*Tariq Majeed1,2, Omar Al Aryani1, Shahd Al Mutawa1, Mohammed Al Qasimi1, Steve W Bougher2, Syed A Haider3 (1.American University of Sharjah, UAE, 2.University of Michigan, Ann Arbor, USA, 3.Physical Research Laboratory, Ahmedabad, India)
Session information
[EJ] Poster
P (Space and Planetary Sciences) » P-PS Planetary Sciences
[P-PS05] [EJ] Mars and Mars system: results from a broad spectrum of Mars studies and aspects for future missions
Sat. May 20, 2017 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall HALL7)
The study of Mars is rapidly adding new chapters with the US, European, Russian, AND Asian missions. A total of seven active missions (5 in orbit: Odyssey, MRO, MAVEN, Mars Express, and Mangalyaan, and 2 on the surface: MSL-Curiosity and MER-Opportunity) is the largest number ever at a given time at Mars, which demonstrates humanity's strong commitment to Mars exploration and its scientific significance. Synergetic investigations with on-going or already completed missions together with theoretical and numerical studies and earth-based remote sensing observations are gradually revealing the nature of Earth's most closely resembling but reddish planet. 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 (the surface, atmosphere, interior, surrounding plasma environment, Mars system including its two satellites, and the system's evolution history). Abstracts on instrumentation and future mission plans are also encouraged for this session, as both the presenters and the listeners would greatly benefit from discussions and feedbacks.
*Omar Al Aryani1, Tariq Majeed1, Shahd Al Mutawa1, Mohammed Al Qasimi1, Steve S Bougher2, Syed A Haider3 (1.American University of Sharjah, 2.University of Michigan, Ann Arbor, USA, 3.Physical Research Laboratory, Ahmedabad, India)
*Mohana manasa P1, Venkateswara Rao N2, Vijaya bhaskara Rao S1 (1.Department of Physics, Sri Venkateshwara University, Tirupati, india, 2.National Atmospheric Research Laboratory, Gadanki, India)
*Kazunori Ogohara1 (1.School of Engineering, University of Shiga Prefecture)
Nakamura Yusuke1, *Yoshiko Ogawa1, Hirohide Demura1 (1.University of Aizu)
Naoya Oya1, *Yoshiko Ogawa1, Hirohide Demura1 (1.University of Aizu)
*Ryodo Hemmi1, Hideaki Miyamoto1 (1.Department of Systems Innovation, School of Engineering, The University of Tokyo)
*Hideaki Miyamoto1, Ryodo Hemmi1, James Dohm1 (1.University of Tokyo)
*Haruhisa Tabata1, Yasuhito Sekine1, Yoshiki Kanzaki2, Seiji Sugita1, Takashi Murakami1 (1.Department of Earth and Planetary Science, The University of Tokyo, 2.Department of Geosciences, The Pennsylvania State University)
*Mai Motoyama1, Hideo Tsunakawa1 (1.Department of Earth and Planetary Sciences, Tokyo Institute of Technology)
*Tomohiro Suzuki2, Hidenori Genda1, Hiroyuki Kurokawa1, Arika Higuchi2, Shigeru Ida1 (1.Earth-Life Sicence Institute, Tokyo Institute of Technology, 2.Department of Earth and Planetary Sciences, Tokyo Institute of Technology)
*James Dohm1 (1.University Museum, University of Tokyo)
*Jianguo Yan1, Xuan Yang1, Mao Ye1, Shengkai Zhang1 (1.Wuhan University)
*Erhu WEI1 (1.School of Geodesy and Geomatics, Wuhan University)