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Whirlpool Galaxy (M51, NGC5194)

Whirlpool Galaxy (M51, NGC5194) is a spiral galaxy object of interest in space. It lies at a distance of 19,000-27,000 kilo light years away in the constellation of Canes Venatici.

It is referred to as M(51) when it was catalogued by Charles Messier in 18th - 19th Century France. It is also referred to as NGC(5194) in the New General Catalogue. This is a list of deep space objects that was compiled by John Louis Emil Dreyer in 1888 in an update to John Herschel earlier catalogue.

The Spiral Galaxy's location is 13:29.9 (R.A.) and +47:12 (Dec.). Its Visual Brightness is a 8.4 Magnitude and has an apparent magnitude of 8 with an apparent dimension of 11x7 . The object can not be seen by the naked eye, you need a telescope to see it.

Whirlpool galaxy (M51,NGC5194) is a spiral galaxy. It was discovered in 1773 by Charles Messier. It's location is RA(13:29.9), Dec(+47:12) and its distance is calculated 19.000-27.000 light years away. Its visual Brightness is 8.4. Its apparent dimensions measured in arcmins is 11x7.

Fact File

NameWhirlpool Galaxy (M51, NGC5194)
TypeSpiral Galaxy
Messier Id51
NGC Id5194
ConstellationCanes Venatici
Right Ascension13:29.9
Distance (Lt.Yr)19,000-27,000 kilo
Visual Brightness8.4
Apparent Dimension11x7
Apparent Magnitude8
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Year of Discovery1773
DiscovererCharles Messier
CoprightN.A.S.A, Hubble Site

Whirlpool Galaxy (M51, NGC5194) Spiral Galaxy in Canes Venatici

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