P-T-density diagram of the Fjørtoft gneiss (Table 4)

P-T-density diagram of the Fjørtoft gneiss (Table 4)

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Constraints on density as a function of pressure, temperature, and composition are crucial to understand isostatic movements during geodynamic processes. Here, we provide a systematic series of density diagrams extracted from thermodynamic calculations for a variety of crustal compositions within a wide P–T range. We quantify systematic density cha...

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... if the basalt is compared to a more Fe-and Mg-rich composition, e.g., mix14p, the difference in density is reduced to 4.8%. Massonne et al. (2007) showed that pelitic rocks can get very dense at high to ultrahigh pressures, which is confirmed by our results. We also compute densities for a Fe-and Al-rich natural rock, the Fjørtoft gneiss ( Fig. 11; Table 4), which was found to be the densest meta-pelite by Massonne et al. (2007) at ultrahigh-pressure conditions. The Fjørtoft gneiss yields 3,304 kg/m 3 at 800°C and 2.5 GPa, and the density difference between mafic and pelitic rocks is reduced to 3.7%. At 700°C and 1.2 GPa, the MORB has a density of 3,111 kg/m 3 and a water ...

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... The density of rocks is a function of pressure, temperature, and chemical composition (Duesterhoeft et al., 2014;Semprich et al., 2010). Key metamorphic mineral reactions and phase transitions can therefore produce significant jumps in density within the crust, causing instability. ...
... Other increases in density are associated with garnet and staurolite formation. The modeling result of density is well consistent with systematic density simulation of metapelite in a large ranges of whole rock compositions (Semprich et al., 2010). The generation of partial melts due to reaction between plagioclase, sillimanite and quartz will dramatically decrease bulk-rock density. ...
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... Previous studies have successfully constrained the phase relations and gravity stability of arc crust (Behn & Kelemen, 2006;T. Chapman et al., 2017;De Paoli et al., 2012;Jull & Kelemen, 2001) and lower continental crust (Hacker et al., 2015;Hetényi et al., 2007;Semprich et al., 2010;Sobolev & Babeyko, 1989). However, the effects of compositional heterogeneity, partial melting, and rheology on crustal stability still lack systematic investigations. ...
... Crustal density has been proven to be very sensitive to bulk SiO 2 content, which directly controls the proportion of low-density quartz in quartz-saturated rocks (De Paoli et al., 2012;Semprich et al., 2010). To constrain the minimum silica value required to maintain mafic lower crust neutral buoyancy, we constructed a Python code using the Theriak-Domino (De Capitani & Brown, 1987) program to calculate the densities of global mafic lower crustal xenoliths at P = 21 kbar and T = 900 C (Figure 8a). ...
... Therefore, we predict that only limited mafic rocks appear gravitationally stable at ≥70 km if T Moho = 900 C ( Figure 11). Previous studies indicate that intermediatefelsic rocks have densities lower than the mantle at HP to ultrahigh-pressure (UHP) conditions due to the high proportion of light quartz or coesite (e.g., Massonne, 2009;Semprich et al., 2010;Tassara, 2006). Our modelling also shows that rock density is negatively correlated with bulk SiO 2 (Figure 8a,b), confirming the low densities of silicarich rocks. ...
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... In petrological studies, geotherms T(z) are often approximated by linear or close to linear functions (e.g., Schreyer, 1995;Semprich et al., 2010;Spear, 1993). Using the data on rocks now located at the surface, temperature gradients dT/ dz = 20 and 30 °C/km are often taken for the Archean crust (e.g., Figs. ...
... However more important are not the density changes under diaphthoresis of individual minerals but the densities of primary and secondary polymineralic parageneses under the assumption of an isochemical character of diaphthoresis for all oxide components except H 2 O. Systematic calculations based on the examples of typical rocks have been done by (Massonne, 2009(Massonne, , 2015Massonne and Calderon, 2008;Massonne and Toulkeridis, 2012;Massonne and Willner, 2008;Massonne et al., 2007;Semprich et al., 2010). The results for a specifi c rock are shown in P-T diagrams contoured by isochores in g/cm 3 in the interval of P from 0.2 to 4 GPa, and T from 300 to 1000 °С. ...
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... Âìåñ òå ñ òåì îñòà åò ñÿ ìíî ãî íå îïðå äåë¸ííîñ òåé â îò íî øå íèè ãëó áèí íûõ ìå õà íèç ìîâ, îá óñëî âèâ øèõ ðàç âè òèå ýòèõ ñòðóêòóð. Ïðåä ëî aeåí íûå ðà íåå ìî äå ëè áàñ ñåé íî îá ðà çîâà íèÿ [1,11,12,19] íå îá ú ÿñ íÿ þò áåç ðèô òî âîå çàëî aeå íèå ðàñ ñìàò ðè âà å ìûõ áàñ ñåé íîâ íà äðåâ íåé ïàñ ñèâ íîé ìà òå ðè êî âîé îêðà è íå è ïðî èñ õîae äå íèå èõ ñïå öè ôè ÷åñ êîé îâàëü íîé ôîð ìû. ...
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A dual model of the Paleozoic basins development, disposing on the Late Proterozoic (Pan-African) and the Early Proterozoic (Eburnean) crust, has been proposed. The formation of the first group basins is connected with the subsiding of the sections of the cooling gneissic-domes of«rejuvenated» (Early Precambrian but tectonically reworked at the end of the Proterozoic) Pan-African crust. Accordingly, the development of the second group basins is a result of the Precambrian deep sited (mantle) magmatic chambers cooling and subsiding together with the sites of the old lithosphere, covering them. The manifestation of the Vendian volcanic units on Anti-Atlas, Ugarta, Regibat-Eglab uplifts is the most possible evidence of the mantle magmatic activity, which could create those chambers.
... The body was probably emplaced during the Caledonian Orogeny (Ritzmann & Faleide 2007) as the eastern margin of the Loppa High and Hammerfest Basin is believed to overlap the Caledonian suture zone (Torsvik & Cocks 2017). Depending on local conditions of pressure and temperature, such mafic bodies may be subject to metamorphic phase changes and associated density changes (Semprich et al. 2010). Compression may cause tectonic overpressure leading to densification and events associated with lithosphere heating (such as rifting or a plume) may supply enough heat to trigger phase changes to produce lighter mineral assemblages Burov & Cloetingh 2009;Cloetingh & Burov 2011). ...
... Compression may cause tectonic overpressure leading to densification and events associated with lithosphere heating (such as rifting or a plume) may supply enough heat to trigger phase changes to produce lighter mineral assemblages Burov & Cloetingh 2009;Cloetingh & Burov 2011). Such density changes may in turn cause vertical surface deformation (Kaus et al. 2005;Semprich et al. 2010;Gac et al. 2013Gac et al. , 2014. ...
... Composition of the mafic body. We modelled the pressuretemperature-dependent density of the mafic body assuming a wet mafic gabbroic composition characterized by low SiO 2 content (Rudnick & Fountain 1995;Semprich et al. 2010) (Fig. 4c). Minor differences in assumed composition would, however, result in considerable variations in calculated densities within the mafic body at given changes in pressure and temperature (e.g. ...
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The Loppa High area has been subject to several events of uplift and subsidence from the Late Paleozoic to Present. The driving mechanisms behind the vertical movements, however, are not fully understood. We propose that uplift and subsidence were influenced by the combination of density changes caused by metamorphic phase changes in a 90 × 140 km wide mafic lower crustal body below the Loppa High and local (rift-related) and far-field stress. Through a numerical modelling approach we analyse the tectonically induced variations in pressure and temperature in the lower crust, their influence on phase changes in the mafic body and the affiliated vertical movements. Results show that (1) densification of the mafic body caused by far-field compression associated with the late Triassic westward translation of Novaya Zemlya could cause surface subsidence, (2) heat and fluid influx provided by early Cretaceous rifting could trigger density reduction and surface uplift and (3) the present-day geometry of the Loppa High as observed in seismic data can be reproduced by combining the modelled effect of rift flank uplift and phase changes in the mafic body. Phase change-driven vertical movements may also have affected other structural highs in the western Barents Sea, including the Stappen High.