There is increasing evidence that a large fraction of asteroids, and even Phobos, have such low densities (<2 g/cu cm) that the are unlikely to be consolidated rocks in space.-Water is unlikely due to close orbits to the sun. Instead, many of these asteroids are thought to be made up of unconsolidated smaller particles of varying size referred to as rubble piles. Images of the asteroid Itokawa reinforce this hypothesis. What holds the rubble piles together? Gravitational forces alone are not strong enough to hold together rubble pile asteroids, at least not those that are rapidly spinning Van der Waals forces and or Electrostatic forces must therefore be responsible for holding them together. Previous work suggests that electrostatic forces...
Meteorite science is rich with compositional indicators by which we classify parent bodies, but few ...
International audienceSpacecraft missions have observed regolith blankets of unconsolidated subcenti...
The Small Bodies of the Solar System are leftover material from the formation of planets. Compared w...
Space missions and ground-based observations have shown that some asteroids are loose collections of...
We explore the hypothesis that, due to small van der Waals forces between constituent grains, small ...
Abstract Recent observations and theory have indicated that rubble pile asteroids may have a small, ...
The scaling of physical forces to the extremely low ambient gravi-tational acceleration regimes foun...
Multiple sources of evidence suggest that asteroids ranging from hundreds meters to few kilometers i...
Adhesive forces play a significant role on airless bodies due to their weak gravities. Investigating...
The shear and cohesive strengths of a rubble-pile asteroid could influence the critical spin at whic...
Aims. Asteroids have been exposed to impacts since their formation, and as a consequence their surfa...
When the OSIRIS-REx spacecraft pressed its sample collection mechanism into the surface of Bennu, it...
Prior investigations of the behavior of regolith on the surface of planetary bodies has considered t...
When the OSIRIS-REx spacecraft pressed its sample collection mechanism into the surface of Bennu, it...
By now it has been accepted that most of the small asteroids in the Solar System are granular aggreg...
Meteorite science is rich with compositional indicators by which we classify parent bodies, but few ...
International audienceSpacecraft missions have observed regolith blankets of unconsolidated subcenti...
The Small Bodies of the Solar System are leftover material from the formation of planets. Compared w...
Space missions and ground-based observations have shown that some asteroids are loose collections of...
We explore the hypothesis that, due to small van der Waals forces between constituent grains, small ...
Abstract Recent observations and theory have indicated that rubble pile asteroids may have a small, ...
The scaling of physical forces to the extremely low ambient gravi-tational acceleration regimes foun...
Multiple sources of evidence suggest that asteroids ranging from hundreds meters to few kilometers i...
Adhesive forces play a significant role on airless bodies due to their weak gravities. Investigating...
The shear and cohesive strengths of a rubble-pile asteroid could influence the critical spin at whic...
Aims. Asteroids have been exposed to impacts since their formation, and as a consequence their surfa...
When the OSIRIS-REx spacecraft pressed its sample collection mechanism into the surface of Bennu, it...
Prior investigations of the behavior of regolith on the surface of planetary bodies has considered t...
When the OSIRIS-REx spacecraft pressed its sample collection mechanism into the surface of Bennu, it...
By now it has been accepted that most of the small asteroids in the Solar System are granular aggreg...
Meteorite science is rich with compositional indicators by which we classify parent bodies, but few ...
International audienceSpacecraft missions have observed regolith blankets of unconsolidated subcenti...
The Small Bodies of the Solar System are leftover material from the formation of planets. Compared w...