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Inside the Sun : Unsolved Problems

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Inside the Sun

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 159))

Abstract

As it is impossible to approach all the problems concerning the inside of the Sun, a number of questions will not be taken into consideration during the meeting. In this brief overview of the presently unsolved questions I shall insist on some special aspects of the solar properties: the variations of the solar radius, the generation of the solar wind, some interesting effects due to the presence of a strong gradient of 3He, the history of the rotating Sun. The presence of the planetary system suggests that the Sun might have been a T Tauri star, with an accretion disc and may have started on the mains sequence as a fast rotating star. A sketch is given of the possible consequences.

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Author information

Authors and Affiliations

  1. Observatoire de Meudon, DASGAL, 92195, Meudon-Cedex, France

    E. Schatzman

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  1. E. Schatzman
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Editor information

Editors and Affiliations

  1. Observatoire de la Côte d’Azur, Nice, France

    Gabrielle Berthomieu

  2. CEN, Saclay, France

    Michel Cribier

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© 1990 Kluwer Academic Publishers

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Schatzman, E. (1990). Inside the Sun : Unsolved Problems. In: Berthomieu, G., Cribier, M. (eds) Inside the Sun. Astrophysics and Space Science Library, vol 159. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0541-2_2

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  • DOI: https://doi.org/10.1007/978-94-009-0541-2_2

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6730-0

  • Online ISBN: 978-94-009-0541-2

  • eBook Packages: Springer Book Archive

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