Why is the areoid like the residual geoid?

[1] The equipotential figures of Earth (residual geoid), and of Mars (areoid) are characterized by pairs of elevated and pairs of depressed antipodal equatorial regions. Elevated regions of the residual geoid lie vertically above the two Large Low Shear Wave Velocity Provinces (LLSVPs) on the Core Mantle Boundary (CMB). There is evidence that the LLSVPs are dense, physicochemically distinct, and have been stable in their positions with respect to each other and to the Earth’s spin axis for at least 550 My. The final event in the planetary-scale development of the Earth’s structure was the moon-forming event and the comparable event on Mars is thought by many to have been the Borealis basinforming impact. We attribute the formation of the LLSVPs and postulated comparable masses underlying the elevated regions of the areoid on the CMB of Mars, to the immediate after-effects of those two giant impacts. Citation: Burke, K., S. C. Werner, B. Steinberger, and T. H. Torsvik (2012), Why is the areoid like the residual geoid?, Geophys. Res. Lett., 39, L17203, doi:10.1029/2012GL052701.