Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids

Details Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975cemec..12..189s&link_type=gif

Celestial Mechanics, vol. 12, Sept. 1975, p. 189-201.

Computer Science

Numerical Analysis

14

Lagrangian Equilibrium Points, Oblate Spheroids, Orbital Mechanics, Three Body Problem, Celestial Mechanics, Libration, Numerical Analysis, Planetary Orbits, Saturn (Planet)

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids 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 Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-910671