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| From: Zardoz ® |
04/11/2001
19:37:47
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| Subject: re: COSMOLOGY FAQ |
post id:
484073
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 Credits: NASA, Donald
Walter (South Carolina State University), Paul Scowen and Brian Moore
(Arizona State University) How does a
star form? From: Greg L. ®
A star is born by the collapse of a cloud of
molecular hydrogen gas under gravity. Initially the cloud is very thin and
dispersed throughout space, but under the influence of external
perturbations and shock waves from violent nearby events such as supernova
explosions, the cloud begins to collapse on itself. As it does so it
begins to heat up and radiate away energy. Eventually the cloud becomes
hot enough to glow, becoming a 'protostar.' Depending on the initial
conditions present during the collapse, the cloud may further fragment
into two or more stars, forming a open star cluster. Many of these stars
will have disks of dust and gas around them, and these will go on to form
planets. Eventually the cloud collapses to the point where the internal
temperatures and pressures are high enough to initiate hydrogen burning at
the core via a series of nuclear fusion reactions. Soon after this occurs
the cloud stops collapsing and a new star is born.
The lifetime of
the newborn star will depend on its mass. Small stars will slowly burn up
their stocks of hydrogen, whilst bigger stars will burn their stocks much
quicker, and may not live longer than a few million years.
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