Dynamics of rotationally fissioned asteroids: Source of observed small asteroid systems

[1]  T. Gold,et al.  On the Eccentricity of Satellite Orbits in the Solar System , 1963 .

[2]  Steven Soter,et al.  Q in the solar system , 1966 .

[3]  R. S. Hudson,et al.  Shape of Asteroid 4769 Castalia (1989 PB) from Inversion of Radar Images , 1994, Science.

[4]  S. Love,et al.  Catastrophic Impacts on Gravity Dominated Asteroids , 1996 .

[5]  Farquhar,et al.  Estimating the mass of asteroid 253 mathilde from tracking data during the NEAR flyby , 1997, Science.

[6]  A. Agresti,et al.  Approximate is Better than “Exact” for Interval Estimation of Binomial Proportions , 1998 .

[7]  Robert Jedicke,et al.  Collisional Models and Scaling Laws: A New Interpretation of the Shape of the Main-Belt Asteroid Size Distribution☆ , 1998 .

[8]  C. Murray,et al.  Solar System Dynamics: Expansion of the Disturbing Function , 1999 .

[9]  W. Benz,et al.  Catastrophic Disruptions Revisited , 1999 .

[10]  S. Ostro,et al.  Radar Observations of Asteroid 2063 Bacchus , 1999 .

[11]  D. Rubincam,et al.  Radiative Spin-up and Spin-down of Small Asteroids , 2000 .

[12]  P. Tanga,et al.  Collisions and Gravitational Reaccumulation: Forming Asteroid Families and Satellites , 2001, Science.

[13]  D. Campbell,et al.  Binary Asteroids in the Near-Earth Object Population , 2002, Science.

[14]  D. Campbell,et al.  1937 UB (Hermes) , 2003 .

[15]  Radar Images of Binary Asteroid 2003 YT1 , 2004 .

[16]  Derek C. Richardson,et al.  Numerical experiments with rubble piles: equilibrium shapes and spins , 2005 .

[17]  Akira Fujiwara,et al.  Pole and Global Shape of 25143 Itokawa , 2006, Science.

[18]  A. Cazenave,et al.  Four new binary minor planets: (854) Frostia, (1089) Tama, (1313) Berna, (4492) Debussy , 2006 .

[19]  M. Shepard,et al.  Radar and infrared observations of binary near-Earth Asteroid 2002 CE26 , 2006 .

[20]  Brian Warner,et al.  NEA rotations and binaries , 2006, Proceedings of the International Astronomical Union.

[21]  S. Ostro,et al.  Near-Earth Asteroid 2005 CR37: Radar Images and Photometry of a Candidate Contact Binary , 2006 .

[22]  Daniel J. Scheeres,et al.  Radar Imaging of Binary Near-Earth Asteroid (66391) 1999 KW4 , 2006, Science.

[23]  J. Kawaguchi,et al.  The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa , 2006, Science.

[24]  R. Roy,et al.  Photometric Survey of Binary Near-Earth Asteroids , 2006 .

[25]  R. S. Hudson,et al.  The Shape and Spin of 101955 (1999 RQ36) from Arecibo and Goldstone Radar Imaging , 2007 .

[26]  Re'em Sari,et al.  TIDAL EVOLUTION OF RUBBLE PILES , 2007, 0712.0446.

[27]  Daniel J. Scheeres,et al.  Rotational fission of contact binary asteroids , 2007 .

[28]  Petr Pravec,et al.  Binary asteroid population 1. Angular momentum content , 2007 .

[29]  M. Ćuk.  Formation and Destruction of Small Binary Asteroids , 2007 .

[30]  Derek C. Richardson,et al.  A steady-state model of NEA binaries formed by tidal disruption of gravitational aggregates , 2008 .

[31]  P. Michel,et al.  Rotational breakup as the origin of small binary asteroids , 2008, Nature.

[32]  David Vokrouhlický,et al.  PAIRS OF ASTEROIDS PROBABLY OF A COMMON ORIGIN , 2008 .

[33]  S. Ostro,et al.  The Shape, Mutual Orbit, and Tidal Evolution of Binary Near-Earth Asteroid 2004 DC , 2008 .

[34]  136617) 1994 CC , 2009 .

[35]  Sarah T. Stewart,et al.  VELOCITY-DEPENDENT CATASTROPHIC DISRUPTION CRITERIA FOR PLANETESIMALS , 2009 .

[36]  Daniel J. Scheeres,et al.  Stability of the planar full 2-body problem , 2009 .

[37]  Secular orbit variation due to solar radiation effects: a detailed model for BYORP , 2009 .

[38]  D. Scheeres.  Minimum energy asteroid reconfigurations and catastrophic disruptions , 2009 .

[39]  Rubble-Pile Reshaping Reproduces Overall Asteroid Shapes , 2009 .

[40]  F. Marzari,et al.  Computing the effects of YORP on the spin rate distribution of the NEO population , 2009 .

[41]  S. Ostro,et al.  Determining asteroid spin states using radar speckles , 2010 .

[42]  A. V. Sergeev,et al.  Formation of asteroid pairs by rotational fission , 2010, Nature.

[43]  K. Holsapple.  On YORP-induced spin deformations of asteroids , 2010 .

[44]  D. Scheeres,et al.  Scaling Forces to the Asteroid Surface: The Role of Cohesion , 2010 .

[45]  D. Scheeres,et al.  Detailed prediction for the BYORP effect on binary near-Earth Asteroid (66391) 1999 KW4 and implications for the binary population , 2010 .

[46]  D. Scheeres,et al.  Scaling forces to asteroid surfaces: The role of cohesion , 2010, 1002.2478.

[47]  Evolution of Small, Rapidly Rotating Asteroids , 2011 .