WOLFRAM NOTEBOOK

WOLFRAM|DEMONSTRATIONS PROJECT

Orbits around Schwarzschild Black Holes

angular momentum
initial radius
proper time
view
symmetric orbit
The gravitational pull of a black hole is so strong that it will warp a two-body orbit away from anything elliptical. In this Demonstration, modifying the angular momentum, initial radius, time, or view shows the effects of extreme gravitation.
Wolfram Cloud

You are using a browser not supported by the Wolfram Cloud

Supported browsers include recent versions of Chrome, Edge, Firefox and Safari.


I understand and wish to continue anyway »

You are using a browser not supported by the Wolfram Cloud. Supported browsers include recent versions of Chrome, Edge, Firefox and Safari.