2018
DOI: 10.1002/gj.3270
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Geochemistry and apatite U–Pb geochronology of alkaline gabbros from the Nodoushan plutonic complex, Sanandaj–Sirjan Zone, Central Iran: Evidence for Early Palaeozoic rifting of northern Gondwana

Abstract: The Zagros Orogen formed during the Cenozoic collision of Arabia with Eurasia and resulted in the closure of the Neo‐Tethys Ocean. Collision was preceded by a complicated tectonic history involving Pan‐African orogenesis, Late Palaeozoic rifting and the formation of Neo‐Tethys, and subsequent Mesozoic convergence on the northern margin of the ocean contemporaneous with ophiolite obduction on its southern margin. The Sanandaj–Sirjan Zone (SaSZ) is a metamorphic belt within the Zagros Orogen of Gondwanan provena… Show more

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Cited by 8 publications
(5 citation statements)
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References 117 publications
(216 reference statements)
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“…Tera–Wasserburg U–Pb lower intercept ages and weighted average 207 Pb‐corrected data (a,d), chondrite‐normalized REE patterns (b,e) and ΣLREE versus Sr/Y diagrams (c,f) for the apatite of Cpx amphibolite and hornblende gabbro from the Saga ophiolitic mélange. Data of trace elements of apatite grains in gabbro are from Shahsavari Alavijeh et al (2019) and granulite are from Duan et al (2022). ALK, alkali‐rich igneous; HM, high‐grade metamorphic; IM, mafic I‐type granitoid and mafic igneous; LM, low‐ and medium‐grade metamorphic and metasomatic; S, S‐type granitoid and high aluminium saturation index ‘felsic’ I‐types; UM, ultramafic.…”
Section: Resultsmentioning
confidence: 99%
“…Tera–Wasserburg U–Pb lower intercept ages and weighted average 207 Pb‐corrected data (a,d), chondrite‐normalized REE patterns (b,e) and ΣLREE versus Sr/Y diagrams (c,f) for the apatite of Cpx amphibolite and hornblende gabbro from the Saga ophiolitic mélange. Data of trace elements of apatite grains in gabbro are from Shahsavari Alavijeh et al (2019) and granulite are from Duan et al (2022). ALK, alkali‐rich igneous; HM, high‐grade metamorphic; IM, mafic I‐type granitoid and mafic igneous; LM, low‐ and medium‐grade metamorphic and metasomatic; S, S‐type granitoid and high aluminium saturation index ‘felsic’ I‐types; UM, ultramafic.…”
Section: Resultsmentioning
confidence: 99%
“…Therefore, we cannot directly calculate the magma SiO 2 content either by using fixed KdIAp/normalL ${\text{Kd}}_{\mathrm{I}}^{\text{Ap}/\mathrm{L}}$ value in mafic or felsic silicate melts, or by using a linear fit through the logarithmic KdIAp/normalL ${\text{Kd}}_{\mathrm{I}}^{\text{Ap}/\mathrm{L}}$ values for intermediate melt without knowing the melt REE concentrations. Instead, we have compiled apatite REE compositions from mafic to felsic silicate melts with known SiO 2 contents (Alavijeh et al., 2019; Belousova et al., 2001; Chu et al., 2009; Jiang et al., 2018; Laurent et al., 2017; Mao et al., 2016; Van Hoose et al., 2013; Xing & Wang, 2017; Zhang et al., 2020). Our results show that the REE (e.g., La, Ce, Sm, Gd, and Dy) concentrations of C‐type, R2‐type, and R1‐type apatite domains generally match well with the apatite from melts with SiO 2 of 45–55 wt.%, 55–65 wt.%, and 65–75 wt.%, respectively (Figure 3f).…”
Section: Discussionmentioning
confidence: 99%
“…Apatite crystallized from primitive mafic magma thus contains lower REE and Si concentrations than those from more evolved intermediate-felsic magma (Chu et al, 2009;Laurent et al, 2017;Prowatke & Klemme, 2006). Laurent et al (2017) (Alavijeh et al, 2019;Belousova et al, 2001;Chu et al, 2009;Jiang et al, 2018;Laurent et al, 2017;Mao et al, 2016;Van Hoose et al, 2013;Xing & Wang, 2017;Zhang et al, 2020). Our results show that the REE (e.g., La, Ce, Sm, Gd, and Dy) concentrations of C-type, R2-type, and R1-type apatite domains generally match well with the apatite from melts with SiO 2 of 45-55 wt.%, 55-65 wt.%, and 65-75 wt.%, respectively (Figure 3f).…”
Section: Nature Of the Mixed Magmatic End-membersmentioning
confidence: 99%
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“…The SaSZ is a part of NW‐SE trending Zagros orogen and extends parallel to the Zagros fold‐thrust belt in southwestern Iran (e.g., Babazadeh, Ghorbani, Cottle, & Bröcker, 2019). The SaSZ is over 1,500 km in length and 150–200 Km in width and separates the Central Iranian Terrane, consisting of the Urumieh‐Dokhtar magmatic belt and the Lut, Tabas, and the Yazd blocks, from the Zagros orogen and the Arabian Plate (Babaahmadi et al, 2021; Sarjoughian, Kananian, Haschke, & Ahmadian, 2016; Shahsavari Alavijeh et al, 2019). The rocks are metamorphosed, deformed, and exhumed during the subduction of the Neo‐Tethys Ocean under SaSZ during the Jurassic and during the collision between the Afro‐Arabian continent and the Central Iranian Terrane in Cretaceous–Paleogene times (e.g., Davoudian et al, 2016; Mohajjel, Fergusson, & Sahandi, 2003).…”
Section: Geological Settingmentioning
confidence: 99%