Dark matter could be composed of macroscopic objects with large masses and geometric cross-sections spanning many decades. We investigate the potential interaction of such “stuff-sized” dark matter by considering its interactions with asteroids, planetary rings, and terrestrial bodies. This hail of dark matter could catastrophically destroy these Solar System objects, evaporate them from their orbits, or cause substantial cratering. We estimate these effects and use them to place competitive bounds on a wide, previously unconstrained swathe of the dark matter parameter space.

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• Dark matter
• Massive compact halo objects
• Asteroids, meteors, & meteorites
• Planetary satellites & rings