9:00 AM - 9:15 AM
*Yuya Yamamoto1, Masahiko Arakawa1, Minami Yasui1, Sunao Hasegawa2, Yusaku Yokota1 (1.Graduate School of Science, Kobe University, 2.Japan Aerospace Exploration Agency)
[E] Oral
P (Space and Planetary Sciences ) » P-PS Planetary Sciences
Tue. May 23, 2023 9:00 AM - 10:15 AM 101 (International Conference Hall, Makuhari Messe)
convener:Koji Wada(Planetary Exploration Research Center, Chiba Institute of Technology), Akiko Nakamura(Graduate School of Science, Kobe University), Patrick Michel(Universite Cote D Azur Observatoire De La Cote D Azur CNRS Laboratoire Lagrange), Kevin J Walsh, Chairperson:Yuya Yamamoto(Graduate School of Science, Kobe University), Akiko Nakamura(Graduate School of Science, Kobe University)
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.
9:00 AM - 9:15 AM
*Yuya Yamamoto1, Masahiko Arakawa1, Minami Yasui1, Sunao Hasegawa2, Yusaku Yokota1 (1.Graduate School of Science, Kobe University, 2.Japan Aerospace Exploration Agency)
9:15 AM - 9:37 AM
*Olivier S Barnouin1, Ronald L. Ballouz1, S. - Marchi2, J.-B. - Vincent3, M. - Pajola4, A. - Lucchetti4, F. - Tusberti4, Ronald T Daly1, Carolyn M. Ernst1, E. - Palmer5, R. Gaskell5, T. - Kohout6, C. - Robin7, N. - Murdoch7, J. - Sunshine8, T. - Farhham8, J. L. Rizos8, Yun - Zhang8, F. - Ferrari9, Harrison - Agrusa8,10, Masatoshi Hirabayashi11, L. - Parro12, S. - Cambioni13, Patrick Michel10, S. D. Raducan14, M. - Jutzi14, E. - Asphaug12, M. C. Nolan12, A. - Campo Bagatin15, J. M. Trigo-Rodriguez16, A. - Zinzi17, V. - Della Corte17, N. L. Chabot1, A. S. Rivkin1, A. F. Cheng1, E. - Dotto18 (1.Johns Hopkins University Applied Physics Laboratory, 2.SWRI (Boulder, Co), 3.DLR (Berlin, Germany), 4.INAF (Padua, Italy), 5.PSI (Tucson, Az), 6.U. Helsinki (Helsinki, Finland), 7.ISAE-SUPAERO (Toulouse, France), 8.U. Maryland (College Park, MD), 9.Politecnico di Milano (Milan, Italy), 10.OCA-CNRS (Nice, France), 11.Auburn U. (Auburn, Al), 12.U. Arizona (Tucson, Az), 13.MIT (Cambridge, MA), 14.U. Bern (Bern, Switzerland), 15.U. Alicante (Alicante, Spain), 16.CSIC-IEEC (Barcelona, Catalonia/Spain), 17.ASI (Rome, Italy), 18.INAF (Rome, Italy))
9:37 AM - 10:00 AM
*Naomi Murdoch1, D Mimoun1, K Hurst2, R D Lorenz3, A E Stott1, M Gillier1, A Spiga4, E Marteau2, M Golombek2, R F Garcia1, C Perrin5, R Widmer-Schnidrig6, S Rodriguez7, N Compaire1, N H Warner22, K Onodera23, T Kawamura7, P Delage8, D Banfield9,10, R Hueso11, M Lemmon12, G Martinez13, V Apéstigue14, D Toledo14, B Chide15, A Munguira11, A Sanchez-Lavega11, A Vicente-Retortillo16, C E Newman17, S Maurice18, M de la Torre Juárez2, T Bertrand19, S Navarro11, M Marin11, J Gomez-Elvira11, X Jacob20, A Cadu1, A Sournac1, A Trebi-Ollennu2, J A Rodriguez-Manfredi16, R C Wiens21, P Lognonné7, W B Banerdt2 (1.Institut Supérieur de l’Aéronautique et de l’Espace (ISAE-SUPAERO), 2.Jet Propulsion Laboratory, California Institute of Technology, 3.Johns Hopkins Applied Physics Laboratory, 4.Laboratoire de Météorologie Dynamique/Institut Pierre Simon Laplace (LMD/IPSL), Sorbonne Université, Centre National de la Recherche Scientifique (CNRS), 5.Laboratoire de Planétologie et Géodynamique, Nantes University, 6.Black Forest Observatory, Stuttgart University, 7.Institut de physique du globe, CNRS, Université de Paris, 8.Écoles de Ponts, ParisTech, 9.Cornell University, 10.NASA AMES Research Center, 11.Física Aplicada, Escuela de Ingeniería de Bilbao, Universidad del País Vasco (UPV/EHU), 12.Space Science Institute, 13.Lunar and Planetary Institute, Universities Space Research Association, 14.Instituto Nacional de Técnica Aeroespacial, 15.Space and Planetary Exploration Team, Los Alamos National Laboratory, 16.Centro de Astrobiología (INTA-CSIC), 17.Aeolis Research, 18.Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse 3 Paul Sabatier, CNRS, 19.Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique (LESIA), Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, 20.Institut de Mécanique des Fluides,Université de Toulouse III Paul Sabatier, INP, CNRS, 21.Earth, Atmospheric, and Planetary Sciences, Purdue University, 22.Department of Geological Sciences, SUNY Geneseo, 23.Earthquake Research Institute / The University of Tokyo)
10:00 AM - 10:15 AM
*Yuta Shimizu1, Hideaki Miyamoto1, Taishi Takada1, Taisuke Suzuki1, Kentaro Masuoka2 (1.University of Tokyo, 2.Taisei Cooperation)
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