
Black Holes
S301 Star Could Reveal Sagittarius A*’s Spin Within a Decade
Astronomers using the GRAVITY instrument have discovered S301, a faint star completing an exceptionally tight 8.7-year orbit around Sagittarius A*, the Milky Way’s central supermassive black hole. Its extreme eccentricity carries it to within roughly 136–142 Schwarzschild radii of the black hole, where relativistic effects become unusually strong. Continued observations could make S301 one of the first stars capable of providing a direct dynamical measurement of Sagittarius A*’s spin within about a decade.






