CHEMISTRY AND MINERALOGY OF OUTCROPS AT MERIDIANI PLANUM

dc.contributor.authorClark B.C.
dc.contributor.authorMorris R.V.
dc.contributor.authorMing D.W.
dc.contributor.authorMcLennan S.M.
dc.contributor.authorTosca N.J.
dc.contributor.authorGellert R.
dc.contributor.authorBrückner J.
dc.contributor.authorDreibus G.
dc.contributor.authorWaenke H.
dc.contributor.authorZipfel J.
dc.contributor.authorRieder R.
dc.contributor.authorJolliff B.
dc.contributor.authorKnoll A.H.
dc.contributor.authorSquyres S.W.
dc.contributor.authorIii J.F.B.
dc.contributor.authorLowenstein T.K.
dc.contributor.authorYen A.
dc.contributor.authorChristensen P.R.
dc.contributor.authorGorevan S.
dc.contributor.authorCalvin W.et al.
dc.date.accessioned2023-12-03T04:00:00Z
dc.date.available2023-12-03T04:00:00Z
dc.date.issued2005
dc.description.abstractAnalyses of outcrops created by the impact craters Endurance, Fram and Eagle reveal the broad lateral continuity of chemical sediments at the Meridiani Planum exploration site on Mars. Approximately ten mineralogical components are implied in these salt-rich silicic sediments, from measurements by instruments on the Opportunity rover. Compositional trends in an apparently intact vertical stratigraphic sequence at the Karatepe West ingress point at Endurance crater are consistent with non-uniform deposition or with subsequent migration of mobile salt components, dominated by sulfates of magnesium. Striking variations in Cl and enrichments of Br, combined with diversity in sulfate species, provide further evidence of episodes during which temperatures, pH, and water to rock ratios underwent significant change. To first order, the sedimentary sequence examined to date is consistent with a uniform reference composition, modified by movement of major sulfates upward and of minor chlorides downward. This reference composition has similarities to martian soils, supplemented by sulfate anion and the alteration products of mafic igneous minerals. Lesser cementation in lower stratigraphic units is reflected in decreased energies for grinding with the Rock Abrasion Tool. Survival of soluble salts in exposed outcrop is most easily explained by absence of episodes of liquid H2O in this region since the time of crater formation.
dc.identifierhttps://www.elibrary.ru/item.asp?id=14757148
dc.identifier.citationEarth and Planetary Science Letters, 2005, 240, 1, 73-94
dc.identifier.doi10.1016/j.epsl.2005.09.040
dc.identifier.issn0012-821X
dc.identifier.urihttps://repository.geologyscience.ru/handle/123456789/42133
dc.subjectMars
dc.subjectoutcrop
dc.subjectMeridiani
dc.subjectchemical sediment
dc.subjectsulfate
dc.subjectkieserite
dc.subjectjarosite
dc.subjectrover
dc.subjectMER
dc.subjectOpportunity
dc.titleCHEMISTRY AND MINERALOGY OF OUTCROPS AT MERIDIANI PLANUM
dc.typeСтатья

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