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Raman spectroscopy: Caution when interpreting organic carbon from oxidising environments
Oxidation on Mars is primarily caused by the high influx of cosmic and solar radiation which interacts with the Martian surface. The evidence of this can be seen in the ubiquitous red colouration of the Martian sediment. This radiation will destroy most signals of life in the top few metres of the M...
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Published in: | Planetary and space science 2016-02, Vol.121, p.53-59 |
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description | Oxidation on Mars is primarily caused by the high influx of cosmic and solar radiation which interacts with the Martian surface. The evidence of this can be seen in the ubiquitous red colouration of the Martian sediment. This radiation will destroy most signals of life in the top few metres of the Martian surface. If organic carbon (one of the building blocks of life) is present within the accessible Martian sediments, it is very likely that it will have experienced some oxidation. ESA׳s ExoMars mission set to fly in 2018, has on board a miniaturised Raman spectrometer. As Raman spectroscopy is sensitive to carbonaceous material and will be primarily used to characterise organics, it is essential that the effect oxidation has on the Raman carbon signal is assessed. Oxidised carbonaceous shales were analysed using Raman spectroscopy to assess this issue. Results show that haematite has a band which occurs in the same frequency as the carbon D band, which cannot be distinguished from each other. This can lead to a misidentification of the carbon D band and a misinterpretation of the carbon order. Consequently, caution must be taken when applying Raman spectroscopy for organic carbon analysis in oxidised terrestrial and extraterrestrial environments, including on Mars.
•The haematite 2LO mode occurs in the same frequency as the carbon D band.•The haematite band overprints the carbon D band in all oxidised samples.•This leads to a misidentification of the Carbon D band in oxidised samples.•The carbon order can be misinterpreted as a result of this.•Caution must be taken when using Raman spectroscopy in oxidising environments. |
doi_str_mv | 10.1016/j.pss.2015.12.008 |
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•The haematite 2LO mode occurs in the same frequency as the carbon D band.•The haematite band overprints the carbon D band in all oxidised samples.•This leads to a misidentification of the Carbon D band in oxidised samples.•The carbon order can be misinterpreted as a result of this.•Caution must be taken when using Raman spectroscopy in oxidising environments.</description><identifier>ISSN: 0032-0633</identifier><identifier>EISSN: 1873-5088</identifier><identifier>DOI: 10.1016/j.pss.2015.12.008</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><subject>Carbon ; ExoMars ; Extraterrestrial environments ; Mars (planet) ; Mars missions ; Mars surface ; Organic carbon ; Oxidation ; Oxidised carbon ; Raman spectroscopy ; Sediments</subject><ispartof>Planetary and space science, 2016-02, Vol.121, p.53-59</ispartof><rights>2015 The Authors</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c406t-7c36c2e3b84a94aa1e1620e663b0dc497b0a816efef5048c80e81a144f42ae913</citedby><cites>FETCH-LOGICAL-c406t-7c36c2e3b84a94aa1e1620e663b0dc497b0a816efef5048c80e81a144f42ae913</cites><orcidid>0000-0003-4714-2121</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids></links><search><creatorcontrib>Brolly, Connor</creatorcontrib><creatorcontrib>Parnell, John</creatorcontrib><creatorcontrib>Bowden, Stephen</creatorcontrib><title>Raman spectroscopy: Caution when interpreting organic carbon from oxidising environments</title><title>Planetary and space science</title><description>Oxidation on Mars is primarily caused by the high influx of cosmic and solar radiation which interacts with the Martian surface. The evidence of this can be seen in the ubiquitous red colouration of the Martian sediment. This radiation will destroy most signals of life in the top few metres of the Martian surface. If organic carbon (one of the building blocks of life) is present within the accessible Martian sediments, it is very likely that it will have experienced some oxidation. ESA׳s ExoMars mission set to fly in 2018, has on board a miniaturised Raman spectrometer. As Raman spectroscopy is sensitive to carbonaceous material and will be primarily used to characterise organics, it is essential that the effect oxidation has on the Raman carbon signal is assessed. Oxidised carbonaceous shales were analysed using Raman spectroscopy to assess this issue. Results show that haematite has a band which occurs in the same frequency as the carbon D band, which cannot be distinguished from each other. This can lead to a misidentification of the carbon D band and a misinterpretation of the carbon order. Consequently, caution must be taken when applying Raman spectroscopy for organic carbon analysis in oxidised terrestrial and extraterrestrial environments, including on Mars.
•The haematite 2LO mode occurs in the same frequency as the carbon D band.•The haematite band overprints the carbon D band in all oxidised samples.•This leads to a misidentification of the Carbon D band in oxidised samples.•The carbon order can be misinterpreted as a result of this.•Caution must be taken when using Raman spectroscopy in oxidising environments.</description><subject>Carbon</subject><subject>ExoMars</subject><subject>Extraterrestrial environments</subject><subject>Mars (planet)</subject><subject>Mars missions</subject><subject>Mars surface</subject><subject>Organic carbon</subject><subject>Oxidation</subject><subject>Oxidised carbon</subject><subject>Raman spectroscopy</subject><subject>Sediments</subject><issn>0032-0633</issn><issn>1873-5088</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNqNkEtLxDAQgIMouD5-gLcevbTOJG2a6kkWX7AgiIK3kM1O1yzbpCZdH__eLutZPM1hvm9gPsbOEAoElBerok-p4IBVgbwAUHtsgqoWeQVK7bMJgOA5SCEO2VFKKwCQktcT9vpkOuOz1JMdYkg29N-X2dRsBhd89vlGPnN-oNhHGpxfZiEujXc2sybOR6CNocvCl1u4tN2S_3Ax-I78kE7YQWvWiU5_5zF7ub15nt7ns8e7h-n1LLclyCGvrZCWk5ir0jSlMUgoOZCUYg4LWzb1HIxCSS21FZTKKiCFBsuyLbmhBsUxO9_d7WN431AadOeSpfXaeAqbpLFuBG94I_k_UFk1CjhWI4o71I5RUqRW99F1Jn5rBL0Nrld6DK63wTVyPQYfnaudQ-O7H46iTtaRt7RwcayrF8H9Yf8Av4CKAA</recordid><startdate>201602</startdate><enddate>201602</enddate><creator>Brolly, Connor</creator><creator>Parnell, John</creator><creator>Bowden, Stephen</creator><general>Elsevier Ltd</general><scope>6I.</scope><scope>AAFTH</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-4714-2121</orcidid></search><sort><creationdate>201602</creationdate><title>Raman spectroscopy: Caution when interpreting organic carbon from oxidising environments</title><author>Brolly, Connor ; Parnell, John ; Bowden, Stephen</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c406t-7c36c2e3b84a94aa1e1620e663b0dc497b0a816efef5048c80e81a144f42ae913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Carbon</topic><topic>ExoMars</topic><topic>Extraterrestrial environments</topic><topic>Mars (planet)</topic><topic>Mars missions</topic><topic>Mars surface</topic><topic>Organic carbon</topic><topic>Oxidation</topic><topic>Oxidised carbon</topic><topic>Raman spectroscopy</topic><topic>Sediments</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Brolly, Connor</creatorcontrib><creatorcontrib>Parnell, John</creatorcontrib><creatorcontrib>Bowden, Stephen</creatorcontrib><collection>ScienceDirect Open Access Titles</collection><collection>Elsevier:ScienceDirect:Open Access</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Planetary and space science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Brolly, Connor</au><au>Parnell, John</au><au>Bowden, Stephen</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Raman spectroscopy: Caution when interpreting organic carbon from oxidising environments</atitle><jtitle>Planetary and space science</jtitle><date>2016-02</date><risdate>2016</risdate><volume>121</volume><spage>53</spage><epage>59</epage><pages>53-59</pages><issn>0032-0633</issn><eissn>1873-5088</eissn><abstract>Oxidation on Mars is primarily caused by the high influx of cosmic and solar radiation which interacts with the Martian surface. The evidence of this can be seen in the ubiquitous red colouration of the Martian sediment. This radiation will destroy most signals of life in the top few metres of the Martian surface. If organic carbon (one of the building blocks of life) is present within the accessible Martian sediments, it is very likely that it will have experienced some oxidation. ESA׳s ExoMars mission set to fly in 2018, has on board a miniaturised Raman spectrometer. As Raman spectroscopy is sensitive to carbonaceous material and will be primarily used to characterise organics, it is essential that the effect oxidation has on the Raman carbon signal is assessed. Oxidised carbonaceous shales were analysed using Raman spectroscopy to assess this issue. Results show that haematite has a band which occurs in the same frequency as the carbon D band, which cannot be distinguished from each other. This can lead to a misidentification of the carbon D band and a misinterpretation of the carbon order. Consequently, caution must be taken when applying Raman spectroscopy for organic carbon analysis in oxidised terrestrial and extraterrestrial environments, including on Mars.
•The haematite 2LO mode occurs in the same frequency as the carbon D band.•The haematite band overprints the carbon D band in all oxidised samples.•This leads to a misidentification of the Carbon D band in oxidised samples.•The carbon order can be misinterpreted as a result of this.•Caution must be taken when using Raman spectroscopy in oxidising environments.</abstract><pub>Elsevier Ltd</pub><doi>10.1016/j.pss.2015.12.008</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0003-4714-2121</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Carbon ExoMars Extraterrestrial environments Mars (planet) Mars missions Mars surface Organic carbon Oxidation Oxidised carbon Raman spectroscopy Sediments |
title | Raman spectroscopy: Caution when interpreting organic carbon from oxidising environments |
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