Experimental constraints on the volatility of germanium, zinc, and lithium in Martian basalts and the role of degassing in alteration of surface minerals
The surface of Mars is enriched in Cl and S which is linked to volcanic activity and degassing. Similarly, elevated Ge and Zn levels in Gale crater sedimentary bedrock indicate a magmatic source for these elements. To constrain the relative effects of Cl and S on the outgassing of these trace metals...
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description | The surface of Mars is enriched in Cl and S which is linked to volcanic activity and degassing. Similarly, elevated Ge and Zn levels in Gale crater sedimentary bedrock indicate a magmatic source for these elements. To constrain the relative effects of Cl and S on the outgassing of these trace metals and chemical characteristics of primary magmatic vapor deposits incorporated to Martian surface, we conducted a set of degassing and fumarolic alteration experiments. Ge is found to be more volatile than Zn in all experiments. In S‐bearing runs, the loss of Ge and Zn was less than any other experiments. In Cl‐only runs, degassing of Zn was more than twice that of Ge within the first 10 min and percent loss increased for both elements with increasing time. In Cl + S runs, S‐induced reduction of GeO
2
and ZnO to metallic Ge and Zn switches the preference of chloride formation from Zn to Ge. Up to 90% of Ge and Zn loss in the 1‐h no volatile‐added (NVA) experiments might be due to the small amounts of Cl contamination in NVA mixes via other oxides used for synthesis. Alteration experiments show different phases between 1‐h and 24‐/72‐h runs. In 1‐h runs, anhydrite and langbeinite dominate while in 24‐/72‐h runs halite and sylvite dominate the condensate assemblages. S‐bearing phases form as the intermediate products of fumarolic deposition, while chlorides are common when the system is allowed to cool gradually. One‐hour exposure was sufficient to form alteration phases and vapor deposits such as NaCl, KCl, CaSO
4
, and langbeinites on the Martian analog minerals. These salts were identified in Martian meteorites and in situ measurements. Our results provide evidence that volcanic degassing along with fumarolic alteration could be a potential source for the enrichment and varying abundances of Cl, S, Fe, Zn, Ge in Martian surface, as well as a cause for Ge depletion in shergottites. |
doi_str_mv | 10.1111/maps.14000 |
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2
and ZnO to metallic Ge and Zn switches the preference of chloride formation from Zn to Ge. Up to 90% of Ge and Zn loss in the 1‐h no volatile‐added (NVA) experiments might be due to the small amounts of Cl contamination in NVA mixes via other oxides used for synthesis. Alteration experiments show different phases between 1‐h and 24‐/72‐h runs. In 1‐h runs, anhydrite and langbeinite dominate while in 24‐/72‐h runs halite and sylvite dominate the condensate assemblages. S‐bearing phases form as the intermediate products of fumarolic deposition, while chlorides are common when the system is allowed to cool gradually. One‐hour exposure was sufficient to form alteration phases and vapor deposits such as NaCl, KCl, CaSO
4
, and langbeinites on the Martian analog minerals. These salts were identified in Martian meteorites and in situ measurements. Our results provide evidence that volcanic degassing along with fumarolic alteration could be a potential source for the enrichment and varying abundances of Cl, S, Fe, Zn, Ge in Martian surface, as well as a cause for Ge depletion in shergottites.</description><identifier>ISSN: 1086-9379</identifier><identifier>EISSN: 1945-5100</identifier><identifier>DOI: 10.1111/maps.14000</identifier><language>eng</language><publisher>Hoboken: Wiley Subscription Services, Inc</publisher><subject>Basalt ; Bedrock ; Chlorides ; Degassing ; Experiments ; Germanium ; Germanium oxides ; In situ measurement ; Lithium ; Mars ; Mars craters ; Mars surface ; Mars volcanoes ; Minerals ; Outgassing ; Phases ; SNC meteorites ; Sodium chloride ; Switches ; Sylvite ; Trace metals ; Vapor deposition ; Volcanic activity ; Zinc ; Zinc oxide</subject><ispartof>Meteoritics & planetary science, 2023-09, Vol.58 (9), p.1183-1210</ispartof><rights>2023. This article is published under http://creativecommons.org/licenses/by-nc-nd/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-a277t-b93a9682d296a7e70240829b6d660479644bef8cc24355e5af10aaf013d9a0c3</cites><orcidid>0000-0002-0380-4683 ; 0000-0001-6950-9700 ; 0000-0002-2840-8863 ; 0000-0001-8516-9435 ; 0000-0002-6075-7908</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Rogaski, Alexander</creatorcontrib><creatorcontrib>Ustunisik, Gokce K.</creatorcontrib><creatorcontrib>Yang, Shuying</creatorcontrib><creatorcontrib>Humayun, Munir</creatorcontrib><creatorcontrib>Righter, Kevin</creatorcontrib><creatorcontrib>Berger, Jeff A.</creatorcontrib><creatorcontrib>DiFrancesco, Nicholas</creatorcontrib><title>Experimental constraints on the volatility of germanium, zinc, and lithium in Martian basalts and the role of degassing in alteration of surface minerals</title><title>Meteoritics & planetary science</title><description>The surface of Mars is enriched in Cl and S which is linked to volcanic activity and degassing. Similarly, elevated Ge and Zn levels in Gale crater sedimentary bedrock indicate a magmatic source for these elements. To constrain the relative effects of Cl and S on the outgassing of these trace metals and chemical characteristics of primary magmatic vapor deposits incorporated to Martian surface, we conducted a set of degassing and fumarolic alteration experiments. Ge is found to be more volatile than Zn in all experiments. In S‐bearing runs, the loss of Ge and Zn was less than any other experiments. In Cl‐only runs, degassing of Zn was more than twice that of Ge within the first 10 min and percent loss increased for both elements with increasing time. In Cl + S runs, S‐induced reduction of GeO
2
and ZnO to metallic Ge and Zn switches the preference of chloride formation from Zn to Ge. Up to 90% of Ge and Zn loss in the 1‐h no volatile‐added (NVA) experiments might be due to the small amounts of Cl contamination in NVA mixes via other oxides used for synthesis. Alteration experiments show different phases between 1‐h and 24‐/72‐h runs. In 1‐h runs, anhydrite and langbeinite dominate while in 24‐/72‐h runs halite and sylvite dominate the condensate assemblages. S‐bearing phases form as the intermediate products of fumarolic deposition, while chlorides are common when the system is allowed to cool gradually. One‐hour exposure was sufficient to form alteration phases and vapor deposits such as NaCl, KCl, CaSO
4
, and langbeinites on the Martian analog minerals. These salts were identified in Martian meteorites and in situ measurements. Our results provide evidence that volcanic degassing along with fumarolic alteration could be a potential source for the enrichment and varying abundances of Cl, S, Fe, Zn, Ge in Martian surface, as well as a cause for Ge depletion in shergottites.</description><subject>Basalt</subject><subject>Bedrock</subject><subject>Chlorides</subject><subject>Degassing</subject><subject>Experiments</subject><subject>Germanium</subject><subject>Germanium oxides</subject><subject>In situ measurement</subject><subject>Lithium</subject><subject>Mars</subject><subject>Mars craters</subject><subject>Mars surface</subject><subject>Mars volcanoes</subject><subject>Minerals</subject><subject>Outgassing</subject><subject>Phases</subject><subject>SNC meteorites</subject><subject>Sodium chloride</subject><subject>Switches</subject><subject>Sylvite</subject><subject>Trace metals</subject><subject>Vapor deposition</subject><subject>Volcanic activity</subject><subject>Zinc</subject><subject>Zinc oxide</subject><issn>1086-9379</issn><issn>1945-5100</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNotUMtOwzAQtBBIlMKFL7DEDTVlHSdOfERVeUhFXHqPNonTukqcYDuI8if8LQ5lL7OamZ2VhpBbBksW5qHDwS1ZAgBnZMZkkkYpAzgPO-QikjyTl-TKuQMATxlPZuRn_TUoqztlPLa06o3zFrXxjvaG-r2in32LXrfaH2nf0J2yHRo9dgv6rU21oGhqGsR9oKg29A2t12hoiQ7bEDLJU4rtWzXd12qHzmmzm8zBoWwID5-C5EbbYKVop01gW3dNLpoA6uYf52T7tN6uXqLN-_Pr6nETYZxlPiolRynyuI6lwExlECeQx7IUtRCQZFIkSamavKrihKepSrFhgNgA47VEqPic3J1iB9t_jMr54tCP1oSPRZyLOM8gz_Lguj-5Kts7Z1VTDKE0tMeCQTE1X0zNF3_N81-eRXlJ</recordid><startdate>202309</startdate><enddate>202309</enddate><creator>Rogaski, Alexander</creator><creator>Ustunisik, Gokce K.</creator><creator>Yang, Shuying</creator><creator>Humayun, Munir</creator><creator>Righter, Kevin</creator><creator>Berger, Jeff A.</creator><creator>DiFrancesco, Nicholas</creator><general>Wiley Subscription Services, Inc</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-0380-4683</orcidid><orcidid>https://orcid.org/0000-0001-6950-9700</orcidid><orcidid>https://orcid.org/0000-0002-2840-8863</orcidid><orcidid>https://orcid.org/0000-0001-8516-9435</orcidid><orcidid>https://orcid.org/0000-0002-6075-7908</orcidid></search><sort><creationdate>202309</creationdate><title>Experimental constraints on the volatility of germanium, zinc, and lithium in Martian basalts and the role of degassing in alteration of surface minerals</title><author>Rogaski, Alexander ; Ustunisik, Gokce K. ; Yang, Shuying ; Humayun, Munir ; Righter, Kevin ; Berger, Jeff A. ; DiFrancesco, Nicholas</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a277t-b93a9682d296a7e70240829b6d660479644bef8cc24355e5af10aaf013d9a0c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Basalt</topic><topic>Bedrock</topic><topic>Chlorides</topic><topic>Degassing</topic><topic>Experiments</topic><topic>Germanium</topic><topic>Germanium oxides</topic><topic>In situ measurement</topic><topic>Lithium</topic><topic>Mars</topic><topic>Mars craters</topic><topic>Mars surface</topic><topic>Mars volcanoes</topic><topic>Minerals</topic><topic>Outgassing</topic><topic>Phases</topic><topic>SNC meteorites</topic><topic>Sodium chloride</topic><topic>Switches</topic><topic>Sylvite</topic><topic>Trace metals</topic><topic>Vapor deposition</topic><topic>Volcanic activity</topic><topic>Zinc</topic><topic>Zinc oxide</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rogaski, Alexander</creatorcontrib><creatorcontrib>Ustunisik, Gokce K.</creatorcontrib><creatorcontrib>Yang, Shuying</creatorcontrib><creatorcontrib>Humayun, Munir</creatorcontrib><creatorcontrib>Righter, Kevin</creatorcontrib><creatorcontrib>Berger, Jeff A.</creatorcontrib><creatorcontrib>DiFrancesco, Nicholas</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Meteoritics & planetary science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Rogaski, Alexander</au><au>Ustunisik, Gokce K.</au><au>Yang, Shuying</au><au>Humayun, Munir</au><au>Righter, Kevin</au><au>Berger, Jeff A.</au><au>DiFrancesco, Nicholas</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Experimental constraints on the volatility of germanium, zinc, and lithium in Martian basalts and the role of degassing in alteration of surface minerals</atitle><jtitle>Meteoritics & planetary science</jtitle><date>2023-09</date><risdate>2023</risdate><volume>58</volume><issue>9</issue><spage>1183</spage><epage>1210</epage><pages>1183-1210</pages><issn>1086-9379</issn><eissn>1945-5100</eissn><abstract>The surface of Mars is enriched in Cl and S which is linked to volcanic activity and degassing. Similarly, elevated Ge and Zn levels in Gale crater sedimentary bedrock indicate a magmatic source for these elements. To constrain the relative effects of Cl and S on the outgassing of these trace metals and chemical characteristics of primary magmatic vapor deposits incorporated to Martian surface, we conducted a set of degassing and fumarolic alteration experiments. Ge is found to be more volatile than Zn in all experiments. In S‐bearing runs, the loss of Ge and Zn was less than any other experiments. In Cl‐only runs, degassing of Zn was more than twice that of Ge within the first 10 min and percent loss increased for both elements with increasing time. In Cl + S runs, S‐induced reduction of GeO
2
and ZnO to metallic Ge and Zn switches the preference of chloride formation from Zn to Ge. Up to 90% of Ge and Zn loss in the 1‐h no volatile‐added (NVA) experiments might be due to the small amounts of Cl contamination in NVA mixes via other oxides used for synthesis. Alteration experiments show different phases between 1‐h and 24‐/72‐h runs. In 1‐h runs, anhydrite and langbeinite dominate while in 24‐/72‐h runs halite and sylvite dominate the condensate assemblages. S‐bearing phases form as the intermediate products of fumarolic deposition, while chlorides are common when the system is allowed to cool gradually. One‐hour exposure was sufficient to form alteration phases and vapor deposits such as NaCl, KCl, CaSO
4
, and langbeinites on the Martian analog minerals. These salts were identified in Martian meteorites and in situ measurements. Our results provide evidence that volcanic degassing along with fumarolic alteration could be a potential source for the enrichment and varying abundances of Cl, S, Fe, Zn, Ge in Martian surface, as well as a cause for Ge depletion in shergottites.</abstract><cop>Hoboken</cop><pub>Wiley Subscription Services, Inc</pub><doi>10.1111/maps.14000</doi><tpages>28</tpages><orcidid>https://orcid.org/0000-0002-0380-4683</orcidid><orcidid>https://orcid.org/0000-0001-6950-9700</orcidid><orcidid>https://orcid.org/0000-0002-2840-8863</orcidid><orcidid>https://orcid.org/0000-0001-8516-9435</orcidid><orcidid>https://orcid.org/0000-0002-6075-7908</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Basalt Bedrock Chlorides Degassing Experiments Germanium Germanium oxides In situ measurement Lithium Mars Mars craters Mars surface Mars volcanoes Minerals Outgassing Phases SNC meteorites Sodium chloride Switches Sylvite Trace metals Vapor deposition Volcanic activity Zinc Zinc oxide |
title | Experimental constraints on the volatility of germanium, zinc, and lithium in Martian basalts and the role of degassing in alteration of surface minerals |
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