# How fast can stars spin?

Everything in the universe is spinning. Spinning planets and their spinning moons orbit around spinning stars, which orbit spinning galaxies. It's spinning all the way down.

Consider that fiery ball in the sky, the . Like all , our sun rotates on its axis. You can't tell because staring at the sun long enough will permanently damage your eyeballs. Instead you can use a special purpose solar telescope to observe sunspots and other features on the surface of the sun. And if you track their movements, you'll see that the sun's equator takes 24.47 days to turn once on its axis. Unlike its slower poles which take 26.24 days to turn.

The sun isn't a solid ball of rock, it's a sphere of hot plasma, so the different regions can complete their rotation at different rates. But it rotates so slowly that it's an almost perfect sphere.

If you were standing on the surface of the sun, which you can't, of course, you would be whipping around at 7,000 km/h. That sounds fast, but just you wait.

How does that compare to other stars, and what's the fastest that a star can spin?

A much faster spinning star is Achenar, the tenth brightest star in the sky, located 139 light-years away in the constellation of Eridanus. It has about 7 times the mass of the sun, but it spins once on its axis every 2 days. If you could see Achenar up close, it would look like a flattened ball. If you measured it from pole to pole, it would be 7.6 suns across, but if you measured across the equator, it would be 11.6 suns across.

If you were standing on the surface of Achenar, you'd be hurtling through space at 900,000 km/h.

The very fastest spinning star we know of is the 25 solar mass VFTS 102, located about 160,000 light-years away in the Large Magellanic Cloud's Tarantula Nebula – a factory for massive stars.

If you were standing on the surface of VFTS 102, you'd be moving at 2 million km/h.

In fact, VFTS 102 is spinning so quickly, it can just barely keep itself together. Any faster, and the outward centripetal force would overcome the gravity holding its guts in, and it would tear itself apart. Perhaps that's why we don't see any spinning faster; because they couldn't handle the speed. It appears that this is the fastest that stars can spin.

One other interesting note about VFTS 102 is that it's also hurtling through space much faster than the stars around it. Astronomers think it was once in a binary system with a partner that detonated as a supernova, releasing it into space like a catapult.

Not only stars can spin. Dead stars can spin too, and they take this to a whole other level.

Neutron stars are what you get when a star with much more mass than the sun detonates as a supernova. Suddenly you've got a stellar remnant with twice the mass of the sun compressed down into a tiny ball about 20 km across. All that angular momentum of the star is retained, and so the neutron star spins at an enormous speed.

The fastest neutron star ever recorded spins around 700 times a second. We know it's turning this quickly because it's blasting out beams of radiation that sweep towards us like an insane lighthouse. This, of course, is a pulsar, and we did a whole episode on them.

A regular star would be torn apart, but have such intense gravity, they can rotate this quickly. Over time, the radiation streaming from the neutron star strips away its , and it slows down.

Black holes can spin even faster than that. In fact, when a black hole is actively feeding from a binary companion, or a is gobbling up stars, it can rotate at nearly the speed of light. The laws of physics prevent anything in the universe spinning faster than the speed of light, and go right up to the edge of the law without breaking it.

Astronomers recently found a supermassive black hole spinning up to 87% the maximum speed permitted by relativity.

If you were hoping there are antimatter lurking out there, hoarding all that precious future energy, I'm sorry to say, but astronomers have looked and they haven't found it. Just like the socks in your dryer, we may never discover where it all went.

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Source: Universe Today

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