[Home]History of Globular cluster

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Revision 6 . . (edit) November 24, 2001 1:52 pm by Alex Kennedy
Revision 5 . . November 24, 2001 12:34 pm by Chenyu
Revision 4 . . November 24, 2001 6:23 am by (logged).253.39.xxx [-> messier 31]
Revision 3 . . November 24, 2001 6:21 am by (logged).253.39.xxx [wikiing]
Revision 2 . . November 24, 2001 6:19 am by (logged).128.164.xxx [wikification, and also "powerful" -> "massive"]
Revision 1 . . November 24, 2001 6:12 am by (logged).92.168.xxx
  

Difference (from prior major revision) (minor diff, author diff)

Added: 2a3,10
It was through the study of globular clusters that the sun's position in
the Milky Way galaxy is know. Until the 1930s, it was thought that the
sun was near the middle of the galaxy because the distribution of stars
in the observable Milky War appeared uniform. However, the distribution
of globular clusters was strongly asymmetric. In looking at the distances to the clusters, it became clear that the observable Milky Way was only a small
part of the total galaxy, most of which was obscured by gas and dust. Because globular clusters lie outside the plane of the Milky Way, they are not
blocked by the gas and dust of the galactic disk.


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