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Quaternary post-collisional high Nb-like basalts from Bijar-Qorveh, NW Iran: A metasomatized lithospheric mantle source
被引:3
|作者:
Akbari, Meysam
[1
]
Ghorbani, Mohammad Reza
[1
]
Cousens, Brian L.
[2
]
Graham, Ian T.
[3
]
机构:
[1] Tarbiat Modares Univ TMU, Dept Geol, Tehran 14115175, Iran
[2] Carleton Univ, Ottawa Carleton Geosci Ctr, Dept Earth Sci, Ottawa, ON K1S 5B6, Canada
[3] Univ New South Wales, Sch Biol Earth & Environm Sci, Sydney, NSW 2052, Australia
来源:
关键词:
Sanandaj-Sirjan Zone;
High Nb-like basalts;
Post-collision;
Metasomatized lithosphere;
Stratified SCLM;
SANANDAJ-SIRJAN ZONE;
VOLCANIC FIELD;
CHEMICAL CLASSIFICATION;
CONTINENTAL COLLISION;
THERMAL STRUCTURE;
MAGMATIC SYSTEMS;
ALKALI BASALTS;
ORIGIN;
LAVAS;
EVOLUTION;
D O I:
10.1016/j.lithos.2022.106781
中图分类号:
P3 [地球物理学];
P59 [地球化学];
学科分类号:
0708 ;
070902 ;
摘要:
The Quaternary Bijar-Qorveh mafic volcanic rocks (BQMVR) occur in the Sanandaj-Sirjan Zone (SSZ) of Iran, a segment of the Alpine-Himalayan Orogeny with a Gondwana-affinity basement. Phases 1 and 2 of BQMVR are silica-undersaturated (basanite, tephrite, and phonotephrite) and form a highly alkaline or HA suite. The last phase, phase 3, of BQMVR is silica-saturated (alkali olivine basalt and hawaiite) and is called the mildly alkaline or MA suite. BQMVR share well-known subduction-related negative Nb-Ta anomalies, and their Nb abundances are high enough to be classified as 'high-Nb like basalts'. However, they do not show geochemical characteristics of typical high-Nb basalts. Trace element abundances and patterns of the MA suite mimic garnet-bearing spinel peridotite partial melts, whereas the HA suite is too rich in incompatible trace elements to match normal mantle partial melts. Enriched trace element patterns of the HA suite are akin to hornblendite experimental partial melts, and are likely derived from a garnet-amphibole peridotite source. Sr-Nd-Pb isotopic characteristics of the BQMVR indicate a subcontinental lithospheric mantle affinity. The HA suite tends toward the EM1 array, whereas the MA suite follows the EM2 array. The highly radiogenic Sr-Nd isotopes of the MA suite indicate significant crustal contamination. Lithospheric delamination beneath the SSZ that followed Arabia-Eurasia collision, triggered garnet-amphibole peridotite partial melting that interacted with 10-30% of the asthenospheric component to have formed the HA suite. Mantle melting at shallower lithosphere depths followed and produced the MA suite. MELTS modeling shows the BQMVR underwent fractional crystallization of clinopyroxene +/- olivine. Whole-rock thermobarometric calculations suggest derivation of the primary melts at a depth of similar to 97 km, however the Cpx-thermobarometer indicates that such melts equilibrated at lower crust depths at a depth of 45 km close to the Moho. The present Quaternary volcanostratigraphic study provides substantial clues for major post-collisional alkaline high-Nb mafic volcanism bearing signatures of two distinct magmatic stages; an early phase (phases 1 and 2) rooted in a deeper garnet amphibole peridotite followed by phase 3 rooted in a garnet-poor spinel peridotite.
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