Cassiopeia A
Astronomical Object
A neutron star is born: Stellar core just 12 miles across spotted 11,000 light years away...X-ray source in 1999. Astronomers now know the source is a neutron star 11,000 light years from Earth at the centre of the supernova Cassiopeia A. This supernova was captured by Nasa's Chandra X-Ray Observatory. The neutron star is the... In this article: Carbon, Chandra X-ray Observatory, NASA, Earth, Neutron, Nuclear fusion, Atom, Nature, and University of Alberta |
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New Kerala | November 05, 2009
Carbon atmosphere discovered on neutron star
...models, Ho and his colleague Craig Heinke, from the University of Alberta, determined that the neutron star in Cassiopeia A, or Cas A for short, has an ultra-thin coating of carbon. This is the first time the composition of an...
In this article: Carbon, Neutron, Chandra X-ray Observatory, Hydrogen, and Helium
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Wired: Wired Science | November 04, 2009
Baby Neutron Star Found Inside Supernova Remnant
...finally identified the mysterious source of X-ray emissions at the center of our galaxy's youngest supernova: Inside the remains of Cassiopeia A sits a baby neutron star surrounded by a thin layer of carbon dioxide. Twenty times heavier...
In this article: NASA, Cassiopeia, Chandra X-ray Observatory, Carbon dioxide, Supernova, Nuclear fusion, Magnetic field, Wired.com, and Carbon
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EurekAlert! - Space and Planetary Science | November 03, 2009
U of A physicist identifies mysterious core left by exploding star
...its surface, producing a carbon atmosphere just 10 centimeters thick." Heinke is co author of a research paper on the identification of the Cassiopeia A supernova remnant as a neutron star. It will be published Nov. 5, in Nature. Great...
In this article: Carbon, Physics, Nuclear fusion, Chandra X-ray Observatory, University of Alberta, and NASA
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Wikipedia | October 10, 2009
Cassiopeia A
...Hubble Space Telescope, and blue and green are data from the Chandra X-ray Observatory Cassiopeia A observed by the Hubble Space Telescope Cassiopeia A (Cas A) is a supernova remnant in the constellation Cassiopeia and the brightest...
In this article: Hubble Space Telescope, Earth, Chandra X-ray Observatory, Spitzer Space Telescope, Milky Way, Cassiopeia, and John Flamsteed
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ScienceDaily: Latest Science News | August 19, 2009
Scientists Make First Discovery Using Revolutionary Long Wavelength Demonstrator Array
...eventually consist of nearly 13,000 similar antennas. Utilizing radio emissions from the approximately 300 year-old Cassiopeia A (Cas A) supernova remnant (SNR)-one of the brightest astronomical radio sources in the sky-to establish...
In this article: National Radio Astronomy Observatory, University of New Mexico, Very Large Array, and Astronomical Journal
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Prime Newswire | July 22, 2009
NASA's Northrop Grumman-Built Chandra X-Ray Observatory Marks 10th Anniversary On-Orbit
...Flight Center, Chandra's first light image gave astronomers their first glimpse of the point source at the center of the supernova remnant Cassiopeia A. Since then, Chandra has significantly expanded the frontiers of astronomy, providing...
In this article: Northrop Grumman Corporation, NASA, Chandra X-ray Observatory, and Nobel Prize
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ScienceDaily: Latest Science News | February 24, 2009
Cassiopeia A Supernova Remnant Is Now 'Dust Factory' Around Dead Star
...the NASA/ESA Hubble Space Telescope provides a detailed look at the tattered remains of a supernova explosion known as Cassiopeia A (Cas A). It is the youngest known remnant ... > read more Infrared Echoes Give NASA's Spitzer A Supernova...
In this article: NASA, Supernova, Royal Astronomical Society, Spitzer Space Telescope, Magnetic field, and University of Nottingham
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Science News Online | January 06, 2009
Evolution, 3-D animation of Cassiopeia A
...per hour. That's in fact considerably slower than expected for an explosion believed to have unleashed Cassiopeia A's estimated energy. Remnants of Cassiopeia A (2D)VIDEO | The evolution of the supernova remnant Cassiopeia A is shown by...
In this article: NASA, Chandra X-ray Observatory, Spitzer Space Telescope, Argon, Harvard-Smithsonian Center for Astrophysics, and MIT
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EurekAlert! - Space and Planetary Science | January 05, 2009
Cassiopeia A comes alive across time and space
...a dramatic three-dimensional visualization of the same remnant. Nearly ten years ago, Chandra's "First Light" image of Cassiopeia A (Cas A) revealed previously unseen structures and detail. Now, after eight years of observation, scientists...
In this article: NASA, Harvard., Smithsonian Astrophysical Observatory, Cambridge, and Massachusetts
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The Hindu - News | May 31, 2008
Unearthed: Secrets of supernova remnant
...in life and ultimately how it met its demise by decoding ghostly echoes of light travelling away from the remains of Cassiopeia A. Cassiopeia A is one of the most explored objects in our sky. It is the burnt-out corpse of a massive star that...
In this article: Hydrogen, Helium, Max Planck Institute for Astronomy, University of California, Subaru, New York, and Germany
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Description from Wikipedia:
Cassiopeia A (Cas A) is a supernova remnant in the constellation Cassiopeia and the brightest astronomical radio source in the sky, with a flux of 2720 Jy at 1 GHz. The supernova occurred approximately 11 kly away in the Milky Way. The expanding cloud of material left over from the supernova is now approximately 10 ly across. Despite its radio brilliance, however, it is extremely faint optically, and is only visible on long-exposure photographs.
It is believed that first light from the stellar explosion reached Earth approximately 300 years ago but there are no historical records of any sightings of the progenitor supernova, probably due to interstellar dust absorbing optical wavelength radiation before it reached Earth (although it is possible that it was recorded as a sixth magnitude star 3 Cassiopeiae by John Flamsteed on August 16, 1680). Possible explanations lean toward the idea that the source star was unusually massive and had previously ejected much of its outer layers. These outer layers would have cloaked the star and reabsorbed much of the light released as the inner star collapsed.
Cas A is 3C461 in the Third Cambridge Catalogue of Radio Sources and G111.7-2.1 in the Green Catalog of Supernova Remnants.
It is known that the expansion shell has a temperature of around 50 million degrees Fahrenheit (30 megakelvins), and is travelling at more than ten million miles per hour (4 Mm/s).
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