NGC 600
NGC 600 is an emission-line galaxy[4] in the constellation Cetus. It was discovered by William Herschel on 10 September 1785.[6] The galaxy has a diameter of 70,000 light years. It is also approximately 90 million light years from the Milky Way.[1]
| NGC 600 | |
|---|---|
 SDSS image of NGC 600 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 33m 05.3s[1] |
| Declination | −07° 18′ 41″[1] |
| Redshift | 0.006144 ± 0.000003[1] |
| Helio radial velocity | 1842 km/s[1] |
| Distance | 92.7 Mly (28.41 Mpc)[1] |
| Group or cluster | [CHM2007] HDC 81,[2] [T2015] nest 200207[3] |
| Apparent magnitude (V) | 12.5±0.1 |
| Apparent magnitude (B) | 13.1[4] |
| Absolute magnitude (V) | −15.69 |
| Characteristics | |
| Type | (R')SB(rs)d |
| Other designations | |
| MCG-01-05-00, PGC 5777[4] | |
References: [5] | |
References
- "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2020-07-21.
- "[CHM2007] HDC 81". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-07-21.
- "[T2015] nest 200207". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-07-21.
- "NGC 600". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-07-21.
- Ford, Dominic. "The galaxy NGC 600 - In-The-Sky.org". in-the-sky.org.
- Seligman, Courtney. "New General Catalogue objects: NGC 600 - 649". cseligman.com. Retrieved 2020-07-21.
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