NGC 1400
Today, NGC 1400 is a topic that remains relevant and of interest to a wide audience. Whether due to its impact on society, its historical relevance, or its influence on popular culture, NGC 1400 continues to be a topic of constant debate and study. From its origins to the present, NGC 1400 has marked a milestone in different aspects of human life, and its importance remains undeniable. In this article, we will explore the multiple facets of NGC 1400 and its impact in various areas, with the intention of offering a complete and enriching look at this significant topic.
| 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 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 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
-
DSS image of NGC 1400 -
Pan-STARRS image of NGC 1400
References
- ^ 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
Media related to NGC 1400 at Wikimedia Commons
