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Chapter 9 Ray Optics And Optical Instruments
Introduction
Light is the portion of the electromagnetic spectrum (wavelength ~400 nm to 750 nm) that is detectable by the human eye. Our understanding and interaction with the world are heavily reliant on light and vision. Key properties of light, based on common experience, are that it travels at an enormous speed and in straight lines.
While the speed of light is finite and measurable (approximately $c = 3 \times 10^8$ m/s in vacuum), the intuitive notion that light travels in straight lines seems to contradict its nature as an electromagnetic wave (as discussed in Chapter 8). This apparent contradiction is resolved by considering the very small wavelength of visible light compared to the size of everyday objects (typically a few cm or larger). In situations where the wavelength is much smaller than the object size, light propagation can be approximated as traveling along straight lines called **rays of light**. A bundle of such rays forms a beam of light.
This chapter uses the **ray picture of light** to study phenomena like reflection, refraction, and dispersion. We will analyse image formation by mirrors and lenses using the laws of reflection and refraction and describe the working principles of common optical instruments.
The historical particle model of light, proposed by Descartes and developed by Newton (corpuscular model), viewed light as tiny massless elastic particles. While it could explain reflection and refraction using mechanics, it faced difficulties explaining wave phenomena like thin film colours or partial reflection, which are better described by the wave picture.
Reflection Of Light By Spherical Mirrors
Reflection is governed by the laws of reflection: (i) The angle of reflection equals the angle of incidence ($ \angle i = \angle r'$). (ii) The incident ray, reflected ray, and the normal to the reflecting surface at the point of incidence all lie in the same plane. These laws apply to any reflecting surface, including spherical ones. For spherical surfaces, the normal at the point of incidence is along the radius vector from the center of curvature to that point.
A **spherical mirror** is a part of a sphere. Its geometric center is the **pole (P)**. The center of the sphere from which it is part is the **center of curvature (C)**. The line joining the pole and the center of curvature is the **principal axis**.
Sign Convention
To derive formulas for spherical mirrors and lenses applicable to all cases, a consistent sign convention is necessary. The **Cartesian sign convention** is followed:
- All distances are measured from the **pole** of the mirror (or optical center of the lens).
- Distances measured in the **same direction as the incident light** are taken as **positive**.
- Distances measured in the **opposite direction to the incident light** are taken as **negative**.
- Heights measured **upwards** from and perpendicular to the principal axis are taken as **positive**.
- Heights measured **downwards** from and perpendicular to the principal axis are taken as **negative**.
Focal Length Of Spherical Mirrors
When a parallel beam of light rays parallel to the principal axis (paraxial rays, incident close to the pole and at small angles) is incident on a spherical mirror:
- A **concave mirror** converges the reflected rays to a point $F$ on the principal axis called the **principal focus** [Fig. 9.3(a)].
- A **convex mirror** causes the reflected rays to appear to diverge from a point $F$ on the principal axis called the **principal focus** [Fig. 9.3(b)].
The **focal length ($f$)** of the mirror is the distance between the principal focus $F$ and the pole $P$. For paraxial rays, the focal length is half the radius of curvature ($R$) of the mirror:
$\mathbf{f = R/2}$
For a concave mirror, the focus is in front of the mirror (in the direction opposite to incident light), so $f$ is negative by the sign convention. For a convex mirror, the focus is behind the mirror (in the direction of incident light), so $f$ is positive.
The Mirror Equation
The **mirror equation** relates the object distance ($u$), image distance ($v$), and focal length ($f$) for spherical mirrors. The **image** of a point object is formed where rays from the object point converge or appear to diverge after reflection. A real image is formed where rays actually converge; a virtual image is where they appear to diverge from.
Using ray diagrams and the laws of reflection, and applying the Cartesian sign convention, the mirror equation is derived:
$\mathbf{\frac{1}{v} + \frac{1}{u} = \frac{1}{f}}$
Here, $u$ is the object distance (distance from pole to object), and $v$ is the image distance (distance from pole to image). Distances are signed according to convention.
The **linear magnification ($m$)** produced by a mirror is the ratio of the height of the image ($h'$) to the height of the object ($h$):
$\mathbf{m = \frac{h'}{h} = -\frac{v}{u}}$
$h'$ and $h$ are signed heights. $m$ is positive for an erect (virtual) image and negative for an inverted (real) image.
Ray diagrams for image formation can be drawn using specific convenient rays (parallel ray through focus, ray through center of curvature tracing back, ray towards focus becoming parallel, ray to pole reflecting according to laws). Any two suffice to locate the image point.
Example 9.1. Suppose that the lower half of the concave mirror’s reflecting surface in Fig. 9.5 is covered with an opaque (non-reflective) material. What effect will this have on the image of an object placed in front of the mirror?
Answer:
The image of an object is formed by rays from every point on the object reflecting off *all* parts of the mirror surface and converging (or appearing to diverge) to form the corresponding image point. If a portion of the mirror is covered, it simply means that the rays hitting that covered portion are no longer reflected to form the image. However, the remaining uncovered portion of the mirror can still reflect rays from the object to form the *entire* image.
Covering the lower half of the mirror will **not** result in only seeing the upper half of the object or half of the image. The **complete image** of the object will still be formed by the rays reflecting from the upper, uncovered half of the mirror.
The effect will be that the **intensity** (brightness) of the image will be reduced. This is because the total number of light rays from the object reaching the image point after reflection is reduced (by approximately half, since half the reflecting area is covered). This will make the image fainter.
Example 9.2. A mobile phone lies along the principal axis of a concave mirror, as shown in Fig. 9.7. Show by suitable diagram, the formation of its image. Explain why the magnification is not uniform. Will the distortion of image depend on the location of the phone with respect to the mirror?
Answer:
The mobile phone is an extended object placed along the principal axis. Different points on the phone are at different distances from the mirror. Let's consider two points on the phone: one closer to the mirror (say, point B) and one farther from the mirror (say, point A). Point C is on the principal axis. An object along the principal axis is sometimes called a longitudinal object. The formula $m = -v/u$ for magnification applies to the lateral magnification of an object perpendicular to the principal axis. Magnification along the axis is different.
Diagram for image formation:
Let's consider the image of point B at distance $u_B$ and point A at distance $u_A$. The image positions $v_B$ and $v_A$ are given by the mirror equation: $1/v_B + 1/u_B = 1/f$ and $1/v_A + 1/u_A = 1/f$. Since the points A and B are at different distances ($u_A \ne u_B$), their images will be formed at different distances ($v_A \ne v_B$), and the magnification $m=-v/u$ will also be different for different parts of the object.
Why magnification is not uniform: The lateral magnification $m = -v/u$ depends on the object distance $u$. Since different parts of the mobile phone (along the principal axis) are at different distances from the mirror, the lateral magnification will be different for each part. This means that a part of the object which is, for example, $1$ cm wide (perpendicular to the axis) at one location will have a different width in the image compared to a part which is $1$ cm wide at a different location along the phone's length. This varying magnification along the length of the object causes the **distortion** of the image.
Will the distortion depend on location? Yes. The magnification $m = -v/u$ changes with $u$. The relationship between $u$ and $v$ is non-linear ($1/v = 1/f - 1/u$). The rate at which magnification changes along the object's length depends on the absolute position of the object relative to the focal length and radius of curvature of the mirror. For example, if the entire phone is far from the mirror compared to its focal length, the object distances for different parts of the phone are relatively similar, and the distortion might be less noticeable. If the phone spans across the focal point or is very close to the mirror, the object distances vary significantly in terms of their relation to $f$, leading to more pronounced variations in magnification and thus greater distortion. The distortion of the image will definitely depend on the location of the phone with respect to the mirror.
Example 9.3. An object is placed at (i) 10 cm, (ii) 5 cm in front of a concave mirror of radius of curvature 15 cm. Find the position, nature, and magnification of the image in each case.
Answer:
Given: Concave mirror, radius of curvature $R = 15$ cm. For a concave mirror, $R$ is taken as negative according to sign convention, so $R = -15$ cm. Focal length $f = R/2 = -15/2 = -7.5$ cm. The object is placed in front of the mirror, so object distance $u$ is negative.
We use the mirror equation $\frac{1}{v} + \frac{1}{u} = \frac{1}{f}$ and magnification formula $m = -v/u$.
(i) Object placed at 10 cm in front: Object distance $u = -10$ cm.
$\frac{1}{v} + \frac{1}{-10} = \frac{1}{-7.5}$.
$\frac{1}{v} = \frac{1}{10} - \frac{1}{7.5} = \frac{1}{10} - \frac{1}{15/2} = \frac{1}{10} - \frac{2}{15}$.
Find a common denominator (30): $\frac{1}{v} = \frac{3}{30} - \frac{4}{30} = \frac{-1}{30}$.
$v = -30$ cm.
Image position: The image is formed at 30 cm in front of the mirror (since $v$ is negative). This is beyond the center of curvature ($R=-15$ cm, so 2f=-15 cm). The object is between f (-7.5 cm) and 2f (-15 cm). Expected image is real, inverted, and magnified, beyond 2f.
Magnification $m = -v/u = -(-30 \text{ cm}) / (-10 \text{ cm}) = 30 / (-10) = -3$.
Nature of image: Since $v$ is negative, the image is formed on the same side as the object, so it is a **real image**. Since $m$ is negative, the image is **inverted**. Since $|m| = 3 > 1$, the image is **magnified**.
Position: 30 cm in front of the mirror. Nature: Real, inverted, magnified. Magnification: -3.
(ii) Object placed at 5 cm in front: Object distance $u = -5$ cm.
$\frac{1}{v} + \frac{1}{-5} = \frac{1}{-7.5}$.
$\frac{1}{v} = \frac{1}{5} - \frac{1}{7.5} = \frac{1}{5} - \frac{2}{15}$.
Common denominator (15): $\frac{1}{v} = \frac{3}{15} - \frac{2}{15} = \frac{1}{15}$.
$v = +15$ cm.
Image position: The image is formed at 15 cm behind the mirror (since $v$ is positive). The object is between the pole (0 cm) and the focus (-7.5 cm). Expected image is virtual, erect, and magnified, behind the mirror.
Magnification $m = -v/u = -(+15 \text{ cm}) / (-5 \text{ cm}) = -15 / (-5) = +3$.
Nature of image: Since $v$ is positive, the image is formed behind the mirror, so it is a **virtual image**. Since $m$ is positive, the image is **erect**. Since $|m| = 3 > 1$, the image is **magnified**.
Position: 15 cm behind the mirror. Nature: Virtual, erect, magnified. Magnification: +3.
Example 9.4. Suppose while sitting in a parked car, you notice a jogger approaching towards you in the side view mirror of R = 2 m. If the jogger is running at a speed of 5 m s–1, how fast the image of the jogger appear to move when the jogger is (a) 39 m, (b) 29 m, (c) 19 m, and (d) 9 m away.
Answer:
The side view mirror of a car is a convex mirror. Radius of curvature $R = 2$ m. For a convex mirror, $R$ is positive, so $R = +2$ m. Focal length $f = R/2 = +2/2 = +1$ m. The jogger is approaching, so object distance $u$ is decreasing. Let the jogger's initial distance be $u_1$. After time $\Delta t$, the distance is $u_2 = u_1 - v_{jogger} \Delta t$. The speed of the image is $|v_{image}| = |\Delta v / \Delta t|$, where $\Delta v$ is the change in image position. We can approximate the instantaneous speed of the image by differentiating the mirror equation with respect to time: $\frac{d}{dt}(\frac{1}{v} + \frac{1}{u} = \frac{1}{f})$.
$\frac{d}{dt}(v^{-1}) + \frac{d}{dt}(u^{-1}) = \frac{d}{dt}(f^{-1})$.
$-1 v^{-2} \frac{dv}{dt} - 1 u^{-2} \frac{du}{dt} = 0$ (since $f$ is constant).
$\frac{1}{v^2} \frac{dv}{dt} = -\frac{1}{u^2} \frac{du}{dt}$.
Here, $\frac{dv}{dt}$ is the speed of the image, and $\frac{du}{dt}$ is the speed of the object. The jogger's speed is $v_{jogger} = |\frac{du}{dt}| = 5$ m/s. The object is approaching, so $u$ is becoming less negative, so $\frac{du}{dt} = +5$ m/s (change in distance from pole per unit time in direction of incident light). So, $\frac{du}{dt}$ is positive if the object is moving towards the mirror from far away (conventionally object is placed to the left, incident light from left). Let's assume object is placed on the left ($u$ is negative) and moves towards the mirror, so its position coordinate becomes less negative with time, meaning $du/dt$ is positive. Thus $du/dt = 5$ m/s.
Speed of the image $\frac{dv}{dt} = -\frac{v^2}{u^2} \frac{du}{dt}$. The term $(v/u)^2$ is the square of the lateral magnification $m^2$. $\frac{v}{u} = \frac{f}{u-f}$. So $\frac{dv}{dt} = -\left(\frac{f}{u-f}\right)^2 \frac{du}{dt}$.
Let's use $u$ as the object position coordinate. Incident light from left is positive. Object is in front, so $u$ coordinate is negative. Jogger moving towards mirror means $|u|$ is decreasing. $du/dt$ is positive if object moves towards positive x direction. Let mirror pole be at origin, principal axis along x-axis. Let incident light be from left to right (+x direction). Object is on the left, $u < 0$. Jogger moves towards mirror, so $u$ coordinate becomes less negative. $du/dt > 0$. $du/dt = +5$ m/s.
Convex mirror, $f = +1$ m. $u$ is negative. $v$ is positive (virtual image behind mirror). $\frac{1}{v} = \frac{1}{f} - \frac{1}{u} = \frac{1}{1} - \frac{1}{u} = \frac{u-1}{u}$. $v = \frac{u}{u-1}$. $\frac{dv}{dt} = \frac{d}{dt}\left(\frac{u}{u-1}\right) = \frac{(u-1)\frac{du}{dt} - u\frac{d(u-1)}{dt}}{(u-1)^2} = \frac{(u-1)\frac{du}{dt} - u\frac{du}{dt}}{(u-1)^2} = \frac{(u-1-u)\frac{du}{dt}}{(u-1)^2} = \frac{-1}{(u-1)^2}\frac{du}{dt}$.
Speed of the image (magnitude) $|v_{image}| = |\frac{dv}{dt}| = \frac{1}{(u-1)^2} |\frac{du}{dt}| = \frac{1}{(u-1)^2} \times 5$. Here $u$ is the negative object distance. Let the distance of the jogger from the mirror be $d = |u|$. So $u = -d$. Then $|v_{image}| = \frac{1}{(-d-1)^2} \times 5 = \frac{1}{(d+1)^2} \times 5$. The image is virtual ($v>0$), located between P and F ($0 < v < 1$ for $d>0$). As $d$ decreases (jogger approaches), $v = -d/(-d-1) = d/(d+1)$ increases (image moves towards F). $dv/dt$ is negative in the frame where image moves to the left. In car frame, image moves away from mirror. Speed is $|dv/dt|$.
Let's use the magnitude of distance $d$ in front of the mirror, so $u=-d$. $\frac{1}{v} + \frac{1}{-d} = \frac{1}{f} \implies \frac{1}{v} = \frac{1}{f} + \frac{1}{d} = \frac{d+f}{fd} \implies v = \frac{fd}{d+f}$. Here $f=+1$. $v = \frac{d}{d+1}$. As $d$ decreases, $v$ increases. $v_{image} = \frac{dv}{dt} = \frac{d}{dt}\left(\frac{d(t)}{d(t)+1}\right) = \frac{\frac{dd}{dt}(d+1) - d\frac{dd}{dt}}{(d+1)^2} = \frac{\frac{dd}{dt}(d+1-d)}{(d+1)^2} = \frac{1}{(d+1)^2}\frac{dd}{dt}$.
Jogger approaches at 5 m/s, so $d$ decreases at 5 m/s. $\frac{dd}{dt} = -5$ m/s. Speed of image is $|\frac{dv}{dt}| = |\frac{1}{(d+1)^2}(-5)| = \frac{5}{(d+1)^2}$. $d$ is the distance of the jogger from the mirror.
Given $f=1$ m.
(a) Jogger is 39 m away, $d = 39$ m. Speed of image $= \frac{5}{(39+1)^2} = \frac{5}{40^2} = \frac{5}{1600} = \frac{1}{320} = 0.003125$ m/s.
(b) Jogger is 29 m away, $d = 29$ m. Speed of image $= \frac{5}{(29+1)^2} = \frac{5}{30^2} = \frac{5}{900} = \frac{1}{180} = 0.00555...$ m/s.
(c) Jogger is 19 m away, $d = 19$ m. Speed of image $= \frac{5}{(19+1)^2} = \frac{5}{20^2} = \frac{5}{400} = \frac{1}{80} = 0.0125$ m/s.
(d) Jogger is 9 m away, $d = 9$ m. Speed of image $= \frac{5}{(9+1)^2} = \frac{5}{10^2} = \frac{5}{100} = \frac{1}{20} = 0.05$ m/s.
The text's values $1/280, 1/150, 1/60, 1/10$ m/s are different. Let's re-read the problem carefully. "how fast the image of the jogger appear to move when the jogger is... away". This usually means the instantaneous speed at that specific distance. My derivative approach calculates this instantaneous speed. Let's re-check the text's sample calculation for u=-39. "after 1 s the position of the image v (for u = –39 + 5 = –34) is (34/35 )m". This seems to assume u becomes -34 after 1 sec, so speed is 5. v for u=-39 is 39/40 m. v for u=-34 is 34/35 m. Shift in position in 1s is $|(34/35) - (39/40)| = |(1360-1365)/1400| = |-5/1400| = 5/1400 = 1/280$ m. Average speed is shift/time = $(1/280)/1 = 1/280$ m/s. The text is calculating the *average* speed of the image over a 1-second interval starting from the stated distance. This is a valid way to interpret "how fast it appears to move" over a small time, but the instantaneous speed from the derivative is more precise.
Using the text's method (average speed over 1s starting from the given distance $d$): Object moves from $u_1=-d$ to $u_2=-(d-5)$. Image moves from $v_1 = \frac{-d}{-d+1} = \frac{d}{d-1}$ (using $u$ negative, $f$ positive for convex mirror, $1/v + 1/u = 1/f$. $1/v = 1/f - 1/u$. $u$ is distance magnitude, so $u=-d$. $1/v = 1/1 - 1/(-d) = 1+1/d = (d+1)/d$. $v=d/(d+1)$). Let's use the distances $d$ as in the original problem. Object distance $u = -d$. $v = \frac{-df}{(-d)-f} = \frac{-d(1)}{-d-1} = \frac{-d}{-d-1} = \frac{d}{d+1}$. $f=+1$. $v = \frac{d}{d+1}$. Okay, my $v$ formula was $d/(d+1)$ and earlier $d/(d+f)$ which simplifies to $d/(d+1)$ for $f=1$. Let's re-calculate $v$. $\frac{1}{v} = \frac{1}{f} - \frac{1}{u} = \frac{1}{1} - \frac{1}{-d} = 1 + \frac{1}{d} = \frac{d+1}{d}$. So $v = \frac{d}{d+1}$. This is image position *behind* the mirror.
Let's use $u$ as the distance value from the mirror, $u>0$ in front. Then $u$ decreases with time, $du/dt = -5$. Mirror equation $\frac{1}{v} - \frac{1}{u} = \frac{1}{f}$ for convex mirror using standard formula for real/virtual image. But with Cartesian signs, $\frac{1}{v} + \frac{1}{-u} = \frac{1}{f}$. $\frac{1}{v} = \frac{1}{f} + \frac{1}{u}$. $u$ is the distance in front, so $u>0$. But using Cartesian signs, $u$ is position coordinate, typically negative for object in front. Let's stick to Cartesian signs: $u_{coord} < 0$. $|u_{coord}|$ is distance $d$. So $u_{coord} = -d$. $d$ is decreasing. $du_{coord}/dt = +5$ m/s. $f=+1$. $\frac{1}{v} + \frac{1}{u_{coord}} = \frac{1}{f}$. $\frac{1}{v} = \frac{1}{f} - \frac{1}{u_{coord}}$. $\frac{dv}{dt} = -\frac{v^2}{u_{coord}^2}\frac{du_{coord}}{dt}$. $|v_{image}| = |\frac{dv}{dt}| = \frac{v^2}{u_{coord}^2}|\frac{du_{coord}}{dt}| = (\frac{v}{u_{coord}})^2 \times 5$. $v = \frac{1}{1/f - 1/u_{coord}}$. Let's use the formula $|v_{image}| = \frac{f^2}{(u_{coord}-f)^2} |\frac{du_{coord}}{dt}| = \frac{1^2}{(u_{coord}-1)^2} \times 5$. $u_{coord} = -d$. $|v_{image}| = \frac{5}{(-d-1)^2} = \frac{5}{(d+1)^2}$. This is my instantaneous speed result.
The text's values suggest average speed over 1s. Using $d$ as the distance from the mirror.
(a) $d=39$. $u_1=-39$. $u_2=-(39-5)=-34$. $v_1 = \frac{1}{1 - 1/(-39)} = \frac{1}{1+1/39} = \frac{39}{40}$. $v_2 = \frac{1}{1 - 1/(-34)} = \frac{1}{1+1/34} = \frac{34}{35}$. Shift $= |v_2 - v_1| = |\frac{34}{35} - \frac{39}{40}| = |\frac{1360 - 1365}{1400}| = |-5/1400| = 5/1400 = 1/280$. Average speed $= 1/280$ m/s.
(b) $d=29$. $u_1=-29$. $u_2=-(29-5)=-24$. $v_1 = \frac{1}{1 - 1/(-29)} = \frac{29}{30}$. $v_2 = \frac{1}{1 - 1/(-24)} = \frac{24}{25}$. Shift $= |\frac{24}{25} - \frac{29}{30}| = |\frac{144 - 145}{150}| = |-1/150| = 1/150$. Average speed $= 1/150$ m/s.
(c) $d=19$. $u_1=-19$. $u_2=-(19-5)=-14$. $v_1 = \frac{1}{1 - 1/(-19)} = \frac{19}{20}$. $v_2 = \frac{1}{1 - 1/(-14)} = \frac{14}{15}$. Shift $= |\frac{14}{15} - \frac{19}{20}| = |\frac{56 - 57}{60}| = |-1/60| = 1/60$. Average speed $= 1/60$ m/s.
(d) $d=9$. $u_1=-9$. $u_2=-(9-5)=-4$. $v_1 = \frac{1}{1 - 1/(-9)} = \frac{9}{10}$. $v_2 = \frac{1}{1 - 1/(-4)} = \frac{4}{5}$. Shift $= |\frac{4}{5} - \frac{9}{10}| = |\frac{8 - 9}{10}| = |-1/10| = 1/10$. Average speed $= 1/10$ m/s.
The text's average speed calculation over 1s starting at the given distance matches the provided answers. So the question intends the average speed over a 1-second interval.
How fast the image of the jogger appear to move (average speed over 1s starting from the given distance): (a) 1/280 m/s, (b) 1/150 m/s, (c) 1/60 m/s, (d) 1/10 m/s.
Refraction
When a ray of light passes from one transparent medium to another, its direction changes at the interface. This phenomenon is called **refraction**. Part of the light is also reflected back (internal reflection when going from denser to rarer medium).
Refraction is governed by **Snell's laws**:
- (i) The incident ray, the refracted ray, and the normal to the interface at the point of incidence all lie in the same plane.
- (ii) The ratio of the sine of the angle of incidence ($i$) to the sine of the angle of refraction ($r$) is a constant for a given pair of media and wavelength of light. This constant is called the **refractive index** of the second medium with respect to the first medium, denoted as $n_{21}$.
$\mathbf{\frac{\sin i}{\sin r} = n_{21}}$
If $n_{21} > 1$, the second medium is optically denser than the first, and the refracted ray bends towards the normal ($r < i$). If $n_{21} < 1$, the second medium is optically rarer, and the refracted ray bends away from the normal ($r > i$). Optical density is related to the speed of light in the medium; light travels slower in an optically denser medium. $n_{21} = v_1/v_2$, where $v_1$ and $v_2$ are speeds of light in medium 1 and 2.
Refractive index is reciprocal: $n_{12} = 1/n_{21}$.
For three media, $n_{31} = n_{32} \times n_{21} = n_{32} \times \frac{n_{1}}{n_{2}}$, where $n_1, n_2, n_3$ are absolute refractive indices relative to vacuum. $n_{21} = n_2/n_1$. So $n_{31} = n_3/n_1$. $n_{32} \times n_{21} = (n_3/n_2) \times (n_2/n_1) = n_3/n_1$.
Refraction causes phenomena like lateral shift through a parallel slab, apparent depth of objects underwater (apparent depth = real depth / refractive index for normal viewing), and advance sunrise/delayed sunset due to atmospheric refraction.
Example 9.5. The earth takes 24 h to rotate once about its axis. How much time does the sun take to shift by 1° when viewed from the earth?
Answer:
The Earth rotates $360^\circ$ in 24 hours. When viewed from Earth, the Sun appears to complete a $360^\circ$ shift across the sky in approximately 24 hours (due to Earth's rotation). Assuming the Sun's apparent motion is uniform:
Time taken for $360^\circ$ shift = 24 hours.
To find the time taken for a $1^\circ$ shift, divide the total time by the total angle:
Time per degree = $\frac{24 \text{ hours}}{360^\circ}$.
Convert hours to minutes: 24 hours = $24 \times 60$ minutes = 1440 minutes.
Time per degree = $\frac{1440 \text{ minutes}}{360^\circ} = \frac{144}{36} \text{ minutes} = 4 \text{ minutes}$.
The Sun takes 4 minutes to shift by 1° when viewed from the Earth.
Total Internal Reflection
**Total internal reflection (TIR)** is a phenomenon that occurs when light travels from an optically denser medium to an optically rarer medium. As the angle of incidence ($i$) increases, the angle of refraction ($r$) increases and bends away from the normal. At a certain angle of incidence, the angle of refraction becomes 90° (the refracted ray grazes the interface). This angle of incidence is called the **critical angle ($i_c$)**.
According to Snell's law, $n_1 \sin i = n_2 \sin r$. At the critical angle, $i = i_c$ and $r = 90^\circ$. $n_1 \sin i_c = n_2 \sin 90^\circ = n_2$.
$\mathbf{\sin i_c = \frac{n_2}{n_1} = n_{21}}$ (where $n_{21}$ is refractive index of rarer medium 2 w.r.t. denser medium 1).
If the angle of incidence $i$ is increased beyond the critical angle ($i > i_c$), no refraction occurs. The light is completely reflected back into the denser medium. This complete reflection is called total internal reflection. Unlike normal reflection where some light is transmitted, in TIR, the reflected ray is as intense as the incident ray.
For TIR to occur, two conditions must be met: (i) Light must travel from an optically denser medium to an optically rarer medium. (ii) The angle of incidence in the denser medium must be greater than the critical angle for the pair of media.
The critical angle depends on the refractive indices of the two media. For air as the rarer medium (n$_2 \approx 1$), $\sin i_c = 1/n_1$, where $n_1$ is the refractive index of the denser medium.
Total Internal Reflection In Nature And Its Technological Applications
TIR explains several natural phenomena and is used in technology:
- (i) Mirage: An optical illusion common in hot conditions (deserts, highways) where light from distant objects is totally internally reflected by layers of air with varying refractive index (hot air near ground is rarer than cooler air above). This creates inverted images appearing like reflections from water.
- (ii) Diamond: The spectacular brilliance of diamonds is largely due to multiple total internal reflections inside them. Diamond has a very high refractive index (about 2.42) and a very small critical angle (~24.4°) with air, making TIR very likely once light enters. Diamond cutters shape diamonds to maximize TIR and enhance sparkle.
- (iii) Prisms: Right-angled prisms can use TIR to bend light by 90° or 180°, or to invert images without changing their size. This requires the prism material's critical angle to be less than 45°.
- (iv) Optical fibres: Used for transmitting signals (audio, video, data) as light pulses over long distances with minimal loss. An optical fibre consists of a core made of glass/quartz with a higher refractive index, surrounded by cladding with a lower refractive index. Light entering the core at a suitable angle undergoes repeated TIR at the core-cladding interface, traveling along the fibre's length even when bent. Bundles of fibres act as light pipes for endoscopy (visual examination of internal body organs) and decorative lamps. The material must have very low light absorption over long distances.
Intext Question 9.1. You have learnt that plane and convex mirrors produce virtual images of objects. Can they produce real images under some circumstances? Explain.
Answer:
A real image is formed when light rays from an object point *actually converge* to a point after reflection or refraction. A virtual image is formed where the rays *appear to diverge* from a point.
For plane mirrors, the image is always virtual, erect, and of the same size as the object. The rays diverge from the virtual image point behind the mirror.
For convex mirrors, the image of a real object is always virtual, erect, diminished, and located between the pole and the focus behind the mirror. The rays diverge from the virtual image point behind the mirror.
However, the mirror equation $1/v + 1/u = 1/f$ is valid for both real and virtual objects and images, using the sign convention. Let's consider if a real image ($v$ positive) can be formed by these mirrors.
- Plane mirror: $f = \infty$. The mirror equation becomes $1/v + 1/u = 0 \implies v = -u$. For a real object in front of the mirror ($u$ negative), $v$ is positive, meaning the image is behind the mirror. Image is virtual. For a virtual object (rays converging towards a point behind the mirror, $u$ positive), $v$ is negative, meaning the image is in front of the mirror. In this case, a real image is formed. So, a plane mirror can form a real image of a virtual object.
- Convex mirror: $f > 0$. The mirror equation is $1/v + 1/u = 1/f$. For a real object in front ($u$ negative), $1/v = 1/f - 1/u = 1/f + 1/|u|$. Since $f>0$ and $|u|>0$, $1/v > 0$, so $v>0$. Image is behind the mirror, virtual. For a virtual object (rays converging towards a point behind the mirror, $u$ positive), $1/v = 1/f - 1/u$. If $u > f$, then $1/v = \frac{u-f}{uf} > 0$, $v>0$, image is virtual. If $u < f$, then $1/v = \frac{f-u}{uf} > 0$, $v>0$, image is virtual. If $u > f$, then $1/v = \frac{u-f}{uf}$. If $u > f$, $u-f > 0$, $v$ positive, image virtual. Is $u$ always positive for virtual object? Yes, point towards mirror is positive. So, if rays are converging towards a point behind the mirror, $u$ is positive distance behind mirror. $u$ is positive coordinate. $1/v = 1/f - 1/u$. Since $f>0$, if $u$ is large positive, $1/v$ is positive, $v$ positive (virtual). If $u$ is small positive (point very close behind mirror), $1/v$ could be negative. Let $u > 0$. If $u > f$, $1/v = (u-f)/uf$. If $u
0$, $v>0$ virtual. If $u=f$, $1/v=0$, $v=\infty$. If $u>f$, $1/v = (u-f)/uf$. If $u 0$, $v$ is positive (virtual). If $1/f - 1/u < 0$, $v$ is negative (real). This happens if $1/u > 1/f$, i.e., $u < f$.
Answer: Yes, both plane and convex mirrors can produce real images if the object is a **virtual object** (i.e., the incident rays are converging towards a point behind the mirror). For a plane mirror, a virtual object at a distance $|u|$ behind the mirror forms a real image at the same distance in front. For a convex mirror, a virtual object located closer to the mirror than its focal point (and behind the mirror, so $u>0$ and $u < f$) will form a real image in front of the mirror ($v<0$).
Intext Question 9.2. A virtual image, we always say, cannot be caught on a screen. Yet when we ‘see’ a virtual image, we are obviously bringing it on to the ‘screen’ (i.e., the retina) of our eye. Is there a contradiction?
Answer:
No, there is no contradiction. The statement that a virtual image cannot be caught on a screen means that the light rays forming the virtual image do not *actually converge* at the location of the virtual image. They only *appear to diverge* from that point. If you place a screen at the location of a virtual image, the light rays will pass through the screen or be blocked by it; they will not converge to form an image on the screen.
When we see a virtual image, for example, in a plane mirror or through a magnifying glass, our eye's lens acts as a converging lens. The diverging rays that appear to come from the virtual image enter our eye and are converged by the eye's lens onto the retina, which acts as a screen. Our brain then interprets the signals from the retina to perceive the image at the location of the virtual image.
So, the virtual image itself is not formed on a screen *at the location of the virtual image*. Instead, the eye's lens forms a *real image* of the virtual image *on the retina*. Our visual system's ability to converge diverging rays allows us to see virtual images. A typical screen placed at the virtual image location cannot perform this convergence.
Intext Question 9.3. A diver under water, looks obliquely at a fisherman standing on the bank of a lake. Would the fisherman look taller or shorter to the diver than what he actually is?
Answer:
Light rays travel from the fisherman (in air, rarer medium) to the diver (under water, denser medium). When light travels from a rarer medium to a denser medium, it bends **towards the normal**. Consider rays coming from the fisherman's head and feet. Let the fisherman be at a distance from the point directly above the diver. Rays from the top of the fisherman's head reach the water surface. They bend towards the normal upon entering the water and travel towards the diver. When the diver traces these refracted rays back into the air, they will appear to originate from a point higher than the fisherman's actual height.
Imagine the fisherman's head at point H above the water. Rays from H refract into the water towards the diver. Due to bending towards the normal, the rays entering the water will seem to come from a point H' higher than H when traced back from underwater. Similarly, rays from the fisherman's feet at F will refract and appear to come from a point F' lower than F (or higher than actual feet position relative to water level, but the apparent effect is related to the height difference). Because the rays from the top bend towards the normal and appear to originate from a higher point, the apparent height of the fisherman observed by the diver will be **taller** than the actual height.
This is the opposite effect of looking at an object underwater from air, where the object appears shallower than its real depth.
Intext Question 9.4. Does the apparent depth of a tank of water change if viewed obliquely? If so, does the apparent depth increase or decrease?
Answer:
Yes, the apparent depth of a tank of water changes if viewed obliquely. The formula that apparent depth = real depth / refractive index ($h_{app} = h_{real} / n$) is strictly valid only for viewing near the normal (at small angles of incidence). When viewed obliquely (at larger angles of incidence), the apparent depth **decreases**. The bottom appears to be raised even more when viewed from an oblique angle compared to viewing near the normal.
Explanation: Consider a point at the bottom. Light rays from this point travel upwards. When viewed near the normal, the rays refract away from the normal upon entering the air, and tracing them back gives the apparent position closer to the surface. When viewed obliquely, the angle of incidence in water is larger. The angle of refraction in air is even larger. Tracing these highly deviated refracted rays back into the water, they intersect at a point *higher* than the apparent position seen near the normal. Thus, the apparent depth decreases when viewed obliquely.
Intext Question 9.5. The refractive index of diamond is much greater than that of ordinary glass. Is this fact of some use to a diamond cutter?
Answer:
Yes, this fact is of great use to a diamond cutter. The brilliance of a diamond is primarily due to **total internal reflection (TIR)**. TIR occurs when light travels from a denser medium to a rarer medium and the angle of incidence in the denser medium exceeds the critical angle ($i_c$). The critical angle is given by $\sin i_c = n_{rarer} / n_{denser}$.
Diamond has a very high refractive index ($n_{diamond} \approx 2.42$) compared to glass ($n_{glass} \approx 1.5$). For the diamond-air interface, the critical angle is $\sin i_c = 1/2.42 \approx 0.413$, which gives $i_c \approx 24.4^\circ$. This critical angle is very small compared to glass-air interface ($i_c = \sin^{-1}(1/1.5) \approx 41.8^\circ$).
A diamond cutter cuts the facets of the diamond in such a way that light entering the diamond undergoes multiple total internal reflections inside before emerging. Because the critical angle is so small, it is much easier for light to undergo TIR inside diamond than inside glass. By carefully cutting the facets at appropriate angles, the cutter can ensure that most of the light entering the diamond is reflected internally multiple times before exiting, making it sparkle brilliantly. The high refractive index also contributes to a large dispersion of light, further enhancing the display of colours (fire) when white light passes through a diamond. While high dispersion is also important, the small critical angle due to the high refractive index is key to maximising TIR.
Refraction At Spherical Surfaces And By Lenses
We extend the study of refraction from plane interfaces to spherical interfaces between two transparent media. An infinitesimal part of a spherical surface can be treated as planar, and Snell's laws apply locally. The normal to the spherical surface at any point passes through its center of curvature.
Refraction At A Spherical Surface
Consider a spherical surface with radius of curvature $R$, separating two media with refractive indices $n_1$ (where object is) and $n_2$ (where image is formed). For an object point O on the principal axis, forming an image point I, and center of curvature C, for paraxial rays (small angles), the relationship between object distance ($u$), image distance ($v$), and radius of curvature ($R$) is given by:
$\mathbf{\frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2 - n_1}{R}}$
Here, distances $u, v, R$ are measured from the pole of the surface and are signed according to the Cartesian sign convention. $u$ is the distance from pole to object, $v$ is the distance from pole to image, and $R$ is the radius of curvature.
Example 9.6. Light from a point source in air falls on a spherical glass surface (n = 1.5 and radius of curvature = 20 cm). The distance of the light source from the glass surface is 100 cm. At what position the image is formed?
Answer:
Given: Point source in air ($n_1 = 1$). Spherical glass surface ($n_2 = 1.5$). Radius of curvature $R = 20$ cm. Distance of light source from glass surface $u = 100$ cm. Since the object is in front of the surface (assuming incident light direction is positive), $u = -100$ cm according to the Cartesian sign convention. The glass surface is convex if $R > 0$, concave if $R < 0$. From the example diagram, it appears to be a convex surface towards the incident light, so let's assume $R = +20$ cm.
We use the refraction formula for a spherical surface: $\frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2 - n_1}{R}$.
Substitute the given values: $n_1 = 1$, $n_2 = 1.5$, $u = -100$ cm, $R = +20$ cm.
$\frac{1.5}{v} - \frac{1}{-100} = \frac{1.5 - 1}{+20}$.
$\frac{1.5}{v} + \frac{1}{100} = \frac{0.5}{20} = \frac{1}{40}$.
$\frac{1.5}{v} = \frac{1}{40} - \frac{1}{100} = \frac{5}{200} - \frac{2}{200} = \frac{3}{200}$.
$v = 1.5 \times \frac{200}{3} = \frac{3}{2} \times \frac{200}{3} = 100$ cm.
The image distance $v = +100$ cm. Since $v$ is positive, the image is formed in the same direction as the incident light (behind the spherical surface). The image is real.
The image is formed at a distance of 100 cm from the glass surface, behind the surface.
Refraction By A Lens
A **lens** is a transparent medium bounded by two surfaces, at least one of which is spherical. A **thin lens** is one where the thickness is negligible compared to the radii of curvature of its surfaces and object/image distances.
Image formation by a lens can be analysed by applying the formula for refraction at a single spherical surface successively at each of the two surfaces. For a thin lens with two spherical surfaces with radii of curvature $R_1$ and $R_2$, separating media with refractive indices $n_1$ (outside) and $n_2$ (lens material), the **lens maker's formula** relates focal length to properties of the lens and surrounding medium:
$\mathbf{\frac{1}{f} = (\frac{n_2}{n_1} - 1) \left(\frac{1}{R_1} - \frac{1}{R_2}\right)}$
Here, $R_1$ is the radius of curvature of the first surface encountered by light, and $R_2$ is for the second surface. Signs of $R_1, R_2$ are according to Cartesian sign convention (center of curvature on the right is positive $R$, on the left is negative $R$). For a convex lens (thicker in middle), $f$ is usually positive. For a concave lens (thinner in middle), $f$ is usually negative.
The **thin lens formula** relates object distance ($u$), image distance ($v$), and focal length ($f$) for a thin lens:
$\mathbf{\frac{1}{v} - \frac{1}{u} = \frac{1}{f}}$
Distances $u, v, f$ are measured from the optical center of the lens and are signed according to convention. $u$ is negative for a real object in front. $v$ is positive for a real image behind, negative for a virtual image in front.
The **linear magnification ($m$)** for a lens is $m = h'/h$, where $h'$ and $h$ are signed heights. Similar to mirrors, for a lens:
$\mathbf{m = \frac{h'}{h} = \frac{v}{u}}$
($m$ is positive for erect image, negative for inverted image).
Ray diagrams for lenses use convenient rays: parallel ray through focus, ray through optical center undeviated, ray through focus becoming parallel.
Power Of A Lens
The **power ($P$)** of a lens is a measure of its ability to converge or diverge light. It is defined as the reciprocal of its focal length in meters:
$\mathbf{P = \frac{1}{f}}$ (where $f$ is in meters)
The SI unit of power is the **dioptre (D)**. $1 \text{ D} = 1 \text{ m}^{-1}$. A converging lens (convex lens) has positive power ($f > 0$); a diverging lens (concave lens) has negative power ($f < 0$). An optician prescribes lenses in dioptres.
Example 9.8. (i) If f = 0.5 m for a glass lens, what is the power of the lens? (ii) The radii of curvature of the faces of a double convex lens are 10 cm and 15 cm. Its focal length is 12 cm. What is the refractive index of glass? (iii) A convex lens has 20 cm focal length in air. What is focal length in water? (Refractive index of air-water = 1.33, refractive index for air-glass = 1.5.)
Answer:
(i) Power of the lens: Given focal length $f = 0.5$ m. The lens is a glass lens, typically a convex lens for positive focal length. Power $P = 1/f$.
$P = \frac{1}{0.5 \text{ m}} = 2 \text{ m}^{-1} = 2 \text{ D}$. Since $f>0$, power is positive. The power of the lens is +2.0 dioptres.
(ii) Refractive index of glass: Double convex lens. Let light be incident from the left. The first surface is convex, so its center of curvature is to the right, $R_1 = +10$ cm $= +0.10$ m. The second surface is also convex, but its center of curvature is to the left (on the side from which light comes *from* the first surface), so $R_2 = -15$ cm $= -0.15$ m. Focal length $f = 12$ cm $= +0.12$ m. Let $n_1$ be the refractive index of the surrounding medium (air, $n_1=1$), and $n_2$ be the refractive index of glass.
Use the lens maker's formula: $\frac{1}{f} = (\frac{n_2}{n_1} - 1) \left(\frac{1}{R_1} - \frac{1}{R_2}\right)$.
$\frac{1}{0.12} = (\frac{n_2}{1} - 1) \left(\frac{1}{+0.10} - \frac{1}{-0.15}\right)$.
$\frac{1}{0.12} = (n_2 - 1) \left(\frac{1}{0.10} + \frac{1}{0.15}\right)$.
$\frac{1}{0.12} = (n_2 - 1) \left(\frac{100}{10} + \frac{100}{15}\right) = (n_2 - 1) \left(10 + \frac{20}{3}\right) = (n_2 - 1) \left(\frac{30 + 20}{3}\right) = (n_2 - 1) \left(\frac{50}{3}\right)$.
$\frac{1}{0.12} = \frac{50}{3} (n_2 - 1)$.
$n_2 - 1 = \frac{3}{50 \times 0.12} = \frac{3}{6.0} = 0.5$.
$n_2 = 1 + 0.5 = 1.5$.
The refractive index of glass is 1.5.
(iii) Focal length in water: Convex lens in air, $f_{air} = 20$ cm $= 0.20$ m. Refractive index of air $n_{air} = 1$, glass $n_{glass} = 1.5$. From lens maker's formula: $\frac{1}{f_{air}} = (n_{glass}/n_{air} - 1)(\frac{1}{R_1} - \frac{1}{R_2})$.
$\frac{1}{0.20} = (1.5/1 - 1) (\frac{1}{R_1} - \frac{1}{R_2}) = (0.5) (\frac{1}{R_1} - \frac{1}{R_2})$.
So, $(\frac{1}{R_1} - \frac{1}{R_2}) = \frac{1}{0.20 \times 0.5} = \frac{1}{0.10} = 10$ m$^{-1}$. This difference of curvatures is 10 m$^{-1}$.
Now, the same lens is placed in water. Refractive index of water $n_{water} = 1.33$. Refractive index of glass relative to water is $n_{glass}/n_{water} = 1.5/1.33 \approx 1.128$. Let $f_{water}$ be the focal length in water.
$\frac{1}{f_{water}} = (n_{glass}/n_{water} - 1)(\frac{1}{R_1} - \frac{1}{R_2})$.
$\frac{1}{f_{water}} = (1.128 - 1) \times (10 \text{ m}^{-1}) = (0.128) \times 10 = 1.28$ m$^{-1}$.
$f_{water} = \frac{1}{1.28} \text{ m} \approx 0.781 \text{ m} = 78.1$ cm. The text gives 78.2 cm.
The focal length of the convex lens in water is approximately 78.1 cm.
Combination Of Thin Lenses In Contact
When two or more thin lenses are placed in contact with each other, the combination acts as a single lens with an equivalent focal length. For two thin lenses with focal lengths $f_1$ and $f_2$ in contact, the equivalent focal length $f$ is given by:
$\mathbf{\frac{1}{f} = \frac{1}{f_1} + \frac{1}{f_2}}$
This formula can be derived by considering image formation by the first lens, which acts as the object for the second lens. For the first lens, $\frac{1}{v_1} - \frac{1}{u} = \frac{1}{f_1}$, where $v_1$ is the image distance. This image $v_1$ is the object for the second lens. Since the lenses are in contact, the object distance for the second lens is $u_2 = -v_1$ (using sign convention appropriately, or just the numerical value if one is a real image becoming a virtual object). For thin lenses in contact, the image from the first lens $I_1$ is at distance $v_1$ from the contact point. This image is the object for the second lens, at distance $u_2=v_1$ from the second lens (which is at the same contact point). So, $\frac{1}{v} - \frac{1}{v_1} = \frac{1}{f_2}$. Adding the two lens equations: $\frac{1}{v} - \frac{1}{u} = \frac{1}{f_1} + \frac{1}{f_2}$. Since $\frac{1}{v} - \frac{1}{u} = \frac{1}{f}$ for the combination, the formula is valid.
For a combination of several thin lenses ($f_1, f_2, ..., f_n$) in contact:
$\mathbf{\frac{1}{f} = \frac{1}{f_1} + \frac{1}{f_2} + ... + \frac{1}{f_n}}$
In terms of power $P = 1/f$, the total power of the combination is the algebraic sum of individual powers:
$\mathbf{P = P_1 + P_2 + ... + P_n}$
The total magnification $m$ of a combination is the product of individual magnifications: $m = m_1 m_2 ... m_n$. Lens combinations are used in complex optical instruments to achieve desired focal lengths, magnifications, and correct aberrations.
Example 9.9. Find the position of the image formed by the lens combination given in the Fig. 9.22.
Answer:
We have three thin lenses along an axis. Lens 1: Convex, $f_1 = +10$ cm. Lens 2: Concave, $f_2 = -10$ cm. Lens 3: Convex, $f_3 = +30$ cm. The object is placed at 30 cm in front of the first lens. Let's denote distances and positions relative to each lens.
Step 1: Image formed by the first lens (L1). Object distance $u_1 = -30$ cm (in front of L1). $f_1 = +10$ cm.
Using the lens formula $\frac{1}{v_1} - \frac{1}{u_1} = \frac{1}{f_1}$.
$\frac{1}{v_1} - \frac{1}{-30} = \frac{1}{+10}$.
$\frac{1}{v_1} + \frac{1}{30} = \frac{1}{10}$.
$\frac{1}{v_1} = \frac{1}{10} - \frac{1}{30} = \frac{3}{30} - \frac{1}{30} = \frac{2}{30} = \frac{1}{15}$.
$v_1 = +15$ cm. The image $I_1$ is formed 15 cm to the right of the first lens. This is a real image.
Step 2: Image formed by the second lens (L2). The second lens is located 5 cm to the right of the first lens. The image $I_1$ formed by L1 is at 15 cm to the right of L1. So, the distance of $I_1$ from L2 is $u_2 = 15 \text{ cm} - 5 \text{ cm} = 10 \text{ cm}$. Since $I_1$ is on the right side of L2, and incident light on L2 is from the left, $I_1$ acts as a virtual object for L2. By sign convention, object distance for a virtual object is positive. So $u_2 = +10$ cm. $f_2 = -10$ cm.
Using the lens formula for L2: $\frac{1}{v_2} - \frac{1}{u_2} = \frac{1}{f_2}$.
$\frac{1}{v_2} - \frac{1}{+10} = \frac{1}{-10}$.
$\frac{1}{v_2} = \frac{1}{10} - \frac{1}{10} = 0$.
$v_2 = \infty$. The image $I_2$ is formed at infinity.
Step 3: Image formed by the third lens (L3). The third lens is located 10 cm to the right of the second lens. The image $I_2$ formed by L2 is at infinity. This serves as the object for L3. The object is at infinity, so $u_3 = \infty$. $f_3 = +30$ cm.
Using the lens formula for L3: $\frac{1}{v_3} - \frac{1}{u_3} = \frac{1}{f_3}$.
$\frac{1}{v_3} - \frac{1}{\infty} = \frac{1}{+30}$.
$\frac{1}{v_3} - 0 = \frac{1}{30}$.
$v_3 = +30$ cm.
The final image $I_3$ is formed 30 cm to the right of the third lens. Since $v_3$ is positive, the final image is real.
The position of the final image is 30 cm to the right of the third lens.
Refraction Through A Prism
A **prism** is a transparent medium bounded by two plane surfaces inclined at an angle. The angle between the two refracting faces is called the **angle of the prism (A)**.
Consider a ray of light PQ incident on face AB of a prism ABC at angle $i$, refracting at angle $r_1$. The refracted ray QR travels through the prism and is incident on face AC at angle $r_2$, refracting out at angle of emergence $e$ (ray RS).
The angle between the emergent ray RS and the direction of the incident ray PQ is the **angle of deviation ($\delta$)**.
From geometry, the angles are related:
- $r_1 + r_2 = A$
- $\delta = (i - r_1) + (e - r_2) = i + e - (r_1 + r_2) = i + e - A$
The angle of deviation $\delta$ depends on the angle of incidence $i$. A plot of $\delta$ versus $i$ shows that there is a minimum angle of deviation ($D_m$) for a specific angle of incidence. At minimum deviation, the angle of incidence equals the angle of emergence ($i=e$), and the angle of refraction at both faces is the same ($r_1 = r_2 = r$).
At minimum deviation ($i=e, r_1=r_2=r$):
- $2r = A \implies r = A/2$
- $D_m = i + i - A = 2i - A \implies i = (A + D_m)/2$
Using Snell's law ($n_1 \sin i = n_2 \sin r$) at the first face, where $n_1$ is the refractive index of the surrounding medium and $n_2$ is the refractive index of the prism material:
$\mathbf{n_1 \sin \left(\frac{A + D_m}{2}\right) = n_2 \sin \left(\frac{A}{2}\right)}$.
If the surrounding medium is air ($n_1=1$), the refractive index of the prism material is:
$\mathbf{n_2 = \frac{\sin \left(\frac{A + D_m}{2}\right)}{\sin \left(\frac{A}{2}\right)}}$.
Measuring $A$ and $D_m$ experimentally allows calculating the refractive index of the prism material. For a thin prism (small angle $A$), the deviation is small, and $D_m \approx (n_{21} - 1)A$, where $n_{21}=n_2/n_1$.
Intext Question 9.6. Find the position of the image formed by the lens combination given in the Fig. 9.22.
Answer:
The text has already worked through this example and found the final image position is 30 cm to the right of the third lens. Please refer back to Example 9.9 in the main text for the solution steps.
Some Natural Phenomena Due To Sunlight
Sunlight interacting with the atmosphere and water droplets creates various beautiful phenomena.
Dispersion: White light (like sunlight) is composed of different colours (frequencies/wavelengths). When white light passes through a transparent medium like glass or water, the refractive index of the medium is slightly different for different frequencies. This causes different colours to bend by slightly different amounts (dispersion), splitting white light into its constituent colours. Red light (longest wavelength) bends the least, and violet light (shortest wavelength) bends the most.
Vacuum (or air approximately) is non-dispersive; all colours travel at the same speed. Glass is a dispersive medium.
The Rainbow
A **rainbow** is a natural spectrum observed after rain, formed by the dispersion of sunlight by spherical water droplets. Conditions for observing a rainbow: Sun shining in one part of the sky, rain in the opposite part, observer with back towards the Sun.
Primary rainbow formation:
- Sunlight enters a raindrop and is refracted, dispersing into its colours.
- These coloured rays hit the inner surface of the drop and undergo **total internal reflection** (if the angle of incidence exceeds the critical angle).
- The reflected rays refract again as they exit the drop into the air, further separating the colours.
Observer sees different colours from different drops at slightly different angles relative to the incoming sunlight. Violet light emerges at about 40°, red at about 42°. Red is on top, violet on bottom in the primary rainbow.
Secondary rainbow formation: When light undergoes **two internal reflections** inside the raindrop. It is fainter and has the colours reversed (red on bottom, violet on top). It is observed at a larger angle than the primary rainbow (around 50°-53°).
Scattering Of Light
As sunlight passes through the atmosphere, it is scattered by atmospheric particles (molecules, dust, water droplets). The amount of scattering depends on the wavelength of light and the size of the scattering particles.
Rayleigh scattering: For particles much smaller than the wavelength of light ($a \ll \lambda$), scattering is inversely proportional to the fourth power of the wavelength ($I \propto 1/\lambda^4$). Shorter wavelengths (blue, violet) are scattered much more strongly than longer wavelengths (red).
- Blue colour of the sky: Due to Rayleigh scattering of sunlight by air molecules. Blue light is scattered much more than other colours, so the sky appears blue from scattered sunlight. Our eyes are more sensitive to blue than violet.
- Reddish appearance of Sun/Moon at sunrise/sunset: Sun's rays travel through a larger distance of atmosphere. Most of the shorter wavelengths (blue, violet) are scattered away. The light that reaches the observer is richer in longer wavelengths (red, orange), making the Sun appear reddish.
For larger particles (dust, water droplets in clouds) where particle size is comparable to or larger than wavelength ($a \approx \lambda$ or $a \gg \lambda$), scattering is less dependent on wavelength; all colours are scattered nearly equally. This is why clouds appear white.
Intext Question 9.7. Find the position of the image formed by the lens combination given in the Fig. 9.22.
Answer:
This refers to Example 9.9, which was already worked through. The final image is formed 30 cm to the right of the third lens.
Optical Instruments
Optical instruments are devices that use mirrors, lenses, and prisms to manipulate light for viewing objects, forming images, or analysing light properties. Examples include microscopes and telescopes.
The Microscope
Microscopes provide magnified images of small objects.
- Simple Microscope: A converging lens of small focal length used as a magnifier. The object is placed within one focal length of the lens. It forms a virtual, erect, and magnified image. For comfortable viewing, the image is usually formed at the near point (distance of distinct vision, $D \approx 25$ cm) or at infinity.
- Magnification when image is at the near point: $\mathbf{m = 1 + \frac{D}{f}}$.
- Magnification when image is at infinity: This is angular magnification, defined as the ratio of the angle subtended by the image at the eye to the angle subtended by the object if placed at the near point $D$. $\mathbf{m = \frac{D}{f}}$. Viewing at infinity is less tiring for the eye.
- Compound Microscope: Used for much higher magnifications. Uses two lenses: an **objective lens** (near the object, small focal length, forms a real, inverted, magnified intermediate image) and an **eyepiece** (functions like a simple microscope, magnifies the intermediate image to form the final virtual, enlarged, and inverted image). The intermediate image is placed near the focal plane of the eyepiece.
- Total magnification is the product of the linear magnification by the objective ($m_o$) and the angular magnification by the eyepiece ($m_e$). $m = m_o \times m_e$.
- Linear magnification of the objective: $m_o = L/f_o$, where $L$ is the distance between the objective and the intermediate image (approximately the tube length) and $f_o$ is the objective focal length.
- Angular magnification of the eyepiece: $m_e = 1 + D/f_e$ (image at near point) or $m_e = D/f_e$ (image at infinity), where $f_e$ is the eyepiece focal length.
Total magnification (image at infinity): $\mathbf{m = \frac{L}{f_o} \frac{D}{f_e}}$. High magnification requires small focal lengths for both objective and eyepiece and a large tube length $L$. Modern microscopes use complex lenses to reduce aberrations.
Telescope
Telescopes provide **angular magnification** of distant objects. Like microscopes, they have an objective and an eyepiece, but the objective has a large focal length and a much larger aperture (for better light gathering power and resolution).
- Refracting Telescope: Uses a lens as the objective. Light from a distant object forms a real, inverted image at the objective's focal point. The eyepiece magnifies this image.
- Magnifying power: $\mathbf{m = \frac{\beta}{\alpha} = \frac{f_o}{f_e}}$, where $f_o$ is the objective focal length and $f_e$ is the eyepiece focal length. $\alpha$ and $\beta$ are angles subtended by object and image.
- For normal adjustment (final image at infinity), separation between objective and eyepiece is $f_o + f_e$.
Large objective diameters are desirable for light gathering power and resolution. However, large lenses are difficult and expensive to make free from aberrations.
- Reflecting Telescope: Uses a concave mirror as the objective. Avoids chromatic aberration. Mirrors are easier to support than large lenses. Light is typically reflected by a secondary mirror to an accessible eyepiece location (e.g., Cassegrain design). Modern large telescopes are reflecting telescopes.
Intext Question 9.8. Find the position of the image formed by the lens combination given in the Fig. 9.22.
Answer:
This refers to Example 9.9 which was worked through already. The final image is formed 30 cm to the right of the third lens.
Summary
This chapter covers the principles of ray optics, focusing on reflection, refraction, dispersion, and their application in optical instruments.
- Ray optics treats light as traveling in straight lines (rays), applicable when wavelength is small compared to object size.
- Reflection: Governed by laws of reflection ($\angle i = \angle r'$, incident/reflected/normal in plane). For spherical mirrors: $\frac{1}{v} + \frac{1}{u} = \frac{1}{f}$ (mirror equation), $f=R/2$. Magnification $m = h'/h = -v/u$. Cartesian sign convention used.
- Refraction: Bending of light at interface. Governed by Snell's law ($n_1 \sin i = n_2 \sin r$). Refractive index $n_{21}=n_2/n_1=v_1/v_2$. Apparent depth, atmospheric refraction are effects of refraction.
- Total Internal Reflection (TIR): Occurs when light goes from denser to rarer medium at angle $i > i_c$ where $\sin i_c = n_{rarer}/n_{denser}$. Applications: mirage, diamond sparkle, reflecting prisms, optical fibres.
- Refraction at spherical surfaces: $\frac{n_2}{v} - \frac{n_1}{u} = \frac{n_2 - n_1}{R}$.
- Lenses: Thin lens formula $\frac{1}{v} - \frac{1}{u} = \frac{1}{f}$. Lens maker's formula $\frac{1}{f} = (\frac{n_2}{n_1} - 1) (\frac{1}{R_1} - \frac{1}{R_2})$. Power $P=1/f$ (in Dioptres, D). Magnification $m = v/u$.
- Combination of thin lenses in contact: $\frac{1}{f} = \frac{1}{f_1} + \frac{1}{f_2} + ...$, $P = P_1 + P_2 + ...$.
- Prism: Refraction causes deviation $\delta = i + e - A$. Minimum deviation $D_m$ occurs at $i=e$, $r_1=r_2=A/2$. $n_2 = \frac{\sin((A+D_m)/2)}{\sin(A/2)}$.
- Dispersion: Splitting of white light into colours by prism/lens due to different refractive indices for different wavelengths.
- Natural phenomena: Rainbow (dispersion + refraction + TIR in raindrops), scattering of light (blue sky, red sunset).
- Optical Instruments: Simple microscope (magnifier, $m = 1+D/f$ or $D/f$), Compound microscope ($m = m_o m_e$, $m_o=L/f_o$, $m_e=D/f_e$ or $1+D/f_e$). Telescope (angular mag, $m = f_o/f_e$). Reflecting telescopes use mirrors as objectives.
Exercises
Questions covering calculations and concepts related to reflection by spherical mirrors (image position, nature, magnification), refraction at plane and spherical surfaces, total internal reflection, prisms (deviation, refractive index), lenses (image formation, lens maker's formula, power, combinations), scattering, rainbows, simple and compound microscopes, and refracting and reflecting telescopes. Includes problems requiring ray diagrams and application of sign conventions and formulas.
Exercises
Question 9.1. A small candle, 2.5 cm in size is placed at 27 cm in front of a concave mirror of radius of curvature 36 cm. At what distance from the mirror should a screen be placed in order to obtain a sharp image? Describe the nature and size of the image. If the candle is moved closer to the mirror, how would the screen have to be moved?
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Question 9.2. A 4.5 cm needle is placed 12 cm away from a convex mirror of focal length 15 cm. Give the location of the image and the magnification. Describe what happens as the needle is moved farther from the mirror.
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Question 9.3. A tank is filled with water to a height of 12.5 cm. The apparent depth of a needle lying at the bottom of the tank is measured by a microscope to be 9.4 cm. What is the refractive index of water? If water is replaced by a liquid of refractive index 1.63 up to the same height, by what distance would the microscope have to be moved to focus on the needle again?
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Question 9.4. Figures 9.31(a) and (b) show refraction of a ray in air incident at 60° with the normal to a glass-air and water-air interface, respectively. Predict the angle of refraction in glass when the angle of incidence in water is 45° with the normal to a water-glass interface [Fig. 9.31(c)].
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Question 9.5. A small bulb is placed at the bottom of a tank containing water to a depth of 80cm. What is the area of the surface of water through which light from the bulb can emerge out? Refractive index of water is 1.33. (Consider the bulb to be a point source.)
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Question 9.6. A prism is made of glass of unknown refractive index. A parallel beam of light is incident on a face of the prism. The angle of minimum deviation is measured to be 40°. What is the refractive index of the material of the prism? The refracting angle of the prism is 60°. If the prism is placed in water (refractive index 1.33), predict the new angle of minimum deviation of a parallel beam of light.
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Question 9.7. Double-convex lenses are to be manufactured from a glass of refractive index 1.55, with both faces of the same radius of curvature. What is the radius of curvature required if the focal length is to be 20cm?
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Question 9.8. A beam of light converges at a point P. Now a lens is placed in the path of the convergent beam 12cm from P. At what point does the beam converge if the lens is (a) a convex lens of focal length 20cm, and (b) a concave lens of focal length 16cm?
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Question 9.9. An object of size 3.0cm is placed 14cm in front of a concave lens of focal length 21cm. Describe the image produced by the lens. What happens if the object is moved further away from the lens?
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Question 9.10. What is the focal length of a convex lens of focal length 30cm in contact with a concave lens of focal length 20cm? Is the system a converging or a diverging lens? Ignore thickness of the lenses.
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Question 9.11. A compound microscope consists of an objective lens of focal length 2.0cm and an eyepiece of focal length 6.25cm separated by a distance of 15cm. How far from the objective should an object be placed in order to obtain the final image at (a) the least distance of distinct vision (25cm), and (b) at infinity? What is the magnifying power of the microscope in each case?
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Question 9.12. A person with a normal near point (25cm) using a compound microscope with objective of focal length 8.0 mm and an eyepiece of focal length 2.5cm can bring an object placed at 9.0mm from the objective in sharp focus. What is the separation between the two lenses? Calculate the magnifying power of the microscope,
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Question 9.13. A small telescope has an objective lens of focal length 144cm and an eyepiece of focal length 6.0cm. What is the magnifying power of the telescope? What is the separation between the objective and the eyepiece?
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Question 9.14. (a) A giant refracting telescope at an observatory has an objective lens of focal length 15m. If an eyepiece of focal length 1.0cm is used, what is the angular magnification of the telescope?
(b) If this telescope is used to view the moon, what is the diameter of the image of the moon formed by the objective lens? The diameter of the moon is $3.48 \times 10^6$m, and the radius of lunar orbit is $3.8 \times 10^8$m.
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Question 9.15. Use the mirror equation to deduce that:
(a) an object placed between f and 2f of a concave mirror produces a real image beyond 2f.
(b) a convex mirror always produces a virtual image independent of the location of the object.
(c) the virtual image produced by a convex mirror is always diminished in size and is located between the focus and the pole.
(d) an object placed between the pole and focus of a concave mirror produces a virtual and enlarged image.
[Note: This exercise helps you deduce algebraically properties of images that one obtains from explicit ray diagrams.]
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Question 9.16. A small pin fixed on a table top is viewed from above from a distance of 50cm. By what distance would the pin appear to be raised if it is viewed from the same point through a 15cm thick glass slab held parallel to the table? Refractive index of glass = 1.5. Does the answer depend on the location of the slab?
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Question 9.17. (a) Figure 9.32 shows a cross-section of a ‘light pipe’ made of a glass fibre of refractive index 1.68. The outer covering of the pipe is made of a material of refractive index 1.44. What is the range of the angles of the incident rays with the axis of the pipe for which total reflections inside the pipe take place, as shown in the figure.
(b) What is the answer if there is no outer covering of the pipe?
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Question 9.18. Answer the following questions:
(a) You have learnt that plane and convex mirrors produce virtual images of objects. Can they produce real images under some circumstances? Explain.
(b) A virtual image, we always say, cannot be caught on a screen. Yet when we ‘see’ a virtual image, we are obviously bringing it on to the ‘screen’ (i.e., the retina) of our eye. Is there a contradiction?
(c) A diver under water, looks obliquely at a fisherman standing on the bank of a lake. Would the fisherman look taller or shorter to the diver than what he actually is?
(d) Does the apparent depth of a tank of water change if viewed obliquely? If so, does the apparent depth increase or decrease?
(e) The refractive index of diamond is much greater than that of ordinary glass. Is this fact of some use to a diamond cutter?
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Question 9.19. The image of a small electric bulb fixed on the wall of a room is to be obtained on the opposite wall 3m away by means of a large convex lens. What is the maximum possible focal length of the lens required for the purpose?
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Question 9.20. A screen is placed 90cm from an object. The image of the object on the screen is formed by a convex lens at two different locations separated by 20cm. Determine the focal length of the lens.
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Question 9.21. (a) Determine the ‘effective focal length’ of the combination of the two lenses in Exercise 9.10, if they are placed 8.0cm apart with their principal axes coincident. Does the answer depend on which side of the combination a beam of parallel light is incident? Is the notion of effective focal length of this system useful at all?
(b) An object 1.5 cm in size is placed on the side of the convex lens in the arrangement (a) above. The distance between the object and the convex lens is 40cm. Determine the magnification produced by the two-lens system, and the size of the image.
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Question 9.22. At what angle should a ray of light be incident on the face of a prism of refracting angle 60° so that it just suffers total internal reflection at the other face? The refractive index of the material of the prism is 1.524.
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Question 9.23. A card sheet divided into squares each of size 1 mm$^2$ is being viewed at a distance of 9 cm through a magnifying glass (a converging lens of focal length 9 cm) held close to the eye.
(a) What is the magnification produced by the lens? How much is the area of each square in the virtual image?
(b) What is the angular magnification (magnifying power) of the lens?
(c) Is the magnification in (a) equal to the magnifying power in (b)? Explain.
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Question 9.24. (a) At what distance should the lens be held from the figure in Exercise 9.29 in order to view the squares distinctly with the maximum possible magnifying power?
(b) What is the magnification in this case?
(c) Is the magnification equal to the magnifying power in this case? Explain.
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Question 9.25. What should be the distance between the object in Exercise 9.24 and the magnifying glass if the virtual image of each square in the figure is to have an area of 6.25 mm$^2$. Would you be able to see the squares distinctly with your eyes very close to the magnifier?
[Note: Exercises 9.23 to 9.25 will help you clearly understand the difference between magnification in absolute size and the angular magnification (or magnifying power) of an instrument.]
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Question 9.26. Answer the following questions:
(a) The angle subtended at the eye by an object is equal to the angle subtended at the eye by the virtual image produced by a magnifying glass. In what sense then does a magnifying glass provide angular magnification?
(b) In viewing through a magnifying glass, one usually positions one’s eyes very close to the lens. Does angular magnification change if the eye is moved back?
(c) Magnifying power of a simple microscope is inversely proportional to the focal length of the lens. What then stops us from using a convex lens of smaller and smaller focal length and achieving greater and greater magnifying power?
(d) Why must both the objective and the eyepiece of a compound microscope have short focal lengths?
(e) When viewing through a compound microscope, our eyes should be positioned not on the eyepiece but a short distance away from it for best viewing. Why? How much should be that short distance between the eye and eyepiece?
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Question 9.27. An angular magnification (magnifying power) of 30X is desired using an objective of focal length 1.25cm and an eyepiece of focal length 5cm. How will you set up the compound microscope?
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Question 9.28. A small telescope has an objective lens of focal length 140cm and an eyepiece of focal length 5.0cm. What is the magnifying power of the telescope for viewing distant objects when
(a) the telescope is in normal adjustment (i.e., when the final image is at infinity)?
(b) the final image is formed at the least distance of distinct vision (25cm)?
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Question 9.29. (a) For the telescope described in Exercise 9.28 (a), what is the separation between the objective lens and the eyepiece?
(b) If this telescope is used to view a 100 m tall tower 3 km away, what is the height of the image of the tower formed by the objective lens?
(c) What is the height of the final image of the tower if it is formed at 25cm?
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Question 9.30. A Cassegrain telescope uses two mirrors as shown in Fig. 9.30. Such a telescope is built with the mirrors 20mm apart. If the radius of curvature of the large mirror is 220mm and the small mirror is 140mm, where will the final image of an object at infinity be?
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Question 9.31. Light incident normally on a plane mirror attached to a galvanometer coil retraces backwards as shown in Fig. 9.33. A current in the coil produces a deflection of 3.5° of the mirror. What is the displacement of the reflected spot of light on a screen placed 1.5 m away?
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Question 9.32. Figure 9.34 shows an equiconvex lens (of refractive index 1.50) in contact with a liquid layer on top of a plane mirror. A small needle with its tip on the principal axis is moved along the axis until its inverted image is found at the position of the needle. The distance of the needle from the lens is measured to be 45.0cm. The liquid is removed and the experiment is repeated. The new distance is measured to be 30.0cm. What is the refractive index of the liquid?
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