About History of solar system
The Solar Systemis the gravitationally bound system of the Sun and the objects that orbit it.It formed about 4.6 billion years ago when a dense region of a molecular cloud collapsed, forming the Sun and a protoplanetary disc. The Sun is a typical star that maintains a balanced equilibrium by the fusion of hydrogen.
PastThe Solar System formed at least 4.568 billion years ago from the gravitational collapse of a region within a large .This initial cloud was likely several light.
The inner Solar System is the region comprising the terrestrial planets and the .Composed mainly ofand metals,the.
Beyond the orbit of Neptune lies the area of the "", with the doughnut-shaped Kuiper belt, home of Pluto and several other dwarf planets, and an overlapping disc.
Astronomers sometimes divide the Solar System structure into separate regions. Theincludes Mercury, Venus, Earth, Mars, and the bodies in the . Theincludes Jupiter, Saturn, Uranus, Neptune, and the bodies in the .
The Sun is the Solar System's star and by far its most massive component. Its large mass (332,900 ),which comprises 99.86% of.
The outer region of the Solar System is home to theand their large moons. Theand manyorbit.
CometsComets are , typically only a few kilometers across, composed largely of volatile ices. They have highly eccentric.
Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a "Solar System", simply because it was not generally thought that the Solar System, in the sense we now understand it, existed. The first step toward a theory of Solar System formation and evolutio.
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