List of supernovae
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(Crab Nebula)
A supernova is an event in which a star destroys itself in an explosion which can briefly become as luminous as an entire galaxy. This list of supernovas of historical significance includes events that were observed prior to the development of photography, and individual events that have been the subject of a scientific paper that contributed to supernova theory.
List of supernovae
In most entries, the year when the supernova was seen is part of the designation (1st column).
| Supernova designation (year) |
Constellation | Observations | Apparent magnitude |
Distance (light years) |
Type | Galaxy | Notes |
|---|---|---|---|---|---|---|---|
| Template:NtshSN 185 | Centaurus | 7 December 185 | Template:Ntsh−4 (?)[1] | 9,100[2] | Template:NtshIa (?) | Milky Way | Surviving description sketchy; modern estimates of maximum apparent magnitude vary from +4 to −8. The remnant is probably RCW 86, some 8200 ly distant,[3] making it comparable to SN 1572. Some researchers have suggested it was a comet, not a supernova.[4][5] |
| Template:NtshSN 386 | Sagittarius | April/May 386 | Template:Ntsh+1.5 | 14,700 | Template:NtshII | Milky Way | "suggested SN",[6] candidate remnant could be G11.2-0.3.[7][8] There are three suggestions and doubtful if SN at all or classical nova or something else.[9] |
| Template:NtshSN 393 | Scorpius | 27 February − 28 March - 22 October − 19 November 393 | Template:Ntsh–0 | 3,400 | Template:Ntsh II/Ib | Milky Way | "possible SN",[6] could also be classical nova or something else[9] |
| Template:NtshSN 1006 | Lupus | 17 April 1006 - 1 May 1006 | Template:Ntsh–7.5[10] | 7,200 | Template:NtshIa | Milky Way | Widely observed on Earth; in apparent magnitude, the brightest stellar event in recorded history.[11] |
| Template:NtshSN 1054 | Taurus | c. Template:TrimScript error: No such module "Check for unknown parameters". [O.S. c. Template:TrimScript error: No such module "Check for unknown parameters".] 1054 c. Template:TrimScript error: No such module "Check for unknown parameters". [O.S. c. Template:TrimScript error: No such module "Check for unknown parameters".] 1056 |
Template:Ntsh–6[12] | 6,500 | Template:NtshII | Milky Way | Remnant is the Crab Nebula with its pulsar (neutron star) |
| Template:NtshSN 1181 | Cassiopeia | 4 August 1181 - 6 August 1181 | Template:Ntsh0 | 7,100 | Template:Ntshsub-luminous Type Iax supernova | Milky Way | Remnant is Pa 31 with its hot stellar remnant[13] |
| Template:NtshSN 1572 | Cassiopeia | November 1572 | Template:Ntsh–4.0 | 8,000 | Template:NtshIa | Milky Way | Tycho's Nova |
| Template:NtshSN 1604 | Ophiuchus | 8–9 October 1604 | Template:Ntsh–3 | 14,000 | Template:NtshIa | Milky Way | Kepler's Supernova; most recent readily visible supernova within the Milky Way |
| Template:NtshCas A, c. 1680 |
Cassiopeia | 1680 | Template:Ntsh+5 | 9,000 | Template:NtshIIb | Milky Way | Apparently never visually conspicuos, due to interstellar dust; but the remnant, Cas A, is the brightest extrasolar radio source in the sky |
| Template:NtshG1.9+0.3, cal. 1868 |
Sagittarius | 1868 | (visible light masked by dust) | 25,000 | Template:NtshIa | Milky Way | Located near the Galactic Center; "Posthummusly" discovered in 1985; age determined in 2008 |
| Template:NtshSN 1885A | Andromeda | 20 August 1885 | Template:Ntsh+5.85[14] | 2,500,000 | Template:NtshIpec | Andromeda Galaxy | First observation of an extragalactic supernova |
| Template:NtshSN 1895B | Centaurus | 12 December 1895 | Template:Ntsh+8.0[15] | 10,900,000 | Template:NtshIa | NGC 5253 | |
| Template:NtshSN 1909A | Ursa Major | January 1909 | Template:Ntsh+12.1 | 21,000,000 | Pinwheel Galaxy (M101) | [16][17] | |
| Template:NtshSN 1937C | Canes Venatici | 24 August 1937 | Template:Ntsh+8.4[15] | 13,000,000 | Template:NtshIa | IC 4182 | |
| Template:NtshSN 1939C | Cepheus | 17 July 1939 | Template:Ntsh+13.0 | 25,200,000 | Template:NtshI | NGC 6946 (Fireworks Galaxy) | |
| Template:NtshSN 1940B | Coma Berenices | 5 May 1940 | Template:Ntsh+12.8 | 38,000,000 | Template:NtshII-P | NGC 4725 | |
| Template:NtshSN 1951H | Ursa Major | 1 September 1951 | Template:Ntsh+17.5 | 21,000,000 | Pinwheel Galaxy (M101) | [18] | |
| Template:NtshSN 1961V | Perseus | 11 July 1961 | Template:Ntsh+12.5 | 30,000,000 | Template:NtshII? | NGC 1058 | Potential supernova impostor[19] |
| Template:NtshSN 1970G | Ursa Major | 30 July 1970 | Template:Ntsh+12.1 | 21,000,000 | Template:NtshII | Pinwheel Galaxy (M101) | [20][21][22] |
| Template:NtshSN 1972E | Centaurus | 13 May 1972 | Template:Ntsh+8.7[23] | 10,900,000 | Template:NtshIa | NGC 5253 | Followed for more than a year; became the prototypical Type Ia supernova |
| Template:NtshSN 1983N | Hydra | 3 July 1983 | Template:Ntsh+11.8 | 15,000,000 | Template:NtshIb | Messier 83 | First observation of a Type Ib supernova |
| Template:NtshSN 1986J | Andromeda | 21 August 1986 | Template:Ntsh+18.4 | 30,000,000 | Template:NtshIIn | NGC 891 | Bright in the radio frequency range |
| Template:NtshSN 1987A | Dorado | 1987 | Template:Ntsh+2.9 | 160,000 | Template:NtshIIpec | Large Magellanic Cloud | Intense radiation reached Earth on February 23, 1987, 7:35:35 UT. Notable for archival photos of progenitor star and detection of supernova neutrinos. Most recent Local Group supernova |
| Template:NtshSN 1993J | Ursa Major | 28 March 1993 | Template:Ntsh+10.7[24] | 11,000,000 | Template:NtshIIb | M81 | One of the brightest supernovae in the northern sky since 1954 |
| Template:NtshSN 1994D | Virgo | 7 March 1994 | Template:Ntsh+15.2 | 50,000,000 | Template:NtshIa | NGC 4526 | |
| Template:NtshSN 1998bw | Telescopium | 26 April 1998 | ? | 140,000,000 | Template:NtshIc | ESO 184-G82 | Linked to GRB 980425, which was the first time a gamma-ray burst has been linked to a supernova. |
| Template:NtshSN 1999eh | Lynx | 12 October 1999 | Template:Ntsh+18.3 +/- 0.3 | 84,000,000 | Template:Ntsh I | NGC 2770 | First supernovae in this galaxy, where 3 more were detected later. |
| Template:NtshSN 2002bj | Lupus | 2002 | Template:Ntsh+14.7 | 160,000,000 | Template:NtshIIn | NGC 1821 | AM Canum Venaticorum-type outburst.[25] |
| Template:NtshSN 2002dd | Ursa Major | 2002 | Template:Ntsh+24.0 | 8,000,000,000 | Template:NtshIa | anonymous galaxy | Furthest supernova observed through Hubble Deep Field.[26] |
| Template:NtshSN 2003fg | Boötes | 2003 | 4,000,000,000 | Template:NtshIa | anonymous galaxy | Also known as the "Champagne supernova" | |
| Template:NtshSN 2004am | Ursa Major | March 2004 | 11,500,000 | Template:NtshII | M82 (Cigar Galaxy) | [27] | |
| Template:NtshSN 2004dj | Camelopardalis | 31 July 2004 18:15 |
8,000,000 | Template:NtshII-P | NGC 2403 | NGC 2403 is an outlying member of the M81 Group | |
| SN 2213-1745 | Aquarius | November 2004-June 2005 | Template:NtshII | [28] | |||
| Template:NtshSN 2005ap | Coma Berenices | 3 March 2005 | 4,700,000,000 | Template:NtshII | ? | Announced in 2007 to be the brightest supernova up to that point. | |
| Template:NtshSN 2005gj | Cetus | 27 September 2005 | 865,000,000 | Template:NtshIa/II-n | ? | Notable for having characteristics of both Type Ia and Type IIn. | |
| Template:NtshSN 2005gl | Pisces | 5 October 2005 | Template:Ntsh+16.5 | 200,000,000 | Template:NtshII-n | NGC 266 | Star could be found on old pictures.[29] |
| Template:NtshSN 2006gy | Perseus | 18 September 2006 | Template:Ntsh+15 | 240,000,000 | Template:NtshIIn (*) | NGC 1260 | Observed by NASA, *with a peak of over 70 days, possibly a new type. |
| Template:NtshSN 2006jc | Lynx | 9 October 2006 | 77,000,000 | Template:NtshIbn | UGC 4904 | ||
| Template:NtshSN 2007bi | Virgo | Early 2007 | Template:Ntsh+18.3 | Template:NtshIa | anonymous dwarf galaxy | Extremely bright and long-lasting, the first good observational match for the pair-instability supernova model postulated for stars of initial mass greater than 140 solar masses (even better than SN 2006gy). The precursor is estimated at 200 solar masses, similar to the first stars of the early universe.[30] | |
| Template:NtshSN 2007uy | Lynx | 31 December 2007 | Template:Ntsh+16.8 | 84,000,000 | Template:NtshIbc | NGC 2770 | Got overshadowed by SN 2008D. |
| Template:NtshSN 2008D | Lynx | 9 January 2008 | 88,000,000 | Template:NtshIbc | NGC 2770 | First supernova to be observed while it exploded. | |
| Template:NtshMENeaC Abell399.3.14.0 | Aries | Template:Ntsh+28.7 | 1,000,000,000 (z=0.0613) |
Template:NtshIa | anonymous red globular cluster associated with anonymous red elliptical galaxy in cluster Abell 399 | Observed in 2009. Supernova associated with a globular cluster[31][32] | |
| Template:NtshSN 2009ip | Piscis Austrinus | 2009 | 66,000,000 | Template:NtshIIn | NGC 7259 | In 2009 classified as supernova. Redesignated as Luminous blue variable (LBV) Supernova impostor.[33] In September 2012 classified as a young type IIn supernova.[34] | |
| Template:NtshSN 2010lt | Camelopardalis | 2 January 2011 | Template:Ntsh+17.0 | 240,000,000 | Template:NtshIa (sub-luminous) | UGC 3378 | Discovered by 10-year-old girl, the youngest person to discover a supernova. |
| Template:NtshSN 2011fe | Ursa Major | 24 August 2011 | Template:Ntsh+10.0 | 21,000,000 | Template:NtshIa | M101 | One of the very few extragalactic supernovae visible in 50mm binoculars. |
| Template:NtshSN UDS10Wil | Cetus | April 2013 | 166,000,000,000 | Also Known as SN Wilson.[35] | |||
| Template:NtshSN 2014J | Ursa Major | Mid January 2014 | Template:Ntsh+10.1 | 11,500,000 | Template:NtshIa | M82 | Closest supernova since SN 2004dj in NGC 2403. |
| Template:NtshSN 2014aa | Leo | 7 March 2014 | 310,000,000 | Template:NtshIa | NGC 3861 | [39][40][41] | |
| Template:NtshSN Refsdal | Leo | 11 November 2014 | 14,400,000,000 | SP 1149 | It is the first detected multiply-lensed supernova, visible within the field of the galaxy cluster MACS J1149+2223.[42][43][44][45] | ||
| Template:NtshASASSN-15ga | Virgo | 1 April 2015 | 1,000,000,000 | Template:NtshIa | NGC 4866 | [46] | |
| Template:NtshASASSN-15lh SN 2015L | Indus | 14 June 2015 | Template:Ntsh+16.9 | 3,800,000,000 | Template:NtshIc | APMUKS(BJ) B215839.70−615403.9 | Most luminous hypernova ever observed. |
| IPTF14hls | Ursa Major | September 2014 | Template:Ntsh+17.7 | 509,000,000 | unknown | SDSS J092034.44+504148.7 (possible dwarf galaxy) | Unusual supernova |
| Template:NtshSN 2016aps | Draco | 22 February 2016 | Template:Ntsh+18.11 | 3,600,000,000 | Template:NtshSLSB-II | ? | Most luminous supernova-like event to date. |
| Template:NtshSN 2017gax | Dorado | 14 August 2017 | 517,000,000 | Template:Ntsh I | NGC 1672 | ||
| Template:NtshSN 2018gv | Puppis | 15 January 2018 | 70,000,000 | Template:NtshIa | NGC 2525 | [47][48][49][50][51] | |
| Template:NtshSN 2018zd | Camelopardalis | 2 March 2018 | Template:Ntsh+17.8 | 70,000,000 | Template:NtshIa-csm | NGC 2146 | First electron capture supernova ever detected |
| Template:NtshSN 2018cow | Hercules | 16 June 2018, 10:35:02 | 200,000,000 | Template:NtshIb | CGCG 137-068 | [52] | |
| SN 2019np | Leo Minor | 9 January 2019 | Template:Ntsh+13.0 | 75,000,000 | Template:Ntsh Ia | NGC 3254 | [53][54] |
| SN 2019hgp | Boötes | Template:Ntsh+20.16 | 920,000,000 | Template:NtshIcn | First detected supernova of a Wolf-Rayet star[55][56] | ||
| SN 2020oi | Coma Berenices | 7 January 2020 | Template:Ntsh+17.28 | 46,000,000 | Template:NtshIc | Messier 100 | Script error: No such module "Unsubst". |
| SN 2020fqv | Virgo | 31 March 2020 | Template:Ntsh+19.0 | 59,400,000 | Template:NtshIIb | NGC 4568 | Earliest known observation of an explosion, 26 hours after[57][58][59] |
| SN 2020jfo | Virgo | 6 May 2020 | 45,610,000 | Template:NtshII | M61 | [60][61][62] | |
| SN 2020tlf | Boötes | 2020 | Template:Ntsh+15.89 | 120,000,000 | Template:NtshIIn | NGC 5731 | First red supergiant observed before, during and after explosion; earliest known observation, at 130 days before explosion[63][64] |
| SN 2021gmj | Ursa Major | 20 March 2021 | Template:Ntsh+11.2 | 34,800,00 | Template:NtshII-P | NGC 3310 | [65] |
| SN 2021hpr | Draco | April 2, 2021 | 129,000,000 ± 29 | Template:NtshIa | NGC 3147 | [66] | |
| SN 2021jad | Lepus | April 2021 | 65,000,000 | Template:NtshIa | NGC 1964 | [67] | |
| Template:NtshSN 2021yja | Eridanus | 8 September 2021 | 750,000,000 | Template:NtshII | NGC 1325[68][69] | ||
| SN 2021aefx | Dorado | 11 November 2021 | Template:Ntsh+17.2 | 69,000,000 | Template:NtshIa | NGC 1566 | [70] |
| Template:NtshSN 2021afdx | Sculptor | 23 November 2021 | Template:Ntsh+18.8 | 500,000,000 | Template:NtshII | Cartwheel Galaxy | [71][72] |
| SN 2022jli | Cetus | 5 May 2022 | Template:Ntsh+14 | 75,000,000 | type I-c | NGC 157 | Type Ic, shows periodicity[73][74][75][76] |
| Template:NtshSN 2022aajn | Gemini | November 2022 | 600,000,000 | Template:NtshIa | [77] | ||
| SN 2023ixf | Ursa Major | 19 May 2023 17:27 |
Template:Ntsh+10.8 | 21,000,000 | type II-L | Pinwheel Galaxy (M101)[78] | Closest and brightest supernova since SN 2014J |
| Template:NtshSN 2023rve | Fornax | 8 September 2023 | Template:Ntsh+13.9 | 450,000,000 | Template:NtshII | NGC 1097[79][80][81][82][83] | Brightest Supernova Since SN 2023ixf. |
| Template:NtshSN 2023vyl | Pegasus | 28 October 2023 | 783,000,000 | Template:NtshIa | NGC 7625 | [84][85] | |
| Template:NtshSN 2023abdg | Grus | 12 December 2023 | 816,000,000 | Template:NtshII | NGC 7421 | [86] | |
| SN 2023ufx | Template:Ntsh+15.55 | Template:Ntsh II | The most metal-poor supernova found to date.[87] | ||||
| SN H0pe | Ursa Major | 2023 | Template:NtshIa | PLCK G165.7+67.0 Arc 1 | [88] | ||
| Template:NtshSN 2024gy | Virgo | 4 January 2024 | Template:Ntsh+12.8 | 55,000,000 | Template:Ntsh Ia | NGC 4216 | [89] |
| Template:NtshSN 2024ggi | Hydra | 11 April 2024 | Template:Ntsh+11.9 | 21,700,000 | Template:Ntsh II | NGC 3621 | [90] |
| Template:NtshSN 2024inv | Leo | 10 May 2024 | Template:Ntsh+12.1 | 82,200,000 | Template:Ntsh Ia | NGC 3524 | [91] |
| Template:NtshSN 2024muv | Virgo | 26 June 2024 | Template:Ntsh+12.7 | 65,000,000 | Template:Ntsh Ia | NGC 4699 | [92] |
| Template:NtshSN 2024abfl | Camelopardalis | 15 November 2024 | 41,000,000 | Template:Ntsh II | NGC 2146 | [93] | |
| Template:NtshSN 2025fvw | Serpens | 26 March 2025 | Template:Ntsh+13.8 | 100,000,000 | Template:Ntsh Ia | NGC 5957 | [94] |
Supernova statistics
| Year | Total | Type I | Type II | LBV (imposters) |
Brighter than apmag 13 |
Apmag of brightest Supernova of that year |
|---|---|---|---|---|---|---|
| 2024[95] | Script error: No such module "val". | 1675 | 473 | 4 | 5 | 11.9 (2024ggi in NGC 3621) |
| 2023[96] | Script error: No such module "val". | 1430 | 417 | 7 | 2 | 10.9 (2023ixf in Messier 101) |
| 2022[97] | Script error: No such module "val". | 1732 | 396 | 7 | 4 | 12.3 (2022hrs in NGC 4647) |
| 2021[98] | Script error: No such module "val". | 1849 | 465 | 5 | 8 | 12.0 (2021aefx in NGC 1566) |
| 2020[99] | Script error: No such module "val". | 1648 | 451 | 7 | 7 | 11.8 (2020ue in NGC 4636) |
| 2019[100] | Script error: No such module "val". | 1652 | 485 | 9 | 1 | 13.0 (2019np in NGC 3254) |
| 2018[101] | Script error: No such module "val". | 1206 | 332 | 7 | 5 | 12.7 (2018pv in NGC 3941) |
| 2017[102] | 8293 | 746 | 218 | 4 | 3 | 11.5 (2017cbv in NGC 5643) |
| 2016[103] | 7737 | 681 | 226 | 3 | 0 | 13.0 (2016coj in NGC 4125) |
| 2015[104] | 4474 | 707 | 214 | 4 | 2 | 12.9 (2015F in NGC 2442) |
| 2014[105] | 2243 | 528 | 175 | 2 | 3 | 10.1 (2014J in Messier 82) |
| 2013[106] | 1922 | 498 | 190 | 7 | 6 | 11.3 (2013aa in NGC 5643) |
| 2012[107] | 1223 | 550 | 152 | 8 | 5 | 11.9 (2012fr in NGC 1365) |
| 2011[108] | 1129 | 439 | 160 | 10 | 7 | 9.9 (2011fe in Messier 101) |
| 2010[109] | 931 | 279 | 135 | 7 | 2 | 12.8 (2010ih in NGC 2325) |
| 2009[110] | 576 | 202 | 137 | 1 | 0 | 13.0 (2009ig in NGC 1015) |
| 2008[111] | 511 | 251 | 143 | 1 | 3 | 12.4 (2008ge in NGC 1527) |
| 2007[112] | 605 | 442 | 130 | 1 | 3 | 12.0 (2007it in NGC 5530) |
| 2006[113] | 558 | 418 | 124 | 2 | 3 | 12.1 (2006dd in NGC 1316) |
| 2005[114] | 385 | 273 | 94 | 1 | 2 | 12.3 (2005df in NGC 1559) |
| 2004[115] | 343 | 221 | 79 | 0 | 2 | 11.2 (2004dj in NGC 2403) |
| 2003[116] | 384 | 198 | 89 | 1 | 1 | 12.3 (2003hv in NGC 1201) |
| 2002[117] | 353 | 163 | 64 | 0 | 1 | 12.3 (2002ap in Messier 74) |
| 2001[118] | 310 | 108 | 75 | 0 | 2 | 12.3 (2001e1 in NGC 1448) |
| 2000[119] | 199 | 76 | 49 | 1 | 0 | 13.1 (2000cx in NGC 528) |
| 2000–2023 | 147,135 | 16,297 (76.5%) |
5000 | 95 | 72 |
See also
- List of most distant supernovae
- List of supernova candidates
- List of supernova remnants
- Lists of astronomical objects
References
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- ↑ Modern estimates vary widely; see SN 185 for more detail.
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- ↑ "New evidence links stellar remains to oldest recorded supernova" Chandra X-ray Observatory, released 2006-09-18, revised 2009-02-20, retrieved 2010-02-26.
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- ↑ SEDS, Supernova 1055 – Creation of the Crab Nebula
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Further reading
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External links
- The Open Cataclysmic Variable Catalog
- IAU Supernovae on the Transient Name Server (TNS)
- Supernovae through 2015 at IAU Central Bureau for Astronomical Telegrams (CBAT).
- WISeREP – The Weizmann Interactive Supernova data Repository
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