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NGC 150

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NGC 150
NGC 150 with DECam
Observation data (J2000 epoch)
ConstellationSculptor
Right ascension00h 34m 15.481s[1]
Declination−27° 48′ 13.17″[1]
Redshift0.005284[2]
Heliocentric 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]

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]

One supernova has been observed in NGC 150. SN 1990K (type II, mag. 14) was discovered by Robert Evans on 25 May 1990.[6][7] It was reported to be similar to SN 1987A.[8]

References

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  1. ^ a b Skrutskie, Michael F.; et al. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
  2. ^ a b c d e "NED results for object NGC 0150". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 19 March 2017.
  3. ^ a b c "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. ^ Evans, R.; Cooper, K.; Sadler, E. (1990). "Supernova 1990K in NGC 150". International Astronomical Union Circular (5022): 1. Bibcode:1990IAUC.5022....1E.
  7. ^ "SN 1990K". Transient Name Server. IAU. Retrieved 6 December 2024.
  8. ^ 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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