The role of fractional crystallization and late-stage peralkaline melt segregation in the mineralogical evolution of Cenozoic nephelinites/phonolites from Saghro (SE Morocco)

被引:31
作者
Berger, J. [1 ,2 ,3 ]
Ennih, N. [4 ]
Mercier, J. C. C. [3 ,5 ]
Liegeois, J. -P. [1 ]
Demaiffe, D. [2 ]
机构
[1] Musee Royal Afr Cent, Sect Geol Isotop, B-3080 Tervuren, Belgium
[2] Univ Libre Bruxelles, Lab Geochim Isotop & Geodynam Chim, B-1050 Brussels, Belgium
[3] Univ La Rochelle, ILE, CNRS, UMR LIENSs 6250, F-17042 La Rochelle, France
[4] Univ El Jadida, Lab Geodynam, El Jadida 24000, Morocco
[5] Univ Nantes, CNRS, UMR Planetol & Geodynam LPGN 6112, F-44322 Nantes, France
关键词
nephelinite; peralkaline phonolite; carbonatite; Daly gap; hainite; fractional-crystallization modelling; Mio-Pliocene volcanism; ANTI-ATLAS MOROCCO; NEPHELINE SYENITE; SOUTH GREENLAND; CANARY-ISLANDS; KERGUELEN ARCHIPELAGO; GEOCHRONOLOGICAL DATA; VOLCANIC-ROCKS; JBEL-SAGHRO; DALY GAP; ALKALINE;
D O I
10.1180/minmag.2009.073.1.59
中图分类号
P57 [矿物学];
学科分类号
070901 ;
摘要
The Saghro Cenozoic lavas form a bimodal suite of nephelinites (with carbonatite xenoliths) and phonolites emplaced in the Anti-Atlas belt of Morocco. Despite the paucity Of samples With intermediate composition between the two main types of lava (only one phonotephrite flow is reported shows that the two main lithologies call be linked by in this area), whole-rock major or element modelling fractional crystallization. The most primitive modelled cumulates are calcite-bearing olivine clinopyroxenites, whereas the final stages of differentiation are characterized by the formation of nepheline-syenite cumulates. This evolution trend is classically observed in plutonic alkaline massifs associated with carbonatites. Late-stage evolution is responsible for the crystallization of hainite- and delhayelite-bearing microdomains, for the transformation of aegirine-augite into aegirine (or augite into aegirine-augite), and for the crystallization of lorenzenite and a cudialyte-group mineral as replacement products of titanite. These phases were probably formed. either by crystallization from late residual peralkaline melts, or by reaction of pre-existing minerals with such melt, or hydrothermal peralkaline fluid.
引用
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页码:59 / 82
页数:24
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