Potential Energy Calculator

Potential energy is the energy stored in an object due to its position or configuration. Gravitational potential energy (PE = mgh) depends on mass, gravitational acceleration, and height above a reference point. A 10 kg object held 5 m above the ground on Earth stores 490.5 J of potential energy. When released, this PE converts to kinetic energy, reaching v = √(2gh) = 9.9 m/s at ground level. Elastic potential energy (PE = ½kx²) is the energy stored in a compressed or stretched spring, where k is the spring constant and x is displacement from equilibrium. This calculator solves both formulas in any direction, compares PE across different planets, and shows the equivalent velocity if all PE were converted to kinetic energy.

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Potential Energy Calculator calculator

tips_and_updates Tips

  • PE = mgh only works near a planet's surface where g is approximately constant. For orbital distances, use PE = -GMm/r.
  • On the Moon (g = 1.62 m/s²), objects store ~16.5% of the gravitational PE they would on Earth at the same height.
  • Elastic PE is always positive regardless of whether the spring is compressed or stretched — energy depends on x².
  • The PE-to-KE velocity equivalence assumes zero friction. Real-world values are lower due to air resistance and other losses.
  • 1 joule = 1 kg·m²/s² = 0.7376 ft·lb. A 1 kg object at 1 m on Earth has PE = 9.81 J.

How to Use the Potential Energy Calculator

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Choose Energy Type

Select Gravitational PE (mgh) for objects at a height, or Elastic PE (½kx²) for springs and elastic materials.

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Pick What to Solve For

Choose to solve for PE, mass, height, gravity (gravitational mode) or PE, spring constant, displacement (elastic mode).

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Enter Values and Review

Input known values with units. Results show PE in multiple units, planet comparisons, and the equivalent free-fall velocity.

The Formula

Gravitational PE is proportional to mass, gravity, and height. Doubling the height doubles the stored energy. On the Moon (g = 1.62 m/s²), the same object at the same height stores about 1/6 the energy compared to Earth. Elastic PE depends on the square of displacement — compressing a spring twice as far stores four times the energy. The PE-to-KE equivalence shows what velocity a falling object would reach if all potential energy converted to kinetic energy with no losses.

PE = m × g × h | PE = ½ × k × x² | v = √(2 × PE / m)

lightbulb Variables Explained

  • PE Potential energy in joules (J)
  • m Mass in kilograms (kg)
  • g Gravitational acceleration in m/s² (Earth = 9.81)
  • h Height in metres (m)
  • k Spring constant in N/m
  • x Displacement from equilibrium in metres (m)
  • v Equivalent velocity in m/s (PE→KE conversion)

tips_and_updates Pro Tips

1

PE = mgh only works near a planet's surface where g is approximately constant. For orbital distances, use PE = -GMm/r.

2

On the Moon (g = 1.62 m/s²), objects store ~16.5% of the gravitational PE they would on Earth at the same height.

3

Elastic PE is always positive regardless of whether the spring is compressed or stretched — energy depends on x².

4

The PE-to-KE velocity equivalence assumes zero friction. Real-world values are lower due to air resistance and other losses.

5

1 joule = 1 kg·m²/s² = 0.7376 ft·lb. A 1 kg object at 1 m on Earth has PE = 9.81 J.

Potential energy is stored energy based on an object's position or configuration — gravitational potential energy (PE = mgh) depends on height above a reference point, elastic potential energy (PE = ½kx²) depends on spring compression or extension, and electric potential energy depends on charge separation. These forms of stored energy convert to kinetic energy when released: a 70 kg person standing on a 10-meter diving platform has PE = 70 × 9.81 × 10 = 6,867 joules of gravitational potential energy, which converts entirely to kinetic energy (and ultimately to thermal energy and sound) upon hitting the water. Our potential energy calculator computes gravitational PE from mass, height, and gravitational acceleration, elastic PE from spring constant and displacement, and electric PE from charges and distance. It handles unit conversions between joules, calories, electron-volts, and foot-pounds, making it useful for physics problems, engineering design, and energy analysis.

Gravitational potential energy

Gravitational PE = mgh, where m is mass (kg), g is gravitational acceleration (9.81 m/s² on Earth), and h is height above the reference point (meters). The reference point is arbitrary — what matters is the change in height.

A 1,000 kg car at the top of a 50-meter hill has PE = 1,000 × 9.81 × 50 = 490,500 J (490.5 kJ) relative to the bottom. This energy converts to kinetic energy as the car descends — at the bottom (assuming no friction), it reaches v = √(2gh) = √(2 × 9.81 × 50) = 31.3 m/s (70 mph).

Hydroelectric dams exploit this principle: water falling through a height (head) drives turbines. The Hoover Dam's 180-meter head generates enormous energy per cubic meter of water: PE = 1,000 × 9.81 × 180 = 1,765,800 J per m³.

Elastic potential energy in springs

Elastic PE = ½kx², where k is the spring constant (N/m or lb/in) and x is the displacement from equilibrium. This relationship is quadratic — doubling the compression quadruples the stored energy.

A spring with k = 500 N/m compressed 0.1 m stores PE = ½ × 500 × 0.01 = 2.5 J. A car suspension spring (k ≈ 25,000 N/m) compressed 5 cm by hitting a bump stores PE = ½ × 25,000 × 0.0025 = 31.25 J per spring. Bows and crossbows store elastic PE — a compound bow with k ≈ 2,500 N/m at 0.7m draw stores approximately 612 J, enough to launch an arrow at 90+ m/s.

The spring constant determines the force-displacement relationship: F = kx (Hooke's law) — a stiffer spring requires more force to compress but stores more energy per unit displacement.

Conservation of energy and practical applications

The conservation of energy principle states that total energy (kinetic + potential) remains constant in an isolated system (ignoring friction and air resistance). At the top of a roller coaster hill, energy is mostly potential; at the bottom, it is mostly kinetic.

This principle enables simple calculations: a ball dropped from 5 meters reaches v = √(2 × 9.81 × 5) = 9.9 m/s at ground level regardless of mass. With friction, some energy converts to heat — a real roller coaster at the bottom of a 30-meter drop reaches approximately 85-90% of the theoretical speed due to friction and air resistance losses.

In engineering, potential energy analysis is critical for:

  • sizing pumps (must overcome gravitational PE of water being lifted)
  • designing safety systems (energy absorbed by crash barriers)
  • energy storage (pumped hydro stores energy as gravitational PE by pumping water uphill during low-demand periods)

How to Calculate Gravitational Potential Energy (PE = mgh)

To calculate gravitational potential energy, multiply mass by gravitational acceleration by height: PE = m × g × h. Mass m is in kilograms, g is the local gravitational acceleration (9.81 m/s² near Earth's surface), and h is height in metres above your chosen reference point. The result is in joules (J).

For example, a 2 kg book placed on a 3 m shelf stores PE = 2 × 9.81 × 3 = 58.86 J relative to the floor. Because the formula is linear in each variable, doubling the height doubles the stored energy.

HyperPhysics (Georgia State University) notes that mgh is a near-surface approximation where g is treated as constant.

What Are the SI Units of Potential Energy?

The SI unit of potential energy is the joule (J), defined by BIPM as one kilogram-metre-squared per second-squared (1 J = 1 kg·m²/s²), equivalent to one newton-metre. In the PE = mgh formula the units combine as kg × (m/s²) × m = kg·m²/s² = J, which confirms the equation is dimensionally consistent. NIST maintains the joule as the coherent SI energy unit.

Common conversions include:

  • 1 J = 0.7376 ft·lb
  • 1 calorie = 4.184 J
  • 1 kilowatt-hour = 3.6 × 10⁶ J
  • 1 electron-volt = 1.602 × 10⁻¹⁹ J

Always keep mass in kilograms and length in metres so the answer emerges directly in joules without extra conversion factors.

How to Solve for Mass, Height, or Gravity from PE

Rearranging PE = mgh lets you solve for any single unknown.

  • To find height, divide energy by the product of mass and gravity: h = PE / (m × g). For instance, a 3 kg object holding 147.15 J on Earth sits at h = 147.15 / (3 × 9.81) = 5 m.
  • To find mass, use m = PE / (g × h).
  • To find local gravity, use g = PE / (m × h).

Because each variable appears to the first power, these inversions are simple division. Khan Academy recommends checking units after rearranging — the answer for height should carry metres, and for mass kilograms — to catch algebra errors before trusting the number.

How Does Potential Energy Convert to Kinetic Energy?

When an object falls freely, gravitational potential energy converts into kinetic energy while total mechanical energy stays constant. Setting the energies equal, mgh = ½mv², the mass cancels and the impact speed becomes v = √(2gh) — independent of mass.

A stone dropped from 20 m on Earth reaches v = √(2 × 9.81 × 20) = √392.4 ≈ 19.81 m/s (about 71 km/h) at the ground, ignoring air resistance.

Encyclopaedia Britannica frames this as the conservation of mechanical energy: energy is transferred between forms rather than created or destroyed. In reality, drag and friction dissipate some energy as heat and sound, so measured speeds fall slightly below the ideal value.

Gravitational Potential Energy on the Moon, Mars, and Other Planets

Gravitational potential energy scales directly with local surface gravity g, so the same mass at the same height stores different energy on each world. NIST and planetary references list g ≈ 1.62 m/s² on the Moon, 3.72 m/s² on Mars, 9.81 m/s² on Earth, and 24.79 m/s² on Jupiter.

A 5 kg object raised 10 m therefore stores:

  • 81 J on the Moon
  • 186 J on Mars
  • 490.5 J on Earth
  • 1,239.5 J on Jupiter

The Moon value is roughly 16.5% of Earth's because 1.62 / 9.81 ≈ 0.165. This is why astronauts can lift heavy loads to great heights on the Moon using far less energy, and why the same fall causes gentler impacts.

How to Calculate Elastic Potential Energy in a Spring

Elastic potential energy is calculated with PE = ½ × k × x², where k is the spring constant in newtons per metre (N/m) and x is the displacement from the equilibrium position in metres. Because energy depends on x², stretching or compressing a spring twice as far stores four times the energy.

A spring with k = 800 N/m compressed 0.05 m stores PE = ½ × 800 × (0.05)² = ½ × 800 × 0.0025 = 1.0 J. The related restoring force follows Hooke's law, F = kx, as described by HyperPhysics.

Elastic PE is always positive whether the spring is stretched or compressed, since x² is never negative — a point Khan Academy emphasises for beginners.

Real-World Applications of Potential Energy in Engineering

Potential energy analysis underpins many engineering systems:

  • Pumped-storage hydropower stores gravitational PE by pumping water uphill during low demand and releasing it through turbines at peak times — a reservoir head of 300 m gives each cubic metre PE = 1,000 × 9.81 × 300 = 2,943,000 J.
  • Roller-coaster designers use the chain-lift hill as a PE reservoir that feeds every drop and loop.
  • Spring-based systems store elastic PE in vehicle suspensions, watch mainsprings, archery bows, and mechanical clamps.
  • Crash barriers and packaging foams are engineered to absorb kinetic energy by converting it into deformation.

Britannica and IEEE resources note that battery and capacitor systems store energy electrically, complementing these mechanical potential-energy stores in modern grids.

Common Mistakes When Calculating Potential Energy

  • The most frequent error is mixing units — using grams instead of kilograms, or centimetres instead of metres — which throws the joule result off by factors of thousands. Convert to kilograms and metres before applying PE = mgh.
  • A second mistake is using g = 9.81 m/s² for non-Earth problems; the Moon and Mars need their own values.
  • For elastic PE, forgetting to square the displacement, or squaring only part of it, is common: PE = ½kx² requires x² in metres-squared.
  • Another slip is treating the reference height as fixed rather than a chosen zero point — only the change in height matters.
  • Finally, the v = √(2gh) impact speed assumes no air resistance, so real measured speeds are lower.

Frequently Asked Questions

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