Japan Geoscience Union Meeting 2014

Presentation information

Oral

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

[P-PS23_2AM2] Lunar science and exploration

Fri. May 2, 2014 11:00 AM - 12:45 PM 413 (4F)

Convener:*Tomokatsu Morota(Graduate School of Environmental Studies, Nagoya University), Chikatoshi Honda(The University of Aizu), Masaki N Nishino(Solar-Terrestrial Environment Laboratory, Nagoya University), Hiroshi Nagaoka(Waseda Univ.), Chair:Hiroshi Nagaoka(Waseda Univ.), Kisara Uemoto(Department of Earth and planetary Science Guraduate School of Science,The University of Tokyo)

11:15 AM - 11:30 AM

[PPS23-09] Rock and mineral distribution of the lunar South Pole-Aitken basin

*Kisara UEMOTO1, Makiko OHTAKE2, Junichi HARUYAMA2, Satoru YAMAMOTO3, Ryosuke NAKAMURA4, Tsuneo MATSUNAGA3, Takahiro IWATA2 (1.The University of Tokyo, 2.Japan Aerospace Exploration Agency, 3.National Institute for Environmental Studies, 4.National Institute of Advanced Industrial Science and Technology)

Keywords:South Pole-Aitken, lunar, rock, mineral

South Pole-Aitken (SPA) basin is one of the largest basin (2500 km in diameter [1] ) on the lunar farside. In pre-vious studies, it has been suggested that most of the crustal material was excavated and that the mantle materials have been exposed [e.g., 1]. Particularly, because this excavation was the biggest at the central area of the basin, mantle materials exposed. Mantle material of this area is melted by the basin impact and produced impact melt [e.g., 2], therefore we suggest that investigation within this impact melt area lead up to understand mantle material conpo-sition. However, because SPA is very old and large, we cannot identify the impact melt area. In our study, we pro-duce a new mineralogical map of SPA basin interior, based on data derived from SELENE Multiband Imager (MI). In particular, we investigated mineralogy within the central depression of SPA by iron and titanium concentration and altitude data derived from SELENE. Using these method, we identified the impact melt area of SPA.We prodused a mineralogical map within the central depression of SPA. As a result, we classified into three mineral type layers on this map ; low-Ca pyroxene layer, high-Ca pyroxene layer and very high-Ca pyroxene layer. From correlations of these layers and occurrences, we created the column diagrams of respective areas. Then, we suggested origins of these mineral type layers : The high-Ca pyroxene layer is impact melt area of the basin. The low-Ca pyroxene layer and the very high-Ca pyroxene layer is the ejecta of SPA basin and mare erupted after SPA basin formation, respectively. In fact, the area of the high-Ca pyroxene layer is impact melt area of SPA. In the fu-ture work, we will analyze mineral and chemical compositions within this area.References: [1] Spudis et al., 1994. [2] Pieters et al., 2000