Supernova: Difference between revisions
Jump to navigation
Jump to search
No edit summary |
No edit summary |
||
| Line 26: | Line 26: | ||
==Known supernova candidates== | ==Known supernova candidates== | ||
* [[Eta Carinae]] (Unclear) | |||
* [[Antares]] (c.10,000y) | * [[Antares]] (c.10,000y) | ||
* [[Betelgeuse]] (c.1my) | * [[Betelgeuse]] (c.1my) | ||
Revision as of 09:27, 6 May 2019
- Massive stellar explosion occurring at the end of a star's natural life cycle due to fusion pressure no longer able to balance against gravitational core collapse
- Results in a stellar remnant in the form of either a neutron star or a black hole
- Resulting explosion produces a wavefront of intense radiation, devastating planetary ecosystems within 25-50 ly
- Often also results in a surrounding micronebula, or even full nebula
Known supernovae
- Limited specifically to supernovae within the Milky Way
- Ganidra - c.8000 BCE
- SN 185 - 185
- SN 386 - 386
- SN 393 - 393
- SN 1006 - 1006
- SN 1054 - 1054
- SN 1181 - 1181
- SN 1572 - 1572
- SN 1604 - 1604
- Cassiopeia A - c.1680
- SNR G1.9+0.3 - c.1868
- FGC-758 - 2168
- Beta Volanis - 2230s
- Alpha Lupi - 2236
- Minara - 2268
- Beta Niobe - 2269
- Beta Stromgren - 2366
Known supernova candidates
- Eta Carinae (Unclear)
- Antares (c.10,000y)
- Betelgeuse (c.1my)
- Deneb (millions of years)