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Trace element geochemistry (Li, Ba, Sr, and Rb) using Curiosity's ChemCam: Early results for Gale crater from Bradbury Landing Site to Rocknest

Identifieur interne : 000B05 ( Istex/Corpus ); précédent : 000B04; suivant : 000B06

Trace element geochemistry (Li, Ba, Sr, and Rb) using Curiosity's ChemCam: Early results for Gale crater from Bradbury Landing Site to Rocknest

Auteurs : Ann M. Ollila ; Horton E. Newsom ; Benton Clark Iii ; Roger C. Wiens ; Agnes Cousin ; Jen G. Blank ; Nicolas Mangold ; Violaine Sautter ; Sylvestre Maurice ; Samuel M. Clegg ; Olivier Gasnault ; Olivier Forni ; Robert Tokar ; Eric Lewin ; M. Darby Dyar ; Jeremie Lasue ; Ryan Anderson ; Scott M. Mclennan ; John Bridges ; Dave Vaniman ; Nina Lanza ; Cecile Fabre ; Noureddine Melikechi ; Glynis M. Perrett ; John L. Campbell ; Penelope L. King ; Bruce Barraclough ; Dorothea Delapp ; Stephen Johnstone ; Pierre-Yves Meslin ; Anya Rosen-Gooding ; Josh Williams

Source :

RBID : ISTEX:3B2C589795282C03E2C65C1EED4018972BE73237

Abstract

The ChemCam instrument package on the Mars rover, Curiosity, provides new capabilities to probe the abundances of certain trace elements in the rocks and soils on Mars using the laser‐induced breakdown spectroscopy technique. We focus on detecting and quantifying Li, Ba, Rb, and Sr in targets analyzed during the first 100 sols, from Bradbury Landing Site to Rocknest. Univariate peak area models and multivariate partial least squares models are presented. Li, detected for the first time directly on Mars, is generally low (<15 ppm). The lack of soil enrichment in Li, which is highly fluid mobile, is consistent with limited influx of subsurface waters contributing to the upper soils. Localized enrichments of up to ~60 ppm Li have been observed in several rocks but the host mineral for Li is unclear. Bathurst_Inlet is a fine‐grained bedrock unit in which several analysis locations show a decrease in Li and other alkalis with depth, which may imply that the unit has undergone low‐level aqueous alteration that has preferentially drawn the alkalis to the surface. Ba (~1000 ppm) was detected in a buried pebble in the Akaitcho sand ripple and it appears to correlate with Si, Al, Na, and K, indicating a possible feldspathic composition. Rb and Sr are in the conglomerate Link at abundances >100 ppm and >1000 ppm, respectively. These analysis locations tend to have high Si and alkali abundances, consistent with a feldspar composition. Together, these trace element observations provide possible evidence of magma differentiation and aqueous alteration.

Url:
DOI: 10.1002/2013JE004517

Links to Exploration step

ISTEX:3B2C589795282C03E2C65C1EED4018972BE73237

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<name sortKey="Clegg, Samuel M" sort="Clegg, Samuel M" uniqKey="Clegg S" first="Samuel M." last="Clegg">Samuel M. Clegg</name>
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<name sortKey="Tokar, Robert" sort="Tokar, Robert" uniqKey="Tokar R" first="Robert" last="Tokar">Robert Tokar</name>
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<name sortKey="Lewin, Eric" sort="Lewin, Eric" uniqKey="Lewin E" first="Eric" last="Lewin">Eric Lewin</name>
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<name sortKey="Dyar, M Darby" sort="Dyar, M Darby" uniqKey="Dyar M" first="M. Darby" last="Dyar">M. Darby Dyar</name>
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<name sortKey="Lasue, Jeremie" sort="Lasue, Jeremie" uniqKey="Lasue J" first="Jeremie" last="Lasue">Jeremie Lasue</name>
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<name sortKey="Anderson, Ryan" sort="Anderson, Ryan" uniqKey="Anderson R" first="Ryan" last="Anderson">Ryan Anderson</name>
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<name sortKey="Mclennan, Scott M" sort="Mclennan, Scott M" uniqKey="Mclennan S" first="Scott M." last="Mclennan">Scott M. Mclennan</name>
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<name sortKey="Bridges, John" sort="Bridges, John" uniqKey="Bridges J" first="John" last="Bridges">John Bridges</name>
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<name sortKey="Vaniman, Dave" sort="Vaniman, Dave" uniqKey="Vaniman D" first="Dave" last="Vaniman">Dave Vaniman</name>
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<name sortKey="Lanza, Nina" sort="Lanza, Nina" uniqKey="Lanza N" first="Nina" last="Lanza">Nina Lanza</name>
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<name sortKey="Fabre, Cecile" sort="Fabre, Cecile" uniqKey="Fabre C" first="Cecile" last="Fabre">Cecile Fabre</name>
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<name sortKey="Melikechi, Noureddine" sort="Melikechi, Noureddine" uniqKey="Melikechi N" first="Noureddine" last="Melikechi">Noureddine Melikechi</name>
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<mods:affiliation>Optical Science Center for Applied Research, Delaware State University, Delaware, Dover, USA</mods:affiliation>
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<name sortKey="Perrett, Glynis M" sort="Perrett, Glynis M" uniqKey="Perrett G" first="Glynis M." last="Perrett">Glynis M. Perrett</name>
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<mods:affiliation>Department of Physics, University of Guelph, Ontario, Guelph, Canada</mods:affiliation>
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<name sortKey="Campbell, John L" sort="Campbell, John L" uniqKey="Campbell J" first="John L." last="Campbell">John L. Campbell</name>
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<mods:affiliation>Department of Physics, University of Guelph, Ontario, Guelph, Canada</mods:affiliation>
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<name sortKey="King, Penelope L" sort="King, Penelope L" uniqKey="King P" first="Penelope L." last="King">Penelope L. King</name>
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<mods:affiliation>Research School of Earth Sciences, Australian National University, ACT, Canberra, Australia</mods:affiliation>
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<name sortKey="Barraclough, Bruce" sort="Barraclough, Bruce" uniqKey="Barraclough B" first="Bruce" last="Barraclough">Bruce Barraclough</name>
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<mods:affiliation>Planetary Science Institute, Arizona, Tucson, USA</mods:affiliation>
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<name sortKey="Delapp, Dorothea" sort="Delapp, Dorothea" uniqKey="Delapp D" first="Dorothea" last="Delapp">Dorothea Delapp</name>
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<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
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<name sortKey="Johnstone, Stephen" sort="Johnstone, Stephen" uniqKey="Johnstone S" first="Stephen" last="Johnstone">Stephen Johnstone</name>
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<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
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<name sortKey="Meslin, Pierre Ves" sort="Meslin, Pierre Ves" uniqKey="Meslin P" first="Pierre-Yves" last="Meslin">Pierre-Yves Meslin</name>
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<mods:affiliation>Institut de Recherche en Astrophysique et Planétologie, Université Paul Sabatier, Toulouse, France</mods:affiliation>
</affiliation>
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<author>
<name sortKey="Rosen Ooding, Anya" sort="Rosen Ooding, Anya" uniqKey="Rosen Ooding A" first="Anya" last="Rosen-Gooding">Anya Rosen-Gooding</name>
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<mods:affiliation>Albuquerque Academy, Albuquerque, New Mexico, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Williams, Josh" sort="Williams, Josh" uniqKey="Williams J" first="Josh" last="Williams">Josh Williams</name>
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<mods:affiliation>Institute of Meteoritics, Department of Earth and Planetary Sciences, New Mexico, Albuquerque, USA</mods:affiliation>
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<title level="a" type="main">Trace element geochemistry (Li, Ba, Sr, and Rb) using
<hi rend="italic">Curiosity</hi>
's ChemCam: Early results for Gale crater from Bradbury Landing Site to Rocknest</title>
<author>
<name sortKey="Ollila, Ann M" sort="Ollila, Ann M" uniqKey="Ollila A" first="Ann M." last="Ollila">Ann M. Ollila</name>
<affiliation>
<mods:affiliation>Institute of Meteoritics, Department of Earth and Planetary Sciences, New Mexico, Albuquerque, USA</mods:affiliation>
</affiliation>
<affiliation>
<mods:affiliation>E-mail: aollila@unm.edu</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Newsom, Horton E" sort="Newsom, Horton E" uniqKey="Newsom H" first="Horton E." last="Newsom">Horton E. Newsom</name>
<affiliation>
<mods:affiliation>Institute of Meteoritics, Department of Earth and Planetary Sciences, New Mexico, Albuquerque, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Clark Iii, Benton" sort="Clark Iii, Benton" uniqKey="Clark Iii B" first="Benton" last="Clark Iii">Benton Clark Iii</name>
<affiliation>
<mods:affiliation>Space Science Institute, Colorado, Boulder, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Wiens, Roger C" sort="Wiens, Roger C" uniqKey="Wiens R" first="Roger C." last="Wiens">Roger C. Wiens</name>
<affiliation>
<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Cousin, Agnes" sort="Cousin, Agnes" uniqKey="Cousin A" first="Agnes" last="Cousin">Agnes Cousin</name>
<affiliation>
<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Blank, Jen G" sort="Blank, Jen G" uniqKey="Blank J" first="Jen G." last="Blank">Jen G. Blank</name>
<affiliation>
<mods:affiliation>NASA Ames Research Center, California, Moffett Field, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Mangold, Nicolas" sort="Mangold, Nicolas" uniqKey="Mangold N" first="Nicolas" last="Mangold">Nicolas Mangold</name>
<affiliation>
<mods:affiliation>LPGN, CNRS, UMR6112, Université Nantes, Nantes, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Sautter, Violaine" sort="Sautter, Violaine" uniqKey="Sautter V" first="Violaine" last="Sautter">Violaine Sautter</name>
<affiliation>
<mods:affiliation>Laboratoire de Minéralogie et Cosmochimie du Muséum, Muséum National d'Histoire Naturelle, Paris, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Maurice, Sylvestre" sort="Maurice, Sylvestre" uniqKey="Maurice S" first="Sylvestre" last="Maurice">Sylvestre Maurice</name>
<affiliation>
<mods:affiliation>Institut de Recherche en Astrophysique et Planétologie, Université Paul Sabatier, Toulouse, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Clegg, Samuel M" sort="Clegg, Samuel M" uniqKey="Clegg S" first="Samuel M." last="Clegg">Samuel M. Clegg</name>
<affiliation>
<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Gasnault, Olivier" sort="Gasnault, Olivier" uniqKey="Gasnault O" first="Olivier" last="Gasnault">Olivier Gasnault</name>
<affiliation>
<mods:affiliation>Institut de Recherche en Astrophysique et Planétologie, Université Paul Sabatier, Toulouse, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Forni, Olivier" sort="Forni, Olivier" uniqKey="Forni O" first="Olivier" last="Forni">Olivier Forni</name>
<affiliation>
<mods:affiliation>Institut de Recherche en Astrophysique et Planétologie, Université Paul Sabatier, Toulouse, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Tokar, Robert" sort="Tokar, Robert" uniqKey="Tokar R" first="Robert" last="Tokar">Robert Tokar</name>
<affiliation>
<mods:affiliation>Planetary Science Institute, Arizona, Tucson, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Lewin, Eric" sort="Lewin, Eric" uniqKey="Lewin E" first="Eric" last="Lewin">Eric Lewin</name>
<affiliation>
<mods:affiliation>ISTerre, Grenoble, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Dyar, M Darby" sort="Dyar, M Darby" uniqKey="Dyar M" first="M. Darby" last="Dyar">M. Darby Dyar</name>
<affiliation>
<mods:affiliation>Department of Astronomy, Mount Holyoke College, Massachusetts, South Hadley, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Lasue, Jeremie" sort="Lasue, Jeremie" uniqKey="Lasue J" first="Jeremie" last="Lasue">Jeremie Lasue</name>
<affiliation>
<mods:affiliation>Institut de Recherche en Astrophysique et Planétologie, Université Paul Sabatier, Toulouse, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Anderson, Ryan" sort="Anderson, Ryan" uniqKey="Anderson R" first="Ryan" last="Anderson">Ryan Anderson</name>
<affiliation>
<mods:affiliation>Astrogeology Science Center, U.S. Geological Survey, Arizona, Flagstaff, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Mclennan, Scott M" sort="Mclennan, Scott M" uniqKey="Mclennan S" first="Scott M." last="Mclennan">Scott M. Mclennan</name>
<affiliation>
<mods:affiliation>Department of Geosciences, State University of New York at Stony Brook, New York, Stony Brook, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Bridges, John" sort="Bridges, John" uniqKey="Bridges J" first="John" last="Bridges">John Bridges</name>
<affiliation>
<mods:affiliation>Space Research Centre, Department of Physics and Astronomy, University of Leicester, Leicester, UK</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Vaniman, Dave" sort="Vaniman, Dave" uniqKey="Vaniman D" first="Dave" last="Vaniman">Dave Vaniman</name>
<affiliation>
<mods:affiliation>Planetary Science Institute, Arizona, Tucson, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Lanza, Nina" sort="Lanza, Nina" uniqKey="Lanza N" first="Nina" last="Lanza">Nina Lanza</name>
<affiliation>
<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Fabre, Cecile" sort="Fabre, Cecile" uniqKey="Fabre C" first="Cecile" last="Fabre">Cecile Fabre</name>
<affiliation>
<mods:affiliation>GeoResources, CNRS, UMR7356, Université de Lorraine, Vandoeuvre lès Nancy, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Melikechi, Noureddine" sort="Melikechi, Noureddine" uniqKey="Melikechi N" first="Noureddine" last="Melikechi">Noureddine Melikechi</name>
<affiliation>
<mods:affiliation>Optical Science Center for Applied Research, Delaware State University, Delaware, Dover, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Perrett, Glynis M" sort="Perrett, Glynis M" uniqKey="Perrett G" first="Glynis M." last="Perrett">Glynis M. Perrett</name>
<affiliation>
<mods:affiliation>Department of Physics, University of Guelph, Ontario, Guelph, Canada</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Campbell, John L" sort="Campbell, John L" uniqKey="Campbell J" first="John L." last="Campbell">John L. Campbell</name>
<affiliation>
<mods:affiliation>Department of Physics, University of Guelph, Ontario, Guelph, Canada</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="King, Penelope L" sort="King, Penelope L" uniqKey="King P" first="Penelope L." last="King">Penelope L. King</name>
<affiliation>
<mods:affiliation>Department of Physics, University of Guelph, Guelph, Ontario, Canada</mods:affiliation>
</affiliation>
<affiliation>
<mods:affiliation>Research School of Earth Sciences, Australian National University, ACT, Canberra, Australia</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Barraclough, Bruce" sort="Barraclough, Bruce" uniqKey="Barraclough B" first="Bruce" last="Barraclough">Bruce Barraclough</name>
<affiliation>
<mods:affiliation>Planetary Science Institute, Arizona, Tucson, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Delapp, Dorothea" sort="Delapp, Dorothea" uniqKey="Delapp D" first="Dorothea" last="Delapp">Dorothea Delapp</name>
<affiliation>
<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Johnstone, Stephen" sort="Johnstone, Stephen" uniqKey="Johnstone S" first="Stephen" last="Johnstone">Stephen Johnstone</name>
<affiliation>
<mods:affiliation>Los Alamos National Laboratory, New Mexico, Los Alamos, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Meslin, Pierre Ves" sort="Meslin, Pierre Ves" uniqKey="Meslin P" first="Pierre-Yves" last="Meslin">Pierre-Yves Meslin</name>
<affiliation>
<mods:affiliation>Institut de Recherche en Astrophysique et Planétologie, Université Paul Sabatier, Toulouse, France</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Rosen Ooding, Anya" sort="Rosen Ooding, Anya" uniqKey="Rosen Ooding A" first="Anya" last="Rosen-Gooding">Anya Rosen-Gooding</name>
<affiliation>
<mods:affiliation>Albuquerque Academy, Albuquerque, New Mexico, USA</mods:affiliation>
</affiliation>
</author>
<author>
<name sortKey="Williams, Josh" sort="Williams, Josh" uniqKey="Williams J" first="Josh" last="Williams">Josh Williams</name>
<affiliation>
<mods:affiliation>Institute of Meteoritics, Department of Earth and Planetary Sciences, New Mexico, Albuquerque, USA</mods:affiliation>
</affiliation>
</author>
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<div type="abstract">The ChemCam instrument package on the Mars rover, Curiosity, provides new capabilities to probe the abundances of certain trace elements in the rocks and soils on Mars using the laser‐induced breakdown spectroscopy technique. We focus on detecting and quantifying Li, Ba, Rb, and Sr in targets analyzed during the first 100 sols, from Bradbury Landing Site to Rocknest. Univariate peak area models and multivariate partial least squares models are presented. Li, detected for the first time directly on Mars, is generally low (<15 ppm). The lack of soil enrichment in Li, which is highly fluid mobile, is consistent with limited influx of subsurface waters contributing to the upper soils. Localized enrichments of up to ~60 ppm Li have been observed in several rocks but the host mineral for Li is unclear. Bathurst_Inlet is a fine‐grained bedrock unit in which several analysis locations show a decrease in Li and other alkalis with depth, which may imply that the unit has undergone low‐level aqueous alteration that has preferentially drawn the alkalis to the surface. Ba (~1000 ppm) was detected in a buried pebble in the Akaitcho sand ripple and it appears to correlate with Si, Al, Na, and K, indicating a possible feldspathic composition. Rb and Sr are in the conglomerate Link at abundances >100 ppm and >1000 ppm, respectively. These analysis locations tend to have high Si and alkali abundances, consistent with a feldspar composition. Together, these trace element observations provide possible evidence of magma differentiation and aqueous alteration.</div>
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<region>Arizona</region>
<country key="US">USA</country>
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<author xml:id="author-0020">
<persName>
<forename type="first">Nina</forename>
<surname>Lanza</surname>
</persName>
<affiliation>
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<address>
<settlement type="city">Los Alamos</settlement>
<region>New Mexico</region>
<country key="US">USA</country>
</address>
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<forename type="first">Cecile</forename>
<surname>Fabre</surname>
</persName>
<affiliation>
<orgName>GeoResources, CNRS, UMR7356</orgName>
<orgName>Université de Lorraine</orgName>
<address>
<settlement type="city">Vandoeuvre lès Nancy</settlement>
<country key="FR">France</country>
</address>
</affiliation>
</author>
<author xml:id="author-0022">
<persName>
<forename type="first">Noureddine</forename>
<surname>Melikechi</surname>
</persName>
<affiliation>
<orgName>Optical Science Center for Applied Research</orgName>
<orgName>Delaware State University</orgName>
<address>
<settlement type="city">Dover</settlement>
<region>Delaware</region>
<country key="US">USA</country>
</address>
</affiliation>
</author>
<author xml:id="author-0023">
<persName>
<forename type="first">Glynis M.</forename>
<surname>Perrett</surname>
</persName>
<affiliation>
<orgName>Department of Physics</orgName>
<orgName>University of Guelph</orgName>
<address>
<settlement type="city">Guelph</settlement>
<region>Ontario</region>
<country key="CA">Canada</country>
</address>
</affiliation>
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<author xml:id="author-0024">
<persName>
<forename type="first">John L.</forename>
<surname>Campbell</surname>
</persName>
<affiliation>
<orgName>Department of Physics</orgName>
<orgName>University of Guelph</orgName>
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<settlement type="city">Guelph</settlement>
<region>Ontario</region>
<country key="CA">Canada</country>
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<persName>
<forename type="first">Penelope L.</forename>
<surname>King</surname>
</persName>
<affiliation>
<orgName>Department of Physics</orgName>
<orgName>University of Guelph</orgName>
<address>
<settlement type="city">Guelph</settlement>
<region>Ontario</region>
<country key="CA">Canada</country>
</address>
</affiliation>
<affiliation>
<orgName>Research School of Earth Sciences</orgName>
<orgName>Australian National University</orgName>
<address>
<settlement type="city">Canberra</settlement>
<region>ACT</region>
<country key="AU">Australia</country>
</address>
</affiliation>
</author>
<author xml:id="author-0026">
<persName>
<forename type="first">Bruce</forename>
<surname>Barraclough</surname>
</persName>
<affiliation>
<orgName>Planetary Science Institute</orgName>
<address>
<settlement type="city">Tucson</settlement>
<region>Arizona</region>
<country key="US">USA</country>
</address>
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<forename type="first">Dorothea</forename>
<surname>Delapp</surname>
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<orgName>Los Alamos National Laboratory</orgName>
<address>
<settlement type="city">Los Alamos</settlement>
<region>New Mexico</region>
<country key="US">USA</country>
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<forename type="first">Stephen</forename>
<surname>Johnstone</surname>
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<orgName>Los Alamos National Laboratory</orgName>
<address>
<settlement type="city">Los Alamos</settlement>
<region>New Mexico</region>
<country key="US">USA</country>
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<persName>
<forename type="first">Pierre‐Yves</forename>
<surname>Meslin</surname>
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<affiliation>
<orgName>Institut de Recherche en Astrophysique et Planétologie</orgName>
<orgName>Université Paul Sabatier</orgName>
<address>
<settlement type="city">Toulouse</settlement>
<country key="FR">France</country>
</address>
</affiliation>
</author>
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<persName>
<forename type="first">Anya</forename>
<surname>Rosen‐Gooding</surname>
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<affiliation>
<orgName>Albuquerque Academy</orgName>
<address>
<settlement type="city">Albuquerque</settlement>
<country key="US">New Mexico, USA</country>
</address>
</affiliation>
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<persName>
<forename type="first">Josh</forename>
<surname>Williams</surname>
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<affiliation>
<orgName>Institute of Meteoritics</orgName>
<orgName>Department of Earth and Planetary Sciences</orgName>
<address>
<settlement type="city">Albuquerque</settlement>
<region>New Mexico</region>
<country key="US">USA</country>
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<title level="j" type="alt">JOURNAL OF GEOPHYSICAL RESEARCH: PLANETS</title>
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<p>The ChemCam instrument package on the Mars rover,
<hi rend="italic">Curiosity</hi>
, provides new capabilities to probe the abundances of certain trace elements in the rocks and soils on Mars using the laser‐induced breakdown spectroscopy technique. We focus on detecting and quantifying Li, Ba, Rb, and Sr in targets analyzed during the first 100 sols, from Bradbury Landing Site to Rocknest. Univariate peak area models and multivariate partial least squares models are presented. Li, detected for the first time directly on Mars, is generally low (<15 ppm). The lack of soil enrichment in Li, which is highly fluid mobile, is consistent with limited influx of subsurface waters contributing to the upper soils. Localized enrichments of up to ~60 ppm Li have been observed in several rocks but the host mineral for Li is unclear. Bathurst_Inlet is a fine‐grained bedrock unit in which several analysis locations show a decrease in Li and other alkalis with depth, which may imply that the unit has undergone low‐level aqueous alteration that has preferentially drawn the alkalis to the surface. Ba (~1000 ppm) was detected in a buried pebble in the Akaitcho sand ripple and it appears to correlate with Si, Al, Na, and K, indicating a possible feldspathic composition. Rb and Sr are in the conglomerate Link at abundances >100 ppm and >1000 ppm, respectively. These analysis locations tend to have high Si and alkali abundances, consistent with a feldspar composition. Together, these trace element observations provide possible evidence of magma differentiation and aqueous alteration.</p>
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<head>Key Points</head>
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<list xml:id="jgre20193-list-0001" style="bulleted">
<item>Quantitative models for Li, Ba, Rb and Sr using ChemCam data are presented</item>
<item>Abundances for the first 100 sols in Gale crater are discussed</item>
<item>These results represent the first in situ measurements of Li and Ba on Mars</item>
</list>
</p>
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<term xml:id="jgre20193-kwd-0001">laser‐induced breakdown spectroscopy</term>
<term xml:id="jgre20193-kwd-0002">Mars</term>
<term xml:id="jgre20193-kwd-0003">Gale crater</term>
<term xml:id="jgre20193-kwd-0004">trace elements</term>
<term xml:id="jgre20193-kwd-0005">ChemCam</term>
<term xml:id="jgre20193-kwd-0006">Mars Science Laboratory</term>
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<classCode scheme="http://psi.agu.org/specialSection/MSLMISSION1">Results from the first 360 sols of the Mars Science Laboratory Mission: Bradbury Landing through Yellowknife Bay</classCode>
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<copyright>©2014. American Geophysical Union. All Rights Reserved.</copyright>
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<copyright ownership="publisher">©2013. American Geophysical Union. All Rights Reserved.</copyright>
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<correspondenceTo>Corresponding author: A. M. Ollila, Institute of Meteoritics, Department of Earth and Planetary Sciences, 1 University of New Mexico, MSC03‐2050, Albuquerque, NM 87131‐0001, USA. (
<email>aollila@unm.edu</email>
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<subject href="http://psi.agu.org/specialSection/MSLMISSION1">Results from the first 360 sols of the Mars Science Laboratory Mission: Bradbury Landing through Yellowknife Bay</subject>
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<subject href="http://psi.agu.org/taxonomy5/0694">Instruments and techniques</subject>
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<subject href="http://psi.agu.org/taxonomy5/1027">Composition of the planets</subject>
<subject href="http://psi.agu.org/taxonomy5/1065">Major and trace element geochemistry</subject>
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<title type="shortAuthors">OLLILA ET AL.</title>
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<abstract>The ChemCam instrument package on the Mars rover, Curiosity, provides new capabilities to probe the abundances of certain trace elements in the rocks and soils on Mars using the laser‐induced breakdown spectroscopy technique. We focus on detecting and quantifying Li, Ba, Rb, and Sr in targets analyzed during the first 100 sols, from Bradbury Landing Site to Rocknest. Univariate peak area models and multivariate partial least squares models are presented. Li, detected for the first time directly on Mars, is generally low (<15 ppm). The lack of soil enrichment in Li, which is highly fluid mobile, is consistent with limited influx of subsurface waters contributing to the upper soils. Localized enrichments of up to ~60 ppm Li have been observed in several rocks but the host mineral for Li is unclear. Bathurst_Inlet is a fine‐grained bedrock unit in which several analysis locations show a decrease in Li and other alkalis with depth, which may imply that the unit has undergone low‐level aqueous alteration that has preferentially drawn the alkalis to the surface. Ba (~1000 ppm) was detected in a buried pebble in the Akaitcho sand ripple and it appears to correlate with Si, Al, Na, and K, indicating a possible feldspathic composition. Rb and Sr are in the conglomerate Link at abundances >100 ppm and >1000 ppm, respectively. These analysis locations tend to have high Si and alkali abundances, consistent with a feldspar composition. Together, these trace element observations provide possible evidence of magma differentiation and aqueous alteration.</abstract>
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