4.Example: Multiple mirrors and virtual images: how far away are the virtual images? 1m3m VII. Mirrors.

Slides:



Advertisements
Similar presentations
Chapter 23 Mirrors and Lenses
Advertisements

Notation for Mirrors and Lenses
Chapter 31: Images and Optical Instruments
Chapter 23:Mirrors and Lenses Flat Mirrors Homework assignment : 20,24,42,45,51  Image of a point source P P’ The reflected rays entering eyes look as.
Flat Mirrors Consider an object placed in front of a flat mirror
Chapter 31 Images.
Chapter 26 Geometrical Optics. Units of Chapter 26 The Reflection of Light Forming Images with a Plane Mirror Spherical Mirrors Ray Tracing and the Mirror.
Physics Light: Geometric Optics 23.1 The Ray Model of Light 23.2 Reflection - Plane Mirror 23.3 Spherical Mirrors 23.5 Refraction - Snell’s law.
Reflection, Refraction and Lenses
Physics 2225: Optics 1 - Activities with Light Rays Purpose of this Minilab Apply the basics of ray tracing to learn about reflection and refraction of.
and Optical Instruments
Reference Book is Geometric Optics.
Reflection and Refraction. Reflection  Reflection occurs when light bounces off a surface.  There are two types of reflection – Specular reflection.
Mirrors Physics 202 Professor Lee Carkner Lecture 22.
Images Formed by Refraction
Fig Reflection of an object (y) from a plane mirror. Lateral magnification m = y ’ / y © 2003 J. F. Becker San Jose State University Physics 52 Heat.
Physics 1502: Lecture 30 Today’s Agenda Announcements: –Midterm 2: Monday Nov. 16 … –Homework 08: due Friday Optics –Mirrors –Lenses –Eye.
Physics 1402: Lecture 31 Today’s Agenda Announcements: –Midterm 2: Monday Nov. 16 … –Homework 08: due Wednesday (after midterm 2) Optics –Lenses –Eye.
Lenses Physics 202 Professor Lee Carkner Lecture 21.
C F V Light In Side S > 0 Real Object Light Out Side S ’ > 0 Real Image C This Side, R > 0 S < 0 Virtual Object S ’ < 0 Virtual Image C This Side, R
Reflection Physics Department, New York City College of Technology.
Mirrors Physics 202 Professor Lee Carkner Lecture 22.
Geometric Optics Ray Model assume light travels in straight line
Copyright © 2012 Pearson Education Inc. PowerPoint ® Lectures for University Physics, Thirteenth Edition – Hugh D. Young and Roger A. Freedman Lectures.
Physics 1502: Lecture 29 Today’s Agenda Announcements: –Midterm 2: Monday Nov. 16 … –Homework 08: due Friday Optics –Index of Refraction.
Optics Can you believe what you see?. Optics Reflection: Light is retransmitted from or “bounces off” an object.
Lecture 14 Images Chapter 34. Law of Reflection Dispersion Snell’s Law Brewsters Angle Preliminary topics before mirrors and lenses.
Example: An object 3 cm high is placed 20 cm from (a) a convex and (b) a concave spherical mirror, each of 10 cm focal length. Determine the position.
Lecture 14 Images Chp. 35 Opening Demo Topics –Plane mirror, Two parallel mirrors, Two plane mirrors at right angles –Spherical mirror/Plane mirror comparison.
Optics 1 - Activities with Light Rays Purpose of this Minilab Apply the basics of ray tracing to learn about reflection and refraction of light.
Index of Refraction Index of refraction of a medium is defined in terms of the speed of light in this medium In general, the speed of light in any material.
Lecture 14 Mirrors Chapter 23.1  23.3 Outline Flat Mirrors Spherical Concave Mirrors Spherical Convex Mirrors.
Mirrors and Lenses.
Geometric Optics Conceptual Quiz 23.
Chapter 14 Light and Reflection
Physics 1C Lecture 26A.
Physics C Chapter 36 From serway book Prepared by Anas A. Alkanoa M.Sc.( master degree) in Theoretical Physics, Electromagnetic Waves (Optical Science),
Mirrors Plane and Spherical. Plane Mirrors Flat mirrors. Which type of image? Virtual We perceive the image at point I where the ray extensions intersect.
Images and Optical Instruments. Definitions Real Image - Light passes through the image point. Virtual Image - Light does not pass through the image point.
 Mirrors that are formed from a section of a sphere.  Convex: The reflection takes place on the outer surface of the spherical shape  Concave: The.
8. Thin lenses Thin lenses are those whose thickness is small compared to their radius of curvature. They may be either converging or diverging. 1) Types.
Last Word on Chapter 22 Geometric Optics Images in a Plane Mirror.
Chapter 36 Image Formation (Lens and Mirrors) Using the ray approximation of geometric optics, we can now study how images are formed with mirrors and.
Unit 11: Part 2 Mirrors and Lenses. Outline Plane Mirrors Spherical Mirrors Lenses The Lens Maker’s Equation Lens Aberrations.
Geometric Optics This chapter covers how images form when light bounces off mirrors and refracts through lenses. There are two different kinds of images:
Chapter 35 MirrorsLenses Images. We will use geometrical optics: light propagates in straight lines until its direction is changed by reflection or refraction.
 When light strikes the surface of an object  Some light is reflected  The rest is absorbed (and transferred into thermal energy)  Shiny objects,
In describing the propagation of light as a wave we need to understand: wavefronts: a surface passing through points of a wave that have the same phase.
1 32 Optical Images image formation reflection & refraction mirror & lens equations Human eye Spherical aberration Chromatic aberration.
Physics 203/204 4: Geometric Optics Images formed by refraction Lens Makers Equation Thin lenses Combination of thin lenses Aberration Optical Instruments.
Dispersion The spreading of light into its color components is called dispersion. When light enters a prism, the refracted ray is bent towards the normal,
Chapter 27 Lenses and Optical Instruments. Lenses Converging lens Diverging lens.
Thin Lenses A lens is an optical device consisting of two refracting surfaces The simplest lens has two spherical surfaces close enough together that we.
Physics 1202: Lecture 23 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
 Mirrors that are formed from a section of a sphere.  Convex: The reflection takes place on the outer surface of the spherical shape  Concave: The.
Today 2/10  Multiple Lens Systems 26.9  Curved Mirrors  Lab: Mirrors and Thin Lenses  HW:“2/10 Two Lenses” Due Thursday 2/12  Exam IThursday,
Image Formation. Flat Mirrors  p is called the object distance  q is called the image distance  θ 1 = θ 2 Virtual Image: formed when light rays do.
Physics 1202: Lecture 22 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Chapter Reflection and Mirrors. Millions of light rays reflect from objects and enter our eyes – that’s how we see them! When we study the formation of.
July © Chuck DiMarzio, Northeastern University ECEG105/ECEU646 Optics for Engineers Course Notes Part 2: Geometric Optics (Reflection,
ECEG105 & ECEU646 Optics for Engineers Course Notes Part 2: Geometric Optics (Reflection, Refraction, Thin Lenses) Prof. Charles A. DiMarzio Northeastern.
1 The law of reflection: The law of refraction: Snell’s Law Image formation.
Example: What kind of lens must be used, in order to give an erect image 1/5 as large as an object placed 15 cm in front of it? M = -q/p  -q/p=1/5 So.
Geometrical Optics.
Light & Optics Chapters Electromagnetic Wave.
Geometric Optics Ray Model assume light travels in straight line
17.2 Mirrors, Lenses, and Images
Mirrors, Plane and Spherical Spherical Refracting Surfaces
Optics Mirrors and Lenses.
Lens Equations.
Presentation transcript:

4.Example: Multiple mirrors and virtual images: how far away are the virtual images? 1m3m VII. Mirrors

4.Example: Multiple mirrors and virtual images: how far away are the virtual images? 2m3m

4.Example: Multiple mirrors and virtual images: how far away are the virtual images? 6m2m

4.Example: Multiple mirrors and virtual images: how far away are the virtual images? 6m2m8m

4.Example: Multiple mirrors and virtual images: how far away are the virtual images? 2m8m10m16m 18m

d) Example: A telescope is designed to take images of distant galaxies. If the diameter of the telescope’s spherical mirror is 40 cm, where should a detector be placed? *Step 1: Stars ~ infinitely far away *Step 2: Use mirror equation: 1/s + 1/s’ = 2/R => 0 + 1/f = 2/R, so f = R/2 = 10 cm. VII. Mirrors

A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r  Exterior angle of a triangle:  1 =   =    VIII. Lenses

A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r  Snell’s Law: n 1 sin  1 =n 2 sin    VIII. Lenses

A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r  Tangents: tan  = r/(s +  ). tan  = r/(s’ -  ). tan  = r/(R -  ). VIII. Lenses

A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r  Small angle approximation: tan  ~  (  << 1). sin  ~  VIII. Lenses

A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r Rewrite Snell’s Law: n 1  1 ~ n 2  2, so  2 = (n 1 /n 2 )(  ). VIII. Lenses

A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r * Use exterior law: (n 1  n 2  ) = (n 2 - n 1 )  VIII. Lenses

A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r * Small angles: tan  ~  ~ r/s (  << s). tan  ~  ~ r/s’ (  <<s’). tan  ~  ~ r/R (  << R). VIII. Lenses

*Put it all together! n 1 /s + n 2 /s’ = (n 2 - n 1 )/R.(VIII.A.2) A.Refraction at a spherical surface 1.Images a)Object distance, Image distance, and Radius of curvature s n 1 < n 2 s’ 11 22 R    r VIII. Lenses

A.Refraction at a spherical surface 1.Images b)Magnification s n 1 < n 2 s’ 11 22 h’ tan  1 = h/s. tan  2 = -h’/s’. M = h’/h = -s’tan  2 /(stan  1 ). h VIII. Lenses

* Use Snell’s Law & small angle M = h’/h ~ -s’  2 /(s  1 ) = -n 1 s’/(n 2 s). (VIII.A.3) A.Refraction at a spherical surface 1.Images b)Magnification s n 1 < n 2 s’ 11 22 h’ h VIII. Lenses

3.Example: An insect is centrally embedded in a spherical globule of amber. The index of refraction for the amber is 2 and the diameter of the globule is 4 cm. How far from the surface does the insect appear? n 1 /s + n 2 /s’ = (n 2 -n 1 )/R; 2/(2 cm) + (1/s’) = (-1)1/(2 cm); 1/s’ = 1/(4 cm) - 1/(1 cm) = -3/4 cm -1. s’ = -4/3 = cm: virtual image VIII. Lenses Magnification: M = -n 1 s/n 2 s’ = -2*(-4/3)/1*2 = 4/3

B.Refraction at a flat surface 1. Let R => infinity. Sphere => plane n 1 /s = -n 2 /s’, or s’ = -(n 2 /n 1 )s.(VIII.B.1) n 1 > n 2. VIII. Lenses

B.Refraction at a flat surface 2.Example: A frog sits at the bottom of a reflecting pool. The pool is.5 m deep with n = 4/3. Where does the frog appear? s’ = -(n 2 /n 1 )s = -(1/[4/3])(0.5 m) = 3/8 m. n 1 > n 2. VIII. Lenses

C.Thin Lenses 2.Ray tracing: single lens VIII. Lenses

C.Thin Lenses 2.Ray tracing: double lens VIII. Lenses

C.Thin Lenses 6.Example: What is the image distance for a thin glass lens with a focal length of 4/3 cm and an object at 10 cm? 1/s’ =1/f - 1/s = 1/(4/3 cm) - 1/10cm =.65 cm -1. Thus, s’ = +1.5 cm. How is the image magnified? M = -s’/s = -1.5/10; M = -.15 VIII. Lenses

7.Example: What is the image distance and magnification for the following pair of lenses: Lens 1: R 1 = infinity, R 2 = -10 cm, n = 1.5 Lens 2: R 1 = 10 cm, R 2 = -10 cm, n = 1.5 The lenses are separated by 50 cm, and the object is at a distance of 45 cm from the first lens. Step 1: Find the focal lengths 1/f1 = (1/2)(0 - 1/(-10cm) => f1 = 20 cm. 1/f2 = (1/2)(1/10cm - 1/(-10cm)) => f2 = 10 cm. VIII. Lenses

7.Example:What is the image distance and magnification for the following pair of lenses: Lens 1: R 1 = infinity, R 2 = -10 cm, n = 1.5 Lens 2: R 1 = 10 cm, R 2 = -10 cm, n = 1.5 The lenses are separated by 50 cm, and the object is at a distance of 45 cm from the first lens. Step 2: Find image distance for lens 1: 1/s’ 1 = 1/f1 - 1/s 1 = 1/20cm - 1/45cm => s’ 1 = 36 cm. VIII. Lenses

7.Example:What is the image distance and magnification for the following pair of lenses: Lens 1: R 1 = infinity, R 2 = -10 cm, n = 1.5 Lens 2: R 1 = 10 cm, R 2 = -10 cm, n = 1.5 The lenses are separated by 50 cm, and the object is at a distance of 45 cm from the first lens. Step 3: Find image magnification for lens 1: M1 = -s’ 1 = -36 cm/45 cm = -0.8 VIII. Lenses

7.Example: What is the image distance and magnification for the following pair of lenses: Lens 1: R 1 = infinity, R 2 = -10 cm, n = 1.5 Lens 2: R 1 = 10 cm, R 2 = -10 cm, n = 1.5 Step 4: Find image distance for lens 2 using image 1 as object: 1/s’ 2 = 1/10 cm - 1/14 cm => s’ 2 = 35 cm. The image is to the right of the second lens. VIII. Lenses

7.Example:What is the image distance and magnification for the following pair of lenses: Lens 1: R 1 = infinity, R 2 = -10 cm, n = 1.5 Lens 2: R 1 = 10 cm, R 2 = -10 cm, n = 1.5 Step 5: Find total magnification M2 = -s’ 2 /s 2 = -35 cm/14 cm = Total magnification: M = M1* M2 = (-0.8)*(-2.5) = 2 VIII. Lenses