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Reassessing the thermal history of martian meteorite Shergotty and Apollo mare basalt 15555 using kinetic isotope fractionation of zoned minerals

Richter, Frank and Saper, Lee M. and Villeneuve, Johan and Chaussidon, Marc and Watson, E. Bruce and Davis, Andrew M. and Mendybaev, Ruslan A. and Simon, Steven B. (2021) Reassessing the thermal history of martian meteorite Shergotty and Apollo mare basalt 15555 using kinetic isotope fractionation of zoned minerals. Geochimica et Cosmochimica Acta, 295 . pp. 265-285. ISSN 0016-7037. https://resolver.caltech.edu/CaltechAUTHORS:20210225-150425007

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Abstract

Elemental abundance and isotopic fractionation profiles across zoned minerals from a martian meteorite (Shergotty) and from a lunar olivine-normative mare basalt (Apollo 15555) were used to place constraints on the thermal evolution of their host rocks. The isotopic measurements were used to determine the extent to which diffusion was responsible for, or modified, the zoning. The key concept is that mineral zoning that is the result of diffusion, or that was significantly affected by diffusion, will have an associated diagnostic isotopic fractionation that can quantify the extent of mass transfer by diffusion. Once the extent of diffusion was determined, the mineral zoning was used to constrain the thermal history. An isotopic and chemical profile measured across a large zoned pigeonite grain from Shergotty showed no significant isotopic fractionation of either magnesium or lithium, which is evidence that the chemical zoning was dominantly the result of crystallization from an evolving melt and that the crystallization must have taken place at a sufficiently fast rate that there was not time for any significant mass transfer by diffusion. Model calculations for the evolution of the fast-diffusing lithium showed that this would have required a cooling at a rate of about ∼150 °C/h or more. Measurable isotopic fractionation across a zoned olivine grain from lunar mare basalt 15555 indicated that the chemical zoning was mainly due to crystallization that was modified by a small but quantifiable amount of diffusion. The results of a diffusion calculation that was able to account for the amplitude and spatial scale of the isotopic fractionation across the olivine grain yielded an estimate of 0.2 °C/h for the cooling rate of 15555. The results of an earlier study of zoned augite and olivine grains from martian nakhlite meteorite NWA 817 were reviewed for comparison with the results from Shergotty. The isotopic fractionations near the edges of grains from NWA 817 showed that, in contrast to Shergotty, the lithium zoning in augite and of magnesium in olivine was due entirely to diffusion. The isotopic fractionation data across zoned minerals from the martian meteorites and from the lunar basalt were key for documenting and quantifying the extent of mass transfer by diffusion, which was a crucial step for validating the use of diffusion modeling to estimate their cooling rates.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1016/j.gca.2020.11.002DOIArticle
ORCID:
AuthorORCID
Saper, Lee M.0000-0002-3995-9986
Additional Information:© 2020 Elsevier Ltd. Received 7 April 2020, Accepted 2 November 2020, Available online 14 November 2020. The work reported here was supported by NASA grants NNX13AH09G S01 (FMR), 80NSSC17K0251 (AMD), NNX16AI26G and NNX17AI43G (SBS), and NNX17AE84G (RAM). Support from Europlanet 2020 Project 16-EPN2-014 (FMR) and Programme National de Planétologie from INSU-CNRS and l'Agence Nationale de la Recherche grant ANR-18-CE31-0010-01 (JV) is also gratefully acknowledged. We thank Yan Liang of Brown University for helping us find the published data we list in Supplementary data 3 and Thomas Stephan of the University of Chicago for implementing the Mahon data analysis algorithm referenced in Supplementary data 2. We also thank three anonymous reviewers and the associate editor for their many suggestions that improved the manuscript. The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Funders:
Funding AgencyGrant Number
NASANNX13AH09G S01
NASA80NSSC17K0251
NASANNX16AI26G
NASANNX17AI43G
NASANNX17AE84G
European Commission16-EPN2-014
Programme National de Planetologie (PNP)UNSPECIFIED
Institut national des sciences de l'Univers (INSU)UNSPECIFIED
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Agence Nationale pour la Recherche (ANR)ANR-18-CE31-0010-01
Subject Keywords:Martian meteorites; Lunar basalt; Zoned minerals; Diffusion; Isotope fractionation; Cooling rates
Record Number:CaltechAUTHORS:20210225-150425007
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210225-150425007
Official Citation:Frank Richter, Lee M. Saper, Johan Villeneuve, Marc Chaussidon, E. Bruce Watson, Andrew M. Davis, Ruslan A. Mendybaev, Steven B. Simon, Reassessing the thermal history of martian meteorite Shergotty and Apollo mare basalt 15555 using kinetic isotope fractionation of zoned minerals, Geochimica et Cosmochimica Acta, Volume 295, 2021, Pages 265-285, ISSN 0016-7037, https://doi.org/10.1016/j.gca.2020.11.002. (https://www.sciencedirect.com/science/article/pii/S0016703720306670)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:108220
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:26 Feb 2021 00:17
Last Modified:26 Feb 2021 00:17

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