A | B | C | D | E | F | G | H | CH | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z | 0 | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9
| NGC 110 | |
|---|---|
| Observation data (J2000 epoch) | |
| Right ascension | 00h 27m 25.2s[1] |
| Declination | +71° 25′ 19″[1] |
| Apparent magnitude (V) | 9.0[2] |
| Apparent dimensions (V) | 20′[2] |
| Physical characteristics | |
| Associations | |
| Constellation | Cassiopeia |
NGC 110 is an open star cluster located in the constellation Cassiopeia. It was discovered by the English astronomer John Herschel on October 29, 1831.[2]
It is unknown if the members are physically related, or if the cluster exists at all. It is barely visible against the background sky, and the two dozen member stars seem to be at various distances.[2] If the cluster does exist, it is at least 2,000 light years away.
References
- ^ a b "NGC 110". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 June 2017.
- ^ a b c d "New General Catalog Objects: NGC 100 - 149". cseligman.com. Retrieved 26 June 2017.
External links
- NGC 110 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |
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