Iron Mobility During Diagenesis at Vera Rubin Ridge, Gale Crater, Mars
Reprint of accepted article : L'Haridon, J., Mangold, N., Fraeman, A. A., Johnson, J. R., Cousin, A., Rapin, W., et al. (2020). Iron mobility during diagenesis at Vera Rubin ridge, Gale Crater, Mars. Journal of Geophysical Research: Planets, 125, e2019JE006299. https://doi.org/10.1029/2019JE006299 Iron Mobility during Diagenesis at Vera Rubin ridge, Gale Crater, Mars J. L’Haridon1, N. Mangold1, A. A. Fraeman2, J. R. Johnson3, A. Cousin4, W. Rapin5, G. David4, E. Dehouck6, V. Sun5, J. Frydenvang7, O. Gasnault4, P. Gasda8, N. Lanza8, O. Forni4, P.-Y. Meslin4, S. P. Schwenzer9, J. Bridges10, B. Horgan11, C. H. House12, M. Salvatore13, S. Maurice4, R. C. Wiens7 1 Laboratoire de Planétologie et Géodynamique, UMR6112, CNRS, Univ Nantes, Univ Angers, Nantes, France 2 Jet Propulsion Laboratory, Pasadena, California, USA 3 Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA 4 IRAP, UPS, OMP, Toulouse, France 5 California Institute of Technology, Pasadena, California, USA 6 Univ Lyon, Univ Lyon 1, ENSL, CNRS, LGL-TPE, F-69622, Villeurbanne, France 7 University of Copenhagen, Copenhagen, Denmark 8 Los Alamos National Laboratory, Los Alamos, New Mexico, USA 9 Open University, Milton Keynes, UK 10 University of Leicester, UK 11 Purdue University, USA 12 Dept of Geosciences, Pennsylvania State University, USA 13 North Arizona University, Flagstaff, USA HIGHLIGHTS → Images from the Curiosity rover show the presence of dark-toned diagenetic features at Vera Rubin ridge → ChemCam analyses of these features point towards a Fe-oxide composition, consistent with crystalline hematite → Depletion of Fe and Mn in bleached halos surrounding the high-Fe diagenetic features indicates mobility of Fe and Mn during the later stages of diagenesis 1 ABSTRACT The Curiosity rover investigated a topographic structure known as Vera Rubin ridge, associated with a hematite signature in orbital spectra.
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