Compositionally-distinct ultra-low velocity zones on Earths core-mantle boundary

The Earths lowermost mantle large low velocity provinces are accompanied by small-scale ultralow velocity zones in localized regions on the core-mantle boundary. Large low velocity provinces are hypothesized to be caused by large-scale compositional heterogeneity (i.e., thermochemical piles). The origin of ultralow velocity zones, however, remains elusive. Here we perform three-dimensional geodynamical calculations to show that the current locations and shapes of ultralow velocity zones are related to their cause. We find that the hottest lowermost mantle regions are commonly located well within the interiors of thermochemical piles. In contrast, accumulations of ultradense compositionally distinct material occur as discontinuous patches along the margins of thermochemical piles and have asymmetrical cross-sectional shape. Furthermore, the lateral morphology of these patches provides insight into mantle flow directions and long-term stability. The global distribution and large variations of morphology of ultralow velocity zones validate a compositionally distinct origin for most ultralow velocity zones.

Code: CitcomCU (modified)

Mingming Li, Allen K. McNamara, Edward J. Garnero, and Shule Yu (2017). Compositionally-distinct ultra-low velocity zones on Earth’s core-mantle boundary, Nature Communications,  8(1).





Tiny regions of compositionally distinct rock (red material, known as ultra-low velocity zones), collect at Earth’s core-mantle boundary (tan surface), nearly halfway to the center of our planet. Small accumulations of this distinct rock collect near the margins of large thermochemical piles (green) that reside at the base of Earth’s mantle.

Sign In