Japan Geoscience Union Meeting 2018

Presentation information

[EJ] Oral

P (Space and Planetary Sciences) » P-PS Planetary Sciences

[P-PS05] Lunar science and exploration

Wed. May 23, 2018 1:45 PM - 3:15 PM A01 (Tokyo Bay Makuhari Hall)

convener:Hiroshi Nagaoka(Waseda Univ.), Tomokatsu Morota(Graduate School of Environmental Studies, Nagoya University), Masaki N (名古屋大学宇宙地球環境研究所, 共同), Masahiro KAYAMA(Department of Earth and Planetary Material Sciences, Faculty of Science, Tohoku University), Chairperson:Nishino Masaki(名古屋大学宇宙地球環境研究所), Karouji Yuzuru

1:45 PM - 2:00 PM

[PPS05-13] Mission Objectives and Observational Requirements of the Planned Lunar Polar Mission

*Makiko Ohtake1, Takeshi Hoshino1, Yuzuru Karouji1, Hiroaki Shiraishi1, JAXA lunar polar mission study team1 (1.Japan Aerospace Exploration Agency)

Keywords:moon, polar mission, volatile

Currently, the International Space Exploration Coordination Group, organized by the space agencies of 15 countries and regions, is discussing future space exploration plans that will be based on international collaboration. A lunar polar mission has been studied by the Japan Aerospace Exploration Agency (JAXA) as a first step. Results derived by recent lunar exploration missions suggest that water ice might be present in the lunar polar region based on remote-sensing observations. In addition to the scientific interest about the origin and concentration mechanism of the water ice, there is strong interest in using water ice (if present) as an in-situ resource. Specifically, using water ice as a propellant will significantly affect future exploration scenarios and activities because the propellant generated from the water can be used in future lunar landing missions. However, it is currently unclear if water ice is really present in the polar region because of the limited available data. Therefore, mission objectives of the lunar polar mission are to obtain information about the quantity (how much), quality (is it pure water or does it contain other phases such as CO2 and CH4), and condensation/transportation mechanism of the water ice by carrying out in-situ measurements for assessing if we can use it as a resource in future space exploration activities. To obtain such information, we identified the following observation requirements.

-To measure water content directly with 0.1wt% accuracy.

-To identify chemical species (H2O, OH, H, CH4, etc.) and measure their abundance.

-To measure temperature at the lunar surface, underground (up to 1.5m), and the water ice itself.

-To measure the partial pressure of water during day and night time.

-To measure the chemical composition of mineral phases, modal abundance, and space weathering degree

In the presentation, we discuss recent remote-sensing results of possible water ice in the lunar polar region, mission objectives of the lunar polar mission, its mission requirements, and instrument candidates.