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dc.date.accessioned2021-04-30T19:50:29Z
dc.date.available2021-04-30T19:50:29Z
dc.date.created2021-03-24T14:40:09Z
dc.date.issued2020
dc.identifier.citationLoizeau, Damien Lequertier, Guillaume Poulet, Francois Hamm, Vincent Pilorget, Cédric Meslier-Lourit, Lionel Lantz, Cateline Werner, Stephanie C. Rull, Fernando Bibring, Jean-Pierre . Planetary Terrestrial Analogues Library project: 2. building a laboratory facility for MicrOmega characterization. Planetary and Space Science. 2020, 193
dc.identifier.urihttp://hdl.handle.net/10852/85803
dc.description.abstractMultiple spectroscopic techniques have been selected on previous, present and forthcoming missions to explore planetary surfaces in the Solar System. In particular, forthcoming ESA/Roscosmos and NASA missions to the surface of Mars will bring instruments capable of near-infrared (NIR), Raman and Laser Induced Breakdown Spectroscopies to analyze the mineralogy and chemistry of rocks. The PTAL (Planetary Terrestrial Analogues Library) project aims at building a multi-instrument spectral database of a large variety of natural Earth rock samples, including Mars analogues. The NIR hyperspectral microscope MicrOmega was selected to characterize the mineralogy of these analogues within the PTAL project. The instrument model used for the PTAL project is a spare flight model that requires specific care. For the safety of the instrument, and because of the large number of samples in the PTAL library and the requirement to optimize the observational conditions, a dedicated and semi-automated setup was built for the use of the MicrOmega instrument for this project. This paper presents the requirements specified for this setup, the technical solutions that have been selected, their implementation and the performances of the set-up. Sample preparation and operations during sample observations are explained, and a characterization example is presented to briefly illustrate the capabilities of MicrOmega in this set-up. The complete results from the MicrOmega characterizations of the PTAL rock analogues will be presented in a forthcoming paper (Loizeau et al. in prep).
dc.languageEN
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.titlePlanetary Terrestrial Analogues Library project: 2. building a laboratory facility for MicrOmega characterization
dc.typeJournal article
dc.creator.authorLoizeau, Damien
dc.creator.authorLequertier, Guillaume
dc.creator.authorPoulet, Francois
dc.creator.authorHamm, Vincent
dc.creator.authorPilorget, Cédric
dc.creator.authorMeslier-Lourit, Lionel
dc.creator.authorLantz, Cateline
dc.creator.authorWerner, Stephanie C.
dc.creator.authorRull, Fernando
dc.creator.authorBibring, Jean-Pierre
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1900703
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Planetary and Space Science&rft.volume=193&rft.spage=&rft.date=2020
dc.identifier.jtitlePlanetary and Space Science
dc.identifier.volume193
dc.identifier.pagecount9
dc.identifier.doihttps://doi.org/10.1016/j.pss.2020.105087
dc.identifier.urnURN:NBN:no-88458
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0032-0633
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/85803/2/1-s2.0-S0032063320303007-main.pdf
dc.type.versionPublishedVersion
cristin.articleid105087


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Attribution-NonCommercial-NoDerivatives 4.0 International
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