From the major planets in our Solar System to the very Sun itself, the sphere is the most common shape of celestial bodies, but why is this?

Gravity is the main force that sculpts the Universe, causing the formation of planets, stars and galaxies.

It works over great distances and has no preferred orientation.

It draws matter in from all directions and when matter clumps together it forms a shape that looks the same from all directions. The shape that meets all these criteria is a sphere.

But the force of gravity also distorts the sphere that we would expect to see, meaning most of the bodies that we think of as being round are really 'almost spherical'.

Take our planet for instance. If I was to travel all around the world from pole to pole, I would have covered a distance of around 39,941km.

If I were to do the same journey, but this time around the equator, I would have travelled an additional 130km.

The Earth bulges at the equator to form a shape close to an oblate spheroid – a slightly squashed sphere.

## Why are planets slightly squashed?

The reason why planets get a bit fat around the middle is due to their rotation about their axes.

Imagine the chairoplane: that fairground ride with lots of chairs hanging down from a central disc.

As the disc starts to rotates, the chairs lift and move outward from the centre or outward from the centre of rotation.

The only thing stopping the chairs from flying off is the chains.

The same thing happens to a planet when it spins. Gravity acts like the chains, pulling everything inwards, but the speed of the rotation pushes everything outwards.

Just like the chairs on the ride moving outward, as a plane rotates on its axis it grows wider around the middle.

How fast a planet rotates seems to be one of the largest influences on the size of the bulge.

• Earth, with its 24-hour rotation, has a bulge of about 0.3%
• One rotation of Jupiter takes 10 hours and it has a bulge of 0.7 per cent
• Venus, which takes 243 Earth days to complete a single rotation, has no discernible bulge at all

But what of something much larger? Do stars bulge as well?

Recent data taken by the Solar Dynamics Observatory (SDO) has revealed that even though the Sun rotates at a rapid 7,000km/h at its equator, the observed measurements of its bulge have found it to be much smaller than expected – virtually negligible in fact.

Is this normal for stars? The SDO only recently made the measurements of the Sun.

Our star’s brightness and turbulent surface make defining its edge hard work.

Doing this for another star has proved to be more challenging still, but Altair in Aquila, which rotates at an even faster 17,000km/h, has been measured and found to have a bulge.

So why does our Sun not bulge as it spin? Well, this currently remains a mystery.

A few theories are being postulated but there is little evidence to back them as yet.

I think the fact that the Sun is lacking a bulge will be the source of much research in the future, and it shows that we can still have a number of surprises on our astronomical doorstep.