2007
DOI: 10.1016/j.precamres.2006.11.015
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Paleoproterozoic potassic–ultrapotassic magmatism: Morro do Afonso Syenite Pluton, Bahia, Brazil

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Cited by 45 publications
(45 citation statements)
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“…Three models are commonly invoked to explain the genesis of alkaline igneous rocks: (1) crustal contamination of mantle-derived melt (e.g., Zhao et al, 1995;Wickham et al, 1996;Panter et al, 1997;Aydin et al, 2008;Yang et al, 2008); (2) fractional crystallization of mantle-derived alkali magmas (e.g., Panter et al, 1997;Weis et al, 1998;Battistini et al, 1998;Yang et al, 2005;Holbig and Grove, 2008); and (3) the partial melting of an enriched lithospheric mantle (e.g., Turner et al, 1996;Miller et al, 1999;Williams et al, 2004;Rios et al, 2007;Peng et al, 2008;Zhao et al, 2009aZhao et al, , 2009bHuang et al, 2010 (Fig. 10), and extreme enrichment in LILEs (e.g., Rb, Ba, and Sr) with negative Ta, Nb, and Ti anomalies (Fig.…”
Section: Genesis Of Cenozoic Mg-rich Potassic Rocks In Tibetmentioning
confidence: 99%
“…Three models are commonly invoked to explain the genesis of alkaline igneous rocks: (1) crustal contamination of mantle-derived melt (e.g., Zhao et al, 1995;Wickham et al, 1996;Panter et al, 1997;Aydin et al, 2008;Yang et al, 2008); (2) fractional crystallization of mantle-derived alkali magmas (e.g., Panter et al, 1997;Weis et al, 1998;Battistini et al, 1998;Yang et al, 2005;Holbig and Grove, 2008); and (3) the partial melting of an enriched lithospheric mantle (e.g., Turner et al, 1996;Miller et al, 1999;Williams et al, 2004;Rios et al, 2007;Peng et al, 2008;Zhao et al, 2009aZhao et al, , 2009bHuang et al, 2010 (Fig. 10), and extreme enrichment in LILEs (e.g., Rb, Ba, and Sr) with negative Ta, Nb, and Ti anomalies (Fig.…”
Section: Genesis Of Cenozoic Mg-rich Potassic Rocks In Tibetmentioning
confidence: 99%
“…The age of the beginning of the sedimentation remains undetermined, but we believe that it is not older than 1.8 Ga because rifts typically record relatively short periods of subsidence (e.g., Sengör, 1995). The Rhyacian source may originate from sin-to post-orogenic granites that are related to the orogenic activities along the belts, which sutured the several crustal blocks that constituted a large paleocontinent, including the Congo and São Francisco domains (for example, Rosa et al, 2000;Conceição et al, 2002Conceição et al, , 2003Conceição et al, , 2007Paim et al, 2002;Rios et al, 2007). The Archean sources are found in the Gavião block (e.g., Nutman and Cordani, 1992;Mougeot, 1996;Pinto et al, 1998;Rosa et al, 2000;Teixeira et al, 2000;Sabaté, 2002, 2004;Lana et al, 2013), which constitutes the main basement of the studied region.…”
Section: Origin and Age Of Riftingmentioning
confidence: 99%
“…The later alkaline plutons, emplaced over the time span 2111e2070 Ma, are represented by syenites, monzonites, tonalites, granites and granodiorites, ranging from high-K calc-alkaline to shoshonite and ultrapotassic (Rios et al, 2007).…”
Section: Geological Settingmentioning
confidence: 99%
“…The plutonic activity at this time, in contrast to the early TTG and calcalkaline plutons, consists of relatively low silica granitoids with high-K 2 O contents and negative eNd(t) values emplaced along the greenstone belt-Archaean basement boundary. This K-rich magmatism is represented by ultrapotassic syenites (Conceição et al, 2002;Rios et al, 2007), lamprophyres (Plá Cid. et al, 2006), and shoshonitic to high-K calc-alkaline granitoids (Nascimento, 1996;Carvalho and Oliveira, 2003;Costa, 2008).…”
Section: Introductionmentioning
confidence: 99%