Geometric Optics
Geometric optics treats light as rays that travel in straight lines, bending at interfaces according to Snell's law. This model accurately describes mirrors, lenses, and optical instruments whenever light wavelengths are much smaller than the objects involved.
Key Concepts
Key Equations
Image Formed by a Converging Lens
A converging lens has focal length . An object is placed from the lens. Find the image distance and magnification.
Apply the thin lens equation.
So . The positive value means the image is real and on the far side of the lens.
Calculate the magnification.
The image is real, inverted (), and twice the size of the object.
Exercises
7 problemsA ray of light travels from air () into glass () at an angle of incidence of . What is the angle of refraction (in degrees)?
Find the critical angle (in degrees) for total internal reflection at a glass–air interface where the glass has refractive index .
A converging lens of focal length has an object placed from it. What is the image distance (in cm)?
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Upgrade to Pro →For the lens in the previous problem (, , ), what is the lateral magnification ? (dimensionless)
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Upgrade to Pro →A diverging lens has focal length . An object is placed from the lens. Find the image distance (in cm).
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Upgrade to Pro →A concave mirror has radius of curvature . An object is placed in front of it. Find the image distance (in cm).
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Upgrade to Pro →What is the speed of light (in m/s) inside a medium with refractive index ? Use .
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Upgrade to Pro →Key Takeaways
- Snell's law governs refraction; total internal reflection occurs when .
- The thin lens and mirror equations share the same form: ; magnification is .
- Converging lenses () can produce real inverted images or virtual upright images depending on whether the object is beyond or inside the focal point.