Место издания:ИНСТИТУТ КОСМИЧЕСКИХ ИССЛЕДОВАНИЙ РОССИЙСКОЙ АКАДЕМИИ НАУК (ИКИ РАН), 117997, Москва, Профсоюзная ул., 84/32 ИНСТИТУТ КОСМИЧЕСКИХ ИССЛЕДОВАНИЙ РОССИЙСКОЙ АКАДЕМИИ НАУК (ИКИ РАН), 117997, Москва, Профсоюзная ул., 84/32
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Аннотация:For the early stage of the Moon’s development, a possible lunar topographyand internal density distribution were determined. The distribution of anomaliesof the attractive force and gravitational potential in various layersof the upper mantle is found, due to the gravity influence of the anomalousstructures of the crust and mantle. An analysis of the results leads to the conclusionabout the possibility of convective movements in molten electricallyconductive layers of the mantle, enriched in Fe, which could generate an ancientmagnetic field.For the current state of the density structure of the Moon [1] (Chuikovaet al., 2020), gravitational anomalies in various layers have also been determined,which can lead to solid-state convection in some hardened regionsof the Moon.REFERENCES:[1] Chuikova N. A., Nasonova L. P., Maksimova T. G. Determination of Global DensityInhomogeneities and Stresses Inside the Moon // Solar System Research. 2020