Looking into the evolution of granular asteroids in the Solar System
By now it has been accepted that most of the small asteroids in the Solar System are granular aggregates kept together by gravitational and possibly, cohesive forces. These aggregates can form, deform and disrupt over millennia subjected to different internal and external factors that would ultimate...
Main Authors: | Sánchez Paul, Scheeres Daniel, Hirabayashi Masatoshi, Tardivel Simon |
---|---|
Format: | Article |
Language: | English |
Published: |
EDP Sciences
2017-01-01
|
Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201714014004 |
Similar Items
-
Seismic waves in the asteroid environment
by: Sánchez Paul, et al.
Published: (2021-01-01) -
The surface sensitivity of rubble-pile asteroids during a distant planetary encounter: Influence of asteroid shape elongation
by: Kim, Yaeji, et al.
Published: (2021) -
The surface sensitivity of rubble-pile asteroids during a distant planetary encounter: Influence of asteroid shape elongation
by: Kim, Yaeji, et al.
Published: (2021) -
The Secular Dynamical Evolution of Binary Asteroid System (65803) Didymos Post-DART
by: Rachel H. Cueva, et al.
Published: (2024-01-01) -
THE SOLAR-RADIATION PRESSURE EFFECTS ON THE ORBITAL EVOLUTION OF ASTEROID MOONS
by: V. V. Troianskyi, et al.
Published: (2016-06-01)