Abstract
The Taihe layered gabbro intrusion in the northernmost part of the Panxi district in southwest China is part of the 260 million year old Emeishan Large Igneous Province. This intrusion hosts a giant Fe–Ti oxide deposit with 810 million tonnes of ore reserves, which makes it one of the largest deposits in the Panxi district. The intrusion covers an areal extent of ~13km2 and has a vertical stratigraphic thickness of ~1400m. It can be divided into a lower zone (LZ) of coarse-grained gabbro, apatite-bearing gabbro, troctolite and intercalated gabbro and clinopyroxene-bearing troctolite, followed upward by a middle zone (MZ) of gabbro and intercalated clinopyroxenite, plagioclase-bearing clinopyroxenite with major oxide layers, and an upper zone (UZ) of olivine gabbro and layered gabbro including unmineralized leucogabbro and melanogabbro, with some small oxide ore bodies in the lower part. Each of these ‘zones’ contains oxide minerals and relatively similar lithologies. Ore textures and associated mineral assemblages indicate that the ore bodies formed by crystallization of Fe–Ti–V-rich melt under high oxygen fugacity and a volatile-rich environment during the late-stage of magmatic differentiation. A general systematic variation of major oxides is seen through the intrusion as reflected by a slight overall decrease in MgO and Fe2O3 (as total iron) and an increase in SiO2, Na2O, Al2O3, and CaO upward in the layered sequences. Based on lithology and bulk-rock geochemical features, such as positive Eu anomalies, the Taihe intrusion is inferred to have been derived from a ferropicritic melt and became more evolved in chemistry upward following a tholeiitic differentiation trend with enrichment in Fe, Ti, and V. The Taihe gabbros define a small range of age-corrected εNd(t) (t=260Ma) from −0.6 to 0.7 and (87Sr/86Sr)t ratios ranging from 0.7040 to 0.7050. The relatively lower εNd(t) values and higher (87Sr/86Sr)t ratios compared to those from Lijiang picrite which represents the initial product of Emeishan plume head, combined with the enrichment in light rare earth element (LREE) relative to heavy rare earth element (HREE) as well as negative high field strength element (HFSE; e.g., Nb, Ta, Zr, and Hf) anomalies, suggest that subduction-related material was involved in the source region. We propose that the parental picritic magma was generated from the interaction of the ~260 million year Emeishan mantle plume with the lithospheric mantle, and the picritic magma interacted with an eclogitic component in the lithospheric mantle. In our view, the eclogitic component was derived from the earlier Neoproterozoic subduction. The junction of these subduction-modified lithospheric mantle sources and the Emeishan plume was a possible crucial factor leading to the production of large Fe–Ti oxide deposits in the Panxi area.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.