Grade by Grade
D. Gravitational, Electric, and Magnetic Fields · Gravitational, Electric and Magnetic Fields

Gravitational, Electric and Magnetic Fields: Unit Review

D1.1 D1.2 D2.1 D2.2 D2.3 D2.4 D2.5 D3.1 D3.2 D3.3About 40 minutes
Learning goals
  • I can solve problems about gravitational forces, fields, orbits and energy, including escape speed.
  • I can solve problems about electric forces, fields, potential energy and potential, and the motion of charged particles in uniform electric fields.
  • I can solve problems about magnetic fields and the forces on currents and moving charges, and explain field technologies.
  • I can compare the three fields and assess the impact of field technologies on society and the environment.

Words to know

field
A region in which an object with mass (gravitational), charge (electric) or moving charge (magnetic) feels a force.
inverse-square law
A quantity that varies as 1/r², like the gravitational field of a mass and the electric field of a point charge.
uniform field
A field with the same strength and direction everywhere in a region, such as near Earth's surface, between parallel plates or inside a solenoid.
potential energy (Eg, Ee)
Energy stored in a system because of the positions of masses or charges. Zero is chosen at infinite separation for point sources.
elementary charge (e)
The smallest free charge, 1.60 × 10⁻¹⁹ C, measured by Millikan.
exchange particle
A particle that carries a force in the Standard Model: photons, gluons, W and Z bosons.

Pulling the unit together

This review covers all sixteen lessons of the unit: gravity and orbits, electric forces, fields and potential, charged particles in electric and magnetic fields, field technologies and their place in society. Each practice set below is named after its lesson, so you can go straight back to the lesson if a question gives you trouble.

How to use this review

  1. Do one practice set at a time without looking at the answers, using a calculator and the constants listed in the unit overview.
  2. Check your answers, including the units and directions.
  3. Mark any set where you missed more than one question, and reread that lesson's examples before trying its "More practice" questions again.
  4. Finish with the 10-question quiz. Aim for 8 out of 10 or better.
  5. On a single page, write every equation from the unit, sorted into gravitational, electric and magnetic columns, with what each symbol means. Compare it with the summary diagram below.
Gravitational fieldsource: massF = Gm₁m₂/r²g = GM/r²Eg = −GMm/rv = √(GM/r)always attractsElectric fieldsource: chargeF = kq₁q₂/r²E = kQ/r² or ΔV/dEe = kQq/r, V = kQ/rqΔV = ½mv²attracts or repelsMagnetic fieldsource: moving chargeB = μ₀I/(2πr)B = μ₀NI/LF = ILB sin θF = qvB sin θr = mv/(qB)
The unit's key equations, sorted by field. Notice the matching shapes of the gravitational and electric equations (mass ↔ charge, G ↔ k).
+ + + + +− − − − −+quniform E: parabola(like a thrown ball)+quniform B ⊥ v: circle(r = mv/qB, constant speed)crossed E and B: straightonly if v = E/B
Three ways a positive charge can move in uniform fields: a parabola in an electric field, a circle in a magnetic field, and a straight line in crossed fields when v = E/B.
Just for fun

The numbers in this unit run from the elementary charge, 1.60 × 10⁻¹⁹ C, to the Sun's mass, 1.99 × 10³⁰ kg: almost 50 powers of ten. Few other units ask your calculator's scientific-notation key to work this hard.

Newton's Law of Universal Gravitation

1

Find the gravitational force between two 70 kg people standing 1.0 m apart.

2

Two asteroids move three times farther apart. What happens to the gravitational force between them?

3

Find the gravitational force between Earth and the Moon (M_E = 5.97 × 10²⁴ kg, M_M = 7.35 × 10²² kg, d = 3.84 × 10⁸ m).

Gravitational Fields: Near Earth and Far Away

1

Find g at the ISS's altitude, 400 km above Earth's surface.

2

At what altitude is g half its surface value?

3

Find g on the surface of Mars (M = 6.42 × 10²³ kg, R = 3.39 × 10⁶ m).

4

Describe how the field lines near Earth's surface differ from the field lines seen from far away.

Satellites and Circular Orbits

1

Find the orbital speed of a RADARSAT Constellation satellite, 600 km above Earth.

2

Why do astronauts on the ISS float, even though g there is about 8.7 N/kg?

3

Find the orbital radius of a satellite with a period of 24.0 h.

Kepler's Laws, Black Holes and Dark Matter

1

Mars orbits the Sun at 1.52 AU. Find its period in Earth years.

2

According to Kepler's second law, where in its orbit does a comet move fastest?

3

Use Earth's orbit (r = 1.50 × 10¹¹ m, T = 3.156 × 10⁷ s) to find the Sun's mass.

4

What evidence from galaxy rotation suggests dark matter?

Gravitational Potential Energy, Escape Speed and Black Holes

1

Find the escape speed from the Moon (M = 7.35 × 10²² kg, R = 1.74 × 10⁶ m).

2

How much gravitational potential energy must be added to raise a 1000 kg satellite from Earth's surface to 400 km altitude (ignore its orbital speed)?

3

Find the Schwarzschild radius of a black hole with the Sun's mass (1.99 × 10³⁰ kg).

Electric Charge and Coulomb's Law

1

Two +2.0 μC charges are 0.30 m apart. Find the force between them.

2

Each charge is doubled and the distance is doubled. What happens to the force?

3

A balloon has a charge of −3.2 nC. How many extra electrons does it carry?

Electric Fields of Point Charges and Field Lines

1

Find the electric field 0.50 m from a +5.0 nC charge.

2

Find the force on an electron in a 2.0 × 10³ N/C field.

3

Charges of +4.0 nC and −4.0 nC are 0.20 m apart. Find the field at the midpoint.

4

Give three rules for drawing electric field lines.

Electric Potential Energy and Electric Potential

1

Find the electric potential 0.25 m from a +3.0 nC charge.

2

Find the electric potential energy of +2.0 μC and −3.0 μC charges 0.10 m apart.

3

How much work is needed to move a +2.0 μC charge through a potential difference of 50 V?

Uniform Electric Fields Between Parallel Plates

1

Parallel plates 4.0 mm apart have a potential difference of 120 V. Find the field between them.

2

Describe the field lines between two large parallel plates, away from the edges.

3

The plates stay connected to the same battery but are pulled twice as far apart. What happens to E?

Charged Particles in Uniform Electric Fields

1

An electron starts from rest and is accelerated through 500 V. Find its speed.

2

How much kinetic energy does a proton gain when accelerated through 500 V, in eV and in joules?

3

An electron enters a uniform field of 1.0 × 10⁴ N/C between plates 5.0 cm long, moving parallel to the plates at 2.0 × 10⁷ m/s. How far is it deflected by the time it leaves?

Millikan's Oil Drop Experiment and the Elementary Charge

1

An oil drop of mass 3.2 × 10⁻¹⁵ kg is held still between horizontal plates 1.0 cm apart when the potential difference is 980 V. Find its charge and the number of excess electrons.

2

A student reports a drop with charge 2.4 × 10⁻¹⁹ C. Why is this result suspicious?

3

For a balanced drop, which force balances gravity, and which way must the electric field point if the drop carries extra electrons?

Magnetic Fields of Currents and the Force on a Conductor

1

Find the magnetic field 5.0 cm from a long straight wire carrying 10 A.

2

A 0.20 m wire carrying 5.0 A is at right angles to a 0.30 T field. Find the force on it.

3

Find the field inside a solenoid with 500 turns, 0.25 m long, carrying 2.0 A.

4

Two long parallel wires carry currents in the same direction. Do they attract or repel?

Magnetic Force on Moving Charges and Circular Motion

1

A proton moves at 2.0 × 10⁶ m/s at right angles to a 0.40 T field. Find the force on it and the radius of its path.

2

Why does a magnetic field never change the speed of a charged particle?

3

A velocity selector has E = 3.0 × 10⁴ N/C and B = 0.15 T. What speed passes straight through?

Field Technologies: Mass Spectrometers, Accelerators and MRI

1

Singly charged sodium ions (23 u, 1 u = 1.66 × 10⁻²⁷ kg) enter a 0.50 T field at 1.0 × 10⁵ m/s. How far from the entrance slit do they land?

2

Find the AC frequency needed for a proton cyclotron with B = 1.0 T.

3

Why can a cyclotron's AC voltage keep a fixed frequency while the particle speeds up?

Comparing Fields and the Fundamental Forces

1

Name the exchange particles of the electromagnetic, strong and weak forces.

2

Give two ways the magnetic force on a charge differs from the electric force.

3

Gravity is by far the weakest force. Why does it control the motion of planets?

Fields, Technology and Society

1

A GPS receiver's clock is off by 5.0 ns. What position error does that cause?

2

Estimate the up-and-down travel time of a signal through a geostationary satellite 3.58 × 10⁷ m above you.

3

Give one benefit and one concern of large internet satellite constellations.

Check your understanding

Quiz

1.

The distance between two masses is halved. The gravitational force between them becomes

2.

What is the gravitational field strength at a distance of 2R_E from Earth's centre (surface g = 9.8 N/kg)?

3.

The speed of a satellite in a circular orbit depends on

4.

A planet orbits the Sun with a semi-major axis of 4.0 AU. Its period is

5.

The escape speed from the surface of a planet of mass M and radius R is

6.

The unit N/C for electric field strength is equivalent to

7.

An electron is released from rest between two charged parallel plates. It accelerates

8.

Millikan's oil drop experiment showed that

9.

A charged particle moves parallel to a uniform magnetic field. The magnetic force on it is

10.

A proton circles in a uniform magnetic field. If the field strength is doubled and the speed stays the same, the radius

For parents and teachers

How to use the results: for each kind of mistake, revisit the lesson shown.

  • Inverse-square and force calculations with masses: Newton's Law of Universal Gravitation.
  • Field strength at different altitudes, g = GM/r², field-line diagrams near and far: Gravitational Fields: Near Earth and Far Away.
  • Orbital speed, period, geostationary orbits, "weightlessness": Satellites and Circular Orbits.
  • Kepler's laws, finding a central mass, dark matter: Kepler's Laws, Black Holes and Dark Matter.
  • Negative potential energy, escape speed, black-hole radius: Gravitational Potential Energy, Escape Speed and Black Holes.
  • Coulomb's law, counting electrons: Electric Charge and Coulomb's Law.
  • Field direction, adding fields as vectors, field-line rules: Electric Fields of Point Charges and Field Lines.
  • Confusing potential with potential energy, or sign errors: Electric Potential Energy and Electric Potential.
  • E = ΔV/d and uniform fields: Uniform Electric Fields Between Parallel Plates.
  • Accelerating and deflecting charges (qΔV = ½mv², projectile-like paths): Charged Particles in Uniform Electric Fields.
  • Balanced drops and quantized charge: Millikan's Oil Drop Experiment and the Elementary Charge.
  • Fields of wires and solenoids, F = ILB sin θ, hand rules: Magnetic Fields of Currents and the Force on a Conductor.
  • F = qvB sin θ, circular paths, velocity selectors: Magnetic Force on Moving Charges and Circular Motion.
  • Mass spectrometers, cyclotrons, MRI: Field Technologies: Mass Spectrometers, Accelerators and MRI.
  • Comparing fields, fundamental forces, exchange particles: Comparing Fields and the Fundamental Forces.
  • GPS timing, satellites and society, debris, decision-making: Fields, Technology and Society.

Common unit-wide mistakes: forgetting to add Earth's radius to an altitude; squaring r when the formula has only r (potential and potential energy) or forgetting to square it (force and field); dropping the sign of a charge; and using the right hand for an electron without reversing the answer.