NGC 600 | |
---|---|
SDSS image of NGC 600 | |
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 01 33 05.3 |
Declination | −07° 18′ 41″ |
Redshift | 0.006144 ± 0.000003 |
Heliocentric radial velocity | 1842 km/s |
Distance | 92.7 Mly (28.41 Mpc) |
Group or cluster | HDC 81, nest 200207 |
Apparent magnitude (V) | 12.5±0.1 |
Apparent magnitude (B) | 13.1 |
Absolute magnitude (V) | −15.69 |
Characteristics | |
Type | (R')SB(rs)d |
Other designations | |
MCG -01-05-007, PGC 5777 | |
References: |
NGC 600 is an emission-line galaxy in the constellation Cetus. It was discovered by William Herschel on 10 September 1785. The galaxy has a diameter of 70,000 light-years. It is also approximately 90 million light-years from the Milky Way.
See also
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.
External links
- Media related to NGC 600 at Wikimedia Commons
This spiral galaxy article is a stub. You can help Misplaced Pages by expanding it. |