Physics
Level 1/Gravitation

4. Gravitational Potential

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Definitions

Gravitational Potential

  • The energy an object posses due to its position in a gravitational field
  • Gravitational potential energy per mass at a that point
  • Work done per unit mass in bringing a mass from infinity to a defined point
  • Always negative

Derivations

The area under the graph g-r gives you the change in gravitational potential

Area Under g-r

Work Done

Since gravitational potential equals work done per unit mass W=FrW = Fr

U(r)=FrmU(r) = - \dfrac{Fr}{m}

subbing in F=GMmr2F = \dfrac{GMm}{r^2}

U(r)=GMr(Jkg1)U(r) = - \dfrac{GM}{r} \quad \quad (\text{Jkg}^{-1})

Integration Method

Since the change in gravitational potential is the area under the graph g-r

g=GMr2g = -\dfrac{GM}{r^2}

integrating

U(r)=rGMr2  drU(r) = \int_{r}^{\infty} -\dfrac{GM}{r^2} \; dr

this results in

U(r)=[GMr]rU(r) = [\dfrac{GM}{r}]_{r}^{\infty}

which looks like

U(r)=GMGMrU(r) = \dfrac{GM}{\infty} - \dfrac{GM}{r}

which simplifies to

U(r)=GMr(Jkg1)U(r) = -\dfrac{GM}{r} \quad \quad (\text{Jkg}^{-1})

Gradient of U-r

Furthermore if you calculate the gradient of U-r you get gg

Gradient U-r

Useful Equations

U(r)=GMrU(r) = -\dfrac{GM}{r}