Refined thorium abundances for lunar red spots: Implications for evolved, nonmare volcanism on the Moon

被引:75
作者
Hagerty, J. J.
Lawrence, D. J.
Hawke, B. R.
Vaniman, D. T.
Elphic, R. C.
Feldman, W. C.
机构
[1] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[2] Univ Hawaii, Hawaii Inst Geophys & Planetol, Honolulu, HI 96822 USA
关键词
D O I
10.1029/2005JE002592
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
[1] We have used improved knowledge of the spatial distribution of thorium (Th) on the lunar surface, in conjunction with a forward modeling analysis of Lunar Prospector gamma ray data, to estimate the thorium abundances of lunar red spots. The results from this study can be combined with preexisting compositional and morphologic evidence to suggest that Hansteen Alpha, the Gruithuisen domes, and the Lassell massif are silicic, nonmare, volcanic constructs, similar in nature to terrestrial rhyolite domes. We propose that either silicate liquid immiscibility or, more likely, basaltic underplating could have produced lunar rhyolite domes. Thus the Lunar Prospector data presented in this study provide new information about the full range of volcanic and crustal processes that could have occurred on the Moon.
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页数:20
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