Astronomy:NGC 1482
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| NGC 1482 | |
|---|---|
 NGC 1482 imaged by Pan-STARRS | |
| Observation data (J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 54m 38.9804s[1] |
| Declination | −20° 30′ 08.011″[1] |
| Redshift | 0.006391[1] |
| Helio radial velocity | 1312 ± 9 km/s[1] |
| Distance | 87.4 ± 6.7 Mly (26.81 ± 2.05 Mpc)[1] |
| Apparent magnitude (V) | 12.2[1] |
| Characteristics | |
| Type | SA0^+ pec edge-on[1] |
| Size | ~89,400 ly (27.40 kpc) (estimated)[1] |
| Apparent size (V) | 2.4′ × 1.4′[1] |
| Other designations | |
| IRAS 03524-2038, MCG-03-10-054, PGC 14084[1] | |
NGC 1482 is a lenticular galaxy in the constellation of Eridanus. Its velocity with respect to the cosmic microwave background is 1817 ± 40 km/s, which corresponds to a Hubble distance of 87.4 ± 6.7 Mly (26.81 ± 2.05 Mpc).[1] In addition, one non-redshift measurement gives a distance of 64 Mly (19.6 Mpc).[2] It was discovered by German-British astronomer William Herschel on 19 December 1799.[3]
Supernova
One supernova has been observed in NGC 1482. SN 1937E (type unknown, mag. 16.5) was discovered by Fritz Zwicky on 26 November 1937.[4][5]
See also
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 "Results for object NGC 1482". NASA and Caltech. http://ned.ipac.caltech.edu/byname?objname=NGC+1482.
- ↑ "Distance Results for NGC 1482". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+1482.
- ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 1482". https://cseligman.com/text/atlas/ngc14a.htm#1482.
- ↑ "SN 1937E". IAU. https://www.wis-tns.org/object/1937E.
- ↑ Zwicky, F. (1939). "Four More Supernovae". Publications of the Astronomical Society of the Pacific 51 (299): 36. doi:10.1086/124993. Bibcode: 1939PASP...51...36Z.
External links
- NGC 1482 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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