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  1. Subjects
  2. Physics
  3. D Fields

D Fields

How fields describe forces at a distance: gravitational, electric and magnetic fields, the motion of masses and charges in them, and electromagnetic induction.

  • IB Physics
  • SL and HL

4 subtopics in Fields

Each one has its own page once something is published for it.

  1. D.1Gravitational fields101 questions · notes · 90 quick fire
  2. D.2Electric and magnetic fields110 questions · notes · 100 quick fire
  3. D.3Motion in electromagnetic fields83 questions · notes · 60 quick fire
  4. D.4InductionHL only68 questions · notes · 55 quick fire

Key terms introduced here

Each is in the Physics glossary, with every other term in the subject.

Equipotential surface

A surface on which every point has the same potential; no work is done moving along it, and field lines cross it at right angles.

Lenz’s law

The direction of an induced emf is such that the current it would produce opposes the change in flux that causes it; a consequence of the conservation of energy.

Magnetic flux

For a flat area AAA in a uniform field, Φ=BAcos⁡θ\Phi = BA\cos\thetaΦ=BAcosθ, where θ\thetaθ is the angle between the field and the normal to the area; measured in webers.

An overview of D Fields

5 min readLast reviewed 14 Oct 2026

A field describes how a mass, a charge or a current changes the space around it, so that another mass, charge or current placed there feels a force without any contact. Theme D builds this one idea for gravity, for electric charge and for magnetism, then uses it to explain orbits, the motion of charged particles and the generation of electricity.

How the four subtopics fit together

Four boxes for the subtopics of Fields. D.1 Gravitational fields links to D.2 Electric and magnetic fields through the same field model (inverse-square law, field lines, potential), and to D.3 through circular motion under a central force.
D.1 and D.2 build the same field model for masses and for charges; D.3 uses it to predict how charged particles and currents move, and D.4 reverses the link, using motion in a magnetic field to produce an emf. D.4, in orange, is studied at HL only.

D.1 Gravitational fields starts with Kepler’s laws of planetary motion and Newton’s law of gravitation, F=Gm1m2/r2F = Gm_1m_2/r^2F=Gm1​m2​/r2. It defines gravitational field strength as force per unit mass, pictures fields with field lines, and explains why satellites and planets move in orbits, with Kepler’s third law derived from the field.

D.2 Electric and magnetic fields applies the same model to charge. Coulomb’s law, F=kq1q2/r2F = kq_1q_2/r^2F=kq1​q2​/r2, has the same inverse-square form as Newton’s law, but charges can repel as well as attract. Electric field strength, field lines between plates and around charges, Millikan’s evidence that charge is quantised, and the magnetic field patterns of magnets, wires and solenoids all belong here.

D.3 Motion in electromagnetic fields asks what fields do to moving charges. A charge in a uniform electric field follows a parabola, like a projectile; a charge moving across a magnetic field follows a circle, like a satellite; and a current-carrying wire in a magnetic field feels a force, which is how electric motors work.

D.4 Induction (HL only) turns the last idea round. When the magnetic flux through a circuit changes, an emf is induced (Faraday’s law), in a direction that opposes the change (Lenz’s law). This is how the generators in power stations produce most of the world’s electricity.

Big ideas across the theme

One field model for several forces

Gravitational and electric fields are described with the same set of tools: a force law, a field strength (force per unit mass or per unit charge), field lines whose spacing shows strength, and, at HL, potential, potential energy and equipotential surfaces. Learning the model once for gravity makes the electric version faster to learn, and comparing the two shows what is different: gravity is always attractive and very weak, while electric forces can attract or repel and are enormously stronger.

Action at a distance and the field idea

Newton was uneasy that his law described a force acting across empty space. The field model answers this by giving each point in space a property, the field, that acts on whatever is placed there. In electromagnetism the field turned out to be physically real: a changing electric field produces a magnetic field and vice versa, and together they travel as light and other electromagnetic waves (C.2).

Energy in fields

Fields store energy. A satellite trades potential energy for kinetic energy as it moves in an elliptical orbit, an electron accelerated through a potential difference gains kinetic energy, and in D.4 mechanical work done against a magnetic force becomes electrical energy. Each is the conservation of energy from A.3, applied to a field.

Links to other themes

  • Circular motion and Newton’s laws (A.2) explain orbits in D.1 and the circular paths of charges in D.3.

  • Projectile motion (A.1) is the model for a charge moving through a uniform electric field.

  • Current, potential difference and emf (B.5) are used throughout D.2 to D.4.

  • Coulomb’s law explains alpha-particle scattering (E.1), and the balance between gravity and pressure keeps stars stable (E.5).

Standard level and higher level

HL only

HL students study D.4 Induction in full and extra sections on potential and energy within D.1 and D.2. D.3 is the same at both levels.

Subtopic

SL and HL

HL only

D.1 Gravitational fields

Kepler’s three laws; Newton’s law of gravitation; when extended bodies act as point masses; gravitational field strength g=GM/r2g = GM/r^2g=GM/r2; field lines; circular orbits, orbital speed and period, Kepler’s third law derived

Gravitational potential energy Ep=−Gm1m2/rE_\mathrm{p} = -Gm_1m_2/rEp​=−Gm1​m2​/r and potential Vg=−GM/rV_\mathrm{g} = -GM/rVg​=−GM/r; potential gradient g=−ΔVg/Δrg = -\Delta V_\mathrm{g}/\Delta rg=−ΔVg​/Δr; work done W=mΔVgW = m\Delta V_\mathrm{g}W=mΔVg​; equipotential surfaces and their relation to field lines; escape speed; the energy of an orbit and of changing orbit; the effect of atmospheric drag on a satellite

D.2 Electric and magnetic fields

Charge and its conservation; Coulomb’s law; Millikan’s experiment; charging by friction, contact and induction; electric field strength and field lines; the uniform field between plates, E=V/dE = V/dE=V/d; magnetic field lines

Electric potential energy Ep=kq1q2/rE_\mathrm{p} = kq_1q_2/rEp​=kq1​q2​/r and potential Ve=kQ/rV_\mathrm{e} = kQ/rVe​=kQ/r; potential gradient E=−ΔVe/ΔrE = -\Delta V_\mathrm{e}/\Delta rE=−ΔVe​/Δr; work done W=qΔVeW = q\Delta V_\mathrm{e}W=qΔVe​; equipotential surfaces for charges, spheres and plates

D.3 Motion in electromagnetic fields

The whole subtopic

—

D.4 Induction

—

The whole subtopic: magnetic flux, Faraday’s and Lenz’s laws, emf induced in moving conductors and rotating coils

At SL the theme concentrates on forces and field strengths: calculating forces between masses and charges, sketching field patterns, and predicting the motion of satellites and charged particles. At HL the same fields are also described by energy. Potential and equipotential surfaces map a field as contour lines map a landscape, and they make it possible to calculate how much energy a spacecraft needs to escape a planet or to change orbit, how much work moves a charge between two points, and, in D.4, how mechanical energy becomes electrical energy in a generator.

Flashcards for D

The official decks for this part of the syllabus.

  • D.1 Gravitational fields211 cards
  • D.2 Electric and magnetic fields265 cards
  • D.3 Motion in electromagnetic fields143 cards
  • D.4 Induction165 cards

From the data booklet

The entries of the physics data booklet that D uses. Each opens in the explained booklet.

  • Acceleration of free fallFundamental constants
  • Gravitational constantFundamental constants
  • Coulomb constantFundamental constants
  • Permittivity of free spaceFundamental constants
  • Permeability of free spaceFundamental constants
  • Elementary chargeFundamental constants
  • Electron rest massFundamental constants
  • 1 astronomical unit (AU) =1.50×1011 m= 1.50\times10^{11}\ \mathrm{m}=1.50×1011 mUnit conversions
  • Newton’s law of gravitationD. Fields › Standard level and higher level › D.1 Gravitational fieldsF=Gm1m2r2F = G\frac{m_1 m_2}{r^2}F=Gr2m1​m2​​
  • Gravitational field strengthD. Fields › Standard level and higher level › D.1 Gravitational fieldsg=Fm=GMr2g = \frac{F}{m} = G\frac{M}{r^2}g=mF​=Gr2M​

And 19 more in the data booklet.

On this page

  • Subtopics
  • Key terms
  • Notes
  • Flashcards
  • Data booklet

Published for D

Exam-style questions
326
Notes pages
5
Quick-fire questions
320
Key terms
87
Counted on 20 October 2026Open it in Augment

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