FTP, identify this quantity that determines the radius an object would need to be compressed to in order to become a black hole.
Its derivation owes to the formulation of the escape velocity by Laplace and the behavior of light in a strong gravitational field by Einstein. It was first published in 1916 and gave the Sun's value at approximately 3 kilometers, along with the first model of a black hole. It is solved for various bodies by multiplying the universal gravitational constant by the mass of the object and dividing by the speed of light squared. FTP, identify this quantity that determines the radius an object would need to be compressed to in order to become a black hole.
Its derivation owes to the formulation of the escape velocity by Laplace and the behavior of light in a strong gravitational field by Einstein.
{Schwarzchild} radius