List of supernovae
Nowadays, with the help of automated search programs, thousands of supernovae are discovered every year that are millions of light years away in other galaxies. In relation to a single galaxy, supernovae are usually comparatively rare events (few events per millennium).
The last directly observed supernova within the Milky Way was the Kepler from 1604. Around 1680 another one took place, which was only later identified with certainty with modern observation methods.
The naming is done according to a systematic scheme by the year followed by one or two letters of the Latin alphabet.
list
designation | Constellation | Type |
Apparent brightness at maximum (mag) |
Absolute brightness at maximum (mag) |
Galaxy | approximate distance (Lj) | Remarks |
---|---|---|---|---|---|---|---|
SN 185 | Cen | Yes | −7 | −19.2 | Milky Way | 9100 | oldest described supernova in history |
SN 393 | Sco | II | 0 | −15.1 | Milky Way | 34000 | |
SN 1006 | Lup | I. | −7.5 | −19.2 | Milky Way | 7000 | |
SN 1054 | dew | II | −6 | −17.5 | Milky Way | 6500 | Remnant is the Crab Nebula (M 1) |
SN 1181 | Cas | II | 0 | −12.1 | Milky Way | 8500 | |
SN 1572 | Cas | Yes | -4 | −15.9 | Milky Way | 8000 | by Tycho Brahe discovered and Nova called |
SN 1604 | Oph | Yes | -3 | −16.2 | Milky Way | 14000 | also Kepler's Supernova or Kepler's Star called |
SN 1680 | Cas | IIb | +6 | −6.6 | Milky Way | 11000 | |
SN 1885A | And | Yes | +7 | −17.4 | Andromeda Galaxy | 2.5 million | first observed supernova outside the Milky Way |
SN 1940B | Com | II P | +12.8 | −17.5 | NGC 4725 | 38 million | |
SN 1968L | Hya | II P | +12 | −16.3 | Messier 83 | 15.2 million | The first supernova to be discovered visually since the invention of the telescope |
SN 1972E | Cen | Yes | +8.7 | −18.9 | NGC 5253 | 10.9 million | |
SN 1979C | Com | II L | +12.1 | −18.8 | Messier 100 | 50 million | |
SN 1983N | Hya | Ib | +11.8 | −16.5 | Messier 83 | 15.2 million | |
SN 1986J | And | IIn | +18.4 | −11.4 | NGC 891 | 30 million | |
SN 1987A | Dor | II P | +2.9 | −15.6 | Large Magellanic Cloud | 160000 | The first supernova in which the previous star could be identified. |
SN 1993J | UMa | IIb | +10.8 | −16.8 | Messier 81 | 11 million | |
SN 1994D | Vir | IIb | +11.8 | −19.3 | NGC 4526 | 55 million | |
SN 2005ap | Com | II | +18.5 | −22.3 | SDSS J130114 + 2743 | 4.7 billion | It was not until 2007 that it was discovered that it shone 300 times brighter than a normal Type II supernova |
SN 2005cs | CVn | II | +14 | −15.6 | Messier 51 | 27 million | |
SN 2006gy | By | IIn | +15 | −19.3 | NGC 1260 | 240 million | |
SN 2007bi | Vir | 1.7 billion | first confirmed couple instability supernova | ||||
SN 2008D | Lyn | Ibc | +17.5 | −14.7 | NGC 2770 | 88 million | |
SN 2011dh | UMa | II P | +12.5 | −16.7 | Messier 51 | 23 million | |
SN 2011fe | UMa | Yes | +10.0 | −19.0 | Messier 101 | 21 million | |
SN 2014J | UMa | Yes | Messier 82 | 12 million | |||
SN 2015L | Ind | I. | +16.9 | −23.4 | APMUKS (BJ) B215839.70−615403.9. | 3.8 billion | 2015 strongest observed supernova |
Web links
Individual evidence
- ↑ Bright supernova. Astronomy Section Rochester Academy of Science. Retrieved October 9, 2019 .