Development of the Mars microbeam Raman spectrometer (MMRS)

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Read Full Article (file size: 633127 bytes) Cited by JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 108, NO. E1, 5005, doi:10.1029/2002JE001902, 2003 Development of the Mars microbeam Raman spectrometer (MMRS) Alian Wang Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri, USA Larry A. Haskin Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri, USA Arthur L. Lane Earth and Space Sciences Division, Jet Propulsion Laboratory, Pasadena, California, USA Thomas J. Wdowiak Department of Physics, University of Alabama at Birmingham, Birmingham, Alabama, USA Steven W. Squyres Center for Radiophysics and Space Physics, Cornell University, Ithaca, New York, USA Robert J. Wilson Observational Systems Division, Jet Propulsion Laboratory, Pasadena, California, USA Larry E. Hovland Observational Systems Division, Jet Propulsion Laboratory, Pasadena, California, USA Ken S. Manatt Earth and Space Sciences Division, Jet Propulsion Laboratory, Pasadena, California, USA Nasrat Raouf Observational Systems Division, Jet Propulsion Laboratory, Pasadena, California, USA Christopher D. Smith Engineering Services, Swales Aerospace Corp., Pasadena, California, USA Abstract Raman spectroscopy is a powerful tool for mineral characterization and for detection of water and organic and inorganic forms of carbon. The Mars microbeam Raman spectrometer (MMRS) is designed for close-up analysis of rocks and soils in planetary surface exploration. The MMRS consists of a probe (in a flight unit to be deployed by a robotic arm) and a spectrograph, laser source, and electronics (in a flight unit to reside on a rover or lander). The Raman probe has a scanning optical bench that enables a 1-cm linear traverse across a target rock or soil, both on target materials as encountered and on fresh surfaces of rocks exposed by abrasion or coring. From these spectra, one can identify major, minor, and trace minerals, obtain their approximate relative proportions, and determine chemical features (e.g., Mg/Fe ratio) and rock textural features (e.g., mineral clusters, amygdular fill, and veins). One can also detect and identify organic species, graphitic carbon, and water-bearing phases. Extensive performance tests have been done on a brassboard model of the MMRS using a variety of geological materials (minerals, rocks, Martian meteorites, etc.). These tests show that a Raman spectrometer can be built that is suitably miniaturized, sufficiently robust, and low enough in power usage to serve as an on-surface planetary instrument, yet the spectrometer can retain high detection sensitivity and yield near laboratory quality spectra over a broad wavelength range. These features are essential to provide definitive mineralogy in a planetary exploration. Published 30 January 2003. Index Terms: 3672 Mineralogy and Petrology: Planetary mineralogy and petrology (5410); 3694 Mineralogy and Petrology: Instruments and techniques; 3994 Mineral Physics: Instruments and techniques; 5494 Planetology: Solid Surface Planets: Instruments and techniques. Read Full Article (file size: 633127 bytes) Cited by Citation: Wang, A., L. A. Haskin, A. L. Lane, T. J. Wdowiak, S. W. Squyres, R. J. Wilson, L. E. Hovland, K. S. Manatt, N. Raouf, and C. D. Smith (2003), Development of the Mars microbeam Raman spectrometer (MMRS), J. Geophys. Res., 108(E1), 5005, doi:10.1029/2002JE001902. Copyright 2003 by the American Geophysical Union.

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