Coupled thermal-orbital models show lava planets undergo two-stage migration from ~0.1 AU requiring initial eccentricities >=0.9 and sustained forcing, with migration rate depending on mantle state.
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Mantle partial melting buffers magma-ocean differentiation more on Earth than Mars due to stronger convection, explaining the presence of a basal dense layer only on Mars.
citing papers explorer
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Coupled orbital and interior structure evolution of lava planets
Coupled thermal-orbital models show lava planets undergo two-stage migration from ~0.1 AU requiring initial eccentricities >=0.9 and sustained forcing, with migration rate depending on mantle state.
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Earth and Mars interior structures set by re-melting of the first solid mantle
Mantle partial melting buffers magma-ocean differentiation more on Earth than Mars due to stronger convection, explaining the presence of a basal dense layer only on Mars.