Walsh, K. J.; Jawin, Erica R.; Ballouz, R. L.; Barnouin, O. S.; Bierhaus, E. B.; Connolly, H. C., Jr.; Molaro, J. L.; McCoy, Timothy J.; Delbo', M.; Hartzell, C. M.; Pajola, M.; Schwartz, S. R.; Trang, D.; Asphaug, E.; Becker, K. J.; Beddingfield, C. B.; Bennett, C. A.; Bottke, W. F.; Burke, K. N.; Clark, B. C.; Daly, M. G.; DellaGiustina, D. N.; Dworkin, J. P.; Elder, C. M.; Golish, D. R.; Hildebrand, A. R.; Malhotra, R.; Marshall, J.; Michel, P.; Nolan, M. C.; Perry, M. E.; Rizk, B.; Ryan, A.; Sandford, S. A.; Scheeres, D. J.; Susorney, H. C. M.; Thuillet, F.; Lauretta, D. S.; The OSIRIS-REx Team
(2019)
Small, kilometre-sized near-Earth asteroids are expected to have young and frequently refreshed surfaces for two reasons: collisional disruptions are frequent in the main asteroid belt where they originate, and thermal or ...