Temporal and Spatial Variability of Lunar Hydration As Observed by the Deep Impact Spacecraft

被引:387
作者
Sunshine, Jessica M. [1 ]
Farnham, Tony L. [1 ]
Feaga, Lori M. [1 ]
Groussin, Olivier [2 ]
Merlin, Frederic [1 ]
Milliken, Ralph E. [3 ]
A'Hearn, Michael F. [1 ]
机构
[1] Univ Maryland, College Pk, MD 20742 USA
[2] Lab Astrophys Marseille, F-13388 Marseille, France
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
SPECTRAL PROPERTIES; WATER; MONTMORILLONITE; MIXTURES; MINERALS;
D O I
10.1126/science.1179788
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
070301 [无机化学]; 070403 [天体物理学]; 070507 [自然资源与国土空间规划学]; 090105 [作物生产系统与生态工程];
摘要
The Moon is generally anhydrous, yet the Deep Impact spacecraft found the entire surface to be hydrated during some portions of the day. Hydroxyl (OH) and water (H2O) absorptions in the near infrared were strongest near the North Pole and are consistent with <0.5 weight percent H2O. Hydration varied with temperature, rather than cumulative solar radiation, but no inherent absorptivity differences with composition were observed. However, comparisons between data collected 1 week (a quarter lunar day) apart show a dynamic process with diurnal changes in hydration that were greater for mare basalts (similar to 70%) than for highlands (similar to 50%). This hydration loss and return to a steady state occurred entirely between local morning and evening, requiring a ready daytime source of water-group ions, which is consistent with a solar wind origin.
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收藏
页码:565 / 568
页数:4
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