|
|
A Hubble photo of whirlpool galaxy M51 offers new insights into the formation of stars, and a new twist on the composition of galactic arms. M51 is 20 million light-years away, in the constellation Canes Venatici. Why is M51 so pretty? The bright red spots dotting the spiral arms and dust clouds of galaxy are regions of STAR BIRTHS. These are triggered by the gravity of a neighbor galaxy (just off the edge of the image). The clusters of young, luminous and energetic stars are glowing red because this is the color of hydrogen gas emissions. Images from Hubble and Kitt Peak Observatory in Arizona were combined in this composite picture. They reveal the intricate structure of cold dust clouds associated with the hot hydrogen emissions. Note the darker dust "spurs" branching out almost perpendicular to the main spiral arms. |
M51 Whirlpool Galaxy CLOSE UP PHOTO |