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HSC Physics exam 2026Exam: Thu 5 Nov · NESA timetable

Your HSC Physics exam:

When and how long

  • Physics9.25 am to 12.30 pm3 h plus 5 min reading time

NESA: the exam start time shown on your timetable is when reading time begins, and you must arrive well before it. Finishing times marked approximate are shown as approx.

Source: 2026 HSC written exam timetable (NESA), checked Wednesday 23 September 2026. Where a start time, reading time or duration isn't shown, the timetable doesn't publish it: check your personal timetable and the front of your paper.

Paper format

Higher School Certificate Examination - Physics: 100 marks, 3 h writing time plus 5 minutes reading time.

  • Section I - Objective response20 marks
  • Section II - Short answer and extended response80 marks

NESA HSC exam specification for the Physics Stage 6 (2017) syllabus: 3 hours plus 5 minutes reading time, 100 marks. Section I is objective-response questions worth 20 marks. Section II is worth 80 marks: 20 to 25 items (questions may contain parts), at least two of them worth 7 to 9 marks. There is no Section III. The time split per section is our suggestion.

From the official specification: source.

Most-examined dot points

From 305 questions on the official NESA papers (2019 to 2025), mapped to the syllabus. Past frequency is a guide to what to secure, not a prediction.

  1. Electromagnetic induction25 questions · examined in 7 of 7 years
  2. Projectile motion explained20 questions · examined in 7 of 7 years
  3. Spectroscopy18 questions · examined in 7 of 7 years
  4. Quantum model of light and the photoelectric effect17 questions · examined in 7 of 7 years
  5. Charged particles in electric fields explained15 questions · examined in 7 of 7 years
  6. Wave model of light15 questions · examined in 7 of 7 years
  7. DC and AC motors13 questions · examined in 6 of 7 years
  8. Force on current-carrying conductors13 questions · examined in 7 of 7 years

See every dot point in the exam trends.

Night-before and exam-morning checklists

The night before

  • Check your personalised timetable on Students Online: the start time shown is when reading time begins.[2]
  • Confirm your venue and the start time.[1]
  • Pack a clear bag: several black pens (no erasable ink), 2B pencils, sharpener, eraser and a ruler.[1]
  • Pack an approved calculator (check NESA's list) and a compass or protractor if the exam needs them.[1]
  • Fill a clear, label-free water bottle.[1]
  • A plain watch only if you want one (no smart or programmable watch); it goes on the desk.[1]
  • Stop revising around 7 to 8 pm, set two alarms and sleep.[1]

Exam morning

  • Eat a real breakfast.[1]
  • Arrive well before the start time to allow for seating and checks.[2]
  • Leave your phone and other electronic devices outside the exam room.[1]
  • Use the bathroom before you go in.[1]
  • In reading time, read and plan only: no writing, marking or annotating.[1]
  • You can't leave in the first hour or the last 15 minutes.[1]
  1. HSC exam day: what to actually expect
  2. NESA: HSC written exam timetable

Exam-week survival kit: The last 7 days · The night before and exam morning · What to bring, and what's banned · How to use reading time · If you're sick or something goes wrong · Handling exam-week stress.

Last-week revision

Syllabus by module

HSC Physics cram sheet

Key formulas, definitions and facts copied from our Physics syllabus pages, most-examined topics first. One page when printed.

Module 5: Advanced Mechanics

Components: v0x=v0cos⁡θv_{0x} = v_0\cos\theta, v0y=v0sin⁡θv_{0y} = v_0\sin\theta.

From: Projectile motion explained

Banked track (frictionless): Ncos⁡θ=mgN\cos\theta = mg, Nsin⁡θ=mv2rN\sin\theta = \dfrac{mv^2}{r}, giving the design speed tan⁡θ=v2rg\tan\theta = \dfrac{v^2}{rg}.

From: Non-uniform circular motion (banked tracks, conical pendulums, vertical circles) explained

Gravitational potential energy in a radial field: U=−GMmrU = -\dfrac{GMm}{r}, with U=0U = 0 taken at r=∞r = \infty. UU is negative for every finite rr.

From: Gravitational potential energy and escape velocity explained

For a circular orbit of radius rr: K=GMm2rK = \dfrac{GMm}{2r}, U=−GMmrU = -\dfrac{GMm}{r}, E=K+U=−GMm2rE = K + U = -\dfrac{GMm}{2r}.

From: Conservation of energy in orbital motion explained

Module 6: Electromagnetism

Field between parallel plates: E=VdE = \dfrac{V}{d} (points from the ++ plate to the −- plate).

From: Charged particles in electric fields explained

Force on a wire in a field: F=BILsin⁡θF = BIL\sin\theta (maximum F=BILF = BIL at θ=90∘\theta = 90^{\circ}; zero at θ=0∘\theta = 0^{\circ} or 180∘180^{\circ}). Direction from the right-hand rule.

From: Force on current-carrying conductors

Faraday's law: ε=−NdΦdt\varepsilon = -N\dfrac{d\Phi}{dt}, where Φ=BAcos⁡θ\Phi = BA\cos\theta is the flux through one turn.

From: Electromagnetic induction

Torque on a current loop: τ=nBIAcos⁡θ\tau = nBIA\cos\theta (θ\theta measured between the coil's plane and the field); maximum τmax⁡=nBIA\tau_{\max} = nBIA at θ=0∘\theta = 0^{\circ} (plane parallel to field), zero at θ=90∘\theta = 90^{\circ} (plane perpendicular to field, the dead spot).

From: DC and AC motors

Module 7: The Nature of Light

Double-slit maxima: dsin⁡θ=mλd\sin\theta = m\lambda; minima: dsin⁡θ=(m+12)λd\sin\theta = (m + \tfrac{1}{2})\lambda; fringe spacing (small angle): Δy=λLd\Delta y = \dfrac{\lambda L}{d}.

From: Wave model of light

Photon energy from an atomic transition: hf=Ei−Efhf = E_i - E_f.

From: Spectroscopy

Photon energy: E=hf=hcλE = hf = \dfrac{hc}{\lambda}.

From: Quantum model of light and the photoelectric effect

Lorentz factor: γ=11−v2/c2\gamma = \dfrac{1}{\sqrt{1 - v^2/c^2}}, always ≥1\geq 1, equal to 11 only when v=0v = 0, and →∞\to \infty as v→cv \to c.

From: Special relativity

Module 8: From the Universe to the Atom

Wien's law: λmax⁡T=b\lambda_{\max} T = b, with b=2.898×10−3 m Kb = 2.898 \times 10^{-3}\ \text{m K}.

From: Stellar evolution and nucleosynthesis

Bohr's postulates: (1) stationary non-radiating orbits; (2) quantised angular momentum mevr=nh/2πm_e v r = n h / 2\pi; (3) photon energy on transition hf=Ei−Efhf = E_i - E_f.

From: Bohr model and the Balmer-Rydberg formula

Fermions (matter, spin 12\tfrac{1}{2}): 6 quarks (charge +23+\tfrac{2}{3} or −13-\tfrac{1}{3}, in u,d ∣ c,s ∣ t,bu,d\,|\,c,s\,|\,t,b) and 6 leptons (e,μ,τe,\mu,\tau each with charge −1-1, plus their neutral neutrinos), in three generations.

From: The Standard Model of particle physics

Decay law: N(t)=N0e−λtN(t) = N_0 e^{-\lambda t}, equivalently N(t)=N0(12)t/T1/2N(t) = N_0 \left(\dfrac{1}{2}\right)^{t/T_{1/2}}.

From: Radioactive decay and half-life
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