Cohesion of regolith: Measurements of meteorite powders

Abstract

The cohesion of particles has a significant effect on the properties of small bodies. In this study, we measured in open air, the cohesive forces of tens of micron-sized irregularly shaped meteorite, silica sand, glass powder, and spherical glass particles, using a centrifugal method. In addition, we estimated the amount of water vapor adsorbed on the particles under the measurement conditions. The measured cohesive forces of the meteorite particles are tens of times smaller than those of an ideally spherical silica particle and correspond to the submicron-scale effective (or equivalent) curvature radius of the particle surface. Moreover, based on the estimated amount of water vapor adsorbed on the particles, we expect the cohesive forces of the particles in airless bodies to be approximately 10 times larger than those measured in open air. Based on the measurement results, we estimate that the cohesive forces of the particles on asteroids are typically in the sub-micro-Newton range, and that the particles on fast-rotating asteroids are tens of microns in size.

arXiv comment32 pages, 9 figures, 7 tables. Accepted for publication in Icarus

References in corpus (10)

• Scaling forces to asteroid surfaces: The role of cohesion
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• Cohesion of Amorphous Silica Spheres: Toward a Better Understanding of the Coagulation Growth of Silicate Dust Aggregates
• Sticking Properties of Silicates in Planetesimal Formation Revisited
• Internal Structure of Asteroids Having Surface Shedding due to Rotational Instability
• Constraints on the Physical Properties of Main Belt Comet P/2013 R3 from its Breakup Event
• A 2 km-size asteroid challenging the rubble-pile spin barrier - a case for cohesion
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• Packing fraction of clusters formed in free-falling granular streams based on flash X-ray radiography
• Deformation of a rotated granular pile governed by body-force-dependent friction
• Impact disruption of Bjurböle porous chondritic projectile
• The Impact of Silicate Grain Coagulation on Millimeter Emission from Massive Protostellar Disks