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Engineering and Science Admissions Test (ESAT) Physics Module Syllabus

The Physics Module syllabus for Engineering and Science Admissions Test (ESAT) in full: 6 chapters, 20 topics and 52 sub-topics, every one listed below, plus 60 Physics Module flashcards with answers.

6Chapters
20Topics
52Sub-topics
60Flashcards

Physics Module syllabus: all 6 chapters

Expand any chapter to see its topics and sub-topics.

  1. Mechanics and Motion

    4 topics
    • Kinematics
      • Displacement, velocity and acceleration
      • Equations of uniformly accelerated motion (SUVAT)
      • Motion graphs and gradients/areas
      • Projectile motion
    • Forces and Newton's Laws
      • Newton's three laws of motion
      • Free-body diagrams and resultant forces
      • Friction, tension and normal contact force
    • Momentum and Impulse
      • Conservation of linear momentum
      • Elastic and inelastic collisions
      • Impulse as change of momentum
    • Moments and Equilibrium
      • Principle of moments and torque
      • Centre of mass and stability
  2. Energy, Work and Power

    3 topics
    • Work and Energy
      • Work done by a force
      • Kinetic and gravitational potential energy
      • Conservation of energy
    • Power and Efficiency
      • Power as rate of energy transfer
      • Efficiency calculations
    • Density and Pressure
      • Density and pressure in solids and fluids
      • Hydrostatic pressure and upthrust
  3. Electricity

    3 topics
    • Charge, Current and Voltage
      • Electric charge and current
      • Potential difference and EMF
    • Resistance and Circuits
      • Ohm's law and resistivity
      • Series and parallel combinations
      • I-V characteristics of components
    • Circuit Analysis
      • Kirchhoff's current and voltage laws
      • Potential dividers
      • Electrical power and energy
  4. Waves and Optics

    4 topics
    • Wave Properties
      • Wavelength, frequency, period and speed
      • Transverse and longitudinal waves
      • The wave equation v = f λ
    • Wave Behaviour
      • Reflection, refraction and total internal reflection
      • Superposition, interference and standing waves
      • Diffraction
    • The Electromagnetic Spectrum
      • Regions of the EM spectrum and their properties
    • Sound
      • Properties and speed of sound
  5. Thermal Physics, Gases and Radioactivity

    3 topics
    • Thermal Energy
      • Temperature and internal energy
      • Specific heat capacity and latent heat
      • Heat transfer mechanisms
    • Gas Laws
      • Boyle's, Charles's and pressure laws
      • The ideal gas equation
    • Radioactivity and the Nuclear Atom
      • Structure of the atom and isotopes
      • Alpha, beta and gamma radiation
      • Half-life and radioactive decay
      • Nuclear fission and fusion
  6. Magnetism, Fields and Measurement

    3 topics
    • Magnetic Fields
      • Magnetic field patterns
      • Force on a current-carrying conductor
      • Electromagnetic induction and the transformer
    • Gravitational and Field Concepts
      • Gravitational field strength
      • Weight and free fall
    • Units, Quantities and Measurement
      • SI base and derived units
      • Scalars and vectors; resolving vectors
      • Uncertainty and significant figures

Engineering and Science Admissions Test (ESAT) Physics Module flashcards — 60 questions with answers

  1. State the three SUVAT equations of motion for constant acceleration (excluding the one that omits final velocity).

    $v = u + at$, $\;s = ut + \frac{1}{2}at^{2}$, $\;v^{2} = u^{2} + 2as$, where $u$ is initial velocity, $v$ final velocity, $a$ acceleration, $s$ displacement and $t$ time.

  2. What is the difference between distance and displacement, and between speed and velocity?

    Distance and speed are scalars (magnitude only); displacement and velocity are vectors (magnitude and direction). Displacement is the straight-line change in position; velocity is rate of change of displacement.

  3. On a velocity-time graph, what do the gradient and the area under the line represent?

    The gradient gives acceleration ($a = \frac{\Delta v}{\Delta t}$); the area under the line gives displacement.

  4. For an object in free fall (no air resistance), what is its acceleration and the equation for vertical distance fallen from rest?

    Acceleration is $g \approx 9.81\ \mathrm{m\,s^{-2}}$ downward. Distance fallen from rest: $s = \frac{1}{2}gt^{2}$.

  5. For a projectile launched at speed $u$ and angle $\theta$, give the horizontal and vertical components of the initial velocity.

    Horizontal: $u_{x} = u\cos\theta$ (constant). Vertical: $u_{y} = u\sin\theta$ (changes under gravity).

  6. State Newton's three laws of motion.

    1st: an object stays at rest or in uniform motion unless acted on by a resultant force. 2nd: $F = ma$ (resultant force = mass × acceleration). 3rd: every action has an equal and opposite reaction on a different body.

  7. Write Newton's second law in terms of momentum.

    $F = \frac{\Delta p}{\Delta t}$, i.e. resultant force equals the rate of change of momentum.

  8. What is the weight of an object and how is it calculated?

    Weight is the gravitational force on a mass: $W = mg$, where $g$ is gravitational field strength ($\approx 9.81\ \mathrm{N\,kg^{-1}}$ on Earth). It is a vector measured in newtons.

  9. Define terminal velocity.

    The constant maximum velocity reached by a falling object when the upward drag (and any upthrust) equals the downward weight, giving zero resultant force and zero acceleration.

  10. State the difference between mass and weight.

    Mass is the amount of matter (scalar, kg, constant everywhere); weight is the gravitational force on that mass (vector, N, depends on local $g$).

  11. Define linear momentum and give its formula and units.

    Momentum is the product of mass and velocity: $p = mv$. It is a vector with units $\mathrm{kg\,m\,s^{-1}}$ (equivalent to $\mathrm{N\,s}$).

  12. State the principle of conservation of momentum.

    In a closed system with no external resultant force, total momentum before a collision or explosion equals total momentum after: $\sum m u = \sum m v$.

  13. Define impulse and relate it to momentum.

    Impulse is force × time: $\text{Impulse} = F\,\Delta t = \Delta p$ (the change in momentum). Units are $\mathrm{N\,s}$ or $\mathrm{kg\,m\,s^{-1}}$.

  14. Compare elastic and inelastic collisions.

    In both, momentum is conserved. In an elastic collision kinetic energy is also conserved; in an inelastic collision some kinetic energy is converted to other forms (e.g. heat, sound).

  15. On a force-time graph, what does the area under the curve represent?

    The area under a force-time graph represents the impulse, equal to the change in momentum $\Delta p$.

  16. Define the moment of a force and give its formula and units.

    A moment is the turning effect of a force: $M = F \times d$, where $d$ is the perpendicular distance from the pivot to the line of action of the force. Units: $\mathrm{N\,m}$.

  17. State the principle of moments for an object in equilibrium.

    For a body in rotational equilibrium, the sum of clockwise moments about any pivot equals the sum of anticlockwise moments: $\sum M_{\text{cw}} = \sum M_{\text{acw}}$.

  18. What two conditions must be satisfied for an object to be in complete (static) equilibrium?

    1) The resultant force is zero (forces balance in all directions). 2) The resultant moment about any point is zero (clockwise moments = anticlockwise moments).

  19. What is the centre of mass (centre of gravity) of an object?

    The single point at which the entire weight of the object can be considered to act. For a uniform symmetric object it lies at the geometric centre.

  20. Define a couple and its moment (torque).

    A couple is a pair of equal, opposite, parallel forces whose lines of action do not coincide. Its moment (torque) is $\tau = F \times d$, where $d$ is the perpendicular distance between the two forces.

Show the other 40 Physics Module flashcards
  1. State the equations for kinetic energy and gravitational potential energy.

    Kinetic energy: $E_{k} = \frac{1}{2}mv^{2}$. Gravitational potential energy: $E_{p} = mgh$.

  2. Define work done by a force and give its formula.

    Work done is energy transferred when a force moves its point of application: $W = Fs\cos\theta$, where $\theta$ is the angle between force and displacement. Units: joules (J).

  3. State the principle of conservation of energy.

    Energy cannot be created or destroyed, only transferred or transformed from one form to another; the total energy of a closed system remains constant.

  4. Using energy conservation, derive the speed of an object that falls freely through height $h$ from rest.

    $mgh = \frac{1}{2}mv^{2} \Rightarrow v = \sqrt{2gh}$.

  5. Define power and give two formulas for it.

    Power is the rate of energy transfer (work done per unit time): $P = \frac{W}{t} = \frac{E}{t}$. For motion at constant velocity: $P = Fv$. Units: watts (W).

  6. Define efficiency and give its formula.

    Efficiency is the fraction of input energy usefully transferred: $\text{efficiency} = \frac{\text{useful energy (or power) output}}{\text{total energy (or power) input}} \times 100\%$. It is always $< 100\%$ for real machines.

  7. Define density and give its formula and SI units.

    Density is mass per unit volume: $\rho = \frac{m}{V}$. SI units: $\mathrm{kg\,m^{-3}}$.

  8. Define pressure and give its formula and SI unit.

    Pressure is force per unit area acting perpendicular to a surface: $P = \frac{F}{A}$. SI unit: the pascal, $1\ \mathrm{Pa} = 1\ \mathrm{N\,m^{-2}}$.

  9. Give the equation for pressure due to a column of fluid of height $h$.

    $P = \rho g h$, where $\rho$ is fluid density, $g$ gravitational field strength and $h$ the depth below the surface.

  10. Define electric current and state its formula and unit.

    Current is the rate of flow of charge: $I = \frac{Q}{t}$. Unit: the ampere (A), where $1\ \mathrm{A} = 1\ \mathrm{C\,s^{-1}}$.

  11. Define potential difference (voltage) and state its formula.

    Potential difference is the energy transferred per unit charge between two points: $V = \frac{W}{Q}$. Unit: the volt, $1\ \mathrm{V} = 1\ \mathrm{J\,C^{-1}}$.

  12. What is the elementary charge, and how is charge related to a number of electrons?

    The elementary charge is $e = 1.6 \times 10^{-19}\ \mathrm{C}$. Total charge $Q = ne$, where $n$ is the number of electrons.

  13. State Ohm's law and the equation linking voltage, current and resistance.

    For an ohmic conductor at constant temperature, current is proportional to potential difference: $V = IR$, where $R$ is resistance in ohms ($\Omega$).

  14. Give the formula for the resistance of a wire in terms of resistivity.

    $R = \frac{\rho L}{A}$, where $\rho$ is resistivity ($\Omega\,\mathrm{m}$), $L$ is length and $A$ is cross-sectional area.

  15. Write the formulas for total resistance of resistors in series and in parallel.

    Series: $R_{\text{total}} = R_{1} + R_{2} + \dots$. Parallel: $\frac{1}{R_{\text{total}}} = \frac{1}{R_{1}} + \frac{1}{R_{2}} + \dots$.

  16. State three equations for electrical power dissipated in a component.

    $P = IV = I^{2}R = \frac{V^{2}}{R}$. Electrical energy is then $E = Pt = IVt$.

  17. State Kirchhoff's two circuit laws.

    Current law: the sum of currents into a junction equals the sum out (conservation of charge). Voltage law: the sum of e.m.f.s around any loop equals the sum of potential differences (conservation of energy).

  18. How do current and potential difference behave in series and parallel circuits?

    Series: current is the same everywhere; voltage is shared (adds up) across components. Parallel: voltage is the same across each branch; current is shared (splits) between branches.

  19. Describe the I-V characteristic of a filament lamp and why it is non-ohmic.

    The graph is an S-shaped curve: as current increases the filament heats up, raising its resistance, so the gradient decreases. It is non-ohmic because resistance changes with temperature.

  20. State the wave equation linking speed, frequency and wavelength.

    $v = f\lambda$, where $v$ is wave speed ($\mathrm{m\,s^{-1}}$), $f$ is frequency (Hz) and $\lambda$ is wavelength (m). Also $f = \frac{1}{T}$ where $T$ is the period.

  21. Distinguish transverse and longitudinal waves, giving an example of each.

    Transverse: oscillations are perpendicular to the direction of energy transfer (e.g. light, water waves). Longitudinal: oscillations are parallel to energy transfer, with compressions and rarefactions (e.g. sound).

  22. Define amplitude, wavelength and frequency of a wave.

    Amplitude: maximum displacement from the rest position. Wavelength: distance between two adjacent points in phase (e.g. crest to crest). Frequency: number of complete waves passing a point per second (Hz).

  23. Name the four wave behaviours and briefly define each.

    Reflection: bouncing off a boundary. Refraction: change of direction due to a change in speed entering a new medium. Diffraction: spreading of waves through a gap or around an obstacle. Interference: superposition of two waves giving reinforcement or cancellation.

  24. State the law of reflection.

    The angle of incidence equals the angle of reflection ($\theta_{i} = \theta_{r}$), both measured from the normal, and the incident ray, reflected ray and normal lie in the same plane.

  25. List the regions of the electromagnetic spectrum in order of increasing frequency.

    Radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, gamma rays (increasing frequency and energy, decreasing wavelength).

  26. What do all electromagnetic waves have in common, including their speed in a vacuum?

    They are transverse, transfer energy, can travel through a vacuum, and all travel at the same speed in vacuum: $c = 3.0 \times 10^{8}\ \mathrm{m\,s^{-1}}$.

  27. What is the audible frequency range for humans, and how does the speed of sound in air compare to its speed in solids?

    Humans hear roughly $20\ \mathrm{Hz}$ to $20\,000\ \mathrm{Hz}$. Sound travels faster in solids than in liquids, and faster in liquids than in gases (it needs a medium and cannot travel through a vacuum).

  28. Define specific heat capacity and give its equation.

    Specific heat capacity is the energy needed to raise the temperature of $1\ \mathrm{kg}$ of a substance by $1\ \mathrm{K}$. Equation: $Q = mc\Delta\theta$, with units of $c$ being $\mathrm{J\,kg^{-1}\,K^{-1}}$.

  29. Define specific latent heat and give its equation.

    Specific latent heat is the energy needed to change the state of $1\ \mathrm{kg}$ of a substance with no temperature change: $Q = mL$. Units of $L$: $\mathrm{J\,kg^{-1}}$ (fusion for melting, vaporisation for boiling).

  30. State the three combined gas laws (Boyle's, Charles's, Pressure law) and the ideal gas relation.

    Boyle: $PV = \text{const}$ (constant $T$). Charles: $\frac{V}{T} = \text{const}$ (constant $P$). Pressure law: $\frac{P}{T} = \text{const}$ (constant $V$). Combined: $\frac{PV}{T} = \text{const}$, with $T$ in kelvin.

  31. Name the three types of nuclear radiation and rank their penetrating and ionising power.

    Alpha ($\alpha$): most ionising, least penetrating (stopped by paper). Beta ($\beta$): medium (stopped by a few mm of aluminium). Gamma ($\gamma$): least ionising, most penetrating (reduced by thick lead/concrete).

  32. Define half-life of a radioactive isotope.

    The half-life is the average time taken for half the radioactive nuclei in a sample to decay, or equivalently for the activity (count rate) to fall to half its initial value.

  33. Write the changes in an alpha decay and a beta-minus decay.

    Alpha: $^{A}_{Z}X \rightarrow\ ^{A-4}_{Z-2}Y +\ ^{4}_{2}\alpha$. Beta-minus: $^{A}_{Z}X \rightarrow\ ^{\;A}_{Z+1}Y +\ ^{\;\;0}_{-1}\beta$ (a neutron becomes a proton plus an electron).

  34. Describe the basic structure of the nuclear atom (constituents and their relative charges).

    A small dense nucleus of protons (charge $+1$) and neutrons (charge $0$) surrounded by orbiting electrons (charge $-1$). Atomic number $Z$ = number of protons; mass number $A$ = protons + neutrons.

  35. Sketch the field pattern and force direction for magnetic fields, and state the motor-effect rule.

    Magnetic field lines run from north to south pole outside a magnet. A current-carrying wire in a field experiences a force given by Fleming's left-hand rule (thumb = force/motion, first finger = field, second finger = current).

  36. What does electromagnetic induction require, and what is its consequence (Faraday/Lenz)?

    A change in magnetic flux linking a conductor induces an e.m.f. The induced e.m.f. is proportional to the rate of change of flux (Faraday), and it opposes the change producing it (Lenz's law).

  37. Give the equation for gravitational field strength near Earth and its meaning.

    $g = \frac{F}{m}$ (force per unit mass on a test mass). Near Earth's surface $g \approx 9.81\ \mathrm{N\,kg^{-1}}$, numerically equal to the free-fall acceleration.

  38. List the SI base quantities and their units for mass, length, time, current and temperature.

    Mass: kilogram (kg); length: metre (m); time: second (s); electric current: ampere (A); thermodynamic temperature: kelvin (K). (Also amount: mole; luminous intensity: candela.)

  39. Distinguish a scalar from a vector and give two examples of each.

    A scalar has magnitude only (e.g. mass, energy, speed, temperature). A vector has magnitude and direction (e.g. force, velocity, acceleration, momentum).

  40. Give the SI prefixes and powers of ten for nano, micro, milli, kilo, mega and giga.

    nano $= 10^{-9}$, micro $= 10^{-6}$, milli $= 10^{-3}$, kilo $= 10^{3}$, mega $= 10^{6}$, giga $= 10^{9}$.

Engineering and Science Admissions Test (ESAT) Physics Module FAQ

What is in the Engineering and Science Admissions Test (ESAT) Physics Module syllabus?

Engineering and Science Admissions Test (ESAT) Physics Module is split into 6 chapters: Mechanics and Motion, Energy, Work and Power, Electricity, Waves and Optics, Thermal Physics, Gases and Radioactivity and Magnetism, Fields and Measurement. Together they contain 20 topics and 52 sub-topics.

How many chapters are in Engineering and Science Admissions Test (ESAT) Physics Module?

6 chapters, containing 20 topics and 52 sub-topics. The largest chapter is Mechanics and Motion, with 4 topics.

Are there flashcards for Engineering and Science Admissions Test (ESAT) Physics Module?

Yes — a 60-card Physics Module deck, printed in full in the flashcards section of this page and available in the Examius app with spaced repetition. The free plan covers one exam of your choice, including its flashcards; Examius Pro, a one-time purchase, unlocks every other exam and deck.