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From stellar nebula to planets: The refractory components

Author： Thiabaud Amaury Marboeuf Ulysse Alibert Yann Cabral Nahuel Leya Ingo Mezger Klaus

Publisher： Edp Sciences

E-ISSN： 1432-0746|562|issue|A27-A27

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.562, Iss.issue, 2014-02, pp. : A27-A27

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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Abstract

Context. To date, calculations of planet formation have mainly focused on dynamics, and only a few have considered the chemical composition of refractory elements and compounds in the planetary bodies. While many studies have been concentrating on the chemical composition of volatile compounds (such as H₂O, CO, CO₂) incorporated in planets, only a few have considered the refractory materials as well, although they are of great importance for the formation of rocky planets.

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