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Chloromethane release from carbonaceous meteorite affords new insight into Mars lander findings
Controversy continues as to whether chloromethane (CH 3 Cl) detected during pyrolysis of Martian soils by the Viking and Curiosity Mars landers is indicative of organic matter indigenous to Mars. Here we demonstrate CH 3 Cl release (up to 8 μg/g) during low temperature (150–400°C) pyrolysis of the c...
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Published in: | Scientific reports 2014-11, Vol.4 (1), p.7010-7010, Article 7010 |
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description | Controversy continues as to whether chloromethane (CH
3
Cl) detected during pyrolysis of Martian soils by the Viking and Curiosity Mars landers is indicative of organic matter indigenous to Mars. Here we demonstrate CH
3
Cl release (up to 8 μg/g) during low temperature (150–400°C) pyrolysis of the carbonaceous chondrite Murchison with chloride or perchlorate as chlorine source and confirm unequivocally by stable isotope analysis the extraterrestrial origin of the methyl group (δ
2
H +800 to +1100‰, δ
13
C −19.2 to +10‰,). In the terrestrial environment CH
3
Cl released during pyrolysis of organic matter derives from the methoxyl pool. The methoxyl pool in Murchison is consistent both in magnitude (0.044%) and isotope signature (δ
2
H +1054 ± 626‰, δ
13
C +43.2 ± 38.8‰,) with that of the CH
3
Cl released on pyrolysis. Thus CH
3
Cl emissions recorded by Mars lander experiments may be attributed to methoxyl groups in undegraded organic matter in meteoritic debris reaching the Martian surface being converted to CH
3
Cl with perchlorate or chloride in Martian soil. However we cannot discount emissions arising additionally from organic matter of indigenous origin. The stable isotope signatures of CH
3
Cl detected on Mars could potentially be utilized to determine its origin by distinguishing between terrestrial contamination, meteoritic infall and indigenous Martian sources. |
doi_str_mv | 10.1038/srep07010 |
format | article |
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3
Cl) detected during pyrolysis of Martian soils by the Viking and Curiosity Mars landers is indicative of organic matter indigenous to Mars. Here we demonstrate CH
3
Cl release (up to 8 μg/g) during low temperature (150–400°C) pyrolysis of the carbonaceous chondrite Murchison with chloride or perchlorate as chlorine source and confirm unequivocally by stable isotope analysis the extraterrestrial origin of the methyl group (δ
2
H +800 to +1100‰, δ
13
C −19.2 to +10‰,). In the terrestrial environment CH
3
Cl released during pyrolysis of organic matter derives from the methoxyl pool. The methoxyl pool in Murchison is consistent both in magnitude (0.044%) and isotope signature (δ
2
H +1054 ± 626‰, δ
13
C +43.2 ± 38.8‰,) with that of the CH
3
Cl released on pyrolysis. Thus CH
3
Cl emissions recorded by Mars lander experiments may be attributed to methoxyl groups in undegraded organic matter in meteoritic debris reaching the Martian surface being converted to CH
3
Cl with perchlorate or chloride in Martian soil. However we cannot discount emissions arising additionally from organic matter of indigenous origin. The stable isotope signatures of CH
3
Cl detected on Mars could potentially be utilized to determine its origin by distinguishing between terrestrial contamination, meteoritic infall and indigenous Martian sources.</description><identifier>ISSN: 2045-2322</identifier><identifier>EISSN: 2045-2322</identifier><identifier>DOI: 10.1038/srep07010</identifier><identifier>PMID: 25394222</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>704/445/209 ; 704/445/849 ; Chlorides ; Chlorine ; Chloromethane ; Contamination ; Emissions ; Humanities and Social Sciences ; Low temperature ; Mars ; multidisciplinary ; Organic matter ; Perchlorate ; Perchloric acid ; Pyrolysis ; Science ; Stable isotopes ; Temperature effects ; Terrestrial environments</subject><ispartof>Scientific reports, 2014-11, Vol.4 (1), p.7010-7010, Article 7010</ispartof><rights>The Author(s) 2014</rights><rights>Copyright Nature Publishing Group Nov 2014</rights><rights>Copyright © 2014, Macmillan Publishers Limited. All rights reserved 2014 Macmillan Publishers Limited. All rights reserved</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c438t-da5de20485bbf5f9389c514af94bc47fc4e13545f68054b1ba0a26ab04ed132e3</citedby><cites>FETCH-LOGICAL-c438t-da5de20485bbf5f9389c514af94bc47fc4e13545f68054b1ba0a26ab04ed132e3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/1898173284/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/1898173284?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>230,314,727,780,784,885,25753,27924,27925,37012,37013,44590,53791,53793,75126</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/25394222$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Keppler, Frank</creatorcontrib><creatorcontrib>Harper, David B.</creatorcontrib><creatorcontrib>Greule, Markus</creatorcontrib><creatorcontrib>Ott, Ulrich</creatorcontrib><creatorcontrib>Sattler, Tobias</creatorcontrib><creatorcontrib>Schöler, Heinz F.</creatorcontrib><creatorcontrib>Hamilton, John T. G.</creatorcontrib><title>Chloromethane release from carbonaceous meteorite affords new insight into Mars lander findings</title><title>Scientific reports</title><addtitle>Sci Rep</addtitle><addtitle>Sci Rep</addtitle><description>Controversy continues as to whether chloromethane (CH
3
Cl) detected during pyrolysis of Martian soils by the Viking and Curiosity Mars landers is indicative of organic matter indigenous to Mars. Here we demonstrate CH
3
Cl release (up to 8 μg/g) during low temperature (150–400°C) pyrolysis of the carbonaceous chondrite Murchison with chloride or perchlorate as chlorine source and confirm unequivocally by stable isotope analysis the extraterrestrial origin of the methyl group (δ
2
H +800 to +1100‰, δ
13
C −19.2 to +10‰,). In the terrestrial environment CH
3
Cl released during pyrolysis of organic matter derives from the methoxyl pool. The methoxyl pool in Murchison is consistent both in magnitude (0.044%) and isotope signature (δ
2
H +1054 ± 626‰, δ
13
C +43.2 ± 38.8‰,) with that of the CH
3
Cl released on pyrolysis. Thus CH
3
Cl emissions recorded by Mars lander experiments may be attributed to methoxyl groups in undegraded organic matter in meteoritic debris reaching the Martian surface being converted to CH
3
Cl with perchlorate or chloride in Martian soil. However we cannot discount emissions arising additionally from organic matter of indigenous origin. The stable isotope signatures of CH
3
Cl detected on Mars could potentially be utilized to determine its origin by distinguishing between terrestrial contamination, meteoritic infall and indigenous Martian sources.</description><subject>704/445/209</subject><subject>704/445/849</subject><subject>Chlorides</subject><subject>Chlorine</subject><subject>Chloromethane</subject><subject>Contamination</subject><subject>Emissions</subject><subject>Humanities and Social Sciences</subject><subject>Low temperature</subject><subject>Mars</subject><subject>multidisciplinary</subject><subject>Organic matter</subject><subject>Perchlorate</subject><subject>Perchloric acid</subject><subject>Pyrolysis</subject><subject>Science</subject><subject>Stable isotopes</subject><subject>Temperature effects</subject><subject>Terrestrial environments</subject><issn>2045-2322</issn><issn>2045-2322</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNplkUtLAzEUhYMotmgX_gEJuFGhmmc7sxGk-IKKG12HTOamTZkmNZkq_nujraVqNjfkfpzccw9CR5RcUMKLyxRhQYaEkh3UZUTIPuOM7W7dO6iX0ozkI1kpaLmPOkzyUjDGukiNpk2IYQ7tVHvAERrQCbDNT9joWAWvDYRlwpmAEF0LWFsbYp2wh3fsfHKTaZtrG_Cjjgk32tcQsXW-dn6SDtGe1U2C3roeoJfbm-fRfX_8dPcwuh73jeBF26-1rCFPXMiqstKWvCiNpELbUlRGDK0RQLkU0g4KIkVFK000G-iKCKgpZ8AP0NVKd7Gs5lAb8G3UjVpEN9fxQwXt1O-Od1M1CW9KMJ43M8gCp2uBGF6XkFo1d8lAk_18-Vd0kJcmmPhGT_6gs7CMPttTtCgLOuSsEJk6W1EmhpRDspthKFFfyalNcpk93p5-Q_7klIHzFZByy08gbn35T-0TlKKkDg</recordid><startdate>20141113</startdate><enddate>20141113</enddate><creator>Keppler, Frank</creator><creator>Harper, David B.</creator><creator>Greule, Markus</creator><creator>Ott, Ulrich</creator><creator>Sattler, Tobias</creator><creator>Schöler, Heinz F.</creator><creator>Hamilton, John T. G.</creator><general>Nature Publishing Group UK</general><general>Nature Publishing Group</general><scope>C6C</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88E</scope><scope>88I</scope><scope>8FE</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BENPR</scope><scope>BHPHI</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>HCIFZ</scope><scope>K9.</scope><scope>LK8</scope><scope>M0S</scope><scope>M1P</scope><scope>M2P</scope><scope>M7P</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope><scope>7X8</scope><scope>5PM</scope></search><sort><creationdate>20141113</creationdate><title>Chloromethane release from carbonaceous meteorite affords new insight into Mars lander findings</title><author>Keppler, Frank ; Harper, David B. ; Greule, Markus ; Ott, Ulrich ; Sattler, Tobias ; Schöler, Heinz F. ; Hamilton, John T. G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c438t-da5de20485bbf5f9389c514af94bc47fc4e13545f68054b1ba0a26ab04ed132e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>704/445/209</topic><topic>704/445/849</topic><topic>Chlorides</topic><topic>Chlorine</topic><topic>Chloromethane</topic><topic>Contamination</topic><topic>Emissions</topic><topic>Humanities and Social Sciences</topic><topic>Low temperature</topic><topic>Mars</topic><topic>multidisciplinary</topic><topic>Organic matter</topic><topic>Perchlorate</topic><topic>Perchloric acid</topic><topic>Pyrolysis</topic><topic>Science</topic><topic>Stable isotopes</topic><topic>Temperature effects</topic><topic>Terrestrial environments</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Keppler, Frank</creatorcontrib><creatorcontrib>Harper, David B.</creatorcontrib><creatorcontrib>Greule, Markus</creatorcontrib><creatorcontrib>Ott, Ulrich</creatorcontrib><creatorcontrib>Sattler, Tobias</creatorcontrib><creatorcontrib>Schöler, Heinz F.</creatorcontrib><creatorcontrib>Hamilton, John T. G.</creatorcontrib><collection>Springer Nature OA Free Journals</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>ProQuest Health and Medical</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Biology Database (Alumni Edition)</collection><collection>Medical Database (Alumni Edition)</collection><collection>Science Database (Alumni Edition)</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Hospital Premium Collection</collection><collection>Hospital Premium Collection (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>Biological Science Collection</collection><collection>ProQuest Central</collection><collection>ProQuest Natural Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>Health Research Premium Collection</collection><collection>Health Research Premium Collection (Alumni)</collection><collection>ProQuest Central Student</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Health & Medical Complete (Alumni)</collection><collection>ProQuest Biological Science Collection</collection><collection>Health & Medical Collection (Alumni Edition)</collection><collection>Medical Database</collection><collection>ProQuest Science Journals</collection><collection>Biological Science Database</collection><collection>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><collection>MEDLINE - Academic</collection><collection>PubMed Central (Full Participant titles)</collection><jtitle>Scientific reports</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Keppler, Frank</au><au>Harper, David B.</au><au>Greule, Markus</au><au>Ott, Ulrich</au><au>Sattler, Tobias</au><au>Schöler, Heinz F.</au><au>Hamilton, John T. G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Chloromethane release from carbonaceous meteorite affords new insight into Mars lander findings</atitle><jtitle>Scientific reports</jtitle><stitle>Sci Rep</stitle><addtitle>Sci Rep</addtitle><date>2014-11-13</date><risdate>2014</risdate><volume>4</volume><issue>1</issue><spage>7010</spage><epage>7010</epage><pages>7010-7010</pages><artnum>7010</artnum><issn>2045-2322</issn><eissn>2045-2322</eissn><abstract>Controversy continues as to whether chloromethane (CH
3
Cl) detected during pyrolysis of Martian soils by the Viking and Curiosity Mars landers is indicative of organic matter indigenous to Mars. Here we demonstrate CH
3
Cl release (up to 8 μg/g) during low temperature (150–400°C) pyrolysis of the carbonaceous chondrite Murchison with chloride or perchlorate as chlorine source and confirm unequivocally by stable isotope analysis the extraterrestrial origin of the methyl group (δ
2
H +800 to +1100‰, δ
13
C −19.2 to +10‰,). In the terrestrial environment CH
3
Cl released during pyrolysis of organic matter derives from the methoxyl pool. The methoxyl pool in Murchison is consistent both in magnitude (0.044%) and isotope signature (δ
2
H +1054 ± 626‰, δ
13
C +43.2 ± 38.8‰,) with that of the CH
3
Cl released on pyrolysis. Thus CH
3
Cl emissions recorded by Mars lander experiments may be attributed to methoxyl groups in undegraded organic matter in meteoritic debris reaching the Martian surface being converted to CH
3
Cl with perchlorate or chloride in Martian soil. However we cannot discount emissions arising additionally from organic matter of indigenous origin. The stable isotope signatures of CH
3
Cl detected on Mars could potentially be utilized to determine its origin by distinguishing between terrestrial contamination, meteoritic infall and indigenous Martian sources.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><pmid>25394222</pmid><doi>10.1038/srep07010</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record> |
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subjects | 704/445/209 704/445/849 Chlorides Chlorine Chloromethane Contamination Emissions Humanities and Social Sciences Low temperature Mars multidisciplinary Organic matter Perchlorate Perchloric acid Pyrolysis Science Stable isotopes Temperature effects Terrestrial environments |
title | Chloromethane release from carbonaceous meteorite affords new insight into Mars lander findings |
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