NGC 998
NGC 998 is a spiral galaxy of the constellation Cetus. It is estimated to be 294 million light years from the Milky Way and has a diameter of approximately 90,000 ly. Together with NGC 997, it forms a gravitationally bound pair of galaxies. NGC 998 was by astronomer Albert Marth using on 10 November 1863 a 48-inch - telescope discovered.[4][5][6]
NGC 998 | |
---|---|
SDSS image of NGC 998 | |
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 02h 37m 16.50891s[1] |
Declination | +07° 20′ 08.7169″[1] |
Redshift | 0.02184[2] |
Helio radial velocity | 6476 km/s[2] |
Distance | 303.7 ± 21.4 Mly (93.11 ± 6.56 Mpc)[3] |
Apparent magnitude (B) | 14.6[2] |
Other designations | |
MCG+01-07-015, PGC 9934[2] |
See also
References
- Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
- "NGC 998". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-06-03.
- "Results for object NGC 0998 (NGC 998)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-06-03.
- "Revised NGC Data for NGC 998". spider.seds.org. Retrieved 2020-03-24.
- "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2020-03-24.
- Ford, Dominic. "The galaxy NGC 998 - In-The-Sky.org". in-the-sky.org. Retrieved 2020-03-24.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.