The stability of masses during three-body encounters

Details The stability of masses during three-body encounters The stability of masses during three-body encounters

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984cemec..32..145d&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 32, Feb. 1984, p. 145-162.

Astronomy and Astrophysics

Astronomy

20

Capture Effect, Celestial Mechanics, Dynamic Stability, Orbit Perturbation, Three Body Problem, Artificial Satellites, Astrodynamics, Binary Stars, Black Holes (Astronomy), Neutron Stars, Planets, Solar System, Stellar Mass Accretion

Scientific paper

The dynamical interaction of a binary system and a third body not moving on a closed orbit arises in a large number of physical situations. The C-squared H condition for determining Hill (1978) stability of coplanar bound three-body systems is extended to cover situations where the outer body moves on a parabolic or hyperbolic orbit. Regions where such a body is stable against exchange or collision with other components of the system are determined for a number of important cases where closed solutions are possible.

Affiliated with

Also associated with

No associations

Rating

The stability of masses during three-body encounters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The stability of masses during three-body encounters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The stability of masses during three-body encounters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1858039