The Origin and Timing of Fluvial Activity at Eberswalde Crater, Mars
Icarus 220 (2012) 530–551 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus The origin and timing of fluvial activity at Eberswalde crater, Mars ⇑ N. Mangold a, , E.S. Kite b, M.G. Kleinhans c, H. Newsom d, V. Ansan a, E. Hauber e, E. Kraal f, C. Quantin g, K. Tanaka h a Laboratoire Planétologie et Géodynamique de Nantes, LPGN/CNRS, Université Nantes, 2, rue de la Houssinière, 44322 Nantes, France b Division of Geological and Planetary Science, Caltech MC 150-21, 1200 E. California Boulevard, Pasadena, CA 91125, USA c Faculty of Geosciences, Universiteit Utrecht, PO Box 80115, 3508 TC Utrecht, The Netherlands d Institute of Meteoritics, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA e Institut für Planetenforschung/Institute of Planetary Research, German Aerospace Center (DLR), Rutherfordstr. 2, 12489 Berlin, Germany f Department of Physical Sciences, Kutztown University of Pennsylvania, PA 19530, USA g Laboratoire Géologie de Lyon, La Doua, Université Claude Bernard Lyon, 69622 Villeurbanne, France h Astrogeology Science Center, U.S. Geological Survey, 2255 N. Gemini Dr. Flagstaff, AZ 86001, USA article info abstract Article history: The fan deposit in Eberswalde crater has been interpreted as strong evidence for sustained liquid water on Received 19 September 2011 early Mars with a paleolake formed during the Noachian period (>3.7 Gy). This location became a key region Revised 2 May 2012 for understanding the Mars paleo-environment. Eberswalde crater is located 50 km north of the rim of the Accepted 22 May 2012 150 km diameter crater Holden.
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