Level 4 — ApplicationOptics

Optics

50 marksprintable — key stays hidden on paper

Time: 60 minutes Total Marks: 50
Instructions: Attempt all questions. No hints given. Show all working. Take c=3×108 m/sc = 3\times10^8\ \text{m/s} unless stated.


Q1. (10 marks) A concave mirror of focal length f=20 cmf = 20\ \text{cm} forms an image on a screen. When the object is moved 10 cm10\ \text{cm} away from the mirror (i.e. further out), the screen must be moved 15 cm15\ \text{cm} closer to the mirror to refocus.

(a) Set up the mirror equation for both configurations and hence determine the original object distance. (7) (b) Compute the magnification in the original configuration and state whether the image is erect or inverted. (3)


Q2. (12 marks) A ray of monochromatic light travels inside a rectangular glass slab (ng=1.50n_g = 1.50) surrounded by air. A thin uniform film of liquid (nLn_L) coats the top surface.

(a) Derive the condition on nLn_L such that a ray inside the glass hitting the glass–liquid interface at 4242^\circ undergoes total internal reflection there, while a ray at 3838^\circ does not. Give the numerical range of nLn_L. (7) (b) Independently, the same liquid forms a soap-like film of thickness tt in air. Determine the two smallest thicknesses tt giving a bright reflection for normally incident light of wavelength 600 nm600\ \text{nm} (in vacuum), taking nL=1.33n_L = 1.33. (5)


Q3. (10 marks) In a Young's double-slit setup (d=0.25 mmd = 0.25\ \text{mm}, D=1.5 mD = 1.5\ \text{m}, λ=500 nm\lambda = 500\ \text{nm}), a transparent sheet of refractive index 1.601.60 and thickness tt is placed over the upper slit. The central bright fringe shifts to where the 8th bright fringe (without the sheet) used to be.

(a) Find tt. (5) (b) The whole apparatus is now immersed in water (nw=1.33n_w = 1.33). Without the sheet, compute the new fringe width and explain physically why it changes. (5)


Q4. (10 marks) A telescope objective has diameter D=10 cmD = 10\ \text{cm} and focal length 120 cm120\ \text{cm}; the eyepiece focal length is 2.0 cm2.0\ \text{cm}. It is used with light of mean wavelength 550 nm550\ \text{nm}.

(a) Compute the angular magnification (normal adjustment) and the length of the telescope tube. (3) (b) Two distant stars are just resolved by this objective (Rayleigh criterion). Find their minimum angular separation, and the smallest linear separation they could have if they are 4 ly4\ \text{ly} away. Take 1 ly=9.46×1015 m1\ \text{ly} = 9.46\times10^{15}\ \text{m}. (7)


Q5. (8 marks) Unpolarised light of intensity I0I_0 passes through three ideal polaroids. The first and third have their transmission axes crossed (perpendicular). The middle polaroid's axis makes angle θ\theta with the first.

(a) Derive an expression for the transmitted intensity through all three as a function of θ\theta. (4) (b) Find the value of θ\theta that maximises the output, and the corresponding intensity as a fraction of I0I_0. (4)


Answer keyMark scheme & solutions

Q1 (10 marks)

Use 1v+1u=1f\frac{1}{v}+\frac{1}{u}=\frac{1}{f} with real-is-positive magnitudes (image on screen ⇒ real).

(a) Original: object uu, image vv, 1v+1u=120\frac1v+\frac1u=\frac1{20}. (1) Object moved further out: u=u+10u'=u+10, image moves closer: v=v15v'=v-15. (1) So 1v15+1u+10=120\frac{1}{v-15}+\frac{1}{u+10}=\frac1{20}. (1)

From config 1: 1v=1201u=u2020uv=20uu20\frac1v=\frac1{20}-\frac1u=\frac{u-20}{20u}\Rightarrow v=\frac{20u}{u-20}. (2)

Substitute into config 2 and solve. Try u=60u=60: v=120040=30v=\frac{1200}{40}=30. Check config 2: u=70, v=15u'=70,\ v'=15: 115+170=0.0667+0.0143=0.08100.05\frac1{15}+\frac1{70}=0.0667+0.0143=0.0810\neq0.05. Reject.

Solve properly: with v=20uu20v=\frac{20u}{u-20}, 120uu2015+1u+10=120\frac{1}{\frac{20u}{u-20}-15}+\frac{1}{u+10}=\frac{1}{20}. 20uu2015=20u15(u20)u20=5u+300u20\frac{20u}{u-20}-15=\frac{20u-15(u-20)}{u-20}=\frac{5u+300}{u-20}. So term =u205u+300=\frac{u-20}{5u+300}. Equation: u205u+300+1u+10=120\frac{u-20}{5u+300}+\frac1{u+10}=\frac1{20}. (2)

Multiply out. Let me solve: u205(u+60)+1u+10=120\frac{u-20}{5(u+60)}+\frac{1}{u+10}=\frac1{20}. Multiply by 2020: 4(u20)u+60+20u+10=1\frac{4(u-20)}{u+60}+\frac{20}{u+10}=1. 4(u20)(u+10)+20(u+60)=(u+60)(u+10)4(u-20)(u+10)+20(u+60)=(u+60)(u+10). 4(u210u200)+20u+1200=u2+70u+6004(u^2-10u-200)+20u+1200=u^2+70u+600. 4u240u800+20u+1200=u2+70u+6004u^2-40u-800+20u+1200=u^2+70u+600. 4u220u+400=u2+70u+6004u^2-20u+400=u^2+70u+600. 3u290u200=03u^2-90u-200=0. u=90±8100+24006=90±105006=90±102.476u=\frac{90\pm\sqrt{8100+2400}}{6}=\frac{90\pm\sqrt{10500}}{6}=\frac{90\pm102.47}{6}. u=32.08 cmu=32.08\ \text{cm} (positive root). (1)

(b) v=20×32.0812.08=53.1 cmv=\frac{20\times32.08}{12.08}=53.1\ \text{cm}. Magnification m=vu=53.132.08=1.66m=-\frac{v}{u}=-\frac{53.1}{32.08}=-1.66; magnitude 1.661.66, inverted (real image). (3)

Q2 (12 marks)

(a) Critical angle at glass–liquid interface: sinθc=nLng\sin\theta_c=\frac{n_L}{n_g} (light going from denser glass to liquid, needs nL<ngn_L<n_g). (2) TIR at 4242^\circ42θcsin42nLng42^\circ\ge\theta_c\Rightarrow \sin42^\circ\ge\frac{n_L}{n_g}. (1) No TIR at 3838^\circ38<θcsin38<nLng38^\circ<\theta_c\Rightarrow \sin38^\circ<\frac{n_L}{n_g}. (1) So ngsin38<nLngsin42n_g\sin38^\circ<n_L\le n_g\sin42^\circ. (1) 1.5×0.6157=0.92351.5\times0.6157=0.9235; 1.5×0.6691=1.00371.5\times0.6691=1.0037. (1) Since nLngn_L\le n_g physically required, range: 0.924<nL<1.00\boxed{0.924<n_L<1.00} (upper bound also ng\le n_g; effective 0.924<nL1.000.924<n_L\lesssim1.00). (1)

(b) Soap film in air: reflection has one π\pi phase change (air→film) ⇒ bright condition 2nLt=(m+12)λ2n_Lt=(m+\tfrac12)\lambda. (2) t=(m+12)λ2nLt=\frac{(m+\frac12)\lambda}{2n_L}. m=0m=0: t=0.5×6002×1.33=3002.66=112.8 nmt=\frac{0.5\times600}{2\times1.33}=\frac{300}{2.66}=112.8\ \text{nm}. (2) m=1m=1: t=1.5×6002.66=338.3 nmt=\frac{1.5\times600}{2.66}=338.3\ \text{nm}. (1)

Q3 (10 marks)

(a) Shift of central fringe by inserting sheet: path added =(n1)t=(n-1)t. This equals shift to 8th fringe position ⇒ (n1)t=8λ(n-1)t=8\lambda. (2) t=8λn1=8×500×1090.60=6.67×106 m=6.67 μmt=\frac{8\lambda}{n-1}=\frac{8\times500\times10^{-9}}{0.60}=6.67\times10^{-6}\ \text{m}=6.67\ \mu\text{m}. (3)

(b) In water, wavelength λ=λ/nw\lambda'=\lambda/n_w. Fringe width β=λDd=λDnwd\beta=\frac{\lambda' D}{d}=\frac{\lambda D}{n_w d}. (2) βair=500×109×1.50.25×103=3.0×103 m=3.0 mm\beta_{air}=\frac{500\times10^{-9}\times1.5}{0.25\times10^{-3}}=3.0\times10^{-3}\ \text{m}=3.0\ \text{mm}. βwater=3.0/1.33=2.26 mm\beta_{water}=3.0/1.33=2.26\ \text{mm}. (2) Physically: wavelength in water is shorter, so fringes are more closely spaced (smaller β\beta). (1)

Q4 (10 marks)

(a) Angular magnification M=fo/fe=120/2.0=60M=f_o/f_e=120/2.0=60. (1.5) Tube length (normal adjustment) L=fo+fe=122 cmL=f_o+f_e=122\ \text{cm}. (1.5)

(b) Rayleigh: θmin=1.22λ/D=1.22×550×1090.10=6.71×106 rad\theta_{min}=1.22\lambda/D=\frac{1.22\times550\times10^{-9}}{0.10}=6.71\times10^{-6}\ \text{rad}. (3) Distance r=4×9.46×1015=3.784×1016 mr=4\times9.46\times10^{15}=3.784\times10^{16}\ \text{m}. (1) Linear separation s=rθmin=3.784×1016×6.71×106=2.54×1011 ms=r\theta_{min}=3.784\times10^{16}\times6.71\times10^{-6}=2.54\times10^{11}\ \text{m}. (3) (≈ 1.71.7 AU.)

Q5 (8 marks)

(a) After polaroid 1: I1=I0/2I_1=I_0/2. (1) After 2 (angle θ\theta from 1): I2=I02cos2θI_2=\frac{I_0}{2}\cos^2\theta. (1) Polaroid 3 at 9090^\circ from 1 ⇒ angle between 2 and 3 is (90θ)(90^\circ-\theta): I3=I2cos2(90θ)=I02cos2θsin2θI_3=I_2\cos^2(90^\circ-\theta)=\frac{I_0}{2}\cos^2\theta\sin^2\theta. (2)

(b) I3=I02cos2θsin2θ=I08sin22θI_3=\frac{I_0}{2}\cos^2\theta\sin^2\theta=\frac{I_0}{8}\sin^2 2\theta. Max when sin2θ=1θ=45\sin2\theta=1\Rightarrow \theta=45^\circ. (2) Imax=I0/8I_{max}=I_0/8. (2)

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{"claim":"Q1 quadratic gives u=32.08cm","code":"u=symbols('u',positive=True); sol=solve(3*u**2-90*u-200,u); val=[s for s in sol if s>0][0]; result=abs(float(val)-32.08)<0.1"},
{"claim":"Q2b m=0 thickness 112.8nm","code":"t=(0.5*600)/(2*1.33); result=abs(t-112.78)<0.5"},
{"claim":"Q3a t=6.67 microns","code":"t=8*500e-9/0.60; result=abs(t-6.667e-6)<1e-8"},
{"claim":"Q4b linear separation approx 2.54e11 m","code":"th=1.22*550e-9/0.10; r=4*9.46e15; s=r*th; result=abs(s-2.54e11)/2.54e11<0.02"},
{"claim":"Q5 max intensity I0/8","code":"th=pi/4; frac=Rational(1,2)*cos(th)**2*sin(th)**2; result=simplify(frac-Rational(1,8))==0"}
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