Please use this identifier to cite or link to this item: http://hdl.handle.net/1893/17071
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dc.contributor.authorKlingelhoefer, Goestaren_UK
dc.contributor.authorMorris, Richard Vanen_UK
dc.contributor.authorBernhardt, Bodoen_UK
dc.contributor.authorRodionov, Daniel Sen_UK
dc.contributor.authorde Souza Jr, Paulo Aen_UK
dc.contributor.authorSquyres, Steven Wen_UK
dc.contributor.authorFoh, Jen_UK
dc.contributor.authorKankeleit, Egberten_UK
dc.contributor.authorBonnes, Uen_UK
dc.contributor.authorGellert, Ralfen_UK
dc.contributor.authorSchröder, Christianen_UK
dc.contributor.authorLinkin, Sen_UK
dc.contributor.authorEvlanov, E Nen_UK
dc.contributor.authorZubkov, B Ven_UK
dc.contributor.authorPrilutski, O Fen_UK
dc.date.accessioned2016-09-29T00:36:20Z-
dc.date.available2016-09-29T00:36:20Z-
dc.date.issued2003-12-19en_UK
dc.identifier.other8067en_UK
dc.identifier.urihttp://hdl.handle.net/1893/17071-
dc.description.abstractMössbauer 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.en_UK
dc.language.isoenen_UK
dc.publisherWiley-Blackwell for the American Geophysical Unionen_UK
dc.relationKlingelhoefer 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. https://doi.org/10.1029/2003JE002138en_UK
dc.rightsCopyright 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.en_UK
dc.subjectMossbauer spectroscopyen_UK
dc.subjectiron mineralogyen_UK
dc.subjectMarsen_UK
dc.subjectweatheringen_UK
dc.subjectinstrumentationen_UK
dc.subjectMIMOS IIen_UK
dc.titleAthena MIMOS II Mossbauer spectrometer investigationen_UK
dc.typeJournal Articleen_UK
dc.identifier.doi10.1029/2003JE002138en_UK
dc.citation.jtitleJournal of Geophysical Research: Planetsen_UK
dc.citation.issn2169-9100en_UK
dc.citation.issn2169-9097en_UK
dc.citation.volume108en_UK
dc.citation.issueE12en_UK
dc.citation.publicationstatusPublisheden_UK
dc.citation.peerreviewedRefereeden_UK
dc.type.statusVoR - Version of Recorden_UK
dc.author.emailchristian.schroeder@stir.ac.uken_UK
dc.contributor.affiliationJohannes Gutenberg University of Mainzen_UK
dc.contributor.affiliationNational Aeronautics and Space Administration (NASA)en_UK
dc.contributor.affiliationJohannes Gutenberg University of Mainzen_UK
dc.contributor.affiliationJohannes Gutenberg University of Mainzen_UK
dc.contributor.affiliationUniversity of Tasmaniaen_UK
dc.contributor.affiliationCornell Universityen_UK
dc.contributor.affiliationJohannes Gutenberg University of Mainzen_UK
dc.contributor.affiliationDarmstadt University of Technology, Germanyen_UK
dc.contributor.affiliationDarmstadt University of Technology, Germanyen_UK
dc.contributor.affiliationUniversity of Guelphen_UK
dc.contributor.affiliationBiological and Environmental Sciencesen_UK
dc.contributor.affiliationSpace Research Institute IKI, Russiaen_UK
dc.contributor.affiliationSpace Research Institute IKI, Russiaen_UK
dc.contributor.affiliationSpace Research Institute IKI, Russiaen_UK
dc.contributor.affiliationSpace Research Institute IKI, Russiaen_UK
dc.identifier.isiWOS:000187859300001en_UK
dc.identifier.wtid683648en_UK
dc.contributor.orcid0000-0002-7935-6039en_UK
dcterms.dateAccepted2003-12-19en_UK
dc.date.filedepositdate2013-10-23en_UK
rioxxterms.typeJournal Article/Reviewen_UK
rioxxterms.versionVoRen_UK
local.rioxx.authorKlingelhoefer, Goestar|en_UK
local.rioxx.authorMorris, Richard Van|en_UK
local.rioxx.authorBernhardt, Bodo|en_UK
local.rioxx.authorRodionov, Daniel S|en_UK
local.rioxx.authorde Souza Jr, Paulo A|en_UK
local.rioxx.authorSquyres, Steven W|en_UK
local.rioxx.authorFoh, J|en_UK
local.rioxx.authorKankeleit, Egbert|en_UK
local.rioxx.authorBonnes, U|en_UK
local.rioxx.authorGellert, Ralf|en_UK
local.rioxx.authorSchröder, Christian|0000-0002-7935-6039en_UK
local.rioxx.authorLinkin, S|en_UK
local.rioxx.authorEvlanov, E N|en_UK
local.rioxx.authorZubkov, B V|en_UK
local.rioxx.authorPrilutski, O F|en_UK
local.rioxx.projectInternal Project|University of Stirling|https://isni.org/isni/0000000122484331en_UK
local.rioxx.freetoreaddate2013-10-23en_UK
local.rioxx.licencehttp://www.rioxx.net/licenses/all-rights-reserved|2013-10-23|en_UK
local.rioxx.filename2003JE002138.pdfen_UK
local.rioxx.filecount1en_UK
local.rioxx.source2169-9097en_UK
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