Cr-Spinel as an Indicator of Cumulates Partial Melting and Liquid Hybridization
Abstract:The Rum Layered Intrusion (Scotland) was emplaced 60.53 ± 0.08 Ma ago , in response to the proto-Iceland plume . The Unit 9 gabbro cumulates were successively intruded by olivine-phyric picritic sills. Reactive liquid flow produced clinopyroxene-poor gabbro, troctolite and dunite restite, and expelled melt crystallized to form gabbro with poikilitic clinopyroxene and Cr-spinel-rich anorthosite . The Cr-spinel origin is strongly debated (e.g. ).
We have run one atmosphere, fO2-controlled equilibrium experiments of the Rum parental picritic parental liquid . At NNO-0.8 conditions, Cr- spinel saturates from 1360°C, olivine from ~1330°C, plagioclase from 1240°C and clinopyroxene from 1220°C, systematically ~40°C above MELTS calculations. Natural Cr- spinel grains have a higher Cr/(Cr+Al+Fe3+) ratio (~0.51 to 0.03) than grains crystallized along the picrite NNO-0.8 liquid line of descent (0.38 to 0.06). Fe3+-rich spinel is abundant (~1 vol%) at NNO+1, and Al-rich spinel occurs as trace at NNO-3. In picrite-troctolite hybrid experiments, plagioclase (~An86) saturates from 1280°C and clinopyroxene from 1200°C. Al- spinel crystallizes at high temperature, and gets more Cr-rich upon cooling, reaching the highest measured Cr/(Cr+Al+Fe3+) ratio of ~0.44 at 1225°C, falling to 0.09 at 1200°C. Plagioclase and clinopyroxene stability plays a major role in spinel composition. Increasing the pressure or the parental magma water content would delay plagioclase saturation and result in spinel with lower Cr/Al ratio.
We deduce that Unit 9 peridotite, troctolite, anorthosite and also gabbro and poikilitic gabbro Cr-rich spinel did not crystallize from the Rum parental picritic liquid. Instead, they crystallized from a hybrid liquid produced by the mixing of invading picritic liquid with a partially molten plagioclase ± clinopyroxene -rich cumulate, leaving an olivine-rich residue/cumulate.
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