chandra_168 September 5th, 2001
Credit: NASA/MIT/F.Baganoff et al.
During a Chandra observation of the X-ray source located at the galactic center, the source was observed to brighten dramatically in a few minutes. After about 3 hours, the source declined rapidly to its pre-flare level. This is the most compelling evidence yet that matter falling toward the supermassive black hole at the center of our galaxy is fueling energetic activity. The amount of material needed to produce the energy released in the flare would have had the mass of a comet.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2001/0204flare/
Curator: Chandra X-ray Observatory, Cambridge, MA, USA
Image Use Policy: http://chandra.harvard.edu/photo/image_use.html
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