Nature Astronomy, Published online: 18 August 2026; doi:10.1038/s41550-026-02956-w Simulations show that the large depression at the south pole of the Martian moon Deimos formed in an oblique impact that also smoothed its surface, revealing a very weak surface over a porous, fractured, rubble-pile-like interior.
Deimos’s shape and geology explained by a subcatastrophic impact
S. Sugita

