Context. An asteroid spun up to its critical limit has unique surface mechanical properties that its gravity and the centrifugal force largely balance, creating a relaxation environment where low-energy events such as mass shedding may trigger subsequent long complex motion of an asteroid’s regolith grains. Exploring such an evolution process may provide key clues for understanding the early formation of multi-asteroid systems. Aims. This paper investigates the complex evolution process of loose particles becoming triggered by shedding events and the dependency of their dynamical propagation on the contact mechanical properties of the asteroid surface. Methods. We present a numerical model for tracking the trajectory of a shed particle that...
More than a half of the asteroids in the main belt have irregular shapes with ratios of the minor to...
Recent remote measurements and in-situ observations confirm the idea that asteroids up to few hundre...
.Past collisions determine the current mechanical properties of asteroids, and hence their response ...
Context. An asteroid spun up to its critical limit has unique surface mechanical properties that its...
We investigate the dynamical behaviour of debris ejected from the surface of an asteroid, due to a g...
The regolith transport near the surface of an asteroid is inherently sensitive to the local topograp...
Abstract The regolith transport near the surface of an asteroid is inherently sensitive to the loca...
Conditions for regolith landslides to occur on spinning, gravitat-ing spheroidal asteroids and their...
This simulation is focused on the specific influence of the gravitational field of a very elongate...
By now it has been accepted that most of the small asteroids in the Solar System are granular aggreg...
Understanding asteroid collisional and dynamical evolution necessitates the use of statistical metho...
Asteroids, since the formation of the solar system, are known to have experienced catastrophic colli...
The solar system is sprinkled with detritus known as asteroids, with tens of thousands of these rock...
The rotation rates of asteroids, which are deduced from periodic fluctuations in their brightnesses,...
Context. NASA’s Double Asteroid Redirection Test (DART) mission will kinetically impact Dimorphos, t...
More than a half of the asteroids in the main belt have irregular shapes with ratios of the minor to...
Recent remote measurements and in-situ observations confirm the idea that asteroids up to few hundre...
.Past collisions determine the current mechanical properties of asteroids, and hence their response ...
Context. An asteroid spun up to its critical limit has unique surface mechanical properties that its...
We investigate the dynamical behaviour of debris ejected from the surface of an asteroid, due to a g...
The regolith transport near the surface of an asteroid is inherently sensitive to the local topograp...
Abstract The regolith transport near the surface of an asteroid is inherently sensitive to the loca...
Conditions for regolith landslides to occur on spinning, gravitat-ing spheroidal asteroids and their...
This simulation is focused on the specific influence of the gravitational field of a very elongate...
By now it has been accepted that most of the small asteroids in the Solar System are granular aggreg...
Understanding asteroid collisional and dynamical evolution necessitates the use of statistical metho...
Asteroids, since the formation of the solar system, are known to have experienced catastrophic colli...
The solar system is sprinkled with detritus known as asteroids, with tens of thousands of these rock...
The rotation rates of asteroids, which are deduced from periodic fluctuations in their brightnesses,...
Context. NASA’s Double Asteroid Redirection Test (DART) mission will kinetically impact Dimorphos, t...
More than a half of the asteroids in the main belt have irregular shapes with ratios of the minor to...
Recent remote measurements and in-situ observations confirm the idea that asteroids up to few hundre...
.Past collisions determine the current mechanical properties of asteroids, and hence their response ...