Ray Optics and Optical Instruments
ЁЯУР Formula & Cheat Sheet (English)
Class 12 Physics - Quick Revision Notes
Chapter: Ray Optics and Optical Instruments (MP Board)
1. Reflection of Light (рдкреНрд░рдХрд╛рд╢ рдХрд╛ рдкрд░рд╛рд╡рд░реНрддрди)
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Laws of Reflection (рдкрд░рд╛рд╡рд░реНрддрди рдХреЗ рдирд┐рдпрдо):
- The angle of incidence ($i$) is equal to the angle of reflection ($r$). $\rightarrow \angle i = \angle r$
- The incident ray, the normal to the mirror at the point of incidence, and the reflected ray all lie in the same plane.
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Mirror Formula (рджрд░реНрдкрдг рд╕реВрддреНрд░): $$\frac{1}{f} = \frac{1}{v} + \frac{1}{u}$$
- Where:
- $f$ = Focal length (рдлреЛрдХрд╕ рджреВрд░реА)
- $v$ = Image distance (рдкреНрд░рддрд┐рдмрд┐рдореНрдм рдХреА рджреВрд░реА)
- $u$ = Object distance (рд╡рд╕реНрддреБ рдХреА рджреВрд░реА)
- Where:
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Linear Magnification (рд░реИрдЦрд┐рдХ рдЖрд╡рд░реНрдзрди - $m$): $$m = \frac{h_2}{h_1} = -\frac{v}{u}$$
- Where $h_1$ is the height of the object and $h_2$ is the height of the image.
- Note: Relation between focal length and radius of curvature ($R$): $f = \frac{R}{2}$
2. Refraction of Light (рдкреНрд░рдХрд╛рд╢ рдХрд╛ рдЕрдкрд╡рд░реНрддрди)
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Snell's Law (рд╕реНрдиреЗрд▓ рдХрд╛ рдирд┐рдпрдо): $$\frac{\sin i}{\sin r} = \text{constant} = {^1}\mu_2 = \frac{n_2}{n_1}$$
- Where ${^1}\mu_2$ is the refractive index of medium 2 with respect to medium 1.
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Absolute Refractive Index ($\mu$ or $n$): $$\mu = \frac{c}{v}$$
- Where $c$ = speed of light in vacuum, $v$ = speed of light in the medium.
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Principle of Reversibility (рдЙрддреНрдХреНрд░рдордгреАрдпрддрд╛ рдХрд╛ рд╕рд┐рджреНрдзрд╛рдиреНрдд): $${^1}\mu_2 \times {^2}\mu_1 = 1 \implies {^1}\mu_2 = \frac{1}{{^2}\mu_1}$$
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Apparent Depth (рдЖрднрд╛рд╕реА рдЧрд╣рд░рд╛рдИ): $$\mu = \frac{\text{Real Depth}}{\text{Apparent Depth}} = \frac{h}{h'}$$
- Shift in position ($x$): $x = h \left(1 - \frac{1}{\mu}\right)$
3. Total Internal Reflection (рдкреВрд░реНрдг рдЖрдВрддрд░рд┐рдХ рдкрд░рд╛рд╡рд░реНрддрди - TIR)
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Conditions for TIR:
- Light must travel from a denser medium to a rarer medium.
- The angle of incidence must be greater than the critical angle ($i > i_c$).
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Critical Angle ($i_c$): $$\sin i_c = \frac{1}{\mu}$$
4. Refraction at Spherical Surfaces & Lenses (рдЧреЛрд▓реАрдп рдкреГрд╖реНрдареЛрдВ рдкрд░ рдЕрдкрд╡рд░реНрддрди рдПрд╡рдВ рд▓реЗрдВрд╕)
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Refraction at a Spherical Surface: $$\frac{\mu_2}{v} - \frac{\mu_1}{u} = \frac{\mu_2 - \mu_1}{R}$$
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Lens MakerтАЩs Formula (рд▓реЗрдВрд╕ рдирд┐рд░реНрдорд╛рддрд╛ рд╕реВрддреНрд░): $$\frac{1}{f} = (\mu - 1) \left(\frac{1}{R_1} - \frac{1}{R_2}\right)$$ (where $\mu$ is the refractive index of the lens material with respect to the surrounding medium).
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Thin Lens Formula (рдкрддрд▓рд╛ рд▓реЗрдВрд╕ рд╕реВрддреНрд░): $$\frac{1}{f} = \frac{1}{v} - \frac{1}{u}$$
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Magnification for Lens (рд▓реЗрдВрд╕ рдХрд╛ рдЖрд╡рд░реНрдзрди): $$m = \frac{h_2}{h_1} = \frac{v}{u}$$
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Power of a Lens (рд▓реЗрдВрд╕ рдХреА рдХреНрд╖рдорддрд╛): $$P = \frac{1}{f \text{ (in meters)}} \quad \text{or} \quad P = \frac{100}{f \text{ (in cm)}}$$
- SI Unit: Dioptre (D)
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Combination of Thin Lenses in Contact (рд╕рдВрдкрд░реНрдХ рдореЗрдВ рд░рдЦреЗ рд▓реЗрдВрд╕реЛрдВ рдХрд╛ рд╕рдВрдпреЛрдЬрди): $$\frac{1}{F} = \frac{1}{f_1} + \frac{1}{f_2} + \dots$$ $$P = P_1 + P_2 + \dots$$ $$m = m_1 \times m_2 \times \dots$$
5. Refraction through a Prism (рдкреНрд░рд┐рдЬреНрдо рд╕реЗ рдЕрдкрд╡рд░реНрддрди)
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Angle of Deviation ($\delta$): $$\delta = (i + e) - A$$
- Where $A$ = Angle of the prism, $i$ = Angle of incidence, $e$ = Angle of emergence.
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Refractive Index of Prism Material: $$\mu = \frac{\sin\left(\frac{A + \delta_m}{2}\right)}{\sin\left(\frac{A}{2}\right)}$$ (where $\delta_m$ is the angle of minimum deviation).
6. Optical Instruments (рдкреНрд░рдХрд╛рд╢рд┐рдХ рдпрдВрддреНрд░)
(A) Simple Microscope (рд╕рд░рд▓ рд╕реВрдХреНрд╖реНрдорджрд░реНрд╢реА / рдЖрд╡рд░реНрдзрдХ рд▓реЗрдВрд╕)
- When final image is formed at the Least Distance of Distinct Vision ($D = 25\text{ cm}$): $$m = 1 + \frac{D}{f}$$
- When final image is formed at Infinity ($v = \infty$): $$m = \frac{D}{f}$$
(B) Compound Microscope (рд╕рдВрдпреБрдХреНрдд рд╕реВрдХреНрд╖реНрдорджрд░реНрд╢реА)
- Magnifying Power ($m$): $$m = m_o \times m_e = -\frac{v_o}{u_o} \left(1 + \frac{D}{f_e}\right)$$
- Length of the Microscope Tube ($L$): $$L = v_o + u_e$$ (Approximate: $L \approx v_o + f_e$)
(C) Astronomical Telescope (рдЦрдЧреЛрд▓реАрдп рджреВрд░рджрд░реНрд╢реА)
- Magnifying Power ($m$) when final image is at Infinity (Normal Adjustment): $$m = -\frac{f_o}{f_e}$$
- Length of the Telescope Tube ($L$): $$L = f_o + f_e$$
- Magnifying Power when final image is at Least Distance of Distinct Vision ($D$): $$m = -\frac{f_o}{f_e} \left(1 + \frac{f_e}{D}\right)$$ $$L = f_o + u_e$$
All the Best for your MP Board Class 12 Physics Examination!