The motion of an asteroid in a two-dimensional space with a star and a planet • University project • 2014 - Laboratorio di Fisica Computazionale - BSc in Physics, II year

Indirect optimization for energy-optimal Lyapunov-to-Lyapunov transfer using heteroclinic connection as initial guess.

A python code to calculate planetary orbits in a three-body gravitational system. The code can demonstrate how one planet affects the orbit of another planet. As an example, Earth, Jupiter, Sun system is analyzed.

Simulation of the Three-body problem using JavaScript

Euler-cromer method for solving the 3-body problem arising in planetary motion

Solving some interesting problems using Python and C++

Numerical solution of Circular restricted three-body problem in which the mass of one of the bodies is negligible, as well as the interaction forces between it and the other two bodies.

三体运动模拟和可视化(three-body motion simulation and visualization)

Here, we can find different simulations of chaotic scenarios in physics. The codes were written as part of the University dissertation and intend to visualise and provide meaningful explanation to the system's characteristics.

Numerical solution to the Three-Body Problem using the Runge-Kutta 4th order method and a corresponding interactive simulation in the GlowScript IDE using Python / VPython.

Cambridge Undergraduate Physics - Part II Long Computing Project

Three-body Problem: Orbital Motions of Sun-Jupiter-Earth System

Project to understand how close passages between galaxies affect the orbits of stars in the galaxies, and see the effects in dramatic tidal features observed in some merging galaxies. The project is done in a team of 2.

Simulating the orbits of a three planetary system composed of the Sun, Jupiter and Saturn.

Three-Body countdown in your browser new tab.

The three body problem implemented in Python

Three-Body english subtitles extracted from Viki

Three Body Problem for Models and Numerical Methods Exam of the University of Bologna

It's a course project to find stable solution of three-body problem with machine learning