NGC 7312 explained

NGC 7312
Constellation Name:Pegasus
Epoch:J2000
Type:SB(s)b[1]
Dist Ly:NaNMpc
Z:0.027609
H Radial V:8277 ± 1 km/s
Appmag V:13.4
Size V:1.5' x 0.8'
Size:~68.97kpc (estimated)

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.[2]

According to the NASA/IPAC database, NGC 7312 forms a galaxy pair with NGC 7311 (also known as UGC 12080). The Hubble distance to NGC 7311 is 61.33 ± 4.31 Mpc (∼200 million al), which means that it is much closer than NGC 7312, and therefore the pairing is purely optical.

Two supernovae have been observed in NGC 7312: PSNJ22343424+0548478 (type II, mag 16.6, discovered 17 September 2015)[3] and SN 2024ixe (type IIb, mag. 19.7).[4]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 7312 . 2 August 2024.
  2. https://cseligman.com/text/atlas/ngc73.htm#7312 Celestial Atlas entry for NGC 7312.
  3. https://www.astronomerstelegram.org/?read=8073 The Astronomer's Telegram #8073.
  4. https://www.wis-tns.org/object/2024ixe Transient Name Server entry for SN 2024ixe.