S.V. Rasskazov1,2, I.S. Chuvashova1,2,
1Institute of the Earth's Crust SB RAS, Irkutsk, Russia
2Irkutsk State University, Irkutsk, Russia
Rasskazov Sergei Vasilievich,
doctor of geological and mineralogical sciences, professor,
664025 Irkutsk, st. Lenina, 3,
Irkutsk State University, Faculty of Geology,
Head of Dynamic Geology Chair,
664033 Irkutsk, st. Lermontova, 128,
Institute of the Earth's Crust SB RAS,
Head of the Laboratory for Isotopic and Geochronological Studies,
tel.: (3952) 51–16–59,
email: rassk@crust.irk.ru.
Chuvashova Irina Sergeevna,
candidate of geological and mineralogical sciences,
Senior Researcher,
664025 Irkutsk, st. Lenina, 3,
Irkutsk State University, Faculty of Geology,
Associate Professor of the Dynamic Geology chair,
664033 Irkutsk, st. Lermontova, 128,
Institute of the Earth's Crust SB RAS,
Senior Researcher,
tel.: (3952) 51–16–59,
email: chuvashova@crust.irk.ru.
Abstract. A review of lunar studies is given that indicate the isotope crisis of the Earth mega-impact hypothesis and the removal of emerging contradictions by a competing model of the origin of the Earth-Moon binary system from a gas-dust cloud. The simultaneous solidification of the magma ocean of the Moon with the solidification of the magma ocean in the global ASITA heterogeneity of the Earth 4.54–4.44 billion years ago is substantiated. From the model of the Earth–Moon binary system, the solidification of the ASITA magma ocean is assumed to precede the solidification of the rest of the Earth. It is concluded that the Earth's crust consolidated at different times after the solidification of the magma ocean: in ASITA – 4.31 billion years ago and in the rest of the Earth – with a delay of up to 3.82 billion years ago.
Keywords: early Earth, Moon, mega impact, gas and dust cloud, magma ocean, geochemistry.
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