Goemmetric optics chapter 3 biology

Page 1

Chapter 3 Geometric Optics

Dr. Mohamed Saudy

1st. Year Biology 1


The Nature of Light 

Before the beginning of the nineteenth century, light was considered to be a stream of particles The particles were either emitted by the object being viewed or emanated from the eyes of the viewer Newton was the chief architect of the particle theory of light 

He believed the particles left the object and stimulated the sense of sight upon entering the eyes

2


Nature of Light – Alternative View  

Huygens argued that light might be some sort of a wave motion Thomas Young (in 1801) provided the first clear demonstration of the wave nature of light  

He showed that light rays interfere with each other Such behavior could not be explained by particles

3


Dual Nature of Light ď Ź

ď Ź

In view of these developments, light must be regarded as having a dual nature Light exhibits the characteristics of a wave in some situations and the characteristics of a particle in other situations

4


The Ray Approximation in Geometric Optics 

Geometric optics involves the study of the propagation of light It uses the assumption that light travels in a straight-line path in a uniform medium and changes its direction when it meets the surface of a different medium or if the optical properties of the medium are non-uniform The ray approximation is used to represent beams of light. 5


Ray Approximation ď Ź

ď Ź

The rays are straight lines perpendicular to the wave fronts With the ray approximation, we assume that a wave moving through a medium travels in a straight line in the direction of its rays

6


Ray Approximation, cont. 

If a wave meets a barrier, we will assume that λ<<d 

d is the diameter of the opening

This approximation is good for the study of mirrors, lenses, prisms, etc. Other effects occur for openings of other sizes 7


Active Figure 35.4

 

Adjust the size of the opening Observe the effects on the waves passing through PLAY ACTIVE FIGURE 8


Reflection of Light 

A ray of light, the incident ray, travels in a medium When it encounters a boundary with a second medium, part of the incident ray is reflected back into the first medium 

This means it is directed backward into the first medium

9


Specular Reflection 

Specular reflection is reflection from a smooth surface The reflected rays are parallel to each other All reflection in this text is assumed to be specular

10


Diffuse Reflection 

Diffuse reflection is reflection from a rough surface The reflected rays travel in a variety of directions A surface behaves as a smooth surface as long as the surface variations are much smaller than the wavelength of the light

11


Law of Reflection 

The normal is a line perpendicular to the surface 

 

It is at the point where the incident ray strikes the surface

The incident ray makes an angle of θ1 with the normal The reflected ray makes an angle of θ1’ with the normal

12


Law of Reflection, cont.  

The angle of reflection is equal to the angle of incidence θ1’= θ1 

 

This relationship is called the Law of Reflection

The incident ray, the reflected ray and the normal are all in the same plane Because this situation happens often, an analysis model, wave under reflection, is identified 13


Active Figure 35.6 

Use the active figure to vary the angle of incidence Observe the effect on the angle of reflection PLAY ACTIVE FIGURE 14


Refraction of Light 

When a ray of light traveling through a transparent medium encounters a boundary leading into another transparent medium, part of the energy is reflected and part enters the second medium The ray that enters the second medium is bent at the boundary 

This bending of the ray is called refraction 15


Refraction, 2 

The incident ray, the reflected ray, the refracted ray, and the normal all lie on the same plane The angle of refraction depends upon the material and the angle of incidence

sin θ 2 v 2  sin θ1 v 1 v1 is the speed of the light in the first medium and v2 is its speed in the second 16


Refraction of Light, 3 

The path of the light through the refracting surface is reversible  For example, a ray that travels from A to B  If the ray originated at B, it would follow the line AB to reach point A 17


Following the Reflected and Refracted Rays     

Ray  is the incident ray Ray  is the reflected ray Ray  is refracted into the lucite Ray  is internally reflected in the lucite Ray  is refracted as it enters the air from the lucite 18


Active Figure 35.10

Use the active figure to vary the incident angle Observe the effect on the reflected and refracted rays

PLAY ACTIVE FIGURE 19


Refraction Details, 1 

Light may refract into a material where its speed is lower The angle of refraction is less than the angle of incidence 

The ray bends toward the normal

20


Refraction Details, 2 

Light may refract into a material where its speed is higher The angle of refraction is greater than the angle of incidence 

The ray bends away from the normal

21


Active Figure 35.11

 

Use the active figure to observe the light passing through three layers of material Vary the incident angle and the materials Observe the effect on the refracted ray

PLAY ACTIVE FIGURE 22


Light in a Medium  

The light enters from the left The light may encounter an electron The electron may absorb the light, oscillate, and reradiate the light The absorption and radiation cause the average speed of the light moving through the material to decrease 23


The Index of Refraction 

The speed of light in any material is less than its speed in vacuum The index of refraction, n, of a medium can be defined as

speed of light in a vacuum c n  speed of light in a medium v

24


Index of Refraction, cont. 

For a vacuum, n = 1 

 

We assume n = 1 for air also

For other media, n > 1 n is a dimensionless number greater than unity 

n is not necessarily an integer

25


Some Indices of Refraction

26


Frequency Between Media 

As light travels from one medium to another, its frequency does not change 

Both the wave speed and the wavelength do change The wavefronts do not pile up, nor are created or destroyed at the boundary, so ƒ must stay the same 27


Index of Refraction Extended 

The frequency stays the same as the wave travels from one medium to the other v = ƒλ 

ƒ1 = ƒ2 but v1  v2 so λ1  λ2

The ratio of the indices of refraction of the two media can be expressed as various ratios c λ1 v1 n1 n2    λ2 v 2 c n1 n2

28


More About Index of Refraction 

The previous relationship can be simplified to compare wavelengths and indices: λ1n1 = λ2n2 In air, n1 = 1 and the index of refraction of the material can be defined in terms of the wavelengths λ n λn

 λ in vacuum    λ in a medium   29


Snell’s Law of Refraction 

n1 sin θ1 = n2 sin θ2  

θ1 is the angle of incidence θ2 is the angle of refraction

The experimental discovery of this relationship is usually credited to Willebrord Snell and is therefore known as Snell’s law of refraction Refraction is a commonplace occurrence, so identify an analysis model as a wave under refraction

30


Snell’s Law – Example  

Light is refracted into a crown glass slab θ1 = 30.0o, θ2 = ? n1 = 1.00 and n2 = 1.52 

From Table 35.1

θ2 = sin-1(n1 / n2) sin θ1 = 19.2o

The ray bends toward the normal, as expected

31


Example 1 Green light with a wavelength of 5Ă—10-7 m in a vacuum enters a glass plate with refractive index 1.5.

A. What is the velocity of light in the glass? B. What is the wavelength of the light in the glass? Solution: A) From the definition n=c/v, the velocity in the glass is

B) In the vacuum, v=c and n=1, thus

32


Example 2 A beam of light of wavelength 550 nm

traveling in air, is incident on a slab of transparent material. The incident beam makes an angle of 400 with the normal, and the refracted beam makes an angle of 260 with the

normal. Find the index of refraction of the material. Solution Using Snell's law of refraction, and taking n1=1 for air

33


Example 3 A light ray of wavelength 589 nm traveling through air is incident on a smooth, flat slab of crown glass of refractive index 1.52 at an angle of 300 to the normal, as in figure. Find the angle of refraction. Solution We rearrange Snell's law of refraction with these data n1=1 for air and n2=1.52 for crown glass to obtain: sin  2 

n1 sin 1 n2

 1    sin 30  0.329  1.52   2  sin 1 (0.329)  19.20

Because this is less than the incident angle of 300, the refracted rays is bent toward the normal.

Its change in direction is called the angle of deviation and is given by   1  2  300  19.20  10.80 34


Example 4 A light beam passes from medium 1 to medium 2, with the later medium being a thick slab of material whose index of refraction is n2 as shown in figure. Show that the emerging beam is parallel to the incident beam. Solution Let us apply Snell's law of refraction to the upper surface:

n1 sin  2  sin 1 n2 Applying this law to the lower surface gives: n sin  3  2 sin  2  n1 n n sin  3  2 ( 1 sin 1 )  sin 1 n1 n2 Therefore, 3=1, and the slab does not alter the direction of the beam. The beam parallel to itself by a distance d. 35


Prism 

A ray of singlewavelength light incident on the prism will emerge at angle  from its original direction of travel 

 is called the angle of deviation F is the apex angle

36


Dispersion 

For a given material, the index of refraction varies with the wavelength of the light passing through the material This dependence of n on λ is called dispersion Snell’s law indicates light of different wavelengths is bent at different angles when incident on a refracting material 37


Variation of Index of Refraction with Wavelength ď Ź

ď Ź

The index of refraction for a material generally decreases with increasing wavelength Violet light bends more than red light when passing into a refracting material

38


Refraction in a Prism 

Since all the colors have different angles of deviation, white light will spread out into a spectrum  

Violet deviates the most Red deviates the least The remaining colors are in between

39


The Rainbow 

A ray of light strikes a drop of water in the atmosphere It undergoes both reflection and refraction 

First refraction at the front of the drop  

Violet light will deviate the most Red light will deviate the least

40


The Rainbow, 2  

At the back surface the light is reflected It is refracted again as it returns to the front surface and moves into the air The rays leave the drop at various angles 

The angle between the white light and the most intense violet ray is 40° The angle between the white light and the most intense red ray is 42° 41


Active Figure 35.23

Use the active figure to vary the point at which the sunlight enters the raindrop Observe the angles and verify the maximum angles PLAY ACTIVE FIGURE 42


Observing the Rainbow

  

If a raindrop high in the sky is observed, the red ray is seen A drop lower in the sky would direct violet light to the observer The other colors of the spectra lie in between the red and the violet

43


Total Internal Reflection ď Ź

A phenomenon called total internal reflection can occur when light is directed from a medium having a given index of refraction toward one having a lower index of refraction

44


Possible Beam Directions ď Ź

ď Ź

Possible directions of the beam are indicated by rays numbered 1 through 5 The refracted rays are bent away from the normal since n1 > n2

45


Critical Angle 

There is a particular angle of incidence that will result in an angle of refraction of 90° 

This angle of incidence is called the critical angle, θC

n2 sin θC  (for n1  n 2 ) n1 46


Active Figure 35.25

Use the active figure to vary the incident angle Observe the effect on the refracted ray PLAY ACTIVE FIGURE 47


Critical Angle, cont. 

For angles of incidence greater than the critical angle, the beam is entirely reflected at the boundary 

This ray obeys the law of reflection at the boundary

Total internal reflection occurs only when light is directed from a medium of a given index of refraction toward a medium of lower index of refraction 48


Example 5 What is the critical angle for light going from glass with refractive index 1.5 into air? Solution: Using n1=1.5 and n2=1

Thus, light incident from the glass on a glass-air boundary will be completely reflected if the angle of incidence exceeds 420. Example 6 Find the critical angle for an air–water boundary. (The index of refraction of water is 1.33) Solution: with the air above the water having index of refraction n2 and the water having index of refraction n1.

49


Fiber Optics 

An application of internal reflection Plastic or glass rods are used to “pipe” light from one place to another Applications include 

Medical examination of internal organs Telecommunications 50


Fiber Optics, cont. ď Ź

ď Ź

A flexible light pipe is called an optical fiber A bundle of parallel fibers (shown) can be used to construct an optical transmission line

51


Construction of an Optical Fiber 

The transparent core is surrounded by cladding 

The cladding has a lower n than the core This allows the light in the core to experience total internal reflection

The combination is surrounded by the jacket

52


Problems 1. The wavelength of red helium–neon laser light in air is 632.8 nm. (a) What is its frequency? (b) What is its wavelength in glass that has an index of refraction of 1.5? (c) What is its speed in the glass? 2. A ray of light is incident on a flat surface of a block of crown glass that is surrounded by water. The angle of refraction is 19.6°. Find the angle of reflection. 3. A laser in a compact disc player generates light that has a wavelength of 780 nm in air.

I.

Find the speed of this light once it enters the plastic of a compact disc (n=1.55).

II.

What is the wavelength of this light in the plastic? Answer

(v=1.94×108

m) and (n=503 nm)

53


Notation for Mirrors and Lenses 

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

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

Denoted by p

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

54


Images ď Ź

ď Ź

Images are always located by extending diverging rays back to a point at which they intersect Images are located either at a point from which the rays of light actually diverge or at a point from which they appear to diverge

55


Types of Images 

A real image is formed when light rays pass through and diverge from the image point 

Real images can be displayed on screens

A virtual image is formed when light rays do not pass through the image point but only appear to diverge from that point 

Virtual images cannot be displayed on screens

56


Images Formed by Flat Mirrors  

Simplest possible mirror Light rays leave the source and are reflected from the mirror Point I is called the image of the object at point O The image is virtual 57


Images Formed by Flat Mirrors, 2  

A flat mirror always produces a virtual image Geometry can be used to determine the properties of the image There are an infinite number of choices of direction in which light rays could leave each point on the object Two rays are needed to determine where an image is formed 58


Images Formed by Flat Mirrors, 3 

One ray starts at point P, travels to Q and reflects back on itself Another ray follows the path PR and reflects according to the law of reflection The triangles PQR and P’QR are congruent 59


Active Figure 36.2 

Use the active figure to move the object Observe the effect on the image

PLAY ACTIVE FIGURE 60


Images Formed by Flat Mirrors, 4 

To observe the image, the observer would trace back the two reflected rays to P’ Point P’ is the point where the rays appear to have originated The image formed by an object placed in front of a flat mirror is as far behind the mirror as the object is in front of the mirror 

|p| = |q| 61


Lateral Magnification 

Lateral magnification, M, is defined as Image height h' M  Object height h 

 

This is the general magnification for any type of mirror It is also valid for images formed by lenses Magnification does not always mean bigger, the size can either increase or decrease 

M can be less than or greater than 1 62


Lateral Magnification of a Flat Mirror  

The lateral magnification of a flat mirror is +1 This means that h’ = h for all images The positive sign indicates the object is upright 

Same orientation as the object

63


Reversals in a Flat Mirror ď Ź

A flat mirror produces an image that has an apparent left-right reversal ď Ź

For example, if you raise your right hand the image you see raises its left hand

64


Reversals, cont. 

The reversal is not actually a left-right reversal The reversal is actually a front-back reversal 

It is caused by the light rays going forward toward the mirror and then reflecting back from it

65


Properties of the Image Formed by a Flat Mirror – Summary 

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

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 

|p| = |q|

It has the same orientation as the object

There is a front-back reversal in the image 66


Spherical Mirrors 

 

A spherical mirror has the shape of a section of a sphere The mirror focuses incoming parallel rays to a point 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

67


Concave Mirror, Notation    

The mirror has a radius of curvature of R Its center of curvature is the point C Point V is the center of the spherical segment A line drawn from C to V is called the principal axis of the mirror

68


Paraxial Rays 

 

We use only rays that diverge from the object and make a small angle with the principal axis Such rays are called paraxial rays All paraxial rays reflect through the image point

69


Spherical Aberration 

Rays that are far from the principal axis converge to other points on the principal axis This produces a blurred image The effect is called spherical aberration

70


Image Formed by a Concave Mirror 

Geometry can be used to determine the magnification of the image

h' q M  h p 

h’ is negative when the image is inverted with respect to the object

71


Image Formed by a Concave Mirror 

Geometry also shows the relationship between the image and object distances

1 1 2   p q R This is called the mirror equation

If p is much greater than R, then the image point is half-way between the center of curvature and the center point of the mirror 

p → ∞ , then 1/p  0 and q  R/2 72


Focal Length 

When the object is very far away, then p → ∞ and the 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

73


Focal Point, cont. 

The colored beams are traveling parallel to the principal axis The mirror reflects all three beams to the focal point The focal point is where all the beams intersect 

It is the white point

74


Focal Point and Focal Length, cont. 

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

 

It also does not depend on the material from which the mirror is made

ƒ=R/2 The mirror equation can be expressed as 1 1 1   p q ƒ 75


Focal Length Shown by Parallel Rays

76


Example 1: Assume that a certain spherical mirror has a focal length of +10 cm. Locate and describe the image for object distances of (A) 25 cm, (B) 10 cm, and (C) 5 cm. Solution: A) Because the focal length is positive f=+10cm, we expect the image to be real. 1 1 1   p q f 1 1 1    25 cm q 10 cm

q  16.7 cm

The magnification of the image is given by M is less than unity tells us that

q 16.7 cm M     0.668 p 25 cm

the image is smaller than the object, and the negative sign for M tells us that the image is inverted

77


B) When the object distance is 10 cm, the object is located at the focal point 1 1 1   p q f 1 1 1    10 cm q 10 cm

q  

so that the image is formed at an infinite distance from the mirror; that is, the rays travel parallel to one another after reflection. This is the situation in a flashlight, where the bulb filament is placed at the focal point of a reflector, producing a parallel beam of light.

78


C) When the object is at p=5 cm, it lies halfway between the focal point and the mirror surface 1 1 1   p q f 1 1 1    5 cm q 10 cm

q  10 cm

The image is virtual because it is located behind the mirror. The magnification of the image is

q 10 cm M    ( )  2 p 5 cm The image is twice as large as the object, and the positive sign for M indicates that the image is upright 79


Convex Mirrors 

A convex mirror is sometimes called a diverging mirror 

The light reflects from the outer, convex side

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 the reflected rays only appear to originate at the image point 80


Image Formed by a Convex Mirror

ď Ź

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

81


Sign Conventions ď Ź

ď Ź

These sign conventions apply to both concave and convex mirrors The equations used for the concave mirror also apply to the convex mirror

82


Sign Conventions, Summary Table

83


Ray Diagrams 

A ray diagram can be used to determine the position and size of an image They are graphical constructions which reveal the nature of the image They can also be used to check the parameters calculated from the mirror and magnification equations

84


Drawing a Ray Diagram 

To draw a ray diagram, you need to know:  

Three rays are drawn 

The position of the object The locations of the focal point and the center of curvature 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 85


The Rays in a Ray Diagram – Concave Mirrors 

Ray 1 is drawn from the top of the object parallel to the principal axis and is reflected through the focal point, F Ray 2 is drawn from the top of the object through the focal point and is reflected parallel to the principal axis Ray 3 is drawn through the center of curvature, C, and is reflected back on itself 86


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

87


Ray Diagram for a Concave Mirror, p > R

   

The center of curvature is between the object and the concave mirror surface The image is real The image is inverted The image is smaller than the object (reduced) 88


Ray Diagram for a Concave Mirror, p < f

   

The object is between the mirror surface and the focal point The image is virtual The image is upright The image is larger than the object (enlarged) 89


The Rays in a Ray Diagram – Convex Mirrors 

Ray 1 is drawn from the top of the object parallel to the principal axis and is reflected away from the focal point, F Ray 2 is drawn from the top of the object toward the focal point and is reflected parallel to the principal axis Ray 3 is drawn through the center of curvature, C, on the back side of the mirror and is reflected back on itself 90


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 (reduced) 91


Active Figure 36.13 

Use the active figure to  

Move the object Change the focal length

Observe the effect on the images

PLAY ACTIVE FIGURE 92


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 decreases, the virtual image increases in size 93


The Image from a Convex Mirror Example 2: An anti-shoplifting mirror, as shown in Figure, shows an image of a woman who is located 3 m from the mirror. The focal length of the mirror is -0.25 m. Find (A) the position of her image and (B) the magnification of the image Solution: (A) We should expect to find an upright, reduced, virtual image 1 1 1   p q f 1 1 1    3m q 0.25 m

q   0.23 m

(B) The magnification of the image is

q 0.23m M    ( )  0.077 p 3m

The image is much smaller than the woman, and it is upright because M is positive 94


Images Formed by Refraction 

Consider two transparent media having indices of refraction n1 and n2 The boundary between the two media is a spherical surface of radius R Rays originate from the object at point O in the medium with n = n1 95


Images Formed by Refraction, 2  

We will consider the paraxial rays leaving O All such rays are refracted at the spherical surface and focus at the image point, I The relationship between object and image distances can be given by n1 n2 n2  n1   p q R

96


Images Formed by Refraction, 3 

 

The side of the surface in which the light rays originate is defined as the front side The other side is called the back side Real images are formed by refraction in the back of the surface 

Because of this, the sign conventions for q and R for refracting surfaces are opposite those for reflecting surfaces

97


Sign Conventions for Refracting Surfaces

98


Flat Refracting Surfaces  

If a refracting surface is flat, then R is infinite Then q = -(n2 / n1)p 

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

A virtual image is formed

99


Active Figure 36.18

Use the active figure to move the object Observe the effect on the location of the image PLAY ACTIVE FIGURE 100


Example 3: A set of coins is embedded in a spherical plastic paperweight having a radius of 3 cm. The index of refraction of the plastic is n1=1.5. One coin is located 2 cm from the edge of the sphere (Figure). Find the position of the image of the coin. Solution Because n1 > n 2, where n2=1 is the index of refraction for air, the rays originating from the coin are refracted away from the normal at the surface and diverge outward. Hence, the image is formed inside the paperweight and is virtual. Note that: (R=-3cm)

n1 n2 n2  n1   p q R 1.5 1 1  1.5    q  1.7cm 2 q 3

The negative sign for q indicates that the image is in front of the surface the image must be virtual. The coin appears to be closer to the paperweight surface than it actually is.

101


Example 4: A small fish is swimming at a depth d below the surface of a pond (Figure). What is the apparent depth of the fish, as viewed from directly overhead? Solution Because the refracting surface is flat, R is infinite. Hence, we can use the Equation to determine the location of the image with p =d

n2 1 q p d  0.752d n1 1.33 Because q is negative, the image is virtual, as indicated by the dashed lines in Figure. The apparent depth is approximately three-fourths the actual depth. 102


Lenses 

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

Cameras Telescopes Microscopes

103


Images from Lenses ď Ź

ď Ź

Light passing through a lens experiences refraction at two surfaces The image formed by one refracting surface serves as the object for the second surface

104


Locating the Image Formed by a Lens 

The lens has an index of refraction n and two spherical surfaces with radii of R1 and R2  R1 is the radius of curvature of the lens surface that the light of the object reaches first  R2 is the radius of curvature of the other surface The object is placed at point O at a distance of p1 in front of the first surface 105


Locating the Image Formed by a Lens, Image From Surface 1  

There is an image formed by surface 1 Since the lens is surrounded by the air, n1 = 1 and n1 n2 n2  n1 1 n n 1      p q R p1 q1 R1

If the image due to surface 1 is virtual, q1 is negative, and it is positive if the image is real

106


Locating the Image Formed by a Lens, Image From Surface 2 

For surface 2, n1 = n and n2 = 1 

The light rays approaching surface 2 are in the lens and are refracted into air

Use p2 for the object distance for surface 2 and q2 for the image distance n1 n2 n2  n1 n 1 1 n      p q R p2 q2 R2

107


Image Formed by a Thick Lens 

If a virtual image is formed from surface 1, then p2 = -q1 + t  

If a real image is formed from surface 1, then p2 = -q1 + t 

q1 is negative t is the thickness of the lens

q1 is positive

Then  1 1 1 1     n  1    p1 q2  R1 R2 

108


Image Formed by a Thin Lens 

A thin lens is one whose thickness is small compared to the radii of curvature For a thin lens, the thickness, t, of the lens can be neglected In this case, p2 = -q1 for either type of image Then the subscripts on p1 and q2 can be omitted

109


Lens Makers’ Equation 

The focal length of a thin lens is the image distance that corresponds to an infinite object distance 

This is the same as for a mirror

The lens makers’ equation is

 1 1 1 1  1   (n  1)    p q  R1 R2  ƒ 110


Thin Lens Equation 

The relationship among the focal length, the object distance and the image distance is the same as for a mirror

1 1 1   p q ƒ

111


Notes on Focal Length and Focal Point of a Thin Lens 

Because light can travel in either direction through a lens, each lens has two focal points 

 

One focal point is for light passing in one direction through the lens and one is for light traveling in the opposite direction

However, there is only one focal length Each focal point is located the same distance from the lens 112


Focal Length of a Converging Lens

ď Ź

ď Ź

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 113


Focal Length of a Diverging Lens

ď Ź

ď Ź

The parallel rays diverge after passing through the diverging lens The focal point is the point where the rays appear to have originated 114


Determining Signs for Thin Lenses ď Ź

ď Ź

ď Ź

The front side of the thin lens is the side of the incident light The light is refracted into the back side of the lens This is also valid for a refracting surface

115


Sign Conventions for Thin Lenses

116


Magnification of Images Through a Thin Lens 

The lateral magnification of the image is h' q M  h p When M is positive, the image is upright and on the same side of the lens as the object When M is negative, the image is inverted and on the side of the lens opposite the object 117


Thin Lens Shapes 

These are examples of converging lenses They have positive focal lengths They are thickest in the middle

118


More Thin Lens Shapes 

These are examples of diverging lenses They have negative focal lengths They are thickest at the edges

119


Ray Diagrams for Thin Lenses – Converging  

Ray diagrams are convenient for locating the images formed by thin lenses or systems of lenses For a converging lens, the following three rays are drawn:   

Ray 1 is drawn parallel to the principal axis and then passes through the focal point on the back side of the lens Ray 2 is drawn through the center of the lens and continues in a straight line Ray 3 is drawn through the focal point on the front of the lens (or as if coming from the focal point if p < ƒ) and emerges from the lens parallel to the principal axis

120


Ray Diagram for Converging Lens, p > f

 

The image is real The image is inverted The image is on the back side of the lens 121


Ray Diagram for Converging Lens, p < f

   

The image is virtual The image is upright The image is larger than the object The image is on the front side of the lens 122


Ray Diagrams for Thin Lenses – Diverging 

For a diverging lens, the following three rays are drawn: 

Ray 1 is drawn parallel to the principal axis and emerges directed away from the focal point on the front side of the lens Ray 2 is drawn through the center of the lens and continues in a straight line Ray 3 is drawn in the direction toward the focal point on the back side of the lens and emerges from the lens parallel to the principal axis

123


Ray Diagram for Diverging Lens

 

 

The image is virtual The image is upright The image is smaller The image is on the front side of the lens 124


Active Figure 36.26 

Use the active figure to  

Move the object Change the focal length of the lens

Observe the effect on the image PLAY ACTIVE FIGURE 125


Image Summary 

For a converging lens, when the object distance is greater than the focal length, (p > ƒ) 

For a converging lens, when the object is between the focal point and the lens, (p < ƒ) 

The image is real and inverted

The image is virtual and upright

For a diverging lens, the image is always virtual and upright 

This is regardless of where the object is placed

126


Example 5: A converging lens of focal length 10 cm forms images of objects placed at (A) 30 cm, (B) 10 cm, and (C) 5 cm from the lens. In each case, construct a ray diagram, find the image distance and describe the image. Solution: (A) we construct a ray diagram as shown in Figure. The diagram shows that we should expect a real, inverted, smaller image to be formed on the back side of the lens.

1 1 1   p q f 1 1 1    q  15 cm 30 q 10 The positive sign for the image distance tells us that the image is indeed real and on the back side of the lens. The magnification of the image is q 15 M    0.5 p 30 Thus, the image is reduced in height by one half, and the negative sign for M tells us that the image is inverted

127


(B) the object is placed at the focal point, the image is formed at infinity. This is readily verified by substituting p=10 cm into the thin lens equation. (C) The ray diagram in Figure shows that in this case the lens acts as a magnifying glass; that is, the image is magnified, upright, on the same side of the lens as the object, and virtual. Because the object distance is 5 cm.

1 1 1   p q f 1 1 1    q  10 cm 5 q 10 and the magnification of the image is

q 10  ( )  2 p 5 The negative image distance tells us that the image is virtual and formed on the side of the lens from which the light is incident, the front side. The image is enlarged, and the positive sign for M tells us that the image is upright M 

128


Example 6: A diverging lens of focal length 10 cm forms images of objects placed at (A) 30 cm, (B) 10 cm, and (C) 5 cm from the lens. In each case, construct a ray diagram, find the image distance and describe the image. Solution: (A) constructing a ray diagram as in Figure taking the object distance to be 30 cm. The diagram shows that we should expect an image that is virtual, smaller than the object, and upright

1 1 1   p q ƒ 1 1 1    q  75 . cm 30 q 10 The magnification of the image is

M 

q 7.5  ( )  0.25 p 30

This result confirms that the image is virtual, smaller than the object, and upright 129


(B) When the object is at the focal point, the ray diagram appears as in Figure

1 1 1   p q f 1 1 1    q  5 cm 10 q 10 The magnification of the image is

M 

q 5  ( )  0.5 p 10

Notice the difference between this situation and that for a converging lens. For a diverging lens, an object at the focal point does not produce an image infinitely far away.

130


(C) When the object is inside the focal point, at p =5 cm, the ray diagram in Figure, shows that we expect a virtual image that is smaller than the object and upright

1 1 1   p q f 1 1 1    q  3.33 cm 5 q 10 and the magnification of the image is

q 3.33 M    ( )  0.667 p 5 This confirms that the image is virtual, smaller than the object, and upright

131


Example 7: A converging glass lens (n =1.52) has a focal length of 40 cm in air. Find its focal length when it is immersed in water, which has an index of refraction of 1.33. Solution We can use the lens makers’ equation in both cases, noting that R1 and R2 remain the same in air and water:

1 1 1  (n  1)(  ) f air R1 R2 1 f water

 (n  1)(

1 1  ) R1 R2

where is the ratio of the index of refraction of glass to that of water: =1.52/1.33=1.14. Dividing the first equation by the second gives

f water n  1 1.52  1    3.71 f air n  1 1.14  1

 f water  3.71 f air  3.71  (40)  148 cm n 1

The focal length of any lens is increased by a factor n  1 when the lens is immersed in a fluid, where is the ratio of the index of refraction n of the lens material to that of the fluid.

132


Fresnal Lens 

Refraction occurs only at the surfaces of the lens A Fresnal lens is designed to take advantage of this fact It produces a powerful lens without great thickness

133


Fresnal Lens, cont. 

Only the surface curvature is important in the refracting qualities of the lens The material in the middle of the Fresnal lens is removed Because the edges of the curved segments cause some distortion, Fresnal lenses are usually used only in situations where image quality is less important than reduction of weight 134


Combinations of Thin Lenses 

The image formed by the first lens is located as though the second lens were not present Then a ray diagram is drawn for the second 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 135


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 as a virtual object for the second lens 

p will be negative

The same procedure can be extended to a system of three or more lenses The overall magnification is the product of the magnification of the separate lenses 136


Two Lenses in Contact 

Consider a case of two lenses in contact with each other 

The lenses have focal lengths of ƒ1 and ƒ2

For the first lens, 1 1 1   p q1 ƒ1

Since the lenses are in contact, p2 = -q1 137


Two Lenses in Contact, cont. 

For the second lens, 1 1 1 1 1     p2 q2 ƒ2 q1 q

For the combination of the two lenses 1 1 1   ƒ ƒ1 ƒ 2

Two thin lenses in contact with each other are equivalent to a single thin lens having a focal length given by the above equation 138


Combination of Thin Lenses, example

139


Combination of Thin Lenses, example  

 

Find the location of the image formed by lens 1 Find the magnification of the image due to lens 1 Find the object distance for the second lens Find the location of the image formed by lens 2 Find the magnification of the image due to lens 2 Find the overall magnification of the system 140


Example 8: Two thin converging lenses of focal lengths f1=10 cm and f2=20 cm are separated by 20 cm, as illustrated in Figure. An object is placed 30 cm to the left of lens 1. Find the position and the magnification of the final image. Solution: To analyze the problem, we first draw a ray diagram showing where the image from the first lens falls and how it acts as the object for the second lens. The location of the image formed by lens 1 is found from the thin lens equation:

1 1 1   p1 q1 f1 1 1 1    q1  15 cm 30 q1 10 The magnification of this image is

q1 15 M1      0.5 p1 30

The image formed by this lens acts as the object for the second lens. Thus, the object distance for the second lens is 20 cm - 15 cm =5 cm. We again apply the thin lens equation to find the location of the final image: 141


1 1 1   p2 q2 f 2 1 1 1    q2  6.67 cm 5 q2 20 The magnification of the second image is M 2   Thus, the overall magnification of the system is

q2 6.67  ( )  1.33 p2 5

M  M1M 2  (0.5)  (1.33)  0.667 Note that the negative sign on the overall magnification indicates that the final image is inverted with respect to the initial object. The fact that the absolute value of the magnification is less than one tells us that the final image is smaller than the object. The fact that q2 is142 negative tells us that the final image is on the front, or left, side of lens 2.


Lens Aberrations 

Assumptions have been:  

The rays from a point object do not focus at a single point 

Rays make small angles with the principal axis The lenses are thin

The result is a blurred image This is a situation where the approximations used in the analysis do not hold

The departures of actual images from the ideal predicted by our model are called aberrations 143


Spherical Aberration 

This results from the focal points of light rays far from the principal axis being different from the focal points of rays passing near the axis For a camera, a small aperture allows a greater percentage of the rays to be paraxial For a mirror, parabolic shapes can be used to correct for spherical aberration 144


Chromatic Aberration 

Different wavelengths of light refracted 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 made of different materials 145


The Camera 

The photographic camera is a simple optical instrument Components  

Light-tight chamber Converging lens  Produces a real image Film behind the lens  Receives the image

146


Camera Operation  

Proper focusing will result in sharp images The camera is focused by varying the distance between the lens and the film 

The lens-to-film distance will depend on the object distance and on the focal length of the lens

The shutter is a mechanical device that is opened for selected time intervals 

The time interval that the shutter is opened is called the exposure time 147


Camera Operation, Intensity 

Light intensity is a measure of the rate at which energy is received by the film per unit area of the image 

The intensity of the light reaching the film is proportional to the area of the lens

The brightness of the image formed on the film depends on the light intensity 

Depends on both the focal length and the diameter of the lens 148


Digital Camera  

Digital cameras are similar in operation The image does not form on photographic film The image does form on a charge-coupled device (CCD) 

This digitizes the image and turns it into a binary code The digital information can then be stored on a memory chip for later retrieval 149


The Eye 

The normal eye focuses light and produces a sharp image Essential parts of the eye: 

Cornea – light passes through this transparent structure Aqueous Humor – clear liquid behind the cornea

150


The Eye – Parts, cont. 

The pupil 

 

A variable aperture An opening in the iris

The crystalline lens Most of the refraction takes place at the outer surface of the eye 

Where the cornea is covered with a film of tears

151


The Eye – Close-up of the Cornea

152


The Eye – Parts, final 

The iris is the colored portion of the eye 

It is a muscular diaphragm that controls pupil size The iris regulates the amount of light entering the eye  

It dilates the pupil in low light conditions It contracts the pupil in high-light conditions

The f-number of the eye is from about 2.8 to 16

153


The Eye – Operation 

The cornea-lens system focuses light onto the back surface of the eye  

This back surface is called the retina The retina contains sensitive receptors called rods and cones These structures send impulses via the optic nerve to the brain 

This is where the image is perceived

154


The Eye – Operation, cont. 

Accommodation 

 

The eye focuses on an object by varying the shape of the pliable crystalline lens through this process Takes place very quickly Limited in that objects very close to the eye produce blurred images

155


The Eye – Near and Far Points 

The near point is the closest distance for which the lens can accommodate to focus light on the retina   

Typically at age 10, this is about 18 cm The average value is about 25 cm It increases with age  Up to 500 cm or greater at age 60

The far point of the eye represents the largest distance for which the lens of the relaxed eye can focus light on the retina 

Normal vision has a far point of infinity 156


The Eye – Seeing Colors 

Only three types of color-sensitive cells are present in the retina 

They are called red, green and blue cones

What color is seen depends on which cones are stimulated

157


Conditions of the Eye 

Eyes may suffer a mismatch between the focusing power of the lens-cornea system and the length of the eye Eyes may be: 

Farsighted 

Light rays reach the retina before they converge to form an image

Nearsighted 

Person can focus on nearby objects but not those far away 158


Farsightedness

  

Also called hyperopia The near point of the farsighted person is much farther away than that of the normal eye The image focuses behind the retina Can usually see far away objects clearly, but not nearby objects 159


Correcting Farsightedness

 

A converging lens placed in front of the eye can correct the condition The lens refracts the incoming rays more toward the principal axis before entering the eye 

This allows the rays to converge and focus on the retina 160


Nearsightedness

  

Also called myopia The far point of the nearsighted person is not infinity and may be less than one meter The nearsighted person can focus on nearby objects but not those far away 161


Correcting Nearsightedness

 

A diverging lens can be used to correct the condition The lens refracts the rays away from the principal axis before they enter the eye 

This allows the rays to focus on the retina 162


Presbyopia and Astigmatism 

Presbyopia (literally, “old-age vision”) is due to a reduction in accommodation ability 

The cornea and lens do not have sufficient focusing power to bring nearby objects into focus on the retina Condition can be corrected with converging lenses

In astigmatism, light from a point source produces a line image on the retina 

Produced when either the cornea or the lens or both are not perfectly symmetric Can be corrected with lenses with different curvatures in two mutually perpendicular directions 163


Diopters 

Optometrists and ophthalmologists usually prescribe lenses measured in diopters 

The power P of a lens in diopters equals the inverse of the focal length in meters 

P = 1/ƒ

164


Example 9: A particular nearsighted person is unable to see objects clearly when they are beyond 2.5 m away (the far point of this particular eye). What should the focal length be in a lens prescribed to correct this problem? Solution The purpose of the lens in this instance is to “move” an object from infinity to a distance where it can be seen clearly. This is accomplished by having the lens produce an image at the far point. From the thin lens equation, we have

1 1 1   p q f 1 1 1    2.5 m f  f  2.5 m

We use a negative sign for the image distance because the image is virtual and in front of the eye. As you should have suspected, the lens must be a diverging lens (one with a negative focal length) to correct nearsightedness. 165


Simple Magnifier ď Ź

ď Ź

ď Ź

A simple magnifier consists of a single converging lens This device is used to increase the apparent size of an object The size of an image formed on the retina depends on the angle subtended by the eye

166


The Size of a Magnified Image 

When an object is placed at the near point, the angle subtended is a maximum 

The near point is about 25 cm

When the object is placed near the focal point of a converging lens, the lens forms a virtual, upright, and enlarged image

167


Angular Magnification 

Angular magnification is defined as θ angle with lens m  θo angle without lens

The angular magnification is at a maximum when the image formed by the lens is at the near point of the eye  

q = - 25 cm 25 cm Calculated by m max  1 

f

168


Angular Magnification, cont. 

The eye is most relaxed when the image is at infinity 

Although the eye can focus on an object anywhere between the near point and infinity

For the image formed by a magnifying glass to appear at infinity, the object has to be at the focal point of the lens θ 25 cm The angular magnification is mmin   θo

ƒ

169


Example 10: What is the maximum magnification that is possible with a lens having a focal length of 10 cm, and what is the magnification of this lens when the eye is relaxed? Solution The maximum magnification occurs when the image is located at the near point of the eye

mmax

25 cm 25 cm  1  1  3.5 f 10 cm

When the eye is relaxed, the image is at infinity

mmin

25 cm 25 cm    2.5 f 10 cm 170


Magnification by a Lens 

With a single lens, it is possible to achieve angular magnification up to about 4 without serious aberrations With multiple lenses, magnifications of up to about 20 can be achieved 

The multiple lenses can correct for aberrations

171


Compound Microscope 

A compound microscope consists of two lenses 

Gives greater magnification than a single lens The objective lens has a short focal length, ƒo< 1 cm The eyepiece has a focal length, ƒe of a few cm

172


Compound Microscope, cont. 

The lenses are separated by a distance L 

The object is placed just outside the focal point of the objective  

L is much greater than either focal length

This forms a real, inverted image This image is located at or close to the focal point of the eyepiece

This image acts as the object for the eyepiece 

The image seen by the eye, I2, is virtual, inverted and very much enlarged 173


Active Figure 36.41 

Use the active figure to adjust the focal lengths of the objective and eyepiece lenses Observe the effect on the final image

PLAY ACTIVE FIGURE 174


Magnifications of the Compound Microscope 

The lateral magnification by the objective is 

The angular magnification by the eyepiece of the microscope is 

Mo = - L / ƒ o

me = 25 cm / ƒe

The overall magnification of the microscope is the product of the individual magnifications L M  M o me   ƒo

 25 cm    ƒ e   175


Other Considerations with a Microscope 

The ability of an optical microscope to view an object depends on the size of the object relative to the wavelength of the light used to observe it 

For example, you could not observe an atom (d  0.1 nm) with visible light (λ  500 nm)

176


Telescopes  

Telescopes are designed to aid in viewing distant objects Two fundamental types of telescopes  

Refracting telescopes use a combination of lenses to form an image Reflecting telescopes use a curved mirror and a lens to form an image

Telescopes can be analyzed by considering them to be two optical elements in a row 

The image of the first element becomes the object of the second element 177


Refracting Telescope 

The two lenses are arranged so that the objective forms a real, inverted image of a distant object The image is formed at the focal point of the eyepiece 

p is essentially infinity

The two lenses are separated by the distance ƒo + ƒe which corresponds to the length of the tube The eyepiece forms an enlarged, inverted image of the first image 178


Active Figure 36.42 

Use the active figure to adjust the focal lengths of the objective and eyepiece lenses Observe the effects on the image

PLAY ACTIVE FIGURE 179


Angular Magnification of a Telescope 

The angular magnification depends on the focal lengths of the objective and eyepiece

θ ƒo m  θo ƒe 

The negative sign indicates the image is inverted

Angular magnification is particularly important for observing nearby objects  

Nearby objects would include the sun or the moon Very distant objects still appear as a small point of light

180


Disadvantages of Refracting Telescopes 

Large diameters are needed to study distant objects Large lenses are difficult and expensive to manufacture The weight of large lenses leads to sagging which produces aberrations

181


Reflecting Telescope 

Helps overcome some of the disadvantages of refracting telescopes  

Replaces the objective lens with a mirror The mirror is often parabolic to overcome spherical aberrations

In addition, the light never passes through glass   

Except the eyepiece Reduced chromatic aberrations Allows for support and eliminates sagging 182


Reflecting Telescope, Newtonian Focus 

The incoming rays are reflected from the mirror and converge toward point A 

At A, an image would be formed

A small flat mirror, M, reflects the light toward an opening in the side and it passes into an eyepiece 

This occurs before the image is formed at A

183


Examples of Telescopes 

Reflecting Telescopes 

Largest in the world are the 10-m diameter Keck telescopes on Mauna Kea in Hawaii 

Each contains 36 hexagonally shaped, computercontrolled mirrors that work together to form a large reflecting surface

Refracting Telescopes 

Largest in the world is Yerkes Observatory in Williams Bay, Wisconsin 

Has a diameter of 1 m 184


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