10:45 AM - 11:00 AM
*Yasuhito Sekine1, Takazo Shibuya2, Taro Funatsu1 (1.Department of Earth and Planetary Science, University of Tokyo, 2.Laboratory of Ocean-Earth Life Evolution Research, JAMSTEC)
International Session (Oral)
Symbol P (Space and Planetary Sciences) » P-PS Planetary Sciences
Sun. May 22, 2016 10:45 AM - 12:15 PM A02 (APA HOTEL&RESORT TOKYO BAY MAKUHARI)
Convener:*Jun Kimura(Earth-Life Science Institute, Tokyo Institute of Technology), Masaki Fujimoto(Institite of Space and Astronautical Science, Japan Aerospace Exploration Agency), Yasumasa Kasaba(Dep. Geophysics Graduate School of Science Tohoku University), Sho Sasaki(Department of Earth and Space Sciences, School of Science, Osaka University), Takayuki Tanigawa(School of Medicine, University of Occupational and Environmental Health), Yasuhito Sekine(Department of Earth and Planetary Science, University of Tokyo), Kunio Sayanagi(Atmospheric and Planetary Sciences Department, Hampton University), Steven Vance(Jet Propulsion Laboratory, Caltech), Chair:Jun Kimura(Earth-Life Science Institute, Tokyo Institute of Technology), Noriyuki Namiki(RISE Project, National Astronomical Observatory of Japan)
The giant planets provide many keys to understanding planetary processes.
They play an important role in shaping our solar system, and the physical and chemical processes they harbor also provide a unique opportunity to study the phenomena relevant for studying Earth and other planets, including exoplanetary systems. In this session, we discuss a wide range of topics encompassing the giant planets and their moons, including their origins, interiors, atmospheres, compositions, surface features, and electromagnetic fields. To advocate for current and future outer planets exploration (Cassini, Juno, New Horizons, JUICE, and beyond), we also call for discussions on future missions to explore giant planet systems, including how to develop better international cooperation. Discussion in this latter category will include progress in developing a solar sail mission concept for observing the Jupiter system and its trojan asteroids.
10:45 AM - 11:00 AM
*Yasuhito Sekine1, Takazo Shibuya2, Taro Funatsu1 (1.Department of Earth and Planetary Science, University of Tokyo, 2.Laboratory of Ocean-Earth Life Evolution Research, JAMSTEC)
11:00 AM - 11:20 AM
*Christophe Sotin1 (1.Jet Propulsion Laboratory - California Institute of Technology, Pasadena, CA (USA))
11:20 AM - 11:35 AM
*Hussmann Hauke1, G. Steinbruegge1, A. Stark1, J. Oberst1, K. Lingenauber1, J. Kimura2, K. Enya3, N. Namiki4, M. Kobayashi5, K. Touhara3, N. Thomas6, K. Seiferlin6, L. Lara7 (1.DLR Institute of Planetary Research, 2.ELSI, Tokyo, 3.ISAS/JAXA, 4.NAOJ, 5.Chiba Inst. Technology, 6.University of Bern, 7.IAA-CSIC)
11:35 AM - 11:55 AM
*Louise M Prockter1, Robert T. Pappalardo2, David A. Senske2, Brian G. Paczkowski2, Rachel L. Klima1, Kathleen L. Craft1, Steven D. Vance2, Barry G. Goldstein2, Thomas J. Magner1, Brian C. Cooke2 (1.Johns Hopkins University Applied Physics Laboratory, 2.Jet Propulsion Laboratory)
11:55 AM - 12:15 PM
*Morgan E O'Neill1, Yohai Kaspi1, Eli Galanti1 (1.Weizmann Institute of Science)