| 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] |
| Heliocentric 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] | |
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]
- ^ a b c d e f "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.
- ^ a b c "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.
-
Media related to
NGC 600 at Wikimedia Commons
 | This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |
| 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] |
| Heliocentric 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] | |
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]
- ^ a b c d e f "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.
- ^ a b c "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.
-
Media related to
NGC 600 at Wikimedia Commons
|
| This spiral galaxy article is a stub. You can help Wikipedia by expanding it. |