SCSA Physics Science Understanding
15 sample questions with marking guides and sample answers
An object experiencing uniform circular motion in a horizontal plane travels at an average speed of .
Calculate the radius of the object’s path if it takes 0.3 s to complete a full rotation.
m
m
m
m
Reveal Answer
m
This is the correct answer. Using the formula for speed in uniform circular motion, , we can rearrange for radius: . Substituting the values gives .
m
This option is incorrect. It is close to the value of the circumference () or the result of dividing speed by , rather than solving for the radius using .
m
This option is incorrect and results from a calculation error or misapplication of the circular motion variables.
m
This option is incorrect. It results from incorrectly rearranging the formula as instead of dividing by .
Two objects on different planets experience different accelerations due to gravity.
| Object | Mass (kg) | Acceleration due to gravity (m s) |
|---|---|---|
| A | 79 | 1.6 |
| B | 32 | 3.7 |
Determine which object has the greatest force acting on it. Show your working.
Reveal Answer
Force on object A = down
Force on object B = down
Object A experiences the greatest force.
| Descriptor | Marks |
|---|---|
Recognises the scenario relates to relationship between the force due to gravity and mass | 1 |
Provides appropriate mathematical reasoning | 1 |
Identifies the object experiencing the greatest force acting on it | 1 |
A spaceship with a velocity of m s is measured to be 125 m in length by an observer at rest.
Calculate the length of the spaceship as measured by somebody on board the spaceship.
119 m
131 m
137 m
178 m
Reveal Answer
119 m
This calculation incorrectly treats the given 125 m as the proper length () and solves for the contracted length. Since the observer on the spaceship is at rest relative to it, they measure the proper length, which must be longer than the contracted length measured by the outside observer.
131 m
The observer on board measures the proper length (). Using the length contraction formula , with m and , we rearrange to find m.
137 m
This answer results from omitting the square root in the Lorentz factor calculation, dividing 125 by instead of .
178 m
This value is incorrect and does not align with the standard length contraction formula. It likely results from a calculation error or misapplication of the Lorentz factor .
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 .
The reaction force equals , giving .
Rearranging the formula to calculate velocity gives .
The period is circumference over time, .
Calculating the period gives .
| Descriptor | Marks |
|---|---|
States that centripetal force is supplied by the reaction force () | 1 |
Equates reaction force to weight () | 1 |
Correctly rearranges formula and calculates velocity () | 1 |
States that period is circumference over time () | 1 |
Correctly calculates period () | 1 |
Two asteroids experience a gravitational force of N between them. Their masses are kg and kg.
Calculate the distance between the two asteroids. Show your working. (m to two significant figures)
Reveal Answer
Distance between asteroids = m (to two significant figures)
| Descriptor | Marks |
|---|---|
Recognises the scenario relates to Newton’s Law of Universal Gravitation | 1 |
Provides appropriate mathematical reasoning | 1 |
Calculates the distance between the asteroids | 1 |
Which property of light is described by the postulates of special relativity?
The energy of light is greater when the frequency of the photons decreases.
The wavelength of light decreases as the velocity of the source increases.
The velocity of light remains constant in all inertial frames of reference.
The frequency of light changes depending on media.
Reveal Answer
The energy of light is greater when the frequency of the photons decreases.
This statement is factually incorrect and unrelated to special relativity. According to the quantum relation , energy is directly proportional to frequency, so energy decreases as frequency decreases.
The wavelength of light decreases as the velocity of the source increases.
This describes the Doppler effect rather than a fundamental postulate. While relativity influences the Doppler shift, the postulates specifically define the behavior of the speed of light, not the change in wavelength due to source motion.
The velocity of light remains constant in all inertial frames of reference.
This is the second postulate of special relativity. It states that the speed of light in a vacuum () is constant and independent of the motion of the light source or the observer in all inertial frames.
The frequency of light changes depending on media.
This is incorrect regarding wave mechanics; frequency remains constant when light changes media, while speed and wavelength change. Furthermore, this is a concept of optics, not a postulate of special relativity.
Particles move at a rate of times per second around a circular particle accelerator with a radius of 35 m.
Calculate the average speed of the particles. Show your working.
Average speed = ______ (two significant figures)
Reveal Answer
Average speed (to two significant figures)
| Descriptor | Marks |
|---|---|
Recognises the scenario relates to average speed of objects in uniform circular motion | 1 |
Provides appropriate mathematical reasoning | 1 |
Calculates the average speed of the particles | 1 |
Kepler’s third law
describes the elliptical orbit of planets.
combines Newton’s first law of motion with uniform circular motion.
equates the area of the arc sweep of a planet to the time taken to complete it.
describes the relationship between uniform circular motion and the Law of Universal Gravitation.
Reveal Answer
describes the elliptical orbit of planets.
This describes Kepler's First Law, also known as the Law of Ellipses, which states that planets move in elliptical orbits with the Sun at one focus.
combines Newton’s first law of motion with uniform circular motion.
Kepler's laws are not derived from combining Newton's first law with uniform circular motion; rather, the third law relates orbital period to distance.
equates the area of the arc sweep of a planet to the time taken to complete it.
This describes Kepler's Second Law, or the Law of Equal Areas, which states that a line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.
describes the relationship between uniform circular motion and the Law of Universal Gravitation.
Kepler's Third Law () is physically derived by equating the centripetal force in uniform circular motion to the gravitational force defined by Newton's Law of Universal Gravitation.
An astronaut has left Earth and is travelling on a spaceship at 0.800c (γ = 1.67) directly towards the star known as Sirius, which is located 8.61 light-years away from Earth, as measured by observers on Earth.
How long will the trip take according to a clock that the astronaut is carrying on his spaceship? Show your working.
Reveal Answer
The distance of 8.61 light-years is the proper length in Earth's frame of reference. The proper time in the Earth's frame of reference is:
This time is the dilated time in the astronaut's frame of reference. The proper time as measured by the astronaut is:
| Descriptor | Marks |
|---|---|
Calculates the time in Earth's frame of reference () OR calculates the contracted length in the astronaut's frame of reference () | 1 |
Calculates the correct proper time of | 1 |
Is the trip time measured by the astronaut in part a. a proper time? Explain your reasoning.
Reveal Answer
The time measured by the astronaut will be proper time because the clock is stationary in the astronaut's frame of reference.
| Descriptor | Marks |
|---|---|
Identifies that the time measured by the astronaut is proper time | 1 |
Explains that this is because the clock is stationary in the astronaut's frame of reference | 1 |
A space-based observatory (SBO) of mass has a circular orbital radius 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?
Reveal Answer
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.
The orbital speed 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 .
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.
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.
The escape velocity from the surface of a planet, which has no atmosphere, is . A mass is launched at to the planet's surface at .
What will be the subsequent motion of the mass?
A circular orbit around the planet
An elliptical orbit around the planet
A parabolic trajectory, returning to land with velocity
A trajectory reaching zero velocity at an infinite distance
Reveal Answer
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.
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.
A parabolic trajectory, returning to land with velocity
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.
A trajectory reaching zero velocity at an infinite distance
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.
A spaceship travelled from Planet A to Planet B at a speed of . An observer that was stationary relative to both planets measured the time taken for the trip to be 4.0 years.
Calculate the time taken for the trip as measured by an observer on the spaceship. (years to 1 decimal place)
Reveal Answer
years
Time = 1.7 years (to 1 decimal place)
| Descriptor | Marks |
|---|---|
Indicates an understanding of the physical scenario in relation to time dilation (or other relevant physical concept/s). | 1 |
Indicates an understanding that the time provided in the question represents relativistic (dilated) time. (If proper time and relativistic time are confused, a maximum of 2 marks can be awarded overall.) | 1 |
Provides pertinent mathematical operation/s correctly performed. | 1 |
Determines the time correctly (accept 1.7 years to 1.8 years inclusive). | 1 |
In which direction does the centripetal force act?
towards the centre of motion
away from the centre of motion
opposite to the object's direction of motion
tangentially to the object's direction of motion
Reveal Answer
towards the centre of motion
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.
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.
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.
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.
Two satellites, and , are in stable circular orbits around the Earth. The radius of satellite 's orbit is three times that of satellite 's orbit. Both satellites have the same kinetic energy.
Show that the mass of is three times the mass of .
Reveal Answer
Substitute :
| Descriptor | Marks |
|---|---|
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 |
Which one of the following is an example of an inertial frame of reference?
a bus travelling at constant velocity
an express train that is accelerating
a car turning a corner at a constant speed
a roller-coaster speeding up while heading down a slope
Reveal Answer
a bus travelling at constant velocity
This is correct because an inertial frame of reference is one that is not accelerating. A bus moving at a constant velocity has zero acceleration, making it an inertial frame where Newton's laws of motion hold true.
an express train that is accelerating
This is incorrect because an accelerating object represents a non-inertial frame of reference. By definition, an inertial frame must have zero acceleration.
a car turning a corner at a constant speed
This is incorrect because turning a corner involves a change in direction, which means the car is experiencing centripetal acceleration. Even at a constant speed, a change in direction makes it a non-inertial frame of reference.
a roller-coaster speeding up while heading down a slope
This is incorrect because the roller-coaster is speeding up, meaning its velocity is changing and it is accelerating. Any accelerating environment is a non-inertial frame of reference.