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Reference Terms
from Wikipedia, the free encyclopedia

Physical cosmology

Physical cosmology, as a branch of astrophysics, is the study of the large-scale structure of the universe and is concerned with fundamental questions about its formation and evolution.

Cosmology involves itself with studying the motions of the celestial bodies and the first cause.

Physical cosmology, as it is now understood, began with the twentieth century development of Albert Einstein's theory of general relativity and detailed astronomical observations of extremely distant objects.

Note:   The above text is excerpted from the Wikipedia article "Physical cosmology", which has been released under the GNU Free Documentation License.
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Space & Time News
October 14, 2016

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updated 12:56 pm ET