Physic Labs

Optics

The eye and optical instruments

Study image formation by a converging lens and an eye model: vary object distance and focal length to determine image character. Verify the thin-lens formula 1/f=1/d+1/d′1/f=1/d+1/d' and magnification.

High school

⚠ Never point a telescope or binoculars at the Sun — it can cause permanent blindness.

Equipment

  • 3D model of rays through a lens/eye (two panels)
  • Incidence-angle, refractive-index, and focal-length sliders
  • Image-position readout and virtual retina

Procedure

  1. Rays through a curved surface

    In panel 1, keep index 1.5 and vary «Incidence angle»: rays through the curved surface bend toward the axis. Shorten/lengthen «Focal length» to see stronger/weaker convergence — short f means stronger curvature and a «stronger» lens.

  2. Verify the thin-lens formula

    Place the object at several distances d (inside and outside f) and read the image position d'. Check 1/f=1/d+1/d′1/f=1/d+1/d' for d > f (real, inverted image) and observe the upright enlarged virtual image for d < f — the magnifier regime.

  3. Eye model and accommodation

    In panel 2, vary «Focal length» to mimic the crystalline lens changing curvature: distant objects need large f (flattened lens), near objects need short f (bulging). Notice the retinal image is always real and inverted — the brain «re-erects» it.

  4. Predict the instruments

    Predict the setup for a magnifier (d < f), a microscope (short-f objective forms a real magnified image, the eyepiece acts as a loupe), and a telescope (distant object → image at the focal plane). Set the sliders accordingly and check with the ray paths.

Simulation

Experiment history

Ibn al-Haytham (Alhazen) wrote the Book of Optics around 1011–1021, proving experimentally that light travels from object to eye — not rays emitted by the eye as Greeks believed — and describing the camera obscura. Eyeglasses appeared in late-13th-century Italy; the microscope and telescope in the Netherlands around 1600, Galileo turning the telescope skyward in 1609–10 to find a rugged Moon and Jupiter's moons — a lever for the astronomical revolution. Newton showed (1666) that white light is a mixture of colors dispersed by prisms according to index — his reason for building a reflecting telescope to dodge chromatic aberration. Understanding of accommodation (the lens changing curvature) matured in the 19th century with Helmholtz; the thin-lens formula 1/f=1/d+1/d′1/f=1/d+1/d' evolved from Kepler–Descartes geometrical optics into its modern form.

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