Predicting Asteroid Material Properties from a DART-like Kinetic Impact
Kathryn M. Kumamoto(Lawrence Livermore National Laboratory), O. S. Barnouin(Johns Hopkins University Applied Physics Laboratory), Megan Bruck Syal(Lawrence Livermore National Laboratory), A. M. Stickle(Johns Hopkins University Applied Physics Laboratory), J. Michael Owen(Lawrence Livermore National Laboratory), Emma S. G. Rainey(Johns Hopkins University Applied Physics Laboratory), Cody Raskin(Lawrence Livermore National Laboratory), R. T. Daly(Lockheed Martin (United States)), Jason M. Pearl(Lawrence Livermore National Laboratory), Wendy K. Caldwell(Los Alamos National Laboratory)
Cited by 21
Related Papers
The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa
|Science|2006|966
Identification of hydrated silicate minerals on Mars using MRO‐CRISM: Geologic context near Nili Fossae and implications for aqueous alteration
|Journal of Geophysical Research Atmospheres|2009|681
OSIRIS-REx: Sample Return from Asteroid (101955) Bennu
|Space Science Reviews|2017|651
Hayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top–shaped rubble pile
|Science|2019|632
The unexpected surface of asteroid (101955) Bennu
|Nature|2019|521