort|927.46|{{val|−927.46}}}} || 149.9 || 0.336 || Norse group (low-inclination) || 2004 || 2005 || Sheppard et al.
|- id="S/2023 S 24" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 24</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18351800}} || {{sort|928.25|−{{val|928.25}}}} || 169.7 || 0.374 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="Greip" style="background:#d3d3d3;"
| {{sort|51|LI}} || {{hid|Greip}} ‡[[Greip (moon)|Greip]] || {{IPAc-en|ˈ|ɡ|r|eɪ|p}} || style="background:black;"| [[File:Greip-cassini.png|frameless|upright=0.3|center]] || 15.3 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|18380000}} || {{sort|930.44|{{val|−930.44}}}} || 174.2 || 0.317 || Norse group (Phoebe){{refn|group=lower-alpha|name="Phoebe/Mundilfari"|The moon has been identified as potentially belonging to the Mundilfari subgroup due to its inclination and semi-major axis.<ref name="Ashton2025a"/>}} || 2006 || 2006 || Sheppard et al.
|- id="S/2020 S 5" style="background:#F4C2C2;"
| {{sort|Zc|}} || {{hid|S/2020E}} ♦<small>[[S/2020 S 5]]</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18391000}} || {{sort|931.19|+{{val|931.19}}}} || 48.2 || 0.220 || Inuit group (Siarnaq) || 2020 || 2023 || Ashton et al.
|- id="S/2019 S 34" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2019 S 34</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18446800}} || {{sort|935.45|+{{val|935.45}}}} || 37.6 || 0.536 || Gallic group || 2019 || 2025 || Ashton et al.
|- id="S/2004 S 13" style="background:#d3d3d3;"
| {{sort|D|}} || {{hid|S/2004C}} ‡<small>[[S/2004 S 13]]</small> || —|| style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18453700}} || {{sort|936.09|{{val|−936.09}}}} || 169.0 || 0.265 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2005 S 7" style="background:#fdd5b1;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♣<small>S/2005 S 7</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18502500}} || {{sort|939.75|+{{val|939.75}}}} || 34.6 || 0.565 || Gallic group || 2005 || 2025 || Sheppard et al.
|- id="S/2007 S 6" style="background:#d3d3d3;"
| {{sort|Ze|}} || {{hid|S/2007D}} ‡<small>S/2007 S 6</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18545000}} || {{sort|942.98|{{val|−942.98}}}} || 166.5 || 0.168 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al.
|- id="S/2019 S 35" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 35</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18557800}} || {{sort|944.00|−{{val|944.00}}}} || 157.3 || 0.577 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2006 S 25" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 25</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18572400}} || {{sort|945.07|−{{val|945.07}}}} || 158.8 || 0.303 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al.
|- id="S/2023 S 22" style="background:#f4c2c2;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ♦<small>S/2023 S 22</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18577500}} || {{sort|945.37|+{{val|945.37}}}} || 47.5 || 0.182 || Inuit group (Siarnaq) || 2023 || 2025 || Ashton et al.
|- id="Mundilfari" style="background:#d3d3d3;"
| {{sort|25|XXV}} || {{hid|Mundilfari}} ‡[[Mundilfari (moon)|Mundilfari]] || {{IPAc-en|m|ʊ|n|d|əl|ˈ|v|ær|i}} || style="background:black;"| [[File:Mundilfari-discovery-CFHT.gif|frameless|upright=0.3|center]] || 14.5 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|18588200}} || {{sort|946.29|{{val|−946.29}}}} || 167.1 || 0.211 || Norse group (Mundilfari) || 2000 || 2000 || Gladman et al.
|- id="S/2006 S 26" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 26</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18619300}} || {{sort|948.67|−{{val|948.67}}}} || 171.9 || 0.248 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al.
|- id="S/2019 S 33" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 33</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18696100}} || {{sort|954.53|−{{val|954.53}}}} || 170.4 || 0.289 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2006 S 1" style="background:#d3d3d3;"
| {{sort|M|}} || {{hid|S/2006A}} ‡<small>[[S/2006 S 1]]</small> || —||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|18746300}} || {{sort|958.32|{{val|−958.32}}}} || 156.1 || 0.105 || Norse group (Kari) || 2006 || 2006 || Sheppard et al.
|- id="S/2023 S 23" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 23</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18783700}} || {{sort|961.22|−{{val|961.22}}}} || 164.8 || 0.350 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 21" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 21</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18862100}} || {{sort|967.26|−{{val|967.26}}}} || 169.9 || 0.307 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2004 S 43" style="background:#d3d3d3;"
| {{sort|Zi|}} || {{hid|S/2004Z}} ‡<small>[[S/2004 S 43]]</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|18935700}} || {{sort|972.85|{{val|−972.85}}}} || 171.1 || 0.432 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2006 S 10" style="background:#d3d3d3;"
| {{sort|Zg|}} || {{hid|S/2006D}} ‡<small>S/2006 S 10</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|18979900}} || {{sort|976.34|{{val|−976.34}}}} || 161.6 || 0.151 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al.
|- id="S/2019 S 5" style="background:#d3d3d3;"
| {{sort|Zh|}} || {{hid|S/2019E}} ‡<small>S/2019 S 5</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19090100}} || {{sort|984.87|{{val|−984.87}}}} || 158.8 || 0.216 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="S/2023 S 25" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 25</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19136600}} || {{sort|988.53|−{{val|988.53}}}} || 166.4 || 0.281 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2004 S 59" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 59</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19170700}} || {{sort|991.18|−{{val|991.18}}}} || 167.3 || 0.262 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al.
|- id="S/2006 S 27" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 27</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19205700}} || {{sort|993.79|−{{val|993.79}}}} || 170.5 || 0.140 || Norse group (Mundilfari) || 2006 || 2025 || Sheppard et al.
|- id="Gridr" style="background:#d3d3d3;"
| {{sort|54|LIV}} || {{hid|Gridr}} ‡[[Gridr (moon)|Gridr]] || {{IPAc-en|ˈ|g|r|i:|D|@r}} ||style="background:black;"| || 15.8 || {{sort|4|≈&thinsp;4}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19250600}} || {{sort|997.33|{{val|−997.33}}}} || 163.9 || 0.187 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="Bergelmir" style="background:#d3d3d3;"
| {{sort|38|XXXVIII}} || {{hid|Bergelmir}} ‡[[Bergelmir (moon)|Bergelmir]] || {{IPAc-en|b|ɛər|ˈ|j|ɛ|l|m|ɪər}} || style="background:black;"| [[File:Bergelmir.png|frameless|upright=0.3|center]] || 15.2 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|19268100}} || {{sort|998.62|{{val|−998.62}}}} || 158.8 || 0.145 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="Jarnsaxa" style="background:#d3d3d3;"
| {{sort|50|L}} || {{hid|Jarnsaxa}} ‡[[Jarnsaxa (moon)|Jarnsaxa]] || {{IPAc-en|j|ɑːr|n|ˈ|s|æ|k|s|ə}} ||style="background:black;"| || 15.6 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19273500}} || {{sort|999.13|{{val|−999.13}}}} || 163.0 || 0.218 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al.
|- id="Narvi" style="background:#d3d3d3;"
| {{sort|31|XXXI}} || {{hid|Narvi}} ‡[[Narvi (moon)|Narvi]] || {{IPAc-en|ˈ|n|ɑːr|v|i}} || style="background:black;"| [[File:Narvi.jpg|frameless|upright=0.3|center]] || 14.5 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|19285000}} || {{sort|999.94|{{val|−999.94}}}} || 142.2 || 0.441 || Norse group (low-inclination) || 2003 || 2003 || Sheppard et al.
|- id="S/2023 S 44" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 44</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19292400}} || {{sort|1000.47|−{{val|1000.47}}}} || 167.4 || 0.434 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="Suttungr" style="background:#d3d3d3;"
| {{sort|23|XXIII}} || {{hid|Suttungr}} ‡[[Suttungr (moon)|Suttungr]] || {{IPAc-en|ˈ|s|ʊ|t|ʊ|ŋ|ɡ|ər}} ||style="background:black;"| [[File:Suttungr-discovery-CFHT.gif|frameless|upright=0.3|center]] || 14.5 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|19391900}} || {{sort|1008.25|{{val|−1008.25}}}} || 175.7 || 0.116 || Norse group (Phoebe) || 2000 || 2000 || Gladman et al.
|- id="S/2020 S 22" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 22</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19443000}} || {{sort|1012.24|−{{val|1012.24}}}} || 161.3 || 0.059 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2004 S 44" style="background:#d3d3d3;"
| {{sort|Zj|}} || {{hid|S/2004Za}} ‡<small>S/2004 S 44</small> || — || style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19515400}} || {{sort|1017.91|{{val|−1017.91}}}} || 167.7 || 0.129 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2004 S 60" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 60</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19517000}} || {{sort|1018.13|−{{val|1018.13}}}} || 173.8 || 0.280 || Norse group (Phoebe) || 2004 || 2025 || Sheppard et al.
|- id="S/2006 S 12" style="background:#FDD5B1;"
| {{sort|Zm|}} || {{hid|S/2006F}} ♣<small>[[S/2006 S 12]]</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19570300}} || {{sort|1022.29|+{{val|1022.29}}}} || 38.6 || 0.542 || Gallic group{{refn|group=lower-alpha|Sheppard et al. suggested in 2023 that the moon's identification with the Gallic group is uncertain,<ref name="Sheppard2023"/> but a later study from Ashton et al considers it confidently Gallic and associated with [[Albiorix (moon)|Albiorix]], unlike [[S/2004 S 24]].<ref name="Ashton2025a"/>}} || 2006 || 2023 || Sheppard et al.
|- id="S/2007 S 3" style="background:#d3d3d3;"
| {{sort|P|}} || {{hid|S/2007B}} ‡<small>[[S/2007 S 3]]</small> || —||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|19614400}} || {{sort|1025.70|{{val|−1025.70}}}} || 173.8 || 0.150 || Norse group (Phoebe) || 2007 || 2007 || Sheppard et al.
|- id="S/2004 S 45" style="background:#d3d3d3;"
| {{sort|Zk|}} || {{hid|S/2004Zb}} ‡<small>S/2004 S 45</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19693700}} || {{sort|1031.86|{{val|−1031.86}}}} || 154.0 || 0.551 || Norse group (Kari) || 2004 || 2023 || Sheppard et al.
|- id="Hati" style="background:#d3d3d3;"
| {{sort|43|XLIII}} || {{hid|Hati}} ‡[[Hati (moon)|Hati]] || {{IPAc-en|ˈ|h|ɑː|t|i}} || style="background:black;"| [[File:Hati-cassini.png|frameless|upright=0.3|center]] || 15.4 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|19695000}} || {{sort|1032.02|{{val|−1032.02}}}} || 165.4 || 0.372 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2004 S 17" style="background:#d3d3d3;"
| {{sort|E|}} || {{hid|S/2004D}} ‡<small>[[S/2004 S 17]]</small> || —||style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19699000}} || {{sort|1032.37|{{val|−1032.37}}}} || 167.9 || 0.162 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2006 S 11" style="background:#d3d3d3;"
| {{sort|Zl|}} || {{hid|S/2006E}} ‡<small>S/2006 S 11</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19711900}} || {{sort|1033.35|{{val|−1033.35}}}} || 174.1 || 0.143 || Norse group (Phoebe) || 2004 || 2023 || Sheppard et al.
|- id="S/2004 S 12" style="background:#d3d3d3;"
| {{sort|C|}} || {{hid|S/2004B}} ‡<small>[[S/2004 S 12]]</small> || —||style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19801000}} || {{sort|1040.39|{{val|−1040.39}}}} || 164.7 || 0.337 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2020 S 23" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 23</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19801500}} || {{sort|1040.38|−{{val|1040.38}}}} || 165.0 || 0.089 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 27" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 27</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19820100}} || {{sort|1041.85|−{{val|1041.85}}}} || 151.1 || 0.652 || Norse group (Kari) || 2023 || 2025 || Ashton et al.
|- id="Eggther" style="background:#d3d3d3;"
| {{sort|59|LIX}} || {{hid|Eggther}} ‡[[Eggther (moon)|Eggther]] || {{IPAc-en|ˈ|E|g|T|E@r}} ||style="background:black;"| || 15.4 || {{sort|6|≈&thinsp;6}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|19844600}} || {{sort|1043.80|{{val|−1043.80}}}} || 165.0 || 0.157 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2023 S 28" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 28</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19881000}} || {{sort|1046.56|−{{val|1046.56}}}} || 168.7 || 0.575 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 37" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 37</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19889800}} || {{sort|1047.39|−{{val|1047.39}}}} || 172.3 || 0.215 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 26" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 26</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19894300}} || {{sort|1047.76|−{{val|1047.76}}}} || 163.9 || 0.306 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2019 S 36" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 36</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19903200}} || {{sort|1048.42|−{{val|1048.42}}}} || 166.9 || 0.161 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2006 S 13" style="background:#d3d3d3;"
| {{sort|Zo|}} || {{hid|S/2006G}} ‡<small>S/2006 S 13</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|19953300}} || {{sort|1052.32|{{val|−1052.32}}}} || 162.0 || 0.313 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al.
|- id="S/2019 S 37" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 37</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|19996900}} || {{sort|1055.78|−{{val|1055.78}}}} || 149.9 || 0.404 || Norse group (low-inclination) || 2019 || 2025 || Ashton et al.
|- id="S/2023 S 48" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 48</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20029200}} || {{sort|1058.35|−{{val|1058.35}}}} || 169.7 || 0.022 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 29" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 29</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20042400}} || {{sort|1059.42|−{{val|1059.42}}}} || 172.2 || 0.141 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2007 S 9" style="background:#d3d3d3;"
| {{sort|Zzy|}} || {{hid|S/2007G}} ‡<small>S/2007 S 9</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20174600}} || {{sort|1069.81|{{val|−1069.81}}}} || 159.3 || 0.360 || Norse group (Mundilfari) || 2007 || 2023 || Sheppard et al.
|- id="S/2019 S 7" style="background:#d3d3d3;"
| {{sort|Zp|}} || {{hid|S/2019G}} ‡<small>S/2019 S 7</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20185100}} || {{sort|1070.80|{{val|−1070.80}}}} || 174.2 || 0.233 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al.
|- id="S/2019 S 8" style="background:#d3d3d3;"
| {{sort|Zq|}} || {{hid|S/2019H}} ‡<small>S/2019 S 8</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20287400}} || {{sort|1078.86|{{val|−1078.86}}}} || 172.8 || 0.311 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al.
|- id="Farbauti" style="background:#d3d3d3;"
| {{sort|40|XL}} || {{hid|Farbauti}} ‡[[Farbauti (moon)|Farbauti]] || {{IPAc-en|f|ɑːr|ˈ|b|aʊ|t|i}} ||style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|20290700}} || {{sort|1079.12|{{val|−1079.12}}}} || 156.2 || 0.249 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="Thrymr" style="background:#d3d3d3;"
| {{sort|30|XXX}} || {{hid|Thrymr}} ‡[[Thrymr (moon)|Thrymr]] || {{IPAc-en|ˈ|θ|r|ɪ|m|ər}} || style="background:black;"| [[File:Thrymr-discovery-CFHT.gif|frameless|upright=0.3|center]] || 14.3 || {{sort|8|≈&thinsp;8}}|| {{sort|0.38|≈&thinsp;{{val|0.38}}}} || {{val|20330500}} || {{sort|1082.23|{{val|−1082.23}}}} || 175.0 || 0.467 || Norse group (Phoebe) || 2000 || 2000 || Gladman et al.
|- id="Bestla" style="background:#d3d3d3;"
| {{sort|39|XXXIX}} || {{hid|Bestla}} ‡[[Bestla (moon)|Bestla]] || {{IPAc-en|ˈ|b|ɛ|s|t|l|ə}} || style="background:black;"| [[File:Bestla-cassini.png|frameless|upright=0.3|center]] || 14.6 || {{sort|7|≈&thinsp;7}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|20337800}} || {{sort|1082.94|{{val|−1082.94}}}} || 138.3 || 0.486 || Norse group (low-inclination) || 2004 || 2005 || Sheppard et al.
|- id="S/2019 S 9" style="background:#d3d3d3;"
| {{sort|Zr|}} || {{hid|S/2019I}} ‡<small>S/2019 S 9</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20359700}} || {{sort|1084.62|{{val|−1084.62}}}} || 159.5 || 0.433 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="S/2023 S 32" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 32</small> || ― || style="background:black;"| || 17.2 || {{sort|2|≈&thinsp;2}} || {{sort|0.004|≈&thinsp;{{val|0.004}}}} || {{val|20454400}} || {{sort|1092.24|−{{val|1092.24}}}} || 169.8 || 0.037 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2004 S 46" style="background:#d3d3d3;"
| {{sort|Zs|}} || {{hid|S/2004Zc}} ‡<small>[[S/2004 S 46]]</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20513800}} || {{sort|1096.99|{{val|−1096.99}}}} || 177.2 || 0.249 || Norse group (Phoebe) || 2004 || 2023 || Sheppard et al.
|- id="Angrboda" style="background:#d3d3d3;"
| {{sort|55|LV}} || {{hid|Angrboda}} ‡[[Angrboda (moon)|Angrboda]] || {{IPAc-en|'|A:|N|g|@r|b|ou|D|@}} ||style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20591500}} || {{sort|1103.20|{{val|−1103.20}}}} || 177.7 || 0.216 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al.
|- id="S/2020 S 24" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 24</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20618300}} || {{sort|1105.41|−{{val|1105.41}}}} || 159.6 || 0.230 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 11" style="background:#d3d3d3;"
| {{sort|Zv|}} || {{hid|S/2019K}} ‡<small>[[S/2019 S 11]]</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20664200}} || {{sort|1109.11|{{val|−1109.11}}}} || 144.6 || 0.513 || Norse group (low-inclination) || 2019 || 2023 || Ashton et al.
|- id="Aegir" style="background:#d3d3d3;"
| {{sort|36|XXXVI}} || {{hid|Aegir}} ‡[[Aegir (moon)|Aegir]] || {{IPAc-en|ˈ|aɪ|.|ɪər}} ||style="background:black;"| || 15.5 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|20664400}} || {{sort|1109.13|{{val|−1109.13}}}} || 166.1 || 0.255 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2019 S 10" style="background:#d3d3d3;"
| {{sort|Zt|}} || {{hid|S/2019J}} ‡<small>S/2019 S 10</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20700300}} || {{sort|1111.99|{{val|−1111.99}}}} || 163.9 || 0.248 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="Beli" style="background:#d3d3d3;"
| {{sort|61|LXI}} || {{hid|Beli}} ‡[[Beli (moon)|Beli]] || {{IPAc-en|ˈ|b|i:|l|i}} ||style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}}|| {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20703700}} || {{sort|1112.27|{{val|−1112.27}}}} || 158.9 || 0.087 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2023 S 31" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 31</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20729200}} || {{sort|1114.29|−{{val|1114.29}}}} || 163.0 || 0.182 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 25" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 25</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20763700}} || {{sort|1117.09|−{{val|1117.09}}}} || 171.8 || 0.316 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 34" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 34</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20803900}} || {{sort|1120.38|−{{val|1120.38}}}} || 168.4 || 0.570 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2023 S 39" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 39</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20824500}} || {{sort|1121.99|−{{val|1121.99}}}} || 164.8 || 0.124 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2019 S 12" style="background:#d3d3d3;"
| {{sort|Zx|}} || {{hid|S/2019L}} ‡<small>S/2019 S 12</small> || — || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20895000}} || {{sort|1127.60|{{val|−1127.60}}}} || 167.1 || 0.476 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="Gerd" style="background:#d3d3d3;"
| {{sort|57|LVII}} || {{hid|Gerd}} ‡[[Gerd (moon)|Gerd]] || {{IPAc-en|ˈ|j|E@r|D}} ||style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}}|| {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20947500}} || {{sort|1131.91|{{val|−1131.91}}}} || 174.4 || 0.517 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al.
|- id="S/2019 S 13" style="background:#d3d3d3;"
| {{sort|Zz|}} || {{hid|S/2019M}} ‡<small>[[S/2019 S 13]]</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|20964500}} || {{sort|1133.27|{{val|−1133.27}}}} || 177.3 || 0.318 || Norse group (Phoebe) || 2019 || 2023 || Ashton et al.
|- id="S/2004 S 61" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2004 S 61</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|20986900}} || {{sort|1135.06|−{{val|1135.06}}}} || 168.4 || 0.466 || Norse group (Mundilfari) || 2004 || 2025 || Sheppard et al.
|- id="S/2006 S 14" style="background:#d3d3d3;"
| {{sort|Zw|}} || {{hid|S/2006H}} ‡<small>[[S/2006 S 14]]</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21062300}} || {{sort|1141.27|{{val|−1141.27}}}} || 166.7 || 0.060 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al.
|- id="S/2023 S 40" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 40</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21065100}} || {{sort|1141.48|−{{val|1141.48}}}} || 169.6 || 0.342 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="Gunnlod" style="background:#d3d3d3;"
| {{sort|62|LXII}} || {{hid|Gunnlod}} ‡[[Gunnlod (moon)|Gunnlod]] || {{IPAc-en|ˈ|g|U|n|l|Q|D}} ||style="background:black;"| || 15.7 || {{sort|4|≈&thinsp;4}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21141800}} || {{sort|1147.74|{{val|−1147.74}}}} || 160.4 || 0.251 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2019 S 15" style="background:#d3d3d3;"
| {{sort|Zzf|}} || {{hid|S/2019O}} ‡<small>S/2019 S 15</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21191100}} || {{sort|1151.66|{{val|−1151.66}}}} || 157.8 || 0.257 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="S/2020 S 6" style="background:#d3d3d3;"
| {{sort|Zy|}} || {{hid|S/2020F}} ‡<small>S/2020 S 6</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21253300}} || {{sort|1156.81|{{val|−1156.81}}}} || 166.9 || 0.480 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al.
|- id="S/2020 S 26" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 26</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21264400}} || {{sort|1157.77|−{{val|1157.77}}}} || 163.2 || 0.273 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 41" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 41</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21286400}} || {{sort|1159.52|−{{val|1159.52}}}} || 172.1 || 0.279 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2004 S 7" style="background:#d3d3d3;"
| {{sort|B|}} || {{hid|S/2004A}} ‡<small>[[S/2004 S 7]]</small> || —||style="background:black;"| || 15.5 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21327600}} || {{sort|1162.93|{{val|−1162.93}}}} || 164.8 || 0.511 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2006 S 3" style="background:#d3d3d3;"
| {{sort|N|}} || {{hid|S/2006B}} ‡<small>[[S/2006 S 3]]</small> || —||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21353100}} || {{sort|1165.02|{{val|−1165.02}}}} || 156.1 || 0.432 || Norse group (Kari) || 2006 || 2006 || Sheppard et al.
|- id="S/2005 S 5" style="background:#d3d3d3;"
| {{sort|Zzg|}} || {{hid|S/2005B}} ‡<small>[[S/2005 S 5]]</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21364900}} || {{sort|1165.96|{{val|−1165.96}}}} || 169.5 || 0.588 || Norse group (Mundilfari) || 2005 || 2023 || Sheppard et al.
|- id="Skrymir" style="background:#d3d3d3;"
| {{sort|56|LVI}} || {{hid|Skrymir}} ‡[[Skrymir (moon)|Skrymir]] || {{IPAc-en|ˈ|s|k|r|I|m|ɪər}} ||style="background:black;"| || 15.5 || {{sort|4|≈&thinsp;4}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21447400}} || {{sort|1172.72|{{val|−1172.72}}}} || 175.6 || 0.437 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al.
|- id="S/2023 S 33" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 33</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21621900}} || {{sort|1187.07|−{{val|1187.07}}}} || 155.8 || 0.665 || Norse group (Kari) || 2023 || 2025 || Ashton et al.
|- id="S/2006 S 16" style="background:#d3d3d3;"
| {{sort|Zzi|}} || {{hid|S/2006J}} ‡<small>S/2006 S 16</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21721200}} || {{sort|1195.13|{{val|−1195.13}}}} || 164.1 || 0.204 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al.
|- id="S/2023 S 49" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 49</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21766500}} || {{sort|1198.99|−{{val|1198.99}}}} || 171.7 || 0.026 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 30" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 30</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21790700}} || {{sort|1201.02|−{{val|1201.02}}}} || 154.2 || 0.601 || Norse group (Kari) || 2020 || 2025 || Ashton et al.
|- id="S/2006 S 15" style="background:#d3d3d3;"
| {{sort|Zzh|}} || {{hid|S/2006I}} ‡<small>S/2006 S 15</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|21799600}} || {{sort|1201.69|{{val|−1201.69}}}} || 161.1 || 0.117 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al.
|- id="S/2020 S 27" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 27</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21802300}} || {{sort|1202.02|−{{val|1202.02}}}} || 145.3 || 0.255 || Norse group (low-inclination) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 42" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 42</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21837000}} || {{sort|1204.81|−{{val|1204.81}}}} || 166.7 || 0.059 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2004 S 28" style="background:#d3d3d3;"
| {{sort|H|}} || {{hid|S/2004L}} ‡<small>[[S/2004 S 28]]</small> || — ||style="background:black;"| || 15.8 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21865900}} || {{sort|1207.18|{{val|−1207.18}}}} || 167.9 || 0.159 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2020 S 32" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 32</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21884100}} || {{sort|1208.85|−{{val|1208.85}}}} || 169.1 || 0.502 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2006 S 28" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 28</small> || ― || style="background:black;"| || 16.3 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|21955100}} || {{sort|1214.53|−{{val|1214.53}}}} || 172.9 || 0.210 || Norse group (Phoebe) || 2006 || 2025 || Sheppard et al.
|- id="S/2020 S 8" style="background:#d3d3d3;"
| {{sort|Zzl|}} || {{hid|S/2020H}} ‡<small>S/2020 S 8</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21967200}} || {{sort|1215.61|{{val|−1215.61}}}} || 161.8 || 0.252 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al.
|- id="S/2020 S 28" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 28</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21993700}} || {{sort|1217.81|−{{val|1217.81}}}} || 160.1 || 0.474 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="Alvaldi" style="background:#d3d3d3;"
| {{sort|65|LXV}} || {{hid|Alvaldi}} ‡[[Alvaldi (moon)|Alvaldi]] || {{IPAc-en|O:|l|ˈ|v|O:|l|d|i}} ||style="background:black;"| || 15.6 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|21993800}} || {{sort|1217.80|{{val|−1217.80}}}} || 177.4 || 0.238 || Norse group (Phoebe) || 2004 || 2019 || Sheppard et al.
|- id="S/2019 S 38" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 38</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|21998400}} || {{sort|1218.27|−{{val|1218.27}}}} || 163.0 || 0.399 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="Kari" style="background:#d3d3d3;"
| {{sort|45|XLV}} || {{hid|Kari}} ‡[[Kari (moon)|Kari]] || {{IPAc-en|ˈ|k|ɑːr|i}} || style="background:black;"| [[File:Kari-cassini.png|frameless|upright=0.3|center]] || 14.5 || {{sort|6|≈&thinsp;6}} || {{sort|0.27|≈&thinsp;{{val|0.27}}}} || {{val|22032100}} || {{sort|1220.98|{{val|−1220.98}}}} || 153.0 || 0.469 || Norse group (Kari) || 2006 || 2006 || Sheppard et al.
|- id="S/2004 S 48" style="background:#d3d3d3;"
| {{sort|Zzk|}} || {{hid|S/2004Ze}} ‡<small>S/2004 S 48</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22137400}} || {{sort|1229.86|{{val|−1229.86}}}} || 161.9 || 0.374 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2023 S 36" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 36</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22230600}} || {{sort|1237.61|−{{val|1237.61}}}} || 166.3 || 0.359 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="Geirrod" style="background:#d3d3d3;"
| {{sort|66|LXVI}} || {{hid|Geirrod}} ‡[[Geirrod (moon)|Geirrod]] || {{IPAc-en|ˈ|j|ei|r|Q|d}} ||style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22259400}} || {{sort|1240.05|{{val|−1240.05}}}} || 154.4 || 0.539 || Norse group (Kari) || 2004 || 2019 || Sheppard et al.
|- id="S/2023 S 35" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 35</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22269700}} || {{sort|1240.76|−{{val|1240.76}}}} || 168.5 || 0.151 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 29" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 29</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22301400}} || {{sort|1243.45|−{{val|1243.45}}}} || 169.1 || 0.047 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="Fenrir" style="background:#d3d3d3;"
| {{sort|41|XLI}} || {{hid|Fenrir}} ‡[[Fenrir (moon)|Fenrir]] || {{IPAc-en|ˈ|f|ɛ|n|r|ɪər}} ||style="background:black;"| || 15.8 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22330800}} || {{sort|1245.92|{{val|−1245.92}}}} || 164.5 || 0.137 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2004 S 50" style="background:#d3d3d3;"
| {{sort|Zzn|}} || {{hid|S/2004Zg}} ‡<small>S/2004 S 50</small> || — || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22345000}} || {{sort|1247.19|{{val|−1247.19}}}} || 164.0 || 0.450 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2006 S 17" style="background:#d3d3d3;"
| {{sort|Zzj|}} || {{hid|S/2006K}} ‡<small>S/2006 S 17</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22384200}} || {{sort|1250.46|{{val|−1250.46}}}} || 168.7 || 0.425 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al.
|- id="S/2004 S 49" style="background:#d3d3d3;"
| {{sort|Zzm|}} || {{hid|S/2004Zf}} ‡<small>S/2004 S 49</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22399400}} || {{sort|1251.68|{{val|−1251.68}}}} || 159.8 || 0.453 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2020 S 34" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 34</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22435600}} || {{sort|1254.61|−{{val|1254.61}}}} || 160.6 || 0.154 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2020 S 31" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 31</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22457300}} || {{sort|1256.50|−{{val|1256.50}}}} || 163.8 || 0.238 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2023 S 43" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 43</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22563900}} || {{sort|1265.57|−{{val|1265.57}}}} || 170.3 || 0.264 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2019 S 17" style="background:#d3d3d3;"
| {{sort|Zzq|}} || {{hid|S/2019Q}} ‡<small>S/2019 S 17</small> || — || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22722700}} || {{sort|1278.96|{{val|−1278.96}}}} || 155.5 || 0.546 || Norse group (Kari) || 2019 || 2023 || Ashton et al.
|- id="Surtur" style="background:#d3d3d3;"
| {{sort|48|XLVIII}} || {{hid|Surtur}} ‡[[Surtur (moon)|Surtur]] || {{IPAc-en|ˈ|s|ɜːr|t|ər}} ||style="background:black;"| || 15.7 || {{sort|6|≈&thinsp;6}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|22748000}} || {{sort|1281.14|{{val|−1281.14}}}} || 168.4 || 0.448 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al.
|- id="S/2006 S 18" style="background:#d3d3d3;"
| {{sort|Zzo|}} || {{hid|S/2006L}} ‡<small>[[S/2006 S 18]]</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|22760600}} || {{sort|1282.09|{{val|−1282.09}}}} || 169.5 || 0.131 || Norse group (Mundilfari) || 2006 || 2023 || Sheppard et al.
|- id="S/2020 S 36" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 36</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22806200}} || {{sort|1286.03|−{{val|1286.03}}}} || 168.8 || 0.336 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="Loge" style="background:#d3d3d3;"
| {{sort|46|XLVI}} || {{hid|Loge}} ‡[[Loge (moon)|Loge]] || {{IPAc-en|ˈ|l|ɔɪ|.|eɪ}} || style="background:black;"| [[File:Loge N1803341947.png|frameless|upright=0.3|center]] || 15.4 || {{sort|5|≈&thinsp;5}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|22919200}} || {{sort|1295.52|{{val|−1295.52}}}} || 168.1 || 0.191 || Norse group (Mundilfari) || 2006 || 2006 || Sheppard et al.
|- id="S/2020 S 33" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 33</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|22922500}} || {{sort|1295.85|−{{val|1295.85}}}} || 162.8 || 0.555 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="Ymir" style="background:#d3d3d3;"
| {{sort|19|XIX}} || {{hid|Ymir}} ‡[[Ymir (moon)|Ymir]] || {{IPAc-en|ˈ|iː|m|ɪər}} || style="background:black;"| [[File:Ymir-CFHT.gif|frameless|upright=0.3|center]] || 12.2 || {{sort|19|≈&thinsp;19}}|| {{sort|5.6|≈&thinsp;{{val|5.6}}}} || {{val|22955600}} || {{sort|1298.68|{{val|−1298.68}}}} || 172.3 || 0.338 || Norse group (Phoebe) || 2000 || 2000 || Gladman et al.
|- id="S/2020 S 35" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 35</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23030300}} || {{sort|1304.97|−{{val|1304.97}}}} || 174.9 || 0.225 || Norse group (Phoebe) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 19" style="background:#d3d3d3;"
| {{sort|Zzs|}} || {{hid|S/2019S}} ‡<small>[[S/2019 S 19]]</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23044400}} || {{sort|1306.16|{{val|−1306.16}}}} || 151.8 || 0.458 || Norse group (Kari) || 2019 || 2023 || Ashton et al.
|- id="S/2019 S 18" style="background:#d3d3d3;"
| {{sort|Zzr|}} || {{hid|S/2019R}} ‡<small>S/2019 S 18</small> || — || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23139500}} || {{sort|1314.27|{{val|−1314.27}}}} || 154.6 || 0.509 || Norse group (Kari) || 2019 || 2023 || Ashton et al.
|- id="S/2004 S 21" style="background:#d3d3d3;"
| {{sort|F|}} || {{hid|S/2004E}} ‡<small>[[S/2004 S 21]]</small> || — ||style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23160900}}|| {{sort|1316.12|{{val|−1316.12}}}}|| 153.2 || 0.394 || Norse group (Kari) || 2004 || 2019 || Sheppard et al.
|- id="S/2004 S 39" style="background:#d3d3d3;"
| {{sort|L|}} || {{hid|S/2004V}} ‡<small>[[S/2004 S 39]]</small> || — || style="background:black;" | || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23192400}} || {{sort|1318.74|{{val|−1318.74}}}} || 165.9 || 0.100 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2019 S 16" style="background:#d3d3d3;"
| {{sort|Zzp|}} || {{hid|S/2019P}} ‡<small>S/2019 S 16</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23265200}} || {{sort|1324.95|{{val|−1324.95}}}} || 162.0 || 0.250 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="S/2004 S 53" style="background:#d3d3d3;"
| {{sort|Zzz|}} || {{hid|S/2004Zj}} ‡<small>S/2004 S 53</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23279800}} || {{sort|1326.18|{{val|−1326.18}}}} || 162.6 || 0.240 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2004 S 24" style="background:#FDD5B1;"
| {{sort|G|}} || {{hid|S/2004H}} ♣<small>[[S/2004 S 24]]</small> || — || style="background:black;" | || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23338200}} || {{sort|1331.32|+{{val|1331.32}}}} || 37.4 || 0.071 || Gallic group{{refn|group=lower-alpha|The moon has a similar inclination, but a significantly larger semi-major axis. Therefore, it is uncertain whether it comes from the same parent body as the rest of the Gallic group.<ref name="Sheppard2023"/><ref name="Ashton2025a"/>}} || 2004 || 2019 || Sheppard et al.
|- id="S/2004 S 36" style="background:#d3d3d3;"
| {{sort|J|}} || {{hid|S/2004S}} ‡<small>[[S/2004 S 36]]</small> || — || style="background:black;" | || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23390800}} || {{sort|1335.80|{{val|−1335.80}}}} || 153.3 || 0.625 || Norse group (Kari) || 2004 || 2019 || Sheppard et al.
|- id="S/2023 S 45" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 45</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23438400}} || {{sort|1339.85|−{{val|1339.85}}}} || 157.4 || 0.633 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="Thiazzi" style="background:#d3d3d3;"
| {{sort|63|LXIII}} || {{hid|Thiazzi}} ‡[[Thiazzi (moon)|Thiazzi]] || {{IPAc-en|T|i|ˈ|ae|t|s|i}} || style="background:black;" | || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23577500}}|| {{sort|1351.83|{{val|−1351.83}}}} || 158.8 || 0.511 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2020 S 38" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 38</small> || ― || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23583900}} || {{sort|1352.43|−{{val|1352.43}}}} || 159.7 || 0.513 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 20" style="background:#d3d3d3;"
| {{sort|Zzt|}} || {{hid|S/2019T}} ‡<small>S/2019 S 20</small> || — || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23677900}} || {{sort|1360.47|{{val|−1360.47}}}} || 156.0 || 0.354 || Norse group (Kari) || 2019 || 2023 || Ashton et al.
|- id="S/2020 S 37" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 37</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23751800}} || {{sort|1366.82|−{{val|1366.82}}}} || 174.8 || 0.344 || Norse group (Phoebe) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 39" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 39</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23784500}} || {{sort|1369.64|−{{val|1369.64}}}} || 174.5 || 0.098 || Norse group (Phoebe) || 2019 || 2025 || Ashton et al.
|- id="S/2020 S 40" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 40</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|23785900}} || {{sort|1369.76|−{{val|1369.76}}}} || 167.3 || 0.412 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2006 S 19" style="background:#d3d3d3;"
| {{sort|Zzu|}} || {{hid|S/2006M}} ‡<small>[[S/2006 S 19]]</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|23800500}} || {{sort|1371.02|{{val|−1371.02}}}} || 175.5 || 0.467 || Norse group (Phoebe) || 2006 || 2023 || Sheppard et al.
|- id="S/2019 S 40" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 40</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24087800}} || {{sort|1395.88|−{{val|1395.88}}}} || 161.8 || 0.088 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2019 S 42" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 42</small> || ― || style="background:black;"| || 15.9 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|24111600}} || {{sort|1397.98|−{{val|1397.98}}}} || 163.2 || 0.121 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="Saturn LXIV" style="background:#d3d3d3;"
| {{sort|64|[[Saturn LXIV|LXIV]]}} || {{hid|S/2004Q}} ‡<small>[[S/2004 S 34]]</small> || — ||style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|24145800}} || {{sort|1400.93|{{val|−1400.93}}}} || 168.3 || 0.279 || Norse group (Mundilfari) || 2004 || 2019 || Sheppard et al.
|- id="S/2020 S 39" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 39</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24262400}} || {{sort|1411.15|−{{val|1411.15}}}} || 160.1 || 0.305 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 41" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 41</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24493600}} || {{sort|1431.30|−{{val|1431.30}}}} || 157.1 || 0.257 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2023 S 46" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 46</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|24708900}} || {{sort|1450.27|−{{val|1450.27}}}} || 143.2 || 0.336 || Norse group (low-inclination) || 2023 || 2025 || Ashton et al.
|- id="Fornjot" style="background:#d3d3d3;"
| {{sort|42|XLII}} || {{hid|Fornjot}} ‡[[Fornjot (moon)|Fornjot]] || {{IPAc-en|ˈ|f|ɔːr|n|j|ɒ|t}} || style="background:black;"| [[File:Fornjot-cassini.png|frameless|upright=0.3|center]] || 14.7 || {{sort|6|≈&thinsp;6}} || {{sort|0.11|≈&thinsp;{{val|0.11}}}} || {{val|24936800}} || {{sort|1470.36|{{val|−1470.36}}}} || 170.0 || 0.213 || Norse group (Mundilfari) || 2004 || 2005 || Sheppard et al.
|- id="S/2023 S 47" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 47</small> || ― || style="background:black;"| || 17.0 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25102300}} || {{sort|1485.04|−{{val|1485.04}}}} || 162.5 || 0.101 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2004 S 51" style="background:#d3d3d3;"
| {{sort|Zzv|}} || {{hid|S/2004Zh}} ‡<small>S/2004 S 51</small> || — || style="background:black;"| || 16.1 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|25207100}} || {{sort|1494.41|{{val|−1494.41}}}} || 171.2 || 0.201 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2006 S 29" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2006 S 29</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25212100}} || {{sort|1494.78|−{{val|1494.78}}}} || 156.2 || 0.239 || Norse group (Kari) || 2006 || 2025 || Sheppard et al.
|- id="S/2020 S 10" style="background:#d3d3d3;"
| {{sort|Zzza|}} || {{hid|S/2020J}} ‡<small>S/2020 S 10</small> || — || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25315300}} || {{sort|1503.97|{{val|−1503.97}}}} || 165.6 || 0.296 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al.
|- id="S/2020 S 42" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 42</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25329400}} || {{sort|1505.31|−{{val|1505.31}}}} || 157.5 || 0.506 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2020 S 9" style="background:#d3d3d3;"
| {{sort|Zzw|}} || {{hid|S/2020I}} ‡<small>[[S/2020 S 9]]</small> || — || style="background:black;"| || 16.0 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|25408700}} || {{sort|1512.38|{{val|−1512.38}}}} || 161.4 || 0.531 || Norse group (Mundilfari) || 2020 || 2023 || Ashton et al.
|- id="S/2023 S 5" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2023 S 5</small> || ― || style="background:black;"| || 16.7 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25583500}} || {{sort|1528.04|−{{val|1528.04}}}} || 168.8 || 0.599 || Norse group (Mundilfari) || 2023 || 2025 || Ashton et al.
|- id="S/2020 S 41" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 41</small> || ― || style="background:black;"| || 16.6 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|25876400}} || {{sort|1554.40|−{{val|1554.40}}}} || 160.2 || 0.402 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="Saturn LVIII" style="background:#d3d3d3;"
| {{sort|58|[[Saturn LVIII|LVIII]]}} || {{hid|S/2004J}} ‡<small>[[S/2004 S 26]]</small> || — ||style="background:black;"| || 15.7 || {{sort|5|≈&thinsp;5}} || {{sort|0.065|≈&thinsp;{{val|0.065}}}} || {{val|26097500}} || {{sort|1574.25|{{val|−1574.25}}}} || 172.9 || 0.147 || Norse group (Phoebe){{refn|group=lower-alpha|name="Phoebe/Mundilfari"}} || 2004 || 2019 || Sheppard et al.
|- id="S/2019 S 21" style="background:#d3d3d3;"
| {{sort|Zzzb|}} || {{hid|S/2019U}} ‡<small>[[S/2019 S 21]]</small> || — || style="background:black;"| || 16.2 || {{sort|4|≈&thinsp;4}} || {{sort|0.034|≈&thinsp;{{val|0.034}}}} || {{val|26439500}} || {{sort|1605.28|{{val|−1605.28}}}} || 171.9 || 0.155 || Norse group (Mundilfari) || 2019 || 2023 || Ashton et al.
|- id="S/2004 S 52" style="background:#d3d3d3;"
| {{sort|Zzx|}} || {{hid|S/2004Zi}} ‡<small>[[S/2004 S 52]]</small> || — || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26446400}} || {{sort|1605.89|{{val|−1605.89}}}} || 165.4 || 0.291 || Norse group (Mundilfari) || 2004 || 2023 || Sheppard et al.
|- id="S/2020 S 43" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 43</small> || ― || style="background:black;"| || 16.9 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26657400}} || {{sort|1625.29|−{{val|1625.29}}}} || 164.6 || 0.203 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|- id="S/2019 S 43" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 43</small> || ― || style="background:black;"| || 16.5 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26664100}} || {{sort|1625.90|−{{val|1625.90}}}} || 165.3 || 0.277 || Norse group (Mundilfari) || 2019 || 2025 || Ashton et al.
|- id="S/2019 S 44" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2019 S 44</small> || ― || style="background:black;"| || 16.4 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|26796900}} || {{sort|1638.11|−{{val|1638.11}}}} || 172.6 || 0.512 || Norse group (Phoebe) || 2019 || 2025 || Ashton et al.
|- id="S/2020 S 44" style="background:#d3d3d3;"
| {{sort|Zzzzp|}} || {{hid|S/2023T}} ‡<small>S/2020 S 44</small> || ― || style="background:black;"| || 16.8 || {{sort|3|≈&thinsp;3}} || {{sort|0.014|≈&thinsp;{{val|0.014}}}} || {{val|27259400}} || {{sort|1680.64|−{{val|1680.64}}}} || 168.5 || 0.199 || Norse group (Mundilfari) || 2020 || 2025 || Ashton et al.
|}
{{sticky table end}}

===Unconfirmed===
These F Ring moonlets listed in the following table (observed by ''[[Cassini–Huygens|Cassini]]'') have not been confirmed as solid bodies. It is not yet clear if these are real satellites or merely persistent clumps within the F Ring.<ref name=Porco2005/>

{| class="wikitable"
|-
! Name
! Image
! Diameter (km)
! Semi-major<br>axis (km)<ref name="Spitale Jacobson et al. 2006" />
! Orbital<br>period ([[day|d]])<ref name="Spitale Jacobson et al. 2006" />
! Position
! Discovery year
! Status
|-
| [[S/2004 S 3]] and [[S/2004 S 4|S 4]]{{refn|group=lower-alpha|S/2004 S 4 was most likely a transient clump—it has not been recovered since the first sighting.<ref name=Porco2005/>|name="note_2a"}}|| style="background:black;" |[[File:S2004 S 3 - PIA06115.png|frameless|upright=0.3]]|| ≈&thinsp;3–5 || ≈&thinsp;{{val|140300}}|| ≈&thinsp;+{{val|0.619}}
| rowspan="2" |uncertain objects around the F Ring|| 2004
|Were undetected in thorough imaging of the region in November 2004, making their existence improbable
|-
| [[S/2004 S 6]]|| style="background:black;" |[[File:S2004 S6.jpg|frameless|upright=0.3|alt=A bright narrow band runs from the top to bottom. To the right of it in the diffuse halo the is a bright small object.]]|| ≈&thinsp;3–5 || ≈&thinsp;{{val|140130}}|| +{{val|0.61801}} || 2004
|Consistently detected into 2005, may be surrounded by fine dust and have a very small physical core
|}

===Spurious===
Two moons were claimed to be discovered by different astronomers but never seen again. Both moons were said to orbit between [[Titan (moon)|Titan]] and [[Hyperion (moon)|Hyperion]].<ref name=Solarviews/>
*[[Chiron (hypothetical moon)|Chiron]] which was supposedly sighted by [[Hermann Goldschmidt]] in 1861, but never observed by anyone else.<ref name=Solarviews/>
*[[Themis (hypothetical moon)|Themis]] was allegedly discovered in 1905 by astronomer [[William Henry Pickering|William Pickering]], but never seen again. Nevertheless, it was included in numerous [[almanac]]s and astronomy books until the 1960s.<ref name=Solarviews/>

===Hypothetical===
In 2022, scientists of the [[Massachusetts Institute of Technology]] proposed the hypothetical former moon [[Chrysalis (moon)|Chrysalis]], using data from the [[Cassini–Huygens]] mission. Chrysalis would have orbited between Titan and Iapetus, but its orbit would have gradually become more eccentric until it was [[Roche limit|torn apart]] by Saturn. 99% of its mass would have been absorbed by Saturn, while the remaining 1% would have formed Saturn's rings.<ref>{{Cite web|url=https://www.newscientist.com/article/2337884-saturns-rings-could-have-come-from-a-destroyed-moon-named-chrysalis/|title=Saturn's rings could have come from a destroyed moon named Chrysalis|date=15 September 2022|website=New Scientist|access-date=16 September 2022|archive-date=16 September 2022|archive-url=https://web.archive.org/web/20220916161501/https://www.newscientist.com/article/2337884-saturns-rings-could-have-come-from-a-destroyed-moon-named-chrysalis/|url-status=live}}</ref><ref>{{Cite journal|url=https://www.science.org/doi/10.1126/science.abn1234|title=Loss of a satellite could explain Saturn's obliquity and young rings|first1=Jack|last1=Wisdom|first2=Rola|last2=Dbouk|first3=Burkhard|last3=Militzer|first4=William B.|last4=Hubbard|first5=Francis|last5=Nimmo|first6=Brynna G.|last6=Downey|first7=Richard G.|last7=French|date=September 16, 2022|journal=Science|volume=377|issue=6612|pages=1285–1289|doi=10.1126/science.abn1234|pmid=36107998|bibcode=2022Sci...377.1285W |hdl=1721.1/148216 |s2cid=252310492 |url-access=subscription|hdl-access=free}}</ref>

===Temporary===
Much like Jupiter, asteroids and comets will infrequently make close approaches to Saturn, even more infrequently becoming captured into orbit of the planet. The comet P/2020 F1 (Leonard) is calculated to have made a close approach of {{val|978000|65000}} km ({{val|608000|40000}} mi) to Saturn on 8 May 1936, closer than the orbit of Titan to the planet, with an [[orbital eccentricity]] of only {{val|1.098|0.007}}. The comet may have been orbiting Saturn prior to this as a temporary satellite, but difficulty modelling the non-gravitational forces makes whether or not it was indeed a temporary satellite uncertain.<ref>{{cite web |last1=Deen |first1=Sam |title=P/2020 F1 (Leonard): A previous-perihelion precovery, and a very, very young comet. |url=https://groups.io/g/mpml/message/35416 |website=groups.io |access-date=27 March 2020 |archive-date=27 March 2020 |archive-url=https://web.archive.org/web/20200327032811/https://groups.io/g/mpml/message/35416 |url-status=live}}</ref>

Other comets and asteroids may have temporarily orbited Saturn at some point, but none are presently known to have.

==Formation==
It is thought that the Saturnian system of Titan, mid-sized moons, and rings developed from a set-up closer to the [[Galilean moons]] of Jupiter, though the details are unclear. It has been proposed either that a second Titan-sized moon broke up, producing the rings and inner mid-sized moons,<ref>{{cite journal | last1 = Canup | first1 = R. | author-link = Robin Canup | title = Origin of Saturn's rings and inner moons by mass removal from a lost Titan-sized satellite | journal = Nature | volume = 468| issue = 7326| pages = 943–6| doi = 10.1038/nature09661 | pmid=21151108 | date=December 2010|bibcode = 2010Natur.468..943C | s2cid = 4326819}}</ref> or that two large moons fused to form Titan, with the collision scattering icy debris that formed the mid-sized moons.<ref name="Asphaug2013" /> On 23 June 2014, NASA claimed to have strong evidence that [[nitrogen]] in the [[atmosphere of Titan]] came from materials in the [[Oort cloud]], associated with [[comets]], and not from the materials that formed Saturn in earlier times.<ref name="NASA-201450623" /> Studies based on Enceladus's tidal-based geologic activity and the lack of evidence of extensive past resonances in Tethys, Dione, and Rhea's orbits suggest that the moons up to and including Rhea may be only 100 million years old.<ref>{{cite magazine|url=http://www.astronomy.com/news/2016/03/moons-of-saturn-may-be-younger-than-the-dinosaurs|title=Moons of Saturn may be younger than the dinosaurs|author=SETI Institute|magazine=[[Astronomy (magazine)|Astronomy]]|date=March 25, 2016|author-link=SETI Institute|access-date=March 30, 2016|archive-date=December 6, 2019|archive-url=https://web.archive.org/web/20191206163235/https://astronomy.com/news/2016/03/moons-of-saturn-may-be-younger-than-the-dinosaurs|url-status=live}}</ref>

==See also==
*[[List of natural satellites]]

==Notes==
{{Reflist|30em| group = lower-alpha}}

==References==
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}}

==External links==
{{Commons category}}
*[[Scott S. Sheppard]]: [https://sites.google.com/carnegiescience.edu/sheppard/moons/saturnmoons Saturn Moons]
*{{cite web|url=http://orinetz.com/planet/animatesystem.php?ephid=Q07IAL5QATR7V073RO44XQVPA00001 |title=Simulation showing the position of Saturn's Moon |access-date=26 May 2010 |url-status=dead |archive-url=https://web.archive.org/web/20110823202308/http://orinetz.com/planet/animatesystem.php?ephid=Q07IAL5QATR7V073RO44XQVPA00001 |archive-date=23 August 2011}}
*{{cite web|url=http://solarsystem.nasa.gov/planets/profile.cfm?Object=Saturn&Display=Rings|title=Saturn's Rings|publisher=NASA's Solar System Exploration|access-date=26 May 2010|url-status=dead|archive-url=https://web.archive.org/web/20100527141504/http://solarsystem.nasa.gov/planets/profile.cfm?Object=Saturn&Display=Rings|archive-date=27 May 2010}}
*{{cite web|url=http://www.astronomycast.com/astronomy/episode-61-saturns-moons/|title=Saturn's Moons|date=6 November 2007 |publisher=[[Astronomy Cast]] episode No. 61, includes full transcript|access-date=26 May 2010}}
*{{cite video|url=https://www.youtube.com/watch?v=xxXa9pxwzoY|people=Carolyn Porco|title=Fly me to the moons of Saturn|access-date=26 May 2010}}
*[https://www.nytimes.com/interactive/2015/12/18/science/space/nasa-cassini-maps-saturns-moons.html Rotate and Spin Maps of 7 Moons] at ''[[The New York Times]]''
*[[Planetary Society]] [http://www.planetary.org/blogs/emily-lakdawalla/2017/0517-saturns-small-satellites-to-scale.html blog post] (2017-05-17) by [[Emily Lakdawalla]] with images giving comparative sizes of the moons
*Tilmann Denk: [https://tilmanndenk.de/outersaturnianmoons/ Outer Moons of Saturn]

{{Moons of Saturn}}
{{Saturn}}
{{Solar System moons (compact)}}
{{Solar System}}
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[[Category:Moons of Saturn| ]]
[[Category:Lists of moons]]
[[Category:Solar System]]