File:187900main colorpress1 lg.jpg

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English: The XMM-Newton spectral signature from superheated iron atoms at the inner edge of the accretion disk orbiting the neutron star in Serpens X-1. Normally, the line would be a symmetrical peak, but it exhibits the classic features of distortion due to relativistic effects. The extremely fast motion of the iron-rich gas causes the line to spread out. The entire line has been shifted to longer wavelengths (left, red) because of the neutron star's powerful gravity. The line is brighter toward shorter wavelengths (right, blue) because Einstein's special theory of relativity predicts that a high-speed source beamed toward Earth will appear brighter than the same source moving away from Earth.
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Source NASA's Imagine the Universe! Goddard Spaceflight Center, Astronomers Pioneer New Method for Probing Exotic Matter
Author Sudip Bhattacharyya and Tod Strohmayer
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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Date/TimeThumbnailDimensionsUserComment
current04:52, 16 November 2009Thumbnail for version as of 04:52, 16 November 2009463 × 413 (39 KB)Materialscientist (talk | contribs)cropped white space
01:51, 4 November 2009Thumbnail for version as of 01:51, 4 November 2009540 × 450 (40 KB)Marshallsumter (talk | contribs){{Information |Description={{en|1="This is fundamental physics," says Sudip Bhattacharyya of NASA's Goddard Space Flight Center in Greenbelt, Md. and the University of Maryland. "There could be exotic kinds of particles or states of matter, such as quark

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