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    Whirlpool Galaxy (M51, NGC 5194)

    Whirlpool Galaxy (M51, NGC 5194)
    The Whirlpool Galaxy. Image courtesy Richard Crisp
    A large, bright spiral galaxy in the constellation Canes Venatici that is interacting with a much smaller neighbor, NGC 5195. The main galaxy was discovered by Charles Messier in 1773, the companion by Pierre Méchain in 1781.

    M51 is the first galaxy in which spiral structure was discovered, by Lord Rosse in 1845. This structure, however, has clearly been influenced by the gravitational effect of the companion, which has triggered a huge burst of star formation in the Whirlpool and has also distorted its arms.

    M51 is the dominant member of a small group of galaxies that also includes the Sunflower Galaxy (M63) and half a dozen other smaller systems.



    Visual magnitude 8.4
    Apparent size 11' × 7'
    Distance 31 million light-years (9.5 Mpc)
    Position R.A. 13h 29.9m, Dec. +47° 12'



    Related categories

       • GALAXIES
       • MESSIER CATALOGUE



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