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Spherical Mirrors

Spherical Mirrors

Edited By Vishal kumar | Updated on Jul 02, 2025 07:56 PM IST

Imagine looking into a shiny, curved spoon. The curved surface creates a fascinating reflection that either enlarges or shrinks your image, depending on which side you are viewing. This is similar to how spherical mirrors work. Spherical mirrors are mirrors with curved surfaces that can either converge or diverge light. There are two types of spherical mirrors: concave and convex.

This Story also Contains
  1. Spherical Mirror
  2. Solved Examples Based on Spherical Mirrors
  3. Summary
Spherical Mirrors
Spherical Mirrors

Concave mirrors, like the inside of a spoon, curve inward. They can focus light to a single point, making them useful in applications like telescopes, shaving mirrors, and headlights, where focused light or magnified images are required. Convex mirrors, like the back of a spoon, curve outward. They spread out light rays, providing a wider field of view, making them ideal for use in vehicle side mirrors and security mirrors in stores.

In this article, we are going to learn about spherical mirrors, some important technology and solved example on this concept of chapter optics.

Spherical Mirror

It is a part of a transparent hollow sphere whose surface is polished.

There are two types of spherical mirrors: concave, and convex.

In the above figure, A concave (left) and a convex (right) mirror is shown.

Some Important Terminology

  • Centre of curvature (C)- The Centre of the sphere of which the mirror is a part is called the Centre of curvature.
  • Pole (P)- The geometrical centre of the spherical reflecting surface.
  • The radius of curvature (R)- The radius of the sphere of which the mirror is a part is called the radius of curvature.

or R= Distance between pole and centre of curvature

$\left(\right.$ Note $\left.\Rightarrow R_{\text {concave }}=-v e, \quad R_{\text {convex }}=+v e, R_{\text {plane }}=\infty\right)$

  • Principle axis- A line passing through P and C is known as the Principle axis.
  • Focus (F)- When a narrow beam of rays of light, parallel to the principal axis and close to it, is incident on the surface of a mirror, the reflected beam is found to coverage to or appears to diverge from a point on the principal axis. This point is called the focus.
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or An image point on the principal axis for which the object is at $\infty$ is called the focus.

C, P, and F for a concave mirror are shown in the below figure.

  • Focal Length (f)- It is the distance between the pole and the principal focus. For spherical mirrors, $f=\frac{R}{2}$

(i.e $\left.f_{\text {concarr }}=-v e, f_{\text {convex }}=+v e, f_{\text {plane }}=\infty\right)$

  • Focal plane- A plane passing from focus and perpendicular to the principal axis.

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Solved Examples Based on Spherical Mirrors

Example 1: A hemispherical glass body of radius 10 cm and refractive index 1.5 is silvered on its curved surface. A small air bubble is 6 cm below the flat surface inside it along the axis. The position of the image of the air bubble made by the mirror is seen :

1) 14 cm below the flat surface

2) 30 cm below the flat surface

3) 20 cm below the flat surface

4) 16 cm below the flat surface

Solution:

Relation between focal length and radius of curvature

$f=\frac{R}{2}$

wherein

R = Radius of curvature

This is valid only for smaller angles of incidence.

i.e.paraxial rays

Mirror Formula

$\frac{1}{v}+\frac{1}{u}=\frac{1}{f}$

wherein

$u=$ Object distance from pole of mirror.
$v=$ Image distance from pole of mirror.
$f=$ focal length of the mirror.

Relation between real depth and apparent depth -

$
\frac{n_i}{d}=\frac{n_r}{d^{\prime}}
$
wherein
$n_i=$ Refractive index of the medium of the incident.
$n_\tau=$ Refractive index of the medium of refraction.
$d=$ distance of the object.
$d^{\prime}=$ apparent depth
Given the radius of hemispherical glass $\mathrm{R}=10 \mathrm{~cm}$
$
\begin{aligned}
& \therefore \text { focal length } f=\frac{10}{2}=-5 \mathrm{~cm} \\
& u=(10-6)=-4 \mathrm{~cm}
\end{aligned}
$

By using the mirror formula
$
\frac{1}{v}+\frac{1}{u}=\frac{1}{f}=\frac{1}{v}+\frac{1}{-4}=\frac{1}{-5} \Rightarrow v=20 \mathrm{~cm}
$

Apparent height
$
h_a=h_r \frac{\mu_1}{\mu_2}=30 \times \frac{1}{1.5}=20 \mathrm{~cm}
$

below the flat surface.

Hence, the answer is option (3).

Example 2: You are asked to design a shaving mirror assuming that a person keeps it 10 cm from his face and views the magnified image of the face at the closest comfortable distance of 25 cm. The radius of curvature of the mirror would then be :

1) 30 cm

2) 24 cm

3) 60 cm

4) 28 cm

Solution:

From question v = 15 cm, u = -10 cm

The radius of curvature R = 2f

Mirror formula $\frac{1}{v}+\frac{1}{u}=\frac{1}{f}=\frac{1}{15}+\frac{1}{(-10)}=\frac{1}{f}$

f = - 30 cm

$\therefore$ R= 2(-30) = - 60 cm

Hence, the answer is option (3).

Example 3: The geometrical centre of the spherical reflecting surface is called -

1) Centre of curvature

2) Pole

3) Principal focus

4) Geometrical focus

Solution:

Pole (P)- The geometrical centre of the spherical reflecting surface.

Represented by 'P' here

Hence, the answer is option (2).

Example 4: What will be the length of the focal point from the pole (cm), if the radius of curvature of the spherical mirror is 28 cm?

1) 56

2) 14

3) 42

4) 7

Solution:

Focal Length (f)- It is the distance between the pole and the principal focus. For spherical mirrors, $f=\frac{R}{2}$

So,

$f=\frac{28}{2}=14 \mathrm{~cm}$

Hence, the answer is the option (2).

Example 5: The focal length f is related to the radius of the curvature r of the spherical convex mirror by:

1) $f=+\frac{1}{2} r$
2) $f=-\frac{1}{2} r$
3) $f=r$
4) $f=-r$

Solution:

In the case of spherical mirrors, there are some sign conventions that we need to consider:-

1. All distances are measured from the pole of the mirror.

2. Distances measured in the direction of the incident ray are positive and the distances measured in the direction opposite to that of the incident rays are negative.

For a convex mirror, the focus is behind the mirror and is taken to positive which is in the direction of the incident ray.

$\therefore f=+\frac{r}{2}$

Hence, the answer is option (1).

Summary

Spherical mirrors are mirrors that are curvy in shape and include two types:i.e., concave and convex. Mirrors that cave inwards are referred to as concave mirrors. Based on an object’s position vis a vis the focal point of the mirror, light can be focused by these. Therefore it could be either a real or virtual image they form. Telescopes make use of them, as well as Headlights, and shaving mirrors just to mention a few examples. Contrarily, on the other hand, mirrors that bulge outwards are convex mirrors like those found on rear-view cars.

Frequently Asked Questions (FAQs)

1. Why is the focal length of a convex mirror considered negative?
The focal length of a convex mirror is considered negative due to the sign convention used in optics. In this convention:
2. How can you determine whether an image formed by a spherical mirror is real or virtual without seeing it?
You can determine if an image is real or virtual by analyzing where the reflected light rays meet:
3. How does the magnification of an image relate to the object and image distances in a spherical mirror?
The magnification (m) of an image in a spherical mirror is related to the object distance (u) and image distance (v) by the equation: m = -v/u. The negative sign indicates that if the image is upright relative to the object, the magnification is positive, and if inverted, it's negative. This relationship shows that as the image distance increases relative to the object distance, the magnification increases in magnitude.
4. What is a spherical mirror?
A spherical mirror is a curved reflective surface that forms part of a sphere. It can be either concave (curved inward) or convex (curved outward). These mirrors reflect light in specific ways based on their curvature, making them useful in various optical applications.
5. How does the curvature of a spherical mirror affect its focal length?
The curvature of a spherical mirror is directly related to its focal length. A more curved mirror (smaller radius of curvature) will have a shorter focal length, while a less curved mirror (larger radius of curvature) will have a longer focal length. This relationship is described by the formula: f = R/2, where f is the focal length and R is the radius of curvature.
6. What's the difference between real and virtual images formed by spherical mirrors?
Real images are formed when light rays actually converge at a point, and can be projected on a screen. Virtual images are formed when light rays appear to diverge from a point, but don't actually meet there. They cannot be projected on a screen. Concave mirrors can form both real and virtual images, while convex mirrors only form virtual images.
7. Why do convex mirrors always produce virtual, upright, and diminished images?
Convex mirrors always produce virtual, upright, and diminished images because the reflected rays diverge after reflection, never converging to form a real image. The diverging rays appear to come from a point behind the mirror, creating a virtual image that is always upright and smaller than the object.
8. How does the position of an object relative to the focal point of a concave mirror affect the image formed?
The image formed by a concave mirror depends on the object's position relative to the focal point:
9. What is the significance of the center of curvature in a spherical mirror?
The center of curvature is the center of the sphere of which the mirror forms a part. It's significant because any incident ray passing through this point will be reflected back along the same path. This property is useful in understanding the behavior of light rays and in constructing ray diagrams for spherical mirrors.
10. How does the mirror equation relate object distance, image distance, and focal length?
The mirror equation relates object distance (u), image distance (v), and focal length (f) of a spherical mirror: 1/f = 1/u + 1/v. This equation allows us to calculate any one of these quantities if the other two are known, making it a fundamental tool in analyzing spherical mirror systems.
11. What is meant by the 'sign convention' in spherical mirrors, and why is it important?
The sign convention in spherical mirrors assigns positive or negative values to distances and heights based on their direction relative to the mirror. For example, object distances are usually considered positive, while image distances are positive for real images and negative for virtual images. This convention is crucial for consistently solving mirror problems and interpreting results correctly.
12. How does a concave mirror form a magnified image of an object?
A concave mirror forms a magnified image when the object is placed between the focal point and the mirror surface. In this case, the reflected rays diverge, creating a virtual, upright image that appears larger than the object. This principle is used in applications like makeup mirrors.
13. Why are spherical mirrors preferred over plane mirrors in many optical instruments?
Spherical mirrors are preferred in many optical instruments because they can converge or diverge light rays, allowing for the formation of real or virtual images with different sizes and orientations. This versatility makes them useful for magnification, focusing light, and creating specific image characteristics that plane mirrors cannot achieve.
14. What is spherical aberration, and how does it affect image quality in spherical mirrors?
Spherical aberration is an optical defect where light rays reflecting from different parts of a spherical mirror don't converge to a single focal point. This occurs because the mirror's curvature isn't perfectly parabolic. It results in a slightly blurred or distorted image, especially for objects far from the mirror's axis. This effect is more pronounced in mirrors with a large aperture relative to their focal length.
15. How does the radius of curvature of a spherical mirror relate to its focal length?
The focal length (f) of a spherical mirror is exactly half of its radius of curvature (R). This relationship is expressed as f = R/2. Understanding this connection is crucial for predicting mirror behavior and designing optical systems. It means that a mirror with a smaller radius of curvature will have a shorter focal length, concentrating light more quickly.
16. Why do concave mirrors form inverted images for distant objects?
Concave mirrors form inverted images for distant objects because these objects are beyond the center of curvature. Light rays from the top of the object reflect off the mirror and converge below the principal axis, while rays from the bottom converge above it. This crossing of rays creates a real, inverted image. The inversion occurs because the mirror changes the direction of light propagation.
17. What is the difference between the focal point and the center of curvature in a spherical mirror?
The focal point and center of curvature are distinct points in a spherical mirror:
18. How does changing the object distance affect the nature of the image formed by a concave mirror?
Changing the object distance affects the image formed by a concave mirror as follows:
19. Why do convex mirrors always produce a smaller image than the object?
Convex mirrors always produce a smaller image because they diverge light rays. When light reflects off a convex surface, it spreads out, making the virtual image appear farther away and smaller than the object. This property is consistent regardless of the object's distance from the mirror, making convex mirrors useful for creating wide-angle views in applications like side-view mirrors on vehicles.
20. What is the significance of the principal axis in a spherical mirror system?
The principal axis is an imaginary line passing through the center of curvature and the center of the mirror surface. It's significant because:
21. How do spherical mirrors differ from parabolic mirrors in terms of image formation?
Spherical and parabolic mirrors differ in image formation:
22. How does the radius of curvature affect the field of view of a spherical mirror?
The radius of curvature of a spherical mirror directly affects its field of view:
23. What is the relationship between the focal length and the power of a spherical mirror?
The power (P) of a spherical mirror is the reciprocal of its focal length (f) measured in meters: P = 1/f. Power is measured in diopters (D). This relationship means:
24. How does the image formed by a spherical mirror change as an object moves towards it?
As an object moves towards a spherical mirror, the image changes as follows:
25. Why do concave mirrors form real images in some cases and virtual images in others?
Concave mirrors form real or virtual images depending on the object's position relative to the focal point:
26. How does the curvature of a spherical mirror affect its ability to collect light?
The curvature of a spherical mirror significantly affects its light-collecting ability:
27. What is the difference between longitudinal and lateral magnification in spherical mirrors?
Longitudinal and lateral magnification in spherical mirrors are different concepts:
28. How does the f-number of a spherical mirror relate to its light-gathering ability?
The f-number (f/#) of a spherical mirror is the ratio of its focal length to its diameter. It relates to light-gathering ability as follows:
29. Why do spherical mirrors produce distorted images for objects far from the principal axis?
Spherical mirrors produce distorted images for objects far from the principal axis due to spherical aberration. This occurs because:
30. How does the concept of caustics relate to spherical mirrors?
Caustics in spherical mirrors refer to the envelope of light rays reflected or refracted by a curved surface. In spherical mirrors:
31. What is the difference between the focal length of a spherical mirror and its focal plane?
The focal length and focal plane of a spherical mirror are related but distinct concepts:
32. How does the concept of optical leverage apply to spherical mirrors?
Optical leverage in spherical mirrors refers to the relationship between small changes in object position and resulting changes in image position. It's characterized by:
33. Why do concave mirrors used in telescopes need to be precisely shaped?
Concave mirrors in telescopes need precise shaping because:
34. How does the thickness of a spherical mirror affect its optical properties?
The thickness of a spherical mirror primarily affects its mechanical properties rather than its optical ones. However, it can indirectly influence optical performance:

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