Oxygen fugacity-dependent stability of magnesite along slab geotherms

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ABSTRACT Magnesite is recognized as a key host of oxidized carbon in the subducted slabs and plays a fundamental role in transporting and storing carbon into the deep Earth. Here, we investigate the stability of magnesite at 14 GPa, 900–1700°C, and oxygen fugacity ( f O 2 ) from the nickel-nickel oxide (Ni-NiO) to iron-wüstite (IW) buffers, using a multi-anvil apparatus. Using ex-situ Raman spectroscopy and ex-situ scanning electron microscopy energy-dispersive spectroscopy, we demonstrate that the magnesite-diamond/graphite boundary along hot slab geotherms tends to occur at higher oxygen fugacity compared to the average mantle, reaching values above IW+3.5 at 14 GPa. We further model that, along cold slab geotherms, magnesite can retain its stability even under highly reduced conditions, whereas it would transform into graphite along hot slab geotherms.

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