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dc.contributor.authorNamur, O.
dc.contributor.authorCharlier, B.
dc.contributor.authorPirard, C.
dc.contributor.authorHermann, J.
dc.contributor.authorLiégeois, J.P.
dc.contributor.authorVander Auwera, J.
dc.date2011
dc.date.accessioned2016-03-15T10:04:49Z
dc.date.available2016-03-15T10:04:49Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/1039
dc.descriptionThe Sept Iles layered intrusion (Quebec, Canada) is dominated by a basal Layered Series made up of troctolites and gabbros, and by anorthosites occurring (1) at the roof of the magma chamber (100 500 m-thick) and (2) as cm- to m-size blocks in gabbros of the Layered Series. Anorthosite rocks are made up of plagioclase, with minor clinopyroxene, olivine and Fe Ti oxide minerals. Plagioclase displays a very restricted range of compositions for major elements (An68 An60), trace elements (Sr: 1023 1071 ppm; Ba: 132 172 ppm) and Sr isotopic ratios (87Sr/86Sri: 0.70356 0.70379). This compositional range is identical to that observed in troctolites, the most primitive cumulates of the Layered Series, whereas plagioclase in layered gabbros is more evolved (An60 An38). The origin of Sept Iles anorthosites has been investigated by calculating the density of plagioclase and that of the evolving melts. The density of the FeO-rich tholeiitic basalt parent magma first increased from 2.70 to 2.75 g/cm3 during early fractionation of troctolites and then decreased continuously to 2.16 g/cm3 with fractionation of Fe Ti oxide-bearing gabbros. Plagioclase (An69 An60) was initially positively buoyant and partly accumulated at the top of the magma chamber to form the roof anorthosite. With further differentiation, plagioclase (<An60) became negatively buoyant and anorthosite stopped forming. Blocks of anorthosite (autoliths) even fell downward to the basal cumulate pile. The presence of positively buoyant plagioclase in basal troctolites is explained by the low efficiency of plagioclase flotation due to crystallization at the floor and/or minor plagioclase nucleation within the main magma body. Dense mafic minerals of the roof anorthosite are shown to have crystallized from the interstitial liquid. The processes related to floating and sinking of plagioclase in a large and shallow layered intrusion serve as a proxy to refine the crystallization model of the lunar magma ocean and explain the vertically stratified structure of the lunar crust, with (gabbro-)noritic rocks at the base and anorthositic rocks at the top. We propose that the lunar crust mainly crystallized bottom-up. This basal crystallization formed a mafic lower crust that might have a geochemical signature similar to the magnesian-suite without KREEP contamination, while flotation of some plagioclase grains produced ferroan anorthosites in the upper crust.
dc.languageeng
dc.titleAnorthosite formation by plagioclase flotation in ferrobasalt
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.subject.freeGeodynamics and mineral resources
dc.source.titleGeochimica et Cosmochimica Acta
dc.source.volume75
dc.source.page4998 5018
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.gca.2011.06.013
dc.identifier.rmca2466


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