Accretion of gas of the solar nebula by the growing terrestrial planets and the early stages of the evolution of the solar system

Details Accretion of gas of the solar nebula by the growing terrestrial planets and the early stages of the evolution of the solar system Accretion of gas of the solar nebula by the growing terrestrial planets and the early stages of the evolution of the solar system

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..283i&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, Mar.-Apr. 1985, p. 283-295. In Russian.

Physics

Accretion Disks, Planetary Evolution, Protoplanets, Solar System, Stellar Mass Ejection, Terrestrial Planets, Gas Dynamics, Planetary Nebulae, Rare Gases, Venera Satellites

Scientific paper

An interpretation of Venera 11-14 measurements of the concentration of rare gases in the Venus atmosphere supports the hypothesis that the predominant part of the primary isotopes of rare gases entered the atmospheres of Venus, earth, and Mars by accretion of gas of the solar nebula during the growth of the solid bodies of these plants. A description is given of the time-dependent conditions that should have existed in order for the growing terrestrial planets to gain through accretion small primordial atmospheres, providing for the observed amount of rare gases.

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