QCAA Physics Alternative Sequence Gravity and motion

15 sample questions with marking guides and sample answers

Q18
2025
NESA
1 mark
Q18
1 mark

The escape velocity from the surface of a planet, which has no atmosphere, is vv. A mass is launched at 4545^\circ to the planet's surface at vv.

What will be the subsequent motion of the mass?

A

A circular orbit around the planet

B

An elliptical orbit around the planet

C

A parabolic trajectory, returning to land with velocity vv

D

A trajectory reaching zero velocity at an infinite distance

Reveal Answer
A

A circular orbit around the planet

A circular orbit requires a negative total energy and a launch parallel to the surface at a specific orbital velocity, which is less than the escape velocity.

B

An elliptical orbit around the planet

An elliptical orbit requires the total energy of the system to be negative, meaning the launch velocity must be strictly less than the escape velocity.

C

A parabolic trajectory, returning to land with velocity vv

While the trajectory is indeed a parabola, an object launched at or above escape velocity will overcome the planet's gravity and never return to land.

D

A trajectory reaching zero velocity at an infinite distance

Correct Answer

At escape velocity, the total energy (kinetic plus gravitational potential) of the mass is exactly zero. Regardless of the outward launch angle, it will escape the planet's gravitational field and reach zero velocity at an infinite distance.

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
Q22
2021
QCAA
Paper 1
3 marks
Q22
3 marks

A planet is orbiting a 3.38×1031 kg3.38 \times 10^{31}\ \text{kg} star. The radius of the orbit is 4.23×108 km4.23 \times 10^8\ \text{km}.

Calculate the average speed of the planet (to the nearest whole number).

Reveal Answer

Assume the planet is undergoing uniform circular motion.

F=mv2rF = \frac{mv^2}{r}

This is equal to the force of gravity.
F=GMmr2F = \frac{GMm}{r^2}

Equating these two equations and rearranging for velocity gives:

v=GMrv=6.67×1011×3.38×10314.23×1011v=73 km s1 or 73  005 m s1\begin{align*} v &= \sqrt{\frac{GM}{r}}\\ v &= \sqrt{\frac{6.67 \times 10^{-11} \times 3.38 \times 10^{31}}{4.23 \times 10^{11}}}\\ v &= 73\text{ km s}^{-1}\text{ or }73\;005\text{ m s}^{-1} \end{align*}

Average speed = 73  005 m s173\;005\text{ m s}^{-1} (to the nearest whole number)

Marking Criteria
DescriptorMarks

recognises the scenario relates to uniform circular motion and universal gravitation

1

provides appropriate mathematical reasoning

1

calculates the average speed

1
Q2
2021
QCAA
Paper 1
1 mark
Q2
1 mark

Calculate the initial horizontal velocity of a projectile with an initial velocity of 38 m s138\ \text{m s}^{-1} at an angle of 4242^\circ up from the horizontal.

A

25 m s125\ \text{m s}^{-1}

B

28 m s128\ \text{m s}^{-1}

C

34 m s134\ \text{m s}^{-1}

D

40 m s140\ \text{m s}^{-1}

Reveal Answer
A

25 m s125\ \text{m s}^{-1}

This is the initial vertical velocity, which is calculated using v0sin(θ)=38sin(42)25 m s1v_0 \sin(\theta) = 38 \sin(42^\circ) \approx 25\ \text{m s}^{-1}.

B

28 m s128\ \text{m s}^{-1}

Correct Answer

The initial horizontal velocity is found using the cosine function: v0x=v0cos(θ)=38cos(42)28 m s1v_{0x} = v_0 \cos(\theta) = 38 \cos(42^\circ) \approx 28\ \text{m s}^{-1}.

C

34 m s134\ \text{m s}^{-1}

This value is incorrect and does not correspond to the proper trigonometric calculation for the horizontal component.

D

40 m s140\ \text{m s}^{-1}

The horizontal component of the velocity cannot be greater than the total initial velocity of 38 m s138\ \text{m s}^{-1}.

Q24
2025
NESA
3 marks
Q24
3 marks

Two satellites, AA and BB, are in stable circular orbits around the Earth. The radius of satellite AA's orbit is three times that of satellite BB's orbit. Both satellites have the same kinetic energy.

Show that the mass of AA is three times the mass of BB.

Reveal Answer

FC=FGmv2r=GMmr2mv2=GMmr12mv2=GMm2rGMmA2rA=GMmB2rB\begin{align*} F_C &= F_G\\ \frac{mv^2}{r} &= \frac{GMm}{r^2}\\ mv^2 &= \frac{GMm}{r}\\ \frac{1}{2}mv^2 &= \frac{GMm}{2r}\\ \therefore \frac{G M m_A}{2 r_A} &= \frac{G M m_B}{2 r_B} \end{align*}

Substitute rA=3rBr_A = 3r_B:

3rBrB=mAmB=3\frac{3r_B}{r_B} = \frac{m_A}{m_B} = 3

mA=3mB\therefore m_A = 3m_B

Marking Criteria
DescriptorMarks

Shows all relevant steps to determine the mass ratio

3

Makes progress towards determining mass ratio

2

Provides some relevant information

1

None of the above

0
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}.

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
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=2Mv2R1r=2RR=2r\begin{align*} \frac{Mv^2}{r} &= \frac{2Mv^2}{R}\\ \frac{1}{r} &= \frac{2}{R}\\ R &= 2r \end{align*}

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
Q18
2021
QCAA
Paper 1
1 mark
Q18
1 mark

A gravitational field is the

A

net gravitational force per unit mass at a particular point in space.

B

energy stored in an object as a result of its position relative to another object.

C

region of space surrounding a body in which another body experiences a force of gravitational attraction.

D

position in space where objects experience a force or acquire potential energy as they are ‘worked’ into that position.

Reveal Answer
A

net gravitational force per unit mass at a particular point in space.

This defines gravitational field strength (g=F/mg = F/m), which is a specific vector quantity at a point, rather than the concept of the field itself.

B

energy stored in an object as a result of its position relative to another object.

This is the definition of gravitational potential energy, which is the energy an object possesses due to its position, not the field.

C

region of space surrounding a body in which another body experiences a force of gravitational attraction.

Correct Answer

A gravitational field is conceptually defined as the region of space around a mass where another mass will experience a force of gravitational attraction.

D

position in space where objects experience a force or acquire potential energy as they are ‘worked’ into that position.

This describes concepts related to gravitational potential and work done, rather than defining the region of space that constitutes the gravitational field.

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 s115\ \text{m s}^{-1} at an angle of 3030^\circ up from the horizontal.

A

2.87 m2.87\ \text{m}

B

3.83 m3.83\ \text{m}

C

8.61 m8.61\ \text{m}

D

11.5 m11.5\ \text{m}

Reveal Answer
A

2.87 m2.87\ \text{m}

Correct Answer

The maximum height is calculated using the vertical component of velocity in the formula H=(v0sinθ)22gH = \frac{(v_0 \sin\theta)^2}{2g}. Substituting the given values yields H=(15sin30)22(9.8)2.87 mH = \frac{(15 \sin 30^\circ)^2}{2(9.8)} \approx 2.87\ \text{m}.

B

3.83 m3.83\ \text{m}

This value is obtained by incorrectly using the tangent function (tan30\tan 30^\circ) instead of the sine function to determine the vertical component of the initial velocity.

C

8.61 m8.61\ \text{m}

This result comes from mistakenly using the horizontal component of velocity (v0cos30v_0 \cos 30^\circ) instead of the vertical component in the maximum height formula.

D

11.5 m11.5\ \text{m}

This calculates the maximum height for a projectile launched vertically upwards (9090^\circ), completely ignoring the 3030^\circ launch angle.

Q7
2021
QCAA
Paper 1
1 mark
Q7
1 mark

Normal force is the force acting along an imaginary line

A

parallel to the surface.

B

perpendicular to the surface.

C

opposite to the gravitational force.

D

in the same direction as the gravitational force.

Reveal Answer
A

parallel to the surface.

Incorrect. A force acting parallel to the surface is typically friction. The term "normal" in physics specifically means perpendicular.

B

perpendicular to the surface.

Correct Answer

Correct. By definition, the normal force is a contact force that always acts perpendicular (at a 9090^\circ angle) to the surface an object is resting on or pressing against.

C

opposite to the gravitational force.

Incorrect. While this is true for objects on a perfectly horizontal surface, the normal force acts at an angle on an inclined plane and horizontally if an object is pressed against a vertical wall.

D

in the same direction as the gravitational force.

Incorrect. Gravitational force always pulls straight down toward the center of the Earth, while the normal force pushes outward perpendicularly from the contact surface.

Q4
2021
QCAA
Paper 2
4 marks
Q4
4 marks

A spacecraft is located between two large asteroids, Asteroid A and Asteroid B, that are 120 km apart. Asteroid A's mass is approximately four times the mass of Asteroid B.

Determine the distance of the spacecraft from Asteroid B (to the nearest whole number) if it experiences no net gravitational force from the two asteroids.

Reveal Answer

Fg.net=0F_{g.net} = 0
Therefore Fg.A=Fg.B|F_{g.A}| = |F_{g.B}|, then:

GmsMArA2=GmsMBrB24MBrA2=MBrB24MB×rB2=rA2×MB4MB×rB2MB=rA2rA2=4rB2rA=2rB\begin{align*} G\frac{m_sM_A}{r_A^2} &= G\frac{m_sM_B}{r_B^2}\\ \frac{4M_B}{r_A^2} &= \frac{M_B}{r_B^2}\\ 4M_B \times r_B^2 &= r_A^2 \times M_B\\ \frac{4M_B \times r_B^2}{M_B} &= r_A^2\\ r_A^2 &= 4r_B^2\\ r_A &= 2r_B \end{align*}

Then:

120=rA+rB120=3rBrB=40\begin{align*} 120 &= r_A + r_B\\ 120 &= 3r_B\\ r_B &= 40 \end{align*}

Distance from Asteroid B = 40 km (to the nearest whole number).

Marking Criteria
DescriptorMarks

recognises the scenario relates to Newton's law of universal gravitation

1

recognises that no net force occurs when the forces are equivalent

1

provides appropriate mathematical reasoning

1

determines distance from the asteroid

1
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.

Q11
2024
NESA
1 mark
Q11
1 mark

A satellite is in a circular orbit.

What is the relationship between its orbital velocity, vv, and its orbital radius, rr?

A

vv is directly proportional to the square of rr.

B

vv is inversely proportional to the square of rr.

C

vv is directly proportional to the square root of rr.

D

vv is inversely proportional to the square root of rr.

Reveal Answer
A

vv is directly proportional to the square of rr.

Equating gravitational force to centripetal force yields v=GM/rv = \sqrt{GM/r}, not vr2v \propto r^2. This option incorrectly suggests velocity increases rapidly as the orbit gets larger.

B

vv is inversely proportional to the square of rr.

While gravitational force is inversely proportional to the square of rr (Fg1/r2F_g \propto 1/r^2), orbital velocity depends on the square root of the inverse of rr.

C

vv is directly proportional to the square root of rr.

This would mean velocity increases as the radius increases (vrv \propto \sqrt{r}). In reality, satellites further away experience weaker gravity and travel slower.

D

vv is inversely proportional to the square root of rr.

Correct Answer

Setting the centripetal force equal to the gravitational force (mv2/r=GMm/r2mv^2/r = GMm/r^2) and solving for velocity gives v=GM/rv = \sqrt{GM/r}. This shows that vv is inversely proportional to the square root of rr.

Q18
2023
QCAA
Paper 1
1 mark
Q18
1 mark

A 20 kg object is placed on an inclined plane with a slope of 35°. 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

Correct. The net force is the component of gravity down the slope minus friction (mgsin(35)40mg \sin(35^\circ) - 40). Dividing this net force (72.472.4 N) by the mass (2020 kg) gives an acceleration of 3.6 m s23.6 \text{ m s}^{-2}.

B

5.6 m s25.6 \text{ m s}^{-2}

Incorrect. This value represents the acceleration of the object if there were no friction acting against it (a=gsin(35)a = g \sin(35^\circ)).

C

6.0 m s26.0 \text{ m s}^{-2}

Incorrect. This result comes from incorrectly using cosine instead of sine to find the component of gravity parallel to the slope (mgcos(35)mg \cos(35^\circ)).

D

7.6 m s27.6 \text{ m s}^{-2}

Incorrect. This calculates the acceleration if friction were incorrectly added to the gravitational force, acting in the same direction down the slope rather than opposing the motion.

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