Basically, a binocular consists of two parallel, identical telescopes, one for each eye. Here you can calculate the exit pupil, focal length, magnification and limiting magnitude.
M = fob / fok
The two focal length must have the same units, commonly those are millimeters.
EP = D / M
At a binocular, often magnification and objective diameter are indicated, e.g. as 8x42. The larger the exit pupil, the more light-gathering it is and the easier it is to look through. 7 mm is the approximate maximum size of the human pupil, higher values don't give any more gain in light. Small objective diameter and large magnification create a small exit pupil, which can make it hard for beginners to see anything at all. Values below 1 mm are difficult.
Mmax = D * 2
At higher magnifications, the image becomes blurred and doesn't reveal further details.
m = 7.5 + 5 * log10 ( D/10 )
Mmin = D / 7
The limiting magnitude is an estimation of the brightness, up to which objects are visible with a certain objective diameter. Not considered here are important factors like seeing and equipment quality. There are different formulas for the estimation of the limiting magnitude, this calculator uses a rather simple one.
The minimum magnification results from the exit pupil, weaker magnifications are possible, but don't reach the limiting magnitude.
R = 5√ 100 b-a
The brightness of celestial bodies is measured in mag. Very bright starts have 0 mag or less, the faintest visible to the naked eye have 6 mag. The scale is logarithmic, 5 mag difference means 100 times more or less brighter.
↔ swaps the values of a and b.