Quote:
Originally Posted by Matt Starwave
Obviously burning hydrogen produces h2O but it is hard to believe any water gases would survive intact after leaving the sun to reach the super cold far flung areas.
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Hi Matt,
Here on Earth, one is familiar with the process of the combustion of hydrogen
and oxygen of which a by-product is water.
However, within the Sun, the process of energy release is primarily through that
of
nuclear fusion, where hydrogen atoms fuse together to form helium and in doing
so release energy. Fusion takes place because the mass of the star causes
it to fall in on itself under the force of gravity and this crushing force results
in the atoms fusing together.
The process of reactions by which it does this can be complex -
http://www.astrophysicsspectator.com...nHydrogen.html
Nevertheless, as a star goes through its life, it generally fuses lighter elements into
heavier elements, up the periodic table.
If a star is large enough when it was born (about 8 solar masses), it eventually
goes through a stage where it "burns" carbon and oxygen which resulted from
fusing helium, which in turn fuses to neon and magnesium and silicon and sulphur.
Once it gets to iron, the star collapses and a supernova occurs. In the
violence of this explosion, all the other elements in the periodic table are
formed and scattered into the surrounding space.
Some of the hydrogen and oxygen will combine to form water.
In the case of the supernova that led to to creation of our solar system,
at least here on Earth, some of the elements, such as gold, had
small abundances.
The iron in your blood was produced at the core of a star that once exploded.