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  2. List of stars in Orion - Wikipedia

    en.wikipedia.org/wiki/List_of_stars_in_Orion

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  3. W Orionis - Wikipedia

    en.wikipedia.org/wiki/W_Orionis

    W Orionis is a carbon star in the constellation Orion, approximately 400 parsecs (1,300 ly) away.It varies regularly in brightness between extremes of magnitude 4.4 and 6.9 roughly every 7 months.

  4. Bellatrix - Wikipedia

    en.wikipedia.org/wiki/Bellatrix

    Bellatrix is the third-brightest star in the constellation of Orion, positioned 5° west of the red supergiant Betelgeuse (Alpha Orionis). It has the Bayer designation γ Orionis, which is Latinized to Gamma Orionis.

  5. Orion (constellation) - Wikipedia

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

    Orion is a prominent set of stars visible during winter in the northern celestial hemisphere.It is one of the 88 modern constellations; it was among the 48 constellations listed by the 2nd-century astronomer Ptolemy.

  6. Bayer designation - Wikipedia

    en.wikipedia.org/wiki/Bayer_designation

    Detail of Bayer's chart for Orion showing the belt stars and Orion Nebula region, with both Greek and Latin letter labels visible. A Bayer designation is a stellar designation in which a specific star is identified by a Greek or Latin letter followed by the genitive form of its parent constellation's Latin name.

  7. Meissa - Wikipedia

    en.wikipedia.org/wiki/Meissa

    Meissa / ˈ m aɪ s ə /, designated Lambda Orionis (λ Orionis, abbreviated Lambda Ori, λ Ori) is a star in the constellation of Orion.It is a multiple star approximately 1,300 ly away with a combined apparent magnitude of 3.33. [11]

  8. FU Orionis - Wikipedia

    en.wikipedia.org/wiki/FU_Orionis

    FU Orionis is a variable and binary star [9] system in the constellation of Orion, that in 1937 rose in apparent visual magnitude from 16.5 to 9.6, and has since been around magnitude 9.

  9. Trapezium Cluster - Wikipedia

    en.wikipedia.org/wiki/Trapezium_Cluster

    The Trapezium is most readily identifiable by the asterism of four relatively bright stars for which it is named. The four are often identified as A, B, C and D in order of increasing right ascension.