D. S. Lauretta   S. S. Balram-Knutson   E. Beshore   W. V. Boynton   C. Drouet d'Aubigny   D. N. DellaGiustina   H. L. Enos   D. R. Golish   C. W. Hergenrother   E. S. Howell   C. A. Bennett   E. T. Morton   M. C. Nolan   B. Rizk   H. L. Roper   A. E. Bartels   B. J. Bos   J. P. Dworkin   D. E. Highsmith   D. A. Lorenz   L. F. Lim   R. Mink   M. C. Moreau   J. A. Nuth   D. C. Reuter   A. A. Simon   E. B. Bierhaus   B. H. Bryan   R. Ballouz   O. S. Barnouin   R. P. Binzel   W. F. Bottke   V. E. Hamilton   K. J. Walsh   S. R. Chesley   P. R. Christensen   B. E. Clark   H. C. Connolly   M. K. Crombie   M. G. Daly   J. P. Emery   T. J. Mccoy   J. W. McMahon   D. J. Scheeres   S. Messenger   K. Nakamura-Messenger   K. Righter   S. A. Sandford   
SPACE SCIENCE REVIEWS 212(1-2) 925-984 2017年10月
In May of 2011, NASA selected the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) asteroid sample return mission as the third mission in the New Frontiers program. The other two New Frontiers ...
Yun Zhang   Derek C. Richardson   Olivier S. Barnouin   Clara Maurel   Patrick Michel   Stephen R. Schwartz   Ronald-Louis Ballouz   Lance A. M. Benner   Shantanu P. Naidu   Junfeng Li   
ICARUS 294 98-123 2017年9月
As the target of the proposed Asteroid Impact & Deflection Assessment (AIDA) mission, the near-Earth binary asteroid 65803 Didymos represents a special class of binary asteroids, those whose primaries are at risk of rotational disruption. To gain ...
Ronald-Louis Ballouz   Derek C. Richardson   Ryuji Morishima   
ASTRONOMICAL JOURNAL 153(4) 2017年4月
We study the B ring's complex optical depth structure. The source of this structure may be the complex dynamics of the Keplerian shear and the self-gravity of the ring particles. The outcome of these dynamic effects depends sensitively on the coll...
Viranga Perera   Alan P. Jackson   Erik Asphaug   Ronald-Louis Ballouz   
ICARUS 278 194-203 2016年11月
Many asteroids are likely rubble-piles that are a collection of smaller objects held together by gravity and possibly cohesion. These asteroids are seismically shaken by impacts, which leads to excitation of their constituent particles. As a resul...
R. -L. Ballouz   D. C. Richardson   P. Michel   S. R. Schwartz   Y. Yu   
PLANETARY AND SPACE SCIENCE 107 29-35 2015年3月
Our knowledge of the strengths of small bodies in the Solar System is limited by our poor understanding of their internal structures, and this, in turn, clouds our understanding of the formation and evolution of these bodies. Observations of the r...
Copyright Institute of Space and Astronautical Science