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Two Views of a Star’s Exploded Remains

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This layout compares two pictures of a supernova remnant called SN 1987A — the left image was taken by the Herschel Space Observatory, and the right is an enlarged view of the circled region at left, taken with NASA’s Hubble Space Telescope. SN 1987A is the result of a stellar blast that occurred 170,000 light-years away and was seen on Earth in 1987. The tiny pink ring in the Hubble image shows where a shock wave from the blast is hitting the surrounding material expelled from the star before the explosion. The cause for the outer, faint rings is unknown…..

When Herschel observed SN 1987A, it saw something different. Herschel sees infrared and submillimeter light, much longer in wavelength than the visible light Hubble detects. For this reason, its picture of the supernova is not as sharp, appearing only as a fuzzy dot inside the circle. But that dot represents an important discovery of vast reservoirs of cold dust around SN 1987A. Herschel can see very cold material — the colder something is, the longer the wavelengths of light it emits.

The finding demonstrates that supernova can indeed create copious amounts of fresh dust, and likely are the primary source of dust in the very early universe.

The Herschel image also shows filamentary structures surrounding the region of SN 1987A. These are from cold dust, as cold as 10 to 20 Kelvin (minus 442 to minus 423 degrees Fahrenheit), filling the space between the stars. The dust in the interstellar space may have originally formed in past explosions of other supernovae.

SN 1987A is located in the Large Magellanic Cloud, a satellite galaxy to our own Milky Way. SN 1987A is the one of the closest supernovae monitored by humans for the last 400 years. It has provided astronomers with an opportunity to understand how a star dies and changes shape over 20 years.

The Hershel image was taken by the Photodetector Array Camera and Spectrometer, and the Spectral and Photometric Imaging Receiver, at wavelengths of 100, 160 and 250 microns, which are just about one-tenth to one-quarter of a millimeter.

Herschel is a European Space Agency cornerstone mission, with science instruments provided by consortia of European institutes and with important participation by NASA. NASA’s Herschel Project Office is based at NASA’s Jet Propulsion Laboratory. JPL contributed mission-enabling technology for two of Herschel’s three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the United States astronomical community. Caltech manages JPL for NASA.
More information is online at

http://www.herschel.caltech.eduhttp://www.nasa.gov/herschel and

http://www.esa.int/SPECIALS/Herschel/index.html and

http://www.nasa.gov/mission_pages/herschel/news/herschel20110707.html

http://www.nasa.gov/mission_pages/herschel/pia14109.html

Written by physicsgg

July 8, 2011 at 1:35 pm

Posted in ASTRONOMY

Tagged with , ,

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