File:SuperNova-PuppisA-XRay-20140910.jpg
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| DescrizioneSuperNova-PuppisA-XRay-20140910.jpg |
English: Unprecedented X-ray View of Supernova Remains — The destructive results of a powerful supernova explosion reveal themselves in a delicate tapestry of X-ray light, as seen in this image from NASA’s Chandra X-Ray Observatory and the European Space Agency's XMM-Newton.
The image shows the remains of a supernova that would have been witnessed on Earth about 3,700 years ago. The remnant is called Puppis A, and is around 7,000 light years away and about 10 light years across. This image provides the most complete and detailed X-ray view of Puppis A ever obtained, made by combining a mosaic of different Chandra and XMM-Newton observations. Low-energy X-rays are shown in red, medium-energy X-rays are in green and high energy X-rays are colored blue. These observations act as a probe of the gas surrounding Puppis A, known as the interstellar medium. The complex appearance of the remnant shows that Puppis A is expanding into an interstellar medium that probably has a knotty structure. Supernova explosions forge the heavy elements that can provide the raw material from which future generations of stars and planets will form. Studying how supernova remnants expand into the galaxy and interact with other material provides critical clues into our own origins. A paper describing these results was published in the July 2013 issue of Astronomy and Astrophysics and is available online. The first author is Gloria Dubner from the Instituto de Astronomía y Física del Espacio in Buenos Aires in Argentina. |
| Data | (release) |
| Fonte | http://chandra.harvard.edu/photo/2014/puppisa/ (image link); see also https://www.nasa.gov/chandra/multimedia/puppisA-2014.html and https://xmm-tools.cosmos.esa.int/external/xmm_science/gallery/public/level3.php?id=1185 |
| Autore | NASA/CXC/IAFE/G. Dubner et al & ESA/XMM-Newton |
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XMM-Newton:
This media was created by the European Space Agency (ESA).
Where expressly so stated, images or videos are covered by the Creative Commons Attribution-ShareAlike 3.0 IGO (CC BY-SA 3.0 IGO) licence, ESA being an Intergovernmental Organisation (IGO), as defined by the CC BY-SA 3.0 IGO licence. The user is allowed under the terms and conditions of the CC BY-SA 3.0 IGO license to Reproduce, Distribute and Publicly Perform the ESA images and videos released under CC BY-SA 3.0 IGO licence and the Adaptations thereof, without further explicit permission being necessary, for as long as the user complies with the conditions and restrictions set forth in the CC BY-SA 3.0 IGO licence, these including that:
See the ESA Creative Commons copyright notice for complete information, and this article for additional details.
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Questo file è disponibile in base alla licenza Creative Commons Attribuzione-Condividi allo stesso modo 3.0 OIG Attribuzione: ESA/XMM-Newton/G. Dubner, N. Loiseau, P. Rodríguez-Pascual, M. J. S. Smith, E. Giacani, and G. Castelletti, CC BY-SA IGO 3.0
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Chandra:
| Public domainPublic domainfalsefalse |
| Questo file è nel pubblico dominio perché creato dalla NASA. La politica sul copyright della NASA afferma che «il materiale della NASA non è protetto da copyright a meno che non sia specificato altrimenti». (NASA copyright policy e JPL Image Use Policy). | ||
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