RT Conference Proceedings
T1 Impact induced motion of boulders and their effect on ejecta emplacement on rubble-pile targets
A1 Ormö, Jens
A1 Raducan, Sabina D.
A1 Luther, Robert
A1 Jutzi, Martin
A1 Herreros Cid, María Isabel
A1 Collins, Gareth
A1 Wünnemann, Kai
A1 Mauri, Valentin
AB Asteroids smaller than about 50 km in diameter are the result of the break-up of a larger parent body. They are often considered to be rubble-pile objects, aggregates held together only by self-gravity or small cohesive forces, and have highly heterogeneous surfaces. Recently, the artificial impact experiment (SCI) of JAXA's Hayabusa2 mission on the surface of asteroid Ryugu created a relatively large crater (~14 m diameter) despite the presence of large boulders close to the impact location...
PB Europlanet Society
YR 2022
FD 2022
LK https://hdl.handle.net/10016/37249
UL https://hdl.handle.net/10016/37249
LA eng
NO Proceeding of: Europlanet Science Congress 2022 (EPSC 2022),  Palacio de Congresos de Granada, Spain, 18-23 September 2022
NO JO and MIH were supported by the Spanish State Research Agency (AEI) Project No. MDM-2017-0737 Unidad de Excelencia "María de Maeztu"-Centro de Astrobiología (CSIC-INTA). SDR, MJ, RL and KW have received fund from the European Union's Horizon 2020 research and innovation program under grant agreement No. 870377 (NEO-MAPP)
DS e-Archivo
RD 18 jul. 2024