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Characterization and Calibration of the CheMin Mineralogical Instrument on Mars Science Laboratory

2012; Springer Science+Business Media; Volume: 170; Issue: 1-4 Linguagem: Inglês

10.1007/s11214-012-9905-1

1572-9672

D. F. Blake, D. T. Vaniman, C. N. Achilles, Robert C. Anderson, D. L. Bish, Tom Bristow, Curtis Chen, S. J. Chipera, J. A. Crisp, David L. Des Marais, Robert T. Downs, Jack D. Farmer, Sabrina Feldman, Mark Fonda, M. Gailhanou, Hongwei Ma, Doug Ming, R. V. Morris, P. Sarrazin, Ed Stolper, A. H. Treiman, A. S. Yen,

Space Exploration and Technology

A principal goal of the Mars Science Laboratory (MSL) rover Curiosity is to identify and characterize past habitable environments on Mars. Determination of the mineralogical and chemical composition of Martian rocks and soils constrains their formation and alteration pathways, providing information on climate and habitability through time. The CheMin X-ray diffraction (XRD) and X-ray fluorescence (XRF) instrument on MSL will return accurate mineralogical identifications and quantitative phase abundances for scooped soil samples and drilled rock powders collected at Gale Crater during Curiosity's 1-Mars-year nominal mission. The instrument has a Co X-ray source and a cooled charge-coupled device (CCD) detector arranged in transmission geometry with the sample. CheMin's angular range of 5∘ to 50∘ 2θ with 13 that are contained in the sample. The CheMin XRD is equipped with internal chemical and mineralogical standards and 27 reusable sample cells with either Mylar® or Kapton® windows to accommodate acidic-to-basic environmental conditions. The CheMin flight model (FM) instrument will be calibrated utilizing analyses of common samples against a demonstration-model (DM) instrument and CheMin-like laboratory instruments. The samples include phyllosilicate and sulfate minerals that are expected at Gale crater on the basis of remote sensing observations.