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NEKVASIL H.; DONDOLINI A.; HORN J.; FILIBERTO J.; LONG H.; LINDSLEY D. H. 《Journal of Petrology》2004,45(4):693-721
Experimental simulation of incremental crystal fractionationof a hy-normative hawaiite indicates that the spectrum of compositionsfrom mildly alkalic hawaiite to sodic rhyolite found in silica-saturatedalkalic suites of the ocean islands and continental hotspotsand rifts can be produced by fractionation at 9·3 kbarwith bulk water contents > 相似文献
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Hanna NEKVASIL Francis M. McCUBBIN Andrea HARRINGTON Stephen ELARDO Donald H. LINDSLEY 《Meteoritics & planetary science》2009,44(6):853-869
Abstract— In order to use igneous surface lithologies to constrain Martian mantle characteristics, secondary processes that lead to compositional modification of primary mantle melts must be considered. Crystal fractionation of a mantle‐derived magma at the base of the crust followed by separation and ascent of residual liquids to the surface is common in continental hotspot regions on Earth. The possibility that this process also takes place on Mars was investigated by experimentally determining whether a surface rock, specifically the hawaiite Backstay analyzed by the MER Spirit could produce a known cumulate lithology with a deep origin (namely the assemblages of the Chassigny meteorite) if trapped at the base of the Martian crust. Both the major cumulus and melt inclusion mineral assemblages of the Chassigny meteorite were produced experimentally by a liquid of Backstay composition within the pressure range 9.3 to 6.8 kbar with bulk water contents between 1.5 and 2.6 wt%. Experiments at 4.3 and 2.8 kbar did not produce the requisite assemblages. This agreement suggests that just as on Earth, Martian mantle‐derived melts may rise to the surface or remain trapped at the base of the crust, fractionate, and lose their residual liquids. Efficient removal of these residual liquids at depth would yield a deep low‐silica cumulate layer for higher magmatic water content; at lower magmatic water content this cumulate layer would be basaltic with shergottitic affinity. 相似文献
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Hanna NEKVASIL Justin FILIBERTO Francis M. McCUBBIN Donald H. LINDSLEY 《Meteoritics & planetary science》2007,42(6):979-992
Abstract Detailed analysis of cumulate and melt inclusion assemblages in the chassignites provide important constraints on the nature of the melt trapped as inclusions in cumulus olivine (and, by extension, parental magma compositions), the pressures of crystallization, and magmatic volatile contents. These mineral assemblages show strong similarities to the experimental fractionation assemblages that produce the sodic silica‐saturated alkalic lavas on Earth (e.g., Ascension Island, Azores, the Nandewar volcano of Australia). The experimental assemblages were produced from silica‐saturated hawaiite at pressures above 4.3 kbar with dissolved water contents above 0.5 wt%. Such pressures are consistent with Ti:Al ratios of the melt‐inclusion pyroxenes in the Chassigny meteorite. Pyroxene compositions suggest early high crystallization temperatures and thus relatively low initial water and F contents. Feldspars indicate that melt evolution proceeded to rhyolite compositions both within the interstices of the cumulate olivine and within the melt inclusions, even though rhyolitic glass is only found within olivine‐hosted polyphase melt inclusions. The observed rhyolite glass is compositionally similar to the alkali‐rich rhyolite of Ascension Island which is produced experimentally by crystallization of hawaiite. It is proposed that the melt trapped in cumulus olivine of the Chassigny dunite was similar to a terrestrial silica‐saturated hawaiite, while that trapped in olivine of the Northwest Africa (NWA) 2727 dunite was less evolved, perhaps mildly alkalic basalt. Melts similar to terrestrial intra‐plate tholeiite could be parental to the cumulus minerals and evolve upon crystallization at pressures above 4.3 kbar and water contents above ?0.4 wt% to mildly alkalic basalt, silica‐saturated hawaiite, and alkali‐rich rhyolite. The melt inclusion assemblages are inconsistent with either crystallization of a low‐Al, high‐Fe basalt, or low‐pressure crystallization of a terrestrial‐like tholeiite. 相似文献
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Crystal Fractionation and the Evolution of Intra-plate hy-normative Igneous Suites: Insights from their Feldspars 总被引：4，自引：2，他引：2
Feldspars and normative feldspar constituents of bulk magmashow trends supportive of fractional crystallization in thethree main types of hy-normative intraplate suites that containqz-oversaturated rocks: ocean island and continental alkalicsuites, ocean island tholeiitic suites and continental tholeiiticsuites. These suites are characterized by the presence of asingle feldspar in each suite member, a shift of this feldsparfrom plagioclase to alkali feldspar, and K enrichment of alkalifeldspar with decreasing temperature in the trachytic members.The modal feldspars provide evidence for a reaction relationshipbetween feldspars and indicate a build-up of magmatic volatilecontent towards saturation with progressive fractionation ofa parental magma having low initial volatile content. The feldsparand normative feldspar evolutionary paths are unique for eachof the three suite types but similar for different suites withinthe same type. This characteristic extends to the felsic members,making it easy to distinguish between rhyolitic or graniticrocks from the different suite types. The feldspars in naturalvolcanic suites commonly show evidence for a polybaric history,particularly in the least-evolved suite members. Late-stagefeldspars of the intermediate members and feldspars of the mostevolved members show paths indicative of significantly lowertemperature and pressure regimes. KEY WORDS: alkalic; intra-plate; feldspars; fractionation; suites 相似文献
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