Collisional history of Ryugu's parent body from bright surface boulders
The asteroid (162173) Ryugu and other rubble-pile asteroids are likely re-accumulated fragments of much larger parent bodies that were disrupted by impacts. However, the collisional and orbital pathways from the original parent bodies to subkilometre rubble-pile asteroids are not yet well understood 1-3. Here we use Hayabusa2 observations to show
Tatsumi, E. et al.
Fecha de publicación:
0
2021