Lunar Fe and Ti abundances: Comparison of lunar prospector and Clementine data

被引:78
作者
Elphic, RC
Lawrence, DJ
Feldman, WC
Barraclough, BL
Maurice, S
Binder, AB
Lucey, PG
机构
[1] Univ Calif Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[2] Observ Midi Pyrenees, F-31400 Toulouse, France
[3] Lunar Res Inst, Gilroy, CA 95020 USA
[4] Univ Hawaii, Hawaii Inst Geophys & Planetol, Honolulu, HI 96822 USA
关键词
D O I
10.1126/science.281.5382.1493
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The Lunar Prospector neutron spectrometer data correlate well with iron and titanium abundances obtained through analysis of Clementine spectral reflectance data. With the iron and titanium dependence removed, the neutron spectrometer data also reveal regions with enhanced amounts of gadolinium and samarium, incompatible rare earth elements that are enriched in the final phases of magma crystallization. These regions are found mainly around the ramparts of the Imbrium impact basin but not around the other basins, including the much larger and deeper South Pole-Aitken basin. This result confirms the compositional uniqueness of the surface and interior of the Imbrium region.
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页码:1493 / 1496
页数:4
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