Session Details
[P-CG10]Small Solar System Bodies: General and Mars Satellite Sample Return Mission
Sun. May 22, 2016 9:00 AM - 10:30 AM JST
Sun. May 22, 2016 12:00 AM - 1:30 AM UTC
Sun. May 22, 2016 12:00 AM - 1:30 AM UTC
303 3F
Convener:*Taishi Nakamoto(Tokyo Institute of Technology), Kiyoshi Kuramoto(Department of Cosmosciences, Graduate School of Sciences, Hokkaido University), Sei-ichiro WATANABE(Division of Earth and Planetary Sciences, Graduate School of Science, Nagoya University), MASATERU ISHIGURO(Department of Physics and Astronomy, Seoul National University), Masahiko Arakawa(Graduate School of Science, Kobe University), Masanao Abe(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Tomoko Arai(Planetary Exploration Research Center, Chiba Institute of Technology), Sho Sasaki(Department of Earth and Space Sciences, School of Science, Osaka University), Chair:Masanao Abe(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
Small solar system bodies, including asteroids, comets, satellites,
inter-planetary dust particles, and planetesimals, are important objects:
their current state is interesting, and they provide lots of information on
the origin and evolution of our solar system for us. In this session, a
variety of papers on small solar system bodies are presented. Studies based
on various kinds of approaches such as space missions, measurements,
laboratory experiments, numerical simulations, and theoretical works are
discussed. Through those discussions, our understanding of the solar system
formation and evolution should be progressed. In 2016, the Mars satellite
sample return mission is paid special attention, though all the topics on
the small solar system bodies are welcome.
inter-planetary dust particles, and planetesimals, are important objects:
their current state is interesting, and they provide lots of information on
the origin and evolution of our solar system for us. In this session, a
variety of papers on small solar system bodies are presented. Studies based
on various kinds of approaches such as space missions, measurements,
laboratory experiments, numerical simulations, and theoretical works are
discussed. Through those discussions, our understanding of the solar system
formation and evolution should be progressed. In 2016, the Mars satellite
sample return mission is paid special attention, though all the topics on
the small solar system bodies are welcome.
[PCG10-01]Thermal Infrared Imager TIR on Hayabsua2 and Its In-Flight Performance using Earth-Moon Thermal Images.
*Tatsuaki Okada1,9, Tetsuya Fukuhara2, Satoshi Tanaka1,9, Makoto Taguchi3, Takeshi Imamura1,9, Takehiko Arai8, Hiroki Senshu4, Yoshiko Ogawa5, Hirohide Demura5, Kohei Kitazato5, Ryosuke Nakamura6, Toru Kouyama6, Tomohiko Sekiguchi7, Sunao Hasegawa1, Tsuneo Matsunaga8, Takehiko Wada1, Jun Takita9, Naoya Sakatani1, Yamato Horikawa10, Ken Endo5, Joern Helbert11, Thomas G. Mueller12, Axel Hagermann13 (1.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 2.National Institute of Information and Communications Technology, 3.Rikkyo University, 4.Chiba Institute of Technology, 5.University of Aizu, 6.National Institute of Advanced Industrial Science and Technology, 7.Hokkaido University of Education, 8.National Institute of Environmental Studies, 9.University of Tokyo, 10.Graduate University for Advanced Studies, 11.German Aerospace Center, 12.Max-Planck Institute for Extraterrestrial Physics, 13.Open University)
[PCG10-02]Image and database browser for TIR on Hayabusa2
*Ken Endo1, Naru Hirata1, Wataru Ueno1, Hirohide Demura1, Takehiko Arai2, Tatsuaki Okada3, Satoshi Tanaka4 (1.The University of Aizu, 2.National Institute for Environmental Studies, 3.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 4.Department of Solid Planetary Sciences Institute of Space and Astronautical Science)
[PCG10-03]Curation works for the Hayabusa samples and development for Hayabusa2 sample curation facility
*Toru Yada1, Masanao Abe1, Tatsuaki Okada1, Hisayoshi Yurimoto3, Masayuki Uesugi1, Yuzuru Karouji1, Aiko Nakato1, Minako Hashiguchi1, Toru Matsumoto1, Masahiro Nishimura2, Kazuya Kumagai1, Shigeo Matsui1, Masaki Fujimoto1 (1.Japan Aerospace Exploration Agency, 2.Marine Works Japan, 3.Hokkaido University)
[PCG10-04]Current Status of Hayabusa2 Landing Site Deliberation
*Aiko Nakato1, Hikaru Yabuta2, Mutsumi Komatsu3, Tomokatsu Morota4, Moe Matsuoka5, Seiji Sugita6, Takaaki Hiroi7, Kohei Kitazato8, Tatsuaki Okada1, Hiroki Senshu9, Sho Sasaki2, Tomoki Nakamura4, Naoki Kobayashi1, Seiichiro Watanabe5, Hayabusa2 Landing Site Working Group (1.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 2.Osaka University, 3.The Graduate University for Advanced Studies [SOKENDAI], 4.Nagoya University, 5.Tohoku University, 6.The University of Tokyo, 7.Brown University, 8.University of Aizu, 9.Chiba Institute of Technology)
[PCG10-05]Opposition Effect and Macroscopic Roughness on an Asteroid (25143) Itokawa taken with the Hayabusa Spacecraft Multi-Band Imaging Camera (AMICA)
*Mingyeong Lee1, MASATERU ISHIGURO1 (1.Seoul National University)
[PCG10-06]The Effect of Rotation Period on Slope Distribution on Asteroid Itokawa
*Masanori Kanamaru1, Sho Sasaki1 (1.Osaka University)