This image of supernova remnant 0509-67.5 was made by combining data from two of NASA's Great Observatories. Optical data of SNR 0509-67.5 and its accompanying star field, taken with the Hubble Space Telescope, are composited with X-ray images from the Chandra X-ray Observatory.
Located approximately 300 million light-years away in the constellation of Volans, AM 0644-741 is one of the most spectacular ‘Ring Galaxies’ currently know. - Image Credit: NASA, ESA, and The Hubble Heritage Team (AURA/STScI)
This true colour image of the giant planet Jupiter, by NASA and ESA's Hubble Space Telescope, reveals the impact sites of fragments 'D' and 'G' from Comet Shoemaker-Levy 9. Credit: H. Hammel, MIT and NASA/ESA
Supernova N49: This is a composite image of N49, the brightest supernova remnant in optical light in the Large Magellanic Cloud. The Chandra X-ray image (blue) shows million-degree gas in the center. Much cooler gas at the outer parts of the remnant is seen in the infrared image from Spitzer (red). Taken on June 15, 2006.
Chandra X-Ray Observatory (NASA, Marshall, Archive, 7/23/99)- NASA's Marshall Space Flight Center Named in honor of the late Indian-American Astronomer, Subrahmanyan Chandrasekhar, launched on July 23, 1999 aboard the Space Shuttle Columbia (STS-93 mission), the Chandra X-ray Observatory uses its four highly sensitive mirrors to focus x-rays from celestial objects to explore black holes, clusters of galaxies, and exploded stars.