[1] The participation of the deep mantle in the global carbon cycle and its ability to sequester carbon over billionyear time scales depends upon the mineralogical host for carbon. Density-functional theory calculations for MgCO 3 -magnesite and structures with tetrahedrally coordinated carbon reveal the stability of magnesite up to $80 GPa, with a bulk modulus of 110 (±2) GPa. Magnesite undergoes a structural transition to a pyroxene-like structure at $80-100 GPa, with a density increase of 4.5-7.1%. Combined with thermodynamic models for the MgSiO 3 -MgCO 3 system, the inter-solubility of MgCO 3 with MgSiO 3 orthoenstatite and perovskite constrains the carbon content in the silicates to an upper bound of 4 and 20 ppm (wt), respectively. The carbon content in lower mantle silicates is estimated to be no more than 1% of the mantle's total carbon budget for degassed regions, such that in even the mantle's most depleted regions, most carbon must be stored in carbonates or diamond. Citation: Panero, W. R., and J. E.Kabbes (2008), Mantle-wide sequestration of carbon in silicates and the structure of magnesite II, Geophys.