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Spectral, Compositional, and Physical Properties of the Upper Murray Formation and Vera Rubin ridge, Gale Crater, Mars

Jacob, S. R. and Wellington, D. F. and Bell, J. F., III and Achilles, C. and Fraeman, A. A. and Horgan, B. and Johnson, J. R. and Maurice, S. and Peters, G. H. and Rampe, E. B. and Thompson, L. M. and Wiens, R. C. (2020) Spectral, Compositional, and Physical Properties of the Upper Murray Formation and Vera Rubin ridge, Gale Crater, Mars. Journal of Geophysical Research. Planets . ISSN 2169-9097. (In Press) https://resolver.caltech.edu/CaltechAUTHORS:20200901-102620010

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Abstract

During 2018 and 2019, the Mars Science Laboratory Curiosity rover investigated the chemistry, morphology, and stratigraphy of Vera Rubin ridge (VRR). Using orbital data from the Compact Reconnaissance Imaging Spectrometer for Mars, scientists attributed the strong 860 nm signal associated with VRR to the presence of red crystalline hematite. However, Mastcam multispectral data and CheMin X‐ray diffraction (XRD) measurements show that the depth of the 860 nm absorption is negatively correlated with the abundance of red crystalline hematite, suggesting other mineralogical or physical parameters are also controlling the 860 nm absorption. Here, we examine Mastcam and ChemCam passive reflectance spectra from VRR and other locations to link the depth, position, and presence or absence of iron‐related mineralogic absorption features to the XRD‐derived rock mineralogy. Correlating CheMin mineralogy to spectral parameters showed that the ~860 nm absorption has a strong positive correlation with the abundance of ferric phyllosilicates. New laboratory reflectance measurements of powdered mineral mixtures can reproduce trends found in Gale crater. We hypothesize that variations in the 860 nm absorption feature in Mastcam and ChemCam observations of VRR materials is a result of three factors: (1) variations in ferric phyllosilicate abundance due to its ~800‐1000 nm absorption; (2) variations in clinopyroxene abundance because of its band maximum at ~860 nm; and (3) the presence of red crystalline hematite because of its absorption centered at 860 nm. We also show that relatively small changes in Ca‐sulfate abundance is one potential cause of the erosional resistance and geomorphic expression of VRR.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1029/2019je006290DOIArticle
https://doi.org/10.5281/zenodo.3827971DOIData
http://an.rsl.wustl.eduRelated ItemCuriosity data
https://pds-imaging.jpl.nasa.gov/volumes/msl.htmlRelated ItemMastcam images
ORCID:
AuthorORCID
Jacob, S. R.0000-0001-9950-1486
Bell, J. F., III0000-0002-2006-4074
Achilles, C.0000-0001-9185-6768
Fraeman, A. A.0000-0003-4017-5158
Horgan, B.0000-0001-6314-9724
Johnson, J. R.0000-0002-5586-4901
Peters, G. H.0000-0003-1590-630X
Rampe, E. B.0000-0002-6999-0028
Thompson, L. M.0000-0002-5444-952X
Wiens, R. C.0000-0002-3409-7344
Additional Information:© 2020 American Geophysical Union. Accepted manuscript online: 28 August 2020; Manuscript accepted: 21 August 2020; Manuscript revised: 20 August 2020; Manuscript received: 27 November 2019. We would like to thank the wonderfully talented engineers and scientists around the world who have made the MSL Curiosity mission such a success and who have helped to obtain and calibrate the data presented in this paper. Reviews by V. Fox and E. Amador were greatly appreciated and helped significantly improve this paper. This work was funded by grants and subcontracts from NASA and Malin Space Science Systems, Inc. (J.R.J. supported by MSL Participating Scientist contract 1546033). A portion of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. The new laboratory data generated and used as part of this research are publicly available on the Zenodo open data depository (10.5281/zenodo.3827971; Jacob (2020)). All Curiosity data can be accessed through the online Analyst’s Notebook tool (http://an.rsl.wustl.edu//) and Mastcam images are available online on the NASA Planetary Data System https://pdsimaging.jpl.nasa.gov/volumes/msl.html.
Funders:
Funding AgencyGrant Number
Malin Space Science Systems, Inc.UNSPECIFIED
JPL1546033
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:Mastcam; Multispectral; Laboratory; Phyllosilicates; Hematite; Ferric Iron
Record Number:CaltechAUTHORS:20200901-102620010
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200901-102620010
Official Citation:Jacob, S. R., Wellington, D. F., Bell, J. F., Achilles, C., Fraeman, A. A., Horgan, B., et al. (2020). Spectral, Compositional, and Physical Properties of the Upper Murray Formation and Vera Rubin ridge, Gale Crater, Mars. Journal of Geophysical Research: Planets, 125, e2019JE006290. https://doi.org/10.1029/2019JE006290
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:105199
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:08 Sep 2020 19:57
Last Modified:08 Sep 2020 19:57

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