9:00 AM - 9:15 AM
*Yasunori MIURA1 (1.Yamaguchi, Visiting Univ.(In & Out))
Oral
Symbol P (Space and Planetary Sciences) » P-CG Complex & General
Wed. May 27, 2015 9:00 AM - 10:45 AM A02 (APA HOTEL&RESORT TOKYO BAY MAKUHARI)
Convener:*Masahiko Arakawa(Graduate School of Science, Kobe University), Taishi Nakamoto(Tokyo Institute of Technology), Sei-ichiro WATANABE(Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University), Masanao Abe(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), MASATERU ISHIGURO(Department of Physics and Astronomy, Seoul National University), Chair:Taishi Nakamoto(Tokyo Institute of Technology)
This session is aimed at setting up a forum to discuss how we can make progresses in our understanding of the solar system evolution with our hands on data. Presentations related to the science of the small bodies in the solar system (satellites, asteroids, comets, interplanetary dust particles, trans-Neptunian objects, and planetesimals) are invited. In addition to the extensive astronomical/remote-sensing observations and theoretical works, Hayabusa has brought us samples back from Itokawa (S-type asteroid) for unprecedentedly detailed analysis. The results of the Hayabusa sample initial analysis do prove that analysis of returned samples will play a key role in our future study of the solar system evolution. While the mission preparation of Hayabusa2, which is targeted at a more primordial asteroid than Itokawa (1999JU3, C-type), will be launched in 2014 winter, expectation of building a new gateway to biology-flavored topics via organic material and aqueous alternation analysis is ramping up. In this session, after summarizing the cutting-edge results obtained by various methods including the Hayabusa sample analysis, we will discuss the future shape of the study of the solar system evolution.
9:00 AM - 9:15 AM
*Yasunori MIURA1 (1.Yamaguchi, Visiting Univ.(In & Out))
9:15 AM - 9:30 AM
*Yusuke NAKAUCHI1, Toru MATSUMOTO2, Masanao ABE3, Akira TSUCHIYAMA2, Kohei KITAZATO4, Koutaku SUZUKI5 (1.SOKENDAI(The Graduate University for Advanced Studies), 2.Kyoto University, 3.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 4.University of Aizu, 5.Wakasa Wan Energy Research Center)
9:30 AM - 9:45 AM
*Masato KIUCHI1, Akiko NAKAMURA1 (1.Graduate School of Science, Kobe University)
9:45 AM - 10:00 AM
*Eri TATSUMI1, Seiji SUGITA2 (1.Dept. of Complexity Science and Engineering, Univ. of Tokyo, 2.Dept. of Earth and Planetary Science, Univ. of Tokyo)
10:00 AM - 10:15 AM
*Shota TAKANO1, Masahiko ARAKAWA1, Minami YASUI1, Sunao HASEGAWA2 (1.Graduate School of Science, Kobe University, 2.Japan Aerospace Exploration Agency)
10:15 AM - 10:30 AM
Sayaka TSUJIDO1, *Masahiko ARAKAWA1, Ayako SUZUKI2, Minami YASUI1, Kazuma MATSUE1, Shota TAKANO1, Sunao HASEGAWA2 (1.Graduate School of Science, Kobe University, 2.Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science)