Syllabus Edition

First teaching 2023

First exams 2025

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Practice Paper 2 (HL IB Physics)

Practice Paper Questions

1a
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2 marks

Naomi stands on the edge of a vertical cliff and throws a stone vertically upwards.

q2a_motion_sl-ib-physics-sq-medium

The stone leaves her hand with a speed of 20 m s–1 at the instant her hand is 73 m above the surface of the sea. Air resistance is negligible.

Calculate the maximum height reached by the stone as measured from the point it was thrown.

1b
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3 marks

Determine the time taken for the stone to pass by the point from which it was released.

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2a
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3 marks

State and explain one piece of experimental evidence that supports the theory of special relativity.

2b
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2 marks

Muons are unstable particles that are created in the Earth's upper atmosphere. Muons have an average half-life of 1.49 µs as measured from the reference frame where the muon is at rest. Muons travel at a speed of 0.987c towards the surface of the Earth relative to Earth. 

A detector positioned at 5196 m above the surface of the Earth detects muons at a rate of 3.2 × 104 per hour.

A second detector is positioned at ground level.

Calculate the half-life of the muons as measured by an observer on Earth.

2c
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1 mark

Calculate the distance between the detectors as measured from the reference frame of the muon.

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3a
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3 marks

The diagram represents a stationary wave formed on a violin string fixed at P and Q when it is plucked at its centre. X is a point on the string at maximum displacement.

q4a_standing-waves_sl-ib-physics-sq-medium

Explain why a stationary wave is formed on the string.  

3b
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3 marks

The stationary wave formed represents the "A" string of a violin which has a frequency of 440 Hz. 

Calculate the time taken for the string at point X to move from maximum displacement to its next maximum displacement.

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4a
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2 marks

The distance from the Earth to the Sun is 1.5 × 1011 m. The mass of the Earth is 6 × 1024 kg and the mass of the Sun is 3.3 × 105  times the mass of the Earth.

Estimate the gravitational force between the Sun and the Earth.

4b
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1 mark

Mars is 1.5 times further away from the Sun than the Earth and is 10 times lighter than Earth.

Predict the gravitational force between Mars and the Sun.

4c
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2 marks

Determine the acceleration of free fall on a planet 20 times as massive as the Earth and with a radius 10 times larger.

4d
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3 marks

Calculate the orbital speed of the Earth around the Sun.

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5a
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3 marks

A magnet is dropped through a vertical solenoid.

ib-sq-11-1-hard-q4a_1

On the axes provided sketch a graph of the expected e.m.f. as time progresses.

ib-sq-11-1-hard-q4a_2
5b
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3 marks

Explain the shape of the graph from part (a).

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6a
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2 marks

The radioactive isotope uranium−238 decays in a decay series to the stable lead−206. 

The half−life of U presubscript 92 presuperscript 238 is 4.5 × 109 years, which is much larger than all the other half−lives of the decays in the series.

A rock sample, when formed originally, contained 6.0 × 1022 atoms of U presubscript 92 presuperscript 238 and no Pb presubscript 82 presuperscript 206 atoms. At any given time, most of the atoms are either straight U presubscript 92 presuperscript 238 or Pb presubscript 82 presuperscript 206 with a negligible number of atoms in other forms in the decay series.

Sketch on the axes below the variation of number of U presubscript 92 presuperscript 238 atoms and the number of Pb presubscript 82 presuperscript 206 atoms in the rock sample as they vary over a period of 1.0 × 1010 years from its formation. Label your graphs U and Pb.

7-1-ib-sl-hard-sqs-q4a-question

6b
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2 marks

A certain time, t, after its formation, the sample contained twice as many U presubscript 92 presuperscript 238 atoms as Pb presubscript 82 presuperscript 206 atoms. 

Show that the number of straight U presubscript 92 presuperscript 238 atoms in the rock sample at time t was 4.0 × 1022.

6c
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2 marks

The ratio of the number of lead nuclei N subscript P b end subscript to the number of uranium nuclei N subscript U at some time t is given by: 

N subscript P b end subscript over N subscript U equals e to the power of lambda t end exponent minus 1

λ is the decay constant and has a value of 1.54 × 10−10 years.

Calculate the time taken (in years) for there to be twice as many straight U presubscript 92 presuperscript 238 atoms as Pb presubscript 82 presuperscript 206 atoms.

6d
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4 marks

Lead−214 is an unstable isotope of lead−206. It decays by emitting a beta to the power of minus particle to form bismuth−214 (Bi) 

Bismuth is also unstable and has two decay modes: 

  • Emitting an α particle to form thallium−210 (Tl) + energy
  • Emitting a β particle to form polonium−214 (Po) + energy

Write decay equations for the decay chain of lead−214 to thallium−210 and to polonium−214. Comment on the nature of the energy released. 

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7a
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1 mark

The Sun emits radiation with a peak emission occurring at a wavelength of 5.2 × 10−7 m.

Show that the Sun has a surface temperature of about 6000 K.

7b
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2 marks

The average intensity of radiation received from the Sun at the surface of the Earth is 1370 W m−2

Show that the Sun's luminosity is about 4 × 1026 W.

Mean distance between the Sun and the Earth = 1.49 × 1011 m

7c
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3 marks

Use the Stefan-Boltzmann law to determine the radius of the Sun.

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8
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3 marks

An idealised refrigerator cycle is shown on the pressure-volume diagram below.

thermodynamics-4d-m-ib-physics

(i)
Draw arrows on the diagram to show the direction of the cycle.
[1]
(ii)
Explain why this direction of the cycle allows heat to be removed from a cold region.
[2]

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9a
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3 marks

An experiment to determine the charge of an electron is shown.   

ib-sl-5-1-sq-4a-question

Oil drops are sprayed into a chamber above two parallel metal plates which are separated by a distance d. The oil drops become charged before entering the region between the plates.

A potential difference V is applied between the plates.

(i)
Explain why the oil drops become charged.
[1]
(ii)
Draw the electric field lines between the plates.
[2]

ib-practice-paper-2-set-a-question-9a

9b
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4 marks

An oil drop is observed to be stationary between the plates when the potential difference is V subscript 1. When the potential difference is increased to V subscript 2, the drop is observed to move upwards with a constant velocity v.

(i)
State the sign of the charge on the oil drop.
[1]
(ii)
Draw the forces acting on the oil drop when V space equals space V subscript 1 and when V space equals space V subscript 2.
[3]

ib-practice-paper-2-set-a-question-9b

9c
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3 marks

Show that the electric charge on the oil drop is given by

q space equals space fraction numerator 6 straight pi eta r v d over denominator V subscript 2 minus V subscript 1 end fraction

where eta is the viscosity of air and r is the radius of the oil drop.

9d
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4 marks

The following measurements are made for the oil drop:

V subscript 1 space equals space 115 space straight V

V subscript 2 space equals space 715 space straight V

v space equals space 0.220 space mm space straight s to the power of negative 1 end exponent

r space equals space 1.29 space straight mu straight m

The viscosity of air between the plates is eta space equals space 1.8 cross times 10 to the power of negative 5 end exponent space Pa space straight s and the separation of the plates is d space equals space 6.0 space mm.

Deduce, using the equation in part (c), whether the value of the charge for the oil drop is consistent with the currently accepted value of the elementary charge.

9e
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4 marks

The voltage supply connected to the parallel plates is switched off. The oil drop falls with a constant velocity v subscript 0.

Show that v subscript 0 over v is about 0.2.

9f
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2 marks

The oil drop collides with another oil drop of charge +14e, where e is the elementary charge.

Deduce the net charge on each oil drop after the collision.

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10a
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4 marks

The Bohr model was developed in order to explain the atomic spectrum of hydrogen.

Outline the Bohr model and give a limitation of it.

10b
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3 marks

Bohr modified the Rutherford model by introducing the condition: 

m v r space equals space n fraction numerator h over denominator 2 straight pi end fraction

Outline the reason for this modification.

10c
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4 marks

The Bohr model for hydrogen can also be applied to a helium atom which has lost one of its electrons through ionisation.

The one remaining electron has a mass of m and moves in a circular orbit of radius r. Deduce an expression for

(i)
the kinetic energy E subscript k of the electron
[2]
(ii)
the electric potential energy E subscript p
[1]
(iii)
the total energy E subscript T of the atom
[1]
10d
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2 marks

Using your answer to (c), describe the predicted effect on the orbital radius of the electron when it

(i)
absorbs an electromagnetic wave
[1]
(ii)
emits an electromagnetic wave.
[1]
10e
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3 marks

The radius of the electron's orbit in the helium atom is 2.43 × 10−10 m.

Determine the principal quantum number of the energy level occupied by the electron.

10f
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1 mark

The total energy of an electron in a stable orbit of a hydrogen atom is given by:

E subscript n space equals space minus K over n squared

State and explain what physical quantity is represented by the constant K.

10g
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3 marks

In 1908, the physicist Friedrich Paschen first observed the photon emissions resulting from transitions from a level n to the level n = 3 of hydrogen and deduced their wavelengths were given by:

lambda space equals space fraction numerator A n squared over denominator n squared space minus space 9 end fraction

where A is a constant.

Justify this formula on the basis of the Bohr theory for hydrogen and determine an expression for the constant A.

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