Low Mg/Si planetary host stars and their Mg-depleted terrestrial planets

Simulations have shown that a diverse range of extrasolar terrestrial planet bulk compositions are likely to exist, based on the observed variations in host star elemental abundances. Based on recent studies, it is expected that a significant proportion of host stars may have Mg/Si ratios below 1. H...

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Veröffentlicht in:arXiv.org 2012-01
Hauptverfasser: Carter-Bond, Jade C, O'Brien, David P, Elisa Delgado Mena, Israelian, Garik, Santos, Nuno C, Gonzalez Hernandez, Jonay I
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Sprache:eng
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