Answer 1:
Excellent question! The planets in our solar
system are each made out of different things. The
inner planets (Mercury, Venus, Earth, and Mars)
are relatively small rocky planets made up mostly
of silicate minerals and iron and nickel metal.
Most of the earth is made up of only three
elements: iron, silicon, and oxygen. Most of the
iron is in the core of the earth. Most of the
oxygen is locked up in minerals with silicon. In
fact, the mineral quartz is made up of only
silicon and oxygen. The inner planets are
relatively small and mostly solid, though earth
has a thin atmosphere made up mostly of nitrogen
and oxygen gases.
The outer planets (Jupiter, Saturn, Uranus, and
Neptune) have much different compositions. They
all have solid cores of rock, metal, and maybe
even ice, but these planets are totally enveloped
in thick atmospheres of gas. Hydrogen and Helium
(the two lightest elements) make up most of the
gases in the atmospheres of these planets. It is
thought that light gases, such as hydrogen and
helium, were “pushed” to the outer solar system by
radiation and matter streaming from the sun
(Grotzinger et al., 2007). Smaller, solid moons
made out of rock and ice orbit the large gaseous
outer planets.
references
Grotzinger, J., Jordan, T.H., Press, F., Siever,
R. (2007). Understanding Earth. New York: Freeman
and Company.
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Answer 2:
That depends on the planet. There are four
kinds of objects just in our own solar system that
are (or have been called) planets. These are:
1. Overgrown asteroids (Mercury, Venus, Earth,
Mars), which are made out of rock but have metal
(probably iron) cores, and may have relatively
thin atmospheres;
2. Giant comets (Pluto, Eris), which are various
kinds of ice, e.g. water, methane, ammonia, carbon
dioxide, and other things that freeze because it's
so cold in the outer solar system (note: right now
these aren't called planets, but I'm including
them because they have been called planets in the
past and may be again in the future);
3. Failed stars (Jupiter, Saturn), which are
mainly hydrogen and helium compressed into liquid
metallic form by the immense pressure inside of
these planets, possibly with rocky cores as well;
4. In-between objects (Uranus, Neptune), which
have thick clouds of water, methane, ammonia, etc.
ices that turn into hot liquid (again due to
pressure), but with large rocky cores in the interior.
In addition, other solar systems are thought to
have:
5. "Ocean" planets, which are mainly composed of
water but with rocky cores where the point where
the air (itself water vapor) meets the sea is
difficult to define due to pressure (incidentally,
Ganymede and Europa might qualify as this kind of
planet if there weren't moons orbiting Jupiter);
6. Only partially-failed stars (called brown
dwarfs), which are big enough to burn deuterium (a
kind of hydrogen), but not regular hydrogen,
preventing them from being true stars;
7. "Pulsar planets", created from debris falling
back on themselves after a supernova;
8. Rock-ice mixtures, containing roughly equal
parts asteroid-like rock and comet-like ice, like
some of the moons of Uranus;
9. "Proto-planets", dense clouds of dust and
asteroids that will become planets but haven't
collapsed completely yet;
10. Other things that we haven't even seen any
evidence yet.
Stars can also orbit other stars - this happens a
lot, in fact.
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