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38.5 MB (3.7 MB compressed)
3199 x 4203 pixels
27.2 x 35.6 cm ⏐ 10.7 x 14.0 in (300dpi)
DR SETH SHOSTAK / SCIENCE PHOTO LIBRARY DR SETH SHOSTAK / SCIENCE PHOTO LIBRARY
Artwork representing the formation of a planetary system around a star based upon the nebular hypothesis. According to this model a solar system derives from the contraction of a rotating disc- shaped nebula mainly formed by hydrogen, helium and dust grains. The contraction may be triggered by shock waves from a nearby supernova explosion or simply by the mutual gravitational attraction of the contents of the nebula. The central part of the nebula collapses into a protostar. Collisions between dust grains in the outer regions of the nebula lead to the formation of small bodies (few kilometres across), which then by accretion will develop into planets.
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