Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  IC 4263  ·  IC 4278  ·  M 51  ·  NGC 5169  ·  NGC 5173  ·  NGC 5194  ·  NGC 5195  ·  NGC 5198  ·  Whirlpool Galaxy
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M51 Whirlpool Galaxy, Andrei Gusan
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M51 Whirlpool Galaxy

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M51 Whirlpool Galaxy, Andrei Gusan
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M51 Whirlpool Galaxy

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Description

The graceful, winding arms of the majestic spiral galaxy M51, also knows as The Whirlpool Galaxy, appear like a grand spiral staircase sweeping through space. They are actually long lanes of stars and gas laced with dust. Such striking arms are a hallmark of so-called grand-design spiral galaxies. In M51 these arms serve an important purpose: they are star-formation factories, compressing hydrogen gas and creating clusters of new stars.

Some astronomers think that the Whirlpool’s arms are particularly prominent because of the effects of a close encounter with NGC 5195, the small, yellowish galaxy at the left-hand-side of one of the arms. The compact galaxy appears to be tugging on the arm, the tidal forces from which trigger new star formation. Hubble’s clear view shows that NGC 5195 is passing behind M51. The small galaxy has been gliding past the Whirlpool for hundreds of millions of years.

In this image taken from my amateur backyard observatory the pink represents hydrogen within giant star-forming regions. The blue color can be attributed to hot, young stars while the yellow color is from older stars.

Discovered by Charles Messier in 1773, M51 is located 23 million light-years from Earth in the constellation Canes Venatici. It has an apparent magnitude of 8.4 and can be spotted with a small telescope most easily during May. The Whirlpool galaxy’s beautiful face-on view and closeness to Earth allow astronomers to study a classic spiral galaxy’s structure and star-forming processes.

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M51 Whirlpool Galaxy, Andrei Gusan