NGC 4452, 2MFGC 9831, VCC 1125, [CHM2007] LDC 904 J122843.62+1145261, ACSVCS 44, 2MFGC 9833, VPC 613, [CHM2007] HDC 720 J122843.62+1145261, LEDA 41060, UGC 7601, Z 1226.2+1202, MCG+02-32-080, UZC J122843.3+114519, Z 70–112
Preview warning: Page using Template:Infobox galaxy with unknown parameter "image_size"
Preview warning: Page using Template:Infobox galaxy with unknown parameter "credit"
NGC 4452 is an edge-on lenticular galaxy that is part of the Virgo Cluster. NGC 4452 is about 60 million light-years (18 Mpc) away from Earth and 35 kly (11 kpc) in diameter.[3] This galaxy was first seen by William Herschel in 1784 with his 47 cm (19 in) telescope.
NGC 4452 is so thin that it is actually difficult to determine what type of disk galaxy it is. Its lack of a visible dust lane indicates that it is a low-dust lenticular galaxy, although it is still possible that a view from on top would reveal spiral structure. The unusual stellar line segment spans about 35,000 light-years from end to end.
Near NGC 4452's center is a slight bulge of stars, while hundreds of background galaxies are visible far in the distance. Galaxies that appear this thin are rare mostly because Earth must reside (nearly) in the extrapolated planes of their thin galactic disks. Galaxies that actually are this thin are relatively common; for example, the Milky Way Galaxy is thought to be about this thin.[4]
NGC 4452 appears to be very similar to galaxy IC 335, an edge-on galaxy in Fornax Cluster, in constellation Fornax.
^"The Interactive NGC Catalog Online". Results for NGC 4452. Retrieved 2010-11-08.
^"SIMBAD Astronomical Database". Results for NGC 4452. Retrieved 2010-11-08.
^Holm, Carl (15 November 2010). "Hubble captures rare galactic view". Australia: ABC. Archived from the original on 17 November 2010. Retrieved 2010-11-15.
^"APOD: 2010 November 9 - NGC 4452: An Extremely Thin Galaxy". NASA. 9 November 2012. Retrieved 28 July 2019. This article incorporates text from this source, which is in the public domain.
NGC4452 is an edge-on lenticular galaxy that is part of the Virgo Cluster. NGC4452 is about 60 million light-years (18 Mpc) away from Earth and 35 kly...
Fornax. It is part of the Fornax Cluster. IC 335 appears very similar to NGC4452, a lenticular galaxy in Virgo. Both galaxies are edge-on, meaning that...
NGC 3599 is a lenticular galaxy located in the constellation Leo. It was discovered by William Herschel on March 14, 1784. The galaxy is located at a...
Ethylene glycol dinitrate, abbreviated EGDN and NGC, also known as Nitroglycol, is a colorless, oily, explosive liquid obtained by nitrating ethylene...
NGC 4036 is the New General Catalogue identifier for a lenticular galaxy in the northern circumpolar constellation of Ursa Major. In the Carnegie Atlas...
NGC 4041 is the New General Catalogue identifier for a spiral galaxy in the northern circumpolar constellation of Ursa Major. It is located an estimated...
(the quasar lies at z=2.69) In 1999, cluster RDCS J0849+4452 (RX J0849+4452, RXJ0848.9+4452) was found at z=1.261 In 1995 and 2001, the cluster around...
Global Information
This article incorporates text from this source, which is in the public domain.
