Observation • October 6th, 2004 • ssc2004-15b1
This infrared image from NASA's Spitzer Space Telescope shows 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 supernova remnant is a fast-moving shell of iron-rich material from an exploded star, surrounded by an expanding shock wave that is sweeping up interstellar gas and dust. The image reveals 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).
The Spitzer telescope shows microscopic dust particles that have been heated by the supernova shock wave. The dust re-radiates the shock wave's energy as infrared light.
Kepler's supernova, the last such object seen to explode in our Milky Way galaxy, resides about 13,000 light-years away in the constellation Ophiuchus.
The Spitzer observations were taken in August 2004.
About the Object
|Infrared||3.6 µm||Spitzer IRAC|
|Infrared||4.5 µm||Spitzer IRAC|
|Infrared||8.0 µm||Spitzer IRAC|
|Infrared||24.0 µm||Spitzer IRAC|