Gravitational Potential Energy — Core Principles
Core Principles
Gravitational potential energy (GPE) is the energy an object possesses due to its position in a gravitational field. It's a scalar quantity and a form of stored energy. For objects near Earth's surface, GPE is approximated as , where is the height above a chosen reference level (often the ground, where ).
This formula assumes constant acceleration due to gravity, . For objects at larger distances, or in general, the GPE of a system of two masses and separated by a distance is given by .
In this general formula, the reference point for zero potential energy is taken at infinity. The negative sign indicates that gravity is an attractive force and the system is bound. Work done against gravity increases GPE, while work done by gravity decreases GPE.
The principle of conservation of mechanical energy () is fundamental when dealing with GPE in the absence of non-conservative forces.
Important Differences
vs Gravitational Potential
| Aspect | This Topic | Gravitational Potential |
|---|---|---|
| Definition | Gravitational Potential Energy ($U$) is the energy possessed by a mass due to its position in a gravitational field. | Gravitational Potential ($V$) is the potential energy per unit mass at a point in a gravitational field. |
| Formula | $U = -rac{GMm}{r}$ (general) or $U = mgh$ (near surface) | $V = -rac{GM}{r}$ (general) or $V = gh$ (near surface) |
| Units | Joules (J) | Joules per kilogram (J/kg) |
| Dependence | Depends on both the source mass ($M$) and the test mass ($m$). | Depends only on the source mass ($M$) and the position, not on the test mass. |
| Nature | Represents the energy of a system of two or more masses. | Represents a characteristic of the gravitational field at a point. |