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dc.date.accessioned2021-03-13T21:10:23Z
dc.date.available2021-03-13T21:10:23Z
dc.date.created2021-02-03T17:04:42Z
dc.date.issued2020
dc.identifier.citationLantz, Cateline Poulet, Francois Loizeau, Damien Riu, Lucie Pilorget, C. Carter, John Dypvik, Henning Rull, Fernando Werner, Stephanie C. . Planetary Terrestrial Analogues Library project: 1. characterization of samples by near-infrared point spectrometer. Planetary and Space Science. 2020, 189
dc.identifier.urihttp://hdl.handle.net/10852/83999
dc.description.abstractThe PTAL project aims at building and exploiting a database involving several analytical techniques, the Planetary Terrestrial Analogues Library, to help characterizing the mineralogical evolution of terrestrial bodies, starting with Mars. A total of 94 natural Earth rocks have been collected from selected locations around the world to get a selection of analogues for Martian geology. The PTAL library gathers a variety of igneous rocks from different plutonic and volcanic origins and compositions, associated to different environments and levels of aqueous alteration. Samples of impact craters and sedimentary units are also present. The full set of samples will be characterized with optical thin section analysis and XRD (Oslo University, Norway), NIR spectroscopy (Paris-Saclay University, France), Raman spectroscopy (Valladolid University, Spain) and LIBS (Paul Sabatier University, France). The multianalytical study used within the PTAL project provides an unique opportunity to coordinate minerals/elements detection by different techniques that are similar to the instruments onboard current and forthcoming Martian missions. Such combined analysis should give the opportunity to prepare and improve ExoMars/ESA-Roscosmos and Mars2020/NASA observations. This paper focuses only on the NIR measurements and interpretations. The diversity of the PTAL samples is well revealed by the diversity of spectra from the NIR observations. The detected minerals are representative of various formation, alteration and geochemical environments. The major diagnostic features observed are those of primary Fe2+ bearing silicates like olivine or pyroxene with low and/or high calcium content; altered silicates detected with vibrational features associated to OH and/or H2O and/or metal-OH features; oxides; zeolites; and carbonates. This collection brings together a set of rocks and minerals that have been reported elsewhere in the Solar System and particularly on Mars.
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: 1. characterization of samples by near-infrared point spectrometer
dc.typeJournal article
dc.creator.authorLantz, Cateline
dc.creator.authorPoulet, Francois
dc.creator.authorLoizeau, Damien
dc.creator.authorRiu, Lucie
dc.creator.authorPilorget, C.
dc.creator.authorCarter, John
dc.creator.authorDypvik, Henning
dc.creator.authorRull, Fernando
dc.creator.authorWerner, Stephanie C.
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1886452
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=189&rft.spage=&rft.date=2020
dc.identifier.jtitlePlanetary and Space Science
dc.identifier.volume189
dc.identifier.pagecount18
dc.identifier.doihttps://doi.org/10.1016/j.pss.2020.104989
dc.identifier.urnURN:NBN:no-86732
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0032-0633
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/83999/2/1-s2.0-S0032063320300246-main%2B%25281%2529.pdf
dc.type.versionPublishedVersion
cristin.articleid104989
dc.relation.projectNFR/223272


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