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.
The angle between the north star and your northern horizon is approximately the same as your latitude north of the equator.
By "within" a black hole, I would imagine you mean within the event horizon. Such an object won't ORBIT the black hole - it will simply fall towards the singularity.
Seattle's latitude is about 47.6 degrees North. So the altitude of Polaris above the northern horizon is always within about 1/3 degree of that angle as seen from there.
The amount of mitochondria within a cell.
No. Nothing, not even light can escape from within the event horizon. Since light can't get out, we can't see anything inside, which is why black holes are black.
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.
No planet has an event horizon. A black hole has an event horizon; it is the radius within which light cannot escape.
"average density" You must combine the weight of the metal hull with that of the air contained within it.
The angle between the north star and your northern horizon is approximately the same as your latitude north of the equator.
That is the "point of no return". Within the event horizon, gravity is so strong that anything that crosses the event horizon can't get out, even if it moves at the speed of light.
soil horizon
Capillary density within tissues varies directly with tissues' rates and metabolism.
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.
The standard unit of measurement is T score which compares your bone density with that of a healthy young woman. A T-score is within the normal range if it is -1.0 or above. A negative number means you have thinner bones than average. It can later on be converted into percentages.
The density increases
Density is a measure of how tightly the matter within it is packed together.
The inner core was discovered in 1936 by Inge Lehmann and is generally believed to be composed primarily of iron and some nickel. Its estimated density is between 12.6 to 13.0 grams to cubic centimeters.