A different perspective for the Mars rover “Opportunity” site: Fine-grained, consolidated hematite and hematite coatings
GEOPHYSICAL RESEARCH LETTERS(2004)
摘要
Since 2001, there have been two, parallel interpretations of Mars Global Surveyor Thermal Emission Spectrometer (TES) observations of Sinus Meridiani, which are: (1) coarse-grained ("gray") hematite is the only spectral match; and (2) fine-grained hematite with particles closer than similar towavelength ("fine-intimate hematite", e. g., coating, ferricrete) is a better match, but coarse hematite is also viable. The TES team interpreted the spectra as consistent only with a large deposit (similar to750 km x 350 km) of coarse hematite (>5-10 mm grain size). Coarse hematite is considered strong evidence for longstanding water, which led to the decision to land the rover Opportunity there. On the other hand, the Aerospace/LPI remote sensing team argued that fine-intimate hematite can better match TES spectra. A thin coating (similar to5-10 mm thick) and a low exposure (<5%) could cause the observed signatures. The distinction is important because: (1) It is unknown whether fine-grained hematite implies abundant water; (2) Fine-intimate hematite may explain the non-detection of coexisting aqueous alteration minerals and the lack of hematite wind streaks; (3) Current "hematite abundance maps" may instead map the surface texture; (4) Coatings may be of astrobiology interest; (5) Studies are needed to determine whether visible-infrared spectra can definitively distinguish fine-intimate from coarse hematite.
更多查看译文
关键词
thermal emission spectrometer,surface texture,grain size,infrared spectra,remote sensing,solar system
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要