NGC 150
Appearance
(Redirected from SN 1990K)
NGC 150 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Sculptor |
Right ascension | 00h 34m 15.481s[1] |
Declination | −27° 48′ 13.17″[1] |
Redshift | 0.005284[2] |
Heliocentric radial velocity | 1584[2] |
Distance | 68.52 ± 11.07 Mly (21.008 ± 3.395 Mpc) |
Apparent magnitude (V) | 11.13[3] |
Apparent magnitude (B) | 12.04[3] |
Characteristics | |
Type | SB(rs)b:[2] |
Size | 37,400 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] The Type II supernova SN 1990K was detected in NGC 150, and was reported to be similar to SN 1987A.[6]
References
[edit]- ^ 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.
- ^ 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.
- ^ a b c "NGC 150". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 19 March 2017.
- ^ "NASA/IPAC Extragalactic Database". NED results for object NGC 0150. NASA.
- ^ "New General Catalog Objects: NGC 150 – 199". seligman.com. Retrieved 9 September 2016.
- ^ 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.