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dc.contributor.author Barrón V.
dc.contributor.author Torrent J.
dc.contributor.author Greenwood J.P.
dc.date.accessioned 2024-10-18T08:57:46Z
dc.date.available 2024-10-18T08:57:46Z
dc.date.issued 2006
dc.identifier https://www.elibrary.ru/item.asp?id=14768881
dc.identifier.citation Earth and Planetary Science Letters, 2006, 251, 3-4, 380-385
dc.identifier.issn 0012-821X
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/46007
dc.description.abstract The presence of jarosite - a hydrous iron sulfate - at Meridiani Planum supports the past existence of water on Mars surface. Thermodynamic calculations suggest that jarosite should transform to ferric oxyhydroxides in aqueous media. Here we show that jarosite can transform directly to hematite - the iron oxide identified at Meridiani Planum - in simulated Martian brines. Our results are consistent with a short aqueous history, but also indicate that jarosite can persist in highly saline Martian brines. The formation of goethite, a common iron oxyhydroxide on Earth, is prevented by the low water activity and/or high phosphate concentration of Martian brines. © 2006 Elsevier B.V. All rights reserved.
dc.subject GOETHITE
dc.subject HEMATITE
dc.subject JAROSITE
dc.subject MERIDIANI PLANUM
dc.subject PHOSPHATE
dc.subject WATER ACTIVITY
dc.title TRANSFORMATION OF JAROSITE TO HEMATITE IN SIMULATED MARTIAN BRINES
dc.type Статья
dc.identifier.doi 10.1016/j.epsl.2006.09.022


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