Mars Goes For A Spin Or At Least Part Of It Might
Planetary scientists have often puzzled over the origins of the Martian landscape, including its so-called hemispheric dichotomy, a pronounced difference in the thickness of the planet’s crust between its northern lowlands and highlands of the south. Another curious feature is an elevated region near the equator called the Tharsis Rise, capped by volcanic peaks located in a relatively straight line. A new study seeks to unify those features by showing how thickness variations in the planet’s outer layers may have given birth to the Tharsis Rise....