Supernova
designation
(year)
| Constellation
| Apparent
magnitude
| Distance
(light years)
| Type
| Galaxy
| Comments
|
---|
7003200700000000000♠SN 2007bi
| Virgo
| 7001183000000000000♠+18.3
| | 7000100000000000000♠Ic?
| 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.[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-14"][SIZE=2][14][/SIZE][/URL]
|
MENeaC Abell399.3.14.0
| | 28.7
| z=0.0613
| Ia
| anonymous red globular cluster associated with anonymous red elliptical galaxy in cluster Abell 399
| First type Ia supernova associated with a globular cluster [URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-2015arXiv150503407G-15"][SIZE=2][15][/SIZE][/URL][URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-UCB-2015-06-04-16"][SIZE=2][16][/SIZE][/URL]
|
7003105400000000000♠SN 1054
| Taurus
| 2999400000000000000♠–6
| 6,500
| 7000200000000000000♠II
| Milky Way
| Remnant is the Crab Nebula with its pulsar (neutron star)
|
7003100600000000000♠SN 1006
| Lupus
| 2999250000000000000♠–7.5[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-7"][SIZE=2][7][/SIZE][/URL]
| 7,200
| 7000100000000000000♠Ia
| Milky Way
| Widely observed on Earth; in apparent magnitude, the brightest stellar event in recorded history.[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-NOAO1-8"][SIZE=2][8][/SIZE][/URL]
|
7003157200000000000♠SN 1572
| Cassiopeia
| 2999600000000000000♠–4.0
| 8,000
| 7000100000000000000♠Ia
| Milky Way
| Tycho's Nova
|
7002185000000000000♠SN 185
| Centaurus
| 2999600000000000000♠−4 (?) [URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-1"][SIZE=2][1][/SIZE][/URL]
| 8,200
| 7000100000000000000♠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,[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-2"][SIZE=2][2][/SIZE][/URL] making it comparable to SN 1572. Some researchers have suggested it was a comet, not a supernova.[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-Chin-3"][SIZE=2][3][/SIZE][/URL][URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-Zhao-4"][SIZE=2][4][/SIZE][/URL]
|
7003118100000000000♠SN 1181
| Cassiopeia
| 5000000000000000000♠0
| 8,500
| | Milky Way
| |
7003168000000000000♠Cas A,
ca. 1680
| Cassiopeia
| 7000500000000000000♠+5
| 9,000
| 7000200000000000000♠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
|
7003160400000000000♠SN 1604
| Ophiuchus
| 2999700000000000000♠–3
| 14,000
| 7000100000000000000♠Ia
| Milky Way
| Kepler's Star; most recent readily visible supernova within the Milky Way
|
7002386000000000000♠SN 386
| Sagittarius
| 7000150000000000000♠+1.5
| 14,700
| 7000200000000000000♠II
| Milky Way
| The candidate remnant is G11.2-0.3.[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-SEDS_SN_386-5"][SIZE=2][5][/SIZE][/URL][URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-6"][SIZE=2][6][/SIZE][/URL]
|
7003186800000000000♠SNR G1.9+0.3,
ca. 1868
| Sagittarius
| | 25,000
| | Milky Way
| "Posthumously" discovered in 1985; age determined in 2008
|
7002393000000000000♠SN 393
| Scorpius
| 5000000000000000000♠–0
| 34,000
| | Milky Way
| |
7003198700000000000♠SN 1987A
| Dorado
| 7000290000000000000♠+2.9
| 160,000
| 7000200000000000000♠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
|
7003188500000000000♠SN 1885A
| Andromeda
| 7000700000000000000♠+7
| 2,400,000
| 7000100000000000000♠Ipec
| Andromeda Galaxy
| First observation of an extragalactic supernova
|
7003189500000000000♠SN 1895B
| Centaurus
| 7000800000000000000♠+8.0[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-cbat-9"][SIZE=2][9][/SIZE][/URL]
| 10,900,000
| | NGC 5253
| |
7003197200000000000♠SN 1972E
| Centaurus
| 7000870000000099999♠+8.7 [URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-11"][SIZE=2][11][/SIZE][/URL]
| 10,900,000
| 7000100000000000000♠Ia
| NGC 5253
| Followed for more than a year; became the prototypical Type Ia supernova
|
7003199300000000000♠SN 1993J
| Ursa Major
| 7001108000000000000♠+10.8
| 11,000,000
| 7000200000000000000♠IIb
| M81
| One of the brightest supernovae in the northern sky since 1954
|
7003201400000000000♠SN 2014J
| Ursa Major
| 7001100000000000000♠+10.5
| 11,500,000
| 7000100000000000000♠Ia
| M82
| Closest supernova since SN 2004dj in NGC 2403
|
7003193700000000000♠SN 1937C
| | 7000800000000000000♠+8.4[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-cbat-9"][SIZE=2][9][/SIZE][/URL]
| 13,000,000
| 7000100000000000000♠Ia
| IC 4182
| |
7003198300000000000♠SN 1983N
| Hydra
| 7001118000000000000♠+11.8
| 15,000,000
| 7000100000000000000♠Ib
| Messier 83
| First observation of a Type Ib supernova
|
7003201100000000000♠SN 2011fe
| Ursa Major
| 7001100000000000000♠+10.0
| 21,000,000
| 7000100000000000000♠Ia
| M101
| One of the very few extragalactic supernovae visible in 50mm binoculars.
|
7003196100000000000♠SN 1961V
| Perseus
| 7001125000000000000♠+12.5
| 30,000,000
| 7000200000000000000♠II?
| NGC 1058
| Potential supernova impostor[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-universetoday-10"][SIZE=2][10][/SIZE][/URL]
|
7003198600000000000♠SN 1986J
| Andromeda
| 7001184009999900000♠+18.4
| 30,000,000
| 7000200000000000000♠IIn
| NGC 891
| Bright in the radio frequency range
|
7003194000000000000♠SN 1940B
| Coma Berenices
| 7001128000000000000♠+12.8
| 38,000,000
| 7000200000000000000♠II-P
| NGC 4725
| |
7003200800000000000♠SN 2008D
| Lynx
| | 88,000,000
| 7000100000000000000♠Ibc
| NGC 2770
| First supernova to be observed while it exploded.
|
7003200200000000000♠SN 2002bj
| Lupus
| 7001147000000000000♠+14.7
| 160,000,000
| 7000100000000000000♠.Ia
| NGC 1821
| AM Canum Venaticorum-type outburst.[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-ucnews-12"][SIZE=2][12][/SIZE][/URL]
|
7003200500000000000♠SN 2005gl
| Pisces
| 7001165000000000000♠+16.5
| 200,000,000
| 7000200000000000000♠II-n
| NGC 266
| Star could be found on old pictures.[URL="https://en.wikipedia.org/wiki/List_of_supernovae#cite_note-13"][SIZE=2][13][/SIZE][/URL]
|
7003200600000000000♠SN 2006gy
| Perseus
| 7001150000000000000♠+15
| 240,000,000
| 7000200000000000000♠IIn [SIZE=2](*)[/SIZE]
| NGC 1260
| Observed by NASA,
[SIZE=2]*[/SIZE]with a peak of over 70 days, possibly a new type.
|
7003200500000000000♠SN 2005gj
| | | 865,000,000
| 7000100000000000000♠Ia/II-n
| ?
| Notable for having characteristics of both Type Ia and Type IIn.
|
7003200300000000000♠SN 2003fg
| Boötes
| | 4,000,000,000
| 7000100000000000000♠Ia
| anonymous galaxy
| Also known as the "Champagne supernova"
|
7003200500000000000♠SN 2005ap
| Coma Berenices
| | 4,700,000,000
| 7000200000000000000♠II
| ?
| Announced in 2007 to be the brightest supernova up to that point.
|
7003200400000000000♠SN 2004dj
| Camelopardalis
| | 8,000,000,000
| 7000100000000000000♠Ia ( SAB)
| NGC 2403
| NGC 2403 is an outlying member of the M81 Group
|