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In this paper, we consider the elliptic relative equilibria of the restricted $N$-body problems, where the $N-1$ primaries form an Euler-Moulton collinear central configuration or a $(1+n)$-gon central configuration. We obtain the…

Dynamical Systems · Mathematics 2024-09-24 Jiashengliang Xie , Bowen Liu , Qinglong Zhou

This paper demonstrates the existence of twistless tori and the associated reconnection bifurcations and meandering curves in the planar circular restricted three-body problem. Near the Lagrangian equilibrium $\mathcal{L}_4$ a twistless…

Mathematical Physics · Physics 2015-06-17 Holger R Dullin , Joachim Worthington

We give a self-contained modern linear stability analysis of a system of n equal mass bodies in circular orbit about a single more massive body. Starting with the mathematical description of the dynamics of the system, we form the linear…

Astrophysics · Physics 2009-11-11 Robert J. Vanderbei , Egemen Kolemen

In this paper we characterize all the solutions of the three body problem on which one body with mass $m_1$ remains in a fixed line and the other two bodies have the same mass $m_2$. We show that all the solutions with negative total energy…

Dynamical Systems · Mathematics 2014-10-08 Oscar Perdomo

The continuation of resonant periodic orbits from the restricted to the general three body problem is studied in a systematic way. Starting from the Keplerian unperturbed system we obtain the resonant families of the circular restricted…

Earth and Planetary Astrophysics · Physics 2010-03-19 G. Voyatzis , T. Kotoulas , J. D. Hadjidemetriou

We present 1349 families of Newtonian periodic planar three-body orbits with unequal mass and zero angular momentum and the initial conditions in case of isosceles collinear configurations. These 1349 families of the periodic collisionless…

Chaotic Dynamics · Physics 2019-08-13 Xiaoming Li , Yipeng Jing , Shijun Liao

We consider the Hill four-body problem where three oblate, massive bodies form a relative equilibrium triangular configuration, and the fourth, infinitesimal body orbits in a neighborhood of the smallest of the three massive bodies. We…

Dynamical Systems · Mathematics 2023-02-22 Edward Belbruno , Marian Gidea , Wai-Ting Lam

The configuration manifold $M$ of a mechanical system consisting of two unconstrained rigid bodies in $\mathbb{R}^n$, $n\geq 1$, is a manifold with boundary (typically with singularities.) A complete description of the system requires…

Dynamical Systems · Mathematics 2015-01-28 Christopher Cox , Renato Feres , Will Ward

Motivated by Xia-Zhou's recent work on applying symmetry groups to the N-body problem, we will study relative equilibria of the equilateral triangle and the square configurations under $\alpha$-homogeneous and quasi-homogeneous potentials…

Classical Analysis and ODEs · Mathematics 2022-07-18 Yingli Li

We consider the special case of the restricted circular three-body problem, when the two primaries are of equal mass, while the third body of negligible mass performs oscillations along a straight line perpendicular to the plane of the…

Earth and Planetary Astrophysics · Physics 2011-02-17 Vladislav Sidorenko

Given $n$ point masses turning in a plane at a constant speed, this paper deals with the global bifurcation of periodic solutions for the masses, in that plane and in space. As a special case, one has a complete study of n identical masses…

Dynamical Systems · Mathematics 2016-01-12 C. García-Azpeitia , J. Ize

In this work we are interested in the central configurations of the spatial seven-body problem where six of them are at vertices of two congruents equilateral triangles belong to parallel planes and one triangle is a rotation by the angle…

Metric Geometry · Mathematics 2015-06-16 Allyson Oliveira

In the $2$-dimensional $n$-body problem, $n\ge 3$, in spaces of constant curvature, $\kappa\ne 0$, we study polygonal homographic solutions. We first provide necessary and sufficient conditions for the existence of these orbits and then…

Dynamical Systems · Mathematics 2012-02-21 Florin Diacu

We study the linear stability of regular $n$-gon rotating equilibria in the $n$-body problem with logarithm interaction. In the presence of a central mass $M$, linear stability is insured if $M$ is bounded below and above by constants…

Dynamical Systems · Mathematics 2024-04-30 Anna-Monika Muscas , Daniel Pasca , Cristina Stoica

For a wide class of two-body interactions, including standard examples like gravitational or Coulomb fields, we show that collision orbits in $n$-body systems are of Liouville measure zero for all energies. We use techniques from symplectic…

Mathematical Physics · Physics 2019-09-04 Stefan Fleischer , Andreas Knauf

In this article, equilibrium points and families of periodic orbits in the vicinity of the collinear equilibrium points of a binary asteroid system are investigated with respect to the angular velocity of the secondary body, the mass ratio…

Earth and Planetary Astrophysics · Physics 2023-07-26 L. B. T. Santos , Allan Kardec de Almeida , P. A. Sousa-Silva , M. O. Terra , D. M. Sanchez , S. Aljbaae , A. F. B. A. Prado , F Monteiro

We study the orbits and manifolds near the equilibrium points of a rotating asteroid. The linearised equations of motion relative to the equilibrium points in the gravitational field of a rotating asteroid, the characteristic equation and…

Earth and Planetary Astrophysics · Physics 2014-03-11 Yu Jiang , Hexi Baoyin , Junfeng Li , Hengnian Li

We prove for a large class of n-body problems including a subclass of quasihomogeneous n-body problems, the classical n-body problem, the n-body problem in spaces of negative constant Gaussian curvature and a restricted case of the n-body…

Mathematical Physics · Physics 2018-06-28 Pieter Tibboel

In this paper, we propose two families of nonconforming finite elements on $n$-rectangle meshes of any dimension to solve the sixth-order elliptic equations. The unisolvent property and the approximation ability of the new finite element…

Numerical Analysis · Mathematics 2023-03-13 Xianlin Jin , Shuonan Wu

We consider the 3-dimensional gravitational $n$-body problem, $n\ge 2$, in spaces of constant Gaussian curvature $\kappa\ne 0$, i.e.\ on spheres ${\mathbb S}_\kappa^3$, for $\kappa>0$, and on hyperbolic manifolds ${\mathbb H}_\kappa^3$, for…

Dynamical Systems · Mathematics 2013-10-02 Florin Diacu