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Geosciences 2018, 8(1), 15; doi:10.3390/geosciences8010015

Oxygen Isotope Thermometry of DaG 476 and SaU 008 Martian Meteorites: Implications for Their Origin

Earth Sciences Research Centre (ESRC), Sultan Qaboos University (SQU), Al-Khodh, Muscat 123, Oman
Department of Earth Sciences, Western University, 1151 Richmond Street N., London, ON N6A 5B7, Canada
Author to whom correspondence should be addressed.
Received: 2 July 2017 / Revised: 3 January 2018 / Accepted: 4 January 2018 / Published: 8 January 2018
(This article belongs to the Special Issue Martian Meteorites)
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We report the equilibration temperatures derived from the oxygen isotope thermometry of pyroxene-olivine pair from the Dar al Ghani (DaG) 476 (1200 +105/−90 °C) and Sayh al Uhaymir (SaU) 008 (1430 +220/−155 °C) meteorites showing a difference of over 200 °C at the face values. Regardless of the large associated uncertainties, contrasting geochemical and isotopic characteristics such as oxygen fugacities, hydrogen isotopic compositions (referred to as the D/H ratios), olivine abundances, presence of merrillite and/or apatite, and their chlorine contents between the two meteorites are observed in the literature. These opposing features lend support to the idea that the relative difference observed in the estimated temperatures is probably real and significant, thus providing insights into the Martian mantle magmatism. Based on our temperature estimation and previous magmatic models, we propose that SaU 008 could have been originated from a deeper depleted mantle source. However, DaG 476 may have been produced by the partial melting of the entrained pockets of the depleted mantle similar to that of the SaU 008’s source at a relatively shallower depth. Both meteorites erupted as a relatively thick lava flow or a shallow intrusion at approximately the same time followed by a launch initiated by a single meteoritic impact 1.1 million years (Ma) ago. View Full-Text
Keywords: oxygen isotopes; thermometry; Martian magmatism; DaG 476; SaU 008 oxygen isotopes; thermometry; Martian magmatism; DaG 476; SaU 008

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This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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Ali, A.; Jabeen, I.; Nasir, S.J.; Banerjee, N.R. Oxygen Isotope Thermometry of DaG 476 and SaU 008 Martian Meteorites: Implications for Their Origin. Geosciences 2018, 8, 15.

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