A simulation of the three-body problem / n-body problem with 100 free masses in two-dimensional space. Each mass moves under the gravity of the others. The masses start with random positions and velocities. The masses can collide. Their collisions are almost, but not quite, perfectly elastic.
Newtonian Gravity
all masses equal
chaos / chaotic motion
velocities and positions calculated using Euler integration
50fps, 4K, 60s
#Physics #PhysicsSimulations #ThreeBodyProblem #Gravity #NewtonianGravity #Collisions