Galaxies go into shock
Posted: Monday, July 13, 2009 8:26 PM by Alan Boyle

NASA / CSC / CfA / CFHT / Coelum |
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Composite photo shows optical and X-ray views of Stephan's Quintet, a galactic collision that has generated a powerful shock wave (indicated here in light blue).
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A shockingly beautiful image of a galactic smash-up known as Stephan's Quintet highlights the powerful shock wave created by a cosmic bullet.
The compact galaxy group, 230 million light-years from Earth in the constellation Pegasus, is one of the favorite targets for astronomers studying gravitational interactions on a grand scale. It was discovered in 1877 by French astronomer Edouard Stephan.
For many astronomers, the most interesting feature is something that doesn't show up quite as well in visible-light pictures: the light blue arc of X-ray emissions running through the center of the image above.
That X-ray arc, detected by NASA's Chandra X-Ray Observatory, shows up prominently in other wavelengths as well - such as the infrared part of the spectrum that is the NASA's Spitzer Space Telescope specialty. Scientists have concluded that it represents a shock wave that is slamming through the group's intergalactic gas and heating it up so much that it emits radiation in a wide range of wavelengths. The shock wave is generated by the passage of one galaxy (NGC 7318b) through the cluster's core at a speed of almost 2 million miles per hour.
If you click on over to the Chandra Web site and roll your cursor over the picture accompanying the image advisory, you'll see pointers to the assorted galaxies in the cluster. The galaxy at lower left, NGC 7320, is in the foreground and doesn't actually interact with the other four. Think of it as a "fifth Beatle," bringing a little extra star power into the picture of an already-stellar quartet.
A larger map of X-ray emissions, charted by the European Space Agency's XMM-Newton observatory, suggests that there may have been earlier shock waves that have created an X-ray halo around Stephan's Quintet. The long tails of stars spinning off the galaxies provide further evidence of past gravitational interactions.
As usual, Chandra's view of Stephan's Quintet is much more than just a pretty picture.
"Stephan's Quintet provides a rare opportunity to observe a galaxy group in the process of evolving from an X-ray-faint system dominated by spiral galaxies to a more developed system dominated by elliptical galaxies and bright X-ray emission," Chandra's science team said. "Being able to witness the dramatic effect of collisions in causing this evolution is important for increasing our understanding of the origins of the hot, X-ray-bright halos of gas in groups of galaxies."
More shockingly beautiful space pictures:
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