The South Pole-Aitken basin region, Moon: GIS-based geologic investigation using Kaguya elemental information

被引:4
|
作者
Kim, Kyeong Ja [1 ]
Dohm, James M. [2 ]
Williams, Jean-Pierre [3 ]
Ruiz, Javier [4 ]
Hare, Trent M. [5 ]
Hasebe, Nobuyuki [6 ]
Karouji, Yuzuru [7 ]
Kobayashi, Shingo [8 ]
Hareyama, Makoto [7 ]
Shibamura, Eido [9 ]
Kobayashi, Masanori [10 ]
d'Uston, Claude [11 ]
Gasnault, Olivier [11 ]
Forni, Olivier [11 ]
Maurice, Sylvestre [11 ]
机构
[1] Korean Inst Geosci & Mineral Resources, Div Geol Res, Taejon 305350, South Korea
[2] Univ Arizona, Dept Hydrol & Water Resources, Tucson, AZ 85721 USA
[3] Univ Calif Los Angeles, Dept Earth & Space Sci, Los Angeles, CA 90095 USA
[4] Univ Complutense Madrid, Fac Ciencias Geol, Dept Geodinam, E-28040 Madrid, Spain
[5] US Geol Survey, Flagstaff, AZ 86001 USA
[6] Waseda Univ, Res Inst Sci & Engn, Shinjuku Ku, Tokyo 1698555, Japan
[7] Japan Aerosp Explorat Agcy, Sagamihara, Kanagawa 2298510, Japan
[8] Natl Inst Radiol Sci, Inage Ku, Chiba 2638555, Japan
[9] Saitama Prefectural Univ, Saitama 3438540, Japan
[10] Chiba Inst Technol, Narashino, Chiba 2750016, Japan
[11] Univ Toulouse, UPS OMP, CNRS, IRAP, F-31028 Toulouse 4, France
关键词
Kaguya (SELENE); Gamma-Ray Spectrometer; South Pole-Aitken basin; Elemental maps; Impact; LUNAR; SURFACE; TIO2; FEO;
D O I
10.1016/j.asr.2012.06.019
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Using Geographic Information Systems (GIS), we performed comparative analysis among stratigraphic information and the Kaguya (SELENE) GRS data of the similar to 2500-km-diameter South Pole-Aitken (SPA) basin and its surroundings. Results indicate that the surface rock materials (including ancient crater materials, mare basalts, and possible SPA impact melt) are average to slightly elevated in K and Th with respect to the rest of the Moon. Also, this study demonstrates that K and Th have not significantly changed since the formation of SPA. The elemental signatures of the impact basin of Fe, Ti, Si, o through time include evidence for resurfacing by ejecta materials and late-stage volcanism. The oldest surfaces of SPA are found to be oxygen-depleted during the heavy bombardment period relative to later stages of geologic development, followed by both an increase in silicon and oxygen, possibly due to ejecta sourced from outside of SPA, and subsequent modification due to mare basaltic volcanism, which increased iron and titanium within SPA. The influence of the distinct geologic history of SPA and surroundings on the mineralogic and elemental abundances is evident as shown in our investigation. (c) 2012 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1629 / 1637
页数:9
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