The Thin-Lens Equation
A lens bends light rays so they meet again at a point, forming an image. Where that image forms depends on how far the object sits from the lens and how strongly the lens bends light, a property called its focal length. The thin-lens equation ties these three distances together, so knowing any two lets you find the third.
1/f = 1/dₒ + 1/dᵢ
- f — focal length (m): how strongly the lens bends light — where parallel rays converge
- dₒ — object distance (m): how far the object is from the lens
- dᵢ — image distance (m): how far the image forms from the lens
A converging lens has a focal length of 10 cm. An object is placed 30 cm in front of it. How far from the lens does the image form?
- f = 10 cm
- dₒ = 30 cm
- 1/dᵢ = 1/f − 1/dₒ
- 1/dᵢ = 1/10 cm − 1/30 cm = 1/15 cm
dᵢ = 15 cm
Using the same 10 cm focal-length lens, if the object is moved to 20 cm away, how far from the lens does the image form?
- 10 cm
- 20 cm
- 30 cm
For the original example (dₒ = 30 cm, dᵢ = 15 cm), what is the magnification, and what does it tell you about the image?
- m = −0.5 — inverted and half size
- m = 0.5 — upright and half size
- m = −2 — inverted and double size