宇宙惑星科学(P)
セッション小記号惑星科学(PS)
セッションIDP-PS04
タイトル和文Regolith Science
英文Regolith Science
タイトル短縮名和文Regolith Science
英文Regolith Science
代表コンビーナ氏名和文和田 浩二
英文Koji Wada
所属和文千葉工業大学惑星探査研究センター
英文Planetary Exploration Research Center, Chiba Institute of Technology
共同コンビーナ 1氏名和文中村 昭子
英文Akiko Nakamura
所属和文神戸大学大学院理学研究科地球惑星科学専攻
英文Graduate School of Science, Kobe University
共同コンビーナ 2氏名和文Patrick Michel
英文Patrick Michel
所属和文Observatoire De La Cote D'Azur
英文Observatoire De La Cote D'Azur
共同コンビーナ 3氏名和文Kevin John Walsh
英文Kevin John Walsh
所属和文Southwest Research Institute Boulder
英文Southwest Research Institute Boulder
発表言語E
スコープ和文Recent planetary explorations have revealed that almost all solid bodies in the solar system are covered with small particles, called regolith. The surface geology, especially regolith behavior on the surfaces of solid bodies, becomes increasingly more important as represented by Hayabusa mission and other on-going and planned sample-return missions such as Hayabusa2, OSIRIS-REx, and MMX.
For fully understanding the regolith science, it is required to know and compare the regolith conditions on various celestial bodies, from asteroids to planets, with various methods.
Therefore, this session welcomes broad topics related to regolith on various celestial bodies, such as asteroids, comets, the Moon, the martian moons, Mars, etc. Papers on the formation, evolution, and alteration processes of regolith particles and regolith systems on the surface of planetary bodies, remote and in-situ observational results and techniques, analyses and results of returned samples, and laboratory, numerical, and theoretical studies on the fundamental physical and chemical processes are all welcome.
Note that what we call regolith is not just fine grains: all kinds of materials (more or less loose) that lie on the surface, from cobbles to finer grains, are our targets.
英文Recent planetary explorations have revealed that almost all solid bodies in the solar system are covered with small particles, called regolith. The surface geology, especially regolith behavior on the surfaces of solid bodies, becomes increasingly more important as represented by Hayabusa mission and other on-going and planned sample-return missions such as Hayabusa2, OSIRIS-REx, and MMX.
For fully understanding the regolith science, it is required to know and compare the regolith conditions on various celestial bodies, from asteroids to planets, with various methods.
Therefore, this session welcomes broad topics related to regolith on various celestial bodies, such as asteroids, comets, the Moon, the martian moons, Mars, etc. Papers on the formation, evolution, and alteration processes of regolith particles and regolith systems on the surface of planetary bodies, remote and in-situ observational results and techniques, analyses and results of returned samples, and laboratory, numerical, and theoretical studies on the fundamental physical and chemical processes are all welcome.
Note that what we call regolith is not just fine grains: all kinds of materials (more or less loose) that lie on the surface, from cobbles to finer grains, are our targets.
発表方法口頭および（または）ポスターセッション