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Galaxy in the constellation Pegasus From Wikipedia, the free encyclopedia
NGC 7331, also known as Caldwell 30, is an unbarred spiral galaxy about 40 million light-years (12 Mpc) away in the constellation Pegasus. It was discovered by William Herschel in 1784.[4] NGC 7331 is the brightest galaxy in the field of a visual grouping known as the NGC 7331 Group of galaxies. In fact, the other members of the group, NGC 7335, 7336, 7337 and 7340, lie far in the background at distances of approximately 300–350 million light years.[5]
| NGC 7331 | |
|---|---|
NGC 7331 imaged by the Phillips 24-inch RCOS Telescope at the Mount Lemmon SkyCenter[1] | |
| Observation data (J2000 epoch) | |
| Constellation | Pegasus |
| Right ascension | 22h 37m 04.1s[2] |
| Declination | +34° 24′ 56″[2] |
| Redshift | 816 ± 1 km/s[2] |
| Distance | 39.8 ± 3.3 Mly (12.2 ± 1.0 Mpc) [3] |
| Apparent magnitude (V) | 10.4[2] |
| Characteristics | |
| Type | SA(s)b[2] |
| Size | 120,000 ly (diameter) |
| Apparent size (V) | 10.5′ × 3.7′[2] |
| Other designations | |
| UGC 12113, PGC 69327,[2] Caldwell 30 | |
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The galaxy appears similar in size and structure to the Milky Way, and is sometimes referred to as "the Milky Way's twin".[6] However, discoveries in the 2000s regarding the structure of the Milky Way may call this similarity into doubt, particularly because the latter is now believed to be a barred spiral, compared to the unbarred status of NGC 7331.[7] In spiral galaxies the central bulge typically co-rotates with the disk but the bulge in the galaxy NGC 7331 is rotating in the opposite direction to the rest of the disk.[8] In both visible light and infrared photos of the NGC 7331, the core of the galaxy appears to be slightly off-center, with one side of the disk appearing to extend further away from the core than the opposite side.
Multiple supernova events have been observed in this galaxy. SN 1959D, a Type IIL supernova,[9] was the first supernova identified within NGC 7331.[2] The supernova was discovered by Milton Humason and H. S. Gates in a survey at Palomar Observatory.[10] More recent supernovae are SN 2013bu (type II, mag. 16.6)[11] and SN 2014C, the latter of which underwent an unusual "metamorphosis" from a hydrogen-poor Type Ib to a hydrogen-rich Type IIn over the course of a year . [12] A 1903 photographic plate from Yerkes Observatory shows a magnitude 16.6 candidate transient that may have also been a supernova.[13]
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