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  2. Rho Aquilae - Wikipedia

    en.wikipedia.org/wiki/Rho_Aquilae

    Rho Aquilae, ρ Aquilae, is the Bayer designation for a star in the northern constellation of Delphinus. It has an apparent visual magnitude of 4.94 [ 2 ] and is bright enough to be seen with the naked eye in good conditions.

  3. 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.

  4. Astronomical symbols - Wikipedia

    en.wikipedia.org/wiki/Astronomical_symbols

    The use of astronomical symbols for the Sun and Moon dates to antiquity. The forms of the symbols that appear in the original papyrus texts of Greek horoscopes are a circle with one ray for the Sun and a crescent for the Moon. [3] The modern Sun symbol, a circle with a dot (☉), first appeared in Europe in the Renaissance. [3]

  5. Theta Aquilae - Wikipedia

    en.wikipedia.org/wiki/Theta_Aquilae

    Theta Aquilae (θ Aql, θ Aquilae), also named Antinous, [8] 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.

  6. Altair - Wikipedia

    en.wikipedia.org/wiki/Altair

    Altair in comparison with the Sun. Along with β Aquilae and γ Aquilae, Altair forms the well-known line of stars sometimes referred to as the Family of Aquila or Shaft of Aquila. [17]: 190 Altair is a type-A main-sequence star with about 1.8 times the mass of the Sun and 11 times its luminosity.

  7. R Aquilae - Wikipedia

    en.wikipedia.org/wiki/R_Aquilae

    R Aquilae is a variable star in the equatorial constellation of Aquila. It is located approximately 760 light years distant from the Sun [ 6 ] and is drifting further away with a radial velocity of 35 km/s. [ 5 ]

  8. Zeta Aquilae - Wikipedia

    en.wikipedia.org/wiki/Zeta_Aquilae

    Zeta Aquilae, or ζ Aquilae, is a binary star [8] system in the equatorial constellation of Aquila. It is readily visible with the naked eye, being of the third magnitude. [ 2 ] Based on parallax measurements obtained during the Hipparcos mission, it is approximately 83 light-years (25 parsecs ) distant from the Sun . [ 1 ]

  9. NGC 6755 - Wikipedia

    en.wikipedia.org/wiki/NGC_6755

    NGC 6755 is an open cluster of stars in the equatorial constellation of Aquila, positioned about 3° to the east of the star Delta Aquilae. [2] It was discovered by the Anglo-German astronomer William Herschel on July 30, 1785 [5] and is located at a distance of 8,060 light years from the Sun. [1]