In this article, our focus will be on the spherical mirror, its formula, sign convention, sign convention for mirror and lenses etc.
A spherical mirror is a mirror that is in the shape of a piece cut from a spherical surface.
It is of two types:-
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Convex mirror
Convex Mirror is a curved mirror, the reflective surface of which curves towards the light source (toward outside). These bulging surfaces reflect light outwards and are not used to focus light. These mirrors form a virtual image because the focal point (F) and the center of curvature (2F) are imaginary points on the mirror that cannot be reached. This results in the formation of images that cannot be projected on a screen because the image is inside the mirror. The image appears smaller than the object from a distance, but becomes larger as the object gets closer to the mirror.
Characteristics :
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Concave mirror
We know that a section of a reflective sphere is a spherical mirror. If the reflective surface is on the inward curved side, it is a concave mirror. Concave mirrors are often used as a shaving mirror or by dentists and even in telescopes. The reflected image is enlarged, but the field of view is limited. Concave mirrors are also called collective mirrors.
Characteristics:
It is an equation that relates the distance of the object and the distance of the image to the focal length and is known as the mirror equation.
In a spherical mirror:
The relation between object distance, image distance, and focal length is given as:
u be the object distance
v be the image distance
f be the focal length,
R be the spherical mirror’s radius of curvature
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What is sign convention?
The Sign Convention is a set of rules to establish signs for the distance of the image, the distance of objects, the focal length, etc.
Rules for sign convention
New cartesian sign convention/ sign convention for reflection by spherical mirror
Sign convention for concave mirror
Sign convention for convex mirror
Also Read:
Types of lenses | U | V | f | Height of the image | Height of the object |
Convex | Negative | Real image- positive Virtual image- negative | Real image- Positive No virtual focus | Real image-negative Virtual image-positive | Positive |
Concave | Negative | No real image is formed Virtual image-negative | No real focus Virtual image- Negative | No real image is formed Virtual image-positive | Positive |
Questions on spherical mirrors
1. The focal length and the object distance in case of a concave mirror are 3 cm and 6 cm respectively. Calculate the image distance.
Ans:
From the mirror formula,
Using sign convention for concave mirror,
u= object distance= 6cm
v= image distance
f= focal length of the concave mirror = 3 cm
putting the values,
Image distance of mirror is -6cm
2. The focal length and the object distance in case of a convex mirror are 6 cm and 8 cm respectively. Calculate the image distance.
Ans.
From the mirror formula,
Using sign convention for convex mirror,
u= object distance= 8cm
f= focal length of the convex mirror = 6 cm
putting the values,
Image distance of mirror is cm
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NCERT Physics Notes:
The Sign Convention is a set of rules to establish signs for the distance of the image, the distance of objects, the focal length, etc.
From the mirror the distances must be measured.
Distances measured in the direction of incidence of light must be evaluated as positive and in the opposite direction of incidence of light as negative.
Object height and image height are positive when measured from the axis up and negative when measured down.
Focal length and radius of curvature are negative for a concave mirror and positive for a convex mirror.
Magnification of concave mirror/ magnification of mirror is given by,
M=vu where v is the image distance, and u is the object distance.
The line connecting the pole and the principal focus of a mirror is called focal length of a spherical mirror.
Length of image divided by the length of the object is called lateral magnification or longitudinal magnification.
The value of angle of the image observed through the telescope divided by the angle of the same object observed in the absence of the telescope is called angular magnification.
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