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• W1965279169 abstract "Coupled thermal–orbital histories of early lunar evolution are considered in a simple model. We consider a plagioclase lid, overlying a magma ocean, overlying a solid mantle. Tidal dissipation occurs in the plagioclase lid and heat transport is by conduction and melt migration. We find that large orbital eccentricities can be obtained in this model. We discuss possible consequences of this phase of large eccentricities for the shape of the Moon and geochronology of lunar samples. We find that the orbit can pass through the shape solution of Garrick-Bethell et al. (Garrick-Bethell, I., Wisdom, J., Zuber, M. [2006]. Science 313, 652), but we argue that the shape cannot be maintained against elastic deformation as the orbit continues to evolve." @default.
• W1965279169 created "2016-06-24" @default.
• W1965279169 creator A5048892543 @default.
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• W1965279169 date "2010-07-01" @default.
• W1965279169 modified "2023-09-26" @default.
• W1965279169 title "Coupled thermal–orbital evolution of the early Moon" @default.
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• W1965279169 doi "https://doi.org/10.1016/j.icarus.2010.01.029" @default.
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