Quiz: Potential Energy Calculator

Enter mass, height, and gravitational acceleration to find gravitational potential energy (PE = m × g × h), plus the equivalent impact velocity and energy in foot-pounds and kilocalories.

Quick Facts

Formula
PE = m × g × h
Mass times gravitational acceleration times height above a reference level.
Standard gravity
g = 9.80665 m/s²
Earth's standard value at sea level; often rounded to 9.81 m/s².
Other worlds
Moon 1.62 m/s² · Mars 3.71 m/s²
The same mass and height store far less potential energy off Earth.

Your Results

Calculated
Potential Energy
-
PE = m × g × h, in joules (J)
Energy in Foot-Pounds
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1 J ≈ 0.737562 ft·lb
Energy in Kilocalories
-
1 kcal = 4,184 J (food-energy comparison)
Impact Velocity
-
v = √(2gh), if dropped from rest

Ready

Enter mass, height, and gravitational acceleration, then press Calculate.

How to Calculate Gravitational Potential Energy

Gravitational potential energy (PE, sometimes written Ep or GPE) is the energy an object holds because of its position in a gravitational field, measured relative to a reference height. Lifting an object stores energy that can later convert into motion — a raised hammer, a drawn pendulum, or water held behind a dam. The formula is PE = m × g × h, where m is mass, g is gravitational acceleration, and h is height above the reference point. This calculator also derives the impact velocity the object would reach if it fell freely from that height, plus the same energy expressed in foot-pounds and kilocalories.

How the calculation works

Enter the mass and its unit, the height and its unit, and the gravitational acceleration (default 9.80665 m/s², Earth's standard gravity at sea level). The calculator converts mass to kilograms and height to meters, then multiplies m × g × h to get energy in joules. It converts that figure to foot-pounds (× 0.737562) and kilocalories (÷ 4,184) for comparison, and — using conservation of energy, m × g × h = ½ × m × v² — solves for the velocity the object would reach after falling that height from rest: v = √(2 × g × h).

Common mistakes

  • Forgetting the reference point: PE is always relative — raising an object from a 2 m ledge to 5 m above the ground only adds energy for the 3 m difference, not the full 5 m, unless the ground is your zero point.
  • Mixing units: keep mass and height in one consistent system before comparing results — convert pounds to kilograms or feet to meters rather than mixing them in the formula.
  • Assuming Earth gravity everywhere: the Moon's gravity (about 1.62 m/s²) and Mars's (about 3.71 m/s²) are far lower than Earth's, so the same mass and height store much less potential energy off-world.
  • Confusing potential with kinetic energy: PE describes stored energy from position; kinetic energy (½mv²) describes energy of motion. They are equal only when energy converts fully between the two, as in idealized free fall.

Real-world applications

  • Hydroelectric dams convert the gravitational potential energy of stored water into electricity as it falls through turbines.
  • Roller coasters store potential energy at the top of the first hill and convert it into kinetic energy — speed — on the way down.
  • Pile drivers and drop hammers use a raised weight's potential energy to drive stakes or forge metal on impact.
  • Pendulum clocks and weight-driven elevators release stored potential energy slowly and steadily over time.

Frequently Asked Questions

What is the formula for gravitational potential energy?
Gravitational potential energy is PE = m × g × h, where m is mass in kilograms, g is gravitational acceleration in m/s² (9.80665 m/s² at Earth's surface), and h is height in meters above a reference level. The result is in joules (J).
What value of g should I use for gravitational acceleration?
Use standard gravity, g = 9.80665 m/s² (often rounded to 9.81 m/s²), for calculations at or near Earth's sea level. Local gravity varies slightly with altitude and latitude (roughly 9.78-9.83 m/s²), and other bodies differ significantly — the Moon is about 1.62 m/s² and Mars is about 3.71 m/s².
Does it matter what height I measure from?
Yes and no — potential energy is always relative to a chosen reference level (often the ground or the lowest point in a system). Only the change in height between two points determines how much energy is available, so pick a consistent reference and enter the height above that point.
How do I find the velocity of a falling object from its potential energy?
By conservation of energy, gravitational potential energy converts to kinetic energy during free fall (ignoring air resistance): m × g × h = ½ × m × v². Solving for velocity gives v = √(2 × g × h), which this calculator reports directly as the impact velocity.