Capture in the Circular and Elliptic Restricted Three-Body Problem

Details Capture in the Circular and Elliptic Restricted Three-Body Problem Capture in the Circular and Elliptic Restricted Three-Body Problem

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cemda..90...51m&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, v. 90, Issue 1, p. 51-58 (2004).

Astronomy and Astrophysics

Astronomy

6

Asteroid, Capture, Elliptic Restricted Three-Body Problem, Hill-Region

Scientific paper

In this paper the authors provide a study of the phenomenon of the gravitational capture by using the models of the circular and elliptic restricted three-body problem. In the first part the inadequacy of the circular restricted three-body problem in the study of the phenomenon of the capture in the case of NEAs is shown. In the model of the spatial elliptic restricted three-body problem criteria of the capture are deduced by using the pulsating Hill-regions.

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