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Messier 89 (M89 for short, also known as NGC 4552) is an elliptical galaxy in the constellation Virgo. It was discovered by Charles Messier on March 18, 1781. M89 is a member of the Virgo Cluster of galaxies. More information...

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  • An elliptical galaxy is a galaxy having an approximately ellipsoidal shape and a smooth, nearly featureless brightness profile. They range in shape from nearly spherical to highly flattened and in size from hundreds of millions to over one trillion stars. Elliptical galaxies are one of the three main classes of galaxy originally described by Edwin Hubble in his 1936 work “The Realm of the Nebulae”, along with spiral and lenticular galaxies.
    http://commons.wikipedia.org/wiki/File:Abell_S740%2C_cropped_to_ESO_325-G004.jpg
  • Messier 87 (also known as M87, Virgo A or NGC 4486) is a giant elliptical galaxy. The galaxy is the largest and brightest galaxy within the northern Virgo Cluster, located about 55 million light years away. The galaxy also contains a notable active galactic nucleus that is a strong source of multiwavelength radiation, particularly radio waves.
    http://commons.wikipedia.org/wiki/File:Celestia.png
  • Dwarf elliptical galaxies, or dEs, are elliptical galaxies that are much smaller than others. They are classified as dE, and are quite common in galaxy groups and clusters, and are usually companions to other galaxies.
    http://commons.wikipedia.org/wiki/File:M110_Lanoue.png
  • Messier 49 (also known as M 49 or NGC 4472) is an elliptical / lenticular galaxy about 49 million light-years away in the constellation Virgo. The galaxy was discovered by Charles Messier in 1771.
    http://commons.wikipedia.org/wiki/File:Celestia.png
  • Messier 59 (also known as M59 or NGC 4621) is an elliptical galaxy in the constellation Virgo.
    http://en.wikipedia.org/wiki/File:Messier_59_DSS2_WikiSky.jpg
  • Messier 60 (also known as NGC 4649) is an elliptical galaxy approximately 55 million light-years away in the constellation Virgo.
    http://commons.wikipedia.org/wiki/File:Messier_60_Hubble_WikiSky.jpg
  • Messier 105 (also known as M105 and NGC 3379) is an elliptical galaxy in the constellation Leo. Messier 105 is known to have a supermassive black hole.
    http://commons.wikipedia.org/wiki/File:Celestia.png
  • Dwarf spheroidal galaxy (dSph) is a term in astronomy applied to low luminosity galaxies that are companions to the Milky Way and to the similar systems that are companions to the Andromeda Galaxy M31. While similar to dwarf elliptical galaxies in appearance and properties such as little to no gas or dust or recent star formation, they are approximately spheroidal in shape, generally lower luminosity, and are only recognized as satellite galaxies in the Local Group.
    http://commons.wikipedia.org/wiki/File:NGC147.jpg
  • NGC 4881 is an elliptical galaxy about 352 million light-years away in the constellation Coma Berenices. It is a member of the Coma cluster of galaxies. NGC 4881 was discovered by Heinrich Louis d'Arrest in 1865. In 1994, the Hubble Space Telescope took a look at the Coma cluster and NGC 4881.
    http://commons.wikipedia.org/wiki/File:Milky_Way_2005.jpg
  • NGC 4555 is a solitary elliptical galaxy about 40,000 parsecs across. Observations by the Chandra X-ray Observatory have shown it to be surrounded by a halo of hot gas about 120,000 parsecs across. The hot gas has a temperature of around 10,000,000 kelvins. The galaxy is one of the few elliptical galaxies proven to have significant amounts of dark matter.

 

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