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<h1>Solar system</h1>
<p>The Solar System is the gravitationally bound system comprising the Sun and the objects that
orbit it, either directly or indirectly. Of those objects that orbit the Sun directly,
the largest eight are the planets, with the remainder being significantly smaller objects,
such as dwarf planets and small Solar System bodies.
Of the objects that orbit the Sun indirectly, the moons,
two are larger than the smallest planet, Mercury.</p>
<p>The Solar System formed 4.6 billion years ago from the gravitational collapse of a giant
interstellar molecular cloud. The vast majority of the system's mass is in the Sun, with most
of the remaining mass contained in Jupiter. The four smaller inner planets, Mercury, Venus,
Earth and Mars, are terrestrial planets, being primarily composed of rock and metal.
The four outer planets are giant planets, being substantially more massive than the terrestrials.
The two largest, Jupiter and Saturn, are gas giants, being composed mainly of hydrogen and helium;
the two outermost planets, Uranus and Neptune, are ice giants,
being composed mostly of substances with relatively high melting points compared with hydrogen
and helium, called volatiles, such as water, ammonia and methane.
All planets have almost circular orbits that lie within a nearly flat disc called the ecliptic.</p>
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<h1>Sun</h1>
<p>The Sun is the Solar System's star and by far its most massive component.
Its large mass (332,900 Earth masses) produces temperatures and densities in its core
high enough to sustain nuclear fusion of hydrogen into helium, making it a main-sequence star.
