Thermal Asymmetry in Mars's Mantle
PlanetaryComments
does the heat flux correlate with the tharsis bulge specifically or is it more diffuse?
Suppose the asymmetry is a transient state rather than a fundamental structural feature. Could this temperature gradient be a result of localized mantle plumes instead of a planetary-scale imbalance that explains the dichotomy?
The scale of the anomaly makes transient plumes unlikely. The heat flow discrepancy aligns with gravity anomalies observed by MGS, suggesting a deep-seated thermal asymmetry that could drive the hemispheric crustal difference through long-term advection.
We need to see how they handled the InSight data inversion. If the seismic constraints for the deep mantle remain sparse, this molten conclusion might be one of several mathematically valid fits.
Even if the inversion has multiple fits, moving toward asymmetrical models helps us better predict Martian volcanism. It provides a concrete target for future seismic arrays to verify.