Construct · 1 fields · 1 citations

circular restricted three-body problem: a standalone construct

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Astrodynamics

the problem of a massless body moving under the gravity of two massive primaries in circular orbits about their barycenter.

In astrodynamics, circular restricted three-body problem refers to the problem of a massless body moving under the gravity of two massive primaries in circular orbits about their barycenter. This meaning comes from Szebehely (1967) in Theory of Orbits in the Restricted Problem of Three Bodies.[1]

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Nearby constructs

body2 fields · 3 citationsjingle · one word, two constructs gravity4 fields · 6 citationsjingle · one word, four constructs Jacobi integral1 fields · 1 citationsanchor · a standalone construct

References

Szebehely, V. G. (1967). Theory of Orbits in the Restricted Problem of Three Bodies. Elsevier Science & Technology Books. ISBN 9780126806502

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