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\begin{document}

\title{Properties of the Nili Fossae Olivine-phyllosilicate-carbonate
lithology: orbital and in situ at S\selectlanguage{ngerman}éítah\selectlanguage{english}}



\author[1]{Adrian Jon Brown}%
\author[2]{Linda C Kah}%
\author[3]{Lucia Mandon}%
\author[4]{Roger C. Wiens}%
\author[5]{Patrick C. Pinet}%
\author[6]{Elise Clavé}%
\author[7]{Stephane Le Mouelic}%
\author[8]{Arya Udry}%
\author[4]{Patrick J Gasda}%
\author[9]{Clement Royer}%
\author[10]{Keyron Hickman-Lewis}%
\author[11]{Agnès Cousin}%
\author[12]{Justin I. Simon}%
\author[13]{Edward Cloutis}%
\author[14]{Thierry Fouchet}%
\author[15]{Alberto Fairen}%
\author[16]{Stephanie Connell}%
\author[17]{David Timothy Flannery}%
\author[16]{Briony Heather Noelle Horgan}%
\author[18]{Lisa Mayhew}%
\author[19]{Allan H. Treiman}%
\author[20]{Jorge I. Núñez}%
\author[21]{Brittan Valhalla Wogsland}%
\author[22]{Hans E. F. Amundsen}%
\author[23]{Cathy Quantin-Nataf}%
\author[24]{Kevin Peter Hand}%
\author[25]{Vinciane Debaille}%
\author[26]{Ari Essunfeld}%
\author[27]{Pierre Beck}%
\author[28]{Nicholas Tosca}%
\author[29]{Juan Manuel Madariaga}%
\author[30]{Eleni Maria Ravanis}%
\author[31]{Karim Benzerara}%
\author[32]{Jade Comellas}%
\author[33]{Olivier Forni}%
\affil[1]{Plancius Research}%
\affil[2]{University of Tennessee at Knoxville}%
\affil[3]{LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France}%
\affil[4]{Los Alamos National Laboratory (DOE)}%
\affil[5]{Univ. de Toulouse / CNRS}%
\affil[6]{University of Bordeaux}%
\affil[7]{LPGN}%
\affil[8]{Department of Geoscience, University of Nevada, Las Vegas}%
\affil[9]{LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris,}%
\affil[10]{The Natural History Museum}%
\affil[11]{Institut de Recherche en Astrophysique et Planétologie - IRAP}%
\affil[12]{Center for Isotope Cosmochemistry and Geochronology, Astromaterials Research and Exploration Science, NASA Johnson Space Center}%
\affil[13]{University of Winnepeg}%
\affil[14]{Observatoire de Paris}%
\affil[15]{Centro de Astrobiologia}%
\affil[16]{Purdue University}%
\affil[17]{Science and Engineering Faculty, Queensland University of Technology}%
\affil[18]{University of Colorado Boulder}%
\affil[19]{Lunar and Planetary Institute}%
\affil[20]{Johns Hopkins University Applied Physics Laboratory}%
\affil[21]{University of Tennessee}%
\affil[22]{Earth and Planetary Exploration Services}%
\affil[23]{laboratoire de Géologie de Lyon}%
\affil[24]{Jet Propulsion Laboratory}%
\affil[25]{Université Libre de Bruxelles}%
\affil[26]{Los Alamos National Laboratory}%
\affil[27]{Institut de Planétologie et d'Astrophysique de Grenoble, Université Joseph Fourier, Grenoble, France}%
\affil[28]{University of Cambridge}%
\affil[29]{University of the Basque Country}%
\affil[30]{Department of Earth Sciences, University of Hawai'i, Honolulu, HI, USA}%
\affil[31]{Institut de Minéralogie, Physique des Matériaux et Cosmochimie, CNRS}%
\affil[32]{University of Hawai'i at Mānoa}%
\affil[33]{Institut de Recherche en Astrophysique et Planétologie (IRAP) - CNRS}%


\vspace{-1em}



  
  \date{May 24, 2024}


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\selectlanguage{english}
\begin{abstract}
We have studied the observed properties of the Nili Fossae
olivine-phyllosilicate-carbonate lithology from orbital data and in situ
by the Mars 2020 rover at the S\selectlanguage{ngerman}éítah unit in Jezero crater, including:
1) composition 2) grain size 3) inferred viscosity (calculated based on
geochemistry collected by SuperCam (Wiens et al., 2022)). Based on the
low viscosity and distribution of the unit we postulate a flood lava
origin for the olivine-phyllosilicate-carbonate at Séítah.

We include a new CRISM map of the phyllosilicate 2.38 \selectlanguage{greek}μ\selectlanguage{english}m band and use in
situ data from Mars 2020 SuperCam Laser Induced Breakdown Spectroscopy
(LIBS) and VISIR and MastCam-Z observations to show that the
phyllosilicate in the olivine cumulate in the S\selectlanguage{ngerman}éítah formation is either
talc, serpentine, hectorite, Fe/Mg smectite, saponite or stevensite.

We discuss two intertwining aspects of the history of the lithology: 1)
the emplacement and properties of the cumulate layer within a lava lake,
based on terrestrial analogs in the Pilbara, Western Australia, and
using previously published models of flood lavas and lava lakes, and 2)
the limited extent of post emplacement alteration, including
phyllosilicate and carbonate alteration.%
\end{abstract}\selectlanguage{ngerman}%



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\textbf{Hosted file}

\verb`957974_0_supp_10772531_rr9bz9.docx`  available at \url{https://authorea.com/users/529644/articles/628832-properties-of-the-nili-fossae-olivine-phyllosilicate-carbonate-lithology-orbital-and-in-situ-at-s%C3%A9%C3%ADtah}

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