*Kevin John Walsh1, Harold C. Connolly Jr.2 (1.Southwest Research Institute, 2.Rowan University)
Session information
[EE] Poster
P (Space and Planetary Sciences) » P-PS Planetary Sciences
[P-PS03] [EE] Regolith Science
Tue. May 23, 2017 3:30 PM - 5:00 PM Poster Hall (International Exhibition Hall HALL7)
convener:Koji Wada(Planetary Exploration Research Center, Chiba Institute of Technology), Patrick Michel(University Cote d'Azur, Cote d'Azur Observatory, CNRS), Akiko Nakamura(Graduate School of Science, Kobe University), Kevin John Walsh(Southwest Research Institute)
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.
*Patrick Michel1, Yang Yu2 (1.University Cote d'Azur, Cote d'Azur Observatory, CNRS, Lagrange Laboratory, 2.Beihang University)
*Koji Wada1, Kazunori Ogawa2, Ko Ishibashi1, Naoya Sakatani3, Masahiko Arakawa2, Rie Honda4, Kei Shirai5, Minami Yasui2, Hirotaka Sawada6 (1.Planetary Exploration Research Center, Chiba Institute of Technology, 2.Kobe University, 3.Meiji University, 4.Kochi University, 5.SOKENDAI, 6.ISAS/JAXA)
*Tomoko Arai1, Masanori Kobayashi1, Manabu Yamada1, Hiroki Senshu1, Koji Wada1, Sohsuke Ohno1, Ko Ishibashi1, Ryo Ishimaru1, Keisuke Maeda1, Takafumi Matsui1 (1.Planetary Exploration Research Center, Chiba Institute of Technology)
*Shinta Takizawa1, Hiroaki Katsuragi1 (1.Nagoya Univ.)
*Masato Kiuchi1, Akiko Nakamura1, Koji Wada2 (1.Graduate School of Science, Kobe University, 2.Planetary Exploration Research Center, Chiba Institute of Technology)
[PPS03-P07] Measurements of cohesive force of regolith- simulated particles using centrifugal method
*Yuuya Nagaashi1, Tomomi Omura1, Akiko Nakamura1 (1.Kobe University)
*Tomomi Omura1, Akiko Nakamura1 (1.Graduate School of Science,Kobe University)
*Ayaka Oyanagi1, Hideaki Miyamoto2, Takafumi Niihara3 (1.Department of Earth and Planetary Science, School of Science, The University of Tokyo, 2.Department of Systems Innovation, School of Engineering, The University of Tokyo, 3.The University Museum, The University of Tokyo)
*Kazunori Ogawa1, Naoya Sakatani2, Shoko Tsuda3, Maho Ogawa3, Rie Honda4, Masahiko Arakawa1, Satoshi Tanaka5 (1.Kobe University, 2.Meiji University, 3.Tokyo University, 4.Kochi University, 5.Japan Aerospace Exploration Agency)
*Akiko Nakamura1, Ryo Ogawa1, Tomomi Omura1, Masato Kiuchi1, Ayako Suzuki2, Sunao Hasegawa2 (1.Graduate School of Science, Kobe University, 2.Japan Aerospace Exploration Agency)
Jan Deca1,2, Andrey Divin3,4, Charles Lue5, *Xu Wang1,2, Mihály Horányi1,2 (1.Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, USA, 2.Institute for Modeling Plasma, Atmospheres and Cosmic Dust, NASA/SSERVI, USA, 3.St. Petersburg State University, St. Petersburg, Russia, 4.Swedish Institute of Space Physics, Uppsala, Sweden, 5.Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa, USA)