NGC 150

NGC 150 (also known as PGC 2052) is a barred spiral galaxy in the constellation Sculptor. It is about 70 million light years away from the solar system, and it has a diameter of about 55,000 light years.[4] It was discovered on 20 November 1886, by Lewis A. Swift.[5] The Type II supernova SN 1990K was detected in NGC 150, and was reported to be similar to SN 1987A.[6]

NGC 150
NGC 150
Observation data (J2000 epoch)
ConstellationSculptor
Right ascension00h 34m 15.481s[1]
Declination−27° 48′ 13.17″[1]
Redshift0.005284[2]
Helio radial velocity1584[2]
Distance68.52 ± 11.07 Mly (21.008 ± 3.395 Mpc)
Apparent magnitude (V)11.13[3]
Apparent magnitude (B)12.04[3]
Characteristics
TypeSB(rs)b:[2]
Size37,400 ly (11,470 pc)[2]
Apparent size (V)3.9′ × 1.9′[2]
Other designations
UGCA 7, MGC-05-02-018, PGC 2052[3]

References
  1. Skrutskie, M. (2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708.
  2. "NED results for object NGC 0150". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 19 March 2017.
  3. "NGC 150". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 19 March 2017.
  4. "NASA/IPAC Extragalactic Database". NED results for object NGC 0150. NASA.
  5. "New General Catalog Objects: NGC 150 – 199". seligman.com. Retrieved 9 September 2016.
  6. Cappellaro, E.; Danziger, I. J.; della Valle, M.; Gouiffes, C.; Turatto, M. (1995). "The bright linear type II SN 1990K". Astronomy and Astrophysics. 293: 723–732. Bibcode:1995A&A...293..723C.
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