Aqueously altered igneous rocks sampled on the floor of Jezero crater, Mars

K. A. Farley, K. M. Stack, D. L. Shuster, B. H.N. Horgan, J. A. Hurowitz, J. D. Tarnas, J. I. Simon, V. Z. Sun, E. L. Scheller, K. R. Moore, S. M. McLennan, P. M. Vasconcelos, R. C. Wiens, A. H. Treiman, L. E. Mayhew, O. Beyssac, T. V. Kizovski, N. J. Tosca, K. H. Williford, L. S. CrumplerL. W. Beegle, J. F. Bell, B. L. Ehlmann, Y. Liu, J. N. Maki, M. E. Schmidt, A. C. Allwood, H. E.F. Amundsen, R. Bhartia, T. Bosak, A. J. Brown, B. C. Clark, A. Cousin, O. Forni, T. S.J. Gabriel, Y. Goreva, S. Gupta, S. E. Hamran, C. D.K. Herd, K. Hickman-Lewis, J. R. Johnson, L. C. Kah, P. B. Kelemen, K. B. Kinch, L. Mandon, N. Mangold, C. Quantin-Nataf, M. S. Rice, P. S. Russell, S. Sharma, S. Siljeström, A. Steele, R. Sullivan, M. Wadhwa, B. P. Weiss, A. J. Williams, B. V. Wogsland, P. A. Willis, T. A. Acosta-Maeda, P. Beck, K. Benzerara, S. Bernard, A. S. Burton, E. L. Cardarelli, B. Chide, E. Clavé, E. A. Cloutis, B. A. Cohen, A. D. Czaja, V. Debaille, E. Dehouck, A. G. Fairén, D. T. Flannery, S. Z. Fleron, T. Fouchet, J. Frydenvang, B. J. Garczynski, E. F. Gibbons, E. M. Hausrath, A. G. Hayes, J. Henneke, J. L. Jørgensen, E. M. Kelly, J. Lasue, S. Le Mouélic, J. M. Madariaga, S. Maurice, M. Merusi, P. Y. Meslin, S. M. Milkovich, C. C. Million, R. C. Moeller, J. I. Núñez, A. M. Ollila, G. Paar, D. A. Paige, D. A.K. Pedersen, P. Pilleri, C. Pilorget, P. C. Pinet, J. W. Rice, C. Royer, V. Sautter, M. Schulte, M. A. Sephton, S. K. Sharma, S. F. Sholes, N. Spanovich, M. ST Clair, C. D. Tate, K. Uckert, S. J. VanBommel, A. G. Yanchilina, M. P. Zorzano

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64 Scopus citations

Abstract

The Perseverance rover landed in Jezero crater, Mars, to investigate ancient lake and river deposits. We report observations of the crater floor, below the crater’s sedimentary delta, finding that the floor consists of igneous rocks altered by water. The lowest exposed unit, informally named Séítah, is a coarsely crystalline olivine-rich rock, which accumulated at the base of a magma body. Magnesium-iron carbonates along grain boundaries indicate reactions with carbon dioxide–rich water under water-poor conditions. Overlying Séítah is a unit informally named Máaz, which we interpret as lava flows or the chemical complement to Séítah in a layered igneous body. Voids in these rocks contain sulfates and perchlorates, likely introduced by later near-surface brine evaporation. Core samples of these rocks have been stored aboard Perseverance for potential return to Earth.

Original languageEnglish (US)
Article number1512
JournalScience
Volume377
Issue number6614
DOIs
StatePublished - Sep 30 2022

ASJC Scopus subject areas

  • General

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