AstroBinAstroBin
Contains:  Other
M51, Stephen Duffy

M51

M51, Stephen Duffy

M51

Description

The graceful, winding arms of the majestic spiral galaxy M51 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, also known as the Whirlpool galaxy, 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 outermost tip of one of the arms. The compact galaxy appears to be tugging on the arm, the tidal forces from which trigger new star formation. NGC 5195 is passing behind M51. The small galaxy has been gliding past the Whirlpool for hundreds of millions of years.

In this image of M51, the red 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 31 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.
Text from NASA\Goddard
Scope: Skywatcher MN190, Camera QSI683, Mount Orion Atlas
L:R:G:B 7.5:2.5:2.5:2.5 hours

Comments

Histogram

M51, Stephen Duffy

In these public groups

Sacramento Valley Astronomical Society
×

Warning!

This operation will reload the current page. If you have any unsaved information in a form, it will be lost.

You can also dismiss this window, and your operation will be applied at the next page navigation.