S62 (star)

S62, in the context of astronomy, typically refers to a star located at the center of our galaxy, the Milky Way, orbiting the supermassive black hole Sagittarius A* (Sgr A*). S62 is known for its extremely short orbital period and high velocity as it approaches Sgr A*. Its close proximity and rapid movement make it a valuable object for testing theories of general relativity and understanding the properties of black holes. Observations of S62 and similar stars provide crucial data for determining the mass and spin of Sagittarius A*, as well as probing the spacetime environment near the black hole's event horizon. The star's orbital parameters, such as its period and eccentricity, are derived from long-term observations using telescopes and sophisticated data analysis techniques. These parameters help scientists refine models of the gravitational field surrounding Sgr A* and test the predictions of Einstein's theory in an extreme environment. The study of S62 and other S-stars contributes significantly to our understanding of black hole dynamics, galactic center environments, and fundamental physics.