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Simply divide the mass of the black hole by the volume contained within the event horizon. This is fairly simple for a typical black hole, since the event horizon will approximate a sphere whose radius is the collapsed object's Schwarzschild radius.

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Q: How to determine Average density within an event horizon?
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When a star collapses its mass is squeezed into a single point that has zero volume What is its density?

Its density becomes infinite. Except that what you have described is a black hole and the ordinary laws of physics and maths do not apply in or within the event horizon of a black hole.


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To find the density of ANYTHING, divide the mass by the volume. The singularity in the black hole is believed to be very small, perhaps of zero volume; that would give an infinite density (physicists are not very happy with this idea, and our ideas of black holes may still change). However, the volume used for the "density" is often the entire volume within the event horizon, which has a finite (i.e., non-zero) size.


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