PhysicsGravitational fields › Gravitational potential

Gravitational potential

Gravitational potential attaches a number to every location in a field, the work per kilogram needed to arrive there from infinity. Every value comes out negative, the zero sits at infinity, and one pair of graphs converts between potential and field strength in both directions.

Builds on Newton's law of gravitation and Conservation of energy.

IN THIS TOPIC

  • Define gravitational potential with its zero at infinity, and use ΔW = mΔV.
  • Use V = −GM/r and explain the significance of the negative sign.
  • Explain why no work is done moving along an equipotential surface.
  • Connect the g and V graphs, with g the negative gradient of V and the size of ΔV the area under g against r.

COMMON MISCONCEPTION

It takes energy to move anywhere in a gravitational field.

Potential, measured from infinity

The gravitational potential V at a point is the work done per unit mass to bring a small mass from infinity to that point. The zero is at infinity, far from everything. In the radial field of a mass M,

V=-GMrV = -\frac{GM}{r}ON THE AQA DATA SHEET
The potential well: V is negative everywhere and climbs towards zero at infinityrVV = 0 at infinitydeep in the wellclimbing out means gaining potential
FIG. 1The potential well: V is negative everywhere, deepest near the mass, climbing towards zero at infinity.

The negative sign matters. Gravity attracts, so the field itself does the work as a mass arrives and nobody has to supply any energy; every location in the universe therefore sits below zero. Moving away from a mass means climbing, with V rising towards zero, and the picture to hold on to is a well. Every planet sits at the bottom of one, and leaving means climbing the full depth.

The potential difference between two points sets the energy transferred in moving between them, and for a mass m,

ΔW=mΔV\Delta W = m\Delta VON THE AQA DATA SHEET

WORKED EXAMPLE

The potential at the Earth's surface

Find the gravitational potential at the Earth's surface (M = 5.97 × 1024 kg, R = 6.37 × 106 m).

V = −GM/r = −(6.67 × 10−11 × 5.97 × 1024)/(6.37 × 106).

V = −6.3 × 107 J kg−1. Every kilogram standing here sits some sixty-three megajoules below free space.

The sign is the physics. You are in a well, and the number is the depth of your shelf; lifting anything anywhere begins by paying against it.

The free directions

Equipotential surfaces ring the planet at right angles to the field lines; moving along one costs no workequipotentials:no work along onefield lines crossat right angles
FIG. 2Equipotential surfaces ring the mass, crossed by field lines at right angles. Along an equipotential, the move is free.

Surfaces of constant potential, equipotentials, ring a mass the way contour lines ring a hill, and they always cross the field lines at right angles. Moving along an equipotential changes V by nothing, so no work is done. A satellite in a circular orbit rides one equipotential the whole way round, takes no work from gravity, and needs no engine to keep going. Only motion between equipotentials costs anything.

The graph dictionary

You need fluency with the graphs of g and V against r, and with the rules that translate between them. Field strength is the negative gradient of the potential,

g=-ΔVΔrg = -\frac{\Delta V}{\Delta r}ON THE AQA DATA SHEET

steep potential, strong field, and the minus sign aims the force downhill into the well. The dictionary reads the other way too.

The size of the potential difference between two distances is the area under the g against r graph between them, with g the magnitude of the potential gradientrgr₁r₂area = |ΔV|one graph, two jobs, in magnitudes:g = |ΔV/Δr| one way; area gives |ΔV| the other
FIG. 3The size of ΔV between two distances is the area under the g against r graph between them. The graph works in magnitudes, g = |ΔV/Δr|: gradient one way, area the other.

the size of the potential difference between two distances is the area under the g against r graph between them, the graph plotting g as a positive magnitude. Gradient in one direction, area in the other, the same pairing motion graphs taught in Year 12, now working on fields.

GUIDED PRACTICE

g, recovered from the dictionary

Near the surface, the potential changes from −6.253 × 107 to −6.185 × 107 J kg−1 over a climb of 70 km. Use the graph dictionary to recover the field strength.

Show the working

g = |ΔV/Δr| = (6.8 × 105)/(7.0 × 104) = 9.7 N kg−1, the magnitude of the potential gradient.

Just below 9.8, as it must be for an average taken over a climb above the surface where the field is weakening. The gradient of the potential curve is the field, and the dictionary between the two graphs runs both ways.

ASSESSMENT FOCUS

  • Define V with both ingredients, work done per unit mass and brought from infinity. Omit either half and the mark goes.
  • The negative sign has a stock explanation. Gravity attracts and the zero sits at infinity, so every real location lies below it. Learn that as one sentence.
  • No work is done moving along an equipotential. A circular orbit is the standard example, and “why does the satellite need no fuel to maintain its speed” is the same fact asked backwards.
  • ΔW = mΔV carries signs. Move outward and ΔV is positive, so work must be supplied; fall inward and the field does the work for you.
  • The graph dictionary earns structured marks. g is minus the gradient of V against r, and the size of ΔV is the area under g against r. Quote whichever direction the data supports.
  • Potential and potential energy are not the same quantity. V is per kilogram, in J kg−1; the potential energy of a mass m sitting at that point is mV, in joules. An answer carrying the wrong unit has usually confused the two ideas, and the arithmetic was never the problem.

CHECK YOURSELF

At the Earth's surface V = −6.25 × 107 J kg−1, and at a satellite's orbit V = −0.94 × 107 J kg−1. Find the energy needed to lift a 1200 kg satellite between the two, ignoring its kinetic energy.

Show a hint

The energy needed is m times the potential difference.

Show the answer

ΔV = (−0.94 × 107) − (−6.25 × 107) = +5.31 × 107 J kg−1. The climb runs out of the well, so ΔV comes out positive.

ΔW=mΔV\Delta W = m\Delta V = 1200 × 5.31 × 107 = 6.4 × 1010 J.

Sixty-four gigajoules simply to be there, before a single joule of orbital kinetic energy. Launch costs are mostly the depth of the well.

Potential is the work per kilogram to arrive from infinity, and it is always negative.

Gradient gives g from V; area gives ΔV from g.

WORKBOOK

Printable practice for this topic: original exam-style questions with room to work, and a fully worked answer book. Free to use; please do not redistribute or sell.

18 questions on this topicAnswer them one at a time and mark yourself against the mark scheme.Practise this topic

Or read them with their mark schemes on the gravitational potential questions page.

6 flashcards on this topicDefinitions, off-sheet equations and a spot-the-error card, scheduled by spaced repetition in your browser.Revise with flashcards

WHERE TO GO NEXT

CHECK YOUR PROGRESS

Rate how confident you feel with each objective for this lesson. Ratings are saved in this browser, on this device, unless you sign in.

  • Define gravitational potential with its zero at infinity, and use ΔW = mΔV.
  • Use V = −GM/r and explain the significance of the negative sign.
  • Explain why no work is done moving along an equipotential surface.
  • Connect the g and V graphs, with g the negative gradient of V and the size of ΔV the area under g against r.

Open the full revision checklist to track your progress across the whole unit.