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Recent Podcast
A Tour of Eta Carinae
A Tour of Eta Carinae
New Chandra data are helping astronomers better understand how the two stars in Eta Carinae interact with one another through powerful winds blowing off their surfaces. (2014-08-27)


G54.1+0.3 in 60 Seconds

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Narrator (Megan Watzke, CXC): Data from the Chandra X-ray Observatory and the Spitzer Space Telescope were combined to create this image of the dusty remains of a collapsed star. This object, known as G54.1+0.3, is a supernova remnant some 20,000 light years from Earth. The white object near the center of the image is a dense, rapidly-rotating neutron star called a pulsar that was left behind after the star collapsed. The pulsar generates a wind of high-energy particles, seen in the Chandra data, that expands into the surrounding environment, illuminating the material ejected in the supernova explosion. This infrared data shows a shell of dust and gas that's being dispersed back into space where it one day may become part of a new generation of stars and planets.

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