
Putting together decades worth of observations, astronomers have shown that S2's orbit isn't a fixed-in-position ellipse; rather, the orbit shifts around like a spirograph drawing - a phenomenon known as Schwarzschild precession.
This is the first time Schwarzschild precession has been detected around a supermassive black hole, demonstrating that it holds true even when we observe the orbits of stars in the most gravitationally extreme environment.
In addition, general relativity equations can be used to accurately predict the orbital changes - and these calculations have precisely matched up with the observations of S2.












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