FeO and TiO2 concentrations in the South Pole Aitken basin:: Implications for mantle composition and basin formation

被引:130
作者
Lucey, PG
Taylor, GJ
Hawke, BR
Spudis, PD
机构
[1] Univ Hawaii, Hawaii Inst Geophys & Planetol, Honolulu, HI 96822 USA
[2] Lunar & Planetary Inst, Houston, TX 77058 USA
关键词
D O I
10.1029/97JE03146
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
We use newly developed spectroscopic methods for determining FeO and TiO2 abundances to study the huge (2500 km diameter) South Pole-Aitken basin. The floor of this basin shows iron and titanium values which are weakly correlated and largely range from 7 to 14 wt % FeO and from 0.5 to 1.5 wt % TiO2. This composition is consistent with an approximate 1:1 mixture of lower crustal material like that found elsewhere on the Moon and mantle rock containing 10-16 wt % FeO and < 0.1 wt % TiO2. Although mantle rock appears to compose about 50% of the floor deposits, models of the formation of large impact basins predict that virtually all the floor materials ought to be derived from the mantle.
引用
收藏
页码:3701 / 3708
页数:8
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