SIGNATURES OF THE HIGHLY SIDEROPHILE ELEMENTS IN THE SNC METEORITES AND MARS: A REVIEW AND PETROLOGIC SYNTHESIS

dc.contributor.author	Jones J.H.
dc.contributor.author	Neal C.R.
dc.contributor.author	Ely J.C.
dc.date.accessioned	2021-12-24T05:12:37Z
dc.date.available	2021-12-24T05:12:37Z
dc.date.issued	2003
dc.identifier	https://www.elibrary.ru/item.asp?id=1470101
dc.identifier.citation	Chemical Geology, 2003, 196, 1-4, 5-25
dc.identifier.issn	0009-2541
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/33787
dc.description.abstract	We have evaluated the highly siderophile element (HSE) signatures of the martian (SNC) meteorites using new and literature data. These Ir and Os concentrations correlate with the Mg# [molar Mg/(Mg+Fe)], Cr and Ni, suggesting that olivine or chromite acts as a host for compatible siderophiles. Our analysis agrees with others who have suggested that the martian mantle has chondritic relative abundances of siderophiles. We also agree that, unlike the Sr and Nd isotopic systems, there is no evidence from Os isotopes for crustal assimilation. Comparisons of the siderophile element ratios of ALH 84001 to younger SNCs give no indication of a change in the martian siderophile element pattern over time.
dc.subject	SNC METEORITES
dc.subject	SIDEROPHILE ELEMENTS
dc.subject	OS ISOTOPES
dc.subject	CORE FORMATION
dc.subject	MARS GEOCHEMISTRY
dc.title	SIGNATURES OF THE HIGHLY SIDEROPHILE ELEMENTS IN THE SNC METEORITES AND MARS: A REVIEW AND PETROLOGIC SYNTHESIS
dc.type	Статья

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