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NGC 7312

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Galaxy in the constellation Pegasus

NGC 7312
The barred spiral galaxy NGC 7312
Observation data (J2000 epoch)
ConstellationPegasus
Right ascension22 34 34.7889
Declination+05° 49′ 02.579″
Redshift0.027609
Heliocentric radial velocity8277 ± 1 km/s
Distance380.6 ± 26.7 Mly (116.68 ± 8.18 Mpc)
Apparent magnitude (V)13.4
Characteristics
TypeSB(s)b
Size~225,000 ly (68.97 kpc) (estimated)
Apparent size (V)1.5′ × 0.8′
Other designations
2MASX J22343478+0549025, UGC 12083, MCG +01-57-010, PGC 69198, CGCG 404-023

NGC 7312 is a barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 7911 ± 26 km/s, which corresponds to a Hubble distance of 116.68 ± 8.18 Mpc (∼381 million light-years). It was discovered by German astronomer Albert Marth on 30 October 1863.

According to Steven D. Peterson, NGC 7312 forms a galaxy pair with NGC 7311. The Hubble distance to NGC 7311 is 61.33 ± 4.31 Mpc (∼200 million light-years), which is much closer than NGC 7312, and therefore the pairing is purely optical.

Supernovae

Two supernovae have been observed in NGC 7312:

See also

References

  1. ^ "Results for object NGC 7312". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 2 August 2024.
  2. Seligman, Courtney. "New General Catalogue Objects: NGC 7312". Celestial Atlas. Retrieved 14 December 2024.
  3. Peterson, S. D. (1979). "Double galaxies. I. Observational data on a well-defined sample". The Astrophysical Journal Supplement Series. 40: 527. Bibcode:1979ApJS...40..527P. doi:10.1086/190597.
  4. Bishop, David. "Bright Supernovae - 2015 (Entry for PSNJ22343424+0548478)". Rochester Astronomy. Retrieved 15 December 2024.
  5. "SN 2024ixe". Transient Name Server. IAU. Retrieved 15 December 2024.

External links

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Category
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