VCAA Physics How do physicists explain motion in two dimensions?

15 sample questions with marking guides and sample answers

Q12
2022
QCAA
Paper 1
1 mark
Q12
1 mark

An object experiencing uniform circular motion in a horizontal plane travels at an average speed of 8.0 m s18.0 \text{ m s}^{-1}.
Calculate the radius of the object’s path if it takes 0.3 s to complete a full rotation.

A

3.8×1013.8 \times 10^{-1} m

B

2.6×1002.6 \times 10^0 m

C

1.5×1011.5 \times 10^1 m

D

1.7×1021.7 \times 10^2 m

Reveal Answer
A

3.8×1013.8 \times 10^{-1} m

Correct Answer

This is the correct answer. Using the formula for speed in uniform circular motion, v=2πrTv = \frac{2\pi r}{T}, we can rearrange for radius: r=vT2πr = \frac{vT}{2\pi}. Substituting the values gives r=8.0×0.32π0.38 mr = \frac{8.0 \times 0.3}{2\pi} \approx 0.38 \text{ m}.

B

2.6×1002.6 \times 10^0 m

This option is incorrect. It is close to the value of the circumference (C=vT=2.4 mC = vT = 2.4 \text{ m}) or the result of dividing speed by π\pi, rather than solving for the radius using 2π2\pi.

C

1.5×1011.5 \times 10^1 m

This option is incorrect and results from a calculation error or misapplication of the circular motion variables.

D

1.7×1021.7 \times 10^2 m

This option is incorrect. It results from incorrectly rearranging the formula as r=2πvTr = \frac{2\pi v}{T} instead of dividing by 2π2\pi.

Q5
2021
QCAA
Paper 2
4 marks
Q5
4 marks

An alpha particle with a charge of +3.2×1019+3.2 \times 10^{-19} C moves through an electric field, accelerating from rest through a potential difference of 240 V.

Determine the velocity of the particle at the end of its acceleration, expressing your answer in scientific notation. (m/s to 2 significant figures)

Reveal Answer

The change in potential energy of an electric charge moving through an electric field is equivalent to the work done on the charge.
V=ΔUqV = \frac{\Delta U}{q}
ΔU=Vq\Delta U = Vq
=240×3.2×1019= 240 \times 3.2 \times 10^{-19}
=7.68×1017J=W= 7.68 \times 10^{-17} J = W

The work done on an object is equal to the change in kinetic energy.
Ek=12mv2E_k = \frac{1}{2}mv^2
7.68×1017=12×6.64×1027×v27.68 \times 10^{-17} = \frac{1}{2} \times 6.64 \times 10^{-27} \times v^2
v2=7.68×101712×6.64×1027v^2 = \frac{7.68 \times 10^{-17}}{\frac{1}{2} \times 6.64 \times 10^{-27}}
v=7.68×101712×6.64×1027v = \sqrt{\frac{7.68 \times 10^{-17}}{\frac{1}{2} \times 6.64 \times 10^{-27}}}
Velocity = 1.5×105 m s11.5 \times 10^5 \text{ m s}^{-1} (to 2 significant figures)

Marking Criteria
DescriptorMarks

Recognises the scenario relates to work done on a moving charge in an electric field

1

Identifies that work done on the charge equates to its kinetic energy

1

Provides appropriate mathematical reasoning

1

Determines the velocity

1
Q9
2021
SCSA
5 marks
Q9
5 marks

A space station is shaped like a huge hollow doughnut that is rotating uniformly. The outer radius is 4.60 × 10² m. What is the period of rotation of the station if a person standing on the outer wall inside the station experiences the same weight force she would experience on Earth?

[Copyrighted image]

Reveal Answer

The centripetal force is supplied by the reaction force, so mv2/r=Rmv^2/r = R.

The reaction force equals mgmg, giving mv2/r=mgmv^2/r = mg.

Rearranging the formula to calculate velocity gives v=rg=4.60×102×9.80=67.1 m s1v = \sqrt{rg} = \sqrt{4.60 \times 10^2 \times 9.80} = 67.1 \text{ m s}^{-1}.

The period is circumference over time, T=2πr/vT = 2\pi r/v.

Calculating the period gives T=43.0 sT = 43.0 \text{ s}.

Marking Criteria
DescriptorMarks

States that centripetal force is supplied by the reaction force (mv2/r=Rmv^2/r = R)

1

Equates reaction force to weight (mv2/r=mgmv^2/r = mg)

1

Correctly rearranges formula and calculates velocity (v=rg=4.60×102×9.80=67.1 m s1v = \sqrt{rg} = \sqrt{4.60 \times 10^2 \times 9.80} = 67.1 \text{ m s}^{-1})

1

States that period is circumference over time (T=2πr/vT = 2\pi r/v)

1

Correctly calculates period (T=43.0 sT = 43.0 \text{ s})

1
Q14
2023
NESA
1 mark
Q14
1 mark

Planet X has a mass 4 times that of Earth and a radius 3 times that of Earth. The escape velocity at the surface of Earth is 11.2 km s1^{-1}.

What is the escape velocity at the surface of planet X?

A

8.40 km s1^{-1}

B

9.70 km s1^{-1}

C

12.9 km s1^{-1}

D

14.9 km s1^{-1}

Reveal Answer
A

8.40 km s1^{-1}

Incorrect. This value is obtained by multiplying Earth's escape velocity by 3/43/4, incorrectly assuming escape velocity is proportional to R/MR/M.

B

9.70 km s1^{-1}

Incorrect. This value is obtained by multiplying Earth's escape velocity by 3/4\sqrt{3/4}, incorrectly assuming escape velocity is proportional to R/M\sqrt{R/M}.

C

12.9 km s1^{-1}

Correct Answer

Correct. Escape velocity is given by v=2GM/Rv = \sqrt{2GM/R}, meaning it is proportional to M/R\sqrt{M/R}. For Planet X, vX=vE4/312.9v_X = v_E \sqrt{4/3} \approx 12.9 km s1^{-1}.

D

14.9 km s1^{-1}

Incorrect. This value is obtained by multiplying Earth's escape velocity by 4/34/3, incorrectly assuming escape velocity is proportional to M/RM/R instead of M/R\sqrt{M/R}.

Q7
2024
QCAA
Paper 1
1 mark
Q7
1 mark

An object experiencing a gravitational force of 50.0 N moves down a frictionless incline of 40.040.0^\circ to the horizontal.
Calculate the net force acting on the object.

A

32.1 N

B

37.3 N

C

38.3 N

D

42.0 N

Reveal Answer
A

32.1 N

Correct Answer

On a frictionless incline, the net force is the component of gravity parallel to the slope, calculated as Fnet=Fgsin(θ)=50.0N×sin(40.0)32.1NF_{net} = F_g \sin(\theta) = 50.0 \, \text{N} \times \sin(40.0^\circ) \approx 32.1 \, \text{N}.

B

37.3 N

This incorrect value results from calculating the sine of the angle in radians (50.0sin(40 rad)37.3N50.0 \sin(40 \text{ rad}) \approx 37.3 \, \text{N}) rather than degrees.

C

38.3 N

This represents the perpendicular component of gravity (Fgcos(40.0)38.3NF_g \cos(40.0^\circ) \approx 38.3 \, \text{N}), which is balanced by the normal force and does not contribute to the net force down the incline.

D

42.0 N

This value corresponds to Fgtan(40.0)42.0NF_g \tan(40.0^\circ) \approx 42.0 \, \text{N}, which is an incorrect trigonometric relationship for finding the parallel force component.

Q20
2025
VCAA
1 mark
Q20
1 mark

Harriet and Tom were investigating how the speed, vv, of a falling object varied with the distance, ss, it had fallen.

They dropped a small steel ball, initially at rest, from the third floor of their school building. The speed of the ball was measured at six positions as it fell.

Air resistance can be ignored.

Which one of the following graphs of their data would be expected to result in a straight line through the origin?

A

vv versus ss

B

vv versus s\sqrt{s}

C

v2v^2 versus s\sqrt{s}

D

v\sqrt{v} versus ss

Reveal Answer
A

vv versus ss

The kinematic equation for an object falling from rest is v2=2gsv^2 = 2gs, meaning vv is proportional to s\sqrt{s}. A graph of vv versus ss would result in a curve, not a straight line.

B

vv versus s\sqrt{s}

Correct Answer

Using the kinematic equation v2=u2+2asv^2 = u^2 + 2as with an initial velocity of u=0u=0, we get v=2gsv = \sqrt{2g}\sqrt{s}. This shows that vv is directly proportional to s\sqrt{s}, which produces a straight line through the origin.

C

v2v^2 versus s\sqrt{s}

Based on the equation v2=2gsv^2 = 2gs, v2v^2 is directly proportional to ss, not s\sqrt{s}. Plotting v2v^2 versus s\sqrt{s} would result in a quadratic curve.

D

v\sqrt{v} versus ss

Since vv is proportional to s1/2s^{1/2}, v\sqrt{v} would be proportional to s1/4s^{1/4}. Plotting v\sqrt{v} versus ss would not produce a straight line.

Q2
2024
VCAA
1 mark
Q2
1 mark

A space-based observatory (SBO) of mass MM has a circular orbital radius RR around Earth. Modifications to the SBO have doubled its mass, but its orbital speed is kept constant.

Which one of the following is closest to the orbital radius of the SBO after the modifications have been made?

A

R4\frac{R}{4}

B

RR

C

2R2R

D

4R4R

Reveal Answer
A

R4\frac{R}{4}

This assumes the orbital radius is inversely proportional to the square of the satellite's mass. However, orbital speed and radius are completely independent of the satellite's mass.

B

RR

Correct Answer

The orbital speed v=GMERv = \sqrt{\frac{G M_E}{R}} depends only on Earth's mass and the orbital radius, not the satellite's mass. Since the speed is kept constant, the orbital radius must remain RR.

C

2R2R

This incorrectly assumes the orbital radius is directly proportional to the satellite's mass. The mass of the orbiting object cancels out when equating gravitational and centripetal forces.

D

4R4R

This incorrectly assumes the orbital radius is proportional to the square of the satellite's mass. A satellite's mass has no effect on its orbital radius for a given constant speed.

Q15
2024
QCAA
Paper 1
1 mark
Q15
1 mark

In which direction does the centripetal force act?

A

towards the centre of motion

B

away from the centre of motion

C

opposite to the object's direction of motion

D

tangentially to the object's direction of motion

Reveal Answer
A

towards the centre of motion

Correct Answer

The term "centripetal" means "center-seeking," and this force acts perpendicular to the velocity vector, directed radially inward, to constantly change the object's direction.

B

away from the centre of motion

This describes the direction of the apparent "centrifugal" force (a pseudo-force); the actual centripetal force must pull inward to keep the object on a curved path.

C

opposite to the object's direction of motion

A force acting opposite to the direction of motion acts as a braking force that slows the object down, rather than causing the perpendicular acceleration required for circular motion.

D

tangentially to the object's direction of motion

A tangential force acts parallel to the velocity and changes the object's speed, whereas centripetal force acts perpendicular to the velocity to change the direction.

Q9
2022
QCAA
Paper 2
9 marks
Q9

A person spins an object 4.3 m above the ground in a horizontal circular path of radius 0.8 m. They release the object horizontally, allowing it to travel to the ground.

Q9a
4 marks

Calculate the centripetal acceleration of the object before it is released, given it takes 5 s for the object to complete 12 revolutions. Show your working. (ms2ms^{-2} to two significant figures)

Reveal Answer

v=2πrTv = \frac{2\pi r}{T}
=2π×0.85÷12= \frac{2\pi \times 0.8}{5 \div 12}
=12.1 m s1= 12.1\ m\ s^{-1}

ac=v2ra_c = \frac{v^2}{r}
=12.120.8= \frac{12.1^2}{0.8}
=180 m s2= 180\ m\ s^{-2}

Centripetal acceleration = 180 m s2^{-2} (to two significant figures)

Marking Criteria
DescriptorMarks

Recognises the scenario relates to velocity in circular motion

1

Recognises the scenario relates to centripetal acceleration

1

Provides appropriate mathematical reasoning

1

Calculates the centripetal acceleration of the object

1
Q9b
5 marks

Calculate the total horizontal displacement for the object after it is released. Show your working. (m to two significant figures)

Reveal Answer

sy=uyt+12at2s_y = u_y t + \frac{1}{2} a t^2
4.3=0+12×9.8t24.3 = 0 + \frac{1}{2} \times 9.8 t^2
t=4.34.9t = \sqrt{\frac{4.3}{4.9}}
=0.94 s= 0.94\ s

sx=uxt+12at2s_x = u_x t + \frac{1}{2} a t^2
=12.1×0.94+12×0×0.942= 12.1 \times 0.94 + \frac{1}{2} \times 0 \times 0.94^2
=11.4 m= 11.4\ m

Horizontal displacement = 11 m (to two significant figures)

Marking Criteria
DescriptorMarks

Recognises the scenario relates to vertical component of projectile motion

1

Provides appropriate mathematical reasoning

1

Determines the time of flight

1

Recognises the scenario relates to the horizontal component of projectile motion

1

Calculates the total horizontal displacement

1
Q25
2020
QCAA
Paper 1
3 marks
Q25
3 marks

Mars has an average orbital radius of approximately 1.5 times the average orbital radius of Earth.
Calculate the time it takes Mars to orbit the Sun. (days to the nearest whole number)

Reveal Answer

TMars2rMars3=4π2GM\frac{T_{\mathrm{Mars}}^2}{r_{\mathrm{Mars}}^3}=\frac{4\pi^2}{GM}

T=4π2GMr3T=\sqrt{\frac{4\pi^2}{GM}\,r^3}

TMars=4π2GM(1.5×rEarth)3T_{\mathrm{Mars}}=\sqrt{\frac{4\pi^2}{GM}\,(1.5 \times r_{\mathrm{Earth}})^3}

Therefore TMars=1.53TEarthT_{\mathrm{Mars}}=\sqrt{1.5^3}T_{\mathrm{Earth}}

TMars=1.8371×365T_{\mathrm{Mars}} = 1.8371 \times 365 days

TMars=670.5T_{\mathrm{Mars}} = 670.5 days

Time = 671 days

Marking Criteria
DescriptorMarks

Indicates an understanding of the physical scenario in relation to Kepler’s law (or other relevant physical concept/s).

1

Provides pertinent mathematical operation/s correctly performed.

1

Determines the time correctly (accept: 1.83 to 1.84 years inclusive; OR 670 to 671 days inclusive; OR 16 080 to 16 107 hours inclusive; OR 57 888 000 to 57 974 400 seconds inclusive). Allow follow-through (FT) error for the time.

1
Q3
2021
QCAA
Paper 2
3 marks
Q3
3 marks

An object undergoes uniform circular motion in a path with a radius of rr.

Determine the effect on the radius if the mass of the object is doubled, but the centripetal force and velocity remain unchanged.

Reveal Answer

F=mv2rF = \frac{mv^2}{r}
Let RR be the radius of the new path
Mv2r=2Mv2R\frac{Mv^2}{r} = \frac{2Mv^2}{R}
1r=2R\frac{1}{r} = \frac{2}{R}
R=2rR = 2r
The radius will double.

Marking Criteria
DescriptorMarks

Recognises the scenario relates to uniform circular motion

1

Provides correct reasoning

1

Indicates that the radius will double

1
Q15
2020
QCAA
Paper 1
1 mark
Q15
1 mark

Calculate the orbital period of a satellite travelling on a 3.00×1083.00 \times 10^8 m radius orbit around the Earth.

A

1.44×1021.44 \times 10^{-2} hours

B

4.54×1024.54 \times 10^2 hours

C

1.64×1061.64 \times 10^6 hours

D

7.44×1087.44 \times 10^8 hours

Reveal Answer
A

1.44×1021.44 \times 10^{-2} hours

This value is extremely small (less than a minute) and is physically impossible for a satellite in such a large orbit.

B

4.54×1024.54 \times 10^2 hours

Correct Answer

Using the orbital period formula T=4π2r3GMT = \sqrt{\frac{4\pi^2 r^3}{GM}}, the period is calculated as 1.64×106\approx 1.64 \times 10^6 seconds. Dividing by 3600 converts this to approximately 454 hours.

C

1.64×1061.64 \times 10^6 hours

This value corresponds to the orbital period in seconds (1.64×1061.64 \times 10^6 s), but the question asks for the answer in hours.

D

7.44×1087.44 \times 10^8 hours

This value is significantly too large and likely results from a calculation error involving the powers of ten or failing to take the square root.

Q12
2021
QCAA
Paper 1
1 mark
Q12
1 mark

Calculate the maximum height reached by a projectile with an initial velocity of 15 m s1^{-1} at an angle of 30° up from the horizontal.

A

2.87 m

B

3.83 m

C

8.61 m

D

11.5 m

Reveal Answer
A

2.87 m

Correct Answer

This is the correct maximum height derived from the formula H=v2sin2(θ)2gH = \frac{v^2 \sin^2(\theta)}{2g}. Substituting the values yields (15)2(0.5)22(9.8)2.87 m\frac{(15)^2 (0.5)^2}{2(9.8)} \approx 2.87 \text{ m}.

B

3.83 m

This option is incorrect; it may result from a calculation error or using an incorrect fraction for the vertical component.

C

8.61 m

This answer incorrectly uses the horizontal component (cosine) instead of the vertical component (sine), calculating v2cos2(θ)2g\frac{v^2 \cos^2(\theta)}{2g}.

D

11.5 m

This option ignores the launch angle and calculates the height as if the projectile were fired straight up (9090^\circ) using v22g\frac{v^2}{2g}.

Q10
2020
SCSA
6 marks
Q10
6 marks

A golfer hits a ball at 37.0 m s1\text{m s}^{-1} at 31.0° to the horizontal on a flat fairway. It travels 123 m. She wants to hit a target 135 m away, so she increases the angle at which she hits the ball, without changing the launch speed. Calculate the smallest increase of angle that allows her to reach the target. (Hint: 2sinθcosθ=sin2θ2\sin\theta\cos\theta = \sin 2\theta)

Reveal Answer

t=135/37cosΘt = 135/37 \cos\Theta
0=37sinΘ4.9(135/37cosΘ)0 = 37 \sin\Theta - 4.9 (135/37 \cos\Theta)
372sinΘcosΘ=4.9×13537^2\sin\Theta\cos\Theta = 4.9 \times 135
sin2Θ=2×4.9×135/372\sin2\Theta = 2 \times 4.9 \times 135/37^2
2Θ=75.12\Theta = 75.1^\circ
Θ=37.5\Theta = 37.5^\circ
37.531=6.537.5 - 31 = 6.5^\circ

Marking Criteria

Expresses t as range over horizontal velocity

Marking Bands
DescriptorMarks

expresses t as range over horizontal velocity (t = 135/37 cosΘ)

1

None of the above

0

Substitutes time into equation for vertical displacement

Marking Bands
DescriptorMarks

substitutes time into equation for vertical displacement (s = 0) and simplifies (0 = 37 sinΘ - 4.9 (135/37 cosΘ), 37²sinΘcosΘ = 4.9 × 135)

2

substitutes time into equation for vertical displacement (s = 0) (0 = 37 sinΘ - 4.9 (135/37 cosΘ))

1

None of the above

0

Solves for angle using expression given

Marking Bands
DescriptorMarks

solves for angle using expression given (sin2Θ = 2 × 4.9 × 135/37², 2Θ = 75.1°, Θ = 37.5°)

2

partially solves for angle using expression given (e.g., sin2Θ = 2 × 4.9 × 135/37²)

1

None of the above

0

Subtracts initial angle to find change of angle

Marking Bands
DescriptorMarks

subtracts initial angle to find change of angle (37.5 - 31 = 6.5°)

1

None of the above

0
Q18
2023
QCAA
Paper 1
1 mark
Q18
1 mark

A 20 kg object is placed on an inclined plane with a slope of 3535^\circ. If the object experiences a frictional force of 40 N and no additional applied force, calculate its acceleration down the inclined plane.

A

3.6 m s23.6\text{ m s}^{-2}

B

5.6 m s25.6\text{ m s}^{-2}

C

6.0 m s26.0\text{ m s}^{-2}

D

7.6 m s27.6\text{ m s}^{-2}

Reveal Answer
A

3.6 m s23.6\text{ m s}^{-2}

Correct Answer

This is correct. The net force is the component of gravity down the slope (mgsin35112.4 Nmg \sin 35^\circ \approx 112.4\text{ N}) minus the opposing frictional force (40 N40\text{ N}), resulting in a net force of 72.4 N72.4\text{ N}. Dividing by the mass (20 kg20\text{ kg}) gives a3.6 m s2a \approx 3.6\text{ m s}^{-2}.

B

5.6 m s25.6\text{ m s}^{-2}

This answer ignores the frictional force. It calculates the acceleration based solely on the component of gravity acting down the slope (a=gsin355.6 m s2a = g \sin 35^\circ \approx 5.6\text{ m s}^{-2}).

C

6.0 m s26.0\text{ m s}^{-2}

This calculation incorrectly uses the cosine function for the parallel component of gravity (mgcos35mg \cos 35^\circ) instead of the sine function. The cosine component represents the normal force, not the force pulling the object down the slope.

D

7.6 m s27.6\text{ m s}^{-2}

This result incorrectly adds the frictional force to the gravitational component instead of subtracting it. Friction always opposes the direction of motion, so it must be subtracted from the driving force.

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