Physics 11–12 · Year 11

Image formation with converging lenses and curved mirrors on an optical bench (syllabus practical)

Module 3: Waves and Thermodynamics (Ray Model of Light)

Practical, model not builtLow risk

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The idea

Rays from each point of an object are redirected by a lens or mirror to meet at an image point whose position and size follow from the focal length.

What you need

  • Optical bench with metre scale, illuminated object (crossed arrows or an LED lamp behind a cut-out), white screen
  • Converging lenses of focal length 10 cm and 20 cm, concave mirror of focal length 15 cm, lens holders
  • Ray box and lens sections for ray diagrams on paper

How to do it

  1. Find the focal length roughly by focusing a distant window onto the screen.
  2. Set the object at 30.0 cm from the 10 cm lens; move the screen until the image is sharp and record the image distance and the image height.
  3. Repeat at object distances of 25, 20, 15 and 12 cm; then place the object at 8 cm and view the enlarged virtual image through the lens.
  4. Plot 1/v against 1/u; the intercepts give 1/f.
  5. Repeat with the concave mirror using a half-screen beside the object.

What you should see

For f = 10.0 cm and u = 30.0 cm the image forms at v = 15.0 cm, real, inverted and half the object's height; at u = 15.0 cm it forms at 30.0 cm and is twice the height. The 1/v against 1/u graph is a straight line of gradient -1 with both intercepts at 0.100 per cm. Inside the focal length no image forms on the screen and the eye sees an upright enlarged virtual image.

What changes

What you change
object distance
What you measure
image distance and magnification
What you keep the same
  • same lens
  • object height
  • screen perpendicular to the axis

Common misconceptions

Each of these ideas is wrong, and the activity is a chance to test it.

  • Covering half the lens removes half the image; the whole image remains, only dimmer.
  • The image sits at the focal point for every object; only very distant objects image at the focus.

Safety card

Low riskLearners carry it out

Hazards

  • hot lamp housing
  • focused sunlight if a window is used

Controls

  • use LED lamps
  • never focus the Sun onto skin or paper

Note

Record the activity in RiskAssess (https://www.riskassess.com.au/) and follow the Science ASSIST risk management information sheet (https://asta.edu.au/resource/ais-risk-management-and-risk-assessment/).

Curriculum references

The NSW syllabus outcomes and Australian Curriculum v9 codes this activity supports. They are references, not a verified or complete curriculum alignment.

  • Physics Stage 6 Syllabus (2017), current: Year 11 until the end of 2026, Year 12 until Term 3 2027PH11-10PH11/12-3
  • Australian Curriculum v9No Australian Curriculum v9 code is listed.

Sources

The pages the author read to write this activity.

  1. www.nsw.gov.au/sites/default/files/noindex/2025-03/physics-stage-6-syllabus-2017.docx
  2. education.nsw.gov.au/content/dam/main-education/teaching-and-learning/curriculum/key-learning-areas/science/s-6/physics/Physics-module-3-guide.docx
  3. phet.colorado.edu/en/simulations/geometric-optics

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