Gravitational Fields: Question 3

Syllabus 13.4

Structured A2 10 marks

A space agency probe is exploring the region around the exoplanet Virellon, which has mass 4.20×1025 kg4.20\times10^{25}\text{ kg}. Virellon may be treated as a uniform sphere, so its mass acts as a point mass at its centre.

Take G=6.67×1011 N m2 kg2G = 6.67\times10^{-11}\text{ N m}^2\text{ kg}^{-2}.

(a) Define gravitational potential at a point, and explain why the gravitational potential due to Virellon is negative at every point a finite distance from it. [3]

(b) Calculate the gravitational potential at a point 8.00×106 m8.00\times10^6\text{ m} from the centre of Virellon. [2]

(c) The probe, of mass 250 kg250\text{ kg}, moves from the point in (b) out to a point 1.60×107 m1.60\times10^7\text{ m} from the centre of Virellon. Calculate the change in the gravitational potential energy of the probe, stating whether this is an increase or a decrease. [3]

(d) State one similarity and one difference between the shape of the graph of gravitational field strength gg against distance rr from the centre of Virellon, and the shape of the graph of gravitational potential ϕ\phi against distance rr, for points outside Virellon. [2]

Show worked solution Hide worked solution

Worked solution

Part (a): Defining gravitational potential and explaining its sign

Definition: the gravitational potential at a point is the work done per unit mass in bringing a small test mass from infinity to that point.

Why it is negative: gravitational forces are always attractive. To move a test mass away from Virellon, out towards infinity, an external agent must do positive work against this attraction. Equivalently, if the test mass instead moves inward, from infinity to a point near Virellon, the gravitational force itself does positive work on it, so the work that would need to be done by an external agent to achieve this same inward motion (quasi-statically, without gaining kinetic energy) is negative. Since gravitational potential is defined as the work done per unit mass bringing the mass in from infinity, and infinity is taken as the zero of potential, the potential at every finite distance from Virellon is therefore negative.

Part (b): Gravitational potential at 8.00×106 m8.00\times10^6\text{ m}

For a point mass, ϕ=GM/r\phi = -GM/r. With M=4.20×1025 kgM=4.20\times10^{25}\text{ kg} and r=8.00×106 mr=8.00\times10^6\text{ m}: ϕ=GMr=(6.67×1011)(4.20×1025)8.00×106\phi = -\frac{GM}{r} = -\frac{(6.67\times10^{-11})(4.20\times10^{25})}{8.00\times10^6}

Numerator: 6.67×4.20=28.0146.67\times4.20=28.014, and 1011×1025=101410^{-11}\times10^{25}=10^{14}, so the numerator is 2.8014×10152.8014\times10^{15}.

ϕ=2.8014×10158.00×106=3.50175×108 J kg13.50×108 J kg1\phi = -\frac{2.8014\times10^{15}}{8.00\times10^6} = -3.50175\times10^8\text{ J kg}^{-1} \approx -3.50\times10^8\text{ J kg}^{-1}

Check by recomputing differently: 2.8014/8.00=0.350182.8014/8.00=0.35018, and 1015/106=10910^{15}/10^{6}=10^{9}, so ϕ=0.35018×109=3.5018×108 J kg1\phi=-0.35018\times10^{9}=-3.5018\times10^8\text{ J kg}^{-1}. Both routes agree.

Part (c): Change in gravitational potential energy

The gravitational potential energy of the probe at a point is Ep=mϕE_p=m\phi.

At r1=8.00×106 mr_1=8.00\times10^6\text{ m}, using ϕ1=3.50175×108 J kg1\phi_1=-3.50175\times10^8\text{ J kg}^{-1} from (b): Ep1=mϕ1=250×(3.50175×108)=8.754×1010 JE_{p1} = m\phi_1 = 250\times(-3.50175\times10^8) = -8.754\times10^{10}\text{ J}

At r2=1.60×107 mr_2=1.60\times10^7\text{ m} (exactly twice r1r_1), since ϕ1/r\phi\propto1/r, the potential is halved: ϕ2=ϕ12=1.75088×108 J kg1\phi_2 = \frac{\phi_1}{2} = -1.75088\times10^8\text{ J kg}^{-1}

Check by recalculating directly: ϕ2=GM/r2=2.8014×1015/(1.60×107)=1.75088×108 J kg1\phi_2=-GM/r_2=-2.8014\times10^{15}/(1.60\times10^7)=-1.75088\times10^8\text{ J kg}^{-1}, matching the halved value exactly.

Ep2=mϕ2=250×(1.75088×108)=4.377×1010 JE_{p2} = m\phi_2 = 250\times(-1.75088\times10^8) = -4.377\times10^{10}\text{ J}

The change in potential energy is: ΔEp=Ep2Ep1=(4.377×1010)(8.754×1010)=+4.377×1010 J+4.38×1010 J\Delta E_p = E_{p2}-E_{p1} = (-4.377\times10^{10})-(-8.754\times10^{10}) = +4.377\times10^{10}\text{ J} \approx +4.38\times10^{10}\text{ J}

Check using the shortcut formula ΔEp=GMm(1r11r2)\Delta E_p = GMm\left(\dfrac{1}{r_1}-\dfrac{1}{r_2}\right): since r2=2r1r_2=2r_1, this is GMm(1r112r1)=GMm2r1=2.8014×1015×2502×8.00×106=7.0035×10171.60×107=4.377×1010 JGMm\left(\dfrac{1}{r_1}-\dfrac{1}{2r_1}\right)=\dfrac{GMm}{2r_1}=\dfrac{2.8014\times10^{15}\times250}{2\times8.00\times10^6}=\dfrac{7.0035\times10^{17}}{1.60\times10^7}=4.377\times10^{10}\text{ J}. This matches, confirming ΔEp+4.38×1010 J\Delta E_p\approx+4.38\times10^{10}\text{ J}.

Since ΔEp\Delta E_p is positive, the potential energy increases as the probe moves away from Virellon. Consistent with gravitational potential energy always increasing as distance from an attracting mass increases.

Part (d): Comparing the shapes of the ggrr and ϕ\phirr graphs

Similarity: for both quantities, the magnitude decreases continuously as rr increases, and both tend towards zero as rr\to\infty (neither graph ever reaches zero at a finite rr).

Difference: the field strength g=GM/r2g=GM/r^2 is always positive and falls off very steeply, as 1/r21/r^2, so it drops rapidly towards zero at large rr. The potential ϕ=GM/r\phi=-GM/r is always negative and falls off much more gradually, as 1/r1/r (i.e. its magnitude decreases more slowly than that of gg), rising smoothly from large negative values towards zero as rr increases.

Final answers

  • (a) Gravitational potential is the work done per unit mass bringing a test mass from infinity to the point; it is negative because gravity is attractive, so bringing a mass in from infinity involves negative work by an external agent (equivalently, the field itself does positive work pulling the mass in).
  • (b) ϕ=3.50×108 J kg1\phi = \boxed{-3.50\times10^8}\text{ J kg}^{-1}
  • (c) ΔEp=+4.38×1010 J\Delta E_p = \boxed{+4.38\times10^{10}}\text{ J}, an increase
  • (d) Both magnitudes fall towards zero as rr\to\infty; but gg is always positive and falls off as 1/r21/r^2 (steeply), while ϕ\phi is always negative and falls off as 1/r1/r (more gradually).