Gravitational potential energy
Is defined by the integral:
U(r) = -
Where is the force due to gravity and we define U(∞) = 0. Doing the integral gives:
U(r) = -
which reduces to U = mgh near the earth.
Is defined as the gravitational potential energy that a 1 kilogram mass would have at some point in space. It is given by:
Φg = -
which reduces to Φg = gh near the earth.
Principle of Equivalence
Asserts that all types of matter fall at the same rate. That is, g for a brick is the same as g for water. This means that the inertial mass appearing in Newton's Second Law is equivalent to the gravitational mass appearing in the Universal Law of Gravitation.
The mass mi that appears in Newton's Second LawF = mia.
The mass that appears in the Universal Law of Gravitation.
States that any spherical mass can be treated as though all its mass were concentrated at its center for the purposes of calculating gravitational force. Also, that a spherical shell of matter exerts no gravitational force on a mass inside it.
|Energy for a circular orbit around the sun||