The role of H2O in Martian magmatic systems

被引：0
|
作者：
Mysen, BO
Virgo, D
Popp, RK
Bertka, CM
机构：
[1] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA
[2] Texas A&M Univ, Dept Geol & Geophys, College Stn, TX 77843 USA
来源：
AMERICAN MINERALOGIST | 1998年 / 83卷 / 9-10期
关键词：
D O I：
暂无
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 have estimated the water content of Mars' interior by using analyzed water contents of kaersutite inclusions from shergottites nakhlites chassignites (SNC) meteorites in conjunction with an experimentally-derived crystal-chemical model of kaersutite amphibole. This model predicts quantitatively the relationships between iron oxidation and hydrogen deficiency in the kaersutite. The H2O content of the magma from which the kaersutites in SNC meteorites could have crystallized is in the 100-1000 ppm range. That H2O content leads to an estimated water content of 1-35 ppm for a Martian mantle that could have been the source rock for such magmas.
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收藏
页码：942 / 946
页数：5
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