Misplaced Pages

Whirlpool Galaxy

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.

This is an old revision of this page, as edited by Adrian.benko (talk | contribs) at 11:02, 7 July 2005 (interwiki (sk)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Revision as of 11:02, 7 July 2005 by Adrian.benko (talk | contribs) (interwiki (sk))(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)
File:M51 whirlpool galaxy.jpeg
Messier Object 51, the Whirlpool Galaxy. From astrophoto.com, used with permission.

The Whirlpool Galaxy (also known as Spiral Galaxy M51, Messier Object 51, Messier 51, M51, or NGC 5194) is a classic spiral galaxy located in the Canes Venatici constellation. It was discovered by Charles Messier on October 13, 1773.

General information

Another perspective of the Whirlpool Galaxy.

The Whirpool Galaxy is one of the brightest, most compelling galaxies in the sky, visible with binoculars. The spiral galactic structure was first observed in this galaxy, which is the dominant member of the M51 group of galaxies.

Its companion galaxy, NGC 5195, was discovered in 1781 by Pierre Méchain. Sometimes M51 is used to refer to the pair of galaxies, in which case the individual galaxies may be referred to as M51A (5194) and M51B (5195). The galaxy is less than 37 million light years away from Earth — some measurements put the distance at only 15 million.

External links

Categories: