Matches in SemOpenAlex for { <https://semopenalex.org/work/W2283915301> ?p ?o ?g. }
- W2283915301 endingPage "1406" @default.
- W2283915301 startingPage "1365" @default.
- W2283915301 abstract "Post-collisional (25–8 Ma) ultrapotassic mafic magmatic rocks occur to the north of the India–Asia collision zone within the Lhasa terrane of the southern Tibetan Plateau, forming a near 1000 km long semi-continuous igneous belt. They include both extrusive and intrusive facies, although lava flows dominate. To understand their petrogenesis, the mineral chemistry of olivine phenocrysts and xenocrysts and whole-rock major and trace element and Sr–Nd–Pb isotope data are presented for the most primitive mafic magmatic rocks (MgO > 6 wt %) from west to east. The studied samples are characterized by high MgO (6·28–15·75 wt %), K2O (4·76–8·89 wt %), SiO2 (46·44–59·74 wt %), Ba (1368–14076 ppm), Th (69–336 ppm) and Ni (106–527 ppm) contents. Chondrite-normalized rare earth element (REE) patterns show enrichment in light rare earth elements (LREE), flat heavy REE (HREE) patterns and negative Eu anomalies. These REE patterns have a very distinctive inverted ‘spoon shape’, which appears to be a common characteristic of collision-related ultrapotassic magmas. Primitive mantle-normalized incompatible trace element patterns exhibit strong enrichments in large ion lithophile elements (LILE) relative to high field strength elements (HFSE) and strong negative Ta–Nb–Ti anomalies, which are typical of subduction-related magmas. The ultrapotassic magmatic rocks studied have extremely radiogenic initial Sr isotopic compositions (0·712379–0·737616) and low (143Nd/144Nd)i (0·511662–0·511984). Combined with their Pb isotope compositions [(206Pb/204Pb)i = 18·30–18·92; (207Pb/204Pb)i = 15·65–15·87; (208Pb/204Pb)i = 39·02–39·76] these data are consistent with the involvement of a subducted continental crustal component in their petrogenesis. The Sr–Nd–Pb isotope compositions exhibit linear trends between depleted mid-ocean ridge basalt (MORB)-source mantle (DMM) and Indian continental crust. The extreme enrichment of the upper mantle below south Tibet is considered to result from the addition of components derived from subducted Indian continental crust to the overlying mantle wedge during northward underthrusting of Indian continental lithosphere beneath the Lhasa terrane since India–Asia collision at ∼55 Ma. The post-collisional K-rich mafic magmas in south Tibet were generated by partial melting of pyroxenite in a mantle source region that was created by reaction of hydrous fluids and siliceous melts from subducted granulite–eclogite-facies Indian continental crustal rocks with the surrounding peridotitic mantle. A continuous process from slab roll-back, through break-off, to detachment of the slab may have induced partial melting of the pyroxenites. Cessation of the post-collisional ultrapotassic magmatism at ∼8 Ma may be linked to the onset of flat slab subduction beneath southern Tibet and the elimination of the wedge of Tibetan subcontinental lithospheric mantle and underlying asthenosphere; geophysical data indicate that at the present day eclogite-facies Indian continental crust directly underthrusts the crust of the Lhasa terrane with no intervening mantle wedge. The proportion of the Indian continental crustal component in the mantle source of the ultrapotassic mafic magmas decreases eastward, as do the ages and volumes of the magmatic rocks. There are no outcrops of post-collisional K-rich mafic magmatic rocks (MgO > 6 wt %) to the east of 87°E in the Lhasa terrane, which may indicate a change in subduction geometry at this longitude." @default.
- W2283915301 created "2016-06-24" @default.
- W2283915301 creator A5010805089 @default.
- W2283915301 creator A5031577240 @default.
- W2283915301 creator A5037649757 @default.
- W2283915301 creator A5051788465 @default.
- W2283915301 creator A5063690498 @default.
- W2283915301 date "2015-07-01" @default.
- W2283915301 modified "2023-10-16" @default.
- W2283915301 title "Post-collisional Ultrapotassic Mafic Magmatism in South Tibet: Products of Partial Melting of Pyroxenite in the Mantle Wedge Induced by Roll-back and Delamination of the Subducted Indian Continental Lithosphere Slab" @default.
- W2283915301 cites W128120171 @default.
- W2283915301 cites W1507573241 @default.
- W2283915301 cites W1524759453 @default.
- W2283915301 cites W1528695685 @default.
- W2283915301 cites W1561193515 @default.
- W2283915301 cites W1649557696 @default.
- W2283915301 cites W1963960391 @default.
- W2283915301 cites W1964723921 @default.
- W2283915301 cites W1965806071 @default.
- W2283915301 cites W1967248360 @default.
- W2283915301 cites W1968074232 @default.
- W2283915301 cites W1968771872 @default.
- W2283915301 cites W1973692153 @default.
- W2283915301 cites W1974731988 @default.
- W2283915301 cites W1976788350 @default.
- W2283915301 cites W1977966931 @default.
- W2283915301 cites W1985957692 @default.
- W2283915301 cites W1987562178 @default.
- W2283915301 cites W1990479851 @default.
- W2283915301 cites W1993519551 @default.
- W2283915301 cites W1993779743 @default.
- W2283915301 cites W1996055672 @default.
- W2283915301 cites W1997698506 @default.
- W2283915301 cites W2003584455 @default.
- W2283915301 cites W2003816434 @default.
- W2283915301 cites W2007800361 @default.
- W2283915301 cites W2009267875 @default.
- W2283915301 cites W2010253617 @default.
- W2283915301 cites W2011607179 @default.
- W2283915301 cites W2014789152 @default.
- W2283915301 cites W2017299506 @default.
- W2283915301 cites W2018644516 @default.
- W2283915301 cites W2019165429 @default.
- W2283915301 cites W2020152301 @default.
- W2283915301 cites W2020726550 @default.
- W2283915301 cites W2022449515 @default.
- W2283915301 cites W2023318308 @default.
- W2283915301 cites W2024005564 @default.
- W2283915301 cites W2025603156 @default.
- W2283915301 cites W2027225510 @default.
- W2283915301 cites W2029330897 @default.
- W2283915301 cites W2030386953 @default.
- W2283915301 cites W2035956928 @default.
- W2283915301 cites W2036078919 @default.
- W2283915301 cites W2036599753 @default.
- W2283915301 cites W2040029696 @default.
- W2283915301 cites W2041774199 @default.
- W2283915301 cites W2042423268 @default.
- W2283915301 cites W2045699793 @default.
- W2283915301 cites W2046761384 @default.
- W2283915301 cites W2047567126 @default.
- W2283915301 cites W2049451277 @default.
- W2283915301 cites W2054368497 @default.
- W2283915301 cites W2054564274 @default.
- W2283915301 cites W2055859870 @default.
- W2283915301 cites W2058269792 @default.
- W2283915301 cites W2059133260 @default.
- W2283915301 cites W2061751167 @default.
- W2283915301 cites W2063215451 @default.
- W2283915301 cites W2064642826 @default.
- W2283915301 cites W2065105994 @default.
- W2283915301 cites W2065581078 @default.
- W2283915301 cites W2068531306 @default.
- W2283915301 cites W2071612360 @default.
- W2283915301 cites W2074324100 @default.
- W2283915301 cites W2075307803 @default.
- W2283915301 cites W2075792469 @default.
- W2283915301 cites W2076373269 @default.
- W2283915301 cites W2076566162 @default.
- W2283915301 cites W2076755830 @default.
- W2283915301 cites W2077039816 @default.
- W2283915301 cites W2078544391 @default.
- W2283915301 cites W2079640846 @default.
- W2283915301 cites W2079993403 @default.
- W2283915301 cites W2081673195 @default.
- W2283915301 cites W2081677058 @default.
- W2283915301 cites W2082270291 @default.
- W2283915301 cites W2083226499 @default.
- W2283915301 cites W2085181355 @default.
- W2283915301 cites W2085292995 @default.
- W2283915301 cites W2086227631 @default.
- W2283915301 cites W2086540936 @default.
- W2283915301 cites W2086820683 @default.
- W2283915301 cites W2088284794 @default.
- W2283915301 cites W2092198681 @default.
- W2283915301 cites W2092367277 @default.
- W2283915301 cites W2094147317 @default.
- W2283915301 cites W2097312591 @default.