Mathematics – Logic
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986stin...8630615f&link_type=abstract
Volatile components and continental material of planets Transl. into ENGLISH from Geokhimiya (Moscow, USSR), no. 9, 1984 p 1251
Mathematics
Logic
Continents, Planetary Atmospheres, Planetary Environments, Planetary Evolution, Planetary Geology, Terrestrial Planets, Gases, Impact Melts, Primitive Earth Atmosphere, Volatility
Scientific paper
It is shown that the continental material of the terrestrial planets varies in composition from planet to planet according to the abundances and composition of true volatiles (H20, CO2, etc.) in the outer shells of the planets. The formation of these shells occurs very early in a planet's evolution when the role of endogenous processes is indistinct and continental materials are subject to melting and vaporizing in the absence of an atmosphere. As a result, the chemical properties of continental materials are related not only to fractionation processes but also to meltability and volatility. For planets retaining a certain quantity of true volatile components, the chemical transformation of continental material is characterized by a close interaction between impact melting vaporization and endogeneous geological processes.
Florenskiy K. P.
Nikolayeva O. V.
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