Explanation: Elliptical galaxy M87 is a type of galaxy that looks much different than our own Milky Way Galaxy. Even for an elliptical galaxy, though, M87 is peculiar. M87 is much bigger than an average galaxy, appears near the center of a whole cluster of galaxies known as the Virgo Cluster, and shows an unusually high number of globular clusters. These globular clusters are visible as faint spots surrounding the bright center of M87. In general, elliptical galaxies contain similar numbers of stars as spiral galaxies, but are ellipsoidal in shape (spirals are mostly flat), have no spiral structure, and little gas and dust. The above image of M87 was taken recently by the Canada-France-Hawaii Telescope on top of the dormant volcano Mauna Kea in Hawaii, USA.

News: APOD turns nine years old today!

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: Elliptical Galaxy - M 87 - ellipticheskaya galaktika Publikacii so slovami: Elliptical Galaxy - M 87 - ellipticheskaya galaktika
Sm. takzhe: Galaktika, dzhet i znamenitaya chernaya dyra Central'naya chernaya dyra v M87 v polyarizovannom svete Galaktika, dzhet i chernaya dyra Obolochki iz zvezd v ellipticheskoi galaktike PGC 42871 Dalekie galaktiki M89: ellipticheskaya galaktika s vneshnimi obolochkami i struyami NGC 1316: posle stolknoveniya galaktik Vse publikacii na tu zhe temu >>