Effect of oblateness on triangular solutions at critical mass

DOI10.1007/BF00644329zbMath0392.70010MaRDI QIDQ1251909

P. V. Subba Rao, Ram Krishan Sharma

Publication date: 1979

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

Celestial MechanicsPeriodic OrbitsCritical MassOblatenessPlanar Three-Body ProblemTriangular Solutions

Mathematics Subject Classification ID

Three-body problems (70F07)

Related Items (4)

On the spatial collinear restricted four-body problem with non-spherical primaries ⋮ The linear stability of libration points of the photogravitational restricted three-body problem when the smaller primary is an oblate spheroid ⋮ On the restricted three body problem with oblate primaries ⋮ Bifurcations of relative equilibria for one spheroidal and two spherical bodies

Cites Work

• Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid
• BURRAU'S PROBLEM OF THREE BODIES

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