The brightness of galaxy centers is attributed to the presence of supermassive black holes, which do not consume all emitted light due to their small event horizons relative to the galaxy's size. The galactic center is not visible from Earth primarily because of dust obstructing visible light, but infrared and microwave observations can penetrate this dust. These observations reveal the dynamics of stars orbiting the black hole, providing evidence of its existence. Light emitted from stars outside the event horizon can still reach observers, as it travels in all directions. Upcoming astronomical events, such as a gas cloud spiraling towards the black hole, are anticipated to enhance visibility and understanding of these phenomena.