Kepler's Supernova
| SN 1604 | |
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| Observation data (Epoch J2000) | |
| Supernova type | Ia [1][2] |
| Remnant type | Shell |
| Host galaxy | Milky Way |
| Constellation | Ophiuchus |
| Right ascension | 17h 30m 42s |
| Declination | −21° 29′ |
| Galactic coordinates | G4.5+6.8 |
| Discovery date | October 9, 1604 |
| Peak magnitude (V) | −2.25 to −2.5 |
| Distance | 20,000 light-years (6.1 kpc) |
| Physical characteristics | |
| Progenitor | Unknown |
| Progenitor type | Unknown |
| Colour (B-V) | Unknown |
| Notable features | Latest observed supernova in our galaxy. Maintained naked-eye visibility for 18 months. |
Supernova 1604, also known as Kepler's Supernova, Kepler's Nova or Kepler's Star, was a supernova of Type Ia[1][2] that occurred in the Milky Way, in the constellation Ophiuchus. Appearing in 1604, it is the most recent supernova to have been unquestionably observed by the naked eye in our own galaxy,[3] occurring no farther than 6 kiloparsecs or about 20,000 light-years from Earth.
Visible to the naked eye, Kepler's Star was brighter at its peak than any other star in the night sky, with an apparent magnitude of −2.5. It was visible during the day for over three weeks.
Johannes Kepler's original drawing depicting the location of the stella nova, marked with an N (8 grid squares down, 4 over from the left)
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The first recorded observation was in northern Italy on October 9, 1604.[4] Johannes Kepler began observing the luminous display on October 17 while working at the imperial court in Prague for Emperor Rudolf II.[5] It was subsequently named after him, even though he was not its first observer, as his observations tracked the object for an entire year and because of his book on the subject, entitled De Stella nova in pede Serpentarii ("On the new star in Ophiuchus's foot", Prague 1606).
The supernova was also recorded in Chinese and Korean sources.[6]
It was the second supernova to be observed in a generation (after SN 1572 seen by Tycho Brahe in Cassiopeia). No further supernovae have since been observed with certainty in the Milky Way, though many others outside our galaxy have been seen since S Andromedae in 1885. SN 1987A in the Large Magellanic Cloud was easily visible to the naked eye.
Strong present day astronomical evidence exists for a Milky Way supernova whose signal would have reached Earth ca. 1680 (Cassiopeia A), and another (G1.9+0.3) whose light should have arrived ca. 1870. There is no historical record of either having been detected at the time, probably because absorption by interstellar dust made them fainter than they would otherwise have been.[7]
The supernova remnant resulting from Kepler's supernova is considered to be one of the prototypical objects of its kind, and is still an object of much study in astronomy.
See also
References
- ↑ 1.0 1.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Delle Colombe L., Discorso di Lodovico Delle Colombe nel quale si dimostra che la nuova Stella apparita l’Ottobre passato 1604 nel Sagittario non è Cometa, ne stella generata, ò creata di nuovo, ne apparente: ma una di quelle che furono da principio nel cielo; e ciò esser conforme alla vera Filosofia, Teologia, e Astronomiche dimostrazioni, Firenze, Giunti, 1606.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Stephenson, F. Richard & Green, David A., Historical Supernovae and their Remnants, Oxford, Clarendon Press, 2002, pp. 60-71.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
Further reading
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External links
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Wikimedia Commons has media related to [[commons:Lua error in Module:WikidataIB at line 506: attempt to index field 'wikibase' (a nil value).|Lua error in Module:WikidataIB at line 506: attempt to index field 'wikibase' (a nil value).]]. |
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