Session Details
[P-PS05]Mars
Thu. May 28, 2015 11:00 AM - 12:45 PM JST
Thu. May 28, 2015 2:00 AM - 3:45 AM UTC
Thu. May 28, 2015 2:00 AM - 3:45 AM UTC
A03 APA HOTEL&RESORT TOKYO BAY MAKUHARI
Convener:*Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Masaki Ishiwatari(Department of Cosmosciences, Graduate school of Science, Hokkaido University), Sho Sasaki(Department of Earth and Space Sciences, School of Science, Osaka University), Yoshiyuki O. Takahashi(Graduate School of Science, Kobe University), Ayako Matsuoka(Research Division for Space Plasma, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Hideaki Miyamoto(The University Museum, The University of Tokyo), Chair:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
The study on Mars has greatly been advanced due to new data from modern missions as well as to new results from theoretical and numerical works. Morphology and variable phenomena, seen on the surface, in the atmosphere and its surrounding plasma, all indicate that Mars is still an active planet. After successful arrivals of American and Indian orbiters in 2014, Mars is now being investigated by 5 orbiters and 2 rovers, the largest ever number.
In Japan, on the other hand, possibilities of small planetary missions are becoming more realistic (Mars is the most important target object, of course) and the roadmap of solar system exploration is under development. In this session, current researches on Mars, including the latest results from missions, as well as future mission plans are discussed.
In Japan, on the other hand, possibilities of small planetary missions are becoming more realistic (Mars is the most important target object, of course) and the roadmap of solar system exploration is under development. In this session, current researches on Mars, including the latest results from missions, as well as future mission plans are discussed.
[PPS05-10]Possible landing sites on Mars for an in-situ K-Ar dating by future Japan's Mars rover mission
*Yayoi N. MIURA1, Yuichiro CHO2, Tomokatsu MOROTA3, Hideaki MIYAMOTO4, Tomohiro USUI5, Shingo KAMEDA2, Seiji SUGITA6, Ryuji OKAZAKI7 (1.ERI, Univ. Tokyo, 2.Rikkyo Univ., 3.Nagoya Univ., 4.Univ. Museum, Univ. Tokyo, 5.Tokyo Inst. Tech., 6.Univ. Tokyo, 7.Kyushu Univ.)
[PPS05-11]Remote sensing of Martian surface events by Electro-magnetic and Sonic Wave observation aboard a Martian rover
*Masa-yuki YAMAMOTO1, Mitsuteru SATO2, Keigo ISHISAKA3, Yukihiro TAKAHASHI2, Masashi KAMOGAWA4, Kazunori OGOHARA5, Hideaki MIYAMOTO6 (1.Kochi University of Technology, 2.Hokkaido University, 3.Toyama Prefectural University, 4.Tokyo Gakugei University, 5.University of Shiga Prefecture, 6.The Unversity of Tokyo)
[PPS05-12]Characterization of Martian Regolith: Toward 2020s Mars Exploration Missions
*Tomohiro USUI1, Akihiko Yamagishi2, Takehiko Sato3, Hideaki Miyamoto4, Shingo Kameda5, Kazuhisa Fujita3, Yasuhito Sekine4, Shogo Tachibana6, Sei-ichro Watanabe7 (1.Tokyo Institute of Technology, 2.Tokyo University of Pharmacy and Life Science, 3.ISAS, JAXA, 4.The University of Tokyo, 5.Rikkyo University, 6.Hokkaido University, 7.Nagoya University)
[PPS05-13]Geological implications of landing-site candidates of the MELOS mission
*Hideaki MIYAMOTO1, Goro KOMATSU2, Tomohiro USUI3, James Dohm1, Ryodo HEMMI1, Takafumi NIIHARA1, Xu LUYUAN1, Shingo KAMEDA4, Takehiko SATOH5, Akihiko YAMAGISHI6 (1.University of Tokyo, 2.IRSPS, 3.TiTech, 4.ISAS/JAXA, 5.TUPLS, 6.Rikkyo University)
[PPS05-14]Meteorological Instruments of Mars EDL
*Naohito OTOBE1, George HASHIMOTO2, Hiroki SENSHU3, Makoto NAKAYOSHI4, Junichi KURIHARA5 (1.Fukuoka Univ, Faculty of Science, 2.Department of Earth Sciences, Okayama University, 3.Planetary Exploration Research Center, Chiba Institute of Technology, 4.Tokyo University of Science, Fuculty of science and technology, 5.Graduate School of Science, Hokkaido University)
[PPS05-15]Assessment of Mars surface environment for a exploration program: application of CReSS to Martian atmosphere
*Ko-ichiro SUGIYAMA1, Masatsugu ODAKA2, Kensuke NAKAJIMA3, Yoshiyuki O. TAKAHASHI4, Naohito OTOBE5, Seiya NISHIZAWA6, Yoshi-yuki HAYASHI4, George HASHIMOTO7, Kouichi HASEGAWA8, Atsusi SAKAKIBARA8, Kazuhisa TSUBOKI9 (1.ISAS/JAXA, 2.Hokkaido University, 3.Kyushu University, 4.Kobe University, 5.Fukuoka University, 6.RIKEN Advanced Institute for Computational Science, 7.Okayama University, 8.chuden CTI, 9.Nagoya University)
[PPS05-16]Scientific significance of sample return from Martian moons
*Shogo TACHIBANA1, Sei-ichiro WATANABE2, Yasuhito SEKINE3, Tomohiro USUI4 (1.Dept. Natural History Sciences, Hokkaido University, 2.Division of Earth and Planetary Sciences, Nagoya University, 3.Dept. Earth and Planetary Science, The University of Tokyo, 4.Dept. Earth and Planetary Sciences,Tokyo Institute of Technology)