Image:Eta Carinae Hubble Chandra Composite.jpg

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Description

The latest composite image shows the remnants of that titanic event with new data from NASA's Chandra X-ray Observatory and the Hubble Space Telescope. The blue regions show the cool optical emission, detected by Hubble, from the dust and gas thrown off the star. This debris forms a bipolar shell around the star, which lies near the brightest point of the optical emission. This bipolar shell is itself surrounded by a ragged cloud of fainter material. An unusual jet points from the star to the upper left.

Chandra's data, depicted in orange and yellow, shows the X-ray emission produced as material thrown off Eta Carinae rams into nearby gas and dust, heating gas to temperatures in excess of a million degrees. This hot shroud extends far beyond the cooler, optical nebula and represents the outer edge of the interaction region.

Source

Chandra X-ray Center

Date

Release Date — June 20, 2007

Author

X-ray: NASA/CXC/GSFC/M.Corcoran et al.; Optical: NASA/STScI

Permission
(Reusing this image)

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[edit] Licensing

Public domain
This file is in the public domain because it was created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (NASA copyright policy page or JPL Image Use Policy).

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current08:58, 26 April 2008720×562 (116 KB)Sumanch ({{Information |Description= The latest composite image shows the remnants of that titanic event with new data from NASA's Chandra X-ray Observatory and the Hubble Space Telescope. The blue regions show the cool optical emission, detected by Hubble, from t)
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