Artistic Imagination of super-massive black hole in the center of The Milky Way |
Before you say "no," what if every star is simply orbiting every other star simultaneously around a shared barycenter in place of the SMBH (like a binary star system but with trillions)? If that is the case, then Kepler's laws wouldn't apply because they rely on a central mass controlling the system and there could be no galactic rotation anomaly. Also, are there any equations pertaining to orbit in a system with no centrally-dominating mass?In the 90's, people had doubts about what would he residing at the center of the Galaxy (which is called as Sgr A*). Could it be a massive black hole, or is it a cluster of highly dense stars, or is it something else?
This problem was solved in 2002 when my former colleague Rainer Schoedel published observations of a star S2 which is the nearest star to Sgr A*. S2 is a star with the smallest orbiting period around Sgr A* and after observing it for more than 10 years, they were able to fit very accurate orbits. [See images]
Fitted orbits of two close stars near Sgr A* S2 and S102 |
Near Infrared image of the two stars and Sgr A* |
From these observations, the mass and size of Sgr A* was deduced, which was 2.6×106M⊙ confined within a region as small as 120 AU. Further observations of star S14 improved these numbers to 4.1×106M⊙ and 45 AU.
Orbits of stars around Sgr A* |
Author: Abhijeet Borkar
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