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- W2367140663 abstract "The admittance signatures (the ratio of the gravity and topography data in spectral domain)for the four lunar mare basins (Smythii,Crisium,Imbrium,Orientale),which of them have different age,is calculated by a Multitaper method,then compare this observed admittance with the theoretical values from the elastic lithospherical flexure model.On the basis of this method,we obtain the elastic thickness for the four mare basins.The elastic thickness of them are averaged about 8 km to support the observed topography since the time of the loading.The crust thickness increase when the evolution wheel of the moon went ahead.The crust thickness increase from 72 km(Smythii basin) to 70 km(Crisium basin) to 60 km (Orientale basin) to 57 km(Imbrium basin).These results are consistent with thermal history of this planets." @default.
- W2367140663 created "2016-06-24" @default.
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- W2367140663 date "2009-01-01" @default.
- W2367140663 modified "2023-09-24" @default.
- W2367140663 title "Estimation of the ancient lunar crust thickness from the admittance" @default.
- W2367140663 hasPublicationYear "2009" @default.
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