Astronomy:NGC 662

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NGC 662
NGC 662 imaged by Pan-STARRS
Observation data (J2000 epoch)
ConstellationAndromeda
Right ascension 01h 44m 35.4353s[1]
Declination+37° 41′ 45.165″[1]
Redshift0.018860[1]
Helio radial velocity5654 ± 4 km/s[1]
Distance259.7 ± 18.2 Mly (79.61 ± 5.58 Mpc)[1]
Apparent magnitude (V)13.0[1]
Characteristics
TypeS pec[1]
Size~89,600 ly (27.48 kpc) (estimated)[1]
Apparent size (V)0.8′ × 0.5′[1]
Other designations
IRAS 01416+3726, UGC 1220, MCG+06-04-060, PGC 6393[1]

NGC 662 is a spiral galaxy in the constellation of Andromeda. Its velocity with respect to the cosmic microwave background is 5,397 ± 18 km/s, which corresponds to a Hubble distance of 79.6 ± 5.6 Mpc (~260 million light-years).[1] It was discovered by French astronomer Édouard Stephan on 22 November 1884.[2]

According to the Simbad database, NGC 662 is a radio galaxy.[3] It features a broad HI line[4] and is classified a field galaxy, meaning it does not belong to the galaxy group nor a cluster and is therefore gravitationally isolated.[5]

Supernovae

Three supernovae have been observed in NGC 662:

  • SN 2001dn (Type Ia, mag. 15.5) was discovered by Tom Boles on 14 August 2001.[6][7]
  • SN 2022ojo (Type II-P, mag. 16.938) was discovered by ATLAS on 5 July 2022.[8]
  • SN 2024pcw (Type II, mag. 18.724) was discovered by ATLAS on 8 July 2024.[9]

See also

References