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The star-system of Sagitarrius A is actually quite complex. There are six seperate stars in varying eliptical orbits around the presumed black hole core of the Milky Way. Because their orbital elipses are varied, their velocities of orbit are also varied, however there is a clear gravitational centre around which they are all revolving, and presumebly, into which they are perpetually being pulled, and one by one snuffed out to feed the black hole core. In this diagram we see the positions of these stars during the years 1995 till 2002. In 2002, we receieved our first time-lapsed photogrpahs of the Sagitarius A system, and the results were indeed a shock among the scientific community.
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