The Big Bang Model is a broadly
accepted theory for the origin and evolution of our universe.
It postulates that 12 to 14 billion years ago, the portion of
the universe we can see today was only a few millimeters across.
It has since expanded from this hot dense state into the vast
and much cooler cosmos we currently inhabit. We can see remnants
of this hot dense matter as the now very cold cosmic microwave
background radiation which still pervades the universe and is
visible to microwave detectors as a uniform glow across the entire
sky.
The first key idea dates to
1916 when Einstein developed his General Theory of Relativity
which he proposed as a new theory of gravity. His theory generalizes
Isaac Newton's original theory of gravity, c. 1680, in that it
is supposed to be valid for bodies in motion as well as bodies
at rest. Newton's gravity is only valid for bodies at rest or
moving very slowly compared to the speed of light. A key concept
of General Relativity is that gravity is no longer described
by a gravitational "field" but rather it is supposed
to be a distortion of space and time itself. Physicist John Wheeler
put it well when he said, "Matter tells space how to curve,
and space tells matter how to move." Originally, the theory
was able to account for peculiarities in the orbit of Mercury
and the bending of light by the Sun, both unexplained in Isaac
Newton's theory of gravity. In recent years, the theory has passed
a series of rigorous tests.
Excerpt courtesy
of WMAP Cosmology 101: Big Bang Theory © map.gsfc.nasa.gov.
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