Orbital evolution of the Gefion and Adeona asteroid families: close encounters with massive asteroids and the Yarkovsky effect

[1]  A. Celletti,et al.  Modern Celestial Mechanics: From Theory to Applications , 2002 .

[2]  Richard P. Binzel,et al.  Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: A Feature-Based Taxonomy , 2002 .

[3]  Alessandro Morbidelli,et al.  The Flora Family: A Case of the Dynamically Dispersed Collisional Swarm? , 2002 .

[4]  J. Burns,et al.  Dynamical Evolution of the Adeona and Gefion Asteroid Families , 2002 .

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

[6]  D. Vokrouhlický,et al.  Dynamical Spreading of Asteroid Families by the Yarkovsky Effect , 2001, Science.

[7]  J. Burns,et al.  Gravitational Scattering of Asteroid Families by Massive Asteroids , 2001 .

[8]  Richard J. Greenberg,et al.  Numerical Evaluation of the General Yarkovsky Effect: Effects on Semimajor Axis , 2001 .

[9]  J. Burns,et al.  Asteroid Mobility due to Encounters with Ceres, Vesta, Pallas: Monte Carlo codes versus Direct Numerical Integrations , 2000 .

[10]  Harold F. Levison,et al.  Symplectically Integrating Close Encounters with the Sun , 2000 .

[11]  Grzegorz Michalak,et al.  Determination of Asteroid Masses , 2000 .

[12]  A. Milani,et al.  Synthetic Proper Elements for Outer Main Belt Asteroids , 2000 .

[13]  Harold F. Levison,et al.  Dynamical Lifetimes and Final Fates of Small Bodies: Orbit Integrations vs Öpik Calculations , 1999 .

[14]  A. Erikson,et al.  ISOPHOT Polarization Measurements of the Asteroids (6) Hebe and (9) Metis at 25 μm , 1999 .

[15]  Paolo Tanga,et al.  The Velocity–Size Relationship for Members of Asteroid Families and Implications for the Physics of Catastrophic Collisions , 1999 .

[16]  W. Benz,et al.  Catastrophic Disruptions Revisited , 1999, astro-ph/9907117.

[17]  A. Morbidelli,et al.  Numerous Weak Resonances Drive Asteroids toward Terrestrial Planets Orbits , 1999 .

[18]  J. Chambers.  A hybrid symplectic integrator that permits close encounters between massive bodies , 1999 .

[19]  D. Vokrouhlický.  A COMPLETE LINEAR MODEL FOR THE YARKOVSKY THERMAL FORCE ON SPHERICAL ASTEROID FRAGMENTS , 1999 .

[20]  Vokrouhlick,et al.  Semimajor axis mobility of asteroidal fragments , 1999, Science.

[21]  Schelte J. Bus,et al.  Compositional structure in the asteroid belt: Results of a spectroscopic survey , 1999 .

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

[23]  A. Morbidelli,et al.  Three-Body Mean Motion Resonances and the Chaotic Structure of the Asteroid Belt , 1998 .

[24]  Harold F. Levison,et al.  A Multiple Time Step Symplectic Algorithm for Integrating Close Encounters , 1998 .

[25]  D. Vokrouhlický,et al.  The Yarkovsky Seasonal Effect on Asteroidal Fragments: A Nonlinearized Theory for the Plane-parallel Case , 1998 .

[26]  Morbidelli,et al.  Origin of multikilometer earth- and mars-crossing asteroids: A quantitative simulation , 1998, Science.

[27]  A. Morbidelli,et al.  An Analytic Model of Three-Body Mean Motion Resonances , 1998 .

[28]  S. Mikkola.  Non-canonical perturbations in symplectic integration , 1998 .

[29]  P. N. Smith,et al.  The Properties of Fragments from Catastrophic Disruption Events , 1998 .

[30]  W. Hartmann,et al.  Meteorite Delivery via Yarkovsky Orbital Drift , 1998 .

[31]  M. Holman,et al.  On the Origin of Chaos in the Asteroid Belt , 1998 .

[32]  M. Holman,et al.  Diffusive chaos in the outer asteroid belt. , 1997 .

[33]  Harold F. Levison,et al.  Dynamical Lifetimes of Objects Injected into Asteroid Belt Resonances , 1997 .

[34]  R. Sullivan,et al.  The Shape of Ida , 1996 .

[35]  Alessandro Morbidelli,et al.  Asteroid Families Close to Mean Motion Resonances: Dynamical Effects and Physical Implications , 1995 .

[36]  Alberto Cellino,et al.  Asteroid Families: Search of a 12,487-Asteroid Sample Using Two Different Clustering Techniques , 1995 .

[37]  D. Rubincam,et al.  Asteroid orbit evolution due to thermal drag , 1995 .

[38]  Francesco Marzari,et al.  Collisional Evolution of Asteroid Families , 1995 .

[39]  Akiko M. Nakamura,et al.  Catastrophic disruption experiments: recent results , 1994 .

[40]  The origin of chaos , 1994 .

[41]  Alberto Cellino,et al.  Asteroid Famalies. II. Extension to Unnumbered Multiopposition Asteroids , 1994 .

[42]  M. Nolan,et al.  Velocity Distributions among Colliding Asteroids , 1994 .

[43]  Andrea Milani,et al.  Asteroid Proper Elements and the Dynamical Structure of the Asteroid Main Belt , 1994 .

[44]  Robert D. Skeel,et al.  Dangers of multiple time step methods , 1993 .

[45]  P. Farinella,et al.  Modelling the outcomes of high-velocity impacts between small solar system bodies , 1993 .

[46]  H. Melosh,et al.  Swapping Rocks: Ejection and Exchange of Surface Material Among the Terrestrial Planets , 1993 .

[47]  W. Bottke,et al.  Asteroidal collision probabilities , 1993 .

[48]  Anne Lemaitre,et al.  Proper Elements: What are They ? , 1993 .

[49]  P. Farinella,et al.  The Injection of Asteroid Fragments into Resonances , 1993 .

[50]  P. Farinella,et al.  Collision rates and impact velocities in the Main Asteroid Belt , 1992 .

[51]  J. Wisdom,et al.  Symplectic maps for the N-body problem. , 1991 .

[52]  Alan W. Harris,et al.  Application of photometric models to asteroids. , 1989 .

[53]  Richard P. Binzel,et al.  Asteroid rotation rates - Distributions and statistics , 1989 .

[54]  S. Roser,et al.  The mass of the asteroid (10) Hygiea derived from observations of (829) Academia , 1987 .

[55]  P. Farinella,et al.  Collisional evolution of asteroids , 1983 .

[56]  Richard Greenberg.  Orbital interactions - A new geometrical formalism , 1982 .

[57]  J. Burns,et al.  Radiation forces on small particles in the solar system , 1979 .

[58]  T. Teichmann,et al.  Fundamentals of celestial mechanics , 1963 .