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The effect of orbital eccentricities on the shape of the hill-type analytical stability surfaces in the general three-body problem - MaRDI portal

The effect of orbital eccentricities on the shape of the hill-type analytical stability surfaces in the general three-body problem (Q3330578)

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The effect of orbital eccentricities on the shape of the hill-type analytical stability surfaces in the general three-body problem
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    The effect of orbital eccentricities on the shape of the hill-type analytical stability surfaces in the general three-body problem (English)
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    1984
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    Hill-type stability surfaces
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    general hierarchical three-body problem
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    non-zero eccentricities
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    initial osculating orbits
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    initial zero eccentricities
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    triple subgroups of solar system
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    solar perturbations
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