Every sufficiently large amount of this quantity has an associated Schwarzschild radius.
Every sufficiently large amount of this quantity has an associated Schwarzschild radius. Kepler's third law of planetary motion assumes that this property for one body is negligible compared to this quantity for the other body. The weak equivalence principle states that the inertial and (*) gravitational forms of this property are the same. In special relativity, this quantity is equal to energy divided by the square of the speed of light. Force equals this quantity times acceleration. For 10 points, name this quantity that is measured in kilograms.
Every sufficiently large amount of this quantity has an associated Schwarzschild radius.
{mass} [do not accept "{weight}"]