### Estimating the radius of the Moon - The medieval way

TL;DR I myself learnt the method from this page here.

Having estimated the radius of Earth, the next step, celestially speaking, would be to estimate the radius of the Moon, our satellite and closest neighbor. And before we proceed any further, let me just point out the fact that the distances or sizes in astronomy are measured in angles and not in meters. From Earth, it looks to us as though the astronomical objects are moving on a celestial sphere and therefore, their motion can be quantified in terms of angular motion and sizes in angles. How to measure these angles you say? Well using a telescope of course! A telescope can be calibrated such that one can move it along or perpendicular to the horizon with milli-degree accuracy, helping us therefore to estimate the angular size of objects in the sky.

Now that we've cleared that, let's look at quantities in the Earth-Moon-Sun system that can actually be measured. We already know the radius of Earth. We can estimate the angular diameter of the Moon, and therefore of the Sun, using telescopes. It is measured to be 31 arcminutes or approximately half a degree. Why is the angular size of the Moon equal to the angular size of the Sun you ask? Hint : Eclipses!

Coming to point, using the small angle approximation, we can say that the ratio of angular size of the Moon and the angular size of the Earth's shadow at a distance equal to the distance between the Earth and the Moon is equal to the ratio of the actual diameter of the moon to the actual diameter of the Earth's shadow at that distance!