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How big is Altair?

2,800,000 kilometroj!

View History Report
Altair

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.

Size

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.

Size comparisons

  • Altair is about twice as wide as the Sun across its equator.
  • About 220 Earths side by side would stretch across its equator.
  • Procyon, which has the same size in the explorer, is almost exactly as wide: about 2.8 million kilometers.
  • Vega, another fast-spinning star, is about 3.8 million kilometers wide at its equator, so Altair is about three-quarters as wide.
  • If the Sun were shrunk to the size of a basketball, Altair would be a slightly squashed ball about 49 centimeters (19 inches) across at its equator and 39 centimeters (15 inches) from pole to pole.

A star that spins in under eight hours

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.

In the night sky

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.

Sources

  • Imaging the Surface of Altair. Monnier et al., Science, 2007.
  • A realistic two-dimensional model of Altair. Bouchaud et al., Astronomy & Astrophysics, 2020.
  • What Are Asterisms. NASA, 2021.
  • IAU Catalog of Star Names. IAU Working Group on Star Names, 2022.
  • The diameter and evolutionary state of Procyon A. Kervella et al., Astronomy & Astrophysics, 2004.
  • Resolving Vega and the inclination controversy with CHARA/MIRC. Monnier et al., The Astrophysical Journal Letters, 2012.
  • Sun Fact Sheet. NASA, 2024.
  • Earth Fact Sheet. NASA, 2024.
  • Official Basketball Rules 2026: Basketball Equipment. FIBA, 2026.

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La Skalo de la Universo > Altair
شباهنگ A
شباهنگ درخشانترین ستاره در آسمان شب است. تقریبا دو برابر درخشان تر از سهیل، دومین ستاره ی درخشان است. با اینحال شباهنگ ستاره ی بزرگی نیست. دلیل درخشندگی زیاد آن نزدیکی آن به ماست چیزی در حدود 8 سال نوری.
آلفا قنطورس A
آلفا قنطورس A بزرگترین ستاره در مجموعه ی ستاره ای آلفا قنطورس )متشکل از سه ستاره(، که نزدیکترین مجموعه ی ستاره ای به ماست می باشد. همچنین چهارمین ستاره ی درخشان در آسمان شب است.
خورشید
نام دیگر خورشید مهر است، خورشید آن چیزی است که به زمین انرژی برای ادامه ی حیات می دهد. قطر خورشید باای 033 برابر قطر زمین است! 20,000 برابر انرژی ای که نژاد بشر مصرف می کند به زمین از طرف خورشید برخورد می کند.
نسر واقع
نسر واقع در صورت فلکی شلیاق قرار دارد. همچنین قسمتی از مثلث تابستانی متشکل از نسر واقع ، نسر طائر، و دنب است. نسر واقع آنقدر سریع به دور خود می چرخد که ورم می کند. گرچه ما آنرا از طرف قطبش مشاهده می کنیم و به نظر دایروی می رسد.
قلب ااسد
قلب ااسد مانند نسر طائر و نسر واقع آنقدر سریع می چرخد که ورم می کند. اگر قلب 1سد 16% بیشتر از سرعت فعلی می چرخید از هم گسیخته می شد! قلب ااسد همچنین درخشانترین ستاره در صورت فلکی شیر است. قلب ااسد B و C نیز وجود دارند.
سماک اعزل
سماک اعزل پانزدهمین ستاره ی درخشان در آسمان شب است و در صورت فلکی سنبله قرار دارد. در واقع سماک اعزل یک سیستم دوتائی است. این دو ستاره بسیار به هم نزدیکند، دوره ی تناوب آنها 4 روز است.

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