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Supermassive Black Hole Sgr A*

This Chandra image of the supermassive black hole at our Galaxy's center, a.k.a. Sagittarius A* or Sgr A*, was made from the longest X-ray exposure of that region to date. (Sgr A* is at the very center of the image. The galaxtic plane is along a line from upper left to lower right.) In addition to Sgr A* more than two thousand other X-ray sources were detected in the region, making this one of the richest fields ever observed. Estimates suggest that the mass of Sgr A* is about 3 million times the mass of the Sun.

During the two-week observation period, Sgr A* flared up in X-ray intensity half a dozen or more times. The rapidity with which they rise and fall indicates that they are occurring near the event horizon, or point of no return, around the black hole. These oubursts are therefore believed to be the result of matter occasionally falling into the black hole. Even during the flares the intensity of the X-ray emission from the vicinity of the black hole is relatively weak. This suggests that Sgr A* is a starved black hole, possibly because explosive events in the past have cleared much of the gas from around it.

Evidence for such explosions was revealed in the image—huge lobes of 20 million-degree Centigrade gas (the red loops in the image at approximately the 2 o'clock and 7 o'clock positions) that extend over dozens of light years on either side of the black hole. They indicate that enormous explosions occurred several times over the last ten thousand years.

Further analysis of the Sgr A* image is expected to give astronomers a much better understanding of how the supermassive black hole in the center of our galaxy grows and how it interacts with its environment. This knowledge will also help to understand the origin and evolution of even larger supermassive black holes found in the centers of other galaxies.

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