The Dynamics of NEO Binary Asteroids Journal Article uri icon



  • AbstractThe dynamics of binary Near-Earth objects (NEO) are discussed and a simple model for the study of their dynamics is introduced. Main results on the motion and stability of binary asteroids are reviewed. The effect of perturbations external to the binary system, including solar gravity, solar radiation pressure, and planetary gravity, are considered.

publication date

  • August 1, 2006

has restriction

  • bronze

Date in CU Experts

  • November 7, 2020 6:05 AM

Full Author List

  • Scheeres DJ

author count

  • 1

Other Profiles

International Standard Serial Number (ISSN)

  • 1743-9213

Electronic International Standard Serial Number (EISSN)

  • 1743-9221

Additional Document Info

start page

  • 177

end page

  • 190


  • 2


  • S236