Astronomy:NGC 7714

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NGC 7714
File:Heic1503a.tif
NGC 7714 imaged by the Hubble Space Telescope[1]
Observation data (J2000 epoch)
ConstellationPisces
Right ascension 23h 36m 14.1232s[2]
Declination+02° 09′ 18.133″[2]
Redshift0.009333[2]
Helio radial velocity2798 ± 1 km/s[2]
Distance116.9 ± 8.3 Mly (35.85 ± 2.54 Mpc)[2]
Apparent magnitude (V)12.2
Characteristics
TypeSB:(s)b? pec,[3] HII[4]
Size~67,100 ly (20.57 kpc) (estimated)[2]
Apparent size (V)1.90 × 1.4 moa[4]
Other designations
KCPG 587A, UM 167, HOLM 810A, IRAS 23336+0152, Arp 284, UGC 12699, MCG+00-60-017, PGC 71868[2]

NGC 7714 is a spiral galaxy in the constellation Pisces. Its velocity with respect to the cosmic microwave background is 2430 ± 26 km/s, which corresponds to a Hubble distance of 116.9 ± 8.3 Mly (35.85 ± 2.54 Mpc).[2] In addition, five non-redshift measurements give a distance of 92.24 ± 8.69 Mly (28.280 ± 2.664 Mpc).[5] It was discovered by British astronomer John Herschel on 18 September 1830.[6]

NGC 7714 and NGC 7715 are interacting galaxies.[4] The pair are included in Halton Arp's Atlas of Peculiar Galaxies, listed as Arp 284.[7] NGC 7714 appears to be a highly distorted spiral, possibly a barred spiral galaxy. NGC 7715 is of uncertain type, probably an edge-on spiral or an irregular galaxy.[3]

Supernovae

Three supernovae have been observed in NGC 7714:

  • SN 1999dn (Type Ib/c, mag. 16.3) was discovered by the BAO Supernova Survey on 19 August 1999.[8][3][9]
  • SN 2007fo (Type Ib/c, mag. 18.2) was discovered by the Lick Observatory Supernova Search on 9 July 2007.[10][11]
  • SN 2023pso (Type Ib, mag. 17.15) was discovered by GOTO on 7 August 2023.[12]
NGC 7714 (right) and NGC 7715 (left) imaged by legacy surveys

See also

References

Coordinates: Sky map 23h 36m 14.1232s, +02° 09′ 18.133″