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Discordant K‐Ar and young exposure dates for the Windjana sandstone, Kimberley, Gale Crater, Mars

Authors :
Vasconcelos, P. M.
Farley, K. A.
Malespin, C. A.
Mahaffy, P.
Ming, D.
McLennan, S. M.
Hurowitz, J. A.
Rice, Melissa S.
Source :
Journal of Geophysical Research - Planets; October 2016, Vol. 121 Issue: 10 p2176-2192, 17p
Publication Year :
2016

Abstract

K‐Ar and noble gas surface exposure age measurements were carried out on the Windjana sandstone, Kimberley region, Gale Crater, Mars, by using the Sample Analysis at Mars instrument on the Curiosity rover. The sandstone is unusually rich in sanidine, as determined by CheMin X‐ray diffraction, contributing to the high K2O concentration of 3.09 ± 0.20 wt % measured by Alpha‐Particle X‐ray Spectrometer analysis. A sandstone aliquot heated to ~915°C yielded a K‐Ar age of 627 ± 50 Ma. Reheating this aliquot yielded no additional Ar. A second aliquot heated in the same way yielded a much higher K‐Ar age of 1710 ± 110 Ma. These data suggest incomplete Ar extraction from a rock with a K‐Ar age older than 1710 Ma. Incomplete extraction at ~900°C is not surprising for a rock with a large fraction of K carried by Ar‐retentive K‐feldspar. Likely, variability in the exact temperature achieved by the sample from run to run, uncertainties in sample mass estimation, and possible mineral fractionation during transport and storage prior to analysis may contribute to these discrepant data. Cosmic ray exposure ages from 3He and 21Ne in the two aliquots are minimum values given the possibility of incomplete extraction. However, the general similarity between the 3He (57 ± 49 and 18 ± 32 Ma, mean 30 Ma) and 21Ne (2 ± 32 and 83 ± 24 Ma, mean 54 Ma) exposure ages provides no evidence for underextraction. The implied erosion rate at the Kimberley location is similar to that reported at the nearby Yellowknife Bay outcrop. Second in situ dating on Mars using SAM in MSLK‐Ar age discrepantCosmogenic isotope ages young and internally compatible

Details

Language :
English
ISSN :
21699097 and 21699100
Volume :
121
Issue :
10
Database :
Supplemental Index
Journal :
Journal of Geophysical Research - Planets
Publication Type :
Periodical
Accession number :
ejs42572429
Full Text :
https://doi.org/10.1002/2016JE005017