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The protosun composition is the initial composition of the giant molecular cloud, from which the solar system has formed (sun and protoplanetary disk). This composition consists of about 70.5 % hydrogen, 27.5 % helium, and 2 % of heavier elements.
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© 2014 Springer-Verlag Berlin Heidelberg
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Alibert, Y., Helled, R. (2014). Protosun Composition. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_5110-2
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DOI: https://doi.org/10.1007/978-3-642-27833-4_5110-2
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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