MYP Physics · Unit 15
Fields and gravity
Gravitational and electric field models, field strength, superposition, orbital motion, and satellite contexts.
- 21
- questions
- 16
- total marks
- 5
- mapped topics
Name the force that keeps a satellite turning
A satellite moves in a circular orbit around Earth at constant speed. Which statement best describes the force on it?
- A
No force acts because its speed is constant
- B
An outward force balances gravity
- C
Gravity provides a resultant force towards Earth's centre
- D
The satellite's engine continuously pushes it forwards
- a
Select and explain Select the correct statement and explain why constant speed does not mean zero acceleration.
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Mark-by-mark answer
Correct choiceC
Selects option C: gravity provides the resultant force directed towards Earth's centre.
States that velocity changes because its direction changes even though speed is constant.
Links the inward acceleration to an inward resultant gravitational force.
Build deeper understandingReveal the teacher insight
Deeper learning cue
Use velocity arrows at several points on the orbit; the change in direction makes the acceleration visible without inventing an outward force.
Gravitational field above Earth
At Earth's surface the gravitational field strength is 9.8 N kg⁻¹. A 500 kg satellite is at a distance of two Earth radii from Earth's centre. Treat Earth as a sphere and use the inverse-square relationship.
- a
Calculate Calculate the gravitational field strength at the satellite.
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Recognises that doubling distance from the centre reduces field strength by 2² = 4.
Calculates 9.8 ÷ 4.
Obtains 2.45 N kg⁻¹.
- b
Calculate Calculate the gravitational force on the satellite.
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Uses F = mg or F = mass × field strength.
Obtains F = 500 × 2.45 = 1225 N, towards Earth's centre.
- c
Explain Explain why the satellite is not weightless at this position.
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Gravity is still acting; apparent weightlessness in orbit is due to continuous free fall, not zero gravitational field.
Build deeper understandingReveal the teacher insight
Deeper learning cue
Emphasise that orbital radius is measured from Earth's centre, not from its surface, before applying inverse-square reasoning.
Test an inverse-square electric field
A simulation reports the electric field magnitude at different distances from one isolated positive point charge.
| Distance from charge / m | Field magnitude / N C⁻¹ |
|---|---|
| 0.10 | 360 |
| 0.20 | 90 |
| 0.30 | 40 |
| 0.40 | 22.5 |
- a
Show Use two data pairs to show that the field follows an inverse-square pattern.
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Selects two suitable distances, such as 0.10 m and 0.20 m.
Shows that distance doubles while field falls from 360 to 90 N C⁻¹, a factor of four.
Connects a factor-four decrease to 1 ÷ 2², supporting E ∝ 1/r².
- b
Predict Predict the field magnitude at 0.50 m.
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Uses the constant Er² = 360 × 0.10² = 3.6 N m² C⁻¹.
Calculates E = 3.6 ÷ 0.50² = 14.4 N C⁻¹.
- c
Evaluate State two reasons why a classroom field-line diagram is not a literal picture of this field.
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Mark-by-mark answer
States that the lines are a chosen representation and there are not physical threads in space.
States another limitation, such as line number or spacing being chosen, a flat drawing representing a three-dimensional field, or arrows showing test-charge direction rather than motion.
Build deeper understandingReveal the teacher insight
Deeper learning cue
A log–log extension can reveal the slope −2, but proportional-factor reasoning is sufficient and keeps the model interpretable.
More focused practice
Seven quick mastery questions
Open one task at a time, reveal the worked reasoning, then mark it mastered or save it to revisit.
Criterion A
Weight on a small planet
3 marks · routineOpen question →Criterion A
Twice as far from a moon
4 marks · demandingOpen question →Criterion A
Climb in a nearly uniform field
4 marks · routineOpen question →Criterion A
Orbit-speed estimate
6 marks · discriminatingOpen question →Criterion C
Read a field-line map
4 marks · routineOpen question →Criterion D
Earth and Moon jump claim
6 marks · demandingOpen question →Criterion B
Measure local g with a pendulum
8 marks · discriminatingOpen question →Criterion C
A radial gravity probe
8 marks · demandingOpen question →Criterion C
A proposed field law
8 marks · demandingOpen question →Criterion C
A nearly uniform field region
8 marks · demandingOpen question →Criterion C
Rounded field readings
8 marks · demandingOpen question →Criterion C
One reading breaks the trend
8 marks · demandingOpen question →Criterion C
A consistent outer-orbit record
8 marks · demandingOpen question →Criterion C
An unexpected far-field value
8 marks · demandingOpen question →Criterion C
A weak-field body
8 marks · demandingOpen question →Criterion C
Checking a numerical field model
8 marks · demandingOpen question →Criterion C
Distances measured from the centre
8 marks · demandingOpen question →Criterion C
Test an inverse-square gravitational field claim
12 marks · discriminatingOpen question →Reference subsectionMapped lessons for this unit
Universal gravitation
Connect weight near Earth to a wider gravitational model and test inverse-square reasoning.
Open lesson →Electric field lines and direction
Treat field lines as a representation: use direction and spacing while naming model limitations.
Open lesson →Electric field strength and force
Connect a field property to force on a test charge while keeping sign and direction distinct.
Open lesson →Point-charge field patterns
Criterion A focus: move between diagrams, proportional reasoning, and radial-field calculations.
Open lesson →Circular motion and orbital systems
Identify the inward resultant in turns and orbits without inventing an outward force in an inertial frame.
Open lesson →