Experiment 3: Reflection

Similar documents
OPAC103 GEOMETRICAL OPTICS LABORATORY MANUAL. Focal Length and Magnification of a Concave Mirror

Basic Optics System OS-8515C

Physics 197 Lab 7: Thin Lenses and Optics

Part 1 Investigating Snell s Law

Determination of Focal Length of A Converging Lens and Mirror

Optics Practice. Version #: 0. Name: Date: 07/01/2010

Geometric Optics. Ray Model. assume light travels in straight line uses rays to understand and predict reflection & refraction

E X P E R I M E N T 12

Physics II. Chapter 23. Spring 2018

PHYS 160 Astronomy. When analyzing light s behavior in a mirror or lens, it is helpful to use a technique called ray tracing.

AP Physics Problems -- Waves and Light

Activity 6.1 Image Formation from Spherical Mirrors

NORTHERN ILLINOIS UNIVERSITY PHYSICS DEPARTMENT. Physics 211 E&M and Quantum Physics Spring Lab #8: Thin Lenses

Laboratory 12: Image Formation by Lenses

28 Thin Lenses: Ray Tracing

P202/219 Laboratory IUPUI Physics Department THIN LENSES

Converging Lenses. Parallel rays are brought to a focus by a converging lens (one that is thicker in the center than it is at the edge).

Ch 24. Geometric Optics

Final Reg Optics Review SHORT ANSWER. Write the word or phrase that best completes each statement or answers the question.

Physics 222, October 25

Physics 1411 Telescopes Lab

Chapter 23. Mirrors and Lenses

Section 3 Curved Mirrors. Calculate distances and focal lengths using the mirror equation for concave and convex spherical mirrors.

WAVES: REFLECTION QUESTIONS

LAB 12 Reflection and Refraction

Notation for Mirrors and Lenses. Chapter 23. Types of Images for Mirrors and Lenses. More About Images

Algebra Based Physics. Reflection. Slide 1 / 66 Slide 2 / 66. Slide 3 / 66. Slide 4 / 66. Slide 5 / 66. Slide 6 / 66.

An image is being formed by a mirror with a spherical radius of R=+40cm. Draw mirror spherical surface curving to the right!

Spherical Mirrors. Concave Mirror, Notation. Spherical Aberration. Image Formed by a Concave Mirror. Image Formed by a Concave Mirror 4/11/2014

Physics 132: Lecture Fundamentals of Physics

Chapter 2 - Geometric Optics

mirrors and lenses PHY232 Remco Zegers Room W109 cyclotron building

Assignment X Light. Reflection and refraction of light. (a) Angle of incidence (b) Angle of reflection (c) principle axis

Gaussian Ray Tracing Technique

Geometric Optics. Objective: To study the basics of geometric optics and to observe the function of some simple and compound optical devices.

Physics 132: Lecture Fundamentals of Physics II

LECTURE 17 MIRRORS AND THIN LENS EQUATION

Laboratory 7: Properties of Lenses and Mirrors

Physics Worksheet. Topic -Light. Q1 If the radius of curvature of spherical mirror is 20 cm, what is its focal length.

2015 EdExcel A Level Physics EdExcel A Level Physics. Lenses

Chapter 23. Mirrors and Lenses

Algebra Based Physics. Reflection. Slide 1 / 66 Slide 2 / 66. Slide 3 / 66. Slide 4 / 66. Slide 5 / 66. Slide 6 / 66.

LO - Lab #05 - How are images formed from light?

LENSES. a. To study the nature of image formed by spherical lenses. b. To study the defects of spherical lenses.

Academic Year: 2017/2018 Term 3 Physics - Grade 10 Revision sheet Chapter 13: section 1,2,3 / Chapter 14: section 1 pages: ( ),( )

Chapter 36. Image Formation

Lenses. Optional Reading Stargazer: the life and times of the TELESCOPE, Fred Watson (Da Capo 2004).

Geometric Optics. PSI AP Physics 2. Multiple-Choice

Geometric Optics. This is a double-convex glass lens mounted in a wooden frame. We will use this as the eyepiece for our microscope.

Chapter 23. Mirrors and Lenses

Physics 132: Lecture Fundamentals of Physics II

King Saud University College of Science Physics & Astronomy Dept.

CH. 23 Mirrors and Lenses HW# 6, 7, 9, 11, 13, 21, 25, 31, 33, 35

Aberrations of a lens

Geometric Optics Practice Problems. Ray Tracing - Draw at least two principle rays and show the image created by the lens or mirror.

10.2 Images Formed by Lenses SUMMARY. Refraction in Lenses. Section 10.1 Questions

Chapter 23. Light Geometric Optics

Chapter 3 Mirrors. The most common and familiar optical device

Chapter 18 Optical Elements

Chapter 34. Images. Copyright 2014 John Wiley & Sons, Inc. All rights reserved.

O5: Lenses and the refractor telescope

Gaussian Ray Tracing Technique

CHAPTER 3LENSES. 1.1 Basics. Convex Lens. Concave Lens. 1 Introduction to convex and concave lenses. Shape: Shape: Symbol: Symbol:

Geometric Optics. Find the focal lengths of lenses and mirrors; Draw and understand ray diagrams; and Build a simple telescope

Supplementary Notes to. IIT JEE Physics. Topic-wise Complete Solutions

BHARATIYA VIDYA BHAVAN S V M PUBLIC SCHOOL, VADODARA QUESTION BANK

Condition Mirror Refractive Lens Concave Focal Length Positive Focal Length Negative. Image distance positive

Mirrors, Lenses &Imaging Systems

Station # 1. Reflection off of a rough surface. The Law of reflection. Problem: How is light reflected off of a flat smooth surface?

Lecture 19 (Geometric Optics I Plane and Spherical Optics) Physics Spring 2018 Douglas Fields

Mirrors and Lenses. Images can be formed by reflection from mirrors. Images can be formed by refraction through lenses.

Refraction is the when a ray changes mediums. Examples of mediums:

INDIAN SCHOOL MUSCAT SENIOR SECTION DEPARTMENT OF PHYSICS CLASS X REFLECTION AND REFRACTION OF LIGHT QUESTION BANK

Lab 11: Lenses and Ray Tracing

Name: Lab Partner: Section:

Preview. Light and Reflection Section 1. Section 1 Characteristics of Light. Section 2 Flat Mirrors. Section 3 Curved Mirrors

Reading: Lenses and Mirrors; Applications Key concepts: Focal points and lengths; real images; virtual images; magnification; angular magnification.

Physics 228 Lecture 3. Today: Spherical Mirrors Lenses.

PHYSICS 289 Experiment 8 Fall Geometric Optics II Thin Lenses

Chapter 23. Geometrical Optics: Mirrors and Lenses and other Instruments

Option G 2: Lenses. The diagram below shows the image of a square grid as produced by a lens that does not cause spherical aberration.

Image Formation. Light from distant things. Geometrical optics. Pinhole camera. Chapter 36

Light and Applications of Optics

Introduction. Strand F Unit 3: Optics. Learning Objectives. Introduction. At the end of this unit you should be able to;

9. THINK A concave mirror has a positive value of focal length.

Astronomy 80 B: Light. Lecture 9: curved mirrors, lenses, aberrations 29 April 2003 Jerry Nelson

Chapter 34 Geometric Optics

Chapter 29/30. Wave Fronts and Rays. Refraction of Sound. Dispersion in a Prism. Index of Refraction. Refraction and Lenses

EXPERIMENT 4 INVESTIGATIONS WITH MIRRORS AND LENSES 4.2 AIM 4.1 INTRODUCTION

Instructions. To run the slideshow:

LIGHT REFLECTION AND REFRACTION

PRINCIPLE PROCEDURE ACTIVITY. AIM To observe diffraction of light due to a thin slit.

Experiment 2 Simple Lenses. Introduction. Focal Lengths of Simple Lenses

REFLECTION THROUGH LENS

Focal Length of Lenses

5. Convex, Concave Lenses and the Lensmaker s Law

PHYSICS OPTICS. Mr Rishi Gopie

Using Mirrors to Form Images. Reflections of Reflections. Key Terms. Find Out ACTIVITY

GEOMETRICAL OPTICS Practical 1. Part I. BASIC ELEMENTS AND METHODS FOR CHARACTERIZATION OF OPTICAL SYSTEMS

Class-X Assignment (Chapter-10) Light-Reflection & Refraction

Transcription:

Model No. OS-8515C Experiment 3: Reflection Experiment 3: Reflection Required Equipment from Basic Optics System Light Source Mirror from Ray Optics Kit Other Required Equipment Drawing compass Protractor Metric ruler White paper Purpose In this experiment, you will study how rays are reflected from different types of mirrors. You will measure the focal length and determine the radius of curvature of a concave mirror and a convex mirror. Part 1: Plane Mirror 1. Place the light source in ray-box mode on a blank sheet of white paper. Turn the wheel to select a single ray. 2. Place the mirror on the paper. Position the plane (flat) surface of the mirror in the path of the incident ray at an angle that allows you to clearly see the incident and reflected rays. 3. On the paper, trace and label the surface of the plane mirror and the incident and reflected rays. Indicate the incoming and the outgoing rays with arrows in the appropriate directions. 4. Remove the light source and mirror from the paper. On the paper, draw the normal to the surface (as in Figure 3.1). Normal to surface Incident ray Reflected ray Figure 3.1 5. Measure the angle of incidence and the angle of reflection. Measure these angles from the normal. Record the angles in the first row Table 3.1. 6. Repeat steps 1 5 with a different angle of incidence. Repeat the procedure again to complete Table 3.1 with three different angles of incidence. Table 3.1: Plane Mirror Results Angle of Incidence Angle of Reflection 7. Turn the wheel on the light source to select the three primary color rays. Shine the colored rays at an angle to the plane mirror. Mark the position of the surface of the plane mirror and trace the incident and reflected rays. Indicate the colors of 13

Basic Optics System Experiment 3: Reflection the incoming and the outgoing rays and mark them with arrows in the appropriate directions. Questions 1. What is the relationship between the angles of incidence and reflection? 2. Are the three colored rays reversed left-to-right by the plane mirror? Part 2: Cylindrical Mirrors Theory A concave cylindrical mirror focuses incoming parallel rays at its focal point. The focal length ( f ) is the distance from the focal point to the center of the mirror surface. The radius of curvature (R) of the mirror is twice the focal length. See Figure 3.2. R focal point f mirror 1. Turn the wheel on the light source to select five parallel rays. Shine the rays straight into the concave mirror so that the light is reflected back toward the ray box (see Figure 3.3). Trace the surface of the mirror and the incident and reflected rays. Indicate the incoming and the outgoing rays with arrows in the appropriate directions. (You can now remove the light source and mirror from the paper.) Figure 3.2 2. The place where the five reflected rays cross each other is the focal point of the mirror. Mark the focal point. Incident rays 3. Measure the focal length from the center of the concave mirror surface (where the middle ray hit the mirror) to the focal point. Record the result in Table 3.2. 4. Use a compass to draw a circle that matches the curvature of the mirror (you will have to make several tries with the compass set to different widths before you find the right one). Measure the radius of curvature and record it in Table 3.2. Figure 3.3 5. Repeat steps 1 4 for the convex mirror. Note that in step 3, the reflected rays will diverge, and they will not cross. Use a ruler to extend the reflected rays back behind the mirror s surface. The focal point is where these extended rays cross. Table 3.2: Cylindrical Mirror Results Concave Mirror Convex Mirror Focal Length Radius of Curvature (determined using compass) Questions 1. What is the relationship between the focal length of a cylindrical mirror and its radius of curvature? Do your results confirm your answer? 2. What is the radius of curvature of a plane mirror? 14

Model No. OS-8515C Experiment 13: Focal Length and Magnification of a Concave Mirror Experiment 13: Focal Length and Magnification of a Concave Mirror Required Equipment from Basic Optics System Light Source Bench Concave/convex Mirror Half-screen Other Equipment Metric ruler Optics Caliper (optional, for measuring image sizes), PASCO part OS-8468 Purpose The purpose of this experiment is to determine the focal length of a concave mirror and to measure the magnification for a certain combination of object and image distances. Theory For a spherically curved mirror: (eq. 13.1) 1 -- f = 1 1 ---- + --- d o d i where f is focal length, d o is the distance between the object and the mirror, and d i is the distance between the image and the mirror. By measuring d o and d i the focal length can be determined. Magnification, M, is the ratio of image size to object size. If the image is inverted, M is negative. Part I: Object at Infinity In this part, you will determine the focal length of the mirror by making a single measurement of d i with d o. Half-screen Distant Object 1. Hold the mirror in one hand and the half-screen in the other hand. Use the concave side of the mirror to focus the image of a distant bright object (such as a window or lamp across the room) on the half-screen. (See Figure 13.1.) Image Mirror 2. Have your partner measure the distance from the mirror to the screen. This is the image distance, d i. Analysis d i = 1. As d o approaches infinity, what does 1/d o approach? Figure 13.1 37

Basic Optics System Experiment 13: Focal Length and Magnification of a Concave Mirror 2. Use the Equation 13.1 to calculate the focal length. f = Part II: Object Closer Than Infinity In this part, you will determine the focal length of the mirror by measuring several pairs of object and image distances and plotting 1/d o versus 1/d i. 50cm Light source Half-screen Mirror Figure 13.2 1. Place the light source and the mirror on the optics bench 50 cm apart with the light source s crossed-arrow object toward the mirror and the concave side of the mirror toward the light source. Place the half-screen between them (see Figure 13.2). 2. Slide the half-screen to a position where a clear image of the crossed-arrow object is formed. Measure the image distance and the object distance. Record these measurements (and all measurements from the following steps) in Table 13.1. 3. Repeat step 2 with object distances of 45 cm, 40 cm, 35 cm, 30 cm, 25 cm. 4. With the mirror at 25 cm from the light source and a clear image formed on the half-screen, measure the object size and image size. To measure the image size, hold a small scrap of paper against the half-screen and mark two opposite points on the crossed-arrow pattern (see Figure 13.3). If at least half of the pattern is not visible on the screen, have your partner slightly twist the mirror to bring more of the image into view. Remove the paper and measure between the points. Measure the object size between the corresponding points directly on the light source. Figure 13.3 Image size Table 13.1: Image and Object Distances d o d i 1/d o 1/d i Image Size Object Size 50.0 cm 45.0 cm 40.0 cm 35.0 cm 30.0 cm 25.0 cm 38

Model No. OS-8515C Experiment 13: Focal Length and Magnification of a Concave Mirror Analysis Part A: Focal Length 1. Calculate 1/d o and 1/d i for all six rows in Table 13.1. 2. Plot 1/d o versus 1/d i and find the best-fit line (linear fit). This will give a straight line with the x- and y-intercepts equal to 1/f. Record the intercepts (including units) here: y-intercept = 1/f = x-intercept = 1/f = Note: You can plot the data and find the best-fit line on paper or on a computer. 3. For each intercept, calculate a value of f and record it in Table 13.2. 4. Find the percent difference between these two values of f and record them in Table 13.2. 5. Average these two values of f. Find the percent difference between this average and the focal length that you found in Part I. Record these data in Table 13.2. Table 13.2: Focal Length f Result from x-intercept Result from y-intercept % difference between results from intercepts Average of results from intercepts Result from Part I % difference between Average of results from intercepts and result from Part I Analysis Part B: Magnification 1. For the last data point only (d o = 25 cm), use the image and object distances to calculate the magnification, M. Record the results in Table 13.3. (eq. 13.2) M = d i ---- d o 2. Calculate the absolute value of M using your measurements of the image size and object size. Record the results in Table 13.3. (eq. 13.3) M = image ------------------------ size object size 39

Basic Optics System Experiment 13: Focal Length and Magnification of a Concave Mirror 3. Calculate the percent differences between the absolute values of M found using the two methods. Record the results in Table 13.3. Table 13.3: Magnification M calculated from image and object distances M calculated from image and object sizes % difference Questions 1. Is the image formed by the mirror upright or inverted? 2. Is the image real or virtual? How do you know? 3. By looking at the image, how can you tell that the magnification is negative? 4. You made three separate determinations of f (by measuring it directly with a distant object, from the x-intercept of your graph, and from the y-intercept). Where these three values equal? If they were not, what might account for the variation? 40