NGC 150

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NGC 150
NGC 150 DECam.jpg
NGC 150 imaged by DECam
Observation data (J2000 epoch)
Constellation Sculptor
Right ascension 00h 34m 17.0652s [1]
Declination −27° 48′ 21.961″ [1]
Redshift 0.005294 [1]
Heliocentric radial velocity 1587 ± 1 km/s [1]
Distance 62.92 ± 2.34  Mly (19.291 ± 0.717  Mpc)
Apparent magnitude  (V)11.13 [2]
Apparent magnitude  (B)12.04 [2]
Characteristics
Type SB(rs)b? [1]
Size94,300  ly (28.90  kpc) [1]
Apparent size  (V)3.9′ × 1.9′ [1]
Other designations
ESO 410- G 019, IRAS 00317-2804, UGCA 7, MCG -05-02-018, PGC 2052 [1]

NGC 150 (also known as PGC 2052) is a barred spiral galaxy in the constellation Sculptor. It is about 63 million light years away from the Solar System, and it has a diameter of about 94,000 light years. [3] It was discovered by Lewis A. Swift on 20 November 1886. [4]

Contents

Supernovae

Two supernovae have been observed in NGC 150:

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 1448</span> Galaxy in the constellation Horologium

NGC 1448 is an unbarred spiral galaxy seen nearly edge-on in the constellation Horologium. It is at a distance of 55 million light years from Earth. It was discovered by British astronomer John Herschel on 24 October 1835. Herschel observed the galaxy again on 14 December 1835, resulting in it being listed twice in the New General Catalogue, as NGC 1448 and as NGC 1457.

<span class="mw-page-title-main">NGC 132</span> Spiral galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 337</span> Galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 7038</span> Galaxy in the constellation Indus

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<span class="mw-page-title-main">NGC 958</span> Galaxy in the constellation Cetus

NGC 958 is a barred spiral galaxy in the constellation of Cetus. Its velocity with respect to the cosmic microwave background is 5505 ± 17 km/s, which corresponds to a Hubble distance of 81.20 ± 5.69 Mpc. However, 19 non-redshift measurements give a distance of 58.93 ± 12.91 Mpc. The galaxy was discovered by German-British astronomer William Herschel on 20 September 1784.

<span class="mw-page-title-main">NGC 6754</span> Galaxy in the constellation Telescopium

NGC 6754 is a barred spiral galaxy in the constellation of Telescopium. Its velocity with respect to the cosmic microwave background is 3176 ± 11 km/s, which corresponds to a Hubble distance of 152.8 ± 10.7 Mly (46.84 ± 3.29 Mpc). Additionally, 10 non-redshift measurements give a distance of 137.15 ± 4.19 Mly (42.05 ± 1.285 Mpc). It was discovered by British astronomer John Herschel on 8 July 1834.

<span class="mw-page-title-main">NGC 846</span> Galaxy in the constellation Andromeda

NGC 846(also known as NGC 847) is a barred spiral galaxy located around 235 million light-years away in the constellation Andromeda. NGC 846 was discovered on November 22nd, 1876 by the French astronomer Édouard Stephan, and it has a diameter of around 162,000 light-years. NGC 846 is not known to have much star-formation, and it is not known to have an active galactic nucleus.

References

  1. 1 2 3 4 5 6 7 8 "Results for object NGC 0150". NASA/IPAC Extragalactic Database. NASA and Caltech . Retrieved 15 January 2025.
  2. 1 2 "NGC 150". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 19 March 2017.
  3. ↑ "NASA/IPAC Extragalactic Database". NED results for object NGC 0150. NASA.
  4. ↑ "New General Catalog Objects: NGC 150 – 199". seligman.com. Retrieved 9 September 2016.
  5. ↑ Evans, R.; Cooper, K.; Sadler, E. (1990). "Supernova 1990K in NGC 150". International Astronomical Union Circular (5022): 1. Bibcode:1990IAUC.5022....1E.
  6. ↑ "SN 1990K". Transient Name Server. IAU . Retrieved 6 December 2024.
  7. ↑ 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.
  8. ↑ "SN 2025mb". Transient Name Server. IAU . Retrieved 15 January 2025.
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