Mg(3)Al(2)Si(3)O(12) jeffbenite inclusion in super-deep diamonds is thermodynamically stable at very shallow Earth's depths

超深钻石中的 Mg(3)Al(2)Si(3)O(12) 杰夫宾石包裹体在地球极浅深度处具有热力学稳定性。

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Abstract

Jeffbenite (having the same chemical composition of pyrope, ~ Mg(3)Al(2)Si(3)O(12), and also known as TAPP phase) is a mineral inclusion only found in diamonds formed between about 300 and 1000 km depth) and is considered a stable phase in the transition zone (410-660 km depth) and/or in the shallowest regions of the lower mantle (around 660-700 km depth). This rare and enigmatic mineral is considered to be a pressure marker for super-deep diamonds and therefore it has a key role in super-deep diamond research. However, the pressure-temperature stability fields for Mg(3)Al(2)Si(3)O(12) jeffbenite is unknown and its actual formation conditions remain unexplored. Here we have determined the thermodynamic pressure-temperature stability field for the jeffbenite Mg-end member and surprisingly discovered that it is stable at low pressure-temperature conditions, i.e., 2-4 GPa at 800 and 500 °C. Thus, Mg(3)Al(2)Si(3)O(12) jeffbenite is not the high-pressure polymorph of pyrope and is likely a retrogressed phase formed during the late ascent stages of super-deep diamonds to the surface.

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