NGC 112

The NGC 112 issue is one that has captured the attention of many as of late. With its relevance in various areas, NGC 112 has managed to establish itself as a point of interest and discussion in today's society. Whether due to its impact on daily life, its influence on popular culture or its importance in technological development, NGC 112 has become a constant topic of conversation. In this article, we will explore different aspects related to NGC 112, from its origin to its possible consequences in the future.
NGC 112
SDSS image of NGC 112
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension00h 26m 48.74910s[1]
Declination+31° 42′ 11.9738″[1]
Redshift0.021028[2]
Heliocentric radial velocity6238 km/s[2]
Distance282.78 ± 0.65 Mly (86.70 ± 0.2 Mpc)[3]
Apparent magnitude (B)14.5[2]
Characteristics
TypeSB(rs)bc?[4]
Other designations
UGC 255, MCG +05-02-013, PGC 1654[2]

NGC 112 is a barred spiral galaxy located in the constellation Andromeda. It was discovered by American astronomer Lewis Swift on September 17, 1885. The galaxy lies approximately 295 million light-years from Earth, and is about 75,000 light-years in diameter.[4]

References

  1. ^ a b 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.
  2. ^ a b c d "NGC 112". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-07.
  3. ^ Tully, R. Brent; et al. (2013). "Cosmicflows-2: The Data". The Astronomical Journal. 146 (4): 86. arXiv:1307.7213. Bibcode:2013AJ....146...86T. doi:10.1088/0004-6256/146/4/86. S2CID 118494842.
  4. ^ a b Seligman, Courtney. "New General Catalogue objects: NGC 100 - 149". cseligman.com. Retrieved 2021-02-07.


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