No problem! Here’s the information about the Schwarzschild Radius and Black Holes ⚫📏 🔹 What is the Schwarzschild Radius? • The Schwarzschild radius defines the size of the event horizon of a black hole, the boundary beyond which nothing, not even light, can escape. It is named after the physicist Karl Schwarzschild, who first derived it in 1916 🔭 • The Schwarzschild radius R_s is calculated by the formula: R_s = 2GM/c² where: - G is the gravitational constant, - M is the mass of the object, -

The Schwarzschild radius (sometimes referred to as the gravitational radius), is the radius of a sphere that has certain properties: if all the mass of an object is compressed within this sphere, the escape speed from the surface of the sphere would equal the speed of light. An example of an object smaller than its Schwarzschild radius is a black hole. Once a stellar remnant collapses below this radius, light can no longer escape and the object is no longer visible. It is a characteristic radius