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Article Dans Une Revue Geochimica et Cosmochimica Acta Année : 2017

The Northwest Africa 8159 martian meteorite: Expanding the martian sample suite to the early Amazonian

Christopher D. K. Herd
  • Fonction : Auteur
Erin L. Walton
  • Fonction : Auteur
Carl B. Agee
  • Fonction : Auteur
Nele Muttik
  • Fonction : Auteur
Karen Ziegler
  • Fonction : Auteur
Charles K. Shearer
  • Fonction : Auteur
Aaron S. Bell
  • Fonction : Auteur
Alison R. Santos
  • Fonction : Auteur
Paul V. Burger
  • Fonction : Auteur
Justin I. Simon
  • Fonction : Auteur
Michael J. Tappa
  • Fonction : Auteur
Francis M. Mccubbin
  • Fonction : Auteur
France Lagroix
Matthew E. Sanborn
  • Fonction : Auteur
Qing-Zhu Yin
William S. Cassata
  • Fonction : Auteur
Lars E. Borg
  • Fonction : Auteur
Rachel E. Lindvall
  • Fonction : Auteur
Thomas S. Kruijer
  • Fonction : Auteur
Gregory A. Brennecka
  • Fonction : Auteur
Thorsten Kleine
  • Fonction : Auteur
Kunihiko Nishiizumi
  • Fonction : Auteur
Marc W. Caffee
  • Fonction : Auteur

Résumé

Northwest Africa (NWA) 8159 is an augite-rich shergottite, with a mineralogy dominated by Ca-, Fe-rich pyroxene, plagioclase, olivine, and magnetite. NWA 8159 crystallized from an evolved melt of basaltic composition under relatively rapid conditions of cooling, likely in a surface lava flow or shallow sill. Redox conditions experienced by the melt shifted from relatively oxidizing (with respect to known Martian lithologies, similar to QFM) on the liquidus to higher oxygen fugacity (similar to QFM + 2) during crystallization of the groundmass, and under subsolidus conditions. This shift resulted in the production of orthopyroxene and magnetite replacing olivine phenocryst rims. NWA 8159 contains both crystalline and shock-amorphized plagioclase (An(5062)), often observed within a single grain; based on known calibrations we bracket the peak shock pressure experienced by NWA 8159 to between 15 and 23 GPa. The bulk composition of NWA 8159 is depleted in LREE, as observed for Tissint and other depleted shergottites; however, NWA 8159 is distinct from all other martian lithologies in its bulk composition and oxygen fugacity. We obtain a Sm-Nd formation age of 2.37 +/- 0.25 Ga for NWA 8159, which represents an interval in Mars geologic time which, until recently, was not represented in the other martian meteorite types. The bulk rock Sm-147/Nd-144 value of 0.37 +/- 0.02 is consistent with it being derived directly from its source and the high initial epsilon(143)(Nd) value indicates this source was geochemically highly depleted. Cr, Nd, and W isotopic compositions further support a unique mantle source. While the rock shares similarities with the 2.4-Ga NWA 7635 meteorite, there are notable distinctions between the two meteorites that suggest differences in mantle source compositions and conditions of crystallization. Nevertheless, the two samples may be launch-paired. NWA 8159 expands the known basalt types, ages and mantle sources within the Mars sample suite to include a second igneous unit from the early Amazonian.(C) 2017 Elsevier Ltd. All rights reserved.

Dates et versions

hal-01765617 , version 1 (13-04-2018)

Identifiants

Citer

Christopher D. K. Herd, Erin L. Walton, Carl B. Agee, Nele Muttik, Karen Ziegler, et al.. The Northwest Africa 8159 martian meteorite: Expanding the martian sample suite to the early Amazonian. Geochimica et Cosmochimica Acta, 2017, 218, pp.1-26. ⟨10.1016/j.gca.2017.08.037⟩. ⟨hal-01765617⟩
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