Regularization of the Hill four-body problem with oblate bodies
@article{Belbruno2022RegularizationOT, title={Regularization of the Hill four-body problem with oblate bodies}, author={Edward Belbruno and Marian Gidea and Wai-Ting Lam}, journal={Celestial Mechanics and Dynamical Astronomy}, year={2022}, volume={135} }
We consider the Hill four-body problem where three oblate, massive bodies form a relative equilibrium triangular configuration, and the 4th, infinitesimal body orbits in a neighborhood of the smallest of the three massive bodies. We regularize collisions between the infinitesimal body and the smallest massive body, via McGehee coordinate transformation. We describe the corresponding collision manifold and show that it undergoes a bifurcation when the oblateness coefficient of the smallest…
References
SHOWING 1-10 OF 27 REFERENCES
Hill Four-Body Problem with Oblate Bodies: An Application to the Sun–Jupiter–Hektor–Skamandrios System
- Physics, GeologyJournal of Nonlinear Science
- 2020
We consider a restricted four-body problem, with a precise hierarchy between the bodies: two larger bodies and a smaller one, all three of oblate shape, and a fourth, infinitesimal body, in the…
Families of periodic orbits in the planar Hill’s four-body problem
- Physics, Geology
- 2016
In this work we perform numerical explorations of some families of planar periodic orbits in the Hill approximation of the restricted four-body problem. This approximation is obtained by performing a…
On the restrited three-body problem when the mass parameter is small
- Mathematics
- 1982
We study some aspects of the restricted three-body problem when the mass parameter μ is sufficiently small. First, we describe the global flow of the two-body rotating problem, μ=0, and we use it for…
Hill’s approximation in a restricted four-body problem
- Physics, Mathematics
- 2015
We consider a restricted four-body problem on the dynamics of a massless particle under the gravitational force produced by three mass points forming an equilateral triangle configuration. We assume…
Surface gravity of rotating dumbbell shapes
- PhysicsAstrophysics and Space Science
- 2021
We investigate the problem of determining the shape of a rotating celestial object – e.g., a comet or an asteroid – under its own gravitational field. More specifically, we consider an object…
Ejection–Collision Orbits in Two Degrees of Freedom Problems in Celestial Mechanics
- Physics, MathematicsJournal of Nonlinear Science
- 2021
The existence of different types of ejection-collision orbits, that is, orbits that start and end at total collision, are proved based on the transversality of 2-dimensional invariant manifolds and on the behavior of the dynamics on the total collision manifold.
The Trojan Manifold in the System Earth–Moon
- Physics
- 1967
Abstract : The Trojan manifold is defined as the analytical manifold of periodic orbits which contains the triangular equilibrium L4 as a singularity. Identification of the Earth-Moon system is made…
Collective branch regularization of simultaneous binary collisions in the 3D N-body problem
- Physics
- 2009
In this work we study simultaneous binary collision (SBC) singularities of M⩽N∕2 binaries in the three dimensional classical gravitational N-body problem. We show the following: (1) In the…
Transversal ejection-collision orbits in Hill's problem forC≫1
- Mathematics
- 1988
In a recent paper [3], Lacomba and Llibre showed numerically the existence of two transversal ejection-collision orbits in Hill's problem for a valueC=5 of the Jacobian constant. This result can be…
Singularities in Classical Mechanical Systems
- Mathematics
- 1981
Singularities in the equations of motion of a classical mechanical system usually play a dominant role in the global phase portrait of the system, and power series or other analytic techniques often yield only a very local description of solutions near the singularity.