Credit: NASA/ESA/R. Sankrit and W. Blair (Johns Hopkins University)

Kepler's Supernova Remnant: Views from Chandra, Hubble and Spitzer

These images represent views of Kepler's supernova remnant taken in X-rays, visible light, and infrared radiation.

Each top panel shows the entire remnant. 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. Astronomers have color-coded those data so they can be seen in these images.

The bottom panels are close-up views of the remnant. In the bottom, center image, Hubble sees fine details in the brightest, densest areas of gas. The region seen in these images is outlined in the top, center panel.

The images indicate that the bubble of gas that makes up the supernova remnant appears different in various types of light. Chandra reveals the hottest gas [colored blue and colored green], which radiates in X-rays. The blue color represents the higher-energy gas; the green, the lower-energy gas. Hubble shows the brightest, densest gas [colored yellow], which appears in visible light. Spitzer unveils heated dust [colored red], which radiates in infrared light.

Individual Images

	Spitzer View Screen-Resolution (450x450): JPEG High-Resolution (1090x1090): JPEG | Mac TIFF | PC TIFF Credit: NASA/ESA/R. Sankrit and W. Blair (Johns Hopkins University)
	Hubble View Screen-Resolution (450x450): JPEG High-Resolution (1666x1666): JPEG | Mac TIFF | PC TIFF Credit: NASA/ESA/R. Sankrit and W. Blair (Johns Hopkins University)
	Chandra View Screen-Resolution (450x450): JPEG High-Resolution (2400x2400): JPEG | Mac TIFF | PC TIFF Credit: NASA/ESA/R. Sankrit and W. Blair (Johns Hopkins University)

The Spitzer Space Telescope is a NASA mission managed by the Jet Propulsion Laboratory. This website is maintained by the Spitzer Science Center, located on the campus of the California Institute of Technology and part of NASA's Infrared Processing and Analysis Center.