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Insights into the Martian Regolith from Martian Meteorite Northwest Africa 7034Everything we know about sedimentary processes on Mars is gleaned from remote sensing observations. Here we report insights from meteorite Northwest Africa (NWA) 7034, which is a water-rich martian regolith breccia that hosts both igneous and sedimentary clasts. The sedimentary clasts in NWA 7034 are poorly-sorted clastic siltstones that we refer to as protobreccia clasts. These protobreccia clasts record aqueous alteration process that occurred prior to breccia formation. The aqueous alteration appears to have occurred at relatively low Eh, high pH conditions based on the co-precipitation of pyrite and magnetite, and the concomitant loss of SiO2 from the system. To determine the origin of the NWA 7034 breccia, we examined the textures and grain-shape characteristics of NWA 7034 clasts. The shapes of the clasts are consistent with rock fragmentation in the absence of transport. Coupled with the clast size distribution, we interpret the protolith of NWA 7034 to have been deposited by atmospheric rainout resulting from pyroclastic eruptions and/or asteroid impacts. Cross-cutting and inclusion relationships and U-Pb data from zircon, baddelleyite, and apatite indicate NWA 7034 lithification occurred at 1.4-1.5 Ga, during a short-lived hydrothermal event at 600-700 C that was texturally imprinted upon the submicron groundmass. The hydrothermal event caused Pb-loss from apatite and U-rich metamict zircons, and it caused partial transformation of pyrite to submicron mixtures of magnetite and maghemite, indicating the fluid had higher Eh than the fluid that caused pyrite-magnetite precipitation in the protobreccia clasts. NWA 7034 also hosts ancient 4.4 Ga crustal materials in the form of baddelleyites and zircons, providing up to a 2.9 Ga record of martian geologic history. This work demonstrates the incredible value of sedimentary basins as scientific targets for Mars sample return missions, but it also highlights the importance of targeting samples that have not been overprinted by metamorphic processes, which is the case for NWA 7034.
Document ID
20150019454
Acquisition Source
Johnson Space Center
Document Type
Abstract
Authors
McCubbin, Francis M.
(NASA Johnson Space Center Houston, TX, United States)
Boyce, Jeremy W.
(California Univ. Los Angeles, CA, United States)
Szabo, Timea
(Budapest Univ. of Technology and Economics Budapest, Hungary)
Santos, Alison R.
(New Mexico Univ. Albuquerque, NM, United States)
Domokos, Gabor
(Budapest Univ. of Technology and Economics Budapest, Hungary)
Vazquez, Jorge
(Geological Survey Menlo Park, CA, United States)
Moser, Desmond E.
(University of Western Ontario London, Ontario, Canada)
Jerolmack, Douglas J.
(Pennsylvania Univ. Philadelphia, PA, United States)
Keller, Lindsay P.
(NASA Johnson Space Center Houston, TX, United States)
Tartese, Romain
(Open Univ. Milton Keynes, United Kingdom)
Date Acquired
October 15, 2015
Publication Date
November 1, 2015
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-34385
Report Number: JSC-CN-34385
Meeting Information
Meeting: GSA 2015
Location: Baltimore, MD
Country: United States
Start Date: November 1, 2015
End Date: November 4, 2015
Sponsors: Geological Society of America
Distribution Limits
Public
Copyright
Public Use Permitted.
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