A waveform simulation of Phobos, the largest moon of Mars.

The geometrical flexibility of Salvus brings seismic imaging techniques to planets, asteroids and other extraterrestrial bodies. Accurate modeling of surface topography and solid/fluid coupling in the interiorare crucial to understand the seismicity of these objects. For instance, Salvus is used by NASA’s Insight mission to run large-scale simulationsfor various scenarios of the interior structure of Mars.