Petrological constraints on the density of the Martian crust | INSTITUT DE PHYSIQUE DU GLOBE DE PARIS

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> > Petrological constraints on the density of the Martian crusn" class=/rdf Petrologica+ constraint+on+ th+ densit+of+ th+ Martia+ crus&rft. titleJ.+Geophys.+Res.+Pplanes&rft./dat=2010&rft.volume=119&rft.s uag=1707&rft.e uag=1727%2C+doi%3A10.1002%2F2010JE200642&rft.aullas=Baeratux&rft.au-firs=D.&rft.au=D.%2C+Samuel&rft.au=Michaut%2C+Chloe&rft.au=Toplis%2C+M.&rft.au=Miooereau%2C+M.&rft.au=Wieczorek%2C+Mark&rft.au=Garcia%2C+R.&rft.au=Kurh3>pType de"publiactio: Jouerna Aartclh>
h3>Souecp: J. Geophys. Res. Pplanes, Volume 1-9, p.1707-1727, doi:10.1002/2010JE200642 (2010)>
h3>URL:>
"http:/dx.doi3.org/0.1002/2010JE200642 h3>Résumé: >p>New iensghntsainof therchminstty of the Martian crusthaivdbeen ma deavralsabld senc the drirmatioy of crusna thickness maps frome Mas Globna Surveyor ogavsityand t"orogaphy /daa that usendal consermativdrangey of density valus (2700–3100 kg/m3). A new rangey of crusna density valus is ocacu-latd frome themajor "elemenerchminstty of Martian

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