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Deciphering Redox State for a Metal-Rich World

The Psyche mission’s Oxidation-Reduction Working Group is focused on understanding, determining, and applying the redox state of (16) Psyche to understand the origin of a metal-rich world. The oxidation-reduction state of an asteroid, along with its temperature, parent body size, and composition, is...

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Autores principales: McCoy, Timothy J., Dibb, Steven D., Peplowski, Patrick N., Maurel, Clara, Bercovici, Hannah L., Corrigan, Catherine M., Bell, James F., Weiss, Benjamin P., Lawrence, David J., Wenkert, Daniel D., Prettyman, Thomas H., Elkins-Tanton, Lindy T.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8942946/
https://www.ncbi.nlm.nih.gov/pubmed/35400764
http://dx.doi.org/10.1007/s11214-022-00872-9
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author McCoy, Timothy J.
Dibb, Steven D.
Peplowski, Patrick N.
Maurel, Clara
Bercovici, Hannah L.
Corrigan, Catherine M.
Bell, James F.
Weiss, Benjamin P.
Lawrence, David J.
Wenkert, Daniel D.
Prettyman, Thomas H.
Elkins-Tanton, Lindy T.
author_facet McCoy, Timothy J.
Dibb, Steven D.
Peplowski, Patrick N.
Maurel, Clara
Bercovici, Hannah L.
Corrigan, Catherine M.
Bell, James F.
Weiss, Benjamin P.
Lawrence, David J.
Wenkert, Daniel D.
Prettyman, Thomas H.
Elkins-Tanton, Lindy T.
author_sort McCoy, Timothy J.
collection PubMed
description The Psyche mission’s Oxidation-Reduction Working Group is focused on understanding, determining, and applying the redox state of (16) Psyche to understand the origin of a metal-rich world. The oxidation-reduction state of an asteroid, along with its temperature, parent body size, and composition, is a key parameter in determining the history of an asteroid. Determining the redox state from spacecraft data is most easily done by examining potential metal-oxide buffer pairs. The occurrence of Ni, Fe, C, Cr, P and Si, in that order, in the metal or sulfide phase of an asteroidal body indicates increasingly reduced conditions. Key observations by the Imager and Gamma-Ray and Neutron Spectrometer (GRNS) of Psyche can bracket the redox state using metal-oxide buffers. The presence of Fe,Ni metal can be confirmed by the ratios of Fe/O or Fe/Si and the concentration of Ni variability in metal across the asteroid can be determined by GRNS. The FeO concentration of silicates is complementary to the Ni concentration of metal and can be constrained using filters on the Imager. The presence of FeO in silicates from ground-based observations is one of the few measurements we already have of redox state, although available data permit a wide range of silicate compositions and mineralogies. The presence of C, P or Si concentrated in the metallic, Fe-rich portion of the asteroid, as measured by GRNS, or Ca-sulfide, determined by imaging, would indicate increasingly reducing conditions. Linkage to known types of meteorites, whether metal-rich chondrites, stony-irons or irons, expands the mineralogical, chemical and isotopic data not available from remote observations alone. Redox also controls both silicate and metal mineralogy, influencing differentiation, solidification, and subsolidus cooling, including the relative abundance of sulfur in the core and possible magnetic signatures. The redox state of Psyche, if a fully-differentiated metallic core, might constrain the location and timing of both the formation of Psyche and any oxidation it might have experienced.
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spelling pubmed-89429462022-04-07 Deciphering Redox State for a Metal-Rich World McCoy, Timothy J. Dibb, Steven D. Peplowski, Patrick N. Maurel, Clara Bercovici, Hannah L. Corrigan, Catherine M. Bell, James F. Weiss, Benjamin P. Lawrence, David J. Wenkert, Daniel D. Prettyman, Thomas H. Elkins-Tanton, Lindy T. Space Sci Rev Article The Psyche mission’s Oxidation-Reduction Working Group is focused on understanding, determining, and applying the redox state of (16) Psyche to understand the origin of a metal-rich world. The oxidation-reduction state of an asteroid, along with its temperature, parent body size, and composition, is a key parameter in determining the history of an asteroid. Determining the redox state from spacecraft data is most easily done by examining potential metal-oxide buffer pairs. The occurrence of Ni, Fe, C, Cr, P and Si, in that order, in the metal or sulfide phase of an asteroidal body indicates increasingly reduced conditions. Key observations by the Imager and Gamma-Ray and Neutron Spectrometer (GRNS) of Psyche can bracket the redox state using metal-oxide buffers. The presence of Fe,Ni metal can be confirmed by the ratios of Fe/O or Fe/Si and the concentration of Ni variability in metal across the asteroid can be determined by GRNS. The FeO concentration of silicates is complementary to the Ni concentration of metal and can be constrained using filters on the Imager. The presence of FeO in silicates from ground-based observations is one of the few measurements we already have of redox state, although available data permit a wide range of silicate compositions and mineralogies. The presence of C, P or Si concentrated in the metallic, Fe-rich portion of the asteroid, as measured by GRNS, or Ca-sulfide, determined by imaging, would indicate increasingly reducing conditions. Linkage to known types of meteorites, whether metal-rich chondrites, stony-irons or irons, expands the mineralogical, chemical and isotopic data not available from remote observations alone. Redox also controls both silicate and metal mineralogy, influencing differentiation, solidification, and subsolidus cooling, including the relative abundance of sulfur in the core and possible magnetic signatures. The redox state of Psyche, if a fully-differentiated metallic core, might constrain the location and timing of both the formation of Psyche and any oxidation it might have experienced. Springer Netherlands 2022-03-01 2022 /pmc/articles/PMC8942946/ /pubmed/35400764 http://dx.doi.org/10.1007/s11214-022-00872-9 Text en © This is a U.S. Government work and not under copyright protection in the US; foreign copyright protection may apply 2022, corrected publication 2022 https://creativecommons.org/licenses/by/4.0/Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) .
spellingShingle Article
McCoy, Timothy J.
Dibb, Steven D.
Peplowski, Patrick N.
Maurel, Clara
Bercovici, Hannah L.
Corrigan, Catherine M.
Bell, James F.
Weiss, Benjamin P.
Lawrence, David J.
Wenkert, Daniel D.
Prettyman, Thomas H.
Elkins-Tanton, Lindy T.
Deciphering Redox State for a Metal-Rich World
title Deciphering Redox State for a Metal-Rich World
title_full Deciphering Redox State for a Metal-Rich World
title_fullStr Deciphering Redox State for a Metal-Rich World
title_full_unstemmed Deciphering Redox State for a Metal-Rich World
title_short Deciphering Redox State for a Metal-Rich World
title_sort deciphering redox state for a metal-rich world
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8942946/
https://www.ncbi.nlm.nih.gov/pubmed/35400764
http://dx.doi.org/10.1007/s11214-022-00872-9
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