Karlsson H R, Clayton R N, Gibson E K, Mayeda T K
Planetary Science Branch, National Aeronautics and Space Administration, Johnson Space Center, Houston, TX 77058.
Science. 1992 Mar 13;255:1409-11. doi: 10.1126/science.11537889.
The Shergotty-Nakhla-Chassigny (SNC) meteorites, purportedly of martian origin, contain 0.04 to 0.4 percent water by weight. Oxygen isotopic analysis can be 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.
舍戈蒂-纳赫拉-沙西尼(SNC)陨石据称起源于火星,其重量含0.04%至0.4%的水。氧同位素分析可用于确定这种水是来自外星还是地球。这种分析表明,一部分水是外星的,而且与母岩不存在氧同位素平衡。水与母岩之间缺乏平衡意味着SNC母体的岩石圈和水圈形成了两个不同的氧同位素储库。如果火星是母体,两个不同储库的维持可能是由于该行星不存在板块构造。