Wolfram Demonstrations Project
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Orbits around Schwarzschild Black Holes

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.

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Thanks to Professor Harold Zapolsky of Rutgers University at whose office blackboard I first sketched black hole orbits.

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"Orbits around Schwarzschild Black Holes" from the Wolfram Demonstrations Project
 http://demonstrations.wolfram.com/OrbitsAroundSchwarzschildBlackHoles/
Contributed by: David Saroff
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