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Volumn 306, Issue 5702, 2004, Pages 1746-1749

Chemistry of rocks and soils at Meridiani Planum from the Alpha Particle X-ray Spectrometer

Author keywords

[No Author keywords available]

Indexed keywords

ALPHA PARTICLE SPECTROMETERS; BASALT; BROMINE; CHLORINE; COMPOSITION; SOILS; SULFUR; WATER; X RAY SPECTROMETERS;

EID: 10044298294     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1104358     Document Type: Article
Times cited : (342)

References (22)
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    • Names have been assigned to aerographic features by the Mars Exploration Rover (MER)team for planning and operations purposes. The names are not formally recognized by the International Astronomical Union.
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    • note
    • The term martian soil is used here to denote any loose unconsolidated materials that can be distinguished from rocks, bedrock, or strongly cohesive sediments. No implication of the presence or absence of organic materials or living matter is intended.
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    • note
    • A martian solar day has a mean period of 24 hours 39 min 35.244 s and is referred to as a sol to distinguish this from a roughly 3% shorter solar day on Earth.
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    • abstr. 1965 Lunar and Planetary Institute, Houston, TX, CD-ROM
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    • note
    • Shergottites are a family of meteorites that are believed to originate from Mars.
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    • H. H. Kieffer, B. M. Jakosky, C. W. Snyder, M. S. Matthews, Eds. Univ. Arizona Press, Tucson, AZ
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    • note
    • 3 and Fe as FeO. Also, all concentration values are based on an assumed homogeneous matrix (4).
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    • note
    • The APXS was mainly funded by the Max-Planck-Society and, in part, by the German Space Agency (DLR) (grant no. 50QM0014). G.K. and R.G. also acknowledge DLR grant 50QM0005. Funding for Athena science team members was provided by NASA contracts through Cornell and JPL.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.