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  2. Orion (constellation) - Wikipedia

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

    It is the middle and brightest of the three stars of Orion's Belt. Alnilam is a B-type blue supergiant; despite being nearly twice as far from the Sun as the other two belt stars, its luminosity makes it nearly equal in magnitude. Alnilam is losing mass quickly, a consequence of its size. It is the farthest major star in Orion at 1,344 light years.

  3. Theta2 Orionis - Wikipedia

    en.wikipedia.org/wiki/Theta2_Orionis

    The three stars of θ 2 Orionis within the Orion Nebula. θ 2 Orionis consists of three stars in a line, each about an arc-minute from the next. In addition to the well-known three stars, the Washington Double Star Catalog confusingly lists a component D which is actually θ 1 Orionis C. [16] There is one other star brighter than 10th magnitude ...

  4. List of stars in Orion - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_in_Orion

    • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] See also [ edit ]

  5. Mintaka - Wikipedia

    en.wikipedia.org/wiki/Mintaka

    Mintaka is the westernmost of the three stars of Orion's belt. It is easily visible to the naked eye, one of the brightest stars in the sky, and has been known since antiquity. Radial velocity measurements taken by Henri-Alexandre Deslandres in 1900 at Paris Observatory showed that Mintaka had a variable radial velocity and therefore was a ...

  6. Pi4 Orionis - Wikipedia

    en.wikipedia.org/wiki/Pi4_Orionis

    Pi 4 Orionis (π 4 Ori, π 4 Orionis) is a binary star system in the western part of the Orion constellation. It is visible to the naked eye with an apparent visual magnitude of 3.7. [ 2 ] Based upon an annual parallax shift of 3.1 mass , [ 1 ] it is located roughly 1,050 light-years from the Sun .

  7. 23 Orionis - Wikipedia

    en.wikipedia.org/wiki/23_Orionis

    23 Orionis is a double star located around 1,200 light-years (370 parsecs) [1] away from the Sun in the equatorial constellation of Orion. [12] It is visible to the naked eye as a dim, blue-white-hued point of light with a combined apparent visual magnitude of 4.99. [2]

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