California Nebula
| Emission nebula | |
|---|---|
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| Observation data: J2000.0 epoch | |
| Right ascension | 04h 03m 18.00s |
| Declination | +36° 25′ 18.0″ |
| Distance | 1,000 ly |
| Apparent magnitude (V) | 6.0 |
| Apparent dimensions (V) | 2.5° long |
| Constellation | Perseus |
| Designations | NGC 1499, Sharpless 220 |
The California Nebula (NGC 1499) is an emission nebula located in the constellation Perseus. It is so named because it appears to resemble the outline of the US State of California on long exposure photographs. It is almost 2.5° long on the sky and, because of its very low surface brightness, it is extremely difficult to observe visually. It can be observed with a Hβ filter (isolates the Hβ line at 486 nm) in a rich-field telescope under dark skies.[1] It lies at a distance of about 1,000 light years from Earth. Its fluorescence is due to excitation of the Hβ line in the nebula by the nearby prodigiously energetic O7 star, xi Persei (also known as Menkib, seen at center below it in the inset at right).[2]
The California Nebula was discovered by E. E. Barnard in 1884.
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California Neb 2007.jpg
Image of the California Nebula with amateur telescope.
References
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).]]. |
- NGC 1499 at SEDS
- Menkhib and the California Nebula by the Wide-field Infrared Survey Explorer (WISE)
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