Test your understanding of gravitational potential energy, gravitational potential, escape velocity, Schwarzschild radius, and Kepler's laws. Covers Lessons 14–18.
1. The gravitational force between two 5 kg spheres with centres 0.5 m apart is:
2. If the distance between two masses is halved, the gravitational force becomes:
3. The gravitational field strength at a point 3 Earth radii from Earth's centre is approximately:
4. Which statement correctly describes the direction of the gravitational force?
5. The correct expression for gravitational potential energy of mass $m$ at distance $r$ from a planet of mass $M$ is:
6. The work done by gravity when a satellite moves from $r_1$ to a larger radius $r_2$ is:
7. Gravitational potential $V$ at distance $r$ from a mass $M$ is defined as:
8. The relationship $g = -\dfrac{dV}{dr}$ tells us that:
9. Equipotential surfaces in a gravitational field are:
10. The escape velocity from a planet's surface depends on:
11. The Schwarzschild radius of a black hole represents:
12. Kepler's Third Law states that for planets orbiting the Sun:
13. A satellite in circular orbit around Earth has total mechanical energy $E$. Its kinetic energy $K$ and potential energy $U$ are related by:
14. To move a spacecraft from a low-Earth orbit to a higher orbit, the total work that must be done against gravity is:
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:
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.
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.
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 $g = -\dfrac{dV}{dr}$.
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.
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.
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 $\sqrt{2/3}$.
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.
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).
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)
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)
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)
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