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The Sombrero Galaxy is 11.5° west of Spica [10] and 5.5° north-east of Eta Corvi. [38] Although it is visible with 7×35 binoculars or a 4-inch (100 mm) amateur telescope, [ 38 ] an 8-inch (200 mm) telescope is needed to distinguish the bulge from the disk, [ 10 ] and a 10- or 12-inch (250 or 300 mm) telescope to see the dark dust lane.
NGC 5746 (also known as the Mini Sombrero Galaxy [3] [4]) is a barred spiral galaxy located in the eastern part of the constellation of Virgo. It was discovered on 24 February 1786 by German-British astronomer William Herschel . [ 5 ]
It is the most luminous member of that cluster and more luminous than any galaxy closer to the Earth. This galaxy forms part of the smaller Virgo B subcluster 4.5° away from the dynamic center of the Virgo Cluster, centered on Messier 87. [6] [9] Messier 49 is gravitationally interacting with the dwarf irregular galaxy UGC 7636. [5]
The Sombrero galaxy, named for its resemblance to the Mexican hat, is about 30 million light-years from Earth, NASA said in a news release. The galaxy is surrounded by multiple rings, where stars ...
The Sombrero galaxy looks entirely different in a new image by the James Webb Space Telescope. Instead of a Mexican hat, it appears more like an archery target.
The galaxy is seen edge-on from Earth. It is sometimes referred to as "the little sombrero", a miniature version of Messier 104 . The star field behind NGC 7814 is known for its density of faint, remote galaxies as can be seen in the image here, in the same vein as the Hubble Deep Field .
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