Computer Science
Scientific paper
Sep 1973
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973cemec...8..291f&link_type=abstract
Celestial Mechanics, Volume 8, Issue 2, pp.291-296
Computer Science
1
Scientific paper
Three-dimensional computer plots were drawn for various zero-velocity contours of the restricted three-body problem (μ=0.1, 0.3, 0.5) and the restricted four-body problem (μ1=μ2=μ3==0.33). The infinitesimal mass was constrained to the plane of the finite masses. The three-dimensional representations yield a clear insight into the regions of motion and the stability of motion near the equilibrium points.
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