List of supernovae

Last updated

SN 1054 remnant
(Crab Nebula) Crab Nebula.jpg
SN 1054 remnant
( 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 supernovae 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.

Contents

List of supernovae

In most entries, the year when the supernova was seen is part of the designation (1st column).

Supernova
designation
(year)
ConstellationObservations Apparent
magnitude
Distance
(light years)
TypeGalaxyComments
Centaurus 7 December 1859,100 [2] 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]
Sagittarius April/May 38614,700Milky 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]
Scorpius 27 February − 28 March - 22 October − 19 November 3933,400Milky Way"possible SN", [6] could also be classical nova or something else [9]
Lupus 17 April 1006 - 1 May 10067,200Milky WayWidely observed on Earth; in apparent magnitude, the brightest stellar event in recorded history. [11]
Taurus c.10 July [ O.S. c.4 July] 1054
c.12 April [ O.S. c.6 April] 1056
6,500Milky WayRemnant is the Crab Nebula with its pulsar (neutron star)
Cassiopeia 4 August 1181 - 6 August 11817,100Milky WayRemnant is Pa 30 with its hot stellar remnant [13]
Cassiopeia November 15728,000Milky Way Tycho's Nova
Ophiuchus 8–9 October 160414,000Milky WayKepler's Supernova; most recent readily visible supernova within the Milky Way
Cassiopeia 16809,000Milky WayApparently never visually conspicuous, due to interstellar dust; but the remnant, Cas A, is the brightest extrasolar radio source in the sky
Sagittarius 1868(visible light masked by dust)25,000Milky WayLocated near the Galactic Center; "Posthumously" discovered in 1985; age determined in 2008
Andromeda 20 August 18852,500,000 Andromeda Galaxy First observation of an extragalactic supernova
Centaurus 12 December 189510,900,000 NGC 5253  
Ursa Major January 190921,000,000 Pinwheel Galaxy (M101) [16] [17]
Canes Venatici 24 August 193713,000,000 IC 4182  
Cepheus 17 July 193925,200,000 NGC 6946 (Fireworks Galaxy) 
Coma Berenices 5 May 194038,000,000 NGC 4725  
Ursa Major 1 September 195121,000,000 Pinwheel Galaxy (M101) [18]
Perseus 11 July 196130,000,000 NGC 1058 Potential supernova impostor [19]
Ursa Major 30 July 197021,000,000 Pinwheel Galaxy (M101) [20] [21] [22]
Centaurus 13 May 197210,900,000 NGC 5253 Followed for more than a year; became the prototypical Type Ia supernova
Hydra 3 July 198315,000,000 Messier 83 First observation of a Type Ib supernova
Andromeda 21 August 198630,000,000 NGC 891 Bright in the radio frequency range
Dorado 1987160,000 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
Ursa Major 28 March 199311,000,000 M81 One of the brightest supernovae in the northern sky since 1954
Virgo 7 March 199450,000,000 NGC 4526
Telescopium 26 April 1998 ?140,000,000 ESO 184-G82 Linked to GRB 980425, which was the first time a gamma-ray burst has been linked to a supernova.
Lynx 12 October 199984,000,000 NGC 2770 First supernovae in this galaxy, where 3 more were detected later.
Lupus 2002160,000,000 NGC 1821 AM Canum Venaticorum-type outburst. [25]
Ursa Major 20028,000,000,000anonymous galaxyFurthest supernova observed through Hubble Deep Field. [26]
Boötes 20034,000,000,000anonymous galaxyAlso known as the "Champagne supernova"
Camelopardalis 31 July 2004
18:15
8,000,000 NGC 2403 NGC 2403 is an outlying member of the M81 Group
Coma Berenices 3 March 20054,700,000,000 ?Announced in 2007 to be the brightest supernova up to that point.
Cetus 27 September 2005865,000,000 ?Notable for having characteristics of both Type Ia and Type IIn.
Pisces 5 October 2005200,000,000 NGC 266 Star could be found on old pictures. [27]
Perseus 18 September 2006240,000,000 NGC 1260 Observed by NASA,
*with a peak of over 70 days, possibly a new type.
Lynx 9 October 200677,000,000 UGC 4904
Virgo Early 2007anonymous dwarf galaxyExtremely 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. [28]
Lynx 31 December 200784,000,000 NGC 2770 Got overshadowed by SN 2008D.
Lynx 9 January 200888,000,000 NGC 2770 First supernova to be observed while it exploded.
Aries 1,000,000,000
(z=0.0613)
anonymous red globular cluster associated with anonymous red elliptical galaxy in cluster Abell 399 Observed in 2009. Supernova associated with a globular cluster [29] [30]
Piscis Austrinus 200966,000,000 NGC 7259 In 2009 classified as supernova. Redesignated as Luminous blue variable (LBV) Supernova impostor. [31] In September 2012 classified as a young type IIn supernova. [32]
Camelopardalis 2 January 2011240,000,000 UGC 3378 Discovered by 10-year-old girl, the youngest person to discover a supernova.
Ursa Major 24 August 201121,000,000 M101 One of the very few extragalactic supernovae visible in 50mm binoculars.
Ursa Major Mid January 201411,500,000 M82 Closest supernova since SN 2004dj in NGC 2403.
Leo 11 November 201414,400,000,000 SP 1149 It is the first detected multiply-lensed supernova, visible within the field of the galaxy cluster MACS J1149+2223.
Virgo 1 April 20151,000,000,000 NGC 4866 [33]
Indus 14 June 20153,800,000,000 APMUKS(BJ) B215839.70−615403.9 Most luminous hypernova ever observed.
IPTF14hls Ursa Major September 2014509,000,000unknownSDSS J092034.44+504148.7 (possible dwarf galaxy)Unusual supernova
Draco 22 February 20163,600,000,000 ?Most luminous supernova-like event to date.
Dorado 14 August 2017517,000,000 NGC 1672
Puppis 15 January 201870,000,000 NGC 2525 [34] [35] [36] [37] [38]
Camelopardalis 2 March 201870,000,000 NGC 2146 First electron capture supernova ever detected
SN 2019hgp Boötes 920,000,000First detected supernova of a Wolf-Rayet star [39] [40]
SN 2020fqv Virgo 31 March 202059,400,000 NGC 4568 Earliest known observation of an explosion, 26 hours after [41] [42] [43]
SN 2020tlf Boötes 2020120,000,000 NGC 5731 First red supergiant observed before, during and after explosion; earliest known observation, at 130 days before explosion [44] [45]
Eridanus 8 September 2021750,000,000 NGC 1325 [46] [47]
Sculptor 23 November 202118.8500,000,000 Cartwheel Galaxy [48] [49]
SN 2022jli Cetus 5 May 202275,000,000 type I-c NGC 157 Type Ic, shows periodicity [50] [51] [52] [53]
Gemini November 2022600,000,000 [54]
SN 2023ixf Ursa Major 19 May 2023
17:27
21,000,000 type II-L Pinwheel Galaxy (M101) [55] Closest and brightest supernova since SN 2014J
Fornax 8 September 2023+13.9450,000,000 NGC 1097 [56] [57] [58] [59] [60] Brightest Supernova Since SN 2023ixf.
Pegasus 28 October 2023783,000,000 NGC 7625 [61] [62]
Grus 12 December 2023816,000,000 NGC 7421 [63]
SN 2023ufx +15.55The most metal-poor supernova found to date. [64]

Supernova statistics

Yearly extragalactic supernovae reported
YearTotalType I Type II LBV
(imposters)
Brighter than
apmag 13
Apmag of brightest
Supernova of that year
2023 [65] 1985914304177210.9 (2023ixf in Messier 101)
2022 [66] 2136817323967412.3 (2022hrs in NGC 4647)
2021 [67] 2366518494655812.0 (2021aefx in NGC 1566)
2020 [68] 2177516484517711.8 (2020ue in NGC 4636)
2019 [69] 1876716524859113.0 (2019np in NGC 3254)
2018 [70] 952512063327512.7 (2018pv in NGC 3941)
2017 [71] 82937462184311.5 (2017cbv in NGC 5643)
2016 [72] 77376812263013.0 (2016coj in NGC 4125)
2015 [73] 44747072144212.9 (2015F in NGC 2442)
2014 [74] 22435281752310.1 (2014J in Messier 82)
2013 [75] 19224981907611.3 (2013aa in NGC 5643)
2012 [76] 12235501528511.9 (2012fr in NGC 1365)
2011 [77] 11294391601079.9 (2011fe in Messier 101)
2010 [78] 9312791357212.8 (2010ih in NGC 2325)
2009 [79] 5762021371013.0 (2009ig in NGC 1015)
2008 [80] 5112511431312.4 (2008ge in NGC 1527)
2007 [81] 6054421301312.0 (2007it in NGC 5530)
2006 [82] 5584181242312.1 (2006dd in NGC 1316)
2005 [83] 385273941212.3 (2005df in NGC 1559)
2004 [84] 343221790211.2 (2004dj in NGC 2403)
2003 [85] 384198891112.3 (2003hv in NGC 1201)
2002 [86] 353163640112.3 (2002ap in Messier 74)
2001 [87] 310108750212.3 (2001e1 in NGC 1448)
2000 [88] 19976491013.1 (2000cx in NGC 528)
2000-2023
 
147135
 
16297
(76.5%)
5000
(23.5%)
95
 
72
 

See also

References

  1. Modern estimates vary widely; see SN 185 for more detail.
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  6. 1 2 "SNR Cat - U Manitoba".
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  79. David Bishop. "Supernova discovery statistics for 2009" . Retrieved 2023-02-21.
  80. David Bishop. "Supernova discovery statistics for 2008" . Retrieved 2023-02-21.
  81. David Bishop. "Supernova discovery statistics for 2007" . Retrieved 2023-02-21.
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  85. David Bishop. "Supernova discovery statistics for 2003" . Retrieved 2023-02-23.
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Further reading