What is the formula for potential energy?

The formula for gravitational potential energy is defined as the energy stored in an object due to its position in a gravitational field. The correct expression for this energy is derived from the principle that potential energy depends on three key factors: the mass of the object, the strength of the gravitational field, and the height of the object above the reference point.

In the case of gravitational potential energy, the formula is given by mass multiplied by gravitational field strength (which is typically denoted as "g" and equals approximately 9.81 m/s² on the surface of the Earth) and height. This means that to calculate the potential energy, you need to know how heavy the object is (mass), how strong the gravitational pull is (gravitational field strength), and how high the object is located (height).

By combining these factors, the formula is expressed as:

Potential Energy (PE) = Mass (m) x Gravitational Field Strength (g) x Height (h)

The other options do not accurately represent the relationship between these factors. For example, velocity is not a factor in the calculation of potential energy, as it pertains more to kinetic energy. Similarly, acceleration and force do not directly relate to potential energy in this context. Understanding the