Results from the Mars global surveyor thermal emission spectrometer

被引:161
|
作者
Christensen, PR [1 ]
Anderson, DL
Chase, SC
Clancy, RT
Clark, RN
Conrath, BJ
Kieffer, HH
Kuzmin, RO
Malin, MC
Pearl, JC
Roush, TL
机构
[1] Arizona State Univ, Tempe, AZ 85287 USA
[2] Univ Colorado, Goleta, CA 93017 USA
[3] US Geol Survey, Denver, CO 80225 USA
[4] Cornell Univ, Ithaca, NY 14850 USA
[5] US Geol Survey, Flagstaff, AZ 86001 USA
[6] VI Vernadskii Inst Geochem & Analyt Chem, Moscow 117975, Russia
[7] Malin Space Sci Syst, San Diego, CA USA
[8] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[9] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[10] Santa Barbara Remote Sensing, Goleta, CA 93017 USA
关键词
D O I
10.1126/science.279.5357.1692
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 Thermal Emission Spectrometer spectra of low albedo surface materials suggests that a four to one mixture of pyroxene to plagioclase, together with about a 35 percent dust component provides the best fit to the spectrum. Qualitative upper limits can be placed on the concentration of carbonates (<10 percent), olivine (<10 percent), clay minerals (<20 percent), and quartz (<5 percent) in the limited regions observed. Limb observations in the northern hemisphere reveal low-lying dust hazes and detached water-ice clouds at altitudes up to 55 kilometers. At an aerocentric longitude of 224 degrees a major dust storm developed in the Noachis Terra region, The south polar cap retreat was similar to that observed by Viking.
引用
收藏
页码:1692 / 1698
页数:7
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