Physical properties of asteroid Dimorphos as derived from the DART impact
Sabina D. Raducan, Martin Jutzi, A. F. Cheng, Yun Zhang, O. S. Barnouin, G. S. Collins, R. T. Daly, T. M. Davison, C. M. Ernst, T. L. Farnham, Fabio Ferrari, Masatoshi Hirabayashi, Kathryn M. Kumamoto, Patrick Michel, Naomi Murdoch, Ryota Nakano, M. Pajola, A. Rossi, Harrison Agrusa, Brent W. Barbee, Megan Bruck Syal, N. L. Chabot, E. Dotto, Eugene G. Fahnestock, P. H. Hasselmann, Isabel Herreros, Stavro Ivanovski, Jian‐Yang Li, Alice Lucchetti, R. Luther, Jens Ormö, Michael J. Owen, Petr Pravec, A. S. Rivkin, Colas Robin, Paul Sánchez, Filippo Tusberti, K. Wünnemann, Angelo Zinzi, E. Mazzotta Epifani, C. Manzoni, B. May
Abstract
Abstract On 26 September 2022, NASA’s Double Asteroid Redirection Test (DART) mission successfully impacted Dimorphos, the natural satellite of the binary near-Earth asteroid (65803) Didymos. Numerical simulations of the impact provide a means to find the surface material properties and structures of the target that are consistent with the observed momentum deflection efficiency, ejecta cone geometry and ejected mass. Our simulation that best matches the observations indicates that Dimorphos is weak, with a cohesive strength of less than a few pascals, like asteroids (162173) Ryugu and (101955) Bennu. We find that the bulk density of Dimorphos ρ B is lower than ~2,400 kg m − 3 and that it has a low volume fraction of boulders (≲40 vol%) on the surface and in the shallow subsurface, which are consistent with data measured by the DART experiment. These findings suggest that Dimorphos is a rubble pile that might have formed through rotational mass shedding and reaccumulation from Didymos. Our simulations indicate that the DART impact caused global deformation and resurfacing of Dimorphos. ESA’s upcoming Hera mission may find a reshaped asteroid rather than a well-defined crater.