Pinhole Camera. Nuts and Bolts

Similar documents
Home Lab 3 Pinhole Viewer Box Continued and Measuring the Diameter of the Sun

Table of Contents DSM II. Lenses and Mirrors (Grades 5 6) Place your order by calling us toll-free

General Physics II. Optical Instruments

The telescope: basics

Human Retina. Sharp Spot: Fovea Blind Spot: Optic Nerve

The Optics of Mirrors

Chapter 25 Optical Instruments

Make a Refractor Telescope

Prac%ce Quiz 2. These are Q s from old quizzes. I do not guarantee that the Q s on this year s quiz will be the same, or even similar.

Kit Contents. The Power House experiment kit contains the following parts:

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

Light and Color Page 1 LIGHT AND COLOR Appendix

An object that refracts light. A from of energy that travels in waves and can be seen when it interacts with matter

Applications of Optics

Try to Recall GRADE VI LIGHT ENERGY. At the end of the module, you should be able to: Identify energy and its uses (light)

Directory of Home Labs, Materials List, and SOLs

Unit 3P.2:Shadows, mirrors and magnifiers

Astronomical Cameras

Lab 12. Optical Instruments

Basic principles of photography. David Capel 346B IST

Lab: Properties of Light

Phys 531 Lecture 9 30 September 2004 Ray Optics II. + 1 s i. = 1 f

Home Lab 2 Pinhole Viewer Box

Complete the diagram to show what happens to the rays. ... (1) What word can be used to describe this type of lens? ... (1)

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

Intermediate 2 Waves & Optics Past Paper questions

OPTICS LENSES AND TELESCOPES

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

Optics and Telescopes

The grade 6 English science unit, Lenses, meets the academic content standards set in the Korean curriculum, which state students should:

Intorduction to light sources, pinhole cameras, and lenses

Topic 1 - What is Light? 1. Radiation is the type of energy transfer which does not require... A matter B heat C waves D light

Optics Laboratory Spring Semester 2017 University of Portland

Chapter 8. The Telescope. 8.1 Purpose. 8.2 Introduction A Brief History of the Early Telescope

Lecture 4: Geometrical Optics 2. Optical Systems. Images and Pupils. Rays. Wavefronts. Aberrations. Outline

There is a range of distances over which objects will be in focus; this is called the depth of field of the lens. Objects closer or farther are

ECEN 4606, UNDERGRADUATE OPTICS LAB

Lecture Outline Chapter 27. Physics, 4 th Edition James S. Walker. Copyright 2010 Pearson Education, Inc.

O5: Lenses and the refractor telescope

Young Inventor s Toolkit Part One: Identification

Science Focus 8. Light and Optical Systems. Pop Quiz Master (5 questions) for each Topic A C B D C C B C C A D B C A B B C C A C A C D B A C B B C D

Grade 8. Light and Optics. Unit exam

Chapter 36. Image Formation

Image Formation by Lenses

Chapter 36. Image Formation

PINHOLES and TRIANGLES

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

INTRODUCTION THIN LENSES. Introduction. given by the paraxial refraction equation derived last lecture: Thin lenses (19.1) = 1. Double-lens systems

The Eye and Vision. Activities: Linda Shore, Ed.D. Exploratorium Teacher Institute Exploratorium, all rights reserved

Lesson Title: The Science of Light and Photography Subject Grade Level Timeline. Physical Science minutes. Objectives

THE TELESCOPE. PART 1: The Eye and Visual Acuity

Projection. Announcements. Müller-Lyer Illusion. Image formation. Readings Nalwa 2.1

Two Fundamental Properties of a Telescope

Pinhole Camera Workshop

DAVISART.COM PHONE FAX

FRAUNHOFER AND FRESNEL DIFFRACTION IN ONE DIMENSION

Table of Contents. Chapter x 2 Using Light. Chapter Preview. 2.1 Waves and the Electromagnetic Spectrum. 2.2 Visible Light and Color

Table of Contents. Light and Color

Unit 3: Energy On the Move

The New. Astronomy. 2 Practical Focusing

What Are The Basic Part Of A Film Camera

Lesson 7 Evolution and the eye

Vision 1. Physical Properties of Light. Overview of Topics. Light, Optics, & The Eye Chaudhuri, Chapter 8

30 Lenses. Lenses change the paths of light.

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

Use these words to complete the sentences about light: absorb different diffuse focus prism refraction same slower specula transmit

[ Summary. 3i = 1* 6i = 4J;

Eric B. Burgh University of Wisconsin. 1. Scope

Geometrical Optics Optical systems

Unit 1: Image Formation

A NEW H-ALPHA SOLAR LIMB-PATROL SYSTEM* George Carroll. Lockheed Solar Observatory, Lockheed-California Co. Burbank, California

Light. Path of Light. Looking at things. Depth and Distance. Getting light to imager. CS559 Lecture 2 Lights, Cameras, Eyes

Lecture PowerPoint. Chapter 25 Physics: Principles with Applications, 6 th edition Giancoli

The Hole Story. Fun with the Exploratorium business card Written by Stephanie Chasteen, and credited to the person who sent me the activity

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

Chapter 3 Op+cal Instrumenta+on

Life Science Chapter 2 Study Guide

1. The convex lens will magnify the print, provided the object is not placed beyond 2F, While the concave lens will shrink the print image.

Unit 6P.2: Light. What is Light? Shadows Reflection The colors of the rainbow. Science skills: Observing Classifying Predicting

12:40-2:40 3:00-4:00 PM

GRADE ONE SCIENCE KIT 1.P.2 PHYSICAL SCIENCE: EXPLORING LIGHT AND SHADOWS

Physics Learning Guide Name:

=, where f is focal length of a lens (positive for convex. Equations: Lens equation

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

Colorado School of Mines. Computer Vision. Professor William Hoff Dept of Electrical Engineering &Computer Science.

Feasibility and Design for the Simplex Electronic Telescope. Brian Dodson

The techniques covered so far -- visual focusing, and

Lens Aperture. South Pasadena High School Final Exam Study Guide- 1 st Semester Photo ½. Study Guide Topics that will be on the Final Exam

PHY 1160C Homework Chapter 26: Optical Instruments Ch 26: 2, 3, 5, 9, 13, 15, 20, 25, 27

"Internet Telescope" Performance Requirements

The eye & corrective lenses

Images painted by the Sun

The diffraction of light

End-of-Chapter Exercises

Lec. 13: Ch. 4 The Camera and Photography. Camera parts

Instructional Resources/Materials: Light vocabulary cards printed (class set) Enough for each student (See card sort below)

Person s Optics Test KEY SSSS

The Photo Lab Louis Abramson, Yeunjin Kim, & Nicole Fields

CAMERA BASICS. Stops of light

Cameras and Exposure

Transcription:

Nuts and Bolts What Students Will Do Build a specialized, Sun-measuring pinhole camera. Safely observe the Sun with the pinhole camera and record image size measurements. Calculate the diameter of the Sun from your measurements and a known distance to the Sun. Key Concepts Light rays tend to travel in straight lines. Light rays emitted or reflected by an object that pass through a small hole can project an image of the object on the other side. An image of an object can be used to determine the object s size or the distance to the object. The ability of the human eye s lens to focus an image on the retina is aided by the eye s pupil (the eye s aperture), which acts as a pinhole camera. Materials Needed Cardboard tube (the longer the better) Cardboard tube scraps Aluminum foil A sharp pin Tape Graph paper (with millimeter grid) Solar-B Touch the Sun, Chabot Space & Science Center 64

Introduction Description Solar-B will use mirrors, lenses, CCD cameras, and other optical components to form images of the Sun. From these images the sizes of objects and events on the Sun and the Sun s disk itself can be measured. You will measure the diameter of the Sun using aluminum foil, a cardboard tube, graph paper, and a pin! 0.5 degrees 0.5 Above: The disk of the Sun shown with a scale of angular separation on the sky. The Sun s disk is approximately one half degree across as seen from Earth. A pinhole camera is the world s simplest image-forming device. You may believe that the only way to take a picture is with an expensive set of lenses and other mechanical accessories. After all, human eyes and cameras and telescopes all use intricate optics to function as they do. Would you believe that a simple pinhole in a piece of foil or paper would do the trick! Light shining from an object (the Sun, the Moon, a traffic light, a person) through a small pinhole will form an image of the object on the other side, much as a camera s lens forms an image of an object on the sheet of film behind the lens. In this case, however, the pinhole serves as the lens. Solar-B Connection Solar-B Touch the Sun, Chabot Space & Science Center 65

An important part of the work to be done by Solar-B scientists will be the measuring of motion of the materials on the Sun. One of the main subjects of study will be how events and processes such as sunspots, solar magnetic fields, flares, prominences, and other dynamic solar features are born, develop, and dissipate. A complete picture of the life cycle of these events will be possible with the data collected by Solar-B. Cameras on Solar-B will take series of images of the Sun s surface, and the motion of materials and magnetic fields will be seen and measured through comparisons of the images. Solar-B Touch the Sun, Chabot Space & Science Center 66

Build It Step by Step : Assembly Diagram 1. Find and/or assemble the tube. The tube should be at least 30 inches long, but even longer is better. (Gift-wrap-paper cardboard tubes can be used, either in single lengths or taped together end-to-end.) 2. Near one end of the tube (half an inch or less from the end), cut out a hole. The hole should be large enough so that you can see most of the opening at the end of the tube from the inside. 3. Cut out a piece of lined graph paper (with a millimeter grid spacing, if possible) just large enough to fit in one end of the tube. 4. Tape the graph paper to cover the opening at the end of the tube the same end in which you cut the viewing hole. 5. Cut out a piece of aluminum foil just large enough to fit on the end of the tube opposite the graph paper. (Or you could cut out a larger piece that can be wrapped over the end of the tube, as shown in the diagram.) 6. Tape the foil to the end of the tube opposite the graph paper. Note: It is important that the foil be smooth, flat, and taut, like a drumhead. 7. Using a sharp point no bigger than that of a pin, poke a very small hole in the center of the aluminum foil. 8. Your pinhole camera is ready to use! Solar-B Touch the Sun, Chabot Space & Science Center 67

Observe Your pinhole camera has been designed specifically to measure the diameter of the Sun. Before you observe the Sun with it, repeat the following sentence one thousand times: I will not look directly at the Sun! It is very important that you do not look directly at the Sun, not with a telescope, not with a camera, not with a pair of binoculars, and not with your pinhole camera. The design of you pinhole camera makes it easy to measure the size of the Sun s image without being in danger of accidentally letting direct sunlight into your eyes. When you point the tube at the Sun and look into the viewer, you are looking away from the Sun, which is always the safest thing to do. Step by Step 1. Stand facing away from the Sun. 2. Lift the viewer hole to your eye and point the tube over your shoulder in the direction of the Sun. 3. Try to find the Sun s image on the graph paper, looking through the viewing hole. When your pinhole camera is pointed properly at the Sun, you will see a small spot of light on the graph paper. The size of the spot will depend on the length of your pinhole camera. If you have difficulty finding the Sun s image (which will be a small and possibly faint spot of light on the graph paper) there is a trick you can try: Look at the shadow that your pinhole camera tube casts on the ground and move the camera around until its shadow is as small as possible. When the tube is pointed directly at the Sun, its shadow will be at its smallest. 4. When you find the Sun s image, attempt to measure its size by counting the number of millimeter lines on the graph paper that it covers, from edge to edge (the image s diameter). Make as careful a measurement as you can. Solar-B Touch the Sun, Chabot Space & Science Center 68

If you have trouble reading the size of the Sun s image because you cannot hold the camera still enough, try resting the camera on some solid object (a table, a chair, a window sill). 5. Record all of your measurements on the Data Sheet. Solar-B Touch the Sun, Chabot Space & Science Center 69