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- W1507050874 abstract "Full Moon convection models of lunar interior evolution are usually simplified in their compositional setup. They are often purely thermal convection-diffusion models, using a homogeneous mantle composition and a heat reservoir to model the core [1, 2]. Other models add only an ilmenite-rich layer at shallow depth [3, 4]. When this compositionally distinct and relatively dense layer is used, the focus is typically on the overturn of the lunar mantle, due to the gravitational instability which originated from the crystallisation of an early lunar magma ocean. In this study, we investigate compositionally more complex models. The initial configuration of our models has a both mineralogically and geochemically layered composition, to determine the influence of a more realistic mantle stratification on mantle dynamics and the thermal evolution of the Moon." @default.
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- W1507050874 date "2011-03-01" @default.
- W1507050874 modified "2023-09-23" @default.
- W1507050874 title "Numerical convection modelling of a compositionally stratified lunar mantle" @default.
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