Haunting patterns within planetary nebula NGC 6543 [ http://nineplanets. ] readily suggest its popular moniker -- the Cat's Eye nebula. In 1995, a stunning false-color optical image from the Hubble Space Telescope [ http://oposite.stsc ] detailed the swirls of this glowing nebula [ http://www.seds.org ], known to be the gaseous shroud expelled from a dying sun-like star [ http://observe.ivv. stellardeath_opening .html ] about 3,000 light-years from Earth. This composite picture combines the famous Hubble image with new x-ray data [ http://chandra.harv history.html ] from the orbiting Chandra Observatory [ http://chandra.harv ] and reveals surprisingly intense x-ray emission indicating the presence of extremely hot gas. X-ray emission is shown as blue-purple hues superimposed on red and green optical emission. The nebula's central star itself is clearly immersed in the multimillion degree, x-ray emitting gas. Other pockets of x-ray hot gas seem to be bordered by cooler gas emitting strongly at optical wavelengths, a clear indication that expanding hot gas is sculpting the visible Cat's Eye [ http://antwrp.gsfc. ] filaments and structures. Gazing into the Cat's Eye, astronomers see the fate of our sun [ http://www.astro.wa ], destined to enter its own planetary nebula phase [ http://ad.usno.navy ] of evolution ... in about 5 billion years [ http://chandra.harv ].