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NGC 830

NGC 830
SDSS image of NGC 830
Observation data (J2000 epoch)
ConstellationCetus
Right ascension02h 08m 58.67851s[1]
Declination−07° 46′ 00.4978″[1]
Redshift0.01349[2]
Heliocentric radial velocity4017 km/s[2]
Distance167.8 Mly (51.44 Mpc)[3]
Apparent magnitude (B)15.0[2]
Characteristics
TypeSB0?[4]
Other designations
MCG -01-06-050, Mrk 1020, PGC 8201[2]

NGC 830 is a barred lenticular galaxy in the constellation Cetus. It is estimated to be about 170 million light-years from the Milky Way[3] and has a diameter of approximately 70,000 light years.[5][6][7]

See also

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References

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  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 830". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-05-24.
  3. ^ a b Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv:astro-ph/0610732. Bibcode:2007ApJ...655..790C. doi:10.1086/510201. S2CID 11672751.
  4. ^ "Results for object NGC 0830 (NGC 830)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2020-05-24.
  5. ^ Ford, Dominic. "The galaxy NGC 830 - In-The-Sky.org". in-the-sky.org. Retrieved 2020-03-18.
  6. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2020-03-18.
  7. ^ "Revised NGC Data for NGC 830". spider.seds.org. Retrieved 2020-03-18.
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