2015
DOI: 10.1016/j.precamres.2015.08.002
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Short-lived high-temperature prograde and retrograde metamorphism in Shaerqin sapphirine-bearing metapelites from the Daqingshan terrane, North China Craton

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Cited by 67 publications
(25 citation statements)
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“…Daqingshan MP pelitic granulite (Cai et al, 2014); 5. Daqingshan Sapphirine-bearing pelitic granulite (Jiao, Guo, Wang, & Peng, 2015); 6. Wulashan MP pelitic granulite (Cai et al, 2016); 7.…”
Section: Tectonic Implicationsmentioning
confidence: 99%
“…Daqingshan MP pelitic granulite (Cai et al, 2014); 5. Daqingshan Sapphirine-bearing pelitic granulite (Jiao, Guo, Wang, & Peng, 2015); 6. Wulashan MP pelitic granulite (Cai et al, 2016); 7.…”
Section: Tectonic Implicationsmentioning
confidence: 99%
“…This model would produce granulites similar to those represented by the HP and MP pelitic granulites, the UHT pelitic granulites, and the garnet‐bearing S‐type granites in the Khondalite Belt (Guo et al., , ; Peng et al., ; Santosh, Tsunogae, et al., ; Yin et al., , ), as well as the spinel‐bearing garnet–sillimanite granulites from the Helanshan in this study. The mantle‐derived magma is considered as the heat source for the UHT metamorphism in the Khondalite Belt, NCC, as evidenced from the existence of coeval mafic intrusion adjacent to UHT rocks (Guo et al., ; Jiao et al., ; Lobjoie et al., ; Peng, Guo, Zhai, & Bleeker, ; Yang et al., ).…”
Section: Discussionmentioning
confidence: 99%
“…1.95–1.94 Ga (Figure b) and experienced the slow close‐to‐isobaric cooling during the period of c . 1.94–1.83 Ga (Gou, Zhang, & Wang, ; Jiao et al., ; Li & Wei, ; Lobjoie et al., ; Zhang et al., ). Thus, we infer that the UHT pelitic granulites were formed in a two‐sided hot collision between the Yinshan and Ordos Terranes at c .…”
Section: Discussionmentioning
confidence: 99%
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