Photographs of the asteroid Itokawa reveal unexpectedly strong size segregation between lowlands populated almost entirely by small pebbles and highlands consisting of larger boulders. We propose that this segregation may be caused by a simple and unexplored effect: pebbles accreting onto the asteroid rebound from boulders, but sink into pebbly regions. By number, overwhelmingly more particles on Itokawa are pebbles, and collisions involving these pebbles must unavoidably cause pebbly regions to grow. We carry out experiments and simulations that demonstrate that this mechanism of size sorting based on simple counting of grains produces strong lateral segregation that reliably obeys an analytic formula
Crucial questions for possible utilization of Near Earth Asteroids include how to break asteroid mat...
Many asteroids with low bulk densities must have a rubble pile structure and internal voids. Althoug...
International audienceWe have developed a new version of the code built by Campo Bagatin \al, 1994a,...
We investigate the dynamics of regolith on rubble-pile asteroids to explain granular processes obser...
This thesis focuses on particle size segregation in rubble-pile asteroids, mostly by using numerical...
Cette thèse porte sur la ségrégation granulaire au sein des astéroïdes lâchement agglomérés, avec un...
In order to understand the geological evolution of asteroids Eros, Itokawa and Ryugu and their colli...
High-resolution images of the surface of asteroid Itokawa from the Hayabusa mission reveal it to be ...
The carbonaceous asteroid (162173) Ryugu formed from fragments which re-accreted after its parent bo...
Small asteroids are often considered to be rubble-pile objects, and such asteroids may be the most l...
International audience; There have been attempts in the past to fit the observed bulk shapes (axial ...
Recent asteroid missions have revealed that many sub-kilometer asteroids are rubble piles. Large par...
Crucial questions for possible utilization of Near Earth Asteroids include how to break asteroid mat...
Space missions and ground-based observations have shown that some asteroids are loose collections of...
Aims. Asteroids have been exposed to impacts since their formation, and as a consequence their surfa...
Crucial questions for possible utilization of Near Earth Asteroids include how to break asteroid mat...
Many asteroids with low bulk densities must have a rubble pile structure and internal voids. Althoug...
International audienceWe have developed a new version of the code built by Campo Bagatin \al, 1994a,...
We investigate the dynamics of regolith on rubble-pile asteroids to explain granular processes obser...
This thesis focuses on particle size segregation in rubble-pile asteroids, mostly by using numerical...
Cette thèse porte sur la ségrégation granulaire au sein des astéroïdes lâchement agglomérés, avec un...
In order to understand the geological evolution of asteroids Eros, Itokawa and Ryugu and their colli...
High-resolution images of the surface of asteroid Itokawa from the Hayabusa mission reveal it to be ...
The carbonaceous asteroid (162173) Ryugu formed from fragments which re-accreted after its parent bo...
Small asteroids are often considered to be rubble-pile objects, and such asteroids may be the most l...
International audience; There have been attempts in the past to fit the observed bulk shapes (axial ...
Recent asteroid missions have revealed that many sub-kilometer asteroids are rubble piles. Large par...
Crucial questions for possible utilization of Near Earth Asteroids include how to break asteroid mat...
Space missions and ground-based observations have shown that some asteroids are loose collections of...
Aims. Asteroids have been exposed to impacts since their formation, and as a consequence their surfa...
Crucial questions for possible utilization of Near Earth Asteroids include how to break asteroid mat...
Many asteroids with low bulk densities must have a rubble pile structure and internal voids. Althoug...
International audienceWe have developed a new version of the code built by Campo Bagatin \al, 1994a,...