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STELLAR CHEMISTRY
Star Explosion Leaves Behind a Rose
by Staff Writers
Pasadena CA (JPL) Dec 13, 2011


Some of the green-colored gas and dust in the image is from yet another ancient supernova - the Vela supernova remnant. That explosion happened around 12,000 years ago and was four times closer to us than Puppis A. If you had X-ray vision like the comic book hero Superman, both of these remnants would be among the largest and brightest objects you would see in the sky.

About 3,700 years ago, people on Earth would have seen a brand-new bright star in the sky. It slowly dimmed out of sight and was eventually forgotten, until modern astronomers later found its remains, called Puppis A.

In this new image from NASA's Wide-field Infrared Survey Explorer (WISE), Puppis A looks less like the remains of a supernova explosion and more like a red rose.

Puppis A (pronounced PUP-pis) was formed when a massive star ended its life in a supernova, the most brilliant and powerful form of an explosion in the known universe.

The expanding shock waves from that explosion are heating up the dust and gas clouds surrounding the supernova, causing them to glow and appear red in this infrared view.

While much of the material from that original star was violently thrown out into space, some of it remained in an incredibly dense object called a neutron star.

This particular neutron star (too faint to be seen in this image) is moving inexplicably fast: over 3 million miles per hour! Astronomers are perplexed over its absurd speed, and have nicknamed the object the "Cosmic Cannonball."

Some of the green-colored gas and dust in the image is from yet another ancient supernova - the Vela supernova remnant.

That explosion happened around 12,000 years ago and was four times closer to us than Puppis A.

The colors in this image represent different wavelengths of infrared light that humans can't see with their eyes.

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Related Links
Wise at NASA
Wise at UCLA
Wise at JPL
Stellar Chemistry, The Universe And All Within It






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Lisbon, Portugal (SPX) Dec 13, 2011
A team of researchers, mainly from Centro de Astrofisica da Universidade do Porto (CAUP), has detected a rare type of active galactic nuclei (AGNs), which have simultaneously characteristics of young and old AGNs. This apparent discrepancy is thought to be due to a recent re-ignition of the central black hole. The team cross-correlated a catalogue of over 13 thousand clusters with a catalo ... read more


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