T313 Partitioning of Chlorine and Associated Halogens between Minerals, Melts, and Brines
Wednesday, 28 September 2016
1:30 PM - 5:30 PM
Room 205
CONSTRAINTS ON THE HALOGEN CONTENT OF MARTIAN MAGMAS AND DEGASSING OF CHLORINE-RICH FLUIDS
Paper number: T313-5
Program: Technical Sessions
Time: 2:20 PM – 2:40 PM
Authors
Abstract
The bulk chlorine contents of unaltered Martian basalts, as represented by the shergottite meteorites, are similar to depleted terrestrial basalts [3]. However, after taking into account igneous fractionation and partial melting, Martian basalts contain 2.5 (+/- 1) times more chlorine than terrestrial basalts and have a source region more consistent with the enriched terrestrial mantle [2, 3]. Similarly, fluorine in the Martian interior is enriched compared with the bulk terrestrial mantle [3]. Bromine in the Martian interior is less well constrained because of the paucity of data of Br contents of Martian meteorites [3].
Eruption of halogen-rich magmas has been used to explain the chlorine-rich nature of the bulk Martian crust [4] and variations in chlorine at the Home Plate outcrop in Gusev Crater [5]. Degassing of chlorine-rich magmatic fluids is also consistent with the mineralogy of Martian meteorites [6-8]. Martian meteorites contain end member Cl-scapolite marialite and chloro-potassic-hastingsite amphibole, which form from magmatic hydrothermal brines [6, 7].
Refs: [1] Dreibus G. and Wänke H. (1987) Icarus, 71. 225-240. [2] Filiberto J. and Treiman A.H. (2009) Geology, 37. 1087-1090. [3] Filiberto J et al. (2016) MaPS. DOI: 10.1111/maps.12624. [4] Keller J.M. et al. (2006) JGR. 111(E03S08). doi:10.1029/2006JE002679. [5] Schmidt M.E. et al. (2008) JGR. 113(E06S12). doi:10.1029/2007JE003027. [6] Filiberto J. et al. (2014) EPSL. 401. 110-115. [7] Giesting P. and Filiberto J. (2016) MaPS. in press. [8] McCubbin F.M. et al. (2013) MaPS. 48. 819-853.
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-279248
© Copyright 2016 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.