Answer 1:
The sun is actually a star, like those
that you
can see at night in the sky. It looks different
though because we are much closer to the sun than
we are to the ones in the night sky. Stars, like
our sun, are basically big balls of gas. The
gases are squished together, and as they are
squished they start to get hot. When the gases
get hot enough, their atoms start to combine to
make new atoms in nuclear reactions. These
reactions in stars are called fusion (2 atoms make
1 new atom. This combination of atoms to make
new ones releases heat. The sun is hot
because of
the nuclear activity within it.
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Answer 2:
This is a really good question. The basic theory of
where our sun came from is that a long time ago
(around five billion years) a large cloud of cold
gas started to collapse due to gravity. As that
gas cloud collapsed it started to heat up as the
released gravitational energy was turned into
thermal energy (heat). Since the gas cloud was
warmer than surrounding space, some of that heat
was radiated away at the surface of the gas cloud
and, because of this, the cloud continued to
contract and become hotter. Eventually, the
cloud collapsed down to around the current size of
the sun. At the point, the center of the cloud
became so hot the nuclear fusion started to
provide the energy to keep up with what was being
radiated away at the surface and the sun stopped
contracting.
So, in a nutshell, the sun
is hot because of the physics of a giant gas cloud
that has collapsed due to gravity and is
surrounded by empty space. The temperature at the
surface of the sun mostly depends on how much mass
it has. Do you think stars that have more
material are hotter or cooler? Do you think
stars with a different mass would have the same
color or a different color?
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