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- W2051056568 abstract "In studying the conditions of formation of stony meteorites, we assume that 1) they are fragments of asteroids fallen to the surface of the earth. During their flight through the atmosphere, the meteorites develop a melted surface layer but their texture and mineralogic composition remain unchanged. 2) According to V. M. Goldschmidt, stone meteorites crystallize in a lesser gravity field than that of the earth, which is the reason for their chondritic texture and high porosity (about 4%). 3) Meteorites were formed in a medium with a deficiency of free oxygen. As a result, part of their iron and nickel was segregated as native metal; in addition, lawrencite and oldhamite, sulfides typical of meteorites, were formed. We identify three stages of meteorite formation: magmatic, pneumatolytic, and hydrothermal. The interval 1450-850°C. corresponds to the magmatic stage at which a silicate phase and native iron with nickel were formed. As a result of thermal dissociation of water and because of the deficiency of..." @default.
- W2051056568 created "2016-06-24" @default.
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- W2051056568 date "1962-06-01" @default.
- W2051056568 modified "2023-09-23" @default.
- W2051056568 title "GEOCHEMICAL AND MINEROLOGIC STUDY OF A STONY METEORITE FROM THE VICINITY OF THE VILLAGE OF SEVRYUKOVO" @default.
- W2051056568 doi "https://doi.org/10.1080/00206816209473714" @default.
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