Please use this identifier to cite or link to this item: http://hdl.handle.net/1893/17071
Appears in Collections:Biological and Environmental Sciences Journal Articles
Peer Review Status: Refereed
Title: Athena MIMOS II Mossbauer spectrometer investigation
Authors: Klingelhoefer, Goestar
Morris, Richard Van
Bernhardt, Bodo
Rodionov, Daniel S
de, Souza Jr Paulo A
Squyres, Steven W
Foh, J
Kankeleit, Egbert
Bonnes, U
Gellert, Ralf
Schröder, Christian
Linkin, S
Evlanov, E N
Zubkov, B V
Prilutski, O F
Contact Email: christian.schroeder@stir.ac.uk
Keywords: Mossbauer spectroscopy
iron mineralogy
Mars
weathering
instrumentation
MIMOS II
Issue Date: 19-Dec-2003
Publisher: Wiley-Blackwell for the American Geophysical Union
Citation: Klingelhoefer G, Morris RV, Bernhardt B, Rodionov DS, de Souza Jr PA, Squyres SW, Foh J, Kankeleit E, Bonnes U, Gellert R, Schröder C, Linkin S, Evlanov EN, Zubkov BV & Prilutski OF (2003) Athena MIMOS II Mossbauer spectrometer investigation, Journal of Geophysical Research: Planets, 108 (E12), Art. No.: 8067.
Abstract: Mössbauer spectroscopy is a powerful tool for quantitative mineralogical analysis of Fe-bearing materials. The miniature Mössbauer spectrometer MIMOS II is a component of the Athena science payload launched to Mars in 2003 on both Mars Exploration Rover missions. The instrument has two major components: (1) a rover-based electronics board that contains power supplies, a dedicated central processing unit, memory, and associated support electronics and (2) a sensor head that is mounted at the end of the instrument deployment device (IDD) for placement of the instrument in physical contact with soil and rock. The velocity transducer operates at a nominal frequency of 25 Hz and is equipped with two 57Co/Rh Mössbauer sources. The reference source (5 mCi landed intensity), reference target (alpha-Fe2O3 plus alpha-Fe0), and PIN-diode detector are configured in transmission geometry and are internal to the instrument and used for its calibration. The analysis Mössbauer source (150 mCi landed intensity) irradiates Martian surface materials with a beam diameter of 1.4 cm. The backscatter radiation is measured by four PIN-diode detectors. Physical contact with surface materials is sensed with a switch-activated contact plate. The contact plate and reference target are instrumented with temperature sensors. Assuming 18% Fe for Martian surface materials, experiment time is 6–12 hours during the night for quality spectra (i.e., good counting statistics); 1–2 hours is sufficient to identify and quantify the most abundant Fe-bearing phases. Data stored internal to the instrument for selectable return to Earth include Mössbauer and pulse-height analysis spectra (512 and 256 channels, respectively) for each of the five detectors in up to 13 temperature intervals (65 Mössbauer spectra), engineering data for the velocity transducer, and temperature measurements. The total data volume is 150 kB. The mass and power consumption are 500 g (400 g for the sensor head) and 2 W, respectively. The scientific measurement objectives of the Mössbauer investigation are to obtain for rock, soil, and dust (1) the mineralogical identification of iron-bearing phases (e.g., oxides, silicates, sulfides, sulfates, and carbonates), (2) the quantitative measurement of the distribution of iron among these iron-bearing phases (e.g., the relative proportions of iron in olivine, pyroxenes, ilmenite, and magnetite in a basalt), (3) the quantitative measurement of the distribution of iron among its oxidation states (e.g., Fe2+, Fe3+, and Fe6+), and (4) the characterization of the size distribution of magnetic particles. Special geologic targets of the Mössbauer investigation are dust collected by the Athena magnets and interior rock and soil surfaces exposed by the Athena Rock Abrasion Tool and by trenching with rover wheels.
Type: Journal Article
URI: http://hdl.handle.net/1893/17071
DOI Link: http://dx.doi.org/10.1029/2003JE002138
Rights: Copyright 2003 by the American Geophysical Union. AGU allows authors to deposit their journal articles if the version is the final published citable version of record, the AGU copyright statement is clearly visible on the posting, and the posting is made 6 months after official publication by the AGU.
Affiliation: Johannes Gutenberg University of Mainz
National Aeronautics and Space Administration (NASA)
Johannes Gutenberg University of Mainz
Johannes Gutenberg University of Mainz
University of Tasmania
Cornell University
Johannes Gutenberg University of Mainz
Darmstadt University of Technology, Germany
Darmstadt University of Technology, Germany
University of Guelph
Biological and Environmental Sciences
Space Research Institute IKI, Russia
Space Research Institute IKI, Russia
Space Research Institute IKI, Russia
Space Research Institute IKI, Russia

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