Physic Labs

Optics

Converging and diverging lenses

Verify the thin-lens equation 1f=1do+1di\frac1f=\frac1{d_o}+\frac1{d_i} by varying the focal length and watching the principal rays construct the image in the 3D model. Read the image distance and magnification m=−di/dom=-d_i/d_o from the ray diagram.

Middle school

Equipment

  • Virtual converging/diverging lens on a 3D canvas
  • Focal-length slider f (readout in cm)
  • Incidence-angle and refractive-index sliders
  • Three principal rays forming the image: through center, parallel–focal, focal–parallel

Procedure

  1. Construct the image with principal rays

    In figure 1, watch three rays from the object tip: the ray through the optical center goes straight, the parallel ray refracts through the image-side focal point, and the focal ray emerges parallel. Their intersection gives the image position and orientation — read did_i in the readout.

  2. Verify the thin-lens formula

    Set focal length f = 10 cm and read the image position: for an object at do=30d_o=30 cm the formula gives di=15d_i=15 cm — compare on the readout. Bring the object closer than f: di<0d_i<0, outgoing rays diverge and the image becomes virtual on the object side.

  3. Change focal length and compute magnification

    Raise the focal-length slider: with do>fd_o>f the image moves farther and grows. At do=30d_o=30 cm, f = 10 cm we get m=−15/30=−0,5m=-15/30=-0{,}5 — a real inverted image at half size. Predict m when the object sits at do=2fd_o=2f and check on the diagram.

Simulation

Experiment history

The thin-lens formula 1/f=1/do+1/di1/f=1/d_o+1/d_i follows from refraction at two spherical surfaces by Snell's law in the paraxial limit; Renaissance opticians already knew lenses empirically — Galileo assembled his telescope in 1609 and Kepler described its optics in 1611. In Opticks (1704) Newton analyzed focal length and chromatic aberration — believing lens color defects uncorrectable, he designed the reflecting telescope in 1668. Today combining two lenses uses 1/feq=1/f1+1/f21/f_{eq}=1/f_1+1/f_2, the basis of every camera lens group and microscope objective.

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