Misplaced Pages

Whirlpool Galaxy: Difference between revisions

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.
Browse history interactively← Previous editNext edit →Content deleted Content addedVisualWikitext
Revision as of 02:08, 8 July 2004 editBryan Derksen (talk | contribs)Extended confirmed users95,333 editsm Category:NGC objects← Previous edit Revision as of 08:33, 28 July 2004 edit undo194.237.245.238 (talk) interwiki sv:Next edit →
Line 11: Line 11:
] ]
] ]

]

Revision as of 08:33, 28 July 2004

The Whirlpool Galaxy, Messier Object 51 (M51), also known as NGC 5194, is a classic spiral galaxy, discovered by Charles Messier on October 13, 1773. It is one of the brightest, most compelling galaxies in the sky, visible with binoculars in the constellation Canes Venatici. The spiral galactic structure was first observed in this galaxy, which is the dominant member of a 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 -- some measurements put the distance at only 15 million.

External links

This article is a stub. You can help Misplaced Pages by expanding it.

Categories: