List of supernovae

From Wikipedia, the free encyclopedia

SN 1054 remnant
(Crab Nebula)

This is a list of supernovae that are of historical significance. These include supernovae that were observed prior to the availability of photography, and individual events that have been the subject of a scientific paper that contributed to supernova theory.

An alternative, complete and updated list can be found in the Open Supernova Catalog.

List[]

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

Supernova
designation
(year) 		Constellation Apparent
magnitude 		Distance
(light years) 		Type Galaxy Comments
SN 185 Centaurus −4 (?)[1] 9,100[2] Ia (?) 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]
SN 386 Sagittarius +1.5 14,700 II 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]
SN 393 Scorpius –0 34,000 II/Ib Milky Way "possible SN",[6] could also be classical nova or something else[9]
SN 1006 Lupus –7.5[10] 7,200 Ia Milky Way Widely observed on Earth; in apparent magnitude, the brightest stellar event in recorded history.[11]
SN 1054 Taurus –6 6,500 II Milky Way Remnant is the Crab Nebula with its pulsar (neutron star)
SN 1181 Cassiopeia 0 8,500   Milky Way "possible SN",[6]

probably no SN but activity at WR-star[12]

SN 1572 Cassiopeia –4.0 8,000 Ia Milky Way Tycho's Nova
SN 1604 Ophiuchus –3 14,000 Ia Milky Way Kepler's Star; most recent readily visible supernova within the Milky Way
Cas A,
ca. 1680 		Cassiopeia +5 9,000 IIb Milky Way Apparently never visually conspicuous, due to interstellar dust; but the remnant, Cas A, is the brightest extrasolar radio source in the sky
SNR G1.9+0.3,
ca. 1868 		Sagittarius (visible light masked by dust) 25,000 Ia Milky Way Located near the galactic center; "Posthumously" discovered in 1985; age determined in 2008
SN 1885A Andromeda +7 2,500,000 Ipec Andromeda Galaxy First observation of an extragalactic supernova
SN 1895B Centaurus +8.0[13] 10,900,000 Ia NGC 5253  
Canes Venatici +8.4[13] 13,000,000 Ia  
SN 1939C Cepheus +13 25,200,000 I Fireworks Galaxy  
SN 1940B Coma Berenices +12.8 38,000,000 II-P NGC 4725  
SN 1961V Perseus +12.5 30,000,000 II? NGC 1058 Potential supernova impostor[14]
SN 1972E Centaurus +8.7[15] 10,900,000 Ia NGC 5253 Followed for more than a year; became the prototypical Type Ia supernova
Hydra +11.8 15,000,000 Ib Messier 83 First observation of a Type Ib supernova
Andromeda +18.4 30,000,000 IIn NGC 891 Bright in the radio frequency range
SN 1987A Dorado +2.9 160,000 IIpec 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
SN 1993J Ursa Major +10.8 11,000,000 IIb M81 One of the brightest supernovae in the northern sky since 1954
SN 1994D Virgo +15.2 50,000,000 Ia NGC 4526
SN 1998bw Telescopium ? 140,000,000 Ic Linked to GRB 980425, which was the first time a gamma-ray burst has been linked to a supernova.
SN 1999eh Lynx +18.3 +/- 0.3 84,000,000 I NGC 2770 First supernovae in this galaxy, where 3 more was detected later.
SN 2002bj Lupus +14.7 160,000,000 IIn AM Canum Venaticorum-type outburst.[16]
SN 2003fg Boötes 4,000,000,000 Ia anonymous galaxy Also known as the "Champagne supernova"
SN 2004dj Camelopardalis 8,000,000 II-P NGC 2403 NGC 2403 is an outlying member of the M81 Group
SN 2005ap Coma Berenices 4,700,000,000 II ? Announced in 2007 to be the brightest supernova up to that point.
SN 2005gj Cetus 865,000,000 Ia/II-n ? Notable for having characteristics of both Type Ia and Type IIn.
SN 2005gl Pisces +16.5 200,000,000 II-n NGC 266 Star could be found on old pictures.[17]
SN 2006gy Perseus +15 240,000,000 IIn (*) NGC 1260 Observed by NASA,
*with a peak of over 70 days, possibly a new type.
SN 2007bi Virgo +18.3 Ia 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.[18]
SN 2007uy Lynx +16.8 84,000,000 Ibc NGC 2770 Got overshadowed by SN 2008D.
SN 2008D Lynx 88,000,000 Ibc NGC 2770 First supernova to be observed while it exploded.
MENeaC Abell399.3.14.0 Aries +28.7 1,000,000,000
(z=0.0613) 		Ia anonymous red globular cluster associated with anonymous red elliptical galaxy in cluster Observed in 2009. Supernova associated with a globular cluster[19][20]
SN 2009ip Piscis Austrinus 66,000,000 IIn NGC 7259 In 2009 classified as supernova. Redesignated as Luminous blue variable (LBV) Supernova impostor.[21] In September 2012 classified as a young type IIn supernova.[22]
SN 2010lt Camelopardalis +17.0 240,000,000 Ia (sub-luminous) Discovered by 10-year-old girl, the youngest person to discover a supernova.
SN 2011fe Ursa Major +10.0 21,000,000 Ia M101 One of the very few extragalactic supernovae visible in 50mm binoculars.
SN 2014J Ursa Major +10.5 11,500,000 Ia M82 Closest supernova since SN 2004dj in NGC 2403.
ASASSN-15lh SN 2015L Indus +16.9 3,800,000,000 Ic Most luminous hypernova ever observed.
IPTF14hls Ursa Major +17.7 509,000,000 unknown ? (dwarf galaxy) Unusual supernova
SN 2016aps Draco 3,600,000,000 SLSB-II ? Most luminous supernova-like event to date.
SN 2018zd Camelopardalis +17.8 70,000,000 Ia-csm NGC 2146 First electron capture supernova ever
SN 2019hgp Boötes +20.16 920,000,000 Icn - First detected supernova of a Wolf-Rayet star[23][24]
SN 2020fqv Virgo +19.0 59,400,000 IIb NGC 4568 Earliest known observation of an explosion, 26 hours after[25][26][27]
SN 2020tlf Boötes 120,000,000 First red supergiant observed before, during and after explosion; earliest known observation, at 130 days before explosion[28][29]

See also[]

References[]

  1. ^ Modern estimates vary widely; see SN 185 for more detail.
  2. ^ Ksenofontov, L. T.; Berezhko, E. G.; Völk, H. J. (2005-04-01). "Magnetic field amplification in Tycho and other shell-type supernova remnants". Astronomy & Astrophysics. 433 (1): 229–240. arXiv:astro-ph/0409453. Bibcode:2005A&A...433..229V. doi:10.1051/0004-6361:20042015. ISSN 0004-6361. S2CID 16726273.
  3. ^ "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.
  4. ^ Chin YN, Huang YL (1994). "Identification of the Guest Star of AD 185 as a comet rather than a supernova". Nature. 371 (6496): 398–399. Bibcode:1994Natur.371..398C. doi:10.1038/371398a0. S2CID 4240119. Archived from the original on 2013-11-05.
  5. ^ Zhao FY, Strom RG, Jiang SY (2006). "The Guest Star of AD185 Must Have Been a Supernova". Chinese Journal of Astronomy and Astrophysics. 6 (5): 635–40. Bibcode:2006ChJAA...6..635Z. doi:10.1088/1009-9271/6/5/17.
  6. ^ a b c "SNR Cat - U Manitoba".{{cite web}}: CS1 maint: url-status (link)
  7. ^ SEDS. "Supernova 386".
  8. ^ National Radio Astronomy Observatory (NRAO). "The Supernova of 386 AD". Archived from the original on 2018-10-06. Retrieved 2012-09-02.
  9. ^ a b Hoffmann, Susanne M; Vogt, Nikolaus (2020-09-11). "A search for the modern counterparts of the Far Eastern guest stars 369 CE, 386 CE and 393 CE". Monthly Notices of the Royal Astronomical Society. 497 (2): 1419–1433. arXiv:2007.01013. doi:10.1093/mnras/staa1970. ISSN 0035-8711.
  10. ^ Winkler, P. Frank; Gupta, Gaurav; Long, Knox S. (2003). "The SN 1006 Remnant: Optical Proper Motions, Deep Imaging, Distance, and Brightness at Maximum". The Astrophysical Journal. 585 (1): 324–335. arXiv:astro-ph/0208415. Bibcode:2003ApJ...585..324W. doi:10.1086/345985. S2CID 1626564.
  11. ^ "Astronomers Peg Brightness of History's Brightest Star" (Press release). National Optical Astronomy Observatory. 2003-03-05. Archived from the original on 2003-04-02. Retrieved 2009-01-12.
  12. ^ Ritter, Andreas; Parker, Quentin A.; Lykou, Foteini; Zijlstra, Albert A.; Guerrero, Martín A.; Le Dû, Pascal (2021-09-01). "The Remnant and Origin of the Historical Supernova 1181 AD". The Astrophysical Journal Letters. 918 (2): L33. arXiv:2105.12384. doi:10.3847/2041-8213/ac2253. ISSN 2041-8205.
  13. ^ a b "List of Supernovae". Central Bureau for Astronomical Telegrams. Harvard University. Retrieved 2021-07-09.
  14. ^ Voisey, Jon (5 November 2010). "What was SN 1961V?". Universe Today. Retrieved 1 August 2011.
  15. ^ Ardeberg, A.; de Groot, M. (1973). "The 1972 supernova in NGC 5253. Photometric results from the first observing season". Astronomy & Astrophysics. 28: 295–304. Bibcode:1973A&A....28..295A.
  16. ^ Sanders, Robert. "Rapid supernova could be new class of exploding star". UC Newsroom. University of California, Berkeley. Archived from the original on 2011-06-13. Retrieved 2009-11-06.
  17. ^ David Bishop (2005). "Supernova 2005gl in NGC 266". Central Bureau Electronic Telegrams. Rochester Academy of Science. 250: 1. Bibcode:2005CBET..250....1P. Retrieved 26 August 2012.
  18. ^ Science Daily, "Superbright Supernova Is First of Its Kind", 5 December 2009 (accessed 2009-12-15)
  19. ^ Melissa L. Graham; David J. Sand; Dennis Zaritsky; Chris J. Pritchet (13 May 2015). "Confirmation of Hostless Type Ia Supernovae Using Hubble Space Telescope Imaging". The Astrophysical Journal. 807 (1): 83. arXiv:1505.03407. Bibcode:2015ApJ...807...83G. doi:10.1088/0004-637X/807/1/83. S2CID 118555601.
  20. ^ Robert Sanders (4 June 2015). "Exiled stars explode far from home". UC Berkeley News Center.
  21. ^ "Supernova impostor explodes for real". www.newscientist.com. Retrieved November 29, 2017.
  22. ^ Maza, J.; Hamuy, M.; Antezana, R.; Gonzalez, L.; Lopez, P.; Silva, S.; Folatelli, G.; Iturra, D.; Cartier, R.; Forster, F.; Marchi, S.; Rojas, A.; Pignata, G.; Conuel, B.; Reichart, D.; Ivarsen, K.; Haislip, J.; Crain, A.; Foster, D.; Nysewander, M.; Lacluyze, A. (2009). "Supernova 2009ip in NGC 7259". Central Bureau Electronic Telegrams. 1928: 1. Bibcode:2009CBET.1928....1M. Archived from the original on September 11, 2016. Retrieved November 29, 2017.
  23. ^ Gal-Yam, A.; Bruch, R.; Schulze, S.; Yang, Y.; Perley, D. A.; Irani, I.; Sollerman, J.; Kool, E. C.; Soumagnac, M. T.; Yaron, O.; Strotjohann, N. L. (12 January 2022). "A WC/WO star exploding within an expanding carbon–oxygen–neon nebula". Nature. 601 (7892): 201–204. arXiv:2111.12435. doi:10.1038/s41586-021-04155-1. ISSN 1476-4687.
  24. ^ "Astronomers discover first supernova explosion of a Wolf-Rayet star". Instituto de Astrofísica de Canarias • IAC. Retrieved 2022-02-08.
  25. ^ Jenner, Lynn (2021-10-19). "Hubble Gives Unprecedented, Early View of a Doomed Star's Destruction". NASA. Retrieved 2021-11-05.
  26. ^ Gough, Evan (2021-10-29). "Quick Action Let Hubble Watch the Earliest Stages of an Unfolding Supernova Detonation". Universe Today. Retrieved 2021-11-05.
  27. ^ Tinyanont, Samaporn; Ridden-Harper, R; Foley, R J; Morozova, V; Kilpatrick, C D; Dimitriadis, G; DeMarchi, L; Gagliano, A; Jacobson-Galán, W V; Messick, A; Pierel, J D R (2021-10-26). "Progenitor and close-in Circumstellar Medium of Type II Supernova 2020fqv from high-cadence photometry and ultra-rapid UV spectroscopy". Monthly Notices of the Royal Astronomical Society (stab2887). arXiv:2110.10742. doi:10.1093/mnras/stab2887. ISSN 0035-8711.
  28. ^ Jacobson-Galán, W. V.; Dessart, L.; Jones, D. O.; Margutti, R.; Coppejans, D.L.; Dimitriadis, G.; Foley, R. J.; Kilpatrick, C. D.; Matthews, D. J.; Rest, S.; Terreran, G.; Aleo, P. D.; Auchettl, K.; Blanchard, P. K.; Coulter, D. A.; Davis, K. W.; de Boer, T. J. L.; DeMarchi, L.; Drout, M. R.; Earl, N.; Gagliano, A.; Gall, C.; Hjorth, J.; Huber, M. E.; Ibik, A. L.; Milisavljevic, D.; Pan, Y.-C.; Rest, A.; Ridden-Harper, R.; Rojas-Bravo, C.; Siebert, M. R.; Smith, K. W.; Taggart, K.; Tinyanont, S.; Wang, Q.; Zenati, Y. (6 January 2022). "Final Moments. I. Precursor Emission, Envelope Inflation, and Enhanced Mass Loss Preceding the Luminous Type II Supernova 2020tlf". The Astrophysical Journal. American Astronomical Society. 924 (1): 15. doi:10.3847/1538-4357/ac3f3a. Retrieved 16 January 2022.
  29. ^ Anderson, Paul Scott (14 January 2022). "Dying star's explosive end seen by astronomers". EarthSky. Deborah Byrd. Retrieved 16 January 2022.

Further reading[]

  • Green, David A. (2015). Orchiston, Wayne; Green, David A.; Strom, Richard (eds.). Historical Supernova Explosions in Our Galaxy and Their Remnants. New Insights From Recent Studies in Historical Astronomy: Following in the Footsteps of F. Richard Stephenson, Astrophysics and Space Science Proceedings. Vol. 43. Switzerland: Springer International Publishing. pp. 91–100. doi:10.1007/978-3-319-07614-0_7. ISBN 978-3-319-07613-3.

External links[]

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