Schwarzschild Radius,   also called gravitational radius, distance that defines the size at which a spherical   astronomical object such as a star becomes a black hole. A black hole is an object so   dense that not even light can escape the pull of its gravitational force (seeGravitation).   If an object collapses to within its Schwarzschild radius, it becomes a black hole. The   radius is named after German astronomer Karl Schwarzschild, who derived the first model of   a black hole in 1916.
Nothing, not even a particle moving at the speed of light, can escape the   gravitational pull of a black hole. Therefore, the Schwarzschild radius is the largest   radius that a body with a specific mass can have and still keep light from escaping. The   formula for the Schwarzschild radius of a body is Rs = GM/c2, where Rs is the Schwarzschild radius of the body, G is   a constant known as the universal constant of gravitation, M is the mass of the object,   and c is the speed of light.
To find the equation for the Schwarzschild radius of an object,   Schwarzschild needed to know how massive a body has to be to keep light from escaping and   how light behaves in such a strong gravitational field. French astronomer Pierre Laplace   found the equation for escape velocity, or the speed an object needs to overcome the   gravitational force of a body. Laplace noted in 1800 that the escape velocity would be   greater than the speed of light for an object leaving a very small, dense body. German   American physicist Albert Einstein explained how light behaves in a strong gravitational   field in his general theory of relativity, published in 1916. In 1916 Karl Schwarzschild   derived the first model of a black hole with help from the work of Laplace and Einstein.
The Schwarzschild radius of a black hole marks its event horizon,   or the boundary past which light can enter but not escape. Astronomers believe that once   an object collapses to within its Schwarzschild radius, it continues collapsing until it   becomes a singularity, or a point with infinite density and a radius of zero.
The sun has a mass of 2×1030 kg (4×1030 lb) and a radius of about 700,000 km (about 400,000 mi). Its Schwarzschild   radius is about 3 km (about 2 mi). If the sun were to collapse into a sphere with a radius   of less than 3 km, light from the sun would be trapped and the sun would become a black   hole. The sun, however, is not massive enough for it to collapse to this size and become a   black hole (see Star: Evolution of Stars).
An object with a mass equal to that of the earth would have a   Schwarzschild radius of about 3 mm (about 0.1 in). For an object with Mount Everest’s   mass, the Schwarzschild radius is only about 1×10-11 mm (4×10-13 in). Some astronomers believe that any black hole smaller than this would   be relatively unstable and would evaporate quickly, releasing gamma rays (see X   Ray). Astronomers have speculated that the mysterious sources of celestial gamma ray   bursts may be evaporating primordial black holes.
 
 
