LIGHT
Types of Mirrors
Spherical
mirrors
Spherical
mirrors are one form of curved mirrors. If the curved mirror is a part of a
sphere, then it is called a ‘spherical mirror’. It resembles the shape of a piece
cut out from a spherical surface. One side of this mirror is silvered and the
reflection of light occurs at the other side.
Concave mirrors
A
spherical mirror, in which the reflection of light occurs at its concave surface,
is called a concave mirror. These
mirrors magnify the object placed
close to them. The most
common example of a concave mirror is the make-up mirror.
Convex mirror
A
spherical mirror, in which the reflection of light occurs at its convex
surface, is called a convex mirror. The
image formed by these mirrors is smaller than the object. Most common
convex mirrors are rear viewing mirrors used in vehicles.
Convex mirrors used in vehicles
as rear-view mirrors are labeled with the safety warning: ‘Objects in the
mirror are closer than they appear’ to warn the drivers. This is because inside
the mirrors, vehicles will appear to be coming at a long distance.
Parabolic mirrors
A parabolic mirror is one type of curved
mirror, which is in the shape of a parabola. It has a concave reflecting
surface and this surface directs the entire incident beam of light to converge
at its focal point.
In the same way,
light rays generated by the source placed at this focal point will fall on this
surface and they will be diverged in a direction, which is parallel to the
principal axis of the parabolic mirror. Hence, the light rays will be reflected
to travel a long distance, without getting diminished.
Parabolic
mirrors, also known as parabolic reflectors, are used to collect or project
energy such as light, heat, sound and radio waves. They are used in reflecting
telescopes, radio telescopes and parabolic microphones. They are also used in
solar cookers and solar water heaters.
Terms related to spherical mirrors
Center of Curvature:
It is the center
of the sphere from which the mirror is made. It is denoted by the letter C in the ray diagrams. (A ray diagram
represents the formation of an image by the spherical mirror. You will study
about them in your next class).
Pole:
It
is the geometric center of the spherical mirror. It is denoted by the letter P.
Radius
of Curvature:
It is the distance between the
center of the sphere and the vertex. It is shown by the letter R in ray diagrams. (The vertex
is the point on the mirror’s surface where the principal axis meets the
mirror. It is also called as ‘pole’.)
Principal Axis:
The line joining the
pole of the mirror and its center of curvature is called principal axis.
Focus:
When a beam of light is incident on
a spherical mirror, the reflected rays converge (concave mirror) at or appear to
diverge from (convex mirror) a point on the principal axis. This point is
called the ‘focus’ or ‘principal focus’. It is also known as the focal point.
It is denoted by the letter F in
ray diagrams.
Focal length:
The distance
between the pole and the principal focus is called focal length (f) of a
spherical mirror.
There is a
relation between the focal length of a spherical mirror and its radius of
curvature. The focal length is half of the radius of curvature.
That
is, focal length = Radius of curvature/2
Images formed by spherical mirrors
Images formed by spherical mirrors are
of two types:
i)
Real image and
ii)
Virtual image.
Real images can be formed on a screen, while
virtual images cannot be formed on a screen.
Image formed by a convex mirror is
always erect, virtual and diminished in size. As a result, images formed by
these mirrors cannot be projected on a screen.
The characteristics of an image are
determined by the location of the object. As the object gets closer to a
concave mirror, the image gets larger, until attaining approximately the size
of the object, when it reaches the Centre of curvature of the mirror. As the object
moves away, the image diminishes in size and gets gradually closer to the
focus, until it is reduced to a point at the focus when the object is at an
infinite distance from the mirror.
The size and nature of the image
formed by a convex mirror is given in Table 1.
Concave mirrors
form a real image and it can be caught on a screen. Unlike convex mirrors,
concave mirrors show different image types. Depending on the position of the
object in front of the mirror, the position, size and nature of the image will
vary. Table 2 provides a summary of images formed by a concave mirror.
Applications of curved mirrors
Concave mirrors
1.
Concave mirrors are used while applying make-up or shaving, as
they provide a magnified image.
2.
They are used in torches, search lights and head lights as they
direct the light to a long distance.
3.
They can collect the light from a larger area and focus it into a
small spot. Hence, they are used in solar cookers.
4.
They are used as head mirrors by doctors to examine the eye, ear
and throat as they provide a shadow-free illumination of the organ.
5.
They are also used in reflecting telescopes.
Convex mirrors
1.
Convex mirrors
are used in vehicles as rear view mirrors because they give an upright image
and provide a wider field of view as they are curved outwards.
2.
They are found in the hallways of various
buildings including hospitals, hotels, schools and stores. They are usually
mounted on a wall or ceiling where hallways make sharp turns.
3.
They are
also used on roads where there are sharp curves and turns.
Laws of reflection
Reflection
involves two rays:
i)
incident ray
ii)
Reflected ray. The incident ray is the light ray
in a medium falling on the shiny surface of a reflecting body. After falling on
the surface, this ray returns into the same medium. This ray is called the
reflected ray. An imaginary line perpendicular to the reflecting surface, at
the point of incidence of the light ray, is called the normal.
The relation between the incident ray, the
reflected ray and the normal is given as the law of reflection. The laws of
reflection are as follows:
1. The
incident ray, the reflected ray and the normal at the point of incidence, all
lie in the same plane.
2.
The
angle of incidence and the angle of reflection are always equal.
Types of
reflection
Regular reflection
When a beam of light (collection of parallel
rays) falls on a smooth surface, it gets reflected. After reflection, the
reflected rays will be parallel to each other. Here, the angle of incidence and
the angle of reflection of each ray will be equal. Hence, the law of reflection
is obeyed in this case and thus a clear image is formed. This reflection is
called ‘regular reflection’ or ‘specular reflection’. Example: Reflection of
light by a plane mirror and reflection of light from the surface of still
water.
Irregular reflection
In the case of a body having
a rough or irregular surface, each region of the surface is inclined at
different angles. When light falls on such a surface, the light rays are
reflected at different angles. In this case, the angle of incidence and the
angle of reflection of each ray are not equal. Hence, the law of reflection is
not obeyed in this case and thus the image is not clear. Such a reflection is
called ‘irregular reflection’ or ‘diff used reflection’. Example: Reflection of
light from a wall.
Multiple
reflections
Kaleidoscope
It is a device, which functions on the principle of multiple
reflection of light, to produce numerous patterns of images. It has two or more
mirrors inclined with each other. It can be designed from inexpensive materials
and the colorful image patterns formed by this will be pleasing to you. This
instrument is used as a toy for children.
Periscope
It is an instrument used for viewing bodies or
ships, which are over and around another body or a submarine. It is based on
the principle of the law of reflection of light. It consists of a long outer
case and inside this case mirrors or prisms are kept at each end, inclined at
an angle of 45°. Light coming from the distant body, falls on the mirror at the
top end of the periscope and gets reflected vertically downward. This light is
reflected again by the second mirror kept at the bottom, so as to travel
horizontally and reach the eye of the observer. In some complex periscopes,
optic fiber
is used instead of mirrors for obtaining a higher resolution. The distance
between the mirrors also varies depending on the purpose of using the
periscope.
Uses
1.
It is used in
warfare and navigation of the submarine.
2.
In military it
is used for pointing and firing guns from a ‘bunker’.
3.
Photographs of
important places can be taken through periscopes without trespassing restricted
military regions.
4.
Fiber optic
periscopes are used by doctors as endoscopes to view internal organs of the
body.
Refraction of
light
When light falls on a transparent material, it
is not reflected completely, but a part of it is reflected and a part of it is absorbed
and most of the light passes through it. Through air, light travels with a
speed of 3 × 108 m s-1, but it cannot travel with the same speed in water or
glass, because, optically denser medium such as water and glass offer some
resistance to the light rays. So, light rays travelling from a rarer medium
like air into a denser medium like glass or water are deviated from their
straight line path. This bending of light about the normal, at the point of
incidence; as it passes from one transparent medium to another is called
refraction of light. When a light ray travels from the rarer medium into the
denser medium, it bends towards the normal and when it travels from the denser
medium into the rarer medium, it bends away from the normal.
Refractive
Index
Refraction
of light in a medium depends on the speed of light in that medium. When the
speed of light in a medium is more, the bending is less and when the speed of
light is less, the bending is more.
The amount of refraction of light in a medium is denoted
by a term known as refractive index of the medium, which is the ratio of the
speed of light in the air to the speed of light in that particular medium. It
is also known as the absolute refractive index and it is denoted by the Greek
letter ‘μ’ (pronounced as ‘mew’).
μ
=
Refractive
index is a ratio of two similar quantities (speed) and so, it has no unit. Since,
the speed of light in any medium is less than its speed in air, refractive
index of any transparent medium is always greater than 1.
In
general, the refractive index of one medium with respect to another medium is given
by the ratio of their absolute refractive indices.
1μ2
=
1μ2
= or
1μ2
=
Thus,
the refractive index of one medium with respect to another medium is also given
by the ratio of the speed of light in first medium to its speed in the second
medium.
Snell’s Law of Refraction
Refraction of light rays, as they travel from one medium to
another medium, obeys two laws, which are known as Snell’s laws of refraction.
They are:
I) The incident ray, the refracted ray and the normal at the point
of intersection, 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 equal to the
refractive index of the medium, which is a constant.
Dispersion
Splitting of white light into its seven
constituent colors (wavelength), on passing through a transparent medium is
known as dispersion of light.
Dispersion occurs because, light of
different colors present in white light have different wavelength and they
travel at different speeds in a medium. Refraction of a light ray in a medium
depends on its speed. As each colored light has a different speed, the
constituent colored lights are refracted at different extents, inside the
Prism. Moreover, refraction of a light ray is inversely proportional to its
wavelength. Thus, the red colored
light, which has a large wavelength, is deviated less while the violet colored
light, which has a short wavelength, is deviated more.