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Photosphere

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Encyclopedia of Astrobiology

  • 203 Accesses

Definition

The photosphere corresponds to the apparent visible surface of a star and especially of the Sun. It is a very thin shell where most of the light a star radiates is produced. Its thickness is less than one thousandth of the star’s radius. Its temperature, which is typically between 3,000 and 40,000 K, is one of the fundamental parameters characterizing a stellar type.

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Authors and Affiliations

  1. LESIA, Observatoire Paris-Site de Meudon, 5 Pl Jules Janssen, 92195, Meudon, France

    Daniel Rouan

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  1. Daniel Rouan
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Correspondence to Daniel Rouan .

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Editors and Affiliations

  1. Centro de Biología Molecular, Universidad Autónoma de Madrid, Madrid, Spain

    Ricardo Amils

  2. Labo. d'Astrophysique de Bordeaux (LAB), Observatoire Aquitain des Sciences de l'Univers (OASU), Floirac CX, France

    Muriel Gargaud

  3. Centro de Astrobiología (CAB), Inst. Nacional de Técnica Aeroespacial, Torrejón de Ardoz, Madrid, Spain

    José Cernicharo Quintanilla

  4. Geophysical Lab., Carnegie Institution of Washington, Washington, District of Columbia, USA

    Henderson James Cleaves

  5. Astronomy Department, University of Massachusetts, Amherst, Massachusetts, USA

    William M. Irvine

  6. Dépt. Sc. de la Terre et de l’Atmosphère, Université du Québec, Montréal, Montreal, Québec, Canada

    Daniele Pinti

  7. Centre National d'Etudes Spatiale (CNES) DPI/E2U, Paris CX, France

    Michel Viso

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© 2014 Springer-Verlag Berlin Heidelberg

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Rouan, D. (2014). Photosphere. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_4013-2

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_4013-2

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Online ISBN: 978-3-642-27833-4

  • eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics

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