Finite element method approach for quantifying the conditions for shape deformation of the primary of binary asteroid Didymos after the DART impact
Masatoshi Hirabayashi1, Eugene Fahnestock2, Harrison F Agrusa3, Derek C Richardson3, Angela M Stickle4, Carolyn M Ernst5, Paul Sanchez6, Cristina Thomas7, Olivier S Barnouin5, Nancy L Chabot8, Andrew Rivkin9, Andrew F. Cheng4 and the NASA/DART Dynamics and Ejecta Working Groups, (1)Auburn University, Aerospace Engineering, Auburn, AL, United States, (2)JPL/Caltech, Pasadena, CA, United States, (3)University of Maryland College Park, College Park, MD, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)JHU Applied Physics Lab, Laurel, MD, United States, (6)University of Colorado at Boulder, Colorado Center for Astrodynamics Research, Boulder, CO, United States, (7)Northern Arizona University, Flagstaff, AZ, United States, (8)Applied Physics Lab, Laurel, MD, United States, (9)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States