Quote:
Originally Posted by Burt
Astronomers observe the expansion to be uniform over very large scales, but 'clumpy' on smaller scales. The reason is that on the large scale there are roughly an equal number of galaxies in all directions and it is the large scale that determines the overall expansion rate.
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Thanks Burt--that makes sense. 
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If something is in me which can be called religious then it is the unbounded admiration for the structure of the world so far as our science can reveal it... of the manifestations of the profoundest reason and the most radiant beauty, which are only accessible to our reason in their most elementary forms...
Albert Einstein
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