Commonly Used Terms in Spherical Mirrors

Aperture 

The part of a spherical mirror that is exposed to all the light rays that incident on it is called the aperture of the spherical mirror. In other words, the diameter (XY) of the aperture of the concave mirrors and convex mirror is shown in the figure, known as its aperture

Centre of Curvature

The center of a hollow sphere of which the curved or spherical mirror forms a part is called the center of curvature. It is denoted by C (as shown in the Figure). 

Radius of curvature

The radius of a hollow sphere of which the spherical mirror forms a part is called the radius of curvature. It is denoted by R. 

Pole 

The center of the spherical surface is called its pole. It is denoted by P

Principal Axis

The line joining the center of curvature (C) and pole (P) of a spherical mirror and extended on either side is called the principal axis

Principal Focus

A point on the principal axis of a spherical mirror where the rays of light parallel to the principal axis meet or appear to meet after reflection from the spherical mirror is called the principal focus. It is denoted by F. 

  • In the case of a concave mirror, the rays of light parallel to the principal axis after reflection actually meet the principal axis at F as shown in figure 2. So, the principal focus of a concave mirror is real.
  • In the case of a convex mirror, the rays of light parallel to the principal axis after reflection appear to meet or diverge from the principal axis at F as shown in figure 3. So, the principal focus of a convex mirror is virtual.

Focal Plane

A plane normal or perpendicular to the principal axis and passing through the principal focus (F) of a spherical mirror is called the focal plane of the spherical mirror.

Focal Length 

The distance between the pole (P) and principal focus (f) of a spherical mirror is called the focal length of the mirror. It is denoted by f. As shown in the figure above, the focal length of the mirror is represented by PF.

Sign Convention for Spherical Mirrors

Sign Convention for Spherical Mirrors: While studying the reflection of light by spherical mirrors and the formation of images by spherical mirrors, a set of sign conventions are needed to learn that is required to measure the focal length, the distance of the object or image from the mirror, and the magnification of the mirror.

Before, understanding the concept of sign conventions for spherical mirrors first discuss some commonly used terms in a spherical mirror.

Table of Content

  • Commonly Used Terms in Spherical Mirrors
  • Sign Convention for Spherical Mirrors
  • Important Points to Remember
  • Mirror Formula 
  • Magnification (or Linear magnification)
  • Solved Examples on Sign Conventions for Spherical Mirrors

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Commonly Used Terms in Spherical Mirrors

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Sign Convention for Spherical Mirrors

The set of guidelines to set signs for image distance, object distance, focal length, etc for mathematical calculation during an image formation is called the Sign Convention. The sign conventions in the case of the spherical mirrors are made in taking into consideration that the objects are always placed on the left side of the mirror, such that the direction of incident light is from left to right....

Important Points to Remember

According to the sign convention, the distances towards the left of the mirror are negative. Since an object is always placed to the left side of a mirror, therefore, the object distance (u) is always negative. The images formed by a concave mirror can be either behind the mirror (virtual) or in front of the mirror (real). So, the image distance (v) for a concave mirror can be either positive or negative depending on the position of the image. If the image is formed behind a concave mirror, the image distance (v) is positive but if the image is formed in front of the mirror, then the image distance will be negative. In a convex mirror, the image is always formed on the right-hand side (behind the mirror), so the image distance (o) for a convex mirror will be always positive. The focus of a concave mirror is in front of the mirror on the left side, so the focal length of a concave mirror will be negative (and written with a minus sign, say, -10 cm). On the other hand, the focus of the convex mirror is behind the mirror on the right side, so the focal length (and written with a plus sign, say +20 cm or just 20 cm), of a convex mirror is positive. The Focal Length and radius of curvature of a concave mirror are taken negatively. The Focal Length and radius of curvature of a convex mirror are taken positively....

Mirror Formula

The distance of the position of an object on the principal axis from the pole of a spherical mirror is known as object distance. It is denoted by u. The distance of the position of the image of an object on the principal axis from the pole of a spherical mirror is known as the image distance. It is denoted by v....

Magnification (or Linear magnification)

Linear Magnification produced by a mirror is defined as the ratio of the size (or height) of the image to the size (or height) of the object. It is denoted by m. If h’ is the size (or height) of the image produced by the mirror and h is the size (or height) of the object....

Solved Examples on Sign Conventions for Spherical Mirrors

Example 1: A concave mirror produces two times magnified real image of an object placed 10 cm in front of it. Find the position of the image....

Sign Conventions for Spherical Mirrors – FAQs

What is the function of a Convex Mirror?...