Bimodal volcanism in the Hegau region (SW Germany): Differentiation of primitive melilititic to nephelinitic rocks produces evolved nosean phonolites

Peculiar bimodal volcanism in the Hegau region (SW Germany) comprises two contrasting SiO2-undersaturated rock suites.
(I) Primitive olivine melilitites and melilite-bearing olivine nephelinites (12–9 Ma) are characterized by high MgO, CaO, Fe2O3, TiO2, Ni, V, F, moderate alkalis, Al2O3, P2O5, Ba, Nb, Zr, and low SiO2, Rb, Pb, and U concentrations. The rocks are composed of forsteritic olivine, diopsidic
clinopyroxene, melilite, perovskite, Cr-bearing oxyspinel, F- and Ba-rich mica, and fluorapatite. In rare cases, they contain coeval coarse-grained ijolite patches generated by rapid in-situ fractionation in small melt pockets.
(II) Evolved nosean phonolites (14–11 Ma) comprise high alkalis, Al2O3, SiO2, Rb, Nb, Zr, U, Pb, S, and low MgO, CaO, Fe2O3, TiO2, P2O5, Ba, Ni, and V concentrations, and contain abundant Babearing alkali feldspar and nosean-haüyne-sodalitess macrocrysts, aegirine-augitic clinopyrox-
ene, as well as accessory apatite, titanite, zircon, and pyrochlore.
The melilititic–nephelinitic rocks formed by low degrees of partial melting of a carbonated amphibole ± phlogopite-bearing garnet wehrlite in the uppermost asthenosphere or in the thermal boundary layer and occur
... mehr
also in neighbouring regions. However, their coexistence with evolved nosean phonolites is a unique and so far, unexplained feature in the southern Central European Volcanic Province. Thermodynamic modelling implies that removal of 11–19% oxyspinel, 4–10% olivine, 42–57% clinopyroxene, <3% mica, <9% feldspathoids, <8% feldspar from melilititic–nephelinitic parental melts at upper crustal conditions (~200 MPa) results in significant amounts of phonolitic residues that are compositionally similar to the exposed nosean phonolites. Strongly negative P and Ti anomalies and a trough of MREE in primitive mantlenormalized trace element patterns of phonolites indicate additional fractionation of titanite and apatite,
consistent with the mineralogy of coarse-grained (nepheline) syenitic cumulates, which are present as enclaves in
both rock suites. The modelling results suggest crystallization of the (nepheline) syenite cumulates between 1050
and 800 ◦C and ascent and eruption of the phonolite residues at no less than ~900 ◦C with complete solidification of the observed assemblage at >750 ◦C. Significant crustal assimilation during fractionation appears
unnecessary to explain the mineralogical, mineral chemical, and geochemical characteristics of the phonolites. Prolonged upper crustal differentiation of the magmas in one case (nosean phonolites) and fast ascent of primitive melts in the other (olivine melilitites and melilite-bearing olivine nephelinites) can be explained by stress field changes from an extensional to a more compressive regime, the magma ascent becoming thereby increasingly structurally controlled and supported by brittle deformation.