The hemispheric dichotomy between the southern highlands and northern lowlands on Mars is characterized by a change in crustal thickness along an apparently irregular boundary, which can be traced around the planet, except where it is presumably buried beneath the Tharsis volcanic rise. The gravity and topography of Mars is used to constrain the location of the dichotomy boundary beneath Tharsis, and finds that the dichotomy boundary along its entire path around the planet is accurately fit by an ellipse measuring about 10,600 by 8,500 km.
- Jeffrey C. Andrews-Hanna
- Maria T. Zuber
- W. Bruce Banerdt