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NGC 1332

NGC 1332 is an almost edge-on elliptical galaxy located in constellation of Eridanus. Situated about 70 million light years away, it is a member of the Eridanus cluster of galaxies, a cluster of about 200 galaxies. It is also the brightest member of the NGC 1332 Group. It was discovered by William Herschel on 9 December 1784.

NGC 1332
Hubble Space Telescope image of NGC 1332
Observation data (J2000 epoch)
ConstellationEridanus
Right ascension03h 26.170m [1]
Declination−21° 20′[1]
Helio radial velocity1553 ± 19 km/s
Distance21.5 Mpc (70.1 Mly)
Apparent magnitude (V)10.3[1]
Characteristics
TypeE[1]
Apparent size (V)4.5′ × 1.4′[1]
Other designations
MCG -04-09-011, PGC 12838[2]

NGC 1332 has a Hubble classification of E, which indicates it is an elliptical galaxy. It is moving away from the Milky Way at a rate of 1,553 km/s. Its size on the night sky is 4.5' x 1.4' which is proportional to its real size of 92 000 ly.[citation needed]

NGC 1332 is an early-type 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.[3]

Black hole

NGC 1332 is known by its possessing a supermassive black hole at the center. In 2016, a team from United States and China used the Atacama Large Millimeter/submillimeter Array (ALMA) to collect high resolution data. They were able to measure the mass of the black hole. They determined the mass of about 660 million solar-masses with an uncertainty of just 10%. NGC 1332's black hole is the most massive black hole in the Eridanus Cluster, and it is even more massive than NGC 1399's black hole (NGC 1399 is the Fornax cluster's central galaxy).[4]

Gallery

References

  1. ^ a b c d e Dunlop, Storm (2005). Atlas of the Night Sky. Collins. ISBN 978-0-00-717223-8.
  2. ^ "NGC 1332". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-19.
  3. ^ Howell, Elizabeth (2015). "Colossal Ancient Galaxies Die from the Inside Out". space.com. Retrieved 5 March 2017.
  4. ^ http://www.sci-news.com/astronomy/mass-ngc-1332-supermassive-black-hole-03843.html

External links

  •   Media related to NGC 1332 at Wikimedia Commons


1332, this, article, uses, bare, urls, which, uninformative, vulnerable, link, please, consider, converting, them, full, citations, ensure, article, remains, verifiable, maintains, consistent, citation, style, several, templates, tools, available, assist, form. This article uses bare URLs which are uninformative and vulnerable to link rot Please consider converting them to full citations to ensure the article remains verifiable and maintains a consistent citation style Several templates and tools are available to assist in formatting such as Reflinks documentation reFill documentation and Citation bot documentation August 2022 Learn how and when to remove this template message NGC 1332 is an almost edge on elliptical galaxy located in constellation of Eridanus Situated about 70 million light years away it is a member of the Eridanus cluster of galaxies a cluster of about 200 galaxies It is also the brightest member of the NGC 1332 Group It was discovered by William Herschel on 9 December 1784 NGC 1332Hubble Space Telescope image of NGC 1332Observation data J2000 epoch ConstellationEridanusRight ascension03h 26 170m 1 Declination 21 20 1 Helio radial velocity1553 19 km sDistance21 5 Mpc 70 1 Mly Apparent magnitude V 10 3 1 CharacteristicsTypeE 1 Apparent size V 4 5 1 4 1 Other designationsMCG 04 09 011 PGC 12838 2 NGC 1332 has a Hubble classification of E which indicates it is an elliptical galaxy It is moving away from the Milky Way at a rate of 1 553 km s Its size on the night sky is 4 5 x 1 4 which is proportional to its real size of 92 000 ly citation needed NGC 1332 is an early type 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 3 Contents 1 Black hole 2 Gallery 3 References 4 External linksBlack hole EditNGC 1332 is known by its possessing a supermassive black hole at the center In 2016 a team from United States and China used the Atacama Large Millimeter submillimeter Array ALMA to collect high resolution data They were able to measure the mass of the black hole They determined the mass of about 660 million solar masses with an uncertainty of just 10 NGC 1332 s black hole is the most massive black hole in the Eridanus Cluster and it is even more massive than NGC 1399 s black hole NGC 1399 is the Fornax cluster s central galaxy 4 Gallery Edit Pan STARRS image of NGC 1332 DSS image of NGC 1332References Edit a b c d e Dunlop Storm 2005 Atlas of the Night Sky Collins ISBN 978 0 00 717223 8 NGC 1332 SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2021 02 19 Howell Elizabeth 2015 Colossal Ancient Galaxies Die from the Inside Out space com Retrieved 5 March 2017 http www sci news com astronomy mass ngc 1332 supermassive black hole 03843 htmlExternal links Edit Media related to NGC 1332 at Wikimedia Commons This elliptical galaxy article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title NGC 1332 amp oldid 1110086642, wikipedia, wiki, book, books, library,

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