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Whirlpool Galaxy

Whirlpool Galaxy Observation data (J2000 epoch) Constellation Canes Venatici Right ascension 13h 29m 52.7s Declination +47° 11' 43? Redshift 463 ± 3 km/s Distance 23 ± 4 Mly (7.1 ± 1.2 Mpc) Type SA(s)bc pec Apparent dimensions (V) 11'.2 × 6'.9 Apparent magnitude (V) 8.4 Notable features Interacting with NGC 5195 Other designations Question Mark Galaxy, Rosse's Galaxy, M51a, NGC 5194, UGC 8493, PGC 47404, VV 001a, VV 403, Arp 85, GC 3572 See also: Galaxy, List of galaxies The Whirlpool Galaxy (also known as Messier 51a, M51a, or NGC 5194) is an interacting grand-design spiral galaxy in the constellation Canes Venatici. Recently it was estimated to be 23 ± 4 million light-years from the Milky Way Galaxy, but different methods yield distances between 15 and 35 million ly. Messier 51 is one of the best known galaxies in the sky.The galaxy and its companion (NGC 5195) are easily observed by amateur astronomers, and the two galaxies may even be seen with binoculars. The Whirlpool Galaxy is also a popular target for professional astronomers, who study it to further understand galaxy structure (particularly structure associated with the spiral arms) and galaxy interactions. Cite error: There are tags on this page, but the references will not show without a {{reflist}} template (see the help page).
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