Context. Impacts on small-body surfaces can occur naturally during cratering events or even strategically during carefully planned impact experiments, sampling maneuvers, and landing attempts. A proper interpretation of impact dynamics allows for a better understanding of the physical properties and the dynamical process of their regolith-covered surfaces and their general evolution. Aims. This work aims to first validate low-velocity, low-gravity impact simulations against experimental results, and then to discuss the observed collision behaviors in terms of a popular phenomenological collision model and a commonly referenced scaling relationship. Methods. We performed simulations using the soft-sphere discrete element method and two diffe...
The penetration by a gravity-driven impact of a solid sphere into a granular medium is studied by tw...
Abstract The dusty regolith covering the surfaces of asteroids and planetary satellites differs in s...
Collisions between planetary ring particles and in some protoplanetary disk environments occur at lo...
Impacts on small-body surfaces can occur naturally during cratering events or even strategically dur...
Context. Slow interactions on small body surfaces occur both naturally and through human interventio...
Slow interactions on small body surfaces occur both naturally and through human intervention. The re...
International audienceWith the flourishing number of small body missions that involve surface intera...
International audienceIn order to improve our understanding of landing on small bodies and of astero...
Oblique, low-velocity impacts onto extraterrestrial terrain are an inevitable occurrence during spac...
Context. Landing on the surface of small bodies is particularly challenging, as the physical propert...
International audienceContext. Landing on the surface of small bodies is particularly challenging, a...
This book focuses on the impact dynamics and cratering of soft matter to describe its importance, di...
Even if craters are very common on Solar System body surfaces, crater formation in granular media su...
The dusty regolith covering the surfaces of asteroids and planetary satellites differs in size, shap...
Context. In situ observations of small asteroids, such as Itokawa, Ryugu, and Bennu, show that surfa...
The penetration by a gravity-driven impact of a solid sphere into a granular medium is studied by tw...
Abstract The dusty regolith covering the surfaces of asteroids and planetary satellites differs in s...
Collisions between planetary ring particles and in some protoplanetary disk environments occur at lo...
Impacts on small-body surfaces can occur naturally during cratering events or even strategically dur...
Context. Slow interactions on small body surfaces occur both naturally and through human interventio...
Slow interactions on small body surfaces occur both naturally and through human intervention. The re...
International audienceWith the flourishing number of small body missions that involve surface intera...
International audienceIn order to improve our understanding of landing on small bodies and of astero...
Oblique, low-velocity impacts onto extraterrestrial terrain are an inevitable occurrence during spac...
Context. Landing on the surface of small bodies is particularly challenging, as the physical propert...
International audienceContext. Landing on the surface of small bodies is particularly challenging, a...
This book focuses on the impact dynamics and cratering of soft matter to describe its importance, di...
Even if craters are very common on Solar System body surfaces, crater formation in granular media su...
The dusty regolith covering the surfaces of asteroids and planetary satellites differs in size, shap...
Context. In situ observations of small asteroids, such as Itokawa, Ryugu, and Bennu, show that surfa...
The penetration by a gravity-driven impact of a solid sphere into a granular medium is studied by tw...
Abstract The dusty regolith covering the surfaces of asteroids and planetary satellites differs in s...
Collisions between planetary ring particles and in some protoplanetary disk environments occur at lo...