Year 12 Physics Module 5: Advanced Mechanics IQ3: Gravitational Fields Lessons 14–18 45 min

Checkpoint 3: Gravitational Fields

Test your understanding of gravitational potential energy, gravitational potential, escape velocity, Schwarzschild radius, and Kepler's laws. Covers Lessons 14–18.

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Lessons 14–15

Module Consolidation

  • $F = \dfrac{GMm}{r^2}$ — universal gravitation
  • $g = \dfrac{GM}{r^2}$ — field strength
  • Inverse square law: $F \propto \dfrac{1}{r^2}$
  • $r = R + h$ centre-to-centre distance
Lessons 16–17

Gravitational Potential Energy & Potential

  • $U = -\dfrac{GMm}{r}$ — GPE (zero at infinity)
  • $W = GMm\left(\dfrac{1}{r_1} - \dfrac{1}{r_2}\right)$ — work done
  • $V = -\dfrac{GM}{r}$ — gravitational potential
  • $g = -\dfrac{dV}{dr}$ — potential gradient
Lesson 18

Escape Velocity & Kepler's Laws

  • $v_e = \sqrt{\dfrac{2GM}{r}}$ — escape velocity
  • $R_s = \dfrac{2GM}{c^2}$ — Schwarzschild radius
  • $T^2 = \dfrac{4\pi^2}{GM}r^3$ — Kepler's Third Law
  • Orbital energy relationships
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Formula Reference — Gravitational Fields

$F = \dfrac{GMm}{r^2}$ F = gravitational force (N)  |  G = $6.67 \times 10^{-11}$ N m$^2$ kg$^{-2}$  |  r = centre-to-centre distance (m)
$g = \dfrac{GM}{r^2} = \dfrac{F}{m}$ g = gravitational field strength (N/kg or m/s$^2$)  |  r = $R + h$
$U = -\dfrac{GMm}{r}$ U = gravitational potential energy (J), negative — zero at infinity
$W = GMm\left(\dfrac{1}{r_1} - \dfrac{1}{r_2}\right)$ W = work done moving mass m from $r_1$ to $r_2$ (J)
$V = -\dfrac{GM}{r}$ V = gravitational potential (J/kg)  |  scalar quantity per unit mass
$g = -\dfrac{dV}{dr}$ Field strength = negative potential gradient (points toward decreasing $V$)
$v_e = \sqrt{\dfrac{2GM}{r}}$ $v_e$ = escape velocity (m/s) — minimum speed to reach infinity
$R_s = \dfrac{2GM}{c^2}$ $R_s$ = Schwarzschild radius (m) — event horizon of a black hole
$T^2 = \dfrac{4\pi^2}{GM}r^3$ T = orbital period (s)  |  r = orbital radius (m)  |  for circular orbits

1. The gravitational force between two 5 kg spheres with centres 0.5 m apart is:

A $1.33 \times 10^{-9}$ N
B $2.67 \times 10^{-8}$ N
C $6.67 \times 10^{-9}$ N
D $3.34 \times 10^{-10}$ N

2. If the distance between two masses is halved, the gravitational force becomes:

A Half the original value
B The same — force does not depend on distance
C Four times the original value
D One-quarter of the original value

3. The gravitational field strength at a point 3 Earth radii from Earth's centre is approximately:

A $9.8 \text{ m/s}^2$
B $3.27 \text{ m/s}^2$
C $1.09 \text{ m/s}^2$
D $0.36 \text{ m/s}^2$

4. Which statement correctly describes the direction of the gravitational force?

A Always attractive, acting along the line joining the centres of the two masses
B Always repulsive, pushing masses away from each other
C Attractive for small masses, repulsive for large masses
D Always perpendicular to the line joining the centres

5. The correct expression for gravitational potential energy of mass $m$ at distance $r$ from a planet of mass $M$ is:

A $U = +\dfrac{GMm}{r}$ (positive, increases with $r$)
B $U = -\dfrac{GMm}{r}$ (negative, zero at infinity)
C $U = GMmr$ (directly proportional to $r$)
D $U = -\dfrac{GMm}{r^2}$ (inverse square, like force)

6. The work done by gravity when a satellite moves from $r_1$ to a larger radius $r_2$ is:

A Negative, because gravity opposes the outward displacement
B Positive, because the satellite gains altitude
C Zero, because gravity is a conservative force
D Always $GMm$ regardless of the radii

7. Gravitational potential $V$ at distance $r$ from a mass $M$ is defined as:

A The force per unit mass: $V = \dfrac{GM}{r^2}$
B The potential energy per unit mass: $V = -\dfrac{GM}{r}$ (J/kg)
C The kinetic energy per unit mass: $V = \dfrac{GM}{2r}$
D The total energy per unit mass: $V = -\dfrac{GM}{2r}$

8. The relationship $g = -\dfrac{dV}{dr}$ tells us that:

A Gravitational field strength increases as potential increases
B $g$ points in the direction of decreasing $V$ (toward the mass), and its magnitude equals the potential gradient
C $g$ and $V$ are directly proportional at all points
D $g$ is always positive because field strength is a magnitude

9. Equipotential surfaces in a gravitational field are:

A Surfaces where the gravitational field strength $g$ is constant
B Surfaces where the gravitational potential $V$ is constant, and no work is done moving along them
C Always flat planes perpendicular to the field lines
D Surfaces where the kinetic energy of a mass is constant

10. The escape velocity from a planet's surface depends on:

A Only the mass of the escaping object
B The mass of the escaping object and the planet's mass
C The planet's mass and radius only — independent of the escaping object's mass
D The direction of launch — higher if launched against the planet's rotation

11. The Schwarzschild radius of a black hole represents:

A The radius of the event horizon — the boundary from which nothing, not even light, can escape
B The physical radius of the singularity at the centre
C The distance at which gravitational force becomes infinite
D The orbital radius of the innermost stable orbit

12. Kepler's Third Law states that for planets orbiting the Sun:

A $T \propto r$ — period is directly proportional to orbital radius
B $T \propto r^2$ — period is proportional to the square of orbital radius
C $T^2 \propto r^3$ — the square of the period is proportional to the cube of the semi-major axis
D $T \propto \dfrac{1}{r^{3/2}}$ — period is inversely proportional to $r^{3/2}$

13. A satellite in circular orbit around Earth has total mechanical energy $E$. Its kinetic energy $K$ and potential energy $U$ are related by:

A $K = U$ and $E = 2U$
B $K = -\dfrac{U}{2}$ and $E = -K = \dfrac{U}{2}$
C $K = -U$ and $E = 0$
D $K = 2U$ and $E = 3U$

14. To move a spacecraft from a low-Earth orbit to a higher orbit, the total work that must be done against gravity is:

A Negative, because the spacecraft loses energy
B Positive, because $U$ becomes less negative (closer to zero) at larger $r$
C Zero, because gravity is conservative and orbital energy is constant
D Equal to the change in kinetic energy only

15. Two planets orbit the same star. Planet X has orbital radius $4r$ and Planet Y has orbital radius $9r$. The ratio of their orbital periods $\dfrac{T_X}{T_Y}$ is:

A $\dfrac{4}{9}$
B $\dfrac{8}{27}$
C $\dfrac{16}{81}$
D $\dfrac{2}{3}$
Short Answer — 5 Questions
Apply Band 4 3 marks

Calculate the gravitational force between Earth ($M_E = 5.97 \times 10^{24}$ kg) and a 1000 kg satellite at altitude 600 km above Earth's surface. Then calculate the gravitational field strength at this altitude. Use $R_E = 6.37 \times 10^6$ m.

Apply Band 5 3 marks

A 500 kg probe moves from $r_1 = 7.0 \times 10^6$ m to $r_2 = 1.2 \times 10^7$ m from Earth's centre. Calculate the change in gravitational potential energy and the work done by the gravitational field. Use $M_E = 5.97 \times 10^{24}$ kg.

Analyse Band 5 4 marks

At a point in Earth's gravitational field, $V = -45$ MJ/kg. At another point 3000 km further from Earth's centre, $V = -36$ MJ/kg. Estimate the average gravitational field strength in this region and explain the meaning of the negative sign in $g = -\dfrac{dV}{dr}$.

Apply Band 6 4 marks

Calculate the escape velocity from the surface of Mars ($M = 6.42 \times 10^{23}$ kg, $R = 3.40 \times 10^6$ m). Calculate the Schwarzschild radius for Mars. Discuss whether Mars could ever become a black hole.

Apply Band 6 4 marks

Europa (Jupiter's moon) has an orbital period of 3.55 days. Using Kepler's Third Law, calculate its orbital radius given Jupiter's mass is $1.90 \times 10^{27}$ kg. Verify your answer is consistent with the known value of 671,000 km.

Model Answers

Multiple Choice Answers

1. C — $F = \dfrac{(6.67 \times 10^{-11}) \times 5 \times 5}{(0.5)^2} = \dfrac{1.6675 \times 10^{-9}}{0.25} = 6.67 \times 10^{-9}$ N. A uses $r = 1$ m, C is $1.33 \times 10^{-9}$ (forgot to square $r$), D uses $r = 0.25$ m.

2. C — From $F \propto 1/r^2$, halving $r$ gives $F' = F/(1/2)^2 = 4F$. A mistakes inverse square for inverse proportionality, B ignores distance, D has the change backwards.

3. C — $g = g_0 \times (R/r)^2 = 9.8 \times (1/3)^2 = 9.8/9 = 1.09$ m/s$^2$. A is surface value, B divides by 3 instead of 9, D divides by 27.

4. A — Gravitational force is always attractive, acting along the line joining centres. B and C describe repulsion which never occurs, D describes a perpendicular force.

5. B — $U = -GMm/r$ with negative sign mandatory; $U = 0$ at $r = \infty$. A has wrong sign, C has wrong dependence, D uses $1/r^2$ like force.

6. A — Gravity points inward; displacement is outward, so $W = \vec{F} \cdot \vec{d} < 0$. Gravity does negative work as the satellite moves outward. B confuses altitude gain with work sign, C confuses conservative with zero work.

7. B — Gravitational potential is GPE per unit mass: $V = U/m = -GM/r$ (J/kg). A confuses potential with field strength, C and D mix in kinetic energy.

8. B — The negative sign means $g$ points toward decreasing $V$ (toward the mass). $|g| = |dV/dr|$ gives the magnitude. A reverses the relationship, C claims direct proportionality which is false, D ignores the vector nature.

9. B — Equipotential surfaces have constant $V$; since $\Delta U = q\Delta V = 0$ along them, no work is done. A confuses equipotential with equal field strength, C is only true for uniform fields, D confuses potential with kinetic energy.

10. C — $v_e = \sqrt{2GM/r}$: depends only on the planet's $M$ and $r$. The escaping object's mass cancels out. A and B incorrectly include the object's mass, D confuses escape velocity with orbital launch.

11. A — $R_s = 2GM/c^2$ is the event horizon radius. B confuses it with the singularity (a point, $r = 0$), C suggests infinite force at $R_s$ which is wrong, D describes the photon sphere.

12. C — Kepler's Third Law: $T^2 \propto r^3$. A and B have wrong exponents, D inverts the relationship.

13. B — For circular orbits: $K = +GMm/2r$, $U = -GMm/r$, so $K = -U/2$ and $E = K + U = -GMm/2r = -K = U/2$. A, C, D have incorrect energy relationships.

14. B — Moving to higher orbit: $U$ increases (becomes less negative), so work done against gravity is positive. A has the sign wrong, C confuses orbital energy conservation with work done, D ignores potential energy change.

15. B — $\dfrac{T_X^2}{T_Y^2} = \dfrac{(4r)^3}{(9r)^3} = \dfrac{64}{729}$, so $\dfrac{T_X}{T_Y} = \sqrt{\dfrac{64}{729}} = \dfrac{8}{27}$. A uses $T \propto r$, C uses $T \propto r^2$, D takes $\sqrt{2/3}$.

Short Answer 1 (3 marks) — Gravitational Force and Field Strength at Altitude

Step 1: Find the centre-to-centre distance: $r = R_E + h = 6.37 \times 10^6 + 6.00 \times 10^5 = 6.97 \times 10^6$ m (1 mark for correct $r$)

Step 2: Calculate the gravitational force:

$F = \dfrac{GM_E m}{r^2} = \dfrac{(6.67 \times 10^{-11}) \times (5.97 \times 10^{24}) \times 1000}{(6.97 \times 10^6)^2}$

$F = \dfrac{3.98 \times 10^{17}}{4.86 \times 10^{13}} = 8.19 \times 10^3$ N (1 mark)

Step 3: Calculate gravitational field strength:

$g = \dfrac{GM_E}{r^2} = \dfrac{(6.67 \times 10^{-11}) \times (5.97 \times 10^{24})}{(6.97 \times 10^6)^2} = \dfrac{3.98 \times 10^{14}}{4.86 \times 10^{13}} = 8.19$ N/kg (or m/s$^2$) (1 mark)

Alternatively: $g = F/m = 8.19 \times 10^3/1000 = 8.19$ N/kg. This is about 84% of surface gravity — astronauts at this altitude still experience strong gravity.

Short Answer 2 (3 marks) — Change in GPE and Work Done

Step 1: Calculate GPE at each position:

$U_1 = -\dfrac{GM_E m}{r_1} = -\dfrac{(6.67 \times 10^{-11}) \times (5.97 \times 10^{24}) \times 500}{7.0 \times 10^6} = -\dfrac{1.99 \times 10^{14}}{7.0 \times 10^6} = -2.84 \times 10^7$ J

$U_2 = -\dfrac{GM_E m}{r_2} = -\dfrac{(6.67 \times 10^{-11}) \times (5.97 \times 10^{24}) \times 500}{1.2 \times 10^7} = -\dfrac{1.99 \times 10^{14}}{1.2 \times 10^7} = -1.66 \times 10^7$ J (1 mark for both GPE values)

Step 2: Calculate the change in GPE:

$\Delta U = U_2 - U_1 = (-1.66 \times 10^7) - (-2.84 \times 10^7) = +1.18 \times 10^7$ J (1 mark)

Step 3: The work done by the gravitational field is:

$W_{\text{field}} = -\Delta U = -1.18 \times 10^7$ J (1 mark)

Alternatively using $W = GMm(1/r_1 - 1/r_2)$:

$W = (6.67 \times 10^{-11}) \times (5.97 \times 10^{24}) \times 500 \times \left(\dfrac{1}{7.0 \times 10^6} - \dfrac{1}{1.2 \times 10^7}\right)$

$W = 1.99 \times 10^{14} \times (1.429 \times 10^{-7} - 8.333 \times 10^{-8}) = 1.99 \times 10^{14} \times 5.95 \times 10^{-8} = 1.18 \times 10^7$ J (work done against gravity)

The gravitational field does negative work as the probe moves outward (force and displacement are in opposite directions).

Short Answer 3 (4 marks) — Potential Gradient and Field Strength

Step 1: Convert values and find the potential difference:

$V_1 = -45$ MJ/kg $= -45 \times 10^6$ J/kg, $V_2 = -36$ MJ/kg $= -36 \times 10^6$ J/kg

$\Delta V = V_2 - V_1 = (-36 \times 10^6) - (-45 \times 10^6) = +9 \times 10^6$ J/kg

$\Delta r = 3000$ km $= 3.0 \times 10^6$ m (1 mark for correct conversions)

Step 2: Estimate average field strength:

$g_{\text{avg}} = -\dfrac{\Delta V}{\Delta r} = -\dfrac{9 \times 10^6}{3.0 \times 10^6} = -3.0$ N/kg (1 mark)

The magnitude is $|g| = 3.0$ N/kg (or 3.0 m/s$^2$). (1 mark)

Step 3: The negative sign in $g = -dV/dr$ means:

Gravitational potential $V$ increases (becomes less negative) as $r$ increases. Since $V$ increases with $r$, the gradient $dV/dr$ is positive. The negative sign ensures that $g$ points in the direction of decreasing $r$ — that is, toward the centre of the Earth. The field strength vector points inward, toward the mass that creates the field. This convention ensures that $g$ correctly represents the direction of gravitational force on a test mass. (1 mark for explanation)

Short Answer 4 (4 marks) — Escape Velocity and Schwarzschild Radius for Mars

Step 1 — Escape velocity:

$v_e = \sqrt{\dfrac{2GM}{R}} = \sqrt{\dfrac{2 \times (6.67 \times 10^{-11}) \times (6.42 \times 10^{23})}{3.40 \times 10^6}}$ (1 mark for formula and substitution)

$v_e = \sqrt{\dfrac{8.56 \times 10^{13}}{3.40 \times 10^6}} = \sqrt{2.52 \times 10^7} = 5.02 \times 10^3$ m/s $= 5.02$ km/s (1 mark)

Step 2 — Schwarzschild radius:

$R_s = \dfrac{2GM}{c^2} = \dfrac{2 \times (6.67 \times 10^{-11}) \times (6.42 \times 10^{23})}{(3.0 \times 10^8)^2}$ (1 mark)

$R_s = \dfrac{8.56 \times 10^{13}}{9.0 \times 10^{16}} = 9.51 \times 10^{-4}$ m $\approx 0.95$ mm

Step 3 — Discussion:

Mars cannot become a black hole under any known physical process. The Schwarzschild radius (~0.95 mm) is many orders of magnitude smaller than Mars's actual radius (3.4 million metres). For Mars to become a black hole, all its mass would need to be compressed into a sphere less than 1 mm across — an impossible density ($\rho \approx 10^{25}$ kg/m$^3$) far exceeding anything achievable by gravitational collapse. Stellar-mass black holes form from stars with core masses exceeding the Chandrasekhar limit (~1.4 solar masses) that undergo supernova collapse. Mars's mass ($\sim 0.1\%$ of solar mass) is far below any threshold for gravitational collapse to a black hole. (1 mark for discussion)

Short Answer 5 (4 marks) — Kepler's Third Law for Europa

Step 1: Convert the orbital period to seconds:

$T = 3.55 \times 24 \times 3600 = 3.067 \times 10^5$ s (1 mark for conversion)

Step 2: Rearrange Kepler's Third Law:

$T^2 = \dfrac{4\pi^2}{GM_J} r^3 \implies r^3 = \dfrac{GM_J T^2}{4\pi^2}$

$r^3 = \dfrac{(6.67 \times 10^{-11}) \times (1.90 \times 10^{27}) \times (3.067 \times 10^5)^2}{4\pi^2}$ (1 mark for correct substitution)

$r^3 = \dfrac{(6.67 \times 10^{-11}) \times (1.90 \times 10^{27}) \times 9.41 \times 10^{10}}{39.48}$

$r^3 = \dfrac{1.19 \times 10^{28}}{39.48} = 3.02 \times 10^{26}$ m$^3$

Step 3: Calculate $r$:

$r = \sqrt[3]{3.02 \times 10^{26}} = 6.71 \times 10^8$ m (1 mark)

$r = 6.71 \times 10^8$ m $= 6.71 \times 10^5$ km $= 671,000$ km

Step 4 — Verification:

The calculated orbital radius of 671,000 km is in excellent agreement with the known value of 671,000 km (to 3 significant figures). This confirms that Kepler's Third Law, when combined with Newton's law of gravitation, accurately predicts the orbital parameters of moons around planets. The small difference ($< 0.1\%$) arises from rounding in the given values. (1 mark for verification)

Mark Checkpoint 3 Complete

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