ExoMars Raman Laser Spectrometer: A Tool for the Potential Recognition of Wet-Target Craters on Mars
In the present work, near-infrared, laser-induced breakdown spectroscopy, Raman, and X-ray diffractometer techniques have been complementarily used to carry out a comprehensive characterization of a terrestrial analogue selected from the Chesapeake Bay impact structure (CBIS). The obtained data clea...
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| Veröffentlicht in: | Astrobiology 2020-03, Vol.20 (3), p.349-363 |
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| creator | Veneranda, Marco Lopez-Reyes, Guillermo Manrique, José Antonio Medina, Jesus Ruiz-Galende, Patricia Torre-Fdez, Imanol Castro, Kepa Lantz, Cateline Poulet, François Dypvik, Henning Werner, Stephanie C Rull, Fernando |
| description | In the present work, near-infrared, laser-induced breakdown spectroscopy, Raman, and X-ray diffractometer techniques have been complementarily used to carry out a comprehensive characterization of a terrestrial analogue selected from the Chesapeake Bay impact structure (CBIS). The obtained data clearly highlight the key role of Raman spectroscopy in the detection of minor and trace compounds, through which inferences about geological processes occurred in the CBIS can be extrapolated. Beside the use of commercial systems, further Raman analyses were performed by the Raman laser spectrometer (RLS) ExoMars Simulator. This instrument represents the most reliable tool to effectively predict the scientific capabilities of the ExoMars/Raman system that will be deployed on Mars in 2021. By emulating the analytical procedures and operational restrictions established by the ExoMars mission rover design, it was proved that the RLS ExoMars Simulator can detect the amorphization of quartz, which constitutes an analytical clue of the impact origin of craters. Beside amorphized minerals, the detection of barite and siderite, compounds crystallizing under hydrothermal conditions, helps indirectly to confirm the presence of water in impact targets. Furthermore, the RLS ExoMars Simulator capability of performing smart molecular mappings was successfully evaluated. |
| doi_str_mv | 10.1089/ast.2019.2095 |
| format | Article |
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The obtained data clearly highlight the key role of Raman spectroscopy in the detection of minor and trace compounds, through which inferences about geological processes occurred in the CBIS can be extrapolated. Beside the use of commercial systems, further Raman analyses were performed by the Raman laser spectrometer (RLS) ExoMars Simulator. This instrument represents the most reliable tool to effectively predict the scientific capabilities of the ExoMars/Raman system that will be deployed on Mars in 2021. By emulating the analytical procedures and operational restrictions established by the ExoMars mission rover design, it was proved that the RLS ExoMars Simulator can detect the amorphization of quartz, which constitutes an analytical clue of the impact origin of craters. Beside amorphized minerals, the detection of barite and siderite, compounds crystallizing under hydrothermal conditions, helps indirectly to confirm the presence of water in impact targets. Furthermore, the RLS ExoMars Simulator capability of performing smart molecular mappings was successfully evaluated.</description><identifier>ISSN: 1531-1074</identifier><identifier>EISSN: 1557-8070</identifier><identifier>DOI: 10.1089/ast.2019.2095</identifier><identifier>PMID: 31985268</identifier><language>eng</language><publisher>United States: Mary Ann Liebert, Inc</publisher><subject>Amorphization ; Analytical methods ; Astrophysics ; Barite ; Detection ; Earth analogs ; Earth and Planetary Astrophysics ; Geological processes ; Infrared lasers ; Laser induced breakdown spectroscopy ; Lasers ; Mars ; Mars craters ; Mars missions ; Mars rovers ; Minerals ; Near infrared radiation ; Physics ; Procedures ; Raman lasers ; Raman spectroscopy ; Siderite ; Simulation ; Simulators ; Spectroscopy ; Spectrum analysis ; Target recognition ; Terrestrial environments</subject><ispartof>Astrobiology, 2020-03, Vol.20 (3), p.349-363</ispartof><rights>Copyright Mary Ann Liebert, Inc. Mar 2020</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c355t-f9f18bfe7f63c80a424d3c30a4ee09fe579e538d246418aecd55530e7ce4544c3</citedby><cites>FETCH-LOGICAL-c355t-f9f18bfe7f63c80a424d3c30a4ee09fe579e538d246418aecd55530e7ce4544c3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,780,784,885,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/31985268$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://hal.science/hal-04490149$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Veneranda, Marco</creatorcontrib><creatorcontrib>Lopez-Reyes, Guillermo</creatorcontrib><creatorcontrib>Manrique, José Antonio</creatorcontrib><creatorcontrib>Medina, Jesus</creatorcontrib><creatorcontrib>Ruiz-Galende, Patricia</creatorcontrib><creatorcontrib>Torre-Fdez, Imanol</creatorcontrib><creatorcontrib>Castro, Kepa</creatorcontrib><creatorcontrib>Lantz, Cateline</creatorcontrib><creatorcontrib>Poulet, François</creatorcontrib><creatorcontrib>Dypvik, Henning</creatorcontrib><creatorcontrib>Werner, Stephanie C</creatorcontrib><creatorcontrib>Rull, Fernando</creatorcontrib><title>ExoMars Raman Laser Spectrometer: A Tool for the Potential Recognition of Wet-Target Craters on Mars</title><title>Astrobiology</title><addtitle>Astrobiology</addtitle><description>In the present work, near-infrared, laser-induced breakdown spectroscopy, Raman, and X-ray diffractometer techniques have been complementarily used to carry out a comprehensive characterization of a terrestrial analogue selected from the Chesapeake Bay impact structure (CBIS). The obtained data clearly highlight the key role of Raman spectroscopy in the detection of minor and trace compounds, through which inferences about geological processes occurred in the CBIS can be extrapolated. Beside the use of commercial systems, further Raman analyses were performed by the Raman laser spectrometer (RLS) ExoMars Simulator. This instrument represents the most reliable tool to effectively predict the scientific capabilities of the ExoMars/Raman system that will be deployed on Mars in 2021. By emulating the analytical procedures and operational restrictions established by the ExoMars mission rover design, it was proved that the RLS ExoMars Simulator can detect the amorphization of quartz, which constitutes an analytical clue of the impact origin of craters. Beside amorphized minerals, the detection of barite and siderite, compounds crystallizing under hydrothermal conditions, helps indirectly to confirm the presence of water in impact targets. Furthermore, the RLS ExoMars Simulator capability of performing smart molecular mappings was successfully evaluated.</description><subject>Amorphization</subject><subject>Analytical methods</subject><subject>Astrophysics</subject><subject>Barite</subject><subject>Detection</subject><subject>Earth analogs</subject><subject>Earth and Planetary Astrophysics</subject><subject>Geological processes</subject><subject>Infrared lasers</subject><subject>Laser induced breakdown spectroscopy</subject><subject>Lasers</subject><subject>Mars</subject><subject>Mars craters</subject><subject>Mars missions</subject><subject>Mars rovers</subject><subject>Minerals</subject><subject>Near infrared radiation</subject><subject>Physics</subject><subject>Procedures</subject><subject>Raman lasers</subject><subject>Raman spectroscopy</subject><subject>Siderite</subject><subject>Simulation</subject><subject>Simulators</subject><subject>Spectroscopy</subject><subject>Spectrum analysis</subject><subject>Target recognition</subject><subject>Terrestrial environments</subject><issn>1531-1074</issn><issn>1557-8070</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNpdkU1PxCAQhonR-H30aki86KEKBdribbNR12SNZl3jkSAdtKYtK7BG_700u3rwwkyYhzdDHoSOKDmnpJIXOsTznFCZDik20C4VoswqUpLNoWc0o6TkO2gvhHdCKMtlsY12GJWVyItqF9VXX-5O-4BnutM9nuoAHj8uwETvOojgL_EIz51rsXUexzfADy5CHxvd4hkY99o3sXE9dhY_Q8zm2r9CxGOv09OA02AIP0BbVrcBDtd1Hz1dX83Hk2x6f3M7Hk0zw4SImZWWVi8WSlswUxHNc14zw1IDQKQFUUoQrKpzXnBaaTC1EIIRKA1wwblh--hslfumW7XwTaf9t3K6UZPRVA13hHNJKJefNLGnK3bh3ccSQlRdEwy0re7BLYPKGS9yycsiT-jJP_TdLX2ffpKoQkpKSz5Q2Yoy3oXgwf5tQIkaVKmkSg2q1KAq8cfr1OVLB_Uf_euG_QCG040l</recordid><startdate>202003</startdate><enddate>202003</enddate><creator>Veneranda, Marco</creator><creator>Lopez-Reyes, Guillermo</creator><creator>Manrique, José Antonio</creator><creator>Medina, Jesus</creator><creator>Ruiz-Galende, Patricia</creator><creator>Torre-Fdez, Imanol</creator><creator>Castro, Kepa</creator><creator>Lantz, Cateline</creator><creator>Poulet, François</creator><creator>Dypvik, Henning</creator><creator>Werner, Stephanie C</creator><creator>Rull, Fernando</creator><general>Mary Ann Liebert, Inc</general><general>Mary Ann Liebert</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7SN</scope><scope>C1K</scope><scope>F1W</scope><scope>H95</scope><scope>L.G</scope><scope>7X8</scope><scope>1XC</scope></search><sort><creationdate>202003</creationdate><title>ExoMars Raman Laser Spectrometer: A Tool for the Potential Recognition of Wet-Target Craters on Mars</title><author>Veneranda, Marco ; Lopez-Reyes, Guillermo ; Manrique, José Antonio ; Medina, Jesus ; Ruiz-Galende, Patricia ; Torre-Fdez, Imanol ; Castro, Kepa ; Lantz, Cateline ; Poulet, François ; Dypvik, Henning ; Werner, Stephanie C ; Rull, Fernando</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c355t-f9f18bfe7f63c80a424d3c30a4ee09fe579e538d246418aecd55530e7ce4544c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Amorphization</topic><topic>Analytical methods</topic><topic>Astrophysics</topic><topic>Barite</topic><topic>Detection</topic><topic>Earth analogs</topic><topic>Earth and Planetary Astrophysics</topic><topic>Geological processes</topic><topic>Infrared lasers</topic><topic>Laser induced breakdown spectroscopy</topic><topic>Lasers</topic><topic>Mars</topic><topic>Mars craters</topic><topic>Mars missions</topic><topic>Mars rovers</topic><topic>Minerals</topic><topic>Near infrared radiation</topic><topic>Physics</topic><topic>Procedures</topic><topic>Raman lasers</topic><topic>Raman spectroscopy</topic><topic>Siderite</topic><topic>Simulation</topic><topic>Simulators</topic><topic>Spectroscopy</topic><topic>Spectrum analysis</topic><topic>Target recognition</topic><topic>Terrestrial environments</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Veneranda, Marco</creatorcontrib><creatorcontrib>Lopez-Reyes, Guillermo</creatorcontrib><creatorcontrib>Manrique, José Antonio</creatorcontrib><creatorcontrib>Medina, Jesus</creatorcontrib><creatorcontrib>Ruiz-Galende, Patricia</creatorcontrib><creatorcontrib>Torre-Fdez, Imanol</creatorcontrib><creatorcontrib>Castro, Kepa</creatorcontrib><creatorcontrib>Lantz, Cateline</creatorcontrib><creatorcontrib>Poulet, François</creatorcontrib><creatorcontrib>Dypvik, Henning</creatorcontrib><creatorcontrib>Werner, Stephanie C</creatorcontrib><creatorcontrib>Rull, Fernando</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>Ecology Abstracts</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 1: Biological Sciences & Living Resources</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>MEDLINE - Academic</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Astrobiology</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Veneranda, Marco</au><au>Lopez-Reyes, Guillermo</au><au>Manrique, José Antonio</au><au>Medina, Jesus</au><au>Ruiz-Galende, Patricia</au><au>Torre-Fdez, Imanol</au><au>Castro, Kepa</au><au>Lantz, Cateline</au><au>Poulet, François</au><au>Dypvik, Henning</au><au>Werner, Stephanie C</au><au>Rull, Fernando</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>ExoMars Raman Laser Spectrometer: A Tool for the Potential Recognition of Wet-Target Craters on Mars</atitle><jtitle>Astrobiology</jtitle><addtitle>Astrobiology</addtitle><date>2020-03</date><risdate>2020</risdate><volume>20</volume><issue>3</issue><spage>349</spage><epage>363</epage><pages>349-363</pages><issn>1531-1074</issn><eissn>1557-8070</eissn><abstract>In the present work, near-infrared, laser-induced breakdown spectroscopy, Raman, and X-ray diffractometer techniques have been complementarily used to carry out a comprehensive characterization of a terrestrial analogue selected from the Chesapeake Bay impact structure (CBIS). The obtained data clearly highlight the key role of Raman spectroscopy in the detection of minor and trace compounds, through which inferences about geological processes occurred in the CBIS can be extrapolated. Beside the use of commercial systems, further Raman analyses were performed by the Raman laser spectrometer (RLS) ExoMars Simulator. This instrument represents the most reliable tool to effectively predict the scientific capabilities of the ExoMars/Raman system that will be deployed on Mars in 2021. By emulating the analytical procedures and operational restrictions established by the ExoMars mission rover design, it was proved that the RLS ExoMars Simulator can detect the amorphization of quartz, which constitutes an analytical clue of the impact origin of craters. Beside amorphized minerals, the detection of barite and siderite, compounds crystallizing under hydrothermal conditions, helps indirectly to confirm the presence of water in impact targets. Furthermore, the RLS ExoMars Simulator capability of performing smart molecular mappings was successfully evaluated.</abstract><cop>United States</cop><pub>Mary Ann Liebert, Inc</pub><pmid>31985268</pmid><doi>10.1089/ast.2019.2095</doi><tpages>15</tpages></addata></record> |
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| source | Alma/SFX Local Collection |
| subjects | Amorphization Analytical methods Astrophysics Barite Detection Earth analogs Earth and Planetary Astrophysics Geological processes Infrared lasers Laser induced breakdown spectroscopy Lasers Mars Mars craters Mars missions Mars rovers Minerals Near infrared radiation Physics Procedures Raman lasers Raman spectroscopy Siderite Simulation Simulators Spectroscopy Spectrum analysis Target recognition Terrestrial environments |
| title | ExoMars Raman Laser Spectrometer: A Tool for the Potential Recognition of Wet-Target Craters on Mars |
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