Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.astronet.ru/db/xware/msg/1333097
Дата изменения: Sun Mar 1 18:27:20 2015
Дата индексирования: Sun Apr 10 13:07:17 2016
Кодировка:
Inside the Coma Cluster of Galaxies
Astronomy Picture of the Day
    


Inside the Coma Cluster of Galaxies
<< Yesterday 28.02.2015 Tomorrow >>
Inside the Coma Cluster of Galaxies
Credit & Copyright: D. Carter (LJMU) et al. and the Coma HST ACS Treasury Team
Explanation: Almost every object in the above photograph is a galaxy. The Coma Cluster of Galaxies pictured above is one of the densest clusters known - it contains thousands of galaxies. Each of these galaxies houses billions of stars - just as our own Milky Way Galaxy does. Although nearby when compared to most other clusters, light from the Coma Cluster still takes hundreds of millions of years to reach us. In fact, the Coma Cluster is so big it takes light millions of years just to go from one side to the other! The above mosaic of images of a small portion of Coma was taken in unprecedented detail in 2006 by the Hubble Space Telescope to investigate how galaxies in rich clusters form and evolve. Most galaxies in Coma and other clusters are ellipticals, although some imaged here are clearly spirals. The spiral galaxy on the upper left of the above image can also be found as one of the bluer galaxies on the upper left of this wider field image. In the background thousands of unrelated galaxies are visible far across the universe.

January
February
March
April
May
June
July
August
September
October
November
December
 < February 2015  >
Mo Tu We Th Fr Sa Su






1
2345678
9101112131415
16171819202122
232425262728
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.

Based on Astronomy Picture Of the Day

Publications with keywords: Coma Cluster
Publications with words: Coma Cluster
See also: