Session Details
[P-PS07]Mars and Mars system: results from a broad spectrum of Mars studies and aspects for future missions
Sun. May 20, 2018 9:00 AM - 10:30 AM JST
Sun. May 20, 2018 12:00 AM - 1:30 AM UTC
Sun. May 20, 2018 12:00 AM - 1:30 AM UTC
201A 2F International Conference Hall, Makuhari Messe
convener:Hideaki Miyamoto(University of Tokyo), Tomohiro Usui(Earth-Life Science Institute, Tokyo Institute of Technology), Ayako Matsuoka(宇宙航空研究開発機構 宇宙科学研究所 太陽系科学研究系, 共同), Sushil K Atreya (University of Michigan Ann Arbor), Chairperson:Matsuoka Ayako, Atreya Sushil
Unprecedented progress in being made in our understanding of the planet Mars, especially because of new data from the US, European, Russian, and Asian missions to Mars. Eight spacecraft are currently 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 Lander is on track for launch in 2018, and Mars 2020, ExoMars and the Emirates Mars Mission in 2020. 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 or 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. Morphology and variable phenomena seen on the surface (RSLs, for example) indicate the red planet may possibly be still active, and require a clear understanding of its current geologic and atmospheric state, climate evolution and habitability. Thus, this session is planned to discuss 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 instrumentation and future mission plans are also encouraged for this session, as both the presenters and the audience would greatly benefit from ensuing discussions and feedbacks.
[PPS07-01]A coupled atmosphere–hydrosphere global climate model of early Mars: “cool and wet” scenario for the formation of water channels★Invited Papers
Arihiro Kamada1, *Takeshi Kuroda2,1, Yasumasa Kasaba1, Naoki Terada1, Hiromu Nakagawa1, Katsushige Toriumi1 (1.Dep. Geophysics, Graduate School of Science, Tohoku University, 2.National Institute of Information and Communication Technology)
[PPS07-02]The effect of radiative cooling on the hydrodynamic escape of a Martian proto-atmosphere
*Yoshida Tatsuya1, Kiyoshi Kuramoto1 (1.Hokkaido University)
[PPS07-03]Wavenumber-frequency spectra in the Mars atmosphere: the 2 sols waves in low latitudes
*Kazunori Ogohara1 (1.School of Engineering, University of Shiga Prefecture)
[PPS07-04]Observation of secondary ions emitted from Phobos by the mass spectrum analyzer on Martian Moons eXploration (MMX)
*Shoichiro Yokota1, Ayako Matsuoka2, Naoki Terada3, Reiko Nomura4, Yoshifumi Saito2, Daiba Kato5 (1.Graduate School of Science, Osaka University, 2.JAXA/ISAS, 3.Graduate School of Science, Tohoku University, 4.JAXA, 5.Graduate School of Science, The University of Tokyo)
[PPS07-05]Capture of satellite precursors and their orbital evolution by a rotating Martian proto-atmosphere
*Ryo Matsuoka1, Kiyoshi Kuramoto1 (1.Department of Cosmosciences, Graduateschool of Science, Hokkaido University)
[PPS07-06]High-resolution digital elevation models of Phobos derived from HiRISE stereo images
*Ryodo Hemmi1, Hideaki Miyamoto1 (1.The University of Tokyo)
