Unit 7 · Topic 03

Gravitational potential energy

The reference U(∞)=0 fixes the sign and supports analysis of bound states and escape.

Unit 7Gravitational energyOpen navigation

Concept 01

Negative potential energy

Essential The minimum you should retain

With U(∞)=0, U(r)=−GMm/r is negative at finite distance.

UnderstandInterpret and connect

Separating the masses raises U toward zero; bringing them closer makes it more negative.

DeepenFormulation and conditions

The sign depends on the reference, but differences and force do not.

ExploreConnections for further study

A bound state has negative mechanical energy with this reference.

Mathematical relation

Gravitational potential energy

U=GMmr,ΔU=GMm(1ri1rf) U=-GMm/r,\quad \Delta U=GMm(1/r_i-1/r_f),\quad U(\infty)=0
Represents

Potential energy and its radial change.

Physical interpretation

U is negative at finite distance with this reference.

DeepenVariables, conditions, and checks

Variables

U
gravitational potential energy; usual unit: J

Conditions of application

  • Reference U(∞)=0; positive radii.

Dimensional check

J.

normalized gravitational potential energy

Normalized U curve versus radial distance.U→0⁻
  • U<0

With U(∞)=0, potential energy is negative and approaches zero from below.

Concept 02

Comparing two radii

Essential The minimum you should retain

ΔU=GMm(1/rᵢ−1/r_f) preserves the initial-to-final order.

UnderstandInterpret and connect

If r_f>rᵢ, ΔU>0 and ideal energy input is required.

DeepenFormulation and conditions

The radial force satisfies F_r=−dU/dr=−GMm/r².

ExploreConnections for further study

The slope, rather than the chosen zero, determines the force.

Worked example

Raising a mass from R to 2R

m=1000 kg, μ_E=3.986×10^14 m³/s², and R_E=6.371×10^6 m.

Given
  • m=1000 kg
  • r_i=R_E
  • r_f=2R_E
Target

Find ΔU.

  1. Model

    ΔU=μm(1/r_i−1/r_f).

  2. Radii

    r_i=R and r_f=2R.

  3. Simplify

    ΔU=μm/(2R).

  4. Result

    ΔU≈+3.13×10^10 J.

Conclusion

Potential energy increases by 3.13×10^10 J.

Concept 03

The local limit

Essential The minimum you should retain

Near a surface and for |Δh|≪R, ΔU≈mgΔh.

UnderstandInterpret and connect

The approximation assumes that g changes little across the region.

DeepenFormulation and conditions

Expanding 1/(R+h) to first order connects the universal expression to mgh.

ExploreConnections for further study

At planetary scales one must return to −GMm/r.

Concept 04

Consistent references

Essential The minimum you should retain

K and U must use the same reference and system.

UnderstandInterpret and connect

Changing the zero adds a common constant to U and E without altering ΔU.

DeepenFormulation and conditions

E=0 is the ideal limit reaching infinity with zero final speed.

ExploreConnections for further study

Losses or propulsion require extra terms in the simple mechanical balance.

Concept review

Common errors

Each warning includes a concrete way to review the reasoning, not only an incorrect-answer marker.

Using U=mgh at planetary scales.

Use U=−GMm/r; mgh is a local approximation.

Assigning U=+GMm/r when U(∞)=0.

That reference requires U=−GMm/r.