WATER IN SNC METEORITES - EVIDENCE FOR A MARTIAN HYDROSPHERE

被引:145
作者
KARLSSON, KR
CLAYTON, RN
GIBSON, EK
MAYEDA, TK
机构
[1] NASA,LYNDON B JOHNSON SPACE CTR,PLANETARY SCI BRANCH,HOUSTON,TX 77058
[2] UNIV CHICAGO,DEPT GEOPHYS SCI,CHICAGO,IL 60637
[3] UNIV CHICAGO,ENRICO FERMI INST,DEPT CHEM,CHICAGO,IL 60637
关键词
D O I
10.1126/science.11537889
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 Shergotty-Nakhla-Chassigny (SNC) meteorites, purportedly of martian origin, contain 0.04 to 0.4 percent water by weight. Oxygen isotopic analysis can bc used to determine whether this water is extraterrestrial or terrestrial. Such analysis reveals that a portion of the water is extraterrestrial and furthermore was not in oxygen isotopic equilibrium with the host rock. Lack of equilibrium between water and host rock implies that the lithosphere and hydrosphere of the SNC parent body formed two distinct oxygen isotopic reservoirs. If Mars was the parent body, the maintenance of two distinct reservoirs may result from the absence of plate tectonics on the planet.
引用
收藏
页码:1409 / 1411
页数:3
相关论文
共 29 条