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Formation of the Sun and its Planets

  • Chapter
Physics of the Sun

Part of the book series: Geophysics and Astrophysics Monographs ((GAAM,volume 26))

Abstract

The Sun formed 4.6 Gy ago, probably as a fragment of a collapsing gas and dust cloud in close association with other stars, from which cluster it was ejected rather early. Conditions in the Galaxy then were not remarkably different from what they are now. Material of the solar system was processed through at least two supernova events within ~200 My before its formation, the last of them recent enough (~2 My) that it plausibly influenced the collapse which formed then Sun.

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Authors and Affiliations

  1. Dept of Earth and Space Sciences, Univ. of California, Los Angeles, CA, 90024, USA

    William M. Kaula

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  1. William M. Kaula
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Editors and Affiliations

  1. Center for Space Science and Astrophysics, Stanford University, Stanford, California, USA

    Peter A. Sturrock

  2. High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado, USA

    Thomas E. Holzer  & Dimitri M. Mihalas  & 

  3. Astronomy Department, University of California, Los Angeles, California, USA

    Roger K. Ulrich

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© 1986 Reidel Publishing Company

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Kaula, W.M. (1986). Formation of the Sun and its Planets. In: Sturrock, P.A., Holzer, T.E., Mihalas, D.M., Ulrich, R.K. (eds) Physics of the Sun. Geophysics and Astrophysics Monographs, vol 26. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5255-3_1

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  • DOI: https://doi.org/10.1007/978-94-009-5255-3_1

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8820-6

  • Online ISBN: 978-94-009-5255-3

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