Two types of co-accretion scenarios for the origin of the Moon
スポンサーリンク
概要
著者
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Watanabe Sei-ichiro
Department Of Earth And Planetary Science Graduate School Of Science Nagoya University
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Watanabe Sei-ichiro
Departmemt Of Earth And Planetary Sciences Nagoya University
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MORISHIMA Ryuji
Departmemt of Earth and Planetary Sciences, Nagoya University
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Morishima Ryuji
Departmemt Of Earth And Planetary Sciences Nagoya University
関連論文
- Two types of co-accretion scenarios for the origin of the Moon
- Numerical simulations of mid-ocean ridge hydrothermal circulation including the phase separation of seawater
- Evaporation of Fe and FeS dust in the active stage of the primordial solar nebula, and Fe/S fractionation
- Analytic model of upper tropospheric clouds in the tropical Hadley cell
- Ice sublimation of dust particles and their detection in the outer solar system
- Sublimation temperature of circumstellar dust particles and its importance for dust ring formation