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  2. Procyon - Wikipedia

    en.wikipedia.org/wiki/Procyon

    Procyon is a binary star system with a bright primary component, Procyon A, having an apparent magnitude of 0.34, [3] and a faint companion, Procyon B, at magnitude 10.7. [4] The pair orbit each other with a period of 40.84 years along an elliptical orbit with an eccentricity of 0.4, [ 9 ] more eccentric than Mercury 's.

  3. Canis Minor - Wikipedia

    en.wikipedia.org/wiki/Canis_Minor

    The constellation's dimmer stars were noted by Johann Bayer, who named eight stars including Alpha and Beta, and John Flamsteed, who numbered fourteen. Procyon is the eighth-brightest star in the night sky, as well as one of the closest. A yellow-white main-sequence star, it has a white dwarf companion. Gomeisa is a blue-white main-sequence star.

  4. List of nearest stars by spectral type - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_stars_by...

    This is a list of F-type stars within 50 light years. Procyon A is the closest F-type star to the Earth. Name Distance Spectral type Stellar radius (R ...

  5. List of brightest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_brightest_stars

    Such multiple star systems are indicated by parentheses showing the individual magnitudes of component stars bright enough to make a detectable contribution. For example, the binary star system Alpha Centauri has the total or combined magnitude of −0.27, while its two component stars have magnitudes of +0.01 and +1.33. [3]

  6. List of proper names of stars - Wikipedia

    en.wikipedia.org/wiki/List_of_proper_names_of_stars

    In 2016, the International Astronomical Union (IAU) organized a Working Group on Star Names (WGSN) [2] to catalog and standardize proper names for stars. The WGSN's first bulletin, dated July 2016, [3] included a table of 125 stars comprising the first two batches of names approved by the WGSN (on 30 June and 20 July 2016) together with names of stars adopted by the IAU Executive Committee ...

  7. Winter Triangle - Wikipedia

    en.wikipedia.org/wiki/Winter_Triangle

    The Winter Triangle is an astronomical asterism formed from three of the brightest stars in the winter sky. It is an imaginary isosceles triangle [a] drawn on the celestial sphere, with its defining vertices at Sirius, Betelgeuse, and Procyon, the primary stars in the three constellations of Canis Major, Orion, and Canis Minor, respectively. [1]

  8. List of supernova candidates - Wikipedia

    en.wikipedia.org/wiki/List_of_supernova_candidates

    Prominent examples of stars in this mass range include Antares, Spica, Gamma Velorum, [2] Mu Cephei, and members of the Quintuplet Cluster. [3] Type Ia supernova progenitors are white dwarf stars that are close to the Chandrasekhar limit of about 1.44 solar masses and are accreting matter from a binary companion star.

  9. Winter Hexagon - Wikipedia

    en.wikipedia.org/wiki/Winter_Hexagon

    All stars of an apparent magnitude of at least 2 mag are labelled. Winter constellations as seen from the tropics Flip book (158 images): Transit of Mars, Sun, Mercury, and Venus in 2017. The Winter Hexagon is an asterism appearing to be in the form of a hexagon with vertices at Rigel, Aldebaran, Capella, Pollux, Procyon, and Sirius.