10:45 AM - 11:00 AM
*Ramses M Ramirez1,2 (1.Earth-life Science Institute, 2.Tokyo Institute of Technology)
[E] Oral
P (Space and Planetary Sciences ) » P-PS Planetary Sciences
Sun. May 26, 2019 10:45 AM - 12:15 PM A02 (TOKYO BAY MAKUHARI HALL)
convener:Hideaki Miyamoto(University of Tokyo), Tomohiro Usui(Earth-Life Science Institute, Tokyo Institute of Technology), Ayako Matsuoka(Research Division for Space Plasma, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Sushil K Atreya(University of Michigan Ann Arbor), Chairperson:Hideaki Miyamoto, Tomohiro Usui
In view of unprecedented advances in our understanding of Mars, primarily due to new and ongoing observations of the planet with a number of spacecraft missions of the US, Europe and Asia, we propose a session on Mars. Mars is an object of intense scrutiny. Currently, eight spacecraft are operating at Mars, with six in orbit (Odyssey, MRO, MAVEN, Mars Express, Mangalyaan and TGO) and two on the surface (MSL-Curiosity and MER-Opportunity), the largest number ever at any given time. In addition, InSight is on track to land on Mars in November 2018, and several spacecraft are in various stages of implementation with launches scheduled for 2020 (Mars 2020, ExoMars 2020, Emirates Mars Mission Hope, Chinese Mars Mission and the Japanese Mars Terahertz Microsatellite), 2022 (ISRO's Mangalyaan 2), and 2024 (JAXA's MMX mission to explore Phobos, Deimos, and Mars). All this is a clear demonstration of public's strong fascination with and commitment to Mars exploration and the resulting scientific bonanza. Synergistic investigations with ongoing and already completed missions along with modeling studies and earth-based observations are gradually revealing the nature of Earth's most closely resembling planet that took on a different evolutionary track than our home planet. Morphology and variable phenomena seen on the surface (RSLs, e.g.) and in the atmosphere (methane) indicate that Mars is possibly currently active. Available data are providing a better understanding of Mars' present geologic and atmospheric state, climate evolution, and habitability. Thus, the scope of this session will be the recent results from a broad spectrum of Mars studies encompassing the interior, surface, atmosphere, plasma environment, and the Mars system including its two satellites. Abstracts on modelling, instrumentation and future mission plans are also encouraged.
10:45 AM - 11:00 AM
*Ramses M Ramirez1,2 (1.Earth-life Science Institute, 2.Tokyo Institute of Technology)
11:00 AM - 11:15 AM
*Takeshi Kuroda1,2, Arihiro Kamada1, Katsushige Toriumi1, Yasumasa Kasaba1, Naoki Terada1, Hiromu Nakagawa1 (1.Faculty of Science, Tohoku University, 2.National Institute of Information and Communications Technology)
11:15 AM - 11:30 AM
*Reid Parsons1,2, Tomohiro Kanzaki3, Ryodo Hemmi1, Hideaki Miyamoto3 (1.University Museum, University of Tokyo, 2.Earth and Geographic Science Dept., Fitchburg State University, 3.Dept. of Systems Innovation, University of Tokyo)
11:30 AM - 11:45 AM
*Trishit Ruj1, Gene W Schimdt2, Goro Komatsu2, Kenji Kawai1 (1.Department of Earth and Planetary Science, School of Science, UTokyo, Japan, 2.International Research School of Planetary Sciences, Università d'Annunzio, Italy)
11:45 AM - 12:00 PM
*James Daniel Paul Moore1, Jon Wade2, Anthony B Watts2, Richard M Palin3, Lars M Hansen2, Brendan Dyck4, Jun Muto6, Andrew J Smye5, Adam D Switzer1 (1.Earth Observatory of Singapore, 2.University of Oxford, 3.Colorado School of Mines, 4.Simon Fraser University, 5.Penn State, 6.Tohoku University)
12:00 PM - 12:15 PM
*Sergey Bulat1 (1.NRC KI - Petersburg Nuclear Physics Institute, Saint-Petersburg-Gatchina, Russia)
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