The Dynamics of NEO Binary Asteroids Journal Article

Overview

abstract

• 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.

CU Boulder Authors

• Scheeres, Daniel J.

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

published in

• Proceedings of the International Astronomical Union  Journal

Other Profiles

International Standard Serial Number (ISSN)

• 1743-9213

Electronic International Standard Serial Number (EISSN)

• 1743-9221

Digital Object Identifier (DOI)

• https://doi.org/10.1017/s1743921307003213

Additional Document Info

start page

• 177

end page

• 190

volume

• 2

issue

• S236