OCR A-Level · Thinka-original Practice Paper

2022 OCR A-Level Physics A - H556 Practice Paper with Answers

Thinka Jun 2022 Cambridge OCR A Level-Style Mock — Physics A - H556

270 marks360 mins2022
An original Thinka practice paper modelled on the structure and difficulty of the Jun 2022 Cambridge OCR A Level Physics A - H556 paper. Not affiliated with or reproduced from Cambridge.

Paper 1 (Modelling Physics)

Answer all questions in Section A (Multiple Choice) and Section B (Structured Questions).
23 Question · 100 marks
Question 1 · Multiple Choice
1 marks
A cylinder of uniform cross-section has the following measurements:

Mass \( m = 24.0 \pm 0.6 \text{ g} \)

Length \( L = 50.0 \pm 1.0 \text{ mm} \)

Diameter \( d = 10.0 \pm 0.1 \text{ mm} \)

What is the percentage uncertainty in the calculated density of the cylinder?
  1. A.\( 3.5\% \)
  2. B.\( 4.5\% \)
  3. C.\( 6.5\% \)
  4. D.\( 7.0\% \)
Show answer & marking scheme

Worked solution

The density is given by the formula:
\( \rho = \frac{m}{V} = \frac{m}{\pi (d/2)^2 L} = \frac{4m}{\pi d^2 L} \)

To find the overall percentage uncertainty, we add the percentage uncertainties of each component, multiplying by their powers in the formula:

1. Percentage uncertainty in \( m \):
\( \frac{0.6}{24.0} \times 100\% = 2.5\% \)

2. Percentage uncertainty in \( d \):
\( \frac{0.1}{10.0} \times 100\% = 1.0\% \)

3. Percentage uncertainty in \( L \):
\( \frac{1.0}{50.0} \times 100\% = 2.0\% \)

Now, combine these using the uncertainty combination rule:
\( \frac{\Delta \rho}{\rho} \% = \frac{\Delta m}{m} \% + 2\left(\frac{\Delta d}{d} \%\right) + \frac{\Delta L}{L} \% \)
\( \frac{\Delta \rho}{\rho} \% = 2.5\% + 2(1.0\%) + 2.0\% = 6.5\% \)

Marking scheme

Award 1 mark for the correct option C.

- Correct calculation of individual percentage uncertainties (Mass: 2.5%, Diameter: 1.0%, Length: 2.0%)
- Correct application of the power rule for combining uncertainties (doubling the uncertainty of diameter)
- Correct total of 6.5%
Question 2 · Multiple Choice
1 marks
A sealed container holds a mixture of helium gas (molar mass \( 4.0 \text{ g mol}^{-1} \)) and oxygen gas (molar mass \( 32.0 \text{ g mol}^{-1} \)) in thermal equilibrium.

What is the value of the ratio:

\( \frac{\text{r.m.s. speed of helium atoms}}{\text{r.m.s. speed of oxygen molecules}} \)?
  1. A.\( 0.13 \)
  2. B.\( 0.35 \)
  3. C.\( 2.8 \)
  4. D.\( 8.0 \)
Show answer & marking scheme

Worked solution

Since the two gases are in thermal equilibrium in the same container, they are at the same temperature \( T \).

The mean kinetic energy of a gas molecule is:
\( E_k = \frac{3}{2} k_B T = \frac{1}{2} m c^2 \)

Therefore, the root-mean-square speed \( c_{\text{rms}} \) is:
\( c_{\text{rms}} = \sqrt{\frac{3 k_B T}{m}} \)

This shows that the r.m.s. speed is inversely proportional to the square root of the mass of the particles:
\( c_{\text{rms}} \propto \frac{1}{\sqrt{M}} \)

Taking the ratio:
\( \frac{c_{\text{rms, He}}}{c_{\text{rms, O}_2}} = \sqrt{\frac{M_{\text{O}_2}}{M_{\text{He}}}} = \sqrt{\frac{32.0}{4.0}} = \sqrt{8.0} \approx 2.83 \)

This rounds to 2.8.

Marking scheme

Award 1 mark for the correct option C.

- Realisation that thermal equilibrium means both gases are at the same temperature, hence same mean kinetic energy
- Correct dependency of r.m.s. speed on the inverse square root of mass
- Correct ratio calculated to be approx 2.8
Question 3 · Multiple Choice
1 marks
Four identical springs, each with a spring constant \( k \), are arranged such that two parallel pairs of springs are connected in series with each other.

What is the total work done in extending this entire system by a total distance \( x \)?
  1. A.\( \frac{1}{8} k x^2 \)
  2. B.\( \frac{1}{4} k x^2 \)
  3. C.\( \frac{1}{2} k x^2 \)
  4. D.\( 2 k x^2 \)
Show answer & marking scheme

Worked solution

First, find the effective spring constant, \( k_{\text{eff}} \), of the system.

1. Each parallel pair consists of two identical springs of constant \( k \).
The effective spring constant of each parallel pair is:
\( k_{\text{parallel}} = k + k = 2k \)

2. The system consists of these two parallel pairs connected in series. Therefore, we have two blocks of spring constant \( 2k \) in series:
\( \frac{1}{k_{\text{eff}}} = \frac{1}{2k} + \frac{1}{2k} = \frac{2}{2k} = \frac{1}{k} \)
So, \( k_{\text{eff}} = k \).

3. The total work done in extending this system of effective stiffness \( k \) by a distance \( x \) is given by:
\( W = \frac{1}{2} k_{\text{eff}} x^2 = \frac{1}{2} k x^2 \)

Marking scheme

Award 1 mark for the correct option C.

- Correct combination of springs in parallel to give \( 2k \)
- Correct combination of parallel pairs in series to find effective spring constant is \( k \)
- Work formula \( W = \frac{1}{2} k_{\text{eff}} x^2 \) correctly applied
Question 4 · Multiple Choice
1 marks
A satellite orbits a planet of mass \( M \) in a circular orbit of radius \( r \) with an orbital period \( T \). A second satellite orbits a different planet of mass \( 4M \) in a circular orbit of radius \( 2r \).

What is the orbital period of the second satellite?
  1. A.\( \sqrt{2} T \)
  2. B.\( 2 T \)
  3. C.\( 2\sqrt{2} T \)
  4. D.\( 4 T \)
Show answer & marking scheme

Worked solution

By equating the gravitational force to the centripetal force:
\( \frac{G M m}{r^2} = m \omega^2 r = m \left(\frac{2\pi}{T}\right)^2 r \)

Simplifying for \( T^2 \):
\( T^2 = \frac{4\pi^2 r^3}{G M} \implies T \propto \sqrt{\frac{r^3}{M}} \)

Let the orbital period of the second satellite be \( T_2 \). Substituting the new parameters:
\( T_2 \propto \sqrt{\frac{(2r)^3}{4M}} = \sqrt{\frac{8r^3}{4M}} = \sqrt{2} \sqrt{\frac{r^3}{M}} \)

Therefore, \( T_2 = \sqrt{2} T \).

Marking scheme

Award 1 mark for the correct option A.

- Derivation of Kepler's Third Law relationship \( T^2 \propto \frac{r^3}{M} \)
- Substitution of \( 2r \) and \( 4M \) into the ratio
- Simplification to find the multiplier is \( \sqrt{2} \)
Question 5 · Multiple Choice
1 marks
An object undergoes simple harmonic motion with an amplitude of \( 5.0 \text{ cm} \) and a maximum acceleration of \( 20 \text{ m s}^{-2} \).

What is the maximum speed of the object during its oscillation?
  1. A.\( 1.0 \text{ m s}^{-1} \)
  2. B.\( 2.0 \text{ m s}^{-1} \)
  3. C.\( 4.0 \text{ m s}^{-1} \)
  4. D.\( 10 \text{ m s}^{-1} \)
Show answer & marking scheme

Worked solution

In simple harmonic motion, maximum acceleration is given by:
\( a_{\text{max}} = \omega^2 A \)
And maximum velocity is given by:
\( v_{\text{max}} = \omega A \)

From these equations, we can write:
\( \omega = \sqrt{\frac{a_{\text{max}}}{A}} \)

Substituting the values (with amplitude converted to meters: \( A = 0.050 \text{ m} \)):
\( \omega = \sqrt{\frac{20}{0.050}} = \sqrt{400} = 20 \text{ rad s}^{-1} \)

Now, calculate the maximum speed:
\( v_{\text{max}} = \omega A = 20 \times 0.050 = 1.0 \text{ m s}^{-1} \)

Marking scheme

Award 1 mark for the correct option A.

- Correct conversions (e.g., converting 5.0 cm to 0.050 m)
- Use of \( a_{\text{max}} = \omega^2 A \) to find \( \omega = 20 \text{ rad s}^{-1} \)
- Correct calculation of \( v_{\text{max}} = 1.0 \text{ m s}^{-1} \)
Question 6 · Multiple Choice
1 marks
An electrical heater of constant power \( 60 \text{ W} \) is used to heat \( 0.20 \text{ kg} \) of a liquid in a well-insulated container. The liquid is initially at its boiling point. If the heater is switched on for \( 5.0 \text{ minutes} \), exactly half of the liquid is vaporised.

What is the specific latent heat of vaporisation of the liquid?
  1. A.\( 9.0 \times 10^4 \text{ J kg}^{-1} \)
  2. B.\( 1.8 \times 10^5 \text{ J kg}^{-1} \)
  3. C.\( 3.6 \times 10^5 \text{ J kg}^{-1} \)
  4. D.\( 1.8 \times 10^6 \text{ J kg}^{-1} \)
Show answer & marking scheme

Worked solution

1. Calculate the total energy \( E \) supplied by the electrical heater in \( 5.0 \text{ minutes} \):
\( t = 5.0 \times 60 = 300 \text{ s} \)
\( E = P \times t = 60 \text{ W} \times 300 \text{ s} = 18000 \text{ J} \)

2. Determine the mass \( m \) of the liquid that actually vaporised:
Only half of the \( 0.20 \text{ kg} \) of liquid vaporised, so:
\( m = 0.10 \text{ kg} \)

3. Use the formula for specific latent heat:
\( E = m L_v \implies L_v = \frac{E}{m} \)
\( L_v = \frac{18000 \text{ J}}{0.10 \text{ kg}} = 1.8 \times 10^5 \text{ J kg}^{-1} \)

Marking scheme

Award 1 mark for the correct option B.

- Correct conversion of time to seconds (300 s) and energy calculation (18,000 J)
- Realisation that only half of the mass (0.10 kg) undergoes phase change
- Correct division of energy by mass to find \( 1.8 \times 10^5 \text{ J kg}^{-1} \)
Question 7 · Multiple Choice
1 marks
The peak wavelength of emission from Star X is twice that of Star Y (\( \lambda_{\text{max, X}} = 2 \lambda_{\text{max, Y}} \)). The radius of Star X is four times the radius of Star Y (\( R_{\text{X}} = 4 R_{\text{Y}} \)).

Assuming both stars behave as perfect black bodies, what is the ratio of their luminosities, \( \frac{L_{\text{X}}}{L_{\text{Y}}} \)?
  1. A.\( 0.25 \)
  2. B.\( 1.0 \)
  3. C.\( 4.0 \)
  4. D.\( 16.0 \)
Show answer & marking scheme

Worked solution

1. From Wien's displacement law (\( \lambda_{\text{max}} T = \text{constant} \)):
\( T \propto \frac{1}{\lambda_{\text{max}}} \)
Therefore, the ratio of temperatures is:
\( \frac{T_{\text{X}}}{T_{\text{Y}}} = \frac{\lambda_{\text{max, Y}}}{\lambda_{\text{max, X}}} = \frac{1}{2} \)

2. From Stefan's Law, the luminosity \( L \) is:
\( L = 4\pi R^2 \sigma T^4 \implies L \propto R^2 T^4 \)

3. Calculate the ratio of the luminosities:
\( \frac{L_{\text{X}}}{L_{\text{Y}}} = \left(\frac{R_{\text{X}}}{R_{\text{Y}}}\right)^2 \left(\frac{T_{\text{X}}}{T_{\text{Y}}}\right)^4 \)
Substituting the ratios:
\( \frac{L_{\text{X}}}{L_{\text{Y}}} = (4)^2 \times \left(\frac{1}{2}\right)^4 = 16 \times \frac{1}{16} = 1.0 \)

Marking scheme

Award 1 mark for the correct option B.

- Correct application of Wien's law to find temperature ratio \( T_{\text{X}}/T_{\text{Y}} = 0.5 \)
- Correct application of Stefan's law showing \( L \propto R^2 T^4 \)
- Correct combination of both ratios to yield 1.0
Question 8 · Multiple Choice
1 marks
Two blocks of masses \( 3.0 \text{ kg} \) and \( 1.0 \text{ kg} \) are in contact on a frictionless horizontal surface. A horizontal force of \( 12 \text{ N} \) is applied directly to the \( 3.0 \text{ kg} \) block, pushing both blocks across the surface.

What is the magnitude of the contact force exerted by the \( 3.0 \text{ kg} \) block on the \( 1.0 \text{ kg} \) block?
  1. A.\( 3.0 \text{ N} \)
  2. B.\( 4.0 \text{ N} \)
  3. C.\( 9.0 \text{ N} \)
  4. D.\( 12 \text{ N} \)
Show answer & marking scheme

Worked solution

1. Treat both blocks as a single combined mass system to find the acceleration \( a \):
\( F_{\text{total}} = (m_1 + m_2) a \)
\( 12 \text{ N} = (3.0 \text{ kg} + 1.0 \text{ kg}) a \implies a = \frac{12}{4.0} = 3.0 \text{ m s}^{-2} \)

2. Now isolate the second block (mass \( 1.0 \text{ kg} \)). The only horizontal force acting on it is the contact force \( F_{\text{contact}} \) exerted by the first block:
\( F_{\text{contact}} = m_2 a \)
\( F_{\text{contact}} = 1.0 \text{ kg} \times 3.0 \text{ m s}^{-2} = 3.0 \text{ N} \)

According to Newton's third law, the magnitude of the force exerted by the first block on the second is equal to the force exerted by the second on the first, which is \( 3.0 \text{ N} \).

Marking scheme

Award 1 mark for the correct option A.

- Correct calculation of the system acceleration (\( 3.0 \text{ m s}^{-2} \))
- Correct application of \( F = ma \) to the \( 1.0 \text{ kg} \) block to determine the contact force of \( 3.0 \text{ N} \)
Question 9 · multiple_choice
1 marks
A student measures the physical dimensions of a uniform metal wire to determine its density \(\rho\).

The experimental measurements and their absolute uncertainties are:
- Mass \(m = 2.50 \pm 0.02\text{ g}\)
- Length \(L = 40.0 \pm 0.5\text{ cm}\)
- Diameter \(d = 0.80 \pm 0.01\text{ mm}\)

What is the percentage uncertainty in the calculated density of the wire?
  1. A.2.1%
  2. B.3.3%
  3. C.4.6%
  4. D.5.8%
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Worked solution

The density \(\rho\) of the wire is given by:

\(\rho = \frac{m}{V} = \frac{4m}{\pi d^2 L}\)

The percentage uncertainty in the calculated density is found by summing the fractional uncertainties of the independent variables, remembering to multiply the fractional uncertainty of the diameter by 2 (due to the exponent):

\(\frac{\Delta \rho}{\rho} = \frac{\Delta m}{m} + 2\left(\frac{\Delta d}{d}\right) + \frac{\Delta L}{L}\)

Calculating each individual percentage uncertainty:
- Mass: \(\frac{0.02}{2.50} \times 100\% = 0.80\%\)
- Diameter: \(\frac{0.01}{0.80} \times 100\% = 1.25\%\)
- Length: \(\frac{0.5}{40.0} \times 100\% = 1.25\%\)

Combining these together:

\(\%\Delta \rho = 0.80\% + 2(1.25\%) + 1.25\% = 0.80\% + 2.50\% + 1.25\% = 4.55\%\)

To two significant figures, this is \(4.6\%\).

Marking scheme

C
Question 10 · multiple_choice
1 marks
Two identical springs, each with a spring constant of \(k = 200\text{ N m}^{-1}\), are connected in parallel. This parallel pair is then connected in series with a third identical spring of spring constant \(k = 200\text{ N m}^{-1}\). A load of \(30\text{ N}\) is suspended from the bottom of the system.

What is the total elastic potential energy stored in the entire system of three springs?
  1. A.1.1 J
  2. B.2.3 J
  3. C.3.4 J
  4. D.6.8 J
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Worked solution

First, find the effective spring constant of the parallel combination \(k_p\):
\(k_p = k + k = 200 + 200 = 400\text{ N m}^{-1}\)

Now, calculate the overall effective spring constant \(k_{\text{eff}}\) of the system, where the parallel combination is in series with the third spring:
\(\frac{1}{k_{\text{eff}}} = \frac{1}{k_p} + \frac{1}{k} = \frac{1}{400} + \frac{1}{200} = \frac{3}{400}\text{ m N}^{-1}\)
\(k_{\text{eff}} = \frac{400}{3} \approx 133.3\text{ N m}^{-1}\)

The elastic potential energy \(E_p\) stored under a load of \(F = 30\text{ N}\) is:
\(E_p = \frac{1}{2} \frac{F^2}{k_{\text{eff}}} = \frac{1}{2} \times \frac{30^2}{400/3} = \frac{1}{2} \times \frac{900 \times 3}{400} = 3.375\text{ J} \approx 3.4\text{ J}\)

Marking scheme

C
Question 11 · multiple_choice
1 marks
An ideal gas in a sealed container of fixed volume has a pressure \(p\) and an absolute temperature \(T\). The root-mean-square (r.m.s.) speed of the gas molecules is \(c_{\text{rms}}\).

The gas is heated so that its pressure increases to \(1.69 p\).

What is the new r.m.s. speed of the gas molecules in terms of \(c_{\text{rms}}\)?
  1. A.1.13 c_rms
  2. B.1.30 c_rms
  3. C.1.69 c_rms
  4. D.2.86 c_rms
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Worked solution

For an ideal gas at a constant volume, the pressure is directly proportional to the absolute temperature (Gay-Lussac's Law):
\(p \propto T\)

Since the pressure increases by a factor of \(1.69\), the absolute temperature must also increase by a factor of \(1.69\).

The r.m.s. speed of gas molecules is given by:
\(c_{\text{rms}} = \sqrt{\frac{3kT}{m}}\)

This shows that \(c_{\text{rms}} \propto \sqrt{T}\).

The new r.m.s. speed \(c_{\text{new}}\) is:
\(c_{\text{new}} = \sqrt{1.69} \times c_{\text{rms}} = 1.30 c_{\text{rms}}\)

Marking scheme

B
Question 12 · multiple_choice
1 marks
A particle of mass \(m\) oscillates with simple harmonic motion of period \(T\). Its displacement \(x\) at time \(t\) is described by \(x = A \cos(\omega t)\), where \(A\) is the amplitude.

At what time \(t > 0\) is the kinetic energy of the particle first equal to its potential energy?
  1. A.t = T/8
  2. B.t = T/6
  3. C.t = T/4
  4. D.t = T/2
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Worked solution

The total energy of the simple harmonic oscillator is given by \(E = E_k + E_p\).

When the kinetic energy \(E_k\) is equal to the potential energy \(E_p\):
\(E = 2E_p\)

Substituting the definitions of total and potential energy:
\(\frac{1}{2} m \omega^2 A^2 = 2 \left(\frac{1}{2} m \omega^2 x^2\right) \implies A^2 = 2x^2 \implies x = \frac{A}{\sqrt{2}}\)

Since \(x = A \cos(\omega t)\):
\(A \cos(\omega t) = \frac{A}{\sqrt{2}} \implies \cos(\omega t) = \frac{1}{\sqrt{2}}\)

The first non-zero solution occurs when:
\(\omega t = \frac{\pi}{4}\)

Substituting \(\omega = \frac{2\pi}{T}\):
\(\frac{2\pi}{T} t = \frac{\pi}{4} \implies t = \frac{T}{8}\)

Marking scheme

A
Question 13 · multiple_choice
1 marks
A satellite is in a stable circular orbit of radius \(R\) around a planet of mass \(M\). It has an orbital speed \(v\) and an orbital period \(T\).

Another satellite is launched into a circular orbit of radius \(4R\) around the same planet.

What are the orbital speed and the orbital period of the second satellite?
  1. A.Speed = 0.25 v, Period = 16 T
  2. B.Speed = 0.5 v, Period = 8 T
  3. C.Speed = 0.5 v, Period = 16 T
  4. D.Speed = 2 v, Period = 8 T
Show answer & marking scheme

Worked solution

For a circular orbit, the gravitational force provides the centripetal force:
\(\frac{GMm}{r^2} = \frac{mv^2}{r} \implies v = \sqrt{\frac{GM}{r}}\)

If the orbital radius increases from \(R\) to \(4R\), the new speed \(v'\) is:
\(v' = \sqrt{\frac{GM}{4R}} = \frac{1}{2} \sqrt{\frac{GM}{R}} = 0.5v\)

According to Kepler's Third Law, the period of the orbit is related to the radius by:
\(T^2 \propto r^3 \implies T \propto r^{1.5}\)

If the radius is multiplied by 4, the new period \(T'\) is:
\(T' = 4^{1.5} T = 8T\)

Marking scheme

B
Question 14 · multiple_choice
1 marks
An estimate for the Hubble constant \(H_0\) is \(68\text{ km s}^{-1}\text{ Mpc}^{-1}\).

Using the relation \(t \approx \frac{1}{H_0}\), what is the corresponding estimate for the age of the Universe in years?

Use the following data:
- \(1\text{ pc} = 3.1 \times 10^{16}\text{ m}\)
- \(1\text{ year} = 3.2 \times 10^7\text{ s}\)
  1. A.4.6 x 10^8 years
  2. B.9.5 x 10^9 years
  3. C.1.4 x 10^10 years
  4. D.4.6 x 10^17 years
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Worked solution

First, convert \(H_0\) from \(\text{km s}^{-1}\text{ Mpc}^{-1}\) to SI base units (\(\text{s}^{-1}\)):

\(H_0 = 68\text{ km s}^{-1}\text{ Mpc}^{-1} = \frac{68 \times 10^3\text{ m s}^{-1}}{10^6 \times 3.1 \times 10^{16}\text{ m}} = 2.1935 \times 10^{-18}\text{ s}^{-1}\)

Now calculate the estimated age of the Universe in seconds:

\(t \approx \frac{1}{H_0} = \frac{1}{2.1935 \times 10^{-18}\text{ s}^{-1}} = 4.5588 \times 10^{17}\text{ s}\)

Convert this value into years:

\(t_{\text{years}} = \frac{4.5588 \times 10^{17}\text{ s}}{3.2 \times 10^7\text{ s year}^{-1}} \approx 1.42 \times 10^{10}\text{ years}\)

This matches \(1.4 \times 10^{10}\text{ years}\).

Marking scheme

C
Question 15 · multiple_choice
1 marks
A block of mass \(m\) slides down a rough ramp at constant velocity. The ramp is inclined at an angle \(\theta\) to the horizontal.

Which expression gives the coefficient of dynamic friction \(\mu\) between the block and the ramp?
  1. A.\mu = \sin\theta
  2. B.\mu = \cos\theta
  3. C.\mu = \tan\theta
  4. D.\mu = 1 / \tan\theta
Show answer & marking scheme

Worked solution

Because the block moves at constant velocity, there is zero net force acting on it.

Resolving forces perpendicular to the ramp:
\(N = mg \cos\theta\)
where \(N\) is the normal contact force.

Resolving forces parallel to the ramp:
\(F_f = mg \sin\theta\)
where \(F_f\) is the dynamic frictional force.

Using the dynamic friction relation \(F_f = \mu N\):
\(mg \sin\theta = \mu (mg \cos\theta)\)

Solving for \(\mu\):
\(\mu = \frac{\sin\theta}{\cos\theta} = \tan\theta\)

Marking scheme

C
Question 16 · Structured
10.625 marks
A weather balloon containing helium gas is released from ground level where the atmospheric pressure is \(1.01 \times 10^5 \text{ Pa}\) and the temperature is \(15.0^\circ\text{C}\). The volume of the balloon at ground level is \(12.5 \text{ m}^3\).

(a) Calculate the number of moles of helium gas inside the balloon.

(b) The balloon rises to an altitude where the pressure is \(3.50 \times 10^4 \text{ Pa}\) and the temperature is \(-42.0^\circ\text{C}\). Calculate the new volume of the balloon, assuming helium behaves as an ideal gas.

(c) Using the kinetic theory of gases, explain how the pressure of the helium gas would change if its volume was kept constant at \(12.5 \text{ m}^3\) while the temperature decreased from \(15.0^\circ\text{C}\) to \(-42.0^\circ\text{C}\).
Show answer & marking scheme

Worked solution

(a) Convert temperature to Kelvin:
\(T = 15.0 + 273.15 = 288.15 \text{ K}\)

Using the ideal gas equation:
\(p V = n R T \implies n = \frac{p V}{R T}\)
\(n = \frac{1.01 \times 10^5 \times 12.5}{8.31 \times 288.15} \approx 527 \text{ mol}\)

(b) Using the ideal gas equation in the form:
\(\frac{p_1 V_1}{T_1} = \frac{p_2 V_2}{T_2}\)

Convert the new temperature to Kelvin:
\(T_2 = -42.0 + 273.15 = 231.15 \text{ K}\)

\(V_2 = \frac{p_1 V_1 T_2}{p_2 T_1} = \frac{1.01 \times 10^5 \times 12.5 \times 231.15}{3.50 \times 10^4 \times 288.15} \approx 28.9 \text{ m}^3\)

(c) As the temperature of the gas decreases, the mean kinetic energy of the helium atoms decreases, meaning their mean speed decreases. This leads to less frequent collisions between the atoms and the walls of the balloon. Additionally, each collision results in a smaller change in momentum. Since pressure is proportional to the rate of change of momentum of the atoms colliding with the walls per unit area, the pressure exerted by the gas decreases.

Marking scheme

(a)
- Use of \(T_1 = 288 \text{ K}\) or \(288.15 \text{ K}\) [1 mark]
- Correct rearrangement of ideal gas law: \(n = \frac{pV}{RT}\) [1 mark]
- Calculation to give \(527 \text{ mol}\) (accept range \(527 - 528 \text{ mol}\)) [1 mark]

(b)
- Use of \(T_2 = 231 \text{ K}\) or \(231.15 \text{ K}\) [1 mark]
- Correct rearrangement: \(V_2 = \frac{p_1 V_1 T_2}{p_2 T_1}\) or use of \(V_2 = \frac{nRT_2}{p_2}\) [1 mark]
- Calculation to give \(28.9 \text{ m}^3\) (accept range \(28.8 - 29.0 \text{ m}^3\)) [1 mark]

(c)
- Absolute temperature is proportional to mean kinetic energy / mean square speed of molecules [1 mark]
- Lower speed means fewer collisions per unit time with the container walls [1 mark]
- Lower speed means smaller change in momentum per collision [1 mark]
- Rate of change of momentum decreases, so force per unit area (pressure) decreases [1.625 marks]
Question 17 · Structured
10.625 marks
A mass of \(0.350 \text{ kg}\) is attached to a vertical spring suspended from a rigid support. When the mass is pulled downwards and released, it performs simple harmonic oscillations with a period of \(0.780 \text{ s}\).

(a) Show that the spring constant \(k\) of the spring is approximately \(23 \text{ N m}^{-1}\).

(b) The mass is displaced by \(0.050 \text{ m}\) from its equilibrium position and released from rest. Calculate:
(i) the maximum acceleration of the mass.
(ii) the maximum speed of the mass.

(c) State the positions during the motion where the kinetic energy is maximum, and where the elastic potential energy is maximum.
Show answer & marking scheme

Worked solution

(a) Using the equation for the period of a mass-spring system:
\(T = 2\pi \sqrt{\frac{m}{k}} \implies T^2 = 4\pi^2 \frac{m}{k}\)

Rearranging for \(k\):
\(k = \frac{4\pi^2 m}{T^2} = \frac{4\pi^2 \times 0.350}{0.780^2} = 22.71 \text{ N m}^{-1} \approx 23 \text{ N m}^{-1}\).

(b) (i) First, calculate the angular frequency \(\omega\):
\(\omega = \frac{2\pi}{T} = \frac{2\pi}{0.780} \approx 8.055 \text{ rad s}^{-1}\)

The maximum acceleration is:
\(a_{\text{max}} = \omega^2 A = (8.055)^2 \times 0.050 = 64.89 \times 0.050 = 3.24 \text{ m s}^{-2}\)

(ii) The maximum speed is:
\(v_{\text{max}} = \omega A = 8.055 \times 0.050 = 0.403 \text{ m s}^{-1}\)

(c) The kinetic energy is maximum when the mass passes through its equilibrium position (displacement \(x = 0\)).
The elastic potential energy is maximum at the points of maximum displacement (amplitude \(x = \pm 0.050 \text{ m}\)).

Marking scheme

(a)
- Recall/use of \(T = 2\pi \sqrt{\frac{m}{k}}\) [1 mark]
- Correct rearrangement to make \(k\) the subject: \(k = \frac{4\pi^2 m}{T^2}\) [1 mark]
- Calculation yielding \(22.7 \text{ N m}^{-1}\) (which rounds to \(23\)) [1 mark]

(b)(i)
- Use of \(\omega = \frac{2\pi}{T}\) to obtain \(8.06 \text{ rad s}^{-1}\) [1 mark]
- Use of \(a_{\text{max}} = \omega^2 A\) (or \(a_{\text{max}} = \frac{k}{m} A\)) [1 mark]
- Correct value of \(3.24 \text{ m s}^{-2}\) (accept range \(3.20 - 3.30\)) [1 mark]

(b)(ii)
- Use of \(v_{\text{max}} = \omega A\) [1 mark]
- Correct value of \(0.403 \text{ m s}^{-1}\) (accept range \(0.40 - 0.41\)) [1 mark]

(c)
- Kinetic energy is maximum at the equilibrium position / where displacement is zero [1 mark]
- Elastic potential energy is maximum at maximum displacement / at amplitude positions [1.625 marks]
Question 18 · Structured
10.625 marks
A steel wire of length \(2.20 \text{ m}\) and cross-sectional area \(1.50 \times 10^{-7} \text{ m}^2\) is suspended vertically. A mass of \(6.00 \text{ kg}\) is attached to its lower end.
The Young modulus of steel is \(2.00 \times 10^{11} \text{ Pa}\).

(a) Calculate the extension of the wire.

(b) Calculate the elastic potential energy stored in the wire, assuming it behaves elastically.

(c) Describe two practical steps a student could take to reduce experimental uncertainties when performing an experiment to determine the Young modulus of this wire.
Show answer & marking scheme

Worked solution

(a) The force acting on the wire is its weight:
\(F = m g = 6.00 \times 9.81 = 58.86 \text{ N}\)

Young modulus \(E\) is given by:
\(E = \frac{\text{Stress}}{\text{Strain}} = \frac{F / A}{x / L} = \frac{F L}{A x}\)

Rearranging for extension \(x\):
\(x = \frac{F L}{A E} = \frac{58.86 \times 2.20}{1.50 \times 10^{-7} \times 2.00 \times 10^{11}} = \frac{129.492}{30000} = 4.316 \times 10^{-3} \text{ m} \approx 4.32 \text{ mm}\)

(b) The elastic potential energy stored in the wire is:
\(E_{\text{p}} = \frac{1}{2} F x = \frac{1}{2} \times 58.86 \times 4.316 \times 10^{-3} \approx 0.127 \text{ J}\)

(c) To reduce uncertainties:
1. Use a micrometer screw gauge to measure the diameter of the wire at several different positions and orientations along its length, and calculate the mean to account for non-uniformity of cross-section.
2. Use a long wire (or a reference wire system like Searles apparatus) to ensure that the extension is large enough to be measured with low percentage uncertainty and to eliminate support flexure.

Marking scheme

(a)
- Correct calculation of tension force \(F = m g = 58.86 \text{ N}\) (accept \(58.9 \text{ N}\) or use of \(g=9.8 \text{ m s}^{-2}\)) [1 mark]
- Correct rearrangement of Young Modulus equation for extension: \(x = \frac{FL}{AE}\) [1 mark]
- Final answer: \(4.32 \times 10^{-3} \text{ m}\) (accept \(4.3 \text{ mm}\)) [1 mark]

(b)
- Recall/use of energy formula: \(E_p = \frac{1}{2} F x\) [1 mark]
- Substitution of tension force and extension values [1 mark]
- Final answer: \(0.127 \text{ J}\) (accept \(0.13 \text{ J}\)) [1 mark]

(c)
- Suggestion to measure diameter at multiple points/orientations [1 mark]
- Use of micrometer screw gauge and calculate average [1 mark]
- Suggestion of using a reference wire (e.g. Searles apparatus) to eliminate errors from support yielding, or using a long test wire to increase extension [2.625 marks]
Question 19 · Structured
10.625 marks
A main-sequence star has a surface temperature of \(5800 \text{ K}\) and a radius of \(7.00 \times 10^8 \text{ m}\).

(a) Use Wien's displacement law to calculate the peak wavelength \(\lambda_{\text{max}}\cap\) of the electromagnetic radiation emitted by the star. (Wien's constant \(= 2.90 \times 10^{-3} \text{ m K}\))

(b) Show that the luminosity of this star is approximately \(4.0 \times 10^{26} \text{ W}\).

(c) The radiant flux intensity (apparent brightness) of this star measured at the surface of an orbiting planet is \(1360 \text{ W m}^{-2}\). Calculate the distance from the centre of the star to the planet.
Show answer & marking scheme

Worked solution

(a) Wien's displacement law states:
\(\lambda_{\text{max}} T = 2.90 \times 10^{-3} \text{ m K}\)

\(\lambda_{\text{max}} = \frac{2.90 \times 10^{-3}}{5800} = 5.00 \times 10^{-7} \text{ m}\) (or \(500 \text{ nm}\))

(b) Stefan's law for luminosity \(L\):
\(L = 4 \pi r^2 \sigma T^4\)

Substitute the values:
\(L = 4 \pi \times (7.00 \times 10^8)^2 \times (5.67 \times 10^{-8}) \times 5800^4\)
\(L = 4 \pi \times (4.90 \times 10^{17}) \times (5.67 \times 10^{-8}) \times (1.1316 \times 10^{15})\)
\(L \approx 3.95 \times 10^{26} \text{ W}\), which is approximately \(4.0 \times 10^{26} \text{ W}\).

(c) Radiant flux intensity (apparent brightness) \(I\) is given by:
\(I = \frac{L}{4 \pi d^2}\)

Rearranging for distance \(d\):
\(d = \sqrt{\frac{L}{4 \pi I}}\)

\(d = \sqrt{\frac{3.953 \times 10^{26}}{4 \pi \times 1360}} = \sqrt{\frac{3.953 \times 10^{26}}{17090.3}} = \sqrt{2.313 \times 10^{22}} \approx 1.52 \times 10^{11} \text{ m}\)

Marking scheme

(a)
- State/use Wien's law formula: \(\lambda_{\text{max}} T = \text{constant}\) [1 mark]
- Correct calculation to give \(5.00 \times 10^{-7} \text{ m}\) (or \(500 \text{ nm}\)) [2 marks]

(b)
- State/use Stefan's law: \(L = 4\pi r^2 \sigma T^4\) [1 mark]
- Substitution of values into formula including \(\sigma = 5.67 \times 10^{-8}\) [1 mark]
- Correct calculation showing \(3.95 \times 10^{26} \text{ W}\) (matching the approximate value of \(4.0 \times 10^{26} \text{ W}\)) [1 mark]

(c)
- State/use equation relating intensity, luminosity, and distance: \(I = \frac{L}{4\pi d^2}\) [1 mark]
- Correct rearrangement: \(d = \sqrt{\frac{L}{4\pi I}}\) [1 mark]
- Substitution of values to find distance [1 mark]
- Final answer: \(1.52 \times 10^{11} \text{ m}\) (accept range \(1.50 \times 10^{11} \text{ m}\) to \(1.53 \times 10^{11} \text{ m}\)) [1.625 marks]
Question 20 · Structured
10.625 marks
A rescue helicopter of mass \(1600 \text{ kg}\) is ascending vertically.

(a) Draw a free-body diagram showing the forces acting on the helicopter when it is accelerating vertically upwards.

(b) The helicopter starts from rest and accelerates uniformly upwards to a speed of \(8.00 \text{ m s}^{-1}\) over a time of \(4.00 \text{ s}\). Calculate the magnitude of the upward lift force produced by the helicopter blades during this acceleration (assume air resistance is negligible).

(c) The helicopter later climbs at a constant vertical speed. At this speed, air resistance (drag) acting on the helicopter is given by \(F_{\text{drag}} = k v^2\), where \(k = 1.15 \text{ kg m}^{-1}\) and \(v\) is the speed.
Calculate the upward lift force required when the helicopter is climbing at a constant speed of \(30.0 \text{ m s}^{-1}\).
Show answer & marking scheme

Worked solution

(a) The free-body force diagram should show two vertical vectors acting on the helicopter:
1. An arrow pointing vertically upwards representing the Lift Force \(L\).
2. An arrow pointing vertically downwards representing the Weight \(W\).
Since the helicopter is accelerating upwards, the upward Lift arrow must be drawn longer than the downward Weight arrow.

(b) First, calculate the acceleration \(a\):
\(a = \frac{v - u}{t} = \frac{8.00 - 0}{4.00} = 2.00 \text{ m s}^{-2}\)

Using Newton's second law:
\(F_{\text{net}} = L - W = m a\)
\(L = m g + m a = m (g + a)\)
\(L = 1600 \times (9.81 + 2.00) = 1600 \times 11.81 = 18896 \text{ N} \approx 1.89 \times 10^4 \text{ N}\)

(c) When climbing at a constant speed of \(30.0 \text{ m s}^{-1}\), the acceleration is zero, so the net vertical force is zero.
\(F_{\text{net}} = L - W - F_{\text{drag}} = 0 \implies L = W + F_{\text{drag}}\)

First, calculate the drag force:
\(F_{\text{drag}} = k v^2 = 1.15 \times (30.0)^2 = 1.15 \times 900 = 1035 \text{ N}\)

Weight of the helicopter:
\(W = m g = 1600 \times 9.81 = 15696 \text{ N}\)

Therefore, the required lift force is:
\(L = 15696 + 1035 = 16731 \text{ N} \approx 1.67 \times 10^4 \text{ N}\)

Marking scheme

(a)
- Upward arrow labelled 'lift' or 'upthrust' and downward arrow labelled 'weight' or 'gravitational force' [1 mark]
- Upward arrow drawn visibly longer than the downward arrow [1 mark]

(b)
- Calculate acceleration: \(a = 2.00 \text{ m s}^{-2}\) [1 mark]
- Express Newton's second law: \(L - mg = ma\) [1 mark]
- Calculate lift force: \(1.89 \times 10^4 \text{ N}\) (accept \(1.88 \times 10^4 \text{ N}\) using \(g=9.8\)) [1 mark]

(c)
- Recognize that at constant speed, \(a=0\), so \(L = W + F_{\text{drag}}\) [1 mark]
- Correct calculation of drag force: \(F_{\text{drag}} = 1035 \text{ N}\) [1 mark]
- Correct calculation of weight: \(W = 15696 \text{ N}\) [1 mark]
- Final total lift force: \(1.67 \times 10^4 \text{ N}\) (accept range \(1.66 \times 10^4 \text{ N}\) to \(1.68 \times 10^4 \text{ N}\)) [2.625 marks]
Question 21 · Structured
10.625 marks
An electric kettle has a power rating of \(2.40 \text{ kW}\). It is filled with \(1.10 \text{ kg}\) of liquid water at an initial temperature of \(18.0^\circ\text{C}\).
(The specific heat capacity of water is \(4180 \text{ J kg}^{-1} \text{ K}^{-1}\). The specific latent heat of vaporisation of water is \(2.26 \times 10^6 \text{ J kg}^{-1}\).)

(a) Show that the minimum time required to heat the water to its boiling point of \(100.0^\circ\text{C}\) is approximately \(150 \text{ s}\).

(b) Once the water is boiling, the kettle continues to operate for a further \(90.0 \text{ s}\). Calculate the mass of water that is converted into steam during this time, assuming no energy is lost to the surroundings.

(c) Explain, in terms of intermolecular forces and the potential energy of the molecules, why the temperature of the water remains constant at \(100.0^\circ\text{C}\) while it is boiling.
Show answer & marking scheme

Worked solution

(a) Calculate the energy required to raise the temperature:
\(\Delta \theta = 100.0 - 18.0 = 82.0^\circ\text{C}\)
\(Q = m c \Delta \theta = 1.10 \times 4180 \times 82.0 = 377036 \text{ J}\)

Minimum time required:
\(t = \frac{Q}{P} = \frac{377036}{2400} \approx 157.1 \text{ s}\), which is approximately \(150 \text{ s}\) (more precisely \(1.6 \times 10^2 \text{ s}\)).

(b) Energy supplied in \(90.0 \text{ s}\):
\(Q_{\text{vap}} = P \times t = 2400 \times 90.0 = 216000 \text{ J}\)

Using \(Q = m L_{\text{v}}\):
\(m = \frac{Q_{\text{vap}}}{L_{\text{v}}} = \frac{216000}{2.26 \times 10^6} \approx 0.0956 \text{ kg}\)

(c) During boiling, the thermal energy supplied does not increase the kinetic energy of the molecules. Instead, the energy is used to break/overcome the strong intermolecular bonds (forces of attraction) holding the molecules in the liquid state. This increases the potential energy of the molecules as they separate. Since temperature depends only on the mean kinetic energy of the molecules, the temperature remains constant during this phase change.

Marking scheme

(a)
- Calculate temperature change \(\Delta \theta = 82 \text{ K}\) [1 mark]
- Apply heat formula: \(Q = mc\Delta\theta\) to find \(Q = 377000 \text{ J}\) [1 mark]
- Use of \(t = \frac{Q}{P}\) to obtain \(157 \text{ s}\) (showing it is close to \(150 \text{ s}\)) [1 mark]

(b)
- Calculate energy supplied during boiling: \(Q = Pt = 2400 \times 90 = 2.16 \times 10^5 \text{ J}\) [1 mark]
- State/use formula: \(Q = mL_v\) [1 mark]
- Correct rearrangement and calculation: \(m = \frac{2.16 \times 10^5}{2.26 \times 10^6} = 0.0956 \text{ kg}\) [2 marks]

(c)
- Supplied thermal energy goes into breaking/overcoming intermolecular bonds [1 mark]
- This results in an increase in the potential energy of the molecules [1 mark]
- Temperature is proportional to the mean kinetic energy of the molecules, which remains constant [1.625 marks]
Question 22 · Structured
10.625 marks
A capacitor of capacitance \(470 \
\mu\text{F}\) is fully charged to a potential difference of \(12.0 \text{ V}\). It is then connected across a \(15.0 \text{ k}\Omega\) resistor to discharge.

(a) Calculate the initial charge stored on the capacitor.

(b) Show that the time constant \(\tau\) of the discharge circuit is approximately \(7.1 \text{ s}\).

(c) Calculate the potential difference across the capacitor after discharging for \(10.0 \text{ s}\).

(d) Calculate the energy remaining in the capacitor after \(10.0 \text{ s}\).
Show answer & marking scheme

Worked solution

(a) Charge stored:
\(Q_0 = C V_0 = (470 \times 10^{-6} \text{ F}) \times 12.0 \text{ V} = 5.64 \times 10^{-3} \text{ C}\) (or \(5.64 \text{ mC}\))

(b) Time constant:
\(\tau = R C = (15.0 \times 10^3 \ \Omega) \times (470 \times 10^{-6} \text{ F}) = 7.05 \text{ s}\)
This is approximately \(7.1 \text{ s}\).

(c) Potential difference after time \(t = 10.0 \text{ s}\):
\(V = V_0 e^{-t / R C}\)
\(V = 12.0 \times e^{-10.0 / 7.05} = 12.0 \times e^{-1.4184} = 12.0 \times 0.2421 = 2.91 \text{ V}\)

(d) Energy remaining in the capacitor:
\(E = \frac{1}{2} C V^2\)
\(E = 0.5 \times (470 \times 10^{-6}) \times (2.905)^2 = 2.35 \times 10^{-4} \times 8.44 = 1.98 \times 10^{-3} \text{ J}\) (or \(1.98 \text{ mJ}\) / \(1.99 \text{ mJ}\) depending on rounding).

Marking scheme

(a)
- State/use: \(Q = CV\) [1 mark]
- Correct calculation of charge: \(5.64 \times 10^{-3} \text{ C}\) [1 mark]

(b)
- State/use: \(\tau = RC\) [1 mark]
- Substitute values: \(15.0 \times 10^3 \times 470 \times 10^{-6}\) to show \(7.05 \text{ s}\) [1 mark]

(c)
- State/use: \(V = V_0 e^{-t/RC}\) [1 mark]
- Substitute \(t = 10.0 \text{ s}\) and \(\tau = 7.05 \text{ s}\) [1 mark]
- Correct calculation: \(2.91 \text{ V}\) (accept range \(2.90 - 2.93 \text{ V}\)) [1 mark]

(d)
- State/use: \(E = \frac{1}{2} C V^2\) or \(E = E_0 e^{-2t/RC}\) [1 mark]
- Substitute correct potential difference (either from (c) or using exact expression) [1 mark]
- Correct calculation of energy: \(1.98 \times 10^{-3} \text{ J}\) to \(1.99 \times 10^{-3} \text{ J}\) [1.625 marks]
Question 23 · Structured
10.625 marks
Two parallel horizontal metal plates are placed in a vacuum, separated by a distance of \(2.50 \text{ cm}\). A potential difference of \(1.50 \text{ kV}\) is applied across the plates.

(a) Calculate the magnitude of the uniform electric field strength between the plates.

(b) An electron is released from rest from the negative plate.
(i) Calculate the electrostatic force acting on the electron.
(ii) Calculate the speed of the electron when it reaches the positive plate.

(c) Describe the path of a proton if it were projected horizontally midway between the plates with an initial speed of \(3.00 \times 10^5 \text{ m s}^{-1}\).
Show answer & marking scheme

Worked solution

(a) Electric field strength:
\(E = \frac{V}{d} = \frac{1500 \text{ V}}{0.0250 \text{ m}} = 6.00 \times 10^4 \text{ V m}^{-1}\) (or \(\text{N C}^{-1}\))

(b) (i) Electrostatic force on the electron:
\(F = e E = (1.60 \times 10^{-19} \text{ C}) \times (6.00 \times 10^4 \text{ V m}^{-1}) = 9.60 \times 10^{-15} \text{ N}\)

(ii) Work done by the field equals kinetic energy gained:
\(e V = \frac{1}{2} m_{\text{e}} v^2\)
\(v = \sqrt{\frac{2 e V}{m_{\text{e}}}} = \sqrt{\frac{2 \times 1.60 \times 10^{-19} \times 1500}{9.11 \times 10^{-31}}} = \sqrt{\frac{4.80 \times 10^{-16}}{9.11 \times 10^{-31}}} = \sqrt{5.269 \times 10^{14}} \approx 2.30 \times 10^7 \text{ m s}^{-1}\)

(c) The proton experiences a constant vertically downward electrostatic force (towards the negative plate). This causes a constant downward acceleration. Since its horizontal velocity remains constant, the proton will follow a parabolic path curving downwards.

Marking scheme

(a)
- State/use: \(E = \frac{V}{d}\) [1 mark]
- Correct calculation: \(6.00 \times 10^4 \text{ V m}^{-1}\) [1 mark]

(b)(i)
- State/use: \(F = q E\) [1 mark]
- Correct substitution of electron charge \(1.60 \times 10^{-19} \text{ C}\) [1 mark]
- Correct force calculation: \(9.60 \times 10^{-15} \text{ N}\) [1 mark]

(b)(ii)
- State/use conservation of energy: \(eV = \frac{1}{2} m v^2\) or equation of motion [1 mark]
- Rearrangement to find \(v\) [1 mark]
- Correct calculation: \(2.30 \times 10^7 \text{ m s}^{-1}\) (accept range \(2.29 \times 10^7 \text{ m s}^{-1}\) to \(2.31 \times 10^7 \text{ m s}^{-1}\)) [1 mark]

(c)
- Constant vertical force/acceleration downwards [1 mark]
- Constant horizontal velocity results in a parabolic trajectory downwards [1.625 marks]

Paper 2 (Exploring Physics)

Answer all questions in Section A (Multiple Choice) and Section B (Structured Questions).
24 Question · 99.95999999999998 marks
Question 1 · Multiple Choice
1 marks
A simple harmonic oscillator has a displacement described by \(x = A \cos(\omega t)\), where \(A\) is the amplitude. What is the ratio of the kinetic energy to the potential energy of the oscillator when the displacement is \(x = \frac{1}{3}A\)?
  1. A.\(1/8\)
  2. B.\(1/3\)
  3. C.\(3\)
  4. D.\(8\)
Show answer & marking scheme

Worked solution

The total energy of the oscillator is proportional to the square of the amplitude, \(E_{\text{total}} = \frac{1}{2} k A^2\). The potential energy at displacement \(x = \frac{1}{3}A\) is given by \(E_p = \frac{1}{2} k x^2 = \frac{1}{2} k \left(\frac{1}{3}A\right)^2 = \frac{1}{9} E_{\text{total}}\). The kinetic energy is therefore \(E_k = E_{\text{total}} - E_p = \frac{8}{9} E_{\text{total}}\). The ratio of kinetic energy to potential energy is \(\frac{E_k}{E_p} = \frac{8/9}{1/9} = 8\).

Marking scheme

Correct option D selected. [1 mark]
Question 2 · Multiple Choice
1 marks
The absolute temperature of an ideal gas is increased by \(21\%\) while its volume is halved by adjusting the pressure. What is the ratio of the new root-mean-square (r.m.s.) speed of the gas molecules to their initial r.m.s. speed?
  1. A.1.10
  2. B.1.21
  3. C.1.44
  4. D.2.20
Show answer & marking scheme

Worked solution

The root-mean-square speed of an ideal gas molecule is given by \(v_{\text{rms}} = \sqrt{\frac{3kT}{m}}\), where \(k\) is the Boltzmann constant, \(T\) is the absolute temperature, and \(m\) is the mass of a molecule. Thus, \(v_{\text{rms}} \propto \sqrt{T}\). Changes in volume and pressure do not alter this direct dependence as long as the temperature is specified. Since the absolute temperature increases by \(21\%\), the final temperature is \(1.21 T_{\text{initial}}\). Therefore, the ratio of the new r.m.s. speed to the initial r.m.s. speed is \(\sqrt{1.21} = 1.10\).

Marking scheme

Correct option A selected. [1 mark]
Question 3 · Multiple Choice
1 marks
A hypothetical unstable baryon \(X\) decays via the weak interaction into a \(\pi^+\) meson and a neutron. Given that \(X\) contains no strange, charm, top, or bottom quarks, what is the quark composition of \(X\)?
  1. A.uud
  2. B.udd
  3. C.u\bar{d}
  4. D.uuu
Show answer & marking scheme

Worked solution

A \(\pi^+\) meson has a charge of \(+1e\) and a baryon number of \(0\). A neutron (\(udd\)) has a charge of \(0\) and a baryon number of \(+1\). Since weak interactions conserve charge and baryon number, the parent particle \(X\) must have a charge of \(+1e\) and a baryon number of \(+1\) (indicating it is a baryon composed of three quarks). The quark combination \(uud\) (proton) has a charge of \(+2/3 + 2/3 - 1/3 = +1e\) and is a baryon. Thus, \(uud\) is the correct composition.

Marking scheme

Correct option A selected. [1 mark]
Question 4 · Multiple Choice
1 marks
A sample contains two radioactive nuclides, P and Q. Initially, the activity of P is twice the activity of Q. The half-life of P is \(3.0\text{ hours}\) and the half-life of Q is \(6.0\text{ hours}\). After what time interval will the activities of the two nuclides in the sample be equal?
  1. A.3.0 hours
  2. B.6.0 hours
  3. C.9.0 hours
  4. D.12 hours
Show answer & marking scheme

Worked solution

Let the initial activity of Q be \(A_0\), meaning the initial activity of P is \(2A_0\). At time \(t\), the activity of P is \(A_P(t) = 2A_0 \times 2^{-t/3.0}\) and the activity of Q is \(A_Q(t) = A_0 \times 2^{-t/6.0}\). Setting these equal: \(2A_0 \times 2^{-t/3.0} = A_0 \times 2^{-t/6.0} \implies 2 \times 2^{-t/3.0} = 2^{-t/6.0}\). Dividing both sides by \(2^{-t/3.0}\) gives \(2 = 2^{-t/6.0 + t/3.0} = 2^{t/6.0}\). This yields \(t/6.0 = 1\), which means \(t = 6.0\text{ hours}\).

Marking scheme

Correct option B selected. [1 mark]
Question 5 · Multiple Choice
1 marks
Two stars, Alpha and Beta, have the same surface temperature. The luminosity of star Alpha is \(1.6 \times 10^5\) times the luminosity of star Beta. What is the ratio of the radius of star Alpha to the radius of star Beta?
  1. A.400
  2. B.800
  3. C.1.6 \times 10^5
  4. D.2.56 \times 10^{10}
Show answer & marking scheme

Worked solution

According to the Stefan-Boltzmann law, the luminosity of a star is given by \(L = 4\pi R^2 \sigma T^4\). Since both stars have the same surface temperature \(T\), their luminosity is proportional to the square of their radius: \(L \propto R^2\). Thus, the ratio of the radii is the square root of the ratio of their luminosities: \(\frac{R_{\text{Alpha}}}{R_{\text{Beta}}} = \sqrt{1.6 \times 10^5} = \sqrt{160000} = 400\).

Marking scheme

Correct option A selected. [1 mark]
Question 6 · Multiple Choice
1 marks
In a double-slit interference experiment, monochromatic light of wavelength \(\lambda\) passes through two slits separated by distance \(d\), producing fringes of spacing \(x\) on a screen at distance \(D\). The experiment is altered so that the wavelength becomes \(1.2\lambda\), the slit separation is doubled, and the distance to the screen is halved. What is the new fringe spacing in terms of \(x\)?
  1. A.0.30x
  2. B.0.60x
  3. C.1.20x
  4. D.3.00x
Show answer & marking scheme

Worked solution

The fringe spacing is given by the formula \(x = \frac{\lambda D}{d}\). The new fringe spacing is \(x' = \frac{\lambda' D'}{d'} = \frac{(1.2\lambda)(0.5D)}{2d} = \frac{0.60}{2} \frac{\lambda D}{d} = 0.30x\).

Marking scheme

Correct option A selected. [1 mark]
Question 7 · Multiple Choice
1 marks
Which of the following statements correctly describes a key physical process occurring during a Positron Emission Tomography (PET) scan?
  1. A.Beta-minus particles emitted by a radioisotope tracer collide with orbital electrons, releasing a single high-energy X-ray photon.
  2. B.Positrons emitted by a radioisotope tracer annihilate with electrons in the patient's body, producing two gamma-ray photons travelling in opposite directions.
  3. C.High-frequency ultrasound pulses reflect at boundary interfaces between tissues with different acoustic impedances.
  4. D.A rotating X-ray tube emits a fan-shaped beam that is attenuated differently by various body tissues to reconstruct a 3D image.
Show answer & marking scheme

Worked solution

In a PET scan, a radioactive tracer that emits positrons is introduced into the patient. The emitted positrons travel a short distance before annihilating with electrons in the body's tissues. This annihilation process converts their mass-energy into two gamma-ray photons travelling in opposite directions, which are then detected by a ring of detectors to construct the image.

Marking scheme

Correct option B selected. [1 mark]
Question 8 · Multiple Choice
1 marks
A laser pointer emits a beam of monochromatic red light of wavelength \(633\text{ nm}\). The output power of the laser is \(5.0\text{ mW}\). How many photons are emitted by the laser per second?
  1. A.1.6 \times 10^{13}
  2. B.1.6 \times 10^{16}
  3. C.3.1 \times 10^{16}
  4. D.3.1 \times 10^{18}
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Worked solution

The energy of a single photon is given by \(E = \frac{hc}{\lambda} = \frac{(6.63 \times 10^{-34}\text{ J s}) \times (3.00 \times 10^8\text{ m s}^{-1})}{633 \times 10^{-9}\text{ m}} \approx 3.142 \times 10^{-19}\text{ J}\). The number of photons emitted per second \(N\) is the power divided by the photon energy: \(N = \frac{P}{E} = \frac{5.0 \times 10^{-3}\text{ W}}{3.142 \times 10^{-19}\text{ J}} \approx 1.59 \times 10^{16}\text{ s}^{-1}\). Rounding to two significant figures gives \(1.6 \times 10^{16}\text{ s}^{-1}\).

Marking scheme

Correct option B selected. [1 mark]
Question 9 · multiple_choice
1 marks
Laser A has a wavelength of 400 nm and a power of 12 mW. Laser B has a wavelength of 600 nm and a power of 18 mW. Both lasers emit monochromatic light. What is the ratio \(\frac{N_A}{N_B}\) of the number of photons emitted per second by Laser A to the number of photons emitted per second by Laser B?
  1. A.\(\frac{4}{9}\)
  2. B.\(\frac{2}{3}\)
  3. C.\(\frac{1}{1}\)
  4. D.\(\frac{9}{4}\)
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Worked solution

The power \(P\) of a laser is given by the total energy of the photons emitted per second: \(P = N E_{\text{photon}} = N \frac{hc}{\lambda}\) where \(N\) is the number of photons emitted per second. Rearranging for \(N\) gives \(N = \frac{P \lambda}{hc}\). Since \(h\) and \(c\) are constants, \(N \propto P \lambda\). The ratio is \(\frac{N_A}{N_B} = \frac{P_A \lambda_A}{P_B \lambda_B} = \frac{12 \times 10^{-3} \times 400 \times 10^{-9}}{18 \times 10^{-3} \times 600 \times 10^{-9}} = \frac{4800}{10800} = \frac{4}{9}\).

Marking scheme

1 mark: Correctly identifies that \(N \propto P \lambda\), substitutes values to obtain \(\frac{4}{9}\), and selects option A.
Question 10 · multiple_choice
1 marks
A student connects three identical capacitors, each of capacitance \(C\), to a constant potential difference \(V\). Two of the capacitors are connected in parallel, and this combination is connected in series with the third capacitor. What is the electrical energy stored in the third (series) capacitor?
  1. A.\(\frac{1}{9}CV^2\)
  2. B.\(\frac{2}{9}CV^2\)
  3. C.\(\frac{4}{9}CV^2\)
  4. D.\(\frac{1}{2}CV^2\)
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Worked solution

First, find the equivalent capacitance of the parallel combination: \(C_p = C + C = 2C\). This combination is in series with the third capacitor \(C_3 = C\). The total equivalent capacitance \(C_{\text{eq}}\) is: \(C_{\text{eq}} = \frac{C_p C_3}{C_p + C_3} = \frac{2C \times C}{2C + C} = \frac{2}{3}C\). The total charge drawn from the supply of potential difference \(V\) is: \(Q = C_{\text{eq}} V = \frac{2}{3}CV\). In a series circuit, the charge stored on the third capacitor is equal to the total charge: \(Q_3 = \frac{2}{3}CV\). The energy stored in the third capacitor is: \(E_3 = \frac{Q_3^2}{2C} = \frac{(\frac{2}{3}CV)^2}{2C} = \frac{2}{9}CV^2\).

Marking scheme

1 mark: Calculates total equivalent capacitance as \(\frac{2}{3}C\), charge as \(\frac{2}{3}CV\), and energy as \(\frac{2}{9}CV^2\) to select option B.
Question 11 · multiple_choice
1 marks
A parallel beam of X-rays is incident on a composite shield consisting of a 1.8 mm thick layer of material A followed by a 3.5 mm thick layer of material B. The linear attenuation coefficient of material A is 0.50 mm\(^{-1}\) and that of material B is 0.20 mm\(^{-1}\). What percentage of the initial intensity of the X-ray beam is transmitted through the composite shield?
  1. A.14\%
  2. B.20\%
  3. C.35\%
  4. D.80\%
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Worked solution

The intensity \(I\) of the X-ray beam after passing through the composite shield is: \(I = I_0 e^{-\mu_A x_A} e^{-\mu_B x_B} = I_0 e^{-(\mu_A x_A + \mu_B x_B)}\). Calculate the total exponent: \(\mu_A x_A + \mu_B x_B = (0.50 \times 1.8) + (0.20 \times 3.5) = 0.90 + 0.70 = 1.60\). The fraction of intensity transmitted is \(\frac{I}{I_0} = e^{-1.60} \approx 0.2019\). This corresponds to approximately 20\%.

Marking scheme

1 mark: Computes the sum of attenuation exponents as 1.60, finds the transmitted percentage as 20\%, and selects option B.
Question 12 · multiple_choice
1 marks
In a double-slit interference experiment, light of frequency \(f\) is incident on two slits separated by a distance \(d\). Fringes of width \(x\) are observed on a screen at a distance \(D\) from the slits. The experiment is modified so that the slit separation is halved, the screen distance is doubled, and the frequency of the light is doubled. What is the new fringe width?
  1. A.\(\frac{1}{2}x\)
  2. B.x
  3. C.2x
  4. D.4x
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Worked solution

The fringe width is given by \(x = \frac{\lambda D}{d}\). Since \(\lambda = \frac{c}{f}\), we can write \(x = \frac{c D}{f d}\). With the modifications, the new fringe width is \(x' = \frac{c (2D)}{(2f)(0.5d)} = 2 \frac{c D}{f d} = 2x\).

Marking scheme

1 mark: Expresses fringe width in terms of frequency, scales the variables appropriately to show that \(x' = 2x\), and selects option C.
Question 13 · multiple_choice
1 marks
Two parallel horizontal plates are separated by a distance \(d\) in a vacuum. A potential difference \(V\) is applied between them to produce a uniform vertical electric field. A small charged sphere of mass \(m\) is held in static equilibrium between the plates by the upward electric force and the downward gravitational force. The potential difference is then increased to 1.5 V and the plate separation is decreased to 0.75 d. What is the magnitude and direction of the initial acceleration of the sphere?
  1. A.0.50 g downwards
  2. B.0.50 g upwards
  3. C.1.0 g downwards
  4. D.1.0 g upwards
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Worked solution

Initially in equilibrium: \(q E = mg \implies q \frac{V}{d} = mg\) with the electric force directed upwards. With the changes, the new electric field strength is \(E' = \frac{1.5 V}{0.75 d} = 2 E\). The new upward force is \(F_E' = q E' = 2 q E = 2 mg\). The net vertical force is \(F_{\text{net}} = F_E' - mg = 2 mg - mg = mg\) upwards. Therefore, the acceleration is \(a = \frac{F_{\text{net}}}{m} = g\) upwards.

Marking scheme

1 mark: Computes the new field strength as \(2E\), determines the net upward force is \(mg\), calculates the acceleration as \(g\) upwards, and selects option D.
Question 14 · multiple_choice
1 marks
During the radioactive \(\beta^+\) decay of a nucleus, a proton decays into a neutron. Which row in the table correctly identifies the change in quark flavor, the exchange boson, and the leptons emitted in this process? Row A: Quark change d to u, Boson W-, Leptons e- and electron antineutrino. Row B: Quark change u to d, Boson W+, Leptons e+ and electron neutrino. Row C: Quark change u to d, Boson W-, Leptons e+ and electron antineutrino. Row D: Quark change d to u, Boson W+, Leptons e- and electron neutrino.
  1. A.Row A
  2. B.Row B
  3. C.Row C
  4. D.Row D
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Worked solution

In \(\beta^+\) decay, a proton decays into a neutron: \(p \rightarrow n + e^+ + \nu_e\). The proton consists of \(uud\) quarks and the neutron consists of \(udd\) quarks, so the quark change is \(u \rightarrow d\). To conserve charge at the vertex, the exchange boson must be \(W^+\). The emitted leptons are a positron \(e^+\) and an electron neutrino \(\nu_e\). This matches Row B.

Marking scheme

1 mark: Identifies the quark change as \(u \rightarrow d\), exchange boson as \(W^+\), and leptons as \(e^+\) and \(\nu_e\), selecting Row B (option B).
Question 15 · multiple_choice
1 marks
A uniform metal wire of length \(L\) and resistance \(R\) is stretched such that its length increases by 10\%. The volume and density of the metal remain constant during stretching. What is the new resistance of the wire?
  1. A.1.10 R
  2. B.1.21 R
  3. C.0.90 R
  4. D.0.83 R
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Worked solution

The resistance is \(R = \rho \frac{L}{A}\). Since the volume \(V_{\text{vol}} = A L\) is constant, we can write \(A = \frac{V_{\text{vol}}}{L}\), leading to \(R = \rho \frac{L^2}{V_{\text{vol}}}\). Thus, \(R \propto L^2\). When the length is increased by 10\%, the new length is \(L' = 1.10 L\). The new resistance is \(R' \propto (1.10 L)^2 = 1.21 L^2\), which means \(R' = 1.21 R\).

Marking scheme

1 mark: Recognizes that for constant volume \(R \propto L^2\), calculates the multiplier as \(1.10^2 = 1.21\), and selects option B.
Question 16 · Structured
9.44 marks
A container of volume 0.045 \text{ m}^3 contains helium-4 gas (molar mass 4.0 \text{ g mol}^{-1}) at a pressure of 1.2 \times 10^5 \text{ Pa} and temperature of 27 \, ^{\circ}\text{C}.

(a) Calculate the initial amount of helium gas in moles. [3]
(b) The container is connected via a valve of negligible volume to another evacuated container of volume 0.015 \text{ m}^3. The valve is opened and the system reaches a new thermal equilibrium at 42 \, ^{\circ}\text{C}. Calculate the final pressure of the gas. [3]
(c) Calculate the root-mean-square (r.m.s.) speed of the helium atoms at the final temperature. [3.44]
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Worked solution

(a) Convert temperature to Kelvin: \( T_1 = 27 + 273.15 = 300.15 \text{ K} \) (accept \( 300 \text{ K} \)). Using the ideal gas equation: \( P_1 V_1 = n R T_1 \) so \( n = \frac{1.2 \times 10^5 \times 0.045}{8.31 \times 300} = 2.166 \approx 2.17 \text{ moles} \).
(b) The total volume is now \( V_2 = 0.045 + 0.015 = 0.060 \text{ m}^3 \). The final temperature is \( T_2 = 42 + 273.15 = 315.15 \text{ K} \) (accept \( 315 \text{ K} \)). Using the ideal gas equation: \( P_2 = \frac{n R T_2}{V_2} = \frac{2.166 \times 8.31 \times 315}{0.060} = 9.45 \times 10^4 \text{ Pa} \) (or \( 9.5 \times 10^4 \text{ Pa} \)).
(c) The molar mass in kilograms is \( M = 4.0 \times 10^{-3} \text{ kg mol}^{-1} \). The root-mean-square speed is given by \( v_{\text{rms}} = \sqrt{\frac{3 R T}{M}} = \sqrt{\frac{3 \times 8.31 \times 315}{4.0 \times 10^{-3}}} = \sqrt{1.963 \times 10^6} = 1.40 \times 10^3 \text{ m s}^{-1} \).

Marking scheme

(a)
- M1: Conversion of 27 \, ^{\circ}\text{C} to 300 K.
- M1: Substitution of values into \( n = \frac{PV}{RT} \).
- A1: Correct calculation of moles as 2.17 (or 2.16) moles.

(b)
- M1: Identification of final volume as \( 0.060 \text{ m}^3 \).
- M1: Use of \( \frac{P_1 V_1}{T_1} = \frac{P_2 V_2}{T_2} \) or \( P_2 = \frac{n R T_2}{V_2} \).
- A1: Correct value of \( 9.45 \times 10^4 \text{ Pa} \) (accept \( 9.5 \times 10^4 \text{ Pa} \)).

(c)
- M1: Use of \( v_{\text{rms}} = \sqrt{\frac{3 R T}{M}} \) or \( \frac{1}{2} m v^2 = \frac{3}{2} k T \).
- M1: Conversion of molar mass to \( 4.0 \times 10^{-3} \text{ kg mol}^{-1} \).
- A1.44: Correct calculation of speed as \( 1.40 \times 10^3 \text{ m s}^{-1} \) (accept \( 1.4 \times 10^3 \text{ m s}^{-1} \)).
Question 17 · Structured
9.44 marks
Two vertical springs, A and B, are suspended from a rigid ceiling. Spring A has stiffness \( k_1 = 150 \text{ N m}^{-1} \) and spring B has stiffness \( k_2 = 300 \text{ N m}^{-1} \). They are connected in series, and a mass of 2.5 kg is suspended from the bottom of the combination.

(a) Show that the effective spring constant of the series combination is \( 100 \text{ N m}^{-1} \). [2]
(b) Calculate the total elastic potential energy stored in the two springs when the mass is in equilibrium. [4]
(c) Determine the ratio of the elastic energy stored in Spring A to that in Spring B. [3.44]
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Worked solution

(a) For a series connection, the effective stiffness \( k_s \) is given by: \( \frac{1}{k_s} = \frac{1}{k_1} + \frac{1}{k_2} = \frac{1}{150} + \frac{1}{300} = \frac{3}{300} = \frac{1}{100} \). Therefore, \( k_s = 100 \text{ N m}^{-1} \) (shown).
(b) The tension in the springs at equilibrium is equal to the weight: \( F = m g = 2.5 \times 9.81 = 24.525 \text{ N} \). Total extension of the combination: \( x = \frac{F}{k_s} = \frac{24.525}{100} = 0.24525 \text{ m} \). The total elastic potential energy is \( E_p = \frac{1}{2} F x = \frac{1}{2} \times 24.525 \times 0.24525 = 3.01 \text{ J} \) (or using \( E_p = \frac{F^2}{2 k_s} = 3.01 \text{ J} \)).
(c) Since they are connected in series, the tension (force \( F \)) in both springs is the same. The energy stored in each spring is given by \( E = \frac{F^2}{2 k} \). Therefore: \( \frac{E_A}{E_B} = \frac{F^2 / (2 k_1)}{F^2 / (2 k_2)} = \frac{k_2}{k_1} = \frac{300}{150} = 2.0 \).

Marking scheme

(a)
- M1: Use of formula \( \frac{1}{k_s} = \frac{1}{k_1} + \frac{1}{k_2} \).
- A1: Correct working leading to exactly 100 \text{ N m}^{-1}.

(b)
- M1: Calculation of weight \( W = 2.5 \times 9.81 = 24.5 \text{ N} \) (or 25 N using g=10).
- M1: Calculation of total extension \( x = 0.245 \text{ m} \).
- M1: Use of \( E_p = \frac{1}{2} k x^2 \) or \( E_p = \frac{1}{2} F x \).
- A1: Final answer of \( 3.01 \text{ J} \) (accept \( 3.0 \text{ J} \) or \( 3.1 \text{ J} \) if g=10 is used).

(c)
- M1: Recognition that the tension/force is the same in both series springs.
- M1: Use of \( E \propto \frac{1}{k} \) or individual energy calculations (\( E_A = 2.0 \text{ J} \), \( E_B = 1.0 \text{ J} \)).
- A1.44: Correct ratio of 2.0.
Question 18 · Structured
9.44 marks
A star has a peak emission wavelength of 410 nm. Its luminosity is measured to be \( 4.5 \times 10^{27} \text{ W} \).

(a) State Wien's displacement law and use it to calculate the surface temperature of this star. [3]
(b) Calculate the radius of the star. [4]
(c) The star is located at a distance of \( 1.2 \times 10^{18} \text{ m} \) from Earth. Calculate the radiant flux intensity (apparent brightness) of the star at Earth. [2.44]
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Worked solution

(a) Wien's displacement law states that the peak emission wavelength \( \lambda_{\text{max}} \) is inversely proportional to the absolute temperature \( T \) of the black body: \( \lambda_{\text{max}} T = \text{constant} \approx 2.90 \times 10^{-3} \text{ m K} \). Therefore: \( T = \frac{2.90 \times 10^{-3}}{410 \times 10^{-9}} = 7073 \approx 7070 \text{ K} \).
(b) From Stefan's Law: \( L = 4 \pi r^2 \sigma T^4 \). Rearranging for radius \( r \): \( r = \sqrt{\frac{L}{4 \pi \sigma T^4}} = \sqrt{\frac{4.5 \times 10^{27}}{4 \pi \times 5.67 \times 10^{-8} \times (7073)^4}} = \sqrt{\frac{4.5 \times 10^{27}}{1.783 \times 10^9}} = 1.59 \times 10^9 \text{ m} \).
(c) The radiant flux intensity \( F \) is: \( F = \frac{L}{4 \pi d^2} = \frac{4.5 \times 10^{27}}{4 \pi \times (1.2 \times 10^{18})^2} = \frac{4.5 \times 10^{27}}{1.81 \times 10^{37}} = 2.49 \times 10^{-10} \text{ W m}^{-2} \).

Marking scheme

(a)
- M1: State that peak wavelength is inversely proportional to absolute temperature.
- M1: Set up \( T = \frac{\text{constant}}{\lambda} \).
- A1: Final temperature of \( 7070 \text{ K} \) (or \( 7100 \text{ K} \) or \( 7050 \text{ K} \) depending on the value of constant used).

(b)
- M1: Recall Stefan-Boltzmann law formula: \( L = 4 \pi r^2 \sigma T^4 \).
- M1: Correct rearrangement for \( r \).
- M1: Substitute values correctly (including Stefan constant \( 5.67 \times 10^{-8} \)).
- A1: Correct calculation of radius \( r = 1.59 \times 10^9 \text{ m} \) (accept \( 1.58 \times 10^9 \) to \( 1.61 \times 10^9 \)).

(c)
- M1: Recall and use \( F = \frac{L}{4 \pi d^2} \).
- A1.44: Correct calculation of radiant flux intensity \( F = 2.49 \times 10^{-10} \text{ W m}^{-2} \) (accept \( 2.5 \times 10^{-10} \)).
Question 19 · Structured
9.44 marks
A block of mass 4.0 kg is released from rest on a rough plane inclined at \( 30^{\circ} \) to the horizontal. The coefficient of friction between the block and the plane is 0.25.

(a) Show that the magnitude of the frictional force acting on the block as it slides is approximately 8.5 N. [3]
(b) Calculate the acceleration of the block down the incline. [3.44]
(c) Calculate the velocity of the block after it has slid a distance of 1.5 m along the plane. [3]
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Worked solution

(a) The normal reaction force \( R \) is given by: \( R = m g \cos(30^{\circ}) = 4.0 \times 9.81 \times \cos(30^{\circ}) = 33.98 \text{ N} \). Frictional force: \( F_f = \mu R = 0.25 \times 33.98 = 8.495 \approx 8.5 \text{ N} \) (shown).
(b) The component of the gravitational force pulling the block down the incline is: \( F_d = m g \sin(30^{\circ}) = 4.0 \times 9.81 \times 0.5 = 19.62 \text{ N} \). The net force acting down the plane is: \( F_{\text{net}} = F_d - F_f = 19.62 - 8.495 = 11.125 \text{ N} \). The acceleration is: \( a = \frac{F_{\text{net}}}{m} = \frac{11.125}{4.0} = 2.78 \text{ m s}^{-2} \).
(c) Using equations of motion with constant acceleration: \( v^2 = u^2 + 2 a s \). Since the block starts from rest, \( u = 0 \): \( v^2 = 0 + 2 \times 2.781 \times 1.5 = 8.343 \implies v = \sqrt{8.343} = 2.89 \text{ m s}^{-1} \).

Marking scheme

(a)
- M1: Use of \( R = m g \cos(\theta) \).
- M1: Use of \( F_f = \mu R \).
- A1: Correct calculation leading to \( 8.495 \text{ N} \) which rounds to \( 8.5 \text{ N} \).

(b)
- M1: Calculation of parallel component of gravity \( F_d = m g \sin(30^{\circ}) = 19.6 \text{ N} \).
- M1: Use of \( F_{\text{net}} = m a \) to set up equation \( m g \sin(30^{\circ}) - F_f = m a \).
- A1.44: Correct calculation of acceleration as \( 2.78 \text{ m s}^{-2} \) (or \( 2.8 \text{ m s}^{-2} \)).

(c)
- M1: Select appropriate kinematic equation \( v^2 = u^2 + 2as \).
- M1: Correct substitution of values with \( u = 0 \).
- A1: Correct final velocity as \( 2.89 \text{ m s}^{-1} \) (or \( 2.9 \text{ m s}^{-1} \)).
Question 20 · Structured
9.44 marks
A small probe of mass 0.12 kg on a vibration test-bed performs horizontal simple harmonic oscillations with a frequency of 25 Hz. The maximum acceleration of the probe during the motion is \( 180 \text{ m s}^{-2} \).

(a) Determine the amplitude of the oscillations. [3]
(b) Calculate the maximum speed of the probe. [3]
(c) Calculate the magnitude of the restoring force acting on the probe when it is at a displacement of 1.5 mm from the equilibrium position. [3.44]
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Worked solution

(a) The angular frequency is: \( \omega = 2 \pi f = 2 \pi \times 25 = 50\pi \approx 157.1 \text{ rad s}^{-1} \). The maximum acceleration is related to amplitude by: \( a_{\text{max}} = \omega^2 A \implies A = \frac{180}{(157.08)^2} = 7.30 \times 10^{-3} \text{ m} \) (or 7.3 mm).
(b) The maximum speed is given by: \( v_{\text{max}} = \omega A = 157.08 \times 7.295 \times 10^{-3} = 1.15 \text{ m s}^{-1} \).
(c) The restoring force magnitude is: \( F = m a = m \omega^2 x \). Converting displacement to meters: \( x = 1.5 \times 10^{-3} \text{ m} \). Hence: \( F = 0.12 \times (157.08)^2 \times 1.5 \times 10^{-3} = 4.44 \text{ N} \).

Marking scheme

(a)
- M1: Correct calculation of \( \omega = 2\pi f \approx 157 \text{ rad s}^{-1} \).
- M1: State and rearrange \( a_{\text{max}} = \omega^2 A \).
- A1: Correct amplitude as \( 7.30 \times 10^{-3} \text{ m} \) (or \( 7.3 \text{ mm} \)).

(b)
- M1: Use of \( v_{\text{max}} = \omega A \) or \( v_{\text{max}} = \sqrt{a_{\text{max}} A} \).
- M1: Correct substitution of values.
- A1: Correct calculation of maximum speed as \( 1.15 \text{ m s}^{-1} \).

(c)
- M1: Recognition that \( F = m \omega^2 x \) or \( a = \omega^2 x \).
- M1: Correct substitution of \( x = 1.5 \times 10^{-3} \text{ m} \).
- A1.44: Correct force magnitude of \( 4.44 \text{ N} \) (accept \( 4.4 \text{ N} \)).
Question 21 · Structured
9.44 marks
A block of ice of mass 0.45 kg at \( -15 \, ^{\circ}\text{C} \) is placed in a well-insulated container. Steam at \( 100 \, ^{\circ}\text{C} \) is passed into the container until all the ice is just melted and the entire mixture reaches a final temperature of \( 0 \, ^{\circ}\text{C} \).

Specific heat capacity of ice = \( 2100 \text{ J kg}^{-1} \text{ K}^{-1} \)
Specific latent heat of fusion of ice = \( 3.34 \times 10^{5} \text{ J kg}^{-1} \)
Specific latent heat of vaporisation of water = \( 2.26 \times 10^{6} \text{ J kg}^{-1} \)
Specific heat capacity of water = \( 4180 \text{ J kg}^{-1} \text{ K}^{-1} \)

(a) Calculate the total thermal energy required to heat the ice from \( -15 \, ^{\circ}\text{C} \) and completely melt it to water at \( 0 \, ^{\circ}\text{C} \). [4]
(b) Explain the difference between specific heat capacity and specific latent heat in terms of spacing and energy of the molecules. [2]
(c) Calculate the mass of steam at \( 100 \, ^{\circ}\text{C} \) required to achieve this. [3.44]
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Worked solution

(a) The process consists of two stages:
1. Heating the ice to \( 0 \, ^{\circ}\text{C} \): \( Q_1 = m_i c_i \Delta T = 0.45 \times 2100 \times 15 = 14175 \text{ J} \).
2. Melting the ice to water: \( Q_2 = m_i L_f = 0.45 \times (3.34 \times 10^5) = 150300 \text{ J} \).
Total thermal energy required: \( Q_{\text{total}} = 14175 + 150300 = 164475 \text{ J} \approx 1.64 \times 10^5 \text{ J} \).
(b) Specific heat capacity is the energy required to change temperature, increasing the average kinetic energy of the molecules (vibrations) without changing state or potential energy. Specific latent heat is the energy required to change the state at constant temperature, breaking bonds (increasing potential energy and separation) without changing kinetic energy.
(c) Thermal energy released by the condensing steam and subsequent cooling of the condensed water to \( 0 \, ^{\circ}\text{C} \):
\( Q_{\text{released}} = m_s L_v + m_s c_w \Delta T_w = m_s \times (2.26 \times 10^6) + m_s \times 4180 \times 100 \)
\( Q_{\text{released}} = m_s (2.26 \times 10^6 + 4.18 \times 10^5) = m_s \times 2.678 \times 10^6 \text{ J} \).
Using conservation of energy: \( m_s \times 2.678 \times 10^6 = 164475 \implies m_s = 0.0614 \text{ kg} \) (or 61.4 g).

Marking scheme

(a)
- M1: Use of \( Q = mc\Delta T \) for heating ice.
- M1: Use of \( Q = mL_f \) for melting ice.
- M1: Correct addition of both energy components.
- A1: Correct final energy as \( 1.64 \times 10^5 \text{ J} \) (accept \( 1.6 \times 10^5 \text{ J} \)).

(b)
- B1: Specific heat capacity associated with changes in kinetic energy of molecules (temperature change).
- B1: Specific latent heat associated with breaking molecular bonds / changes in potential energy of molecules (state change).

(c)
- M1: Expression for steam condensation: \( m L_v \).
- M1: Expression for hot water cooling: \( m c \Delta T \).
- M1: Setting heat gained equal to heat lost.
- A1.44: Correct mass calculation to give \( 0.0614 \text{ kg} \) (or \( 6.14 \times 10^{-2} \text{ kg} \)).
Question 22 · Structured
9.44 marks
A stationary free neutron undergoes beta-minus (\( \beta^{-} \)) decay.

(a) Write the full nuclear equation for this decay. [3]
(b) Describe this decay in terms of quarks, showing how charge is conserved. [3]
(c) In a particular decay, the emitted electron has a kinetic energy of \( 5.2 \times 10^{-14} \text{ J} \). Calculate the de Broglie wavelength of this electron. [3.44]
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Worked solution

(a) The nuclear equation is: \( {}_0^1\text{n} \rightarrow {}_1^1\text{p} + {}_{-1}^{\phantom{-}0}\text{e} + \bar{\nu}_e \) (accept \( \text{n} \rightarrow \text{p} + \text{e}^- + \bar{\nu}_e \)).
(b) In terms of quarks, a down quark decays into an up quark: \( \text{d} \rightarrow \text{u} + \text{e}^- + \bar{\nu}_e \). On the left-hand side, the charge of the down quark is \( -1/3 \, e \). On the right-hand side, the total charge is: \( +2/3 \, e \text{ (up quark)} + (-1 \, e \text{ (electron)}) + 0 \text{ (antineutrino)} = -1/3 \, e \). Thus, charge is conserved.
(c) The momentum \( p \) of the electron is related to its kinetic energy \( E_k \) by: \( E_k = \frac{p^2}{2m} \implies p = \sqrt{2 m E_k} = \sqrt{2 \times 9.11 \times 10^{-31} \times 5.2 \times 10^{-14}} = 3.078 \times 10^{-22} \text{ kg m s}^{-1} \). The de Broglie wavelength is: \( \lambda = \frac{h}{p} = \frac{6.63 \times 10^{-34}}{3.078 \times 10^{-22}} = 2.15 \times 10^{-12} \text{ m} \).

Marking scheme

(a)
- M1: Neutron on LHS, proton and electron on RHS.
- M1: Electron antineutrino on RHS (with bar over nu).
- A1: Balance of nucleon and proton numbers shown correctly.

(b)
- M1: State quark change as \( \text{d} \rightarrow \text{u} \).
- M1: Identify charges of down quark (\( -1/3 \, e \)) and up quark (\( +2/3 \, e \)).
- A1: Show sum of charges on RHS is \( +2/3 - 1 = -1/3 \, e \), balancing the LHS.

(c)
- M1: Use of \( p = \sqrt{2 m E_k} \) or calculate velocity first using \( E_k = \frac{1}{2} m v^2 \).
- M1: Use of de Broglie equation \( \lambda = \frac{h}{p} \).
- A1.44: Correct calculation of wavelength as \( 2.15 \times 10^{-12} \text{ m} \) (accept \( 2.2 \times 10^{-12} \text{ m} \)).
Question 23 · Structured
9.44 marks
In a double-slit experiment, red light of wavelength 650 nm is incident on two slits separated by a distance d. The interference pattern is observed on a screen placed 1.8 m from the slits. The distance from the central bright fringe to the 5th bright fringe is 12.5 mm.

(a) Determine the fringe spacing x of the interference pattern. [2]
(b) Calculate the slit separation d. [4]
(c) The red light source is replaced with blue light of wavelength 450 nm. State and explain how the appearance of the fringes changes, and calculate the new distance between the central fringe and the 5th bright fringe. [3.44]
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Worked solution

(a) The distance from the central bright fringe to the 5th bright fringe is equal to 5 fringe widths (\( 5x \)). Hence: \( x = \frac{12.5 \text{ mm}}{5} = 2.5 \text{ mm} = 2.5 \times 10^{-3} \text{ m} \).
(b) Using the double-slit equation \( \lambda = \frac{a x}{D} \) (where slit separation \( a = d \)): \( d = \frac{\lambda D}{x} = \frac{650 \times 10^{-9} \times 1.8}{2.5 \times 10^{-3}} = 4.68 \times 10^{-4} \text{ m} \) (or \( 0.47 \text{ mm} \)).
(c) Since wavelength decreases (from 650 nm to 450 nm), the fringe spacing decreases, so the fringes become narrower and closer together. The new fringe spacing is: \( x_{\text{new}} = \frac{\lambda_{\text{new}} D}{d} = \frac{450 \times 10^{-9} \times 1.8}{4.68 \times 10^{-4}} = 1.73 \times 10^{-3} \text{ m} \). The distance to the 5th bright fringe is: \( 5 \times x_{\text{new}} = 5 \times 1.73 \times 10^{-3} = 8.65 \times 10^{-3} \text{ m} \) (or 8.65 mm).

Marking scheme

(a)
- M1: State that the distance is 5 fringe spacings.
- A1: Correctly calculate \( x = 2.5 \text{ mm} \).

(b)
- M1: Recall \( \lambda = \frac{a x}{D} \).
- M1: Correct rearrangement for slit separation \( d = a \).
- M1: Correct substitution of values with consistent units.
- A1: Final answer of \( 4.68 \times 10^{-4} \text{ m} \) (or \( 4.7 \times 10^{-4} \text{ m} \)).

(c)
- B1: State that fringes become closer together/narrower because wavelength decreases.
- M1: Set up calculation for new spacing or use ratio method (e.g., \( 12.5 \times \frac{450}{650} \)).
- A1.44: Correct calculation of the 5th fringe distance as \( 8.65 \text{ mm} \) (accept \( 8.6 \text{ mm} \) or \( 8.7 \text{ mm} \)).
Question 24 · structured
9.44 marks
An astronomer is analysing the electromagnetic spectrum of a distant star, catalogued as Star-X9. (a) The peak wavelength of the electromagnetic radiation emitted from the star's surface is determined to be \(\lambda_{\text{max}} = 3.80 \times 10^{-7}\text{ m}\). Calculate the surface temperature \(T\) of Star-X9. (b) The radius of Star-X9 is estimated to be \(1.40 \times 10^9\text{ m}\). Calculate the luminosity \(L\) of the star. (c) The intensity of the radiation received from Star-X9 at a detector on Earth is \(1.65 \times 10^{-11}\text{ W m}^{-2}\). Calculate the distance from Earth to Star-X9 in light-years (ly), where \(1\text{ ly} = 9.46 \times 10^{15}\text{ m}\).
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Worked solution

Part (a): Wien's displacement law states that \(\lambda_{\text{max}} T = 2.90 \times 10^{-3}\text{ m K}\). Rearranging for \(T\): \(T = \frac{2.90 \times 10^{-3}}{3.80 \times 10^{-7}} = 7631.6\text{ K}\), which rounds to \(7.63 \times 10^3\text{ K}\) or \(7630\text{ K}\). Part (b): Stefan's law for stellar luminosity is \(L = 4 \pi R^2 \sigma T^4\). Substituting the radius \(R = 1.40 \times 10^9\text{ m}\), Stefan's constant \(\sigma = 5.67 \times 10^{-8}\text{ W m}^{-2}\text{ K}^{-4}\), and the temperature \(T = 7632\text{ K}\): \(L = 4 \pi (1.40 \times 10^9)^2 \times (5.67 \times 10^{-8}) \times (7632)^4 = 4.74 \times 10^{27}\text{ W}\). Part (c): The intensity of the radiation at a distance \(d\) is given by the inverse square law: \(I = \frac{L}{4 \pi d^2}\). Rearranging for \(d\): \(d = \sqrt{\frac{L}{4 \pi I}} = \sqrt{\frac{4.74 \times 10^{27}}{4 \pi \times 1.65 \times 10^{-11}}} = \sqrt{2.286 \times 10^{37}} = 4.78 \times 10^{18}\text{ m}\). To convert this distance to light-years: \(d = \frac{4.78 \times 10^{18}\text{ m}}{9.46 \times 10^{15}\text{ m ly}^{-1}} = 505\text{ ly}\).

Marking scheme

Part (a) [2 marks]:
- C1: Wien's law formula used correctly: \(T = \frac{2.90 \times 10^{-3}}{\lambda_{\text{max}}}\)
- A1: Correct calculation of temperature, \(7.6 \times 10^3\text{ K}\) or \(7630\text{ K}\) (allow 7600 to 7640 K).

Part (b) [3 marks]:
- C1: Recall and use of Stefan's law formula: \(L = 4 \pi R^2 \sigma T^4\)
- C1: Correct substitution of values including \(R^2\) and \(T^4\)
- A1: Final answer for luminosity of \(4.7 \times 10^{27}\text{ W}\) to \(4.8 \times 10^{27}\text{ W}\) (value dependent on rounding in part a).

Part (c) [4 marks]:
- C1: Recall and use of inverse square law: \(I = \frac{L}{4 \pi d^2}\)
- C1: Correct rearrangement for distance: \(d = \sqrt{\frac{L}{4 \pi I}}\)
- C1: Correct conversion from metres to light-years by dividing by \(9.46 \times 10^{15}\)
- A1: Correct final distance in light-years: 500 to 510 ly (allow ecf from part b).

Paper 3 (Unified Physics)

Answer all structured and synoptic questions.
6 Question · 70.02 marks
Question 1 · structured
11.67 marks
(a) Define the *time constant* of a discharging capacitor circuit. [1]

(b) A capacitor of capacitance \(C = 470\ \mu\text{F}\) is charged to an initial potential difference \(V_0\) and then discharged through a resistor of resistance \(R\). The time taken for the potential difference across the capacitor to fall to \(25\%\) of its initial value is \(8.2\ \text{s}\).
Calculate:
(i) the time constant \(\tau\) of the circuit. [3]
(ii) the resistance \(R\). [2]

(c) The amplitude of a damped simple pendulum decays exponentially over time according to the relation \(A = A_0 e^{-\gamma t}\), where \(\gamma\) is the decay constant. In a particular experiment, the decay constant \(\gamma\) is equal to the reciprocal of the time constant \(\tau\) calculated in (b)(i).
(i) Show that the unit of \(\gamma\) is \(\text{s}^{-1}\). [2]
(ii) Calculate the time taken for the pendulum's amplitude to fall to \(10\%\) of its initial value. [4]
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Worked solution

(a) By definition, the time constant \(\tau = RC\) is the time taken for the charge, potential difference, or current in a discharging capacitor circuit to fall to \(1/e \approx 36.8\%\) of its initial value.

(b)(i) Using the capacitor discharge equation:
\(V = V_0 e^{-t/\tau}\)
Given \(V / V_0 = 0.25\) at \(t = 8.2\ \text{s}\):
\(0.25 = e^{-8.2/\tau}\)
Taking the natural logarithm of both sides:
\(\ln(0.25) = -\frac{8.2}{\tau}\)
\(-1.3863 = -\frac{8.2}{\tau}\)
\(\tau = \frac{8.2}{1.3863} = 5.915\ \text{s} \approx 5.9\ \text{s}\).

(b)(ii) Using \(\tau = RC\):
\(R = \frac{\tau}{C} = \frac{5.915}{470 \times 10^{-6}} = 12585\ \Omega \approx 1.3 \times 10^4\ \Omega\).

(c)(i) The exponent \(\gamma t\) must be a dimensionless quantity (having no units).
Therefore, \([\gamma] \times [t] = 1 \implies [\gamma] = \text{s}^{-1}\).
Alternatively, since \(\gamma = 1/\tau\) and the unit of \(\tau\) is seconds (\(\text{s}\)), the unit of \(\gamma\) must be \(\text{s}^{-1}\).

(c)(ii) We are given \(\gamma = \frac{1}{\tau} = \frac{1}{5.915\ \text{s}} = 0.1691\ \text{s}^{-1}\).
To find the time \(t\) for the amplitude \(A\) to decay to \(10\%\) of its initial value \(A_0\):
\(A = A_0 e^{-\gamma t} \implies 0.10 = e^{-0.1691 t}\)
\(\ln(0.10) = -0.1691 t\)
\(-2.3026 = -0.1691 t\)
\(t = \frac{2.3026}{0.1691} = 13.62\ \text{s} \approx 14\ \text{s}\) (or \(13.6\ \text{s}\)).

Marking scheme

(a) B1: Time taken for the potential difference/charge/current of a discharging capacitor to fall to 1/e (approx. 37%) of its initial value.
(b)(i)
C1: Recalls and uses V = V_0 * e^(-t / tau) or equivalent log form.
C1: Correctly substitutes 0.25 and 8.2 s into the equation.
A1: tau = 5.9 s (accept 5.92 s).
(b)(ii)
C1: Recalls and uses R = tau / C.
A1: R = 1.3 x 10^4 ohms (allow ecf from b(i)).
(c)(i)
B1: States that the exponential argument gamma * t must be dimensionless (or states gamma = 1 / tau).
B1: Shows unit of gamma = s^(-1).
(c)(ii)
C1: Calculates gamma = 0.169 s^(-1) (allow ecf from b(i)).
C1: Sets up the equation 0.10 = e^(-gamma * t).
C1: Rearranges to t = -ln(0.10) / gamma.
A1: t = 14 s (or 13.6 s).
Question 2 · structured
11.67 marks
A spacecraft of mass \(m = 320\ \text{kg}\) is placed into a stable circular orbit around Mars.

(a) State Kepler's third law of planetary motion. [1]

(b) The radius of Mars is \(3.39 \times 10^6\ \text{m}\) and its mass is \(6.42 \times 10^{23}\ \text{kg}\).
The spacecraft orbits at a height of \(2.10 \times 10^6\ \text{m}\) above the surface of Mars.
(i) Show that the orbital speed \(v\) of the spacecraft is approximately \(2.8 \times 10^3\ \text{m s}^{-1}\). [3]
(ii) Calculate the period \(T\) of the orbit in hours. [3]
(iii) Calculate the gravitational potential energy of the spacecraft in this orbit. [2]

(c) To escape Mars' gravitational field completely from this orbit, the spacecraft must be given additional kinetic energy. Explain, with a calculation, the minimum change in speed \(\Delta v\) required to escape. [3]
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Worked solution

(a) Kepler's third law states that the square of the orbital period \(T\) of a body in orbit is directly proportional to the cube of its orbital radius \(r\) (i.e., \(T^2 \propto r^3\)).

(b)(i) The total orbital radius \(r\) of the spacecraft is the sum of the radius of Mars \(R_{\text{Mars}}\) and its height \(h\) above the surface:
\(r = R_{\text{Mars}} + h = 3.39 \times 10^6\ \text{m} + 2.10 \times 10^6\ \text{m} = 5.49 \times 10^6\ \text{m}\).
The gravitational force provides the centripetal force:
\(\frac{G M m}{r^2} = \frac{m v^2}{r} \implies v = \sqrt{\frac{G M}{r}}\)
\(v = \sqrt{\frac{6.67 \times 10^{-11} \times 6.42 \times 10^{23}}{5.49 \times 10^6}}\)
\(v = \sqrt{7.7998 \times 10^6} = 2.7928 \times 10^3\ \text{m s}^{-1} \approx 2.8 \times 10^3\ \text{m s}^{-1}\).

(b)(ii) The orbital speed is given by \(v = \frac{2\pi r}{T}\). Rearranging for the period \(T\):
\(T = \frac{2\pi r}{v} = \frac{2\pi \times 5.49 \times 10^6}{2792.8} = 12351\ \text{s}\).
To express this in hours:
\(T = \frac{12351}{3600} = 3.43\ \text{hours}\).

(b)(iii) The gravitational potential energy is:
\(E_p = -\frac{G M m}{r} = -\frac{6.67 \times 10^{-11} \times 6.42 \times 10^{23} \times 320}{5.49 \times 10^6} = -2.494 \times 10^9\ \text{J} \approx -2.49 \times 10^9\ \text{J}\).

(c) To escape the gravitational field of Mars completely, the spacecraft's total mechanical energy must be at least zero (\(E_{\text{total}} \ge 0\)).
The minimum escape velocity \(v_{\text{esc}}\) is given by:
\(\frac{1}{2} m v_{\text{esc}}^2 - \frac{G M m}{r} = 0 \implies v_{\text{esc}} = \sqrt{\frac{2 G M}{r}} = \sqrt{2} v\)
\(v_{\text{esc}} = \sqrt{2} \times 2792.8\ \text{m s}^{-1} = 3949.6\ \text{m s}^{-1}\).
The minimum change in speed \(\Delta v\) required is:
\(\Delta v = v_{\text{esc}} - v = 3949.6 - 2792.8 = 1156.8\ \text{m s}^{-1} \approx 1.16 \times 10^3\ \text{m s}^{-1}\) (or \(1.16\ \text{km s}^{-1}\)).

Marking scheme

(a) B1: Period squared is proportional to orbital radius cubed (T^2 proportional to r^3).
(b)(i)
C1: Calculates total orbital radius r = 5.49 x 10^6 m.
C1: Equates gravitational force to centripetal force and obtains v = sqrt(GM/r).
A1: Shows value evaluates to 2.79 x 10^3 m/s.
(b)(ii)
C1: Uses T = 2 * pi * r / v.
C1: Divides seconds by 3600 to convert to hours.
A1: T = 3.43 hours (accept 3.4 hours).
(b)(iii)
C1: Uses E_p = -G M m / r.
A1: E_p = -2.49 x 10^9 J (ignore sign if only magnitude is given, but accept fully correct signed value).
(c)
C1: Explains that total mechanical energy must equal zero to escape (or uses escape speed formula v_esc = sqrt(2GM/r)).
C1: Calculates escape speed v_esc = 3.95 x 10^3 m/s (or states v_esc = sqrt(2) * v).
A1: Delta v = 1.16 x 10^3 m/s (or 1.16 km/s).
Question 3 · structured
11.67 marks
An aluminum cylinder of mass \(0.45\ \text{kg}\) contains \(0.082\ \text{mol}\) of an ideal gas.

(a) State two assumptions of the kinetic theory of gases. [2]

(b) Initially, the gas and the cylinder are in thermal equilibrium at a temperature of \(20\ ^∘\text{C}\).
The gas occupies a volume of \(2.0 \times 10^{-3}\ \text{m}^3\).
(i) Show that the initial pressure of the gas is approximately \(1.0 \times 10^5\ \text{Pa}\). [2]
(ii) The gas is now compressed rapidly to a volume of \(5.0 \times 10^{-4}\ \text{m}^3\). During this rapid compression, no thermal energy is transferred to the cylinder, and the pressure rises to \(6.1 \times 10^5\ \text{Pa}\).
Calculate the new temperature of the gas in \(^∘\text{C}\). [3]

(c) After compression, the gas is allowed to cool back to the room temperature of \(20\ ^∘\text{C}\) by transferring thermal energy to the aluminum cylinder.
The specific heat capacity of aluminum is \(900\ \text{J kg}^{-1}\ \text{K}^{-1}\).
(i) Calculate the thermal energy lost by the gas as it cools back to \(20\ ^∘\text{C}\). You may assume the internal energy of \(n\) moles of an ideal gas is given by \(U = \frac{3}{2} n R T\). [3]
(ii) Calculate the temperature rise of the aluminum cylinder, assuming all the heat lost by the gas is absorbed by the cylinder and there are no external heat losses. [2]
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Worked solution

(a) Standard assumptions include: (1) The gas contains a very large number of molecules in rapid, random motion. (2) The volume of the gas molecules is negligible compared to the volume of the container. (3) Collisions between molecules and the container walls are perfectly elastic. (4) The duration of collisions is negligible compared to the time between collisions. (5) Intermolecular forces are negligible except during collisions.

(b)(i) Converting initial temperature to Kelvin:
\(T_1 = 20 + 273.15 = 293.15\ \text{K}\).
Using the ideal gas equation \(p V = n R T\):
\(p_1 = \frac{n R T_1}{V_1} = \frac{0.082 \times 8.31 \times 293.15}{2.0 \times 10^{-3}} = 99879\ \text{Pa} \approx 1.0 \times 10^5\ \text{Pa}\).

(b)(ii) Using the ideal gas equation for state 2:
\(p_2 V_2 = n R T_2 \implies T_2 = \frac{p_2 V_2}{n R}\)
\(T_2 = \frac{6.1 \times 10^5 \times 5.0 \times 10^{-4}}{0.082 \times 8.31} = \frac{305}{0.68142} = 447.59\ \text{K}\).
Converting to Celsius:
\(\theta_2 = 447.59 - 273.15 = 174.44\ ^∘\text{C} \approx 174\ ^∘\text{C}\).

(c)(i) The thermal energy lost by the gas is equal to its change in internal energy as it cools:
\(\Delta U = \frac{3}{2} n R \Delta T\)
where \(\Delta T = T_2 - T_1 = 447.59 - 293.15 = 154.44\ \text{K}\).
\(\Delta U = 1.5 \times 0.082 \times 8.31 \times 154.44 = 157.86\ \text{J} \approx 158\ \text{J}\).

(c)(ii) Using \(Q = m c \Delta T_{\text{cyl}}\) for the aluminum container:
\(\Delta T_{\text{cyl}} = \frac{Q}{m c} = \frac{157.86}{0.45 \times 900} = \frac{157.86}{405} = 0.390\ \text{K}\) (or \(^∘\text{C}\)).

Marking scheme

(a) B1, B1: Any two standard ideal gas assumptions stated clearly.
(b)(i)
C1: Converts temperature to Kelvin (293 K).
A1: Rearranges ideal gas law and shows calculation yielding approx. 1.0 x 10^5 Pa.
(b)(ii)
C1: Recalls and uses p_1*V_1/T_1 = p_2*V_2/T_2 or p_2*V_2 = n*R*T_2.
C1: Calculates T_2 = 448 K.
A1: theta_2 = 174 °C.
(c)(i)
C1: Recalls and uses Delta U = 3/2 * n * R * Delta T.
C1: Identifies temperature change Delta T = 154 K.
A1: Delta U = 158 J (accept 157.9 J).
(c)(ii)
C1: Uses Q = m * c * Delta T.
A1: Delta T = 0.39 K (or °C) (allow ecf from c(i)).
Question 4 · structured
11.67 marks
A small, negatively charged oil drop of mass \(m = 4.2 \times 10^{-14}\ \text{kg}\) carries a charge of \(q = -2.4 \times 10^{-18}\ \text{C}\). It enters the horizontal space between two parallel plates with a horizontal velocity \(u = 0.85\ \text{m s}^{-1}\). The plates are separated by a distance \(d = 12\ \text{mm}\) and have a potential difference \(V = 1.8\ \text{kV}\) across them, with the upper plate being positive.

(a) Draw a labeled diagram showing the vertical forces acting on the oil drop while it is between the plates. [2]

(b)(i) Show that the electric force acting on the oil drop is about \(3.6 \times 10^{-13}\ \text{N}\). [2]
(ii) Calculate the net vertical acceleration of the oil drop. State whether it accelerates upwards or downwards. [3]

(c) The plates have a length of \(5.0\ \text{cm}\).
(i) Calculate the time the oil drop spends between the plates. [2]
(ii) Determine the vertical displacement of the oil drop by the time it exits the plates. [3]
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Worked solution

(a) The diagram must depict the oil drop with two opposite vertical force vectors:
1. An upward electric force vector, \(F_E\), because the negative charge is attracted towards the positive upper plate.
2. A downward gravitational force vector (weight), \(W = mg\).

(b)(i) The magnitude of the electric field \(E\) between the parallel plates is:
\(E = \frac{V}{d} = \frac{1800\ \text{V}}{12 \times 10^{-3}\ \text{m}} = 1.50 \times 10^5\ \text{V m}^{-1}\).
The electric force \(F_E\) is given by:
\(F_E = q E = (2.4 \times 10^{-18}\ \text{C}) \times (1.50 \times 10^5\ \text{V m}^{-1}) = 3.60 \times 10^{-13}\ \text{N}\).

(b)(ii) The gravitational force (weight) acting on the oil drop is:
\(W = m g = (4.2 \times 10^{-14}\ \text{kg}) \times 9.81\ \text{m s}^{-2} = 4.12 \times 10^{-13}\ \text{N}\).
Since \(W > F_E\), the net vertical force acts downwards:
\(F_{\text{net}} = W - F_E = 4.12 \times 10^{-13}\ \text{N} - 3.60 \times 10^{-13}\ \text{N} = 5.20 \times 10^{-14}\ \text{N}\).
The net vertical acceleration is:
\(a = \frac{F_{\text{net}}}{m} = \frac{5.20 \times 10^{-14}\ \text{N}}{4.2 \times 10^{-14}\ \text{kg}} = 1.238\ \text{m s}^{-2} \approx 1.24\ \text{m s}^{-2}\) downwards.

(c)(i) The horizontal motion of the oil drop has a constant velocity \(u = 0.85\ \text{m s}^{-1}\):
\(t = \frac{L}{u} = \frac{0.050\ \text{m}}{0.85\ \text{m s}^{-1}} = 0.0588\ \text{s} \approx 0.059\ \text{s}\).

(c)(ii) The vertical displacement \(s\) can be found using the equations of motion for constant acceleration:
\(s = \frac{1}{2} a t^2 = 0.5 \times 1.238\ \text{m s}^{-2} \times (0.0588\ \text{s})^2 = 2.14 \times 10^{-3}\ \text{m}\) (or \(2.1\ \text{mm}\)).

Marking scheme

(a)
B1: Draws a diagram with a vertical upward force labeled electric force (or F_E).
B1: Draws a downward force labeled weight (or W or gravitational force / mg).
(b)(i)
C1: Recalls and uses E = V / d to find E = 1.5 x 10^5 V/m.
A1: Shows F_E = q * E evaluates to 3.6 x 10^-13 N.
(b)(ii)
C1: Calculates weight W = mg = 4.12 x 10^-13 N.
C1: Subtracts forces to find F_net = 5.2 x 10^-14 N.
A1: Acceleration a = 1.2 m/s^2 (or 1.24 m/s^2) and specifies direction as downwards.
(c)(i)
C1: Recalls and uses t = distance / horizontal speed.
A1: t = 0.059 s (or 0.0588 s).
(c)(ii)
C1: Uses s = 1/2 * a * t^2.
C1: Substitutes values of a and t (allow ecf from previous parts).
A1: s = 2.1 x 10^-3 m (or 2.1 mm).
Question 5 · structured
11.67 marks
A light spring has an unstretched length of \(0.25\ \text{m}\). A mass of \(0.60\ \text{kg}\) is attached to the lower end, and the system is allowed to come to rest at its equilibrium position where the spring's length is now \(0.38\ \text{m}\).

(a) Show that the spring constant \(k\) of the spring is approximately \(45\ \text{N m}^{-1}\). [2]

(b) The mass is pulled down vertically a further \(4.0\ \text{cm}\) from equilibrium and released from rest to perform simple harmonic oscillations.
(i) Explain why the motion of the mass is simple harmonic. [2]
(ii) Calculate the period \(T\) of the oscillations. [3]
(iii) Calculate the maximum velocity of the mass during its oscillation. [2]

(c) Calculate the change in total potential energy (gravitational plus elastic) of the spring-mass system when the mass is moved from its equilibrium position to its lowest point. [3]
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Worked solution

(a) The extension \(x_0\) of the spring when the mass is in equilibrium is:
\(x_0 = 0.38\ \text{m} - 0.25\ \text{m} = 0.13\ \text{m}\).
At equilibrium, the upward tension equals the downward gravitational force:
\(k x_0 = m g \implies k = \frac{m g}{x_0}\)
\(k = \frac{0.60\ \text{kg} \times 9.81\ \text{m s}^{-2}}{0.13\ \text{m}} = 45.28\ \text{N m}^{-1} \approx 45\ \text{N m}^{-1}\).

(b)(i) According to Hooke's law, the tension is proportional to the extension. When displaced from equilibrium by a distance \(y\), the net restoring force is \(F = m g - k(x_0 + y) = -k y\). Because the restoring force is directly proportional to the displacement and is directed towards the equilibrium position, the motion is simple harmonic.

(b)(ii) The period \(T\) of oscillation for a mass-spring system is:
\(T = 2\pi \sqrt{\frac{m}{k}} = 2\pi \sqrt{\frac{0.60\ \text{kg}}{45.28\ \text{N m}^{-1}}} = 0.723\ \text{s} \approx 0.72\ \text{s}\).

(b)(iii) The maximum velocity is given by \(v_{\max} = \omega A\).
The angular frequency is:
\(\omega = \sqrt{\frac{k}{m}} = \sqrt{\frac{45.28}{0.60}} = 8.687\ \text{rad s}^{-1}\).
The amplitude of the oscillation is \(A = 4.0\ \text{cm} = 0.040\ \text{m}\).
\(v_{\max} = 8.687\ \text{rad s}^{-1} \times 0.040\ \text{m} = 0.347\ \text{m s}^{-1} \approx 0.35\ \text{m s}^{-1}\).

(c) Relative to the equilibrium position:
When the mass is at its lowest point, it has been displaced downward by \(y = -0.040\ \text{m}\).
The change in gravitational potential energy is:
\(\Delta E_g = m g y = 0.60 \times 9.81 \times (-0.040) = -0.2354\ \text{J}\).
The change in elastic potential energy is:
\(\Delta E_e = \frac{1}{2} k (x_0 + A)^2 - \frac{1}{2} k x_0^2\)
\(\Delta E_e = 0.5 \times 45.28 \times (0.13 + 0.04)^2 - 0.5 \times 45.28 \times (0.13)^2\)
\(\Delta E_e = 22.64 \times [0.0289 - 0.0169] = 22.64 \times 0.0120 = 0.2717\ \text{J}\).
The total potential energy change of the system is:
\(\Delta E_{\text{pot}} = \Delta E_g + \Delta E_e = -0.2354\ \text{J} + 0.2717\ \text{J} = 0.0363\ \text{J} \approx 0.036\ \text{J}\).
(Alternatively, using the SHM potential energy formula, \(\Delta E_{\text{pot}} = \frac{1}{2} k A^2 = 0.5 \times 45.28 \times (0.040)^2 = 0.0362\ \text{J}\).)

Marking scheme

(a)
C1: Finds extension x_0 = 0.13 m.
A1: Shows calculation of k = mg/x_0 = 45.3 N/m (approximating to 45 N/m).
(b)(i)
B1: States that the net restoring force is proportional to displacement from equilibrium.
B1: States that the force/acceleration is always directed towards the equilibrium position.
(b)(ii)
C1: Recalls T = 2 * pi * sqrt(m / k).
C1: Substitutes mass and spring constant correctly.
A1: T = 0.72 s.
(b)(iii)
C1: Uses v_max = omega * A.
A1: v_max = 0.35 m/s (accept 0.347 m/s).
(c)
C1: Calculates change in GPE = -0.235 J OR states total potential energy change is 1/2 * k * A^2.
C1: Calculates change in elastic energy = 0.272 J OR substitutes correctly into 1/2 * k * A^2.
A1: Total potential energy change = 0.036 J (accept 0.0362 J).
Question 6 · structured
11.67 marks
Vega is a bright star in the northern constellation of Lyra. It has a surface temperature of \(9600\ \text{K}\).

(a) Calculate the wavelength \(\lambda_{\max}\) at which Vega emits its maximum intensity of electromagnetic radiation. [2]

(b) The radius of Vega is \(1.6 \times 10^9\ \text{m}\).
(i) Show that the luminosity \(L\) of Vega is approximately \(1.5 \times 10^{28}\ \text{W}\). [3]
(ii) The distance from Earth to Vega is \(2.37 \times 10^{17}\ \text{m}\).
Calculate the radiant flux intensity (radiation intensity) of Vega at the Earth's atmosphere. [3]

(c) Light from Vega is analyzed in a laboratory using a diffraction grating. The grating has 600 lines per millimeter.
Calculate the angle of the second-order maximum for the wavelength \(\lambda_{\max}\) calculated in part (a). [4]
Show answer & marking scheme

Worked solution

(a) Wien's displacement law relates the surface temperature to peak emission wavelength:
\(\lambda_{\max} T = 2.90 \times 10^{-3}\ \text{m K}\)
\(\lambda_{\max} = \frac{2.90 \times 10^{-3}}{9600} = 3.02 \times 10^{-7}\ \text{m} \approx 3.0 \times 10^{-7}\ \text{m}\) (or \(302\ \text{nm}\)).

(b)(i) According to the Stefan-Boltzmann law:
\(L = 4 \pi R^2 \sigma T^4\)
Substituting the values:
\(L = 4 \pi \times (1.6 \times 10^9\ \text{m})^2 \times (5.67 \times 10^{-8}\ \text{W m}^{-2}\ \text{K}^{-4}) \times (9600\ \text{K})^4\)
\(L = 4 \pi \times (2.56 \times 10^{18}) \times (5.67 \times 10^{-8}) \times (8.4935 \times 10^{15})\)
\(L = 1.549 \times 10^{28}\ \text{W} \approx 1.5 \times 10^{28}\ \text{W}\).

(b)(ii) The radiant flux intensity (intensity at Earth) is given by:
\(I = \frac{L}{4 \pi d^2}\)
\(I = \frac{1.549 \times 10^{28}\ \text{W}}{4 \pi \times (2.37 \times 10^{17}\ \text{m})^2} = \frac{1.549 \times 10^{28}}{7.0583 \times 10^{35}} = 2.195 \times 10^{-8}\ \text{W m}^{-2} \approx 2.2 \times 10^{-8}\ \text{W m}^{-2}\).

(c) First, find the grating spacing \(d_{\text{slit}}\):
\(d_{\text{slit}} = \frac{1.0 \times 10^{-3}\ \text{m}}{600} = 1.667 \times 10^{-6}\ \text{m}\).
Using the diffraction grating equation:
\(d_{\text{slit}} \sin\theta = n \lambda\)
For the second-order maximum (\(n = 2\)) and \(\lambda_{\max} = 3.02 \times 10^{-7}\ \text{m}\):
\(\sin\theta = \frac{2 \times 3.02 \times 10^{-7}\ \text{m}}{1.667 \times 10^{-6}\ \text{m}} = 0.3623\)
\ heta = \sin^{-1}(0.3623) = 21.2^\circ \approx 21^\circ\ (or \(0.37\ \text{rad}\)).

Marking scheme

(a)
C1: Recalls Wien's displacement law expression.
A1: Wavelength = 3.0 x 10^-7 m (or 302 nm).
(b)(i)
C1: Recalls Stefan's law formula.
C1: Substitutes correct value of Stefan-Boltzmann constant (5.67 x 10^-8).
A1: Shows clear working leading to L = 1.5 x 10^28 W.
(b)(ii)
C1: Recalls the inverse-square law for intensity, I = L / (4 * pi * d^2).
C1: Correctly substitutes distance d into the formula.
A1: Intensity = 2.2 x 10^-8 W/m^2.
(c)
C1: Calculates grating spacing d_slit = 1.67 x 10^-6 m.
C1: Recalls d_slit * sin(theta) = n * lambda.
C1: Substitutes n = 2 and wavelength from (a).
A1: Angle theta = 21° (allow ecf from (a)).

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