Ultralow velocity zones are the largest seismic anomalies in the mantle, with 10-30% seismic velocity reduction observed in thin layers less than 20-40 km thick, just above the Earth's core-mantle boundary (CMB). The presence of silicate melts, possibly a remnant of a deep magma ocean in the early Earth, have been proposed to explain ultralow velocity zones. It is, however, still an open question as to whether such silicate melts are gravitationally stable at the pressure conditions above the CMB. Fe enrichment is usually invoked to explain why melts would remain at the CMB, but this has not been substantiated experimentally. Here we report in situ high-pressure acoustic velocity measurements that suggest a new transformation to a denser structure of MgSiO 3 glass at pressures close to those of the CMB. The result suggests that MgSiO 3 melt is likely to become denser than crystalline MgSiO 3 above the CMB. The presence of negatively buoyant and gravitationally stable silicate melts at the bottom of the mantle, would provide a mechanism for observed ultralow seismic velocities above the CMB without enrichment of Fe in the melt. An ultradense melt phase and its geochemical inventory would be isolated from overlying convective flow over geologic time.dynamics | early Earth evolution | high-pressure experiment | sound velocity measurement | pressure-induced polymorphism T he buoyancy relations between silicate melts and crystals in a deep terrestrial magma ocean are the primary constraints on the possible chemical stratification of Earth's interior (1, 2). The nature of silicate melts under high-pressure conditions is therefore critically important for elucidating the formation and differentiation of the Earth through massive primordial melting of the proto-Earth. Extensive melting of the proto-Earth and the formation of a deep magma ocean, induced by massive planetesimal collisions and possibly encompassing an entire planet, facilitated metal-silicate (core-mantle) segregation, with the subsequent fractional crystallization of silicate melt leading to chemical and gravitational equilibrium (3-6). Because of the high compressibility of melts, a density crossover between crystals and coexisting magmas is expected in the course of fractional crystallization in a deep magma ocean, which would enhance chemical differentiation and could result in a stratified structure of the Earth's interior (7,8). The possible presence of dense, gravitationally stable magmas deep within the Earth at pressures above 100 gigapascals (GPa) has thus been proposed as a consequence of partial melting and a remnant of a deep magma ocean (9, 10), which might explain the observation of anomalously ultralow seismic velocities (ULVZ) above the core-mantle boundary (CMB) (11). However, the behavior of silicate melts under such extreme pressures is poorly understood, and it is still an open question as to whether a density crossover between silicate melt and coexisting mantle phases occurs in the D′′ region above the CMB (approximately 2,900 km dep...