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Solar system formation

Solar system formation

R301/0027

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Credit

MARK GARLICK / SCIENCE PHOTO LIBRARY MARK GARLICK / SCIENCE PHOTO LIBRARY

Caption

Solar system formation. Artwork of the early solar system being formed. It is thought that the Sun and the planets formed from a cloud of gas and dust around 4. Gravitational condensation of this cloud (or nebula) formed a protostar (lower centre) which has ignited under its own weight. The remaining material forms a rotating disc around this newly-formed Sun. The planets are forming from the disc by accretion, a slow process of gravitational attraction. This formation of a disc occurs throughout the universe as it follows from a universal law requiring the conservation of a rotational property (angular momentum) of the collapsing nebula.

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