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The center of a Black Hole is called the
Singularity, where all of it’s mass is concentrated into a tiny volume. This mass is the source of the enormous amount of gravitational force directed into the Black Hole, as well as the source of the event horizon. The event horizon is the border at which nothing inside can escape the force due to gravity from the singularity. If a non-rotating Black Hole pulls something inside of its event horizon that object will inevitably be crushed by the tidal forces and will always hit the singularity. Not only is it guaranteed to hit the singularity, but because of the strange reversal of time and space inside a Black Hole, it can be calculated exactly how long it will take before it hits the singularity. This is a result of the mass of the Black Hole and nothing else. If you know the mass of a Black Hole you can find exactly how long you will have before you hit the singularity after crossing the event horizon. |
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These are two identical programs for calculating
the time to the singularity. The one uses a graphics library only supported at Syracuse University computer clusters, and the other is a boring dos version which can be run anywhere. |
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