NGC 3172

NGC 3172
NGC 3172 imaged by Pan-STARRS
Observation data (J2000 epoch)
ConstellationUrsa Minor
Right ascension11h 47m 11.928s[1]
Declination+89° 05′ 35.77″[1]
Redshift0.020334±0.0000970[2]
Heliocentric radial velocity6,096±29 km/s[2]
Distance291.4 ± 20.5 Mly (89.33 ± 6.28 Mpc)[2]
Apparent magnitude (V)14.9[1]
Characteristics
TypeS0[3]
Apparent size (V)0.92′ × 0.79′[1]
Notable featuresClosest NGC object to the north celestial pole
Other designations
MCG +15-01-011, PGC 36847, CGCG 370-002[2]

NGC 3172 (also known as Polarissima Borealis[1]) is a lenticular galaxy located in the constellation Ursa Minor. It is the closest NGC object to the north celestial pole.[1] Discovered by John Herschel in 1831, it is about 285 million light-years away and about 85 thousand light-years across.[4]

Supernovae

Two supernovae have been observed in NGC 3172:

  • SN 2010af (Type Ia, mag. 17.2), was discovered by Tom Boles on 4 March 2010.[5][6]
  • SN 2017gla (Type Ia, mag. 16), was discovered on by Giancarlo Cortini on 1 September 2017.[7]

See also

References

  1. ^ a b c d e f SIMBAD:%20NGC%203054%20--%20Galaxy "NGC 3172". sim-id. Retrieved 2020-05-29.
  2. ^ a b c d "Results for object NGC 5442". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 18 August 2025.
  3. ^ "Search specification: NGC 3172". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-24.
  4. ^ "New General Catalog Objects: NGC 3150 - 3199". cseligman.com. Retrieved 2020-05-30.
  5. ^ Boles, T. (2010). "Supernova 2010af in NGC 3172". Central Bureau Electronic Telegrams (2194): 1. Bibcode:2010CBET.2194....1B.
  6. ^ "SN 2010af". Transient Name Server. IAU. Retrieved 18 August 2025.
  7. ^ "SN 2017gla". Transient Name Server. IAU. Retrieved 18 August 2025.