Geometric Optics
Geometric optics treats light as rays that travel in straight lines and obey simple reflection and refraction laws. The thin-lens equation and mirror equation allow us to locate images formed by optical elements.
Key Concepts
- Law of reflection: θᵢ = θᵣ
- Snell's law: n₁sinθ₁ = n₂sinθ₂
- Thin lens equation: 1/f = 1/dₒ + 1/dᵢ
- Magnification: m = -dᵢ/dₒ
- Critical angle for total internal reflection: sinθ_c = n₂/n₁
Key Equations
Example Problem
An object is placed 30 cm from a converging lens with f = 10 cm. Find the image distance and magnification.
1/dᵢ = 1/f - 1/dₒ = 1/10 - 1/30 = 2/30 → dᵢ = 15 cm. m = -dᵢ/dₒ = -15/30 = -0.5 (inverted, half-size).
Exercises
7 problemsAn object 40 cm from a converging lens (f=15 cm). Find the image distance dᵢ in cm.
For the same setup (dₒ=40 cm, f=15 cm), find the magnification m.
Light travels from glass (n=1.5) to air (n=1.0). Find the critical angle for total internal reflection in degrees.
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Upgrade to Pro →A ray in air hits glass (n=1.5) at 45° from the normal. Find the refraction angle in the glass in degrees.
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Upgrade to Pro →A concave mirror has f = 20 cm. An object is at dₒ = 60 cm. Find dᵢ in cm.
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Upgrade to Pro →Two thin lenses with f₁=20 cm and f₂=30 cm are in contact. Find the combined focal length in cm.
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Upgrade to Pro →A fish in water (n=1.33) is 2.0 m deep. At what apparent depth does it appear to an observer in air?
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Upgrade to Pro →Key Takeaways
- Snell's law governs refraction at interfaces between media of different refractive index
- The thin-lens equation locates images; sign conventions determine real vs. virtual
- Total internal reflection occurs above the critical angle
- Magnification tells the ratio of image to object size with sign indicating orientation