russ_watters said:
How can it have enough mass to be a black hole in a small enough volume to have an event horizon and not have a high density? Is this a peculiarity of supermassive black holes?
Yes.
The following calculation is only suggestive, and it is in no way rigorous. Because of the curvature and nature of spacetime, it probably doesn't make sense to calculate the spatial volume inside the event horizon of a black hole.
Using units for which [itex]c = G = 1[/itex], the event horizon of a mass [itex]M[/itex] spherical black hole occurs at [itex]R = 2M[/itex]. Using this in the standard flat space expression for density, and treating the black hole as a sphere of radius [itex]2M[/itex], gives
[tex]
\rho = \frac{M}{V} = \frac{M}{\frac{4}{3} \pi R^3} = \frac{3}{32 \pi M^2}.[/tex]
Notice how the "density" of a black hole rapidly decreases as its mass increases.
Even, though this isn't really the density of a black hole, this "back of the envelope" calculation is good enough to make predictions.
Setting [itex]\rho[/itex] to the average density of the sun, about 1400 kg/m^3, gives a black hole mass of about 100 million solar masses. So, if more than 100 million solar-mass stars or so (within an order of magnitude) congregate in the centre of a galaxy, they don't have to touch (initially) to form a black hole.