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  2. Aquila (constellation) - Wikipedia

    en.wikipedia.org/wiki/Aquila_(constellation)

    Aquila is a constellation on the celestial equator. Its name is Latin for 'eagle' and it represents the bird that carried Zeus/Jupiter's thunderbolts in Greek-Roman mythology. Its brightest star, Altair, is one vertex of the Summer Triangle asterism. The constellation is best seen in the northern summer, as it is located along the Milky Way.

  3. Altair - Wikipedia

    en.wikipedia.org/wiki/Altair

    Altair is the brightest star in the constellation Aquila. α Aquilae (Latinised to Alpha Aquilae) is the star's Bayer designation. The traditional name Altair has been used since medieval times. It is an abbreviation of the Arabic phrase النسر الطائر Al-Nisr Al-Ṭa'ir, "the flying eagle ". [22]

  4. List of stars in Aquila - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_in_Aquila

    List of stars in Aquila. ... This is the list of 143 notable stars in the constellation Aquila, ... Atair, Al Nesr Al Tair, Vulture Volans; [1] 12th brightest star; ...

  5. Eta Aquilae - Wikipedia

    en.wikipedia.org/wiki/Eta_Aquilae

    Eta Aquilae (η Aql, η Aquilae) is a multiple star in the equatorial constellation of Aquila, the eagle.It was once part of the former constellation Antinous.Its apparent visual magnitude varies between 3.49 and 4.3, [3] making it one of the brighter members of Aquila.

  6. Iota Aquilae - Wikipedia

    en.wikipedia.org/wiki/Iota_Aquilae

    Iota Aquilae, Latinized from ι Aquilae, is the Bayer designation for a star in the equatorial constellation of Aquila. It has the traditional name Al Thalimain / æ l ˌ θ æ l ɪ ˈ m eɪ n /, which it shares with λ Aquilae. The name is derived from the Arabic term الظليمین al-ẓalīmayn meaning "The Two Ostriches". [9]

  7. V603 Aquilae - Wikipedia

    en.wikipedia.org/wiki/V603_Aquilae

    V603 Aquilae (or Nova Aquilae 1918) was a bright nova first observed (from Earth) in the constellation Aquila in 1918. It was the brightest "new star" to appear in the sky since Kepler's Supernova in 1604. Like all novae, it is a binary system, comprising a white dwarf and donor low-mass star in close orbit to the point of being only semidetached.

  8. Theta Aquilae - Wikipedia

    en.wikipedia.org/wiki/Theta_Aquilae

    Theta Aquilae (θ Aql, θ Aquilae) is a binary star in the constellation Aquila.The combined apparent visual magnitude of the pair is 3.26, [2] making it the fourth-brightest member of the constellation.

  9. TT Aquilae - Wikipedia

    en.wikipedia.org/wiki/TT_Aquilae

    TT Aquilae (TT Aql) is a Classical Cepheid (δ Cep) variable star in the constellation Aquila. The visual apparent magnitude of TT Aql ranges from 6.52 to 7.65 over 13.7546 days. [3] The light curve is asymmetric, with the rise from minimum to maximum brightness only taking half the time of the fall from maximum to minimum. [11]