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> Spiral galaxy M64 in Coma Berenices
Spiral galaxy M64 in Coma Berenices
author: Nasa/Hubble heritage team/Novapix
reference: a-gax48-26002
Image Size 300 DPI: 7 * 9 cm
Messier 64 (M64) has a spectacular dark band of absorbing dust in front of the galaxy's bright nucleus, giving rise to its nicknames of the "Black Eye" or "Evil Eye" galaxy. Fine details of the dark band are revealed in this image of the central portion of M64 obtained with the Hubble Space Telescope. Located in the northern constellation Coma Berenices, M64 resides roughly 17 million light-years from Earth. As in the majority of galaxies, all of the stars in M64 are rotating in the same direction, clockwise as seen in the Hubble image. However, detailed studies in the 1990's led to the remarkable discovery that the interstellar gas in the outer regions of M64 rotates in the opposite direction from the gas and stars in the inner regions. Active formation of new stars is occurring in the shear region where the oppositely rotating gases collide, are compressed, and contract. Particularly noticeable in the image are hot, blue young stars that have just formed, along with pink clouds of glowing hydrogen gas that fluoresce when exposed to ultraviolet light from newly formed stars. Astronomers believe that the oppositely rotating gas arose when M64 absorbed a satellite galaxy that collided with it, perhaps more than one billion years ago. This small galaxy has now been almost completely destroyed, but signs of the collision persist in the backward motion of gas at the outer edge of M64.
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