Simulation of the SCI impact. a) – c) Snapshots of the simulation at different times. At t = 1200s, the development of the crater is over. d) SCI crater on the asteroid Ryugu. The key characteristics of the observed crater, including the displacement of the boulders, are recreated in the simulation. (IMAGE)

University of Bern

Simulation of the SCI impact. a) – c) Snapshots of the simulation at different times. At t = 1200s, the development of the crater is over. d) SCI crater on the asteroid Ryugu. The key characteristics of the observed crater, including the displacement of the boulders, are recreated in the simulation.

Caption

Simulation of the SCI impact. a) – c) Snapshots of the simulation at different times. At t = 1200s, the development of the crater is over. d) SCI crater on the asteroid Ryugu. The key characteristics of the observed crater, including the displacement of the boulders, are recreated in the simulation.

Credit

© Courtesy of Martin Jutzi

Usage Restrictions

Credit must be given to the creator.

License

CC BY

Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.