Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate

Cl isotope ratios measured on HCl thermally evolved from as-yet-unknown phases in sedimentary rocks and sand in Gale Crater provide unexpected insights to the Martian surficial Cl cycle. The seven samples yield δ 37 Cl values ranging from −1 ± 25h to −51 ± 5h. Five analyses from two samples of the S...

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Main Authors: K A Farley, P Martin, P D Archer Jr, S K Atreya, P G Conrad, J L Eigenbrode, A G Fairén, H B Franz, C Freissinet, D P Glavin, P R Mahaffy, C Malespin, D W Ming, R Navarro-Gonzalez, B Sutter
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2016
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Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1078.9706
http://www-personal.umich.edu/%7Eatreya/Articles/2016EPSL_Mars_Cl_Isotopes_Farley_etal.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.1078.9706 2023-05-15T18:45:44+02:00 Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate K A Farley P Martin P D Archer Jr S K Atreya P G Conrad J L Eigenbrode A G Fairén H B Franz C Freissinet D P Glavin P R Mahaffy C Malespin D W Ming R Navarro-Gonzalez B Sutter The Pennsylvania State University CiteSeerX Archives 2016 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1078.9706 http://www-personal.umich.edu/%7Eatreya/Articles/2016EPSL_Mars_Cl_Isotopes_Farley_etal.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1078.9706 http://www-personal.umich.edu/%7Eatreya/Articles/2016EPSL_Mars_Cl_Isotopes_Farley_etal.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www-personal.umich.edu/%7Eatreya/Articles/2016EPSL_Mars_Cl_Isotopes_Farley_etal.pdf text 2016 ftciteseerx 2020-05-03T00:19:33Z Cl isotope ratios measured on HCl thermally evolved from as-yet-unknown phases in sedimentary rocks and sand in Gale Crater provide unexpected insights to the Martian surficial Cl cycle. The seven samples yield δ 37 Cl values ranging from −1 ± 25h to −51 ± 5h. Five analyses from two samples of the Sheepbed mudstone (Yellowknife Bay study area) are analytically indistinguishable with a mean δ 37 Cl of −11 ± 7h (1σ ). In contrast, four mudstones/sandstones from the Kimberley and Pahrump study areas also yielded indistinguishable ratios, but with a mean δ 37 Cl of −43 ± 6h. The Rocknest sand deposit gave a highly uncertain δ 37 Cl value of −7 ± 44h. These light and highly variable δ 37 Cl values are unique among known solar system materials. Two endmember models are offered to account for these observations, and in both, perchlorate, with its extreme ability to fractionate Cl isotopes, is critical. In the first model, SAM is detecting HCl from an oxychlorine compound (e.g., perchlorate) produced from volcanic gas emissions by atmospheric chemical reactions. Similar reactions in Earth's atmosphere may be responsible for the isotopically lightest known Cl outside of this study, in perchlorate from the Atacama Desert. Some of the Gale Crater δ 37 Cl values are more negative than those in Atacama perchlorate, but because reaction mechanisms and associated fractionation factors are unknown, it is impossible to assess whether this difference is prohibitive. If the negative δ 37 Cl signal is produced in this fashion, the isotopic variability among samples could arise either from variations in the relative size of the reactant chloride and product perchlorate reservoirs, or from variations in the fraction of perchlorate reduced back to chloride after deposition. Such reduction strongly enriches 37 Cl in the residual perchlorate. Perchlorate reduction alone offers an alternative endmember model that can explain the observed data if SAM measured HCl derived from chloride. In this model isotopically normal perchlorate ... Text Yellowknife Unknown Yellowknife Yellowknife Bay ENVELOPE(-114.336,-114.336,62.367,62.367)
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description Cl isotope ratios measured on HCl thermally evolved from as-yet-unknown phases in sedimentary rocks and sand in Gale Crater provide unexpected insights to the Martian surficial Cl cycle. The seven samples yield δ 37 Cl values ranging from −1 ± 25h to −51 ± 5h. Five analyses from two samples of the Sheepbed mudstone (Yellowknife Bay study area) are analytically indistinguishable with a mean δ 37 Cl of −11 ± 7h (1σ ). In contrast, four mudstones/sandstones from the Kimberley and Pahrump study areas also yielded indistinguishable ratios, but with a mean δ 37 Cl of −43 ± 6h. The Rocknest sand deposit gave a highly uncertain δ 37 Cl value of −7 ± 44h. These light and highly variable δ 37 Cl values are unique among known solar system materials. Two endmember models are offered to account for these observations, and in both, perchlorate, with its extreme ability to fractionate Cl isotopes, is critical. In the first model, SAM is detecting HCl from an oxychlorine compound (e.g., perchlorate) produced from volcanic gas emissions by atmospheric chemical reactions. Similar reactions in Earth's atmosphere may be responsible for the isotopically lightest known Cl outside of this study, in perchlorate from the Atacama Desert. Some of the Gale Crater δ 37 Cl values are more negative than those in Atacama perchlorate, but because reaction mechanisms and associated fractionation factors are unknown, it is impossible to assess whether this difference is prohibitive. If the negative δ 37 Cl signal is produced in this fashion, the isotopic variability among samples could arise either from variations in the relative size of the reactant chloride and product perchlorate reservoirs, or from variations in the fraction of perchlorate reduced back to chloride after deposition. Such reduction strongly enriches 37 Cl in the residual perchlorate. Perchlorate reduction alone offers an alternative endmember model that can explain the observed data if SAM measured HCl derived from chloride. In this model isotopically normal perchlorate ...
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author K A Farley
P Martin
P D Archer Jr
S K Atreya
P G Conrad
J L Eigenbrode
A G Fairén
H B Franz
C Freissinet
D P Glavin
P R Mahaffy
C Malespin
D W Ming
R Navarro-Gonzalez
B Sutter
spellingShingle K A Farley
P Martin
P D Archer Jr
S K Atreya
P G Conrad
J L Eigenbrode
A G Fairén
H B Franz
C Freissinet
D P Glavin
P R Mahaffy
C Malespin
D W Ming
R Navarro-Gonzalez
B Sutter
Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate
author_facet K A Farley
P Martin
P D Archer Jr
S K Atreya
P G Conrad
J L Eigenbrode
A G Fairén
H B Franz
C Freissinet
D P Glavin
P R Mahaffy
C Malespin
D W Ming
R Navarro-Gonzalez
B Sutter
author_sort K A Farley
title Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate
title_short Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate
title_full Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate
title_fullStr Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate
title_full_unstemmed Light and variable 37 Cl/ 35 Cl ratios in rocks from Gale Crater, Mars: Possible signature of perchlorate
title_sort light and variable 37 cl/ 35 cl ratios in rocks from gale crater, mars: possible signature of perchlorate
publishDate 2016
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1078.9706
http://www-personal.umich.edu/%7Eatreya/Articles/2016EPSL_Mars_Cl_Isotopes_Farley_etal.pdf
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op_source http://www-personal.umich.edu/%7Eatreya/Articles/2016EPSL_Mars_Cl_Isotopes_Farley_etal.pdf
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http://www-personal.umich.edu/%7Eatreya/Articles/2016EPSL_Mars_Cl_Isotopes_Farley_etal.pdf
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