Free Collisions in a Microgravity Many-Particle Experiment. I. Dust Aggregate Sticking at Low Velocities

TL;DR

This study used a microgravity experiment to observe dust-aggregate collisions at very low velocities, revealing a probabilistic sticking behavior and establishing a critical velocity below which aggregates always stick, informing planetesimal formation models.

Contribution

First experimental measurement of dust-aggregate sticking at velocities as low as 0.1 cm/s, providing new insights into the early stages of planetesimal growth.

Findings

Seven out of 125 collisions resulted in sticking.

Identified a velocity threshold (~8e-5 m/s) for guaranteed sticking.

Developed a physical model explaining dust-aggregate sticking behavior.

Abstract

Over the past years the processes involved in the growth of planetesimals have extensively been studied in the laboratory. Based on these experiments, a dust-aggregate collision model was developed upon which computer simulations were based to evaluate how big protoplanetary dust aggregates can grow and to analyze which kinds of collisions are relevant in the solar nebula and are worth further studies in the laboratory. The sticking threshold velocity of millimeter-sized dust aggregates is such a critical value that had so far only theoretically been derived, as the relevant velocities could not be reached in the laboratory. We developed a microgravity experiment that allows us for the first time to study free collisions of mm-sized dust aggregates down to velocities of ~0.1 cm/s to assess this part of the protoplanetary dust evolution model. Here, we present the results of 125 free collisions between dust aggregates of 0.5 to 2 mm diameter. Seven collisions with velocities between 0.2 and 3 cm/s led to sticking, suggesting a transition from perfect sticking to perfect bouncing with a certain sticking probability instead of a sharp velocity threshold. We developed a model to explain the physical processes involved in dust-aggregate sticking, derived dynamic material properties of the dust aggregates from the results of the collisions, and deduced the velocity below which aggregates always stick. For millimeter-sized porous dust aggregates this velocity is 8e-5 m/s.