Summary
NGC 1400 is an elliptical galaxy in the constellation Eridanus. At a distance of 65 million light-years from Earth, it was discovered by John Herschel in 1786. It is a member of the NGC 1407 group, whose brightest member is NGC 1407. The NGC 1407 group is part of the Eridanus Cluster, a cluster of 200 galaxies.
| NGC 1400 | |
|---|---|
 Hubble Space Telescope image of NGC 1400 | |
| Observation data (J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 39m 30.851s[1] |
| Declination | −18° 41′ 17.25″[1] |
| Redshift | 0.001769[2] |
| Heliocentric radial velocity | 530 km/s[2] |
| Distance | 82 Mly (25 Mpc)[3] |
| Apparent magnitude (V) | 10.96[3] |
| Apparent magnitude (B) | 11.92[3] |
| Characteristics | |
| Type | SA0−[3] |
| Apparent size (V) | 2.3′ × 2.0′[3] |
| Other designations | |
| MCG -03-10-022, PGC 13470[2] | |
NGC 1400 is an early-type E0 galaxy. Despite their name, early-type galaxies are much older than spiral galaxies, and mostly comprise old, red-colored stars. Very little star formation occurs in these galaxies; the lack of star formation in elliptical galaxies appears to start at the center and then slowly propagates outward.[4]
NGC 1400 has had star formation in the past, which was caused by NGC 1400 falling into the NGC 1407 group.[5]
One supernova has been observed in NGC 1400: SN 2021hcz (type Ia, mag. 15.4).[6]
Gallery edit
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DSS image of NGC 1400 -
Pan-STARRS image of NGC 1400
References edit
- ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
- ^ a b c "NGC 1400". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-21.
- ^ a b c d e Gil de Paz, Armando; et al. (December 2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies". The Astrophysical Journal Supplement Series. 173 (2): 185–255. arXiv:astro-ph/0606440. Bibcode:2007ApJS..173..185G. doi:10.1086/516636. S2CID 119085482.
- ^ Howell, Elizabeth (2015). "Colossal Ancient Galaxies Die from the Inside Out". space.com. Retrieved 5 March 2017.
- ^ Spolaor, Max; Forbes, Duncan A.; Proctor, Robert N.; Hau, George K. T.; Brough, Sarah (2008). "The early-type galaxies NGC 1407 and NGC 1400 – II. Star formation and chemical evolutionary history". Monthly Notices of the Royal Astronomical Society. 385 (2): 675–686. arXiv:0801.2005. Bibcode:2008MNRAS.385..675S. doi:10.1111/j.1365-2966.2008.12892.x. S2CID 15326784.
- ^ Transient Name Server entry for SN 2021hcz. Retrieved 23 March 2023.
External links edit
Media related to NGC 1400 at Wikimedia Commons
