Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  IC 4277  ·  IC 4278  ·  M 51  ·  NGC 5194  ·  NGC 5195  ·  Whirlpool Galaxy
M51 Galaxy, Luca Dinoi
M51 Galaxy
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M51 Galaxy

M51 Galaxy, Luca Dinoi
M51 Galaxy
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M51 Galaxy

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Description

M 51 is an astronomical object from Messier's catalog which includes two distinct galaxies, in the boreal constellation of Cani Hunting:

The larger and more famous Whirlpool Galaxy (also known as NGC 5194 and sometimes M51A) is a classic spiral galaxy. It was discovered by Charles Messier on October 13, 1773.
The smaller companion galaxy known as NGC 5195 (or also M51B), is partially covered by a dust arm of the Vortex spiral (with which it interacts) and was discovered by Pierre Méchain in 1781.

The Whirlpool Galaxy is one of the brightest and most interesting galaxies in the sky: it is 15 to 37 million light-years from Earth and 50,000 to 100,000 light-years wide. It is also the dominant member of a small group of galaxies called the M51 group. Much of its intense brightness is due to the presence, in the arms, of young star clusters. This galaxy was the first whose spiral structure was observed, by William Parsons in 1845; astronomers speculate that the spiral shape is mainly due to gravitational interactions with the smaller galaxy. The spiral drawn by the arms of the galaxy is a logarithmic spiral.

The Whirlpool Galaxy is joined to NGC 5195 through a common envelope of gas. The interaction between the two galaxies has led to increased star creation in NGC 5195. The core of the Whirlpool Galaxy is also brighter than one might expect, leading some scholars to classify it as an active Seyfert galaxy.

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M51 Galaxy, Luca Dinoi