2021 A/L Physics Past Paper · Question 20 (English Medium)

Gravitational intensity on Jupiter

The diameter and mean density of Jupiter are 1111 times and 14\dfrac{1}{4} times respectively to that of Earth. If the gravitational intensity at the surface of Earth is 10 N kg−110\ \text{N kg}^{-1} what is the gravitational intensity at the surface of Jupiter?

  1. (1) 27.5 N kg−127.5\ \text{N kg}^{-1}
  2. (2) 44.0 N kg−144.0\ \text{N kg}^{-1}
  3. (3) 48.4 N kg−148.4\ \text{N kg}^{-1}
  4. (4) 110 N kg−1110\ \text{N kg}^{-1}
  5. (5) 440 N kg−1440\ \text{N kg}^{-1}
Answer and explanation

Answer: (1) 27.5 N kg−127.5\ \text{N kg}^{-1}

What the question asks

Find the gravitational intensity gJg_J at the surface of Jupiter.

We only need how gg changes when the size and the density change.

Relevant theory

The intensity of a gravitational field at such a point is the force acting on a unit mass placed at that point.

Hence it is seen that the acceleration due to gravity and the gravitational field intensity on the surface of Earth take the same value.

The mass of a unit volume of a substance is termed its density.

Required equations

g=GMR2g = \dfrac{GM}{R^2}

M=ρ×43πR3M = \rho \times \tfrac{4}{3}\pi R^3

g=43πGρRg = \tfrac{4}{3}\pi G \rho R

Reasoning and calculation

What stays the same: GG and 43π\tfrac{4}{3}\pi.

What changes: the density ρ\rho and the radius RR.

The diameter is 1111 times, so the radius is 1111 times too.

So the gravitational intensity is proportional to the density times the radius:

g∝ρRg \propto \rho R

Take the ratio of Jupiter to Earth:

gJgE=ρJRJρERE=14×11\dfrac{g_J}{g_E} = \dfrac{\rho_J R_J}{\rho_E R_E} = \dfrac{1}{4} \times 11

Simplify:

gJgE=114=2.75\dfrac{g_J}{g_E} = \dfrac{11}{4} = 2.75

gJ=2.75×10=27.5 N kg−1g_J = 2.75 \times 10 = 27.5\ \text{N kg}^{-1}

Reading the options

The value 27.5 N kg−127.5\ \text{N kg}^{-1} is option (1).

The options 110110 and 440440 are too big. They ignore the density, or turn it upside down.

Checks

Dimension check:

[GρR]=M−1L3T−2×ML−3×L=LT−2[G\rho R] = M^{-1}L^3T^{-2} \times ML^{-3} \times L = LT^{-2}

This is the dimension of gg (N kg−1=m s−2\text{N kg}^{-1} = \text{m s}^{-2}). It matches.

g∗d∗Dg * d * D

Does it make sense?

Jupiter is much bigger than Earth, so a bigger gg is right.

But the density is smaller, so gg is not 1111 times bigger. 2.752.75 is between 11 and 1111.

A limiting case. If the density were the same as Earth, we would get gJgE=11\dfrac{g_J}{g_E} = 11.

With a quarter of the density the factor is a quarter of that: 114\dfrac{11}{4}.

Conclusion

gJ=14×11×10=27.5 N kg−1g_J = \dfrac{1}{4} \times 11 \times 10 = 27.5\ \text{N kg}^{-1}

g∝ρRg \propto \rho R, so gJgE=14×11=2.75\dfrac{g_J}{g_E} = \dfrac{1}{4} \times 11 = 2.75.

gJ=27.5 N kg−1g_J = 27.5\ \text{N kg}^{-1}. The answer is (1).

For a planet, gg goes with density times radius.

Write the ratio of the two planets and the constants cancel.

Exam tip

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