2021/04/10 by Felix Jungmann, Gerhard Wurm · 17 citations
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Astro and Planetary Science #Astrophysics #Astrophysics and Star Formation Studies #Charge (physics) #Chemical physics #Context (archaeology) #Coulomb #Geology #Magnetic and Electromagnetic Effects #Materials science #Multipole expansion #Nuclear physics #Particle (ecology) #Particle physics #Physics #Planet #Range (aeronautics) #Triboelectric effect #astro-ph.EP #astro-ph.IM
paper · pdf · doi:10.1051/0004-6361/202039430
published in Astronomy and Astrophysics 650, A77 (EDP Sciences)
openalex publication_date 2021/04/10 · openalex created_date 2021/04/26 · arxiv created 2021/06/02 · arxiv updated 2021/06/09 · openalex updated_date 2026/08/05
Context. Particles in protoplanetary disks go through a number of phases that are dominated by collisions. In each of these events, grains exchange electrical charge via triboelectric effects. This enhances the stability of particle aggregates. Aims. Dielectric grains are easily charged by collisions. Here, we investigate whether a charge is capable of inducing an aggregation of particles and we consider how collision properties, such as sticking velocities and collisional cross-sections, are altered. Methods. We explored aggregation in microgravity experiments based on the observation of the motion of submillimeter (submm) grains following many collisions. In the process, grains attract each other, collide, stick, and ultimately form small aggregates. Results. We observed a bottom-up formation of irregular aggregates from submm grains. While some of the observed trajectories during the approach of grains reflect the presence of a pure Coulomb potential, the motion is not always in agreement with pure Kepler motion. Higher-order potentials of multipole charge distributions stand as a plausible explanation for this behavior. An immediate consequence of charging is that the particles continue to stick to each other at velocities of ~10 cm s −1 , while surface forces of neutral grains are only expected to allow sticking below ~1 mm s −1 . No bouncing collision was observed among hundreds of collisions in the given parameter range. Applied to early phases of planet formation, the forming aggregates are therefore the first steps in a new growth phase beyond the traditional bouncing barrier in planet formation.