Of course you know the answer to this: the Sun. (Though often when I ask people they tend to look sheepish and say nothing, for fear of being wrong!)

Actually, it’s not at all obvious which one is bigger: after all, they look the same size. You know which one is bigger because you were told it when you were very young. Which rather spoils the pleasure of trying to work it out. But *how* do we know the Sun is bigger?

It’s fairly easy to establish that the Sun is a least a bit bigger than the Moon. They look the same size in the sky, but during a solar eclipse the Moon completely covers the face of the Sun. So the Sun must be further away than the Moon and therefore it must be bigger. But *how* much bigger?

To establish this we need another rare sighting in the sky: have you ever seen the Moon and the Sun in the sky at the same time? It does happen — as the picture above shows. (Indeed, Lewis Carroll wrote about it in the first two verses of ** The Walrus and the Carpenter**.)

But imagine that you can see both the Sun and the Moon in the sky together and that the Moon is a *half *Moon. What must the geometry of the solar system be at that moment?

The Sun-Moon-Earth forms a giant right-angled triangle, with the Moon at the right-angle. If we can measure the Sun-Earth-Moon angle, then we can use trigonometry to find the relative distances of the Sun and the Moon from Earth. Since the Sun and the Moon look the same size in the sky, these relative distances must also be the relative sizes of the Sun and Moon themselves.

The hard part is measuring the angle. You need it to be *exactly* a half Moon. You need to measure the angle between the Sun (**without** looking at it directly), you and the Moon.

But it gets worse, if you’re even *slightly* wrong with your measurement, the relative distances and sizes change by a surprisingly large amount. This is because the angle is very nearly 90° — and that is because the Sun is really *very* much farther away than the Moon and *very* much bigger. In fact the angle is about 89 5/6°, which indicates that the Sun is about 340 times the size of the Moon. But if you measure it as 89 4/6°, you’ll get the Sun being only 170 times the size of the Moon, in other words *half* the size (and therefore one-eighth of the volume, and one-eighth of the mass). So your measurement needs to be incredibly precise!

**Notes**

The diagram above is merely intended to indicate the relative positions of the Sun, Moon and Earth. The sizes are not to the same scale (compared with the Earth, the Sun should be vastly bigger than shown and the Moon slightly smaller) and the distances are not in proportion (the Earth-Sun distance is substantially bigger than the Earth-Moon distance – indeed, the triangle should look almost like two parallel lines).

The Sun is, in fact, almost exactly 400 times the size of the Moon, by which I mean its radius is about 400 times the radius of the Moon. This means that its volume is 400×400×400 times the volume of the Moon, which makes it 64 million times as large. (The ratio of the masses of the Sun and the Moon is different, however, because they do not have the same average density.)

The figures of 340 and 170 come from tan(89 5/6°) and tan(89 4/6°), which actually represent the Moon:Sun and Moon:Earth distance ratios. It’s an incredible coincidence that, although the angle differs by one-sixth of a degree, one tangent is (almost exactly) double the size of the other. (In fact, it’s double to one part in a hundred thousand!)