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Gravitational Potential Energy (Orbital)

Calculate gravitational PE between two masses at distance r.

Reviewed for accuracy by the Math Ora X team Last updated

Result

Understanding Gravitational Potential Energy (Orbital)

Gravitational PE between two masses is always negative (bound system). It approaches zero as the distance increases to infinity.

$$U = -\frac{GMm}{r}$$

How to use this calculator

  1. Enter the two masses, such as a planet and a satellite.
  2. Enter the distance between their centers in meters.
  3. Check that the units are in kilograms and meters so the result is in joules.
  4. Click calculate to find the gravitational potential energy using the formula \(U = -\frac{GMm}{r}\).

The formula explained

The formula \(U = -\frac{GMm}{r}\) computes the gravitational potential energy between two masses separated by distance \(r\). The negative sign means the energy is lower when the masses are closer together.

  • U = gravitational potential energy, in joules
  • G = gravitational constant, about \(6.674 \times 10^{-11}\) \(\text{N} \cdot \text{m}^2/\text{kg}^2\)
  • M = first mass, in kilograms
  • m = second mass, in kilograms
  • r = distance between the centers of the two masses, in meters

Step by step method

  1. Write down the values of \(G\), \(M\), \(m\), and \(r\).
  2. Multiply \(G\), \(M\), and \(m\).
  3. Divide the result by \(r\), then apply the negative sign to get \(U\).

Worked example

Problem. Find the gravitational potential energy between Earth, with mass \(5.97 \times 10^{24}\) kg, and a \(1000\) kg satellite that is \(7.00 \times 10^{6}\) m from Earth's center.

  1. Use \(U = -\frac{GMm}{r}\).
  2. Substitute the values, \(U = -\frac{(6.674 \times 10^{-11})(5.97 \times 10^{24})(1000)}{7.00 \times 10^{6}}\).
  3. Compute the result, \(U \approx -5.70 \times 10^{10}\) J.

Answer. \(U \approx -5.70 \times 10^{10}\) J

Tips and common mistakes

  • Make sure \(r\) is the distance between the centers of the two masses, not the height above the surface.
  • Keep masses in kilograms and distance in meters, because unit mistakes can change the answer a lot.

Frequently asked questions

How do I use the gravitational potential energy orbital calculator?+

Enter the two masses and the distance between their centers, then the tool applies U = -GMm/r. Use consistent units, such as kilograms for mass and meters for distance, so the result comes out in joules.

What does the negative sign in U = -GMm/r mean?+

It means the gravitational potential energy is defined to be lower, and usually negative, when the masses are closer together. You would need to add energy to separate the objects to a very large distance, where the potential energy approaches zero.

What distance should I use in the formula?+

Use the center to center distance r, not the distance between the surfaces. For example, for a planet and a satellite, r is measured from the planet’s center to the satellite’s center.

What happens if one mass or the distance is zero?+

If either mass is zero, the gravitational potential energy is zero. If the distance is zero, the formula is undefined because dividing by zero is not allowed, and in real situations two extended objects cannot occupy the same point.

How is orbital gravitational potential energy different from gravitational potential energy near Earth’s surface?+

This formula gives the exact interaction energy between any two masses, while the near surface version mgh is an approximation for small height changes close to Earth. Use U = -GMm/r when the distance to the center matters, such as satellites, planets, or moons.

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