High-pressure experiments and theoretical calculations demonstrate that an iron-rich ferromagnesian silicate phase can be synthesized at the pressure-temperature conditions near the coremantle boundary. The iron-rich phase is up to 20% denser than any known silicate at the core-mantle boundary. The high mean atomic number of the silicate greatly reduces the seismic velocity and provides an explanation to the low-velocity and ultra-low-velocity zones. Formation of this previously undescribed phase from reaction between the silicate mantle and the iron core may be responsible for the unusual geophysical and geochemical signatures observed at the base of the lower mantle.core-mantle boundary ͉ high pressure ͉ mineral physics ͉ post-perovskite M odern deep-Earth mineralogical research began with highpressure experiments on iron silicate, a major component in the solid Earth. The discovery of the fayalite (Fe 2 SiO 4 ) olivine-spinel transition in 1959 (1) marked the first known transition beyond the upper mantle. The disproportionation of fayalite spinel into mixed oxides using the newly invented laser-heated and resistive-heated diamond-anvil cell in the early 1970s (2, 3) marked the first phase transition under lower mantle conditions. In the Earth's crust, upper mantle, and transition zone, iron silicates form extensive solid solutions with the magnesium endmembers in major rock-forming minerals, e.g., fayalite in ␣-(Fe,Mg) 2 SiO 4 (olivine), ferrosilite in (Fe,Mg)SiO 3 (pyroxene), almandine in (Fe,Mg) 3 Al 2 Si 3 O 12 (garnet), and fayalite spinel in ␥-(Fe,Mg) 2 SiO 4 (ringwoodite). No iron-rich silicate, however, was known to exist under the high pressuretemperature (P-T) conditions beyond the 670-km discontinuity that accounts for approximately three-quarters of the Earth's total silicates and oxides. Following Birch's 1952 postulation (4), iron-rich silicates break down to mixed oxides in the lower mantle.In the lower-mantle silicate, (Fe x Mg 1Ϫx )SiO 3 perovskite, iron can only participate as a minor component with x Ͻ 0.15 (5), even at the core-mantle boundary with an unlimited supply of iron from the core. Without a stable iron-rich silicate phase, previous explanations of the complex geochemical and geophysical signatures of the DЉ layer have been limited to heterogeneous, solid͞melt mixtures of iron-poor silicates and iron-rich metals and oxides (6, 7). Recently, MgSiO 3 has been found to transform from perovskite to CaIrO 3 structure under the P-T conditions of the DЉ layer (8)(9)(10)(11)(12). This postperovskite (ppv) phase also was observed to coexist with silicate perovskite and magnesiowüstite in experiments with orthopyroxene and olivine starting materials with x up to 0.4, but the iron content in this phase is undefined because of the unknown Fe͞Mg distributions among multiple coexisting ferromagnesian phases (13). Here, we report experimental and theoretical investigations across the ferrosilite (FeSiO 3 )-enstatite (MgSiO 3 ) join. We found that iron-rich (Fe x Mg 1Ϫx )SiO 3 with x as high as 0...