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Link to original content: http://dx.doi.org/10.1023/A:1005161325181
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Standard Solar Composition

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Abstract

We review the current status of our knowledge of the chemical composition of the Sun, essentially derived from the analysis of the solar photospheric spectrum. The comparison of solar and meteoritic abundances confirms that there is a very good agreement between the two sets of abundances. They are used to construct a Standard Abundance Distribution.

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Authors and Affiliations

  1. Institut d'Astrophysique et de Géophysique, Université de Liège, B-4000, Liège, Belgium (

    N. Grevesse & A.J. Sauval

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  1. N. Grevesse
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  2. A.J. Sauval
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Grevesse, N., Sauval, A. Standard Solar Composition. Space Science Reviews 85, 161–174 (1998). https://doi.org/10.1023/A:1005161325181

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