Astronomy:NGC 538
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Short description: Galaxy in the constellation Cetus
NGC 538 | |
---|---|
SDSS image of NGC 538 | |
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 01h 25m 26.06364s[1] |
Declination | −01° 33′ 02.2258″[1] |
Redshift | 0.017756[1] |
Helio radial velocity | 5276 km/s[1] |
Distance | 250 Mly (77 Mpc)[2] |
Apparent magnitude (B) | 14.58[1] |
Characteristics | |
Type | SB(s)ab:[2] |
Other designations | |
UGC 991, MCG+00-04-130, PGC 5275[1] |
NGC 538 is a barred spiral galaxy in the constellation of Cetus. It is located about 250 million light-years from the Milky Way[2] with a diameter of approximately 95,000 ly.[citation needed] NGC 538 was discovered by the American astronomer Lewis Swift in 1886.[3][4][5]
NGC 538 is estimated to be about 2.5 billion years old.[6]
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "NGC 538". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+538.
- ↑ 2.0 2.1 2.2 Gil de Paz, Armando et al. (December 2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies". The Astrophysical Journal Supplement Series 173 (2): 185–255. doi:10.1086/516636. Bibcode: 2007ApJS..173..185G.
- ↑ Ford, Dominic. "The galaxy NGC 538 - In-The-Sky.org" (in en). https://in-the-sky.org/data/object.php?id=NGC538.
- ↑ "Your NED Search Results". http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=ngc+538&img_stamp=YES.
- ↑ "Revised NGC Data for NGC 538". http://spider.seds.org/ngc/revngcic.cgi?NGC538.
- ↑ Fraser-Mckelvie, Amelia; Brown, Michael J. I.; Pimbblet, Kevin A.; Dolley, Tim; Crossett, Jacob P.; Bonne, Nicolas J. (2016). "A photometrically and spectroscopically confirmed population of passive spiral galaxies". Monthly Notices of the Royal Astronomical Society: Letters 462 (1): L11–L15. doi:10.1093/mnrasl/slw117. Bibcode: 2016MNRAS.462L..11F.
External links
Original source: https://en.wikipedia.org/wiki/NGC 538.
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