Cited by 381Planetary Science and ExplorationAstro and Planetary ScienceGeological formations and processes

Martian Fluvial Conglomerates at Gale Crater

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Williams, R. M. E., Grotzinger, J. P., Dietrich, W. E., Gupta, S., Sumner, D. Y., Wiens, R. C., Mangold, N., Malin, M. C. +436 more·2013·Science

Abstract

Observations by the Mars Science Laboratory Mast Camera (Mastcam) in Gale crater reveal isolated outcrops of cemented pebbles (2 to 40 millimeters in diameter) and sand grains with textures typical of fluvial sedimentary conglomerates. Rounded pebbles in the conglomerates indicate substantial fluvial abrasion. ChemCam emission spectra at one outcrop show a predominantly feldspathic composition, consistent with minimal aqueous alteration of sediments. Sediment was mobilized in ancient water flows that likely exceeded the threshold conditions (depth 0.03 to 0.9 meter, average velocity 0.20 to 0.75 meter per second) required to transport the pebbles. Climate conditions at the time sediment was transported must have differed substantially from the cold, hyper-arid modern environment to permit aqueous flows across several kilometers.

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Crossref · 10.1126/science.1237317

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  • NASA's Curiosity rover found conglomerate outcrops at Gale Crater that are morphologically remarkably similar to sediment deposits found on Earth.

    “Striking evidence of in situ fluvial erosion was found by NASA's Curiosity rover in the form of conglomerate outcrops at Gale Crater (Williams et al. 2013). Morphologically, the conglomerates are remarkably similar to sediment deposits found on Earth (see Fig. 1).”

    From The Climate of Early Mars (2016) · cites this paper as Williams et al. 2013

  • Chemical analysis of the Gale Crater conglomerate outcrops suggested low chemical alteration of the material by water.

    “However, chemical analysis of the outcrops suggested low chemical alteration of the material by water (Williams et al. 2013).”

    From The Climate of Early Mars (2016) · cites this paper as Williams et al. 2013

  • The flows responsible for eroding the late Noachian and Hesperian surface were relatively short-lived.

    “This suggests that the flows responsible for eroding the late Noachian and Hesperian surface were relatively short-lived.”

    From The Climate of Early Mars (2016) · cites this paper as Williams et al. 2013

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Williams, R. M. E., Grotzinger, J. P., Dietrich, W. E., Gupta, S., Sumner, D. Y., Wiens, R. C., Mangold, N., Malin, M. C., Edgett, K. S., Maurice, S., Forni, O., Gasnault, O., Ollila, A., Newsom, H. E., Dromart, G., Palucis, M. C., Yingst, R. A., Anderson, R. B., Herkenhoff, K. E., Le Mouélic, S., Goetz, W., Madsen, M. B., Koefoed, A., Jensen, J. K., Bridges, J. C., Schwenzer, S. P., Lewis, K. W., Stack, K. M., Rubin, D., Kah, L. C., Bell, J. F., Farmer, J. D., Sullivan, R., Van Beek, T., Blaney, D. L., Pariser, O., Deen, R. G., MSL Science Team, Kemppinen, O., Bridges, N., Johnson, J. R., Minitti, M., Cremers, D., Edgar, L., Godber, A., Wadhwa, M., Wellington, D., McEwan, I., Newman, C., Richardson, M., Charpentier, A., Peret, L., King, P., Blank, J., Weigle, G., Schmidt, M., Li, S., Milliken, R., Robertson, K., Sun, V., Baker, M., Edwards, C., Ehlmann, B., Farley, K., Griffes, J., Miller, H., Newcombe, M., Pilorget, C., Rice, M., Siebach, K., Stolper, E., Brunet, C., Hipkin, V., Léveillé, R., Marchand, G., Sobrón Sánchez, P., Favot, L., Cody, G., Steele, A., Flückiger, L., Lees, D., Nefian, A., Martin, M., Gailhanou, M., Westall, F., Israël, G., Agard, C., Baroukh, J., Donny, C., Gaboriaud, A., Guillemot, P., Lafaille, V., Lorigny, E., Paillet, A., Pérez, R., Saccoccio, M., Yana, C., Aparicio, C. A., Caride Rodríguez, J., Carrasco Blázquez, I., Gómez Gómez, F., Elvira, J. G., Hettrich, S., Lepinette Malvitte, A., Marín Jiménez, M., Frías, J. M., Soler, J. M., Torres, F. J. M., Molina Jurado, A., Sotomayor, L. M., Muñoz Caro, G., Navarro López, S., González, V. P., García, J. P., Rodriguez Manfredi, J. A., Planelló, J. J. R., Alejandra Sans Fuentes, S., Sebastian Martinez, E., Torres Redondo, J., O'Callaghan, R. U., Zorzano Mier, M.-P., Chipera, S., Lacour, J.-L., Mauchien, P., Sirven, J.-B., Manning, H., Fairén, A., Hayes, A., Joseph, J., Squyres, S., Thomas, P., Dupont, A., Lundberg, A., Melikechi, N., Mezzacappa, A., DeMarines, J., Grinspoon, D., Reitz, G., Prats, B., Atlaskin, E., Genzer, M., Harri, A.-M., Haukka, H., Kahanpää, H., Kauhanen, J., Paton, M., Polkko, J., Schmidt, W., Siili, T., Fabre, C., Wray, J., Wilhelm, M. B., Poitrasson, F., Patel, K., Gorevan, S., Indyk, S., Paulsen, G., Bish, D., Schieber, J., Gondet, B., Langevin, Y., Geffroy, C., Baratoux, D., Berger, G., Cros, A., Uston, C. D., Lasue, J., Lee, Q.-M., Meslin, P.-Y., Pallier, E., Parot, Y., Pinet, P., Schröder, S., Toplis, M., Lewin, É., Brunner, W., Heydari, E., Achilles, C., Oehler, D., Sutter, B., Cabane, M., Coscia, D., Szopa, C., Robert, F., Sautter, V., Nachon, M., Buch, A., Stalport, F., Coll, P., François, P., Raulin, F., Teinturier, S., Cameron, J., Clegg, S., Cousin, A., DeLapp, D., Dingler, R., Jackson, R. S., Johnstone, S., Lanza, N., Little, C., Nelson, T., Williams, R. B., Jones, A., Kirkland, L., Treiman, A., Baker, B., Cantor, B., Caplinger, M., Davis, S., Duston, B., Fay, D., Hardgrove, C., Harker, D., Herrera, P., Jensen, E., Kennedy, M. R., Krezoski, G., Krysak, D., Lipkaman, L., McCartney, E., McNair, S., Nixon, B., Posiolova, L., Ravine, M., Salamon, A., Saper, L., Stoiber, K., Supulver, K., Van Beek, J., Zimdar, R., French, K. L., Iagnemma, K., Miller, K., Summons, R., Goesmann, F., Hviid, S., Johnson, M., Lefavor, M., Lyness, E., Breves, E., Dyar, M. D., Fassett, C., Blake, D. F., Bristow, T., DesMarais, D., Edwards, L., Haberle, R., Hoehler, T., Hollingsworth, J., Kahre, M., Keely, L., McKay, C., Bleacher, L., Brinckerhoff, W., Choi, D., Conrad, P., Dworkin, J. P., Eigenbrode, J., Floyd, M., Freissinet, C., Garvin, J., Glavin, D., Harpold, D., Mahaffy, P., Martin, D. K., McAdam, A., Pavlov, A., Raaen, E., Smith, M. D., Stern, J., Tan, F., Trainer, M., Meyer, M., Posner, A., Voytek, M., Anderson, R. C., Aubrey, A., Beegle, L. W., Behar, A., Brinza, D., Calef, F., Christensen, L., Crisp, J. A., DeFlores, L., Feldman, J., Feldman, S., Flesch, G., Hurowitz, J., Jun, I., Keymeulen, D., Maki, J., Mischna, M., Morookian, J. M., Parker, T., Pavri, B., Schoppers, M., Sengstacken, A., Simmonds, J. J., Spanovich, N., de la Torre Juarez, M., Vasavada, A. R., Webster, C. R., Yen, A., Archer, P. D., Cucinotta, F., Jones, J. H., Ming, D., Morris, R. V., Niles, P., Rampe, E., Nolan, T., Fisk, M., Radziemski, L., Barraclough, B., Bender, S., Berman, D., Dobrea, E. N., Tokar, R., Vaniman, D., Leshin, L., Cleghorn, T., Huntress, W., Manhès, G., Hudgins, J., Olson, T., Stewart, N., Sarrazin, P., Grant, J., Vicenzi, E., Wilson, S. A., Bullock, M., Ehresmann, B., Hamilton, V., Hassler, D., Peterson, J., Rafkin, S., Zeitlin, C., Fedosov, F., Golovin, D., Karpushkina, N., Kozyrev, A., Litvak, M., Malakhov, A., Mitrofanov, I., Mokrousov, M., Nikiforov, S., Prokhorov, V., Sanin, A., Tretyakov, V., Varenikov, A., Vostrukhin, A., Kuzmin, R., Clark, B., Wolff, M., McLennan, S., Botta, O., Drake, D., Bean, K., Lemmon, M., Lee, E. M., Sucharski, R., Hernández, M. Á. D. P., Blanco Ávalos, J. J., Ramos, M., Kim, M.-H., Malespin, C., Plante, I., Muller, J.-P., González, R. N., Ewing, R., Boynton, W., Downs, R., Fitzgibbon, M., Harshman, K., Morrison, S., Kortmann, O., Williams, A., Lugmair, G., Wilson, M. A., Jakosky, B., Zunic, T. B., Frydenvang, J., Kinch, K., Stipp, S. L. S., Boyd, N., Campbell, J. L., Gellert, R., Perrett, G., Pradler, I., VanBommel, S., Jacob, S., Owen, T., Rowland, S., Savijärvi, H., Boehm, E., Böttcher, S., Burmeister, S., Guo, J., Köhler, J., García, C. M., Mellin, R. M., Schweingruber, R. W., McConnochie, T., Benna, M., Franz, H., Bower, H., Brunner, A., Blau, H., Boucher, T., Carmosino, M., Atreya, S., Elliott, H., Halleaux, D., Rennó, N., Wong, M., Pepin, R., Elliott, B., Spray, J., Thompson, L., Gordon, S., Williams, J., Vasconcelos, P., Bentz, J., Nealson, K., Popa, R., Moersch, J., Tate, C., Day, M., Kocurek, G., Hallet, B., Sletten, R., Francis, R., McCullough, E., Cloutis, E., ten Kate, I. L., Arvidson, R., Fraeman, A., Scholes, D., Slavney, S., Stein, T., Ward, J., Berger, J., & Moores, J. E.
Affiliations
  • Planetary Science Institute (US)
  • California Institute of Technology (US)
  • University of California, Berkeley (US)
  • Imperial College London (GB)
  • University of California, Davis (US)
  • Los Alamos National Laboratory (US)
  • Centre National de la Recherche Scientifique (FR)
  • Malin Space Science Systems (United States) (US)
  • University of New Mexico (US)
  • Université de Lyon (FR)
  • United States Geological Survey (US)
  • Laboratoire Planétologie et Géodynamique de Nantes, LPGN/CNRS UMR6112 and Université de Nantes, 44322 Nantes, France.
  • Max Planck Society (DE)
  • University of Copenhagen (DK)
  • University of Leicester (GB)
  • The Open University (GB)
  • Princeton University (US)
  • University of Tennessee at Knoxville (US)
  • School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.
  • Arizona State University (US)
  • Cornell University (US)
  • Malin Space Science Systems, San Diego, CA 92121, USA.
  • GeoRessources (FR)
Corresponding author
  • Williams, R. M. E.
  • Williams, Richard B.
ORCID
Venue
Science
Published
2013-05-31
Volume
340
Issue
6136
Pages
1068-1072
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2100451067
Cited by
381
References
0
Citations by year
2026: 10 · 2025: 19 · 2024: 14 · 2023: 15 · 2022: 23 · 2021: 32 · 2020: 36 · 2019: 27 · 2018: 32 · 2017: 34 · 2016: 35 · 2015: 44 · 2014: 45 · 2013: 14
FWCI
24.84
Type
journal article
Language
en
Licence
cc-by
Locations
  • Science (publishedVersion)
  • PubMed (publishedVersion)
  • Research at the University of Copenhagen (University of Copenhagen) (publishedVersion)
  • elib (German Aerospace Center) (acceptedVersion)
  • Open Research Online (The Open University) (acceptedVersion)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
  • HAL (submittedVersion)
  • Utrecht University Repository (Utrecht University) (submittedVersion)
  • elib (German Aerospace Center) (submittedVersion)
  • UCL Discovery (University College London) (submittedVersion)
  • Max Planck Digital Library (submittedVersion)
  • Leicester Research Archive (University of Leicester) (submittedVersion)
  • GoeScholar The Publication Server of the Georg-August-Universität Göttingen (Georg-August-Universität Göttingen) (submittedVersion, cc-by)
  • MPG.PuRe (Max Planck Society) (submittedVersion)
  • Smithsonian Digital Repository (Smithsonian Institution) (submittedVersion)
Funders
  • National Aeronautics and Space Administration
  • Science and Technology Facilities Council (1195655)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Earth and Planetary Sciences › Earth-Surface Processes › Geological formations and processes
Keywords
Gale Crater, Mars Science Laboratory, fluvial sediment transport, aqueous alteration, Mars paleoclimate

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