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Extraformational Sediment Recycling on Mars

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Extraformational Sediment Recycling on Mars Extraformational sediment recycling on Mars Kenneth Edgett, Steven Banham, Kristen Bennett, Lauren Edgar, Christopher Edwards, Alberto Fairén, Christopher Fedo, Deirdra Fey, James Garvin, John Grotzinger, et al. To cite this version: Kenneth Edgett, Steven Banham, Kristen Bennett, Lauren Edgar, Christopher Edwards, et al.. Ex- traformational sediment recycling on Mars. Geosphere, Geological Society of America, 2020, 16 (6), pp.1508-1537. 10.1130/GES02244.1. hal-03104177 HAL Id: hal-03104177 https://hal.archives-ouvertes.fr/hal-03104177 Submitted on 8 Jan 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Research Paper GEOSPHERE Extraformational sediment recycling on Mars Kenneth S. Edgett1, Steven G. Banham2, Kristen A. Bennett3, Lauren A. Edgar3, Christopher S. Edwards4, Alberto G. Fairén5,6, Christopher M. Fedo7, Deirdra M. Fey1, James B. Garvin8, John P. Grotzinger9, Sanjeev Gupta2, Marie J. Henderson10, Christopher H. House11, Nicolas Mangold12, GEOSPHERE, v. 16, no. X Scott M. McLennan13, Horton E. Newsom14, Scott K. Rowland15, Kirsten L. Siebach16, Lucy Thompson17, Scott J. VanBommel18, Roger C. Wiens19, 20 20 https://doi.org/10.1130/GES02244.1 Rebecca M.E. Williams , and R. Aileen Yingst 1Malin Space Science Systems, P.O. Box 910148, San Diego, California 92191-0148, USA 2Department of Earth Science and Engineering, Imperial College London, South Kensington, London SW7 2AZ, UK 19 figures; 1 set of supplemental files 3U.S. Geological Survey, Astrogeology Science Center, 2255 N. Gemini Drive, Flagstaff, Arizona 86001, USA 4Department of Astronomy and Planetary Science, Northern Arizona University, P.O. Box 6010, Flagstaff, Arizona 86011, USA CORRESPONDENCE: [email protected] 5Department of Planetology and Habitability, Centro de Astrobiología (CSIC-INTA), M-108, km 4, 28850 Madrid, Spain 6Department of Astronomy, Cornell University, Ithaca, New York 14853, USA 7 CITATION: Edgett, K.S., Banham, S.G., Bennett, K.A., Department of Earth and Planetary Sciences, The University of Tennessee, 1621 Cumberland Avenue, 602 Strong Hall, Knoxville, Tennessee 37996-1410, USA 8 Edgar, L.A., Edwards, C.S., Fairén, A.G., Fedo, C.M., National Aeronautics and Space Administration (NASA) Goddard Space Flight Center, Mail Code 600, Greenbelt, Maryland 20771, USA 9 Fey, D.M., Garvin, J.B., Grotzinger, J.P., Gupta, S., Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA 10 Henderson, M.J., House, C.H., Mangold, N., McLen- Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, 550 Stadium Mall Drive, West Lafayette, Indiana 47907, USA 11 nan, S.M., Newsom, H.E., Rowland, S.K., Siebach, Department of Geosciences, The Pennsylvania State University, University Park, Pennsylvania 16802, USA 12 K.L., Thompson, L., VanBommel, S.J., Wiens, R.C., Laboratoire de Planétologie et Géodynamique de Nantes, CNRS UMR 6112, Université de Nantes, Université Angers, 44300 Nantes, France 13 Williams, R.M.E., and Yingst, R.A., 2020, Extraforma- Department of Geosciences, Stony Brook University, Stony Brook, New York 11794-2100, USA 14 tional sediment recycling on Mars: Geosphere, v. 16, Institute of Meteoritics and Department of Earth and Planetary Sciences, 1 University of New Mexico, MSC03-2050, Albuquerque, New Mexico 87131, USA 15 no. X, p. 1– 30, https://doi.org/10.1130/GES02244.1. Department of Earth Sciences, University of Hawai‘i at Mānoa, Honolulu, Hawai‘i 96822, USA 16Department of Earth, Environmental and Planetary Sciences, Rice University, MS-126, 6100 Main Street, Houston, Texas 77005, USA 17Department of Earth Sciences, University of New Brunswick, P.O. Box 4400, Fredericton, New Brunswick E3B 5A3, Canada Science Editor: Shanaka de Silva 18Department of Earth and Planetary Sciences, Washington University in St. Louis, 1 Brookings Drive, St. Louis, Missouri 63130, USA Associate Editor: Lesli Wood 19MS C331, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA 20Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, Arizona 85719-2395, USA Received 8 February 2020 Revision received 21 July 2020 Accepted 25 August 2020 ABSTRACT ■ INTRODUCTION Extraformational sediment recycling (old sedimentary rock to new sedimentary rock) is a fundamental The processes of fragment production, weath- aspect of Earth’s geological record; tectonism exposes sedimentary rock, whereupon it is weathered and ering, transport, deposition, burial, and diagenesis eroded to form new sediment that later becomes lithified. On Mars, tectonism has been minor, but two would have begun to create a sedimentary record decades of orbiter instrument–based studies show that some sedimentary rocks previously buried to depths almost as soon as the Martian crust formed, per- of kilometers have been exposed, by erosion, at the surface. Four locations in Gale crater, explored using haps just ~20 m.y. (Bouvier et al., 2018) after the National Aeronautics and Space Administration’s Curiosity rover, exhibit sedimentary lithoclasts in crystallization of the solar system’s first solid sedimentary rock: At Marias Pass, they are mudstone fragments in sandstone derived from strata below particles. Although battered, shocked, and redis- an erosional unconformity; at Bimbe, they are pebble-sized sandstone and, possibly, laminated, intra- tributed by impact events (Abramov and Mojzsis, clast-bearing, chemical (calcium sulfate) sediment fragments in conglomerates; at Cooperstown, they 2016), without sustained, mobile-lid (plate) tecton- are pebble-sized fragments of sandstone within coarse sandstone; at Dingo Gap, they are cobble-sized, ics (Zhang and O’Neill, 2016), the Martian crust has stratified sandstone fragments in conglomerate derived from an immediately underlying sandstone. Mars largely retained its ancient sedimentary archive orbiter images show lithified sediment fans at the termini of canyons that incise sedimentary rock in Gale (Grotzinger et al., 2011). This record includes rocks crater; these, too, consist of recycled, extraformational sediment. The recycled sediments in Gale crater are older than the oldest sedimentary and metasedi- compositionally immature, indicating the dominance of physical weathering processes during the second mentary strata on Earth (cf. Condie, 2019). known cycle. The observations at Marias Pass indicate that sediment eroded and removed from craters As occurs on Earth (e.g., Dunne et al., 1998; such as Gale crater during the Martian Hesperian Period could have been recycled to form new rock else- Marriott and Wright, 1996; East et al., 2015; Licht where. Our results permit prediction that lithified deltaic sediments at the Perseverance (landing in 2021) et al., 2016), Martian sediments can be recycled, or and Rosalind Franklin (landing in 2023) rover field sites could contain extraformational recycled sediment. even multicycled, during transport and temporary This paper is published under the terms of the storage on their way to their ultimate depositional CC-BY-NC license. Kenneth S. Edgett http://orcid.org/0000-0001-7197-5751 basins. Such penecontemporaneous recycling can © 2020 The Authors GEOSPHERE | Volume 16 | Number X Edgett et al. | Mars sediment recycling Downloaded from http://pubs.geoscienceworld.org/gsa/geosphere/article-pdf/doi/10.1130/GES02244.1/5159754/ges02244.pdf 1 by guest on 07 October 2020 Research Paper include creation and deposition of intraclasts, that is, dissolution or (on Earth) subduction. Cannibalistic that fluvial systems had been superimposed across fragments of indurated sediment eroded from and multicycling of clastic sediment on Earth “accumu- others (Malin and Edgett, 2001, figure 32; Edgett, reworked “within the area of deposition” (Folk, 1959, lates the effects of several episodes of weathering, 2016, figure 1). Whether all of this erosion and p. 4). On early Mars, such short-term recycling would transport, and diagenesis,” (Cox and Lowe, 1995b, p. redeposition on early Mars led to recycling of have been a normal consequence of the interactions 5), providing one of the pathways (see Dott, 2003) extraformational sediment into new sedimentary between and within the planet’s fluvial, lacustrine, toward sediment compositional maturation. rock seemed likely but remained an open question mass movement, and eolian transport and temporary Although tectonism has been negligible as (McLennan and Grotzinger, 2008), until now. storage systems. A key example of this is recorded compared to Earth, images of the Martian surface The presence of just one extraformational sed- by the Burns formation of Meridiani Planum, where present considerable evidence that some of its sed- imentary rock fragment in a younger sedimentary sand-sized mud pellets are interpreted to have been imentary rocks were lithified at depths measured rock is direct evidence that cannibalistic sediment deflated from playas, accumulated nearby to form in kilometers and later exposed at the surface by recycling has transpired (Zuffa, 1987). Here, we eolian dunes, and
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