Where Did the Asteroid Fountain's Splashes Land? ✛

Original: "Dynamical evolution and surface accretion of DART impact ejecta in the (65803) Didymos system"
arXiv:2607.26342v1 · 2026-07-28 · CC BY 4.0 · 1 min
Almost all debris knocked out by the probe impact flew away forever, but fine dust covered both asteroids, and in one place — a surprisingly thick layer.

When NASA's DART spacecraft slammed into Dimorphos, the asteroid's moon, the impact sent a plume of debris into space. Scientists tracked the fate of 20 million particles using computer simulations.

Most of the splashes never came back. Some 93,5% of particles were swept away by solar radiation — light pushes on dust grains like wind on a sail. But a fraction fell back. On Dimorphos, dust settled in a layer about 1,5 mm thick. On the larger asteroid Didymos, a dense patch formed, reaching 3 to 11,5 mm in thickness.

It all came down to the direction of the ejecta. If the cloud of fragments flew into the impact direction, Didymos got a thick deposit — as if someone had deliberately splattered paint.

Why does this matter? In 2026, the Hera mission will arrive. It will photograph the dust trails and verify the calculations. It will also avoid dangerous zones with leftover debris. The fountain has nearly dried up. Its pattern on the rocks remains. It will tell us about the force of the impact.

If Dimorphos were the size of a football field, the dust layer that settled would be thinner than a human hair.

Kinetic impact is a favorite trope in Hollywood blockbusters from 'Armageddon' to 'Don't Look Up', but DART was the first real test without nuclear bombs.

v_{\text{max}} = \kappa \, r^{-\gamma}
Exponent γ = 0.4; smaller particles are accelerated to higher speeds
Scientists
John Henry Poynting
Concepts
asteroid belt asteroid impact lunar formation giant impact ejecta