1. Asthenospheric kimberlites: Volatile contents and bulk compositions at 7 GPa.
- Author
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Stamm, Natalia and Schmidt, Max W.
- Subjects
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KIMBERLITE , *GEOCHEMISTRY , *MAGMATISM , *CARBONATITES , *EARTH'S mantle - Abstract
During ascent, kimberlites react with the lithospheric mantle, entrain and assimilate xenolithic material, loose volatiles and suffer from syn- and post-magmatic alteration. Consequently, kimberlite rocks deviate heavily from their primary melt. Experiments at 7 GPa, 1300–1480 °C, 10–30 wt% CO 2 and 0.46 wt% H 2 O on a proposed primitive composition from the Jericho kimberlite show that saturation with a lherzolitic mineral assemblage occurs only at 1300–1350 °C for a carbonatitic melt with <8 wt% SiO 2 and >35 wt% CO 2 . At asthenospheric temperatures of >1400 °C, where the Jericho melt stays kimberlitic, this composition saturates only in low-Ca pyroxene, garnet and partly olivine. We hence forced the primitive Jericho kimberlite into multiple saturation with a lherzolitic assemblage by adding a compound peridotite. Saturation in olivine, low- and high-Ca pyroxene and garnet was obtained at 1400–1650 °C (7 GPa), melts are kimberlitic with 18–29 wt% SiO 2 + Al 2 O 3 , 22.1–24.6 wt% MgO, 15–27 wt% CO 2 and 0.4–7.1 wt% H 2 O; with a trade-off of H 2 O vs. CO 2 and temperature. Melts in equilibrium with high-Ca pyroxene with typical mantle compositions have ≥2.5 wt% Na 2 O, much higher than the commonly proposed 0.1–0.2 wt%. The experiments allow for a model of kimberlite origin in the convective upper mantle, which only requires mantle upwelling that causes melting at the depth where elemental carbon (in metal, diamond or carbide) converts to CO 2 (at ∼250 km). If primary melts leading to kimberlites contain a few wt% H 2 O, then adiabatic temperatures of 1400–1500 °C would yield asthenospheric mantle melts that are kimberlitic (>18 wt% SiO 2 + Al 2 O 3 ) but not carbonatitic (<10 wt% SiO 2 + Al 2 O 3 ) in composition, carbonatites only forming 100–200 °C below the adiabat. These kimberlites represent small melt fractions concentrating CO 2 and H 2 O and then acquire part of their chemical signature by assimilation/fractionation during ascent in the subcratonic lithosphere. [ABSTRACT FROM AUTHOR]
- Published
- 2017
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