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More Images of G299.2-2.9
Click for large jpg X-ray
Jpeg, Tif
Click for large jpg Infrared
Jpeg, Tif
Click for large jpg B 1.4-3.0keV
Jpeg, Tif
Click for large jpg G 0.72-1.4keV
Jpeg, Tif
Click for large jpg R 0.4-0.72keV
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X-ray & Infrared Images of G299.2-2.9
This debris field, which glows brightly in X-rays, was left over when a star exploded about 4,500 years ago. This object, known as G299.2-2.9, belongs to a particular class of supernovas called Type Ia. Astronomers think that a Type Ia supernova involves a thermonuclear explosion - involving the fusion of elements and release of vast amounts of energy - of a white dwarf star in a tight orbit with a companion star. In the Chandra image, red, green, and blue represent low, medium, and high-energy X-rays, respectively, detected by the telescope. Infrared data show the stars in the Chandra field of view.
(Credit: X-ray: NASA/CXC/U.Texas/S.Post et al, Infrared: 2MASS/UMass/IPAC-Caltech/NASA/NSF)

Return to G299.2-2.9 (February 12, 2015)