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The galactic center of the Milky Way Galaxy is dominated by a supermassive black hole known as Sagittarius A* (Sgr A*). This black hole, located in the constellation Sagittarius, possesses a mass equivalent to about 4.3 million Suns.12

Direct observation of the galactic center is hindered by dust, making non-visual wavelengths like radio, infrared, X-ray, and gamma-ray crucial for study. Observations of stars orbiting Sgr A* provide evidence for its existence as a black hole. The Event Horizon Telescope has even imaged the shadow of this black hole against the surrounding hot gas.21

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