2,800,000 kilomeetrit!
Altair is a hot star in the constellation Aquila, about 17 light-years from Earth. A light-year is the distance light travels in one year. It spins so fast that it bulges at its equator. It is about 2.8 million kilometers (1.7 million miles) across at its equator, twice the width of the Sun, but only about 2.3 million kilometers from pole to pole.
A star has no solid surface, so its size is the width of the glowing layer that its light comes from. In 2007, astronomers measured Altair with the CHARA Array, which combines the light of several telescopes to see detail too fine for any one of them. They used it to make an image of the star's surface, and fitted a model of a spinning star to their measurements.
The model gave a radius at the equator of 2.03 times the Sun's and a radius at the poles of 1.63 times. So the star is about a quarter wider at its equator than from pole to pole. A 2020 study, using a more detailed model of the star's interior, found an equatorial radius of 2.01 times the Sun's, within about 1% of the earlier result.
Altair turns once every 7 hours and 46 minutes, and its equator moves at about 314 kilometers per second. The Sun, by comparison, takes about 25 days to turn once. Spinning this fast pushes Altair's equator outward, which is why the star is flattened.
The bulging equator is also cooler than the poles, an effect called gravity darkening. The 2007 study measured about 8,200 degrees Celsius at the poles and about 6,600 at the equator. Its image showed the effect directly: a bright region around the pole, and a darker band along the equator that is only 60–70% as bright as the pole.
Altair is one of the three bright stars of the Summer Triangle, with Vega and Deneb. The triangle is an asterism, a familiar pattern of stars that is not one of the 88 official constellations. In the Northern Hemisphere it appears high overhead on summer evenings, and it can be seen even from light-polluted cities.