Mars has northern and southern hemispheres like Earth, but their defining characteristics are markedly different, a phenomenon known as Martian dichotomy. The Southern Highlands are older, higher in elevation and more cratered than the Northern Lowlands. The elevated terrain of the former acts as a natural barrier to airflow, resulting in varied wind patterns and contributing to localized weather phenomena.
Explanations for the origin of this dichotomy primarily surround giant impactors (~2,000 kilometers in diameter) from space and large-scale convective movements of the mantle caused by differences in its temperature and density.
Research published in Geophysical Research Letters has attempted to further unravel this origin story through study of Martian earthquakes, or marsquakes. Much like on Earth, this seismic activity can be used to explore driving mechanisms beneath Mars’s surface.
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