SN 2006X
 M100 before and after the supernova explosion | |
| Event type | Supernova  |
|---|---|
| Ia | |
| Date | February 4, 2006 |
| Constellation | Coma Berenices |
| Right ascension | 12h 22m 53.92s |
| Declination | +15° 48′ 31.2″ |
| Epoch | B1950.0 |
| Distance | 65 mly[1] |
| Redshift | 0.0036, 0.007, 0.0067, 0.0071, 0.0068, 0.0037, 0.0043 |
| Host | M100 |
| Peak apparent magnitude | +13[2] |
| Other designations | SN 2006X |
 Related media on Commons | |
SN 2006X was a Type Ia supernova about 65 million light-years away[1] in Messier 100, a spiral galaxy in the constellation Coma Berenices. The supernova was independently discovered in early February 2006 by Shoji Suzuki of Japan and Marco Migliardi of Italy.
SN 2006X is particularly significant because it is a Type Ia supernova. These supernovae are used for measuring distances, so observations of these supernovae in nearby galaxies are needed for calibration. SN 2006X is located in a well-studied galaxy, and it was discovered two weeks before its peak brightness, so it may be extraordinarily useful for understanding supernovae and for calibrating supernovae for distance measurements. It may even be possible to identify the progenitor of this supernova.
References
- ^ a b Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (February 2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 79–813. arXiv:astro-ph/0610732. Bibcode:2007ApJ...655..790C. doi:10.1086/510201.
- ^ Suzuki, Shoji. "in: SUPERNOVAE 2006U, 2006V, 2006W, 2006X". Central Bureau for Astronomical Telegrams. Havard University. Retrieved 2 May 2015.
External links
- Supernova 2006X in M100
- Brightness measures for SN 2006X
- NASA page with images of SN 2006X
- Large collection of SN 2006X images
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