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- W319830798 abstract "This study is aimed at the interior structure and thermal state of massive rocky exoplanets. We have modeled the interior structure of confirmed super-Earths CoRoT-7b and Kepler-10b, applying a mixing length approach for the radial temperature distribution. 2-D cylindrical mantle convection simulations are performed using the compressible anelastic approximation. These demonstrate the importance of the usage of depth-dependent thermodynamic parameters such as thermal expansivity, conductivity, and density. The calculations indicate that CoRoT-7b and Kepler-10b are similarly composed. Whereas thermal conductivity and density increase with depth by a factor of two, thermal expansivity decreases by more than an order of magnitude across the mantle. The planform of mantle convection is strongly modified in the presence of depth-dependent material properties with hot plumes rising across the whole mantle and cold downwellings assimilated in the mid mantle." @default.
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- W319830798 date "2011-07-01" @default.
- W319830798 modified "2023-09-27" @default.
- W319830798 title "Thermal structure and interior dynamics of the first rocky exoplanets" @default.
- W319830798 hasPublicationYear "2011" @default.
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