The zero velocity surfaces in the photogravitational restricted three- body problem

DOI10.1007/BF00113988zbMath0666.70006MaRDI QIDQ1116719

Omiros Ragos, C. G. Zagouras

Publication date: 1988

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

zbMATH Keywords

equilibrium pointsrestricted three-body problemmass parameterluminous``out of planemore massive bodyradiation pressure parametersurfaces of zero velocity

Mathematics Subject Classification ID

Three-body problems (70F07) Computational methods for problems pertaining to mechanics of particles and systems (70-08)

Related Items (5)

On the existence of the ``out of plane equilibrium points in the photogravitational restricted three-body problem ⋮ Modified characteristics projection finite element method for time-dependent conduction-convection problems ⋮ Periodic solutions around the collinear Lagrangian points in the photogravitational restricted three-body problem: Sun-Jupiter case ⋮ Periodic solutions around the out-of-plane equilibrium points in the restricted three-body problem with radiation and angular velocity variation ⋮ BIFURCATIONS IN THE TOPOLOGY OF ZERO-VELOCITY SURFACES IN THE PHOTO-GRAVITATIONAL COPENHAGEN PROBLEM

Cites Work

• Unnamed Item
• On the collinear libration points in the photo-gravitational three-body problem
• Stability of L4 and L5 against radiation pressure
• On the stability of triangular libration points of the photogravitational restricted circular three-body problem
• The restricted 3-body problem with radiation pressure
• BURRAU'S PROBLEM OF THREE BODIES

This page was built for publication: The zero velocity surfaces in the photogravitational restricted three- body problem