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Published May 2018 | Published + Supplemental Material
Journal Article Open

Diverse Lithologies and Alteration Events on the Rim of Noachian-Aged Endeavour Crater, Meridiani Planum, Mars: In-Situ Compositional Evidence

Abstract

We report the results of geological studies by the Opportunity Mars rover on the Endeavour Crater rim. Four major units occur in the region (oldest to youngest): the Matijevic, Shoemaker, Grasberg, and Burns formations. The Matijevic formation, consisting of fine‐grained clastic sediments, is the only pre‐Endeavour‐impact unit and might be part of the Noachian etched units of Meridiani Planum. The Shoemaker formation is a heterogeneous polymict impact breccia; its lowermost member incorporates material eroded from the underlying Matijevic formation. The Shoemaker formation is a close analog to the Bunte Breccia of the Ries Crater, although the average clast sizes are substantially larger in the latter. The Grasberg formation is a thin, fine‐grained, homogeneous sediment unconformably overlying the Shoemaker formation and likely formed as an airfall deposit of unknown areal extent. The Burns formation sandstone overlies the Grasberg, but compositions of the two units are distinct; there is no evidence that the Grasberg formation is a fine‐grained subfacies of the Burns formation. The rocks along the Endeavour Crater rim were affected by at least four episodes of alteration in the Noachian and Early Hesperian: (i) vein formation and alteration of preimpact Matijevic formation rocks, (ii) low‐water/rock alteration along the disconformity between the Matijevic and Shoemaker formations, (iii) alteration of the Shoemaker formation along fracture zones, and (iv) differential mobilization of Fe and Mn, and CaSO_4‐vein formation in the Grasberg and Shoemaker formations. Episodes (ii) and (iii) possibly occurred together, but (i) and (iv) are distinct from either of these.

Additional Information

© 2018 American Geophysical Union. This article has been contributed to by US Government employees and their work is in the public domain in the USA. Received 8 NOV 2017; Accepted 8 FEB 2018; Accepted article online 20 FEB 2018; Published online 24 MAY 2018. Rover operations described in this paper were conducted at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. We thank the members of the MER project who enabled daily science observations at the Opportunity landing site. The senior author is supported by the NASA Mars Exploration Rover Participating Scientist Program. We thank F. Hörz for enlightening and enormously helpful discussions on the geology of the Ries crater. We thank him and M. Cintala for discussions on cratering and impact phenomena in general, B. L. Redding for preparing the MI mosaics used here, J. B. Proton for help with some of the Pancam images, and J. R. Johnson and S. M. McLennan for comments on a draft version of the manuscript. We thank the reviewers A. Fraeman and H. Newsom, and Associate Editor A. D. Rogers for their comments and suggestions which led to substantial improvement of the manuscript. All data used in this article are listed in the references, tables, and supplements. Data for APXS integrations on all rock and soil targets acquired by Opportunity through Sol 4000 are available on the NASA Planetary Data System website: http://pds‐geosciences.wustl.edu/.

Attached Files

Published - Mittlefehldt_et_al-2018-Journal_of_Geophysical_Research_3A_Planets.pdf

Supplemental Material - jgre20812-sup-0001-mittlefehldt_et_al_-_endeavour_crater_rim_rocks_apxs_-_supplementary_information.pdf

Supplemental Material - jgre20812-sup-0002-2017je005474r-st02.xlsx

Supplemental Material - jgre20812-sup-0003-2017je005474r-st04.xlsx

Supplemental Material - jgre20812-sup-0004-2017je005474r-st05.xlsx

Files

Mittlefehldt_et_al-2018-Journal_of_Geophysical_Research_3A_Planets.pdf

Additional details

Created:
August 21, 2023
Modified:
October 18, 2023