Space and Planetary Sciences (P) | ||
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Session Sub-category | Planetary Sciences(PS) | |
Session ID | P-PS04 | |
Title | Mars and Mars system: results from a broad spectrum of Mars studies and aspects for future missions | |
Short Title | Mars and Mars system | |
Main Convener | Name | Hideaki Miyamoto |
Affiliation | University of Tokyo | |
Co-Convener 1 | Name | Tomohiro Usui |
Affiliation | Earth-Life Science Institute, Tokyo Institute of Technology | |
Co-Convener 2 | Name | Ayako Matsuoka |
Affiliation | Research Division for Space Plasma, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency | |
Co-Convener 3 | Name | Sushil K Atreya |
Affiliation | University of Michigan Ann Arbor | |
Session Language | E | |
Scope | 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. | |
Presentation Format | Oral and Poster presentation | |
Joint Session with | AGU | |
Invited Authors | Reid Parsons (University of Tokyo) Nicholas McCord Schneider (University of Colorado Boulder) |
Time | Presentation No | Title | Presenter | Abstract |
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Oral Presentation May 26 AM1 | ||||
09:00 - 09:15 | PPS04-01 | Recent results from the MAVEN mission | Dave A Brain | |
09:15 - 09:30 | PPS04-02 | From Clouds to Aurora to Atmospheric Escape: Highlights from MAVEN’s Imaging UltraViolet Spectrograph | Nicholas McCord Schneider | |
09:30 - 09:45 | PPS04-03 | Variation in Martian Crustal Magnetic Field Cusp Topology | Tristan David Weber | |
09:45 - 10:00 | PPS04-04 | The Induced Global Looping Magnetic Field on Mars | Lihui Chai | |
10:00 - 10:15 | PPS04-05 | First Observation of Magnetic Pulsations on Martian Surface | Peter J Chi | |
10:15 - 10:30 | PPS04-06 | Retrieval of vertical aerosol and gas profiles considering multiple scattering from Martian limb observations by MRO/CRISM | Yasumasa Kasaba | |
Oral Presentation May 26 AM2 | ||||
10:45 - 11:00 | PPS04-07 | MODELING MORE COMPLEX EARLY MARTIAN ATMOSPHERES AND DETERMINING THE RESULTING PRECIPITATION AND EROSION RATES | Ramses M Ramirez | |
11:00 - 11:15 | PPS04-08 | GCM simulations of the present and past water environment on Mars | Takeshi Kuroda | |
11:15 - 11:30 | PPS04-09 | Cold-based glaciation at Pavonis Mons, Mars: Evidence for moraine deposition during glacial advance | Reid Parsons | |
11:30 - 11:45 | PPS04-10 | Possible Earth-like tectonic scenario on Mars; a mineralogical and geochemical perspective | Trishit Ruj | |
11:45 - 12:00 | PPS04-11 | Hydration state of the Martian lithosphere constrained from gravity and topography | James Daniel Paul Moore | |
12:00 - 12:15 | PPS04-12 | SUBGLACIAL ANTARCTIC LAKE VOSTOK VS. SUBGLACIAL SOUTH POLE MARTIAN LAKE AND HYPERSALINE CANADIAN ARCTIC LAKES – PROSPECTS FOR LIFE | Sergey Bulat | |
Presentation No | Title | Presenter | Abstract |
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Poster Presentation May 26 PM2 | |||
PPS04-P01 | Observation of the O2+ first negative band (1,0) emissions in the Mars ionosphere with a visible spectrograph on Haleakala T60 | Toshihisa Suzuki | |
PPS04-P02 | Search of shallow subsurface reflectors around RSLs in Martian Chryse and Acidalia planitiae by the MRO/SHARAD public data | Aina Oura | |
PPS04-P03 | Detecting surface changes on Mars using principle component analysis of repeat imagery | Reid Parsons | |
PPS04-P04 | Evaluation of the detectability of hydrated salts on recurring slope lineae on Mars. | Shoko Imamura | |
PPS04-P05 | Frequency of ice sheet growth recorded on Mons Pavonis, Mars | Tomohiro Kanzaki | |
PPS04-P06 | Development of Life Detection Microscope (LDM) for in situ imaging of living cells on Mars surface | Yoshitaka Yoshimura | |
PPS04-P07 | Development of a Mars Web-GIS for viewing multiple kinds of spectral data from orbiters | Yuya Matsubara | |
PPS04-P08 | Visualization and Analysis of the Surface of Mars with NASA’s Mars Trek Portal | Brian Hamilton Day | |
PPS04-P09 | Increase in Dissolved Iron Concentration from Fayalite by UltravioletA・C Irradiation | Nobuo Komori | |
PPS04-P10 | Small-scale ridges newly identified on the equatorial region of the Phobos nearside | Ryodo Hemmi | |
PPS04-P11 | Development of a compact Muography instrument for future Mars exploration missions | Hiroaki Kamiyoshihara |