Galaxy in the constellation Pegasus
NGC 7312 |
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![](//upload.wikimedia.org/wikipedia/commons/thumb/4/46/NGC7312_-_SDSS_DR14.jpg/250px-NGC7312_-_SDSS_DR14.jpg) The barred spiral galaxy NGC 7312. |
Observation data (J2000 epoch) |
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Constellation | Pegasus |
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Right ascension | 22h 34m 34.79s[1] |
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Declination | +05° 49′ 02.5″[1] |
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Redshift | 0.027609[1] |
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Heliocentric radial velocity | 8277 ± 1 km/s[1] |
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Distance | 380.6 ± 26.7 Mly (116.68 ± 8.18 Mpc)[1] |
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Apparent magnitude (V) | 13.4[1] |
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Characteristics |
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Type | SB(s)b[1] |
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Size | ~225,000 ly (68.97 kpc) (estimated)[1] |
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Apparent size (V) | 1.5' x 0.8'[1] |
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Other designations |
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2MASX J22343478+0549025, UGC 12083, MCG +01-57-010, PGC 69198, CGCG 404-023[1] |
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).[1] 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).[1] 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
- List of NGC objects (7001–7840)
References
- ^ a b c d e f g h i j k l "NASA/IPAC Extragalactic Database". Results for NGC 7312. Retrieved 2 August 2024.
- ^ Celestial Atlas entry for NGC 7312. Retrieved 2 August 2024.
- ^ The Astronomer's Telegram #8073. Retrieved 2 August 2024.
- ^ Transient Name Server entry for SN 2024ixe. Retrieved 2 August 2024.
External links
Media related to NGC 7312 at Wikimedia Commons - NGC 7312 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images