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UIS5099417
UIS5099415
NHM1456136
NHM1456134
NHM1456138
NHM1456135
NHM1456129
NHM1454043
UDK844821
UIS5073697
![Remains of the supernova Kepler in Ophiuchus - Nasa's three Great Observatories - - the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X - ray Observatory - joined forces to probe the expanding remains of a supernova, called Kepler's supernova remnant, first seen 400 years ago by sky watchers, including famous astronomer Johannes Kepler. The combined image unveils a bubble - shaped shroud of gas and dust that is 14 light - years wide and is expanding at 4 million miles per hour (2,000 kilometers per second). Observations from each telescope highlight distinct features of the supernova remnant, a fast - moving shell of iron - rich material from the exploded star, surrounded by an expanding shock wave that is sweeping up interstellar gas and dust. Each color in this image represents a different region of the electromagnetic spectrum, from X - rays to infrared light. The X - ray and infrared data cannot be seen with the human eye. By color - coding those data and combining them with Hubble's visible - light view, astronomers are presenting a more complete picture of the supernova remnant. Visible - light images from the Hubble telescope's Advanced Camera for Surveys [colored yellow] reveal where the supernova shock wave is slamming into the densest regions of surrounding gas. The bright glowing knots are dense clumps from instabilities that form behind the shock wave. The Hubble data also show thin filaments of gas that look like rippled sheets seen edge - on. These filaments reveal where the shock wave is encountering lower - density, more uniform interstellar material. The Spitzer telescope shows microscopic dust particles [colored red] that have been heated by the supernova shock wave. The dust re - radiates the shock wave's energy as infrared light. The Spitzer data are brightest in the regions surrounding those seen in detail by the Hubble telescope. The Chandra X - ray data show regions of very hot gas, and extremely high - energy particles](https://images-cdn.bridgemanimages.com/api/1.0/image/600wm.PIX.93168540.7055475/4582960.jpg?old-wm)
UIS5104157
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