Chapter 23

Mirrors and Lenses

Notation for Mirrors and Lenses

The object distance is the distance from the object to the mirror or lens

Denoted by p

The image distance is the distance from the image to the mirror or lens

Denoted by q

The lateral magnification of the mirror or lens is the ratio of the image height to the object height

Denoted by M

Types of Images for Mirrors and Lenses

A real image is one in which light actually passes through the image point

Real images can be displayed on screens

A virtual image is one in which the light does not pass through the image point

The light appears to diverge from that point

Virtual images cannot be displayed on screens

More About Images

To find where an image is formed, it is always necessary to follow at least two rays of light as they reflect from the mirror

Flat Mirror

       

Simplest possible mirror

Properties of the image can be determined by geometry

One ray starts at P, follows path PQ and reflects back on itself

A second ray follows path PR and reflects according to the Law of Reflection

Properties of the Image Formed by a Flat Mirror

The image is as far behind the mirror as the object is in front

q = p

The image is unmagnified

The image height is the same as the object height

h = h and M = 1

The image is virtual

The image is upright

It has the same orientation as the object

There is an apparent left-right reversal in the image

 

Application Day and Night Settings on Auto Mirrors

With the daytime setting, the bright beam of reflected light is directed into the drivers eyes

With the nighttime setting, the dim beam of reflected light is directed into the drivers eyes, while the bright beam goes elsewhere

Spherical Mirrors

A spherical mirror has the shape of a segment of a sphere

A concave spherical mirror has the silvered surface of the mirror on the inner, or concave, side of the curve

A convex spherical mirror has the silvered surface of the mirror on the outer, or convex, side of the curve

Concave Mirror, Notation

 

 

The mirror has a radius of curvature of R

Its center of curvature is the point C

Point V (vertex) is the center of the spherical segment

A line drawn from C to V is called the principle axis of the mirror

Image Formed by a Concave Mirror

Geometry shows the relationship between the image and object distances

 

 

This is called the mirror equation

Equivalent Equations

 

 

 

Image Formed by a Concave Mirror

Spherical Aberration

Rays are generally assumed to make small angles with the mirror

When the rays make large angles, they may converge to points other than the image point

This results in a blurred image

Focal Length

If an object is very far away, then p® ¥ and 1/p ® 0

Incoming rays are essentially parallel

In this special case, the image point is called the focal point

The distance from the mirror to the focal point is called the focal length

The focal length is ½ the radius of curvature

Focal Point and Focal Length, cont

The focal point is dependent solely on the curvature of the mirror, not by the location of the object

f = R / 2

The mirror equation can be expressed as

 

 

Focal Length Shown by Parallel Rays

Convex Mirrors

A convex mirror is sometimes called a diverging mirror

The rays from any point on the object diverge after reflection as though they were coming from some point behind the mirror

The image is virtual because it lies behind the mirror at the point where the reflected rays appear to originate

In general, the image formed by a convex mirror is upright, virtual, and smaller than the object

Image Formed by a Convex Mirror

 

Ray Diagrams

A ray diagram can be used to determine the position and size of an image

They are graphical constructions which tell the overall nature of the image

They can also be used to check the parameters calculated from the mirror and magnification equations

Drawing A Ray Diagram

To make the ray diagram, you need to know

The position of the object

The position of the center of curvature

Three rays are drawn

They all start from the same position on the object

The intersection of any two of the rays at a point locates the image

The third ray serves as a check of the construction

The Rays in a Ray Diagram

Ray 1 is drawn parallel to the principle axis and is reflected back through the focal point, F

Ray 2 is drawn through the focal point and is reflected parallel to the principle axis

Ray 3 is drawn through the center of curvature and is reflected back on itself

Notes About the Rays

The rays actually go in all directions from the object

The three rays were chosen for their ease of construction

The image point obtained by the ray diagram must agree with the value of q calculated from the mirror equation

Ray Diagram for Concave Mirror, p > R

 

 

 

 

The object is outside the center of curvature of the mirror

The image is real

The image is inverted

The image is smaller than the object

Ray Diagram for a Concave Mirror, p < f

 

 

 

 

The object is between the mirror and the focal point

The image is virtual

The image is upright

The image is larger than the object

Ray Diagram for a Convex Mirror

 

 

 

 

The object is in front of a convex mirror

The image is virtual

The image is upright

The image is smaller than the object

Notes on Images

With a concave mirror, the image may be either real or virtual

When the object is outside the focal point, the image is real

When the object is at the focal point, the image is infinitely far away

When the object is between the mirror and the focal point, the image is virtual

With a convex mirror, the image is always virtual and upright

As the object distance increases, the virtual image gets smaller

Sign Conventions for Mirrors

Quantity
Positive When
Negative When
Object location (p)
Object is in front of the mirror
Object is behind the mirror
Image location (q)
Image is in front of mirror
Image is behind mirror
Image height (h’)
Image is upright
Image is inverted
Focal length (f) and radius (R)
Mirror is concave
Mirror is convex
Magnification (M)
Image is upright
Image is inverted

 

Images Formed by Refraction

Rays originate from the object point, O, and pass through the image point, I

When n2 > n1,

 

Real images are formed on the side opposite from the object

Sign Conventions for Refracting Surfaces

Quantity
Positive When
Negative When
Object location (p)
Object is in front of surface
Object is in back of surface
Image location (q)
Image is in back of surface
Image is in front of surface
Image height (h’)
Image is upright
Image is inverted
Radius (R)
Center of curvature is in back of surface
Center of curvature is in front of surface

 Flat Refracting Surface

The image formed by a flat refracting surface is on the same side of the surface as the object

The image is virtual

The image forms between the object and the surface

The rays bend away from the normal since n1 > n2

Atmospheric Refraction

There are many interesting results of refraction in the atmosphere

Sunsets

Mirages

Atmospheric Refraction and Sunsets

Light rays from the sun are bent as they pass into the atmosphere

It is a gradual bend because the light passes through layers of the atmosphere

Each layer has a slightly different index of refraction

The Sun is seen to be above the horizon even after it has fallen below it

Atmospheric Refraction and Mirages

A mirage can be observed when the air above the ground is warmer than the air at higher elevations

The rays in path B are directed toward the ground and then bent by refraction

The observer sees both an upright and an inverted image

Thin Lenses

A thin lens consists of a piece of glass or plastic, ground so that each of its two refracting surfaces is a segment of either a sphere or a plane

Lenses are commonly used to form images by refraction in optical instruments

Thin Lens Shapes

These are examples of converging lenses

They have positive focal lengths

They are thickest in the middle

More Thin Lens Shapes

These are examples of diverging lenses

They have negative focal lengths

They are thickest at the edges

Focal Length of Lenses

The focal length, ƒ, is the image distance that corresponds to an infinite object distance

This is the same as for mirrors

A thin lens has two focal points, corresponding to parallel rays from the left and from the right

A thin lens is one in which the distance between the surface of the lens and the center of the lens is negligible

Focal Length of a Converging Lens

The parallel rays pass through the lens and converge at the focal point

The parallel rays can come from the left or right of the lens

Focal Length of a Diverging Lens

The parallel rays diverge after passing through the diverging lens

The focal point is the point where the rays appear to have originated

Lens Equations

 

The geometric derivation of the equations is very similar to that of mirrors

Lens Equations

The equations can be used for both converging and diverging lenses

A converging lens has a positive focal length

A diverging lens has a negative focal length

Sign Conventions for Thin Lenses

Quantity
Positive When
Negative When
Object location (p)
Object is in front of the lens
Object is in back of the lens
Image location (q)
Image is in back of the lens
Image is in front of the lens
Image height (h’)
Image is upright
Image is inverted
R1 and R2
Center of curvature is in back of the lens
Center of curvature is in front of the lens
Focal length (f)
Converging lens
Diverging lens

Focal Length for a Lens

The focal length of a lens is related to the curvature of its front and back surfaces and the index of refraction of the material

 

 

This is called the lens makers equation

Ray Diagrams for Thin Lenses

Ray diagrams are essential for understanding the overall image formation

Three rays are drawn

The first ray is drawn parallel to the first principle axis and then passes through (or appears to come from) one of the focal points

The second ray is drawn through the center of the lens and continues in a straight line

The third ray is drawn from the other focal point and emerges from the lens parallel to the principle axis

There are an infinite number of rays, these are convenient

Ray Diagram for Converging Lens, p > f

 

The image is real

The image is inverted

Ray Diagram for Converging Lens, p < f

The image is virtual

The image is upright

Ray Diagram for Diverging Lens

 

The image is virtual

The image is upright

Problem Solving Strategy

Be very careful about sign conventions

Do lots of problems for practice

Draw confirming ray diagrams

Combinations of Thin Lenses

The image produced by the first lens is calculated as though the second lens were not present

The light then approaches the second lens as if it had come from the image of the first lens

The image of the first lens is treated as the object of the second lens

The image formed by the second lens is the final image of the system

Combination of Thin Lenses, 2

If the image formed by the first lens lies on the back side of the second lens, then the image is treated at a virtual object for the second lens

p will be negative

The overall magnification is the product of the magnification of the separate lenses

Combination of Thin Lenses, example

Lens and Mirror Aberrations

One of the basic problems is the imperfect quality of the images

Largely the result of defects in shape and form

Two common types of aberrations exist

Spherical aberration

Chromatic aberration

Spherical Aberration

Results from the focal points of light rays far from the principle axis are different from the focal points of rays passing near the axis

For a mirror, parabolic shapes can be used to correct for spherical aberration

Chromatic Aberration

Different wavelengths of light refracted by by a lens focus at different points

Violet rays are refracted more than red rays

The focal length for red light is greater than the focal length for violet light

Chromatic aberration can be minimized by the use of a combination of converging and diverging lenses

Real vs. Apparent Depth

 

 

Real vs. Apparent Depth