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CalibratePhysics

Chapter 9

Ray Optics and Optical Instruments

CBSE · 6 subtopics

Formula SheetEvery formula this chapter can be examined on, in one table.

Cartesian sign convention — apply it before every substitution

  • Every distance is measured from the pole PP of the mirror, or from the optical centre OO of the lens, along the principal axis.
  • Distances measured in the same direction as the incident light are positive; distances measured opposite to the direction of incident light are negative.
  • Heights measured upwards from the principal axis are positive; heights measured downwards are negative.
  • Incident light is always drawn travelling left to right, so a real object in front of the mirror or lens always has uu negative.
  • With one convention adopted, a single mirror formula and a single lens formula cover every case — concave or convex, real or virtual image.
  • QuantitySignCase
  • uunegativereal object (in front)
  • uupositivevirtual object (converging beam intercepted)
  • vv (mirror)negativereal image, in front of the mirror
  • vv (mirror)positivevirtual image, behind the mirror
  • vv (lens)positivereal image, on the far side
  • vv (lens)negativevirtual image, on the object's side
  • f, Rf,\ R (mirror)negativeconcave mirror
  • f, Rf,\ R (mirror)positiveconvex mirror
  • ff (lens)positiveconvex (converging) lens
  • ff (lens)negativeconcave (diverging) lens
  • hhpositiveerect object or image
  • h′h'negativeinverted image

Constants and standard data CBSE expects

FormulaSymbols, units and conditions
c=3×108 m s−1D=25 cm1 D=1 m−1c = 3\times10^{8}\ \text{m s}^{-1} \qquad D = 25\ \text{cm} \qquad 1\ \text{D} = 1\ \text{m}^{-1}
  • cc = speed of light in vacuum (exact value 2.99792458×1082.99792458\times10^{8} m s−1^{-1}; use 3×1083\times10^{8}). DD = least distance of distinct vision for a normal eye. 11 dioptre is the power of a lens of focal length 11 m.
  • Visible light: wavelength about 400400 nm to 750750 nm.
  • Standard refractive indices (with respect to air): water 1.331.33 (or 4/34/3), crown glass 1.521.52 (often taken as 1.51.5 or 3/23/2), dense flint glass 1.621.62, diamond 2.422.42.
  • Corresponding critical angles with air: water 48.75∘48.75^\circ, crown glass 41.14∘41.14^\circ, dense flint glass 37.31∘37.31^\circ, diamond 24.41∘24.41^\circ.

Reflection of light by spherical mirrors

FormulaSymbols, units and conditions
∠i=∠r\angle i = \angle r
  • Law of reflection: angle of incidence equals angle of reflection, and the incident ray, the reflected ray and the normal at the point of incidence lie in one plane. For a spherical mirror the normal is along the radius, i.e. along the line joining the centre of curvature to the point of incidence.
f=R2f = \dfrac{R}{2}
  • ff = focal length (m or cm), RR = radius of curvature. Valid for paraxial rays on a mirror of small aperture. Concave: both negative. Convex: both positive.
1v+1u=1f\dfrac{1}{v} + \dfrac{1}{u} = \dfrac{1}{f}
  • Mirror equation. uu = object distance, vv = image distance, ff = focal length, all with signs. Valid for concave and convex mirrors, real and virtual images.
m=h′h=−vum = \dfrac{h'}{h} = -\dfrac{v}{u}
  • Linear (transverse) magnification. hh = object height, h′h' = image height. mm negative ⇒\Rightarrow real and inverted; mm positive ⇒\Rightarrow virtual and erect. ∣m∣>1\lvert m\rvert > 1 magnified, ∣m∣<1\lvert m\rvert < 1 diminished.
m=ff−u=f−vfm = \dfrac{f}{f-u} = \dfrac{f-v}{f}
  • Useful alternative forms of the magnification for a mirror, obtained by eliminating vv or uu from the mirror equation.
v=fuu−fv = \dfrac{fu}{u-f}
  • Mirror equation rearranged; used for "how fast does the image move" questions (rear-view mirror numericals).

Refraction of light

FormulaSymbols, units and conditions
n21=sin⁡isin⁡r=n2n1=v1v2=λ1λ2n_{21} = \dfrac{\sin i}{\sin r} = \dfrac{n_2}{n_1} = \dfrac{v_1}{v_2} = \dfrac{\lambda_1}{\lambda_2}
  • Snell's law. ii = angle of incidence, rr = angle of refraction, both measured from the normal; n21n_{21} = refractive index of medium 2 with respect to medium 1. It is a property of the pair of media and of the wavelength, but is independent of the angle of incidence.
n1sin⁡i=n2sin⁡rn_1\sin i = n_2\sin r
  • Snell's law in the symmetric form; the one to use whenever neither medium is air.
n=cvλmedium=λvacuumnν unchangedn = \dfrac{c}{v} \qquad \lambda_{medium} = \dfrac{\lambda_{vacuum}}{n} \qquad \nu\ \text{unchanged}
  • nn = absolute refractive index of a medium, vv = speed of light in it. On refraction the frequency ν\nu does not change; the speed and the wavelength both fall by the factor nn.
n12=1n21n32=n31×n12n_{12} = \dfrac{1}{n_{21}} \qquad n_{32} = n_{31}\times n_{12}
  • Reciprocal and chain relations between relative refractive indices.
n=real depthapparent depth=h2h1n = \dfrac{\text{real depth}}{\text{apparent depth}} = \dfrac{h_2}{h_1}
  • For near-normal viewing of an object under a denser medium. The bottom of a water tank appears raised.
normal shift=t(1−1n)\text{normal shift} = t\left(1 - \dfrac{1}{n}\right)
  • tt = thickness of a glass slab, nn = its refractive index. The apparent rise of an object viewed normally through the slab; independent of where the slab is placed between object and eye.
d=tsin⁡(i−r)cos⁡rd = \dfrac{t\sin(i-r)}{\cos r}
  • Lateral shift of a ray passing through a parallel-sided slab of thickness tt. The emergent ray is parallel to the incident ray, so there is no net deviation — only this sideways displacement.

Total internal reflection

FormulaSymbols, units and conditions
sin⁡ic=n21=nrarerndenserndenser=1sin⁡ic\sin i_c = n_{21} = \dfrac{n_{rarer}}{n_{denser}} \qquad n_{denser} = \dfrac{1}{\sin i_c}
  • ici_c = critical angle: the angle of incidence in the denser medium for which the angle of refraction is 90∘90^\circ. For i>ici > i_c no refraction is possible and the light is totally internally reflected.
sin⁡ic=1n(denser medium of index n against air)\sin i_c = \dfrac{1}{n} \quad \text{(denser medium of index } n \text{ against air)}
  • The usual working form. Larger nn gives a smaller critical angle: diamond 24.4∘24.4^\circ, glass about 41∘41^\circ, water about 48.8∘48.8^\circ.
r=dn2−1A=πr2=πd2n2−1r = \dfrac{d}{\sqrt{n^2-1}} \qquad A = \pi r^2 = \dfrac{\pi d^2}{n^2-1}
  • Light from a point source at depth dd below the surface of a liquid of index nn escapes only through a circle of radius rr on the surface; AA is the area of that circle. From r=dtan⁡icr = d\tan i_c.

Refraction at a spherical surface

FormulaSymbols, units and conditions
n2v−n1u=n2−n1R\dfrac{n_2}{v} - \dfrac{n_1}{u} = \dfrac{n_2 - n_1}{R}
  • Light travelling from medium n1n_1 into medium n2n_2 across a spherical surface of radius RR; uu and vv measured from the pole of the surface with the Cartesian convention. Valid for convex and concave surfaces, real and virtual images. Note it is n2n_2 (the medium the light enters) that goes with vv.

Thin lenses

FormulaSymbols, units and conditions
1f=(n21−1)(1R1−1R2),n21=n2n1\dfrac{1}{f} = (n_{21} - 1)\left(\dfrac{1}{R_1} - \dfrac{1}{R_2}\right), \qquad n_{21} = \dfrac{n_2}{n_1}
  • Lens maker's formula. n2n_2 = refractive index of the lens material, n1n_1 = that of the surrounding medium, R1R_1 = radius of the first surface met by the light, R2R_2 = that of the second. Signs by the Cartesian convention: biconvex R1=+RR_1 = +R, R2=−RR_2 = -R; biconcave R1=−RR_1 = -R, R2=+RR_2 = +R; a plane face has R=∞R = \infty, so 1/R=01/R = 0.
1v−1u=1f\dfrac{1}{v} - \dfrac{1}{u} = \dfrac{1}{f}
  • Thin lens formula. Valid for convex and concave lenses, real and virtual images. Note the minus sign — it is the commonest place to lose a mark, since the mirror formula carries a plus.
m=h′h=vum = \dfrac{h'}{h} = \dfrac{v}{u}
  • Magnification of a lens (no minus sign, unlike the mirror). mm positive ⇒\Rightarrow erect and virtual; mm negative ⇒\Rightarrow inverted and real.
P=1f (in metres)=100f (in cm)P = \dfrac{1}{f\ (\text{in metres})} = \dfrac{100}{f\ (\text{in cm})}
  • Power of a lens, in dioptre (D). Positive for a converging lens, negative for a diverging lens. P=+2.5P = +2.5 D means a convex lens of f=+40f = +40 cm; P=−4.0P = -4.0 D means a concave lens of f=−25f = -25 cm.
1f=1f1+1f2+1f3+…P=P1+P2+P3+…m=m1m2m3…\dfrac{1}{f} = \dfrac{1}{f_1} + \dfrac{1}{f_2} + \dfrac{1}{f_3} + \dots \qquad P = P_1 + P_2 + P_3 + \dots \qquad m = m_1m_2m_3\dots
  • Thin lenses in contact. Powers add algebraically (convex positive, concave negative); magnifications multiply.
1fmedium=(nlensnmedium−1)(1R1−1R2)\dfrac{1}{f_{medium}} = \left(\dfrac{n_{lens}}{n_{medium}} - 1\right)\left(\dfrac{1}{R_1} - \dfrac{1}{R_2}\right)
  • A lens immersed in a liquid. If nlens>nmediumn_{lens} > n_{medium} the lens keeps its character but is weaker; if nlens<nmediumn_{lens} < n_{medium} the sign of ff reverses and a convex lens diverges; if nlens=nmediumn_{lens} = n_{medium} then 1/f=01/f = 0 and the lens disappears.
f=D2−d24Df = \dfrac{D^2 - d^2}{4D}
  • Displacement (conjugate-foci) method: DD = fixed distance between object and screen, dd = separation of the two lens positions that give a sharp image.
μliquid=1+(x−y)Rxy\mu_{liquid} = 1 + \dfrac{(x-y)R}{xy}
  • Liquid-lens experiment: an equiconvex lens of radius RR on a plane mirror, a needle coinciding with its own image at distance xx with a liquid film present and at yy with the film removed.

Refraction through a prism

FormulaSymbols, units and conditions
r1+r2=Aδ=i+e−Ai+e=A+δr_1 + r_2 = A \qquad \delta = i + e - A \qquad i + e = A + \delta
  • AA = angle of the prism (refracting angle), r1,r2r_1,r_2 = angles of refraction at the two faces, ii = angle of incidence, ee = angle of emergence, δ\delta = angle of deviation.
δ=δm ⇒ i=e,r1=r2=A2,δm=2i−A,i=A+δm2\delta = \delta_m \ \Rightarrow\ i = e,\quad r_1 = r_2 = \dfrac{A}{2},\quad \delta_m = 2i - A,\quad i = \dfrac{A+\delta_m}{2}
  • Conditions at minimum deviation: the refracted ray inside the prism is parallel to the base.
n21=sin⁡(A+δm2)sin⁡(A2)n_{21} = \dfrac{\sin\left(\dfrac{A+\delta_m}{2}\right)}{\sin\left(\dfrac{A}{2}\right)}
  • Prism formula. Gives the refractive index of the prism material from two measurable angles. If the prism is in a medium, this returns the relative index nprism/nmediumn_{prism}/n_{medium}.
δm=(n−1)A\delta_m = (n - 1)A
  • Thin (small-angle) prism only. Shows that thin prisms deviate light very little, and that δm\delta_m grows with nn.
n=sin⁡Asin⁡(A/2)when δm=An = \dfrac{\sin A}{\sin(A/2)} \quad \text{when } \delta_m = A
  • The special case CBSE likes: for an equilateral prism with δm=A=60∘\delta_m = A = 60^\circ, n=sin⁡60∘/sin⁡30∘=3n = \sin 60^\circ/\sin 30^\circ = \sqrt3.
nviolet>nred ⇒ δviolet>δredn_{violet} > n_{red} \ \Rightarrow\ \delta_{violet} > \delta_{red}
  • Dispersion: refractive index falls as wavelength rises, so red is deviated least and violet most, and δm\delta_m is smallest for red.

Simple microscope (magnifying glass)

FormulaSymbols, units and conditions
m=1+Df(image at the near point, D=25 cm)m = 1 + \dfrac{D}{f} \qquad \text{(image at the near point, } D = 25 \text{ cm)}—
m=Df(image at infinity, relaxed eye)m = \dfrac{D}{f} \qquad \text{(image at infinity, relaxed eye)}
  • ff = focal length of the converging lens. The near-point value is one greater, but the infinity setting is more comfortable. A lens with f>Df > D gives m<1m < 1 and is useless as a magnifier.

Compound microscope

FormulaSymbols, units and conditions
mo=vouo≈Lfome=1+Dfe or Dfem_o = \dfrac{v_o}{u_o} \approx \dfrac{L}{f_o} \qquad m_e = 1 + \dfrac{D}{f_e} \ \text{or}\ \dfrac{D}{f_e}
  • fo,fef_o,f_e = focal lengths of objective and eyepiece; LL = tube length, the distance between the second focal point of the objective and the first focal point of the eyepiece (in numericals, effectively the separation between the lenses).
m=mo×me=vouo(1+Dfe)≈Lfo(1+Dfe)m = m_o\times m_e = \dfrac{v_o}{u_o}\left(1 + \dfrac{D}{f_e}\right) \approx \dfrac{L}{f_o}\left(1 + \dfrac{D}{f_e}\right)
  • Final image at the near point.
m=Lfo×Dfem = \dfrac{L}{f_o}\times\dfrac{D}{f_e}
  • Final image at infinity (normal adjustment). Both fof_o and fef_e must be short for large mm.
separation=vo+∣ue∣(near point)separation=vo+fe(infinity)\text{separation} = v_o + \lvert u_e\rvert \quad\text{(near point)} \qquad \text{separation} = v_o + f_e \quad\text{(infinity)}
  • How to get the tube length in a numerical once vov_o and ueu_e have been found from the lens formula applied to each lens in turn.

Astronomical (refracting) telescope

FormulaSymbols, units and conditions
m=βα=fofeL=fo+fem = \dfrac{\beta}{\alpha} = \dfrac{f_o}{f_e} \qquad L = f_o + f_e
  • Normal adjustment (final image at infinity). β\beta = angle subtended at the eye by the final image, α\alpha = angle subtended at the objective by the distant object. LL = length of the telescope tube.
m=fofe(1+feD)m = \dfrac{f_o}{f_e}\left(1 + \dfrac{f_e}{D}\right)
  • Final image at the least distance of distinct vision.
h=fo θ=fo×size of objectdistance of objecth = f_o\,\theta = f_o\times\dfrac{\text{size of object}}{\text{distance of object}}
  • Height (or diameter) of the intermediate image formed by the objective of a distant object subtending angle θ\theta. Used for the Moon and tall-tower numericals: for the Moon, take θ\theta = (diameter of Moon)/(Earth–Moon distance) and the answer is the image diameter.
Short NotesThe chapter subtopic by subtopic, in the textbook's own order.6 subtopics
  1. 1Reflection of Light by Spherical Mirrors10 board questions
  2. 2Refraction1 board question
  3. 3Total Internal Reflection3 board questions
  4. 4Refraction at Spherical Surfaces and by Lenses36 board questions
  5. 5Refraction through a Prism19 board questions
  6. 6Optical Instruments30 board questions
The whole chapter in brief

9.1 Introduction — the ray picture

  • Light is the part of the electromagnetic spectrum the eye detects, wavelength about 400400 nm to 750750 nm.
  • Speed of light in vacuum c=2.99792458×108c = 2.99792458\times10^8 m s−1^{-1}, taken as 3×1083\times10^8 m s−1^{-1}; it is the highest speed attainable in nature.
  • Because the wavelength of light is tiny compared with ordinary objects, light travels in straight lines: the path is a ray, a bundle of rays is a beam. This chapter uses only that ray picture.
  • Reflection, refraction and dispersion are all treated with two laws: the law of reflection and Snell's law of refraction.

Cartesian sign convention

  • Distances are measured from the pole of the mirror or the optical centre of the lens.
  • Along the direction of the incident light: positive. Against it: negative.
  • Heights above the principal axis: positive. Below it: negative.
  • Consequences to memorise: concave mirror ff negative, convex mirror ff positive; convex lens ff positive, concave lens ff negative; a real object always has uu negative.

Reflection at spherical mirrors

  • Laws of reflection: ∠i=∠r\angle i = \angle r, and the incident ray, reflected ray and normal lie in one plane. The normal at any point of a spherical mirror lies along the radius through that point.
  • Pole PP: geometric centre of the mirror. Centre of curvature CC, radius of curvature RR, principal axis PCPC, principal focus FF, focal plane: the plane through FF perpendicular to the axis, where an oblique parallel beam converges.
  • Paraxial rays: rays close to the axis making small angles with it. All mirror and lens formulae in this chapter assume them.
  • f=R/2f = R/2, mirror equation 1v+1u=1f\dfrac1v + \dfrac1u = \dfrac1f, magnification m=h′h=−vum = \dfrac{h'}{h} = -\dfrac{v}{u}.
  • Rays used for the diagram: (i) parallel to the axis, reflects through FF; (ii) through CC, retraces its path; (iii) through FF, reflects parallel to the axis; (iv) striking the pole, reflects at an equal angle to the axis.
Object position (concave mirror)Image positionNatureSize
At infinityAt FFReal, invertedPoint-sized
Beyond CCBetween FF and CCReal, invertedDiminished
At CCAt CCReal, invertedSame size
Between CC and FFBeyond CCReal, invertedMagnified
At FFAt infinityReal, invertedHighly magnified
Between FF and PPBehind the mirrorVirtual, erectMagnified
  • A convex mirror always gives a virtual, erect, diminished image between PP and FF, for every position of a real object. Proof: f>0f > 0 and u<0u < 0, so 1v=1f−1u\dfrac1v = \dfrac1f - \dfrac1u is a sum of two positive terms, hence v>0v > 0 always.
  • Convex mirrors are used as rear-view mirrors: always erect, and a wide field of view.
  • Covering half a mirror does not halve the image: the whole image still forms, only its intensity falls, because every remaining point still obeys the laws of reflection.

Refraction

  • Laws: (i) the incident ray, refracted ray and normal lie in one plane; (ii) sin⁡isin⁡r=n21\dfrac{\sin i}{\sin r} = n_{21}, a constant for the pair of media, independent of the angle of incidence.
  • n21=n2n1=v1v2=λ1λ2n_{21} = \dfrac{n_2}{n_1} = \dfrac{v_1}{v_2} = \dfrac{\lambda_1}{\lambda_2}; absolute index n=cvn = \dfrac{c}{v}.
  • On refraction the frequency stays the same; the speed and wavelength change.
  • n21>1n_{21} > 1: medium 2 is optically denser, the ray bends towards the normal. n21<1n_{21} < 1: the ray bends away from the normal.
  • Optical density is not mass density: turpentine is optically denser than water but less massive per unit volume.
  • n12=1/n21n_{12} = 1/n_{21} and n32=n31×n12n_{32} = n_{31}\times n_{12}.
  • Parallel-sided slab: r2=i1r_2 = i_1, so the emergent ray is parallel to the incident ray — no deviation, only a lateral shift d=tsin⁡(i−r)cos⁡rd = \dfrac{t\sin(i-r)}{\cos r}.
  • Apparent depth: n=real depthapparent depthn = \dfrac{\text{real depth}}{\text{apparent depth}}; normal shift through a slab =t(1−1n)= t\left(1 - \dfrac1n\right), independent of the slab's position.

Total internal reflection

  • Occurs when light in a denser medium meets the boundary with a rarer medium at an angle of incidence greater than the critical angle. Both conditions must be stated.
  • Critical angle: the angle of incidence in the denser medium for which the angle of refraction is 90∘90^\circ; sin⁡ic=nrarerndenser\sin i_c = \dfrac{n_{rarer}}{n_{denser}}, and against air n=1sin⁡icn = \dfrac{1}{\sin i_c}.
  • In total internal reflection no light is transmitted at all — unlike ordinary reflection, which is always partial.
MediumnnCritical angle with air
Water1.3348.75∘48.75^\circ
Crown glass1.5241.14∘41.14^\circ
Dense flint glass1.6237.31∘37.31^\circ
Diamond2.4224.41∘24.41^\circ
  • Applications: mirage; the sparkle of diamond (very small ici_c, so light is trapped by repeated internal reflections); totally reflecting prisms that turn light through 90∘90^\circ or 180∘180^\circ, or invert an image without changing its size (they need ic<45∘i_c < 45^\circ, true for crown and flint glass); optical fibres.
  • Optical fibre: a core of high refractive index sheathed in a cladding of lower index. Light launched at a suitable angle strikes the core–cladding boundary above the critical angle and is totally internally reflected repeatedly along the fibre, even round bends, with almost no loss — over 95% transmitted through 1 km of silica fibre. Used for communication signals and as a light pipe in endoscopy and decorative lamps.

Refraction at a spherical surface

n2v−n1u=n2−n1R\dfrac{n_2}{v} - \dfrac{n_1}{u} = \dfrac{n_2-n_1}{R}

  • Light passes from n1n_1 into n2n_2 at a surface of radius RR; distances measured from the pole. The index of the medium the light enters goes with vv.

Lenses

  • Lens maker's formula: 1f=(n21−1)(1R1−1R2)\dfrac1f = (n_{21}-1)\left(\dfrac1{R_1} - \dfrac1{R_2}\right), obtained by applying the spherical-surface relation at each face of a thin lens and adding.
  • Thin lens formula 1v−1u=1f\dfrac1v - \dfrac1u = \dfrac1f; magnification m=h′h=vum = \dfrac{h'}{h} = \dfrac vu.
  • Rays used for the diagram: (i) parallel to the axis, refracts through the second focus F′F' (or appears to come from FF for a concave lens); (ii) through the optical centre, passes undeviated; (iii) through the first focus, emerges parallel to the axis.
  • The two foci are equidistant from the optical centre. The focus on the side of the source is the first focal point.
Object position (convex lens)Image positionNatureSize
At infinityAt F′F'Real, invertedPoint-sized
Beyond 2F2FBetween F′F' and 2F′2F'Real, invertedDiminished
At 2F2FAt 2F′2F'Real, invertedSame size
Between FF and 2F2FBeyond 2F′2F'Real, invertedMagnified
At FFAt infinityReal, invertedHighly magnified
Between FF and the lensSame side as objectVirtual, erectMagnified
  • A concave lens always gives a virtual, erect, diminished image between the optical centre and FF.
  • Power P=1/fP = 1/f in dioptre; positive for converging, negative for diverging lenses.
  • Lenses in contact: 1f=1f1+1f2+…\dfrac1f = \dfrac1{f_1} + \dfrac1{f_2}+\dots, P=P1+P2+…P = P_1+P_2+\dots, m=m1m2…m = m_1m_2\dots
  • A lens in a liquid: 1f=(nlensnmedium−1)(1R1−1R2)\dfrac1f = \left(\dfrac{n_{lens}}{n_{medium}}-1\right)\left(\dfrac1{R_1}-\dfrac1{R_2}\right). Denser surroundings weaken it; surroundings denser than the lens reverse its character; equal indices make it vanish.
  • Wavelength dependence: as λ\lambda increases, nn falls, so ff increases and PP falls. Violet is focused nearest the lens, red farthest.

Prisms

  • r1+r2=Ar_1 + r_2 = A and δ=i+e−A\delta = i + e - A.
  • The δ\delta–ii graph falls to a single minimum and rises again; every δ\delta except δm\delta_m corresponds to two angles of incidence, because ii and ee are interchangeable.
  • At minimum deviation the ray passes symmetrically: i=ei = e, r1=r2=A/2r_1 = r_2 = A/2, the refracted ray is parallel to the base, and δm=2i−A\delta_m = 2i - A.
  • Prism formula n=sin⁡(A+δm2)sin⁡(A2)n = \dfrac{\sin\left(\dfrac{A+\delta_m}{2}\right)}{\sin\left(\dfrac{A}{2}\right)}; for a thin prism δm=(n−1)A\delta_m = (n-1)A.
  • Since nviolet>nredn_{violet} > n_{red}, δm\delta_m is largest for violet and smallest for red — this is dispersion.
  • Immersing a prism in water lowers the relative refractive index, so δm\delta_m decreases.

Optical instruments

  • Simple microscope: a converging lens of short focal length held near the object. m=1+Dfm = 1 + \dfrac Df with the image at the near point, m=Dfm = \dfrac Df with the image at infinity.
  • Compound microscope: objective of very short focal length and small aperture forms a real, inverted, magnified image inside the tube; the eyepiece, acting as a magnifier, makes the final image virtual, inverted with respect to the object, and further magnified. m=Lfo(1+Dfe)m = \dfrac{L}{f_o}\left(1+\dfrac{D}{f_e}\right) at the near point, Lfo×Dfe\dfrac{L}{f_o}\times\dfrac{D}{f_e} at infinity.
  • Astronomical telescope: objective of large focal length and large aperture, eyepiece of short focal length. m=fofem = \dfrac{f_o}{f_e}, tube length fo+fef_o + f_e in normal adjustment; m=fofe(1+feD)m = \dfrac{f_o}{f_e}\left(1+\dfrac{f_e}{D}\right) at the near point. The final image is inverted and virtual.
  • Reflecting (Cassegrain) telescope: a large concave paraboloidal primary mirror converges light onto a small convex secondary, which sends it back through a hole in the primary to the eyepiece. Advantages: no chromatic aberration; a paraboloidal mirror also removes spherical aberration; a mirror can be supported over its whole back so much larger apertures are possible, giving a brighter image and higher resolving power; mirrors are lighter and cheaper to make free of defects.
FeatureCompound microscopeAstronomical telescope
PurposeTiny nearby objectsLarge distant objects
Objective fof_oVery smallVery large
Relation of focal lengthsfo<fef_o < f_efo≫fef_o \gg f_e
Objective apertureSmallLarge
MagnificationLfo×Dfe\dfrac{L}{f_o}\times\dfrac{D}{f_e}fofe\dfrac{f_o}{f_e}
Tube length (normal adjustment)vo+fev_o + f_efo+fef_o + f_e
  • Why a large objective aperture in a telescope: more light gathered (brighter image of faint stars) and higher resolving power.
  • Why short focal lengths in a microscope: mm is inversely proportional to both fof_o and fef_e.
  • Why the image at infinity is preferred: the eye is fully relaxed, so viewing causes least strain.
  • Modern microscopes use multi-component lenses for objective and eyepiece to minimise chromatic and spherical aberration.

Traps that cost marks

  • The mirror formula has a plus, the lens formula a minus: 1v+1u=1f\dfrac1v+\dfrac1u=\dfrac1f but 1v−1u=1f\dfrac1v-\dfrac1u=\dfrac1f. Mixing them is the single commonest error in this chapter.
  • Mirror magnification carries a minus sign, m=−v/um = -v/u; lens magnification does not, m=v/um = v/u.
  • Substitute signed values, not magnitudes: a concave mirror has f=−R/2f = -R/2, a real object has uu negative. Never write u=20u = 20 cm.
  • In n2v−n1u=n2−n1R\dfrac{n_2}{v}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R}, n2n_2 is the medium the light goes into. If light travels back the other way at the second surface of a lens, the indices swap.
  • R1R_1 is the radius of the surface the light meets first, not the left-hand one by habit. For a biconvex lens R1=+RR_1 = +R, R2=−RR_2 = -R, giving 1f=2(n−1)R\dfrac1f = \dfrac{2(n-1)}{R}.
  • A plane face has R=∞R = \infty, so its term is zero — not one.
  • Cutting a lens along the principal axis (vertically, halving the aperture) leaves ff and PP unchanged; cutting it perpendicular to the axis into two plano-lenses doubles each focal length and halves each power.
  • Critical angle exists only for light going from denser to rarer. "Total internal reflection when light goes from air into glass" earns zero.
  • State both conditions for total internal reflection; one alone loses a mark.
  • At minimum deviation write all three of i=ei=e, r1=r2=A/2r_1=r_2=A/2 and "refracted ray parallel to the base" — CBSE marks the statement, not just the formula.
  • δm=(n−1)A\delta_m = (n-1)A is only for a thin prism. For a 60∘60^\circ prism use the full prism formula.
  • Least distance of distinct vision D=25D = 25 cm — put it in centimetres and keep every length in centimetres in microscope and telescope numericals.
  • Near point magnification of a magnifier is 1+D/f1 + D/f; at infinity it is D/fD/f. Choosing the wrong one is a whole mark.
  • For a telescope at the near point it is fofe(1+feD)\dfrac{f_o}{f_e}\left(1+\dfrac{f_e}{D}\right) — note fe/Df_e/D, not D/feD/f_e.
  • Objective for a telescope: large ff and large aperture. Objective for a microscope: small ff and small aperture. Swapping them in a lens-selection question is a common slip.
  • Aperture affects brightness and resolving power, never magnification.
  • A converging beam intercepted by a lens gives a virtual object with uu positive.
  • Frequency does not change on refraction; only speed and wavelength do.
  • Answer "nature of image" in full: real or virtual, erect or inverted, magnified or diminished, and where.
Solved Numerical ExamplesWorked numericals to attempt first, each with a hint before the full solution.Coming soon

These are being added chapter by chapter. They are solved numericals from the prescribed book and the reference guides — not previous board questions, which live under Practice — so that you can work through the method before meeting it in a real paper.

Important DerivationsEvery derive / obtain / prove question in this chapter.18
  1. 1
    Derivation 1
    Use the mirror equation to show that an object placed between ff and 2f2f of a concave mirror produces a real image beyond 2f2f.

    Asked in: CBSE Class 12 Physics — SA · Delhi 2015 · Section B, 2 marks

    Show the derivation

    For a concave mirror, f<0f<0. Let the object lie between ff and 2f2f, i.e. 2f<u<f2f<u<f (both negative), which can be written as 12f>1u>1f  \dfrac{1}{2f}>\dfrac1u>\dfrac1f\; or   −12f<−1u<−1f\;-\dfrac{1}{2f}<-\dfrac1u<-\dfrac1f. From the mirror formula, 1v=1f−1u\dfrac1v=\dfrac1f-\dfrac1u. Since 2f<u<f2f<u<f: subtracting 1u\dfrac1u (using the above inequality) from 1f\dfrac1f gives   1f−12f<1f−1u<1f−1f  \;\dfrac1f-\dfrac1{2f}<\dfrac1f-\dfrac1u<\dfrac1f-\dfrac1f\; i.e.   12f<1v<0\;\dfrac{1}{2f}<\dfrac1v<0 This implies v<0v<0 (real image) so that 2f>v2f>v i.e. ∣v∣>∣2f∣|v|>|2f|, meaning the image is formed beyond 2f2f (and the inequality 1v<0\dfrac1v<0 together with 12f<1v\dfrac1{2f}<\dfrac1v forces ∣v∣>2∣f∣|v|>2|f| since both are negative). Hence, an object placed between ff and 2f2f of a concave mirror produces a real image formed beyond 2f2f.

  2. 2
    Derivation 2
    An object is placed in front of a concave mirror. It is observed that a virtual image is formed. Draw the ray diagram to show the image formation and hence derive the mirror equation 1f=1u+1v\dfrac1f=\dfrac1u+\dfrac1v.

    Asked in: CBSE Class 12 Physics — Long Answer · 3/5, 2020 · Section E, 5 marks

    Show the derivation

    Consider an object ABAB placed on the principal axis of a concave mirror between its pole PP and focus FF. A ray AMAM from the object, parallel to the principal axis, strikes the mirror at MM and, after reflection, appears to come from the focus FF (i.e. the reflected ray, extended backwards, passes through FF). A second ray APAP incident at the pole PP reflects such that ∠APB=∠B′PA′\angle APB=\angle B'PA' (laws of reflection). The two reflected rays, when produced backwards, meet at a point A′A' behind the mirror — this is the virtual, erect, magnified image of AA; likewise, A′B′A'B' is the virtual image of ABAB. Using the Cartesian sign convention: object distance BP=−uBP=-u, image distance PB′=vPB'=v (note: since the image is virtual, B′B' lies on the same side as the object's ray extension, so with the convention used, PB′=vPB'=v is taken as measured to the virtual image point), focal length FP=−fFP=-f, and radius of curvature CP=−R=−2fCP=-R=-2f. From similar triangles △ABC∼△A′B′C\triangle ABC\sim\triangle A'B'C:   ABA′B′=CBCB′=CP−BPCP+PB′=−2f+u−2f+v\;\dfrac{AB}{A'B'}=\dfrac{CB}{CB'}=\dfrac{CP-BP}{CP+PB'}=\dfrac{-2f+u}{-2f+v} From similar triangles △MPF∼△A′B′F\triangle MPF\sim\triangle A'B'F:   MPA′B′=FPFB′=FPFP+PB′  \;\dfrac{MP}{A'B'}=\dfrac{FP}{FB'}=\dfrac{FP}{FP+PB'}\; i.e.   ABA′B′=−f−f+v\;\dfrac{AB}{A'B'}=\dfrac{-f}{-f+v} (since MP=ABMP=AB, both being perpendicular heights at the pole and at the object). Equating the two expressions for AB/A′B′AB/A'B':   −2f+u−2f+v=−f−f+v\;\dfrac{-2f+u}{-2f+v}=\dfrac{-f}{-f+v} Cross-multiplying and simplifying (expanding both sides and cancelling the 2f22f^2 terms) leads to   uv=fv+fu  \;uv=fv+fu\;, i.e. dividing throughout by uvfuvf:   1f=1u+1v\;\dfrac1f=\dfrac1u+\dfrac1v This proves the mirror equation for a concave mirror forming a virtual image.

  3. 3
    Derivation 3
    Using lens maker's formula, derive the thin lens formula 1f=1v−1u\dfrac1f=\dfrac1v-\dfrac1u.

    Asked in: CBSE Class 12 Physics — SA · 2020 · Section B, 2 marks

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    Consider a thin lens with surfaces of radii R1R_1 and R2R_2, refractive index n2n_2, placed in a medium of refractive index n1n_1. For refraction at the first surface XP1YXP_1Y alone (ignoring the second surface for now), with the object at OO (distance uu) and a virtual intermediate image at I′I' (distance v′v'), light travels from n1n_1 to n2n_2: n2v′−n1u=n2−n1R1...(i)\dfrac{n_2}{v'}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R_1}\qquad\text{...(i)} For refraction at the second surface XP2YXP_2Y, the point I′I' acts as a virtual object, and light now travels from n2n_2 to n1n_1, forming the final image at II (distance vv): n1v−n2v′=n1−n2R2...(ii)\dfrac{n_1}{v}-\dfrac{n_2}{v'}=\dfrac{n_1-n_2}{R_2}\qquad\text{...(ii)} Adding equations (i) and (ii), the n2/v′n_2/v' terms cancel:   n1v−n1u=(n2−n1)(1R1−1R2)\;\dfrac{n_1}{v}-\dfrac{n_1}{u}=(n_2-n_1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right) Dividing throughout by n1n_1:   1v−1u=(n2n1−1)(1R1−1R2)=(n21−1)(1R1−1R2)...(iii)\;\dfrac1v-\dfrac1u=\left(\dfrac{n_2}{n_1}-1\right)\left(\dfrac1{R_1}-\dfrac1{R_2}\right)=(n_{21}-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right)\qquad\text{...(iii)} When the object is at infinity (u→−∞u\to-\infty), the image forms at the focus, v=fv=f:   1f=(n21−1)(1R1−1R2)...(iv)\;\dfrac1f=(n_{21}-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right)\qquad\text{...(iv)} — this is the lens-maker's formula. Comparing equations (iii) and (iv), the right-hand sides are identical, so:   1v−1u=1f\;\dfrac1v-\dfrac1u=\dfrac1f — this is the thin lens formula, valid for a biconvex (and any thin) lens.

  4. 4
    Derivation 4
    (a) Derive lens maker's formula for a biconvex lens. (b) A point object is placed at a distance of 12 cm on the principal axis of a convex lens of focal length 10 cm. A convex mirror is placed coaxially on the other side of the lens at a distance of 10 cm. If the final image coincides with the object, sketch the ray diagram and find the focal length of the convex mirror.

    Asked in: CBSE Class 12 Physics — Long Answer · 2020 · Section E, 5 marks

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    (a) [See the general derivation: for refraction at each of the lens's two surfaces in turn, combining n2−n1R1=n2v′−n1u\dfrac{n_2-n_1}{R_1}=\dfrac{n_2}{v'}-\dfrac{n_1}{u} and n1−n2R2=n1v−n2v′\dfrac{n_1-n_2}{R_2}=\dfrac{n_1}{v}-\dfrac{n_2}{v'} and adding, one obtains 1v−1u=(n21−1)(1R1−1R2)\dfrac1v-\dfrac1u=(n_{21}-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right), and setting u→−∞u\to-\infty, v→fv\to f, gives the lens-maker's formula 1f=(n21−1)(1R1−1R2)\dfrac1f=(n_{21}-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right) — see Q24/Q39 for the full step-by-step version of this derivation.] (b) Since the final image coincides with the object itself, the rays from the object, after refraction through the lens and reflection from the mirror, must retrace their original path. This requires the rays refracted by the lens to fall normally on the mirror — which happens only if these refracted rays are directed exactly towards the mirror's centre of curvature. So the image formed by the lens alone must coincide with the centre of curvature of the mirror. For the lens: u=−12u=-12 cm, f=10f=10 cm. Using the lens formula:   1v−1−12=110  ⇒  1v=110−112=6−560=160\;\dfrac1v-\dfrac1{-12}=\dfrac1{10}\;\Rightarrow\;\dfrac1v=\dfrac1{10}-\dfrac1{12}=\dfrac{6-5}{60}=\dfrac1{60} ⇒v=60\Rightarrow v=60 cm. So the lens forms an image 60 cm from the lens. Since the mirror is 10 cm from the lens, this image lies at a distance R=v−d=60−10=50R=v-d=60-10=50 cm from the mirror — this must equal the mirror's radius of curvature for the rays to strike it normally. Hence R=50R=50 cm, and the focal length of the convex mirror is fmirror=R2=25f_{mirror}=\dfrac R2=25 cm.

  5. 5
    Derivation 5
    (a) Derive the mathematical relation between refractive indices n1n_1 and n2n_2 of two media and radius of curvature RR for refraction at a convex spherical surface. Consider the object to be a point source lying on the principal axis in rarer medium of refractive index n1n_1 and a real image formed in the denser medium of refractive index n2n_2. Hence, derive lens maker's formula. (b) Light from a point source in air falls on a convex spherical glass surface of refractive index 1.5 and radius of curvature 20 cm. The distance of the light source from the glass surface is 100 cm. At what position is the image formed?

    Asked in: CBSE Class 12 Physics — Long Answer · AI 2016 · Section E, 5 marks

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    (a) Let a point object OO lie in the rarer medium (n1n_1) on the axis, with a ray OAOA striking the convex spherical surface (centre CC, pole PP) at AA, refracting into the denser medium (n2n_2) and meeting the axis at the real image point II. Let α,β,γ\alpha,\beta,\gamma be the (small) angles that OAOA, IAIA and CACA make with the axis. In △OAC\triangle OAC, the angle of incidence i=α+γi=\alpha+\gamma; in △AIC\triangle AIC, γ=r+β\gamma=r+\beta, so the angle of refraction r=γ−βr=\gamma-\beta. By Snell's law:   1n2=sin⁡isin⁡r≈ir=α+γγ−β  ⇒  n2(γ−β)=n1(α+γ)  ⇒  (n2−n1)γ=n1α+n2β...(i)\;^1n_2=\dfrac{\sin i}{\sin r}\approx\dfrac ir=\dfrac{\alpha+\gamma}{\gamma-\beta}\;\Rightarrow\;n_2(\gamma-\beta)=n_1(\alpha+\gamma)\;\Rightarrow\;(n_2-n_1)\gamma=n_1\alpha+n_2\beta\qquad\text{...(i)} For paraxial rays (α,β,γ\alpha,\beta,\gamma small, and P,NP,N nearly coincident):   α≈ANPO,β≈ANPI,γ≈ANPC\;\alpha\approx\dfrac{AN}{PO},\quad\beta\approx\dfrac{AN}{PI},\quad\gamma\approx\dfrac{AN}{PC} Substituting into (i):   (n2−n1)ANPC=n1ANPO+n2ANPI  ⇒  n2−n1PC=n1PO+n2PI\;(n_2-n_1)\dfrac{AN}{PC}=n_1\dfrac{AN}{PO}+n_2\dfrac{AN}{PI}\;\Rightarrow\;\dfrac{n_2-n_1}{PC}=\dfrac{n_1}{PO}+\dfrac{n_2}{PI} With sign convention PC=+RPC=+R, PO=−uPO=-u, PI=+vPI=+v:   n2−n1R=n1−u+n2v  \;\dfrac{n_2-n_1}{R}=\dfrac{n_1}{-u}+\dfrac{n_2}{v}\;, i.e.   n2v−n1u=n2−n1R\;\dfrac{n_2}{v}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R} This is the required relation for refraction at a convex spherical surface, object in the rarer medium, real image in the denser medium. For a thin lens, applying this at both surfaces in turn and combining (as in Q24) gives the lens-maker's formula 1f=(n2n1−1)(1R1−1R2)\dfrac1f=\left(\dfrac{n_2}{n_1}-1\right)\left(\dfrac1{R_1}-\dfrac1{R_2}\right). (b) R=20R=20 cm, n2=1.5n_2=1.5, n1=1n_1=1, u=−100u=-100 cm.   n2v−n1u=n2−n1R  ⇒  1.5v+1100=0.520\;\dfrac{n_2}{v}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R}\;\Rightarrow\;\dfrac{1.5}{v}+\dfrac1{100}=\dfrac{0.5}{20} 1.5v=140−1100=5−2200=3200  ⇒  v=2003×1.5=100 cm\dfrac{1.5}{v}=\dfrac1{40}-\dfrac1{100}=\dfrac{5-2}{200}=\dfrac{3}{200}\;\Rightarrow\;v=\dfrac{200}{3}\times1.5=100\text{ cm} So a real image is formed 100 cm away from the surface, on the other (glass) side.

  6. 6
    Derivation 6
    (a) A point object 'O' is kept in a medium of refractive index n1n_1 in front of a convex spherical surface of radius of curvature RR which separates the second medium of refractive index n2n_2 from the first one, as shown in the figure. Draw the ray diagram showing the image formation and deduce the relationship between the object distance and the image distance in terms of n1n_1, n2n_2 and RR. (b) (i) When the image formed above acts as a virtual object for a concave spherical surface separating the medium n2n_2 from n1n_1 (n2>n1n_2>n_1), draw this ray diagram and write the similar (similar to (a)) relation. (ii) Hence, obtain the expression for the lens maker's formula.

    Asked in: CBSE Class 12 Physics — Long Answer · Delhi 2015, Ev · Section E, 5 marks

    Show the derivation

    (a) [Same derivation as Q37(a) above]: for a point object OO in medium n1n_1, refracting at a convex surface of radius RR into medium n2n_2 (n1<n2n_1<n_2), the relation obtained is   n2v−n1u=n2−n1R...(i)\;\dfrac{n_2}{v}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R}\qquad\text{...(i)}, with u,vu,v measured from the pole using the Cartesian sign convention. (b) (i) Now consider the image from (a) acting as a virtual object for a second, concave spherical surface (radius R′R') which separates the denser medium n2n_2 (in which the virtual object now sits) from n1n_1 on the far side (n2>n1n_2>n_1). By the same method (now with light travelling from n2n_2 into n1n_1 across this second surface):   n1v′−n2v=n1−n2R′...(ii)\;\dfrac{n_1}{v'}-\dfrac{n_2}{v}=\dfrac{n_1-n_2}{R'}\qquad\text{...(ii)} (ii) Adding equations (i) and (ii) (with appropriate relabelling for a thin lens, where the two surfaces are close together so the intermediate image distance vv is common to both), the n2n_2 terms cancel, giving   n1v′−n1u=(n2−n1)(1R−1R′)\;\dfrac{n_1}{v'}-\dfrac{n_1}{u}=(n_2-n_1)\left(\dfrac1R-\dfrac1{R'}\right) Dividing by n1n_1 and writing R=R1R=R_1, R′=R2R'=R_2, v′=vv'=v (final image):   1v−1u=(n2n1−1)(1R1−1R2)\;\dfrac1v-\dfrac1u=\left(\dfrac{n_2}{n_1}-1\right)\left(\dfrac1{R_1}-\dfrac1{R_2}\right) Setting u→−∞u\to-\infty gives v→fv\to f, so   1f=(n2n1−1)(1R1−1R2)\;\dfrac1f=\left(\dfrac{n_2}{n_1}-1\right)\left(\dfrac1{R_1}-\dfrac1{R_2}\right) — the lens-maker's formula — and hence, generally, 1v−1u=1f\dfrac1v-\dfrac1u=\dfrac1f (the thin lens formula).

  7. 7
    Derivation 7
    Draw a ray diagram showing the formation of the image by a point object on the principal axis of a spherical convex surface separating two media of refractive indices n1n_1 and n2n_2, when a point source is kept in the rarer medium of refractive index n1n_1. Derive the relation between object and image distance in terms of refractive index of the medium and radius of curvature of the surface. Hence obtain the expression for lens-maker's formula in the case of a thin convex lens.

    Asked in: CBSE Class 12 Physics — Long Answer · Delhi 2014C · Section E, 5 marks

    Show the derivation

    [Same derivation as Q37(a)]: for a point object OO in the rarer medium n1n_1, on the axis, refracting at a convex spherical surface of radius RR into the denser medium n2n_2, using the small-angle (paraxial) approximation for the angles subtended at the surface by the incident ray, the normal, and the refracted ray, and applying Snell's law, one obtains: n2v−n1u=n2−n1R\dfrac{n_2}{v}-\dfrac{n_1}{u}=\dfrac{n_2-n_1}{R} Applying this relation successively at the two surfaces of a thin convex lens (as in Q24/Q38) and adding, the intermediate-image term cancels, giving the thin lens formula 1v−1u=(n21−1)(1R1−1R2)\dfrac1v-\dfrac1u=(n_{21}-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right), and setting the object at infinity gives the lens-maker's formula 1f=(n21−1)(1R1−1R2)\dfrac1f=(n_{21}-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right).

  8. 8
    Derivation 8
    A symmetric biconvex lens of radius of curvature RR and made of glass of refractive index 1.5, is placed on a layer of liquid placed on top of a plane mirror. An optical needle with its tip on the principal axis of the lens is moved along the axis until its real, inverted image coincides with the needle itself. The distance of the needle from the lens is measured to be xx. On removing the liquid layer and repeating the experiment, the distance is found to be yy. Obtain the expression for the refractive index of the liquid in terms of xx and yy.

    Asked in: CBSE Class 12 Physics — SA · 2018, Cr · Section C, 3 marks

    Show the derivation

    In each case, the needle coincides with its own image only when the light retraces its path — i.e. when the object is placed exactly at the focus of the (lens + liquid-lens + mirror) combination. With the liquid present, the equivalent focal length of the (biconvex lens + liquid plano-concave lens) combination equals xx: so, if f1=yf_1=y is the biconvex lens's own focal length (found from the second experiment, with the liquid removed) and f2f_2 is the liquid lens's focal length:   1x=1f1+1f2=1y+1f2\;\dfrac1x=\dfrac1{f_1}+\dfrac1{f_2}=\dfrac1y+\dfrac1{f_2} ⇒1f2=1x−1y=y−xxy  ⇒  f2=xyy−x\Rightarrow\dfrac1{f_2}=\dfrac1x-\dfrac1y=\dfrac{y-x}{xy}\;\Rightarrow\;f_2=\dfrac{xy}{y-x} The liquid layer trapped between the lens's lower curved surface and the plane mirror forms a plano-concave lens, with R1=−RR_1=-R (curved face) and R2=∞R_2=\infty (flat face, against the mirror). Using the lens-maker's formula for this liquid lens (refractive index μl\mu_l):   1f2=(μl−1)(1R1−1R2)=(μl−1)(−1R)\;\dfrac1{f_2}=(\mu_l-1)\left(\dfrac1{R_1}-\dfrac1{R_2}\right)=(\mu_l-1)\left(-\dfrac1R\right) ⇒y−xxy=−(μl−1)R  ⇒  μl−1=(x−y)Rxy\Rightarrow\dfrac{y-x}{xy}=-\dfrac{(\mu_l-1)}{R}\;\Rightarrow\;\mu_l-1=\dfrac{(x-y)R}{xy} μl=1+(x−y)Rxy\mu_l=1+\dfrac{(x-y)R}{xy}

  9. 9
    Derivation 9
    (a) Using the ray diagram for a system of two lenses of focal lengths f1f_1 and f2f_2 in contact with each other, show that the two lens system can be regarded as equivalent to a single lens of focal length ff, where 1f=1f1+1f2\dfrac1f=\dfrac1{f_1}+\dfrac1{f_2}. Also write the relation for the equivalent power of the lens combination. (b) Determine the position of the image formed by the lens combination given in the figure: three thin lenses of focal lengths f1=+10f_1=+10 cm, f2=−10f_2=-10 cm and f3=+30f_3=+30 cm placed coaxially, with an object 30 cm in front of the first lens, a gap of 5 cm between the first and second lens, and a gap of 10 cm between the second and third lens.

    Asked in: CBSE Class 12 Physics — Long Answer · AI 2019, Ev · Section E, 5 marks

    Show the derivation

    (a) An object is placed at OO. Lens AA (focal length f1f_1) produces an image at I1I_1, which serves as a virtual object for lens BB (focal length f2f_2), which produces the final image at II. The lenses are thin, so their optical centres coincide. For lens AA:   1v1−1u=1f1...(i)\;\dfrac1{v_1}-\dfrac1u=\dfrac1{f_1}\qquad\text{...(i)} For lens BB:   1v−1v1=1f2...(ii)\;\dfrac1v-\dfrac1{v_1}=\dfrac1{f_2}\qquad\text{...(ii)} Adding (i) and (ii), the 1/v11/v_1 terms cancel:   1v−1u=1f1+1f2...(iii)\;\dfrac1v-\dfrac1u=\dfrac1{f_1}+\dfrac1{f_2}\qquad\text{...(iii)} If the combination is equivalent to a single lens of focal length ff:   1v−1u=1f...(iv)\;\dfrac1v-\dfrac1u=\dfrac1f\qquad\text{...(iv)} From (iii) and (iv):   1f=1f1+1f2  \;\dfrac1f=\dfrac1{f_1}+\dfrac1{f_2}\;, and correspondingly P=P1+P2P=P_1+P_2. (b) For lens L1L_1 (f=+10f=+10 cm): u=−30u=-30 cm.   1v1−1u=1f  ⇒  1v1=110−130=3−130=230\;\dfrac1{v_1}-\dfrac1u=\dfrac1f\;\Rightarrow\;\dfrac1{v_1}=\dfrac1{10}-\dfrac1{30}=\dfrac{3-1}{30}=\dfrac2{30} ⇒v1=15\Rightarrow v_1=15 cm. For lens L2L_2 (5 cm from L1L_1, f=−10f=-10 cm): the image from L1L_1 lies 15−5=1015-5=10 cm beyond L2L_2, acting as a virtual object, u=+10u=+10 cm. 1v2=1f+1u=1−10+110=0  ⇒  v2=∞\dfrac1{v_2}=\dfrac1f+\dfrac1u=\dfrac1{-10}+\dfrac1{10}=0\;\Rightarrow\;v_2=\infty — the rays emerge parallel after L2L_2. For lens L3L_3 (10 cm from L2L_2, f=+30f=+30 cm): since the incoming rays are parallel (object effectively at infinity), the final image forms at the focus of L3L_3. Hence the final image is formed at a distance of 30 cm from L3L_3 (the last lens).

  10. 10
    Derivation 10
    Draw a ray diagram to show the image formation by a combination of two thin convex lenses in contact. Obtain the expression for the power of this combination in terms of the focal lengths of the lenses.

    Asked in: CBSE Class 12 Physics — Long Answer · 2/5, AI 2015 · Section E, 5 marks

    Show the derivation

    Consider two thin convex lenses AA and BB, of focal lengths f1f_1 and f2f_2, placed in contact. For an object at OO, lens AA forms an intermediate image at I′I' (distance v′v'), which acts as the object for lens BB, which forms the final image at II (distance vv). For lens AA:   1v′−1u=1f1...(i)\;\dfrac1{v'}-\dfrac1u=\dfrac1{f_1}\qquad\text{...(i)} For lens BB:   1v−1v′=1f2...(ii)\;\dfrac1v-\dfrac1{v'}=\dfrac1{f_2}\qquad\text{...(ii)} Adding (i) and (ii):   1v−1u=1f1+1f2\;\dfrac1v-\dfrac1u=\dfrac1{f_1}+\dfrac1{f_2} Since the combination behaves as a single lens of focal length ff with 1v−1u=1f\dfrac1v-\dfrac1u=\dfrac1f, we get:   1f=1f1+1f2\;\dfrac1f=\dfrac1{f_1}+\dfrac1{f_2} Since power P=1/fP=1/f:   PT=P1+P2\;P_T=P_1+P_2

  11. 11
    Derivation 11
    Figure shows a ray of light PQ passing through a prism ABC (apex angle AA), refracting at Q on face AB and again at R on face AC, with the refracted ray QR parallel to the base BC. If the refracted ray QR is parallel to the base BC, show that (i) r1=r2=A/2r_1=r_2=A/2, (ii) the angle of minimum deviation is δm=2i−A\delta_m=2i-A.

    Asked in: CBSE Class 12 Physics — SA · Foreign 2014 · Section C, 3 marks

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    (i) Since QR is parallel to the base BC, by geometry the two base angles of the triangle formed by QR and the normals are equal, which forces the ray to be travelling symmetrically inside the prism: the angle of incidence at the first face equals the angle of emergence at the second face, i.e. i=ei=e, and correspondingly r1=r2r_1=r_2. Since r1+r2=Ar_1+r_2=A (the prism relation) and r1=r2r_1=r_2:   2r1=A  ⇒  r1=r2=A2\;2r_1=A\;\Rightarrow\;r_1=r_2=\dfrac A2 (ii) The general relation for a prism is A+δ=i+eA+\delta=i+e, where δ\delta is the angle of deviation. When the ray travels symmetrically (i=ei=e), the deviation is minimum, i.e. δ=δm\delta=\delta_m:   A+δm=i+i=2i\;A+\delta_m=i+i=2i ⇒  δm=2i−A\Rightarrow\;\delta_m=2i-A

  12. 12
    Derivation 12
    (a) Plot a graph showing the variation of the angle of deviation as a function of the angle of incidence, for light passing through a triangular prism. (b) Derive the relation for the refractive index of the material of the prism in terms of the angle of minimum deviation and the angle of the prism.

    Asked in: CBSE Class 12 Physics — Long Answer · AI 2019 · Section E, 5 marks

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    (a) As the angle of incidence ii is increased from a small value, the angle of deviation δ\delta first decreases, reaches a single minimum value δm\delta_m (at some particular ii, where the ray passes symmetrically through the prism, i=ei=e), and then increases again. The δ\delta-versus-ii graph is thus a smooth curve, concave-up, with a single minimum — it is NOT symmetric about the minimum in general shape but does have i=ei=e at that minimum. (b) For a prism of apex angle AA:   A=r1+r2...(i)\;A=r_1+r_2\qquad\text{...(i)}, and the total deviation   δ=(i−r1)+(e−r2)=(i+e)−(r1+r2)=(i+e)−A...(ii)\;\delta=(i-r_1)+(e-r_2)=(i+e)-(r_1+r_2)=(i+e)-A\qquad\text{...(ii)} At minimum deviation, δ=δm\delta=\delta_m, i=ei=e, and correspondingly r1=r2=rr_1=r_2=r (by symmetry). From (i):   r=A2\;r=\dfrac A2 From (ii):   δm=2i−A  ⇒  i=A+δm2\;\delta_m=2i-A\;\Rightarrow\;i=\dfrac{A+\delta_m}2 The refractive index of the prism material is then:   μ=sin⁡isin⁡r=sin⁡(A+δm2)sin⁡(A2)\;\mu=\dfrac{\sin i}{\sin r}=\dfrac{\sin\left(\dfrac{A+\delta_m}2\right)}{\sin\left(\dfrac A2\right)}

  13. 13
    Derivation 13
    (a) A ray PQ of light is incident on face AB of a glass prism ABC and emerges out of face AC. Trace the path of the ray and show that ∠i+∠e=∠A+∠δ\angle i+\angle e=\angle A+\angle\delta, where δ\delta and ee denote the angle of deviation and the angle of emergence respectively. Plot a graph showing the variation of the angle of deviation as a function of the angle of incidence. State the condition under which ∠δ\angle\delta is minimum. (b) Find the relation between the refractive index (μ\mu) of the glass prism and ∠A\angle A, for the case when the angle of the prism AA is equal to the angle of minimum deviation δm\delta_m. Hence obtain the value of the refractive index for a prism angle A=60°A=60°.

    Asked in: CBSE Class 12 Physics — Long Answer · AI 2015, Ev · Section E, 5 marks

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    (a) At face AB, the deviation produced is δ1=i−r1\delta_1=i-r_1. At face AC, the deviation produced is δ2=e−r2\delta_2=e-r_2. The total deviation is   δ=δ1+δ2=(i−r1)+(e−r2)=(i+e)−(r1+r2)\;\delta=\delta_1+\delta_2=(i-r_1)+(e-r_2)=(i+e)-(r_1+r_2) Since r1+r2=Ar_1+r_2=A:   δ=(i+e)−A  ⇒  i+e=A+δ\;\delta=(i+e)-A\;\Rightarrow\;i+e=A+\delta Graph: same δ\delta-versus-ii curve as in Q61/Q68 — decreasing then increasing, with a single minimum. The deviation δ\delta is minimum when the ray traverses the prism symmetrically, i.e. when i=ei=e (equivalently r1=r2r_1=r_2). (b) When A=δmA=\delta_m: from δm=2i−A\delta_m=2i-A, we get   A=2i−A  ⇒  i=A\;A=2i-A\;\Rightarrow\;i=A, and (since r1=r2=A/2r_1=r_2=A/2 at minimum deviation)   r=A2\;r=\dfrac A2   μ=sin⁡isin⁡r=sin⁡Asin⁡(A/2)\;\mu=\dfrac{\sin i}{\sin r}=\dfrac{\sin A}{\sin(A/2)} For A=60°A=60°:   μ=sin⁡60°sin⁡30°=3/21/2=3≈1.732\;\mu=\dfrac{\sin60°}{\sin30°}=\dfrac{\sqrt3/2}{1/2}=\sqrt3\approx1.732

  14. 14
    Derivation 14
    With the help of a ray diagram, show how a compound microscope forms a magnified image of a tiny object at the least distance of distinct vision. Hence derive an expression for the magnification produced by it. OR With the help of a ray diagram, explain the formation of the image in a compound microscope when the final image is formed at the near point. Obtain the expression for the magnifying power in this case.

    Asked in: CBSE Class 12 Physics — SA · Term II 2021-22 · Section C, 3 marks

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    Ray diagram: the tiny object OO is placed just beyond the focus of the objective lens (short focal length, small aperture); the objective forms a real, inverted, magnified image A′B′A'B' inside the tube. This image acts as the object for the eyepiece (also short focal length), which is positioned so that A′B′A'B' lies between its focus and optical centre; the eyepiece then forms a final virtual, magnified image A′′B′′A''B'' at the near point (or, in normal adjustment, at infinity). Magnification produced by the objective:   mo=vouo\;m_o=\dfrac{v_o}{u_o} Magnification produced by the eyepiece (acting as a simple magnifier, final image at near point DD):   me=1+Dfe\;m_e=1+\dfrac D{f_e} Total magnification:   m=mo×me=vouo(1+Dfe)\;m=m_o\times m_e=\dfrac{v_o}{u_o}\left(1+\dfrac D{f_e}\right) Since uo≈fou_o\approx f_o (object placed very close to the focus) and vo≈Lv_o\approx L (the tube length, i.e. separation between the lenses), this is often approximated as   m≈Lfo(1+Dfe)\;m\approx\dfrac L{f_o}\left(1+\dfrac D{f_e}\right)

  15. 15
    Derivation 15
    Draw a ray diagram showing the image formation by a compound microscope. Obtain the expression for the total magnification produced, when the final image is formed at infinity (normal adjustment).

    Asked in: CBSE Class 12 Physics — Long Answer · AI 2015C · Section E, 5 marks

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    Ray diagram: as in Q74, with the eyepiece now positioned so that the intermediate real image A′B′A'B' falls exactly at its focus, so the final image forms at infinity. Magnification by objective:   mo=vouo≈Lfo\;m_o=\dfrac{v_o}{u_o}\approx\dfrac L{f_o} (since vo≈Lv_o\approx L, the tube length, and uo≈fou_o\approx f_o). Magnification by eyepiece (final image at infinity):   me=Dfe\;m_e=\dfrac D{f_e} Total magnification:   M=mo×me=Lfo×Dfe\;M=m_o\times m_e=\dfrac L{f_o}\times\dfrac D{f_e}

  16. 16
    Derivation 16
    (i) Draw a ray diagram to show the working of a compound microscope. Obtain the expression for the total magnification when the final image is formed at the near point. (ii) In a compound microscope, an object is placed at a distance of 1.5 cm from the objective of focal length 1.25 cm. If the eyepiece has a focal length of 5 cm and the final image is formed at the near point, find the magnifying power of the microscope.

    Asked in: CBSE Class 12 Physics — Long Answer · 2023 · Section E, 5 marks

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    (i) Same ray diagram and derivation as Q74:   M=vouo(1+Dfe)\;M=\dfrac{v_o}{u_o}\left(1+\dfrac D{f_e}\right) (ii) uo=−1.5u_o=-1.5 cm, fo=1.25f_o=1.25 cm:   1vo=1fo+1uo=11.25−11.5=0.8−0.667=0.133  ⇒  vo=7.5 cm\;\dfrac1{v_o}=\dfrac1{f_o}+\dfrac1{u_o}=\dfrac1{1.25}-\dfrac1{1.5}=0.8-0.667=0.133\;\Rightarrow\;v_o=7.5\text{ cm}   mo=vouo=7.5−1.5=−5\;m_o=\dfrac{v_o}{u_o}=\dfrac{7.5}{-1.5}=-5   me=1+Dfe=1+255=6\;m_e=1+\dfrac D{f_e}=1+\dfrac{25}5=6   M=mo×me=(−5)(6)=−30\;M=m_o\times m_e=(-5)(6)=-30 (magnitude 30)

  17. 17
    Derivation 17
    (i) Draw a ray diagram to show how the final image is formed at infinity in an astronomical refracting telescope. Obtain an expression for its magnifying power. (ii) Two thin lenses L1L_1 and L2L_2 — L1L_1 a convex lens of focal length 24 cm, and L2L_2 a concave lens of focal length 18 cm — are placed coaxially at a separation of 45 cm. A 1 cm tall object is placed in front of lens L1L_1 at a distance of 36 cm. Find the location and height of the image formed by the combination.

    Asked in: CBSE Class 12 Physics — Long Answer · 2023 · Section E, 5 marks

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    (i) Same ray diagram and derivation as Q86/Q89:   M=fofe\;M=\dfrac{f_o}{f_e} (ii) For L1L_1 (f1=+24f_1=+24 cm): u1=−36u_1=-36 cm.   1v1=1f1+1u1=124−136=3−272=172  ⇒  v1=72 cm\;\dfrac1{v_1}=\dfrac1{f_1}+\dfrac1{u_1}=\dfrac1{24}-\dfrac1{36}=\dfrac{3-2}{72}=\dfrac1{72}\;\Rightarrow\;v_1=72\text{ cm} So L1L_1 would form its image 72 cm to its right — but L2L_2 is only 45 cm away, so this image forms 72−45=2772-45=27 cm beyond L2L_2, acting as a virtual object for L2L_2:   u2=+27 cm\;u_2=+27\text{ cm} For L2L_2 (f2=−18f_2=-18 cm):   1v2=1f2+1u2=−118+127=−3+254=−154  ⇒  v2=−54 cm\;\dfrac1{v_2}=\dfrac1{f_2}+\dfrac1{u_2}=-\dfrac1{18}+\dfrac1{27}=\dfrac{-3+2}{54}=-\dfrac1{54}\;\Rightarrow\;v_2=-54\text{ cm} So the final image forms 54 cm to the left of L2L_2 — since L1L_1 is 45 cm to the left of L2L_2, this places the final image 54−45=954-45=9 cm to the left of L1L_1 (i.e. on the object's side, between the object and L1L_1). This image is virtual. Overall magnification:   m=m1×m2=v1u1×v2u2=72−36×−5427=(−2)×(−2)=4\;m=m_1\times m_2=\dfrac{v_1}{u_1}\times\dfrac{v_2}{u_2}=\dfrac{72}{-36}\times\dfrac{-54}{27}=(-2)\times(-2)=4 Image height:   hi=m×ho=4×1 cm=4 cm\;h_i=m\times h_o=4\times1\text{ cm}=4\text{ cm} (erect relative to the object, since mm is positive; virtual).

  18. 18
    Derivation 18
    (i) Draw a ray diagram for the formation of the image of an object by an astronomical telescope in normal adjustment. Obtain the expression for its magnifying power. (ii) The magnifying power of an astronomical telescope in normal adjustment is 2.9, and the objective and the eyepiece are separated by a distance of 150 cm. Find the focal lengths of the two lenses.

    Asked in: CBSE Class 12 Physics — Long Answer · 2023 · Section E, 5 marks

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    (i) Same ray diagram and derivation as Q86/Q89/Q92:   M=fofe\;M=\dfrac{f_o}{f_e} (ii)   M=fofe=2.9  ⇒  fo=2.9fe\;M=\dfrac{f_o}{f_e}=2.9\;\Rightarrow\;f_o=2.9f_e, and (normal adjustment)   L=fo+fe=150 cm\;L=f_o+f_e=150\text{ cm} ⇒  2.9fe+fe=150  ⇒  3.9fe=150  ⇒  fe≈38.5 cm\Rightarrow\;2.9f_e+f_e=150\;\Rightarrow\;3.9f_e=150\;\Rightarrow\;f_e\approx38.5\text{ cm}   fo=150−38.5=111.5 cm\;f_o=150-38.5=111.5\text{ cm}

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