Reflection, refraction, lenses, mirrors, and interference
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Optics is the study of light and its interactions, and AP Physics 2 divides the topic into geometric optics (rays and images) and physical optics (waves, interference, and diffraction). In geometric optics, you treat light as traveling in straight lines called rays. The law of reflection states that the angle of incidence equals the angle of reflection. Snell's law, n₁ sinθ₁ = n₂ sinθ₂, governs refraction—the bending of light as it crosses between media with different indices of refraction. When light travels from a medium with a higher index to one with a lower index at a sufficiently large angle, total internal reflection occurs, trapping light inside the denser medium; this is the operating principle of fiber optics. You will analyze image formation by plane mirrors, concave mirrors, convex mirrors, converging lenses, and diverging lenses using ray tracing and the mirror/lens equation: 1/f = 1/do + 1/di. Magnification M = −di/do = hi/ho tells you the image size and orientation. Sign conventions are critical: for lenses, real images have positive di and inverted images have negative M; for mirrors, focal length is positive for concave and negative for convex. Physical optics treats light as a wave. When coherent light passes through two narrow slits, it produces an interference pattern of bright and dark fringes on a screen. Constructive interference occurs when the path difference d sinθ = mλ; destructive interference when d sinθ = (m + ½)λ. A single slit also produces a diffraction pattern, with dark fringes at a sinθ = mλ. Diffraction gratings, with many closely spaced slits, produce sharp, widely separated maxima useful for spectroscopy. Polarization refers to the orientation of the electric field oscillations in a transverse wave. Malus's law, I = I₀ cos²θ, describes the intensity of polarized light passing through a polarizer. On the AP Exam, optics problems often combine ray tracing with calculations, or ask you to predict the effect of changing wavelength or slit separation on an interference pattern.
θ_i = θ_rn1*sinθ1 = n2*sinθ2 (Snell's Law)sinθ_c = n2/n1 (n1 > n2, critical angle)1/f = 1/do + 1/diM = -di/do = hi/hof = R/2 (mirror)d*sinθ = m*λ (bright double-slit)d*sinθ = (m + ½)*λ (dark double-slit)a*sinθ = m*λ (dark single-slit)I = I0*cos²θ (Malus's Law)Answer each question one at a time. Click an option to select your answer.
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Geometric Optics: Crash Course Physics #38 by CrashCourse
AP Physics 2 Light and Optics Review by physicsbybowman
AP Physics 2 - Unit 6 Optics by Shane Barry
Quick reference for Geometric and Physical Optics. Print this out and review before the exam!
θ_i = θ_rn1*sinθ1 = n2*sinθ2 (Snell's Law)sinθ_c = n2/n1 (critical angle, n1 > n2)1/f = 1/do + 1/diM = -di/do = hi/hof = R/2 (mirror)d*sinθ = m*λ (bright double-slit)d*sinθ = (m + ½)*λ (dark double-slit)a*sinθ = m*λ (dark single-slit)I = I0*cos²θ (Malus's Law)Download official review materials for this unit.
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