[S-IT32] Do plumes exist?

[SIT32-P04] Genesis of high-Ni olivine phenocrysts of the Dali picrites in the Central Emeishan large igneous province

★Invited Papers

*Wenchang Cai¹, Zhaochong Zhang¹, Jiang Zhu², M. Santosh^1,3, Ronghao Pan¹ (1. China University of Geosciences, Beijing, China, 2.Yunnan Institute of Geological Sciences, Kunming,, China, 3.Department of Earth Sciences, University of Adelaide, Australia)

Keywords:Emeishan large igneous province, Picrite, Olivine, Trace element geochemistry, Mantle plume

The Emeishan Large Igneous Province (ELIP) is considered as one of the typical mantle plume-derived LIPs. The picrites formed at relatively high temperatures in this ELIP provide one of the important lines of argument for the role of mantle plume. Here we report trace element data on olivine phenocrysts in the Dali picrites from the ELIP. The olivines are Ni-rich, and characterized by high (>1.4) 100*Mn/Fe value and low (<13) 10000*Zn/Fe value, indicating a peridotite dominated source. Since olivine-melt Ni partition coefficient (K_DNi^ol/melt) will decrease at high temperature and pressure, the picrites derived from peridotite melting at high pressure and which crystallized olivines at lower pressure can generate high concentrations of Ni in olivine phenocrysts, excluding the necessity of a metasomatic pyroxenite contribution. Based on the Al-in-olvine thermometer, olivine crystallization temperature and mantle potential temperature (T_P) were calculated at ~1491℃ and ~1559℃ respectively. Our results are ~200℃ higher than that of the normal asthenospheric mantle, and are consistent with the role of mantle thermal plume for the ELIP.