10/25/2017. Light and Telescope. Reflector - Mirror. Refractor - Lens. PHYS 1411 Introduction to Astronomy. Topics for Today s class
|
|
- Barbra Sims
- 6 years ago
- Views:
Transcription
1 PHYS 1411 Introduction to Astronomy Light and Telescope Chapter 6 Reminders Homework on Chapter 4, 5 and 6 due November 1 st. No extensions. Lab 8 handout is on class web page. Due Week of November 27 th. Exam 2 Wednesday November 1 st. Chapters 4, 5 and 6 50 multiple choice questions Allowed: Calculator, One page of equations, formula, conversions or constants. Bring Green Scantron, No. 2 Pencil Not allowed: cell phones, ear phones, laptops, tablets. Review/Practice Questions are on Class Web Page. Topics for Today s class Optical Telescopes Big Telescopes Advances in Telescope Designs Telescopes Mountings Problems with Mirrors and Lenses Astronomical Detectors CCD Camera Spectrometer Hobby Telescopes Eyepiece Modern Optical Telescopes Schnmidt - Cassegrain Focus Cassegrain Focus Prime Focus Refractor - Lens Jtwastronomy.com Reflector - Mirror Astroshop.eu 1
2 Modern Optical Telescopes (cont d.) The 4-m Mayall Telescope at Kitt Peak National Observatory (Arizona) Advances in Modern Telescope Design Lighter mirrors with lighter support structures, to be controlled dynamically by computers Floppy mirror Segmented mirror Examples of Modern Telescopic Design Examples of Modern Telescopic Design (cont d.) Funding Federal Government (DOE FIPSE) Tarleton State University Manufacturer Astronomical Consultant and Equipment Inc.(ACE) 32-inch (0.8m) Reflector f/ratio= f/7 Remotely Control ACE Software * Observatory CCD Camera Finger Lakes - FOV = 17 x 17 Resolution /pixel Imaging and Photometry UBVRI, Hα, OIII and Neutral Density 2
3 Telescopes Mounts Telescope require mounts that allow rotation Popular Equatorial Mount No counterweight needed counterweight GeekWrapped.com Starizona.com Comparing Refracting Telescopes telescopes/telescope10.html LGP ~ A = (D/2) 2 M = F p /F e min = 11.6 arcsec / D[cm] Lenses and Mirrors have Inherent Problems Correcting for Spherical Aberration Spherical Aberration Both Lenses and Mirrors Chromatic Aberration Found in Lenses Openphotography.com Researchgate.net amazingspace.com Phys.apps.org Amazing-space.stsci.edu 3
4 Example of Spherical Aberration Disadvantage of Refractors Before After Tube very long for big telescope Lenses are expensive compared to mirrors More Engineering Maintenance Alt-Az mounting not Suitable Image not remarkably better than mirrors Chromatic Aberration Clspectrum.com Correcting for Chromatic Aberration Example of Chromatic Aberration Chromatic aberration: Different wavelengths are focused at different focal lengths (prism effect). Can be corrected, but not eliminated by second lens out of different material. Difficult and expensive to produce: All surfaces must be perfectly shaped; glass must be flawless; lens can only be Cengage Learning supported 2016 at the edges Vimeo.com Astronomical Detectors How to Measure and Record Light The Eye Limited ability The Photographic plate now obsolete Photomultiplier Very limited in capability The CCD (Charge Couple Device) Making Digital Image The Spectrograph Making a Spectrum - Measuring; Chemical Composition Temperature Velocity 4
5 CCD Camera Makes Digital Images How does a CCD work? It is a imaging device A CCD Image and Pixel Values Astrophotography Mathworks.com NASA Science from multiple wavelength CCD Images Science from a CCD Image Analyzing a sequence of such image gives us this light curve NASA Brightskies.us 5
6 Spectrographs/Spectrometer Spectrographs/Spectrometer A CCD spectrometer has a CCD camera and a Spectrometer A CCD image shows the spectrum It is an instrument that allows us to see to colors of white light coming from a star or a hot source Analysis of a Spectrum tells us chemical composition and temperature How to make a simple spectrometer Spectra of Some Astronomical Objects Popularmechanics.com Spectra of Chemical Elements Spectra can give us velocity information 6
7 Acknowledgment The slides in this lecture is for Tarleton: PHYS1411/PHYS1403 class use only Images and text material have been borrowed from various sources with appropriate citations in the slides, including PowerPoint slides from Seeds/Backman text that has been adopted for class. 7
Two Fundamental Properties of a Telescope
Two Fundamental Properties of a Telescope 1. Angular Resolution smallest angle which can be seen = 1.22 / D 2. Light-Collecting Area The telescope is a photon bucket A = (D/2)2 D A Parts of the Human Eye
More informationThe Imaging Chain in Optical Astronomy
The Imaging Chain in Optical Astronomy Review and Overview Imaging Chain includes these elements: 1. energy source 2. object 3. collector 4. detector (or sensor) 5. processor 6. display 7. analysis 8.
More informationThe Imaging Chain in Optical Astronomy
The Imaging Chain in Optical Astronomy 1 Review and Overview Imaging Chain includes these elements: 1. energy source 2. object 3. collector 4. detector (or sensor) 5. processor 6. display 7. analysis 8.
More informationLecture PowerPoint. Chapter 25 Physics: Principles with Applications, 6 th edition Giancoli
Lecture PowerPoint Chapter 25 Physics: Principles with Applications, 6 th edition Giancoli 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the
More informationLecture 15 Chap. 6 Optical Instruments. Single lens instruments Eyeglasses Magnifying glass. Two lens Telescope & binoculars Microscope
Lecture 15 Chap. 6 Optical Instruments Single lens instruments Eyeglasses Magnifying glass Two lens Telescope & binoculars Microscope The projector Projection lens Field lens October 12, 2010 all these
More informationPhysics 1411 Telescopes Lab
Name: Section: Partners: Physics 1411 Telescopes Lab Refracting and Reflecting telescopes are the two most common types of telescopes you will find. Each of these can be mounted on either an equatorial
More informationReflectors vs. Refractors
1 Telescope Types - Telescopes collect and concentrate light (which can then be magnified, dispersed as a spectrum, etc). - In the end it is the collecting area that counts. - There are two primary telescope
More informationOptics and Telescopes
Optics and Telescopes Properties of Light Law of Reflection - reflection Angle of Incidence = Angle of Law of Refraction - Light beam is bent towards the normal when passing into a medium of higher Index
More informationObservational Astronomy
Observational Astronomy Instruments The telescope- instruments combination forms a tightly coupled system: Telescope = collecting photons and forming an image Instruments = registering and analyzing the
More informationFeasibility and Design for the Simplex Electronic Telescope. Brian Dodson
Feasibility and Design for the Simplex Electronic Telescope Brian Dodson Charge: A feasibility check and design hints are wanted for the proposed Simplex Electronic Telescope (SET). The telescope is based
More informationGeneral Physics Experiment 5 Optical Instruments: Simple Magnifier, Microscope, and Newtonian Telescope
General Physics Experiment 5 Optical Instruments: Simple Magnifier, Microscope, and Newtonian Telescope Objective: < To observe the magnifying properties of the simple magnifier, the microscope and the
More informationUniversity of Rochester Department of Physics and Astronomy Physics123, Spring Homework 5 - Solutions
Problem 5. University of Rochester Department of Physics and Astronomy Physics23, Spring 202 Homework 5 - Solutions An optometrist finds that a farsighted person has a near point at 25 cm. a) If the eye
More informationChapter 25. Optical Instruments
Chapter 25 Optical Instruments Optical Instruments Analysis generally involves the laws of reflection and refraction Analysis uses the procedures of geometric optics To explain certain phenomena, the wave
More informationPHYSICS. Chapter 35 Lecture FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E RANDALL D. KNIGHT
PHYSICS FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E Chapter 35 Lecture RANDALL D. KNIGHT Chapter 35 Optical Instruments IN THIS CHAPTER, you will learn about some common optical instruments and
More informationGetting started with Digital Astrophotography - Part I Rodger King - May 2016
Getting started with Digital Astrophotography - Part I Rodger King - May 2016 Flame Nebula orsehead Nebula. Question Astronomy Which type of Telescope is better - A Lens or Mirror? 500-900 More compact
More informationLecture Outline Chapter 27. Physics, 4 th Edition James S. Walker. Copyright 2010 Pearson Education, Inc.
Lecture Outline Chapter 27 Physics, 4 th Edition James S. Walker Chapter 27 Optical Instruments Units of Chapter 27 The Human Eye and the Camera Lenses in Combination and Corrective Optics The Magnifying
More informationConsumer digital CCD cameras
CAMERAS Consumer digital CCD cameras Leica RC-30 Aerial Cameras Zeiss RMK Zeiss RMK in aircraft Vexcel UltraCam Digital (note multiple apertures Lenses for Leica RC-30. Many elements needed to minimize
More informationApplications of Optics
Nicholas J. Giordano www.cengage.com/physics/giordano Chapter 26 Applications of Optics Marilyn Akins, PhD Broome Community College Applications of Optics Many devices are based on the principles of optics
More informationAstronomical Cameras
Astronomical Cameras I. The Pinhole Camera Pinhole Camera (or Camera Obscura) Whenever light passes through a small hole or aperture it creates an image opposite the hole This is an effect wherever apertures
More informationPhys 2310 Mon. Oct. 16, 2017 Today s Topics. Finish Chapter 34: Geometric Optics Homework this Week
Phys 2310 Mon. Oct. 16, 2017 Today s Topics Finish Chapter 34: Geometric Optics Homework this Week 1 Homework this Week (HW #10) Homework this week due Mon., Oct. 23: Chapter 34: #47, 57, 59, 60, 61, 62,
More informationTelescopes and their configurations. Quick review at the GO level
Telescopes and their configurations Quick review at the GO level Refraction & Reflection Light travels slower in denser material Speed depends on wavelength Image Formation real Focal Length (f) : Distance
More informationGeometric optics & aberrations
Geometric optics & aberrations Department of Astrophysical Sciences University AST 542 http://www.northerneye.co.uk/ Outline Introduction: Optics in astronomy Basics of geometric optics Paraxial approximation
More informationEE119 Introduction to Optical Engineering Spring 2002 Final Exam. Name:
EE119 Introduction to Optical Engineering Spring 2002 Final Exam Name: SID: CLOSED BOOK. FOUR 8 1/2 X 11 SHEETS OF NOTES, AND SCIENTIFIC POCKET CALCULATOR PERMITTED. TIME ALLOTTED: 180 MINUTES Fundamental
More informationCH. 23 Mirrors and Lenses HW# 6, 7, 9, 11, 13, 21, 25, 31, 33, 35
CH. 23 Mirrors and Lenses HW# 6, 7, 9, 11, 13, 21, 25, 31, 33, 35 Mirrors Rays of light reflect off of mirrors, and where the reflected rays either intersect or appear to originate from, will be the location
More informationInstructor: Doc. Ivan Kassamakov, Assistant: Kalle Hanhijärvi, Doctoral student
Instructor: Doc. Ivan Kassamakov, Assistant: Kalle Hanhijärvi, Doctoral student Course webpage: http://electronics.physics.helsinki.fi/teaching/optics-2014 Gaussian Optics Errors Taylor series 3 θ sin
More informationPHYS 202 OUTLINE FOR PART III LIGHT & OPTICS
PHYS 202 OUTLINE FOR PART III LIGHT & OPTICS Electromagnetic Waves A. Electromagnetic waves S-23,24 1. speed of waves = 1/( o o ) ½ = 3 x 10 8 m/s = c 2. waves and frequency: the spectrum (a) radio red
More informationPHY170: OPTICS. Things to do in the lab INTRODUCTORY REMARKS OPTICS SIMULATIONS
INTRODUCTORY REMARKS PHY170: OPTICS The optics experiments consist of two major parts. Setting up various components and performing the experiments described below. Computer simulation of images generated
More informationLecture 5. Telescopes (part II) and Detectors
Lecture 5 Telescopes (part II) and Detectors Please take a moment to remember the crew of STS-107, the space shuttle Columbia, as well as their families. Crew of the Space Shuttle Columbia Lost February
More informationLast time: Built a telescope (1 each!)
Last time: Built a telescope (1 each!) 1. Got parts: TWO lenses, cardboard tubes, two red caps, foam, little tube, white paper disk. 2. Assembled the parts into a useful optical instrument, a telescope!
More informationPhy Ph s y 102 Lecture Lectur 21 Optical instruments 1
Phys 102 Lecture 21 Optical instruments 1 Today we will... Learn how combinations of lenses form images Thin lens equation & magnification Learn about the compound microscope Eyepiece & objective Total
More informationLenses. A transparent object used to change the path of light Examples: Human eye Eye glasses Camera Microscope Telescope
SNC2D Lenses A transparent object used to change the path of light Examples: Human eye Eye glasses Camera Microscope Telescope Reading stones used by monks, nuns, and scholars ~1000 C.E. Lenses THERE ARE
More informationUNCOMPLICATED ASTROPHOTOGRAPHY. Bill Weaver
UNCOMPLICATED ASTROPHOTOGRAPHY Bill Weaver WHAT CAN YOU REALLY SEE & CAPTURE? Star Party Marvel OVERVIEW OF PHOTOGRAPHIC DEVICES Discuss and display fundamental equipment, techniques & factors for simple
More informationGRADE 11-LESSON 2 PHENOMENA RELATED TO OPTICS
REFLECTION OF LIGHT GRADE 11-LESSON 2 PHENOMENA RELATED TO OPTICS 1.i. What is reflection of light?.. ii. What are the laws of reflection? a...... b.... iii. Consider the diagram at the right. Which one
More informationPerson s Optics Test KEY SSSS
Person s Optics Test KEY SSSS 2017-18 Competitors Names: School Name: All questions are worth one point unless otherwise stated. Show ALL WORK or you may not receive credit. Include correct units whenever
More informationPhys 102 Lecture 21 Optical instruments
Phys 102 Lecture 21 Optical instruments 1 Today we will... Learn how combinations of lenses form images Thin lens equation & magnification Learn about the compound microscope Eyepiece & objective Total
More information12:40-2:40 3:00-4:00 PM
Physics 294H l Professor: Joey Huston l email:huston@msu.edu l office: BPS3230 l Homework will be with Mastering Physics (and an average of 1 hand-written problem per week) Help-room hours: 12:40-2:40
More informationAverage: Standard Deviation: Max: 99 Min: 40
1 st Midterm Exam Average: 83.1 Standard Deviation: 12.0 Max: 99 Min: 40 Please contact me to fix an appointment, if you took less than 65. Chapter 33 Lenses and Op/cal Instruments Units of Chapter 33
More informationAstro 500 A500/L-8! 1!
Astro 500 1! Optics! Review! Compound systems: Outline o Pupils, stops, and telecentricity Telescopes! Review! Two-mirror systems! Figures of merit Examples: WIYN & SALT 2! Review: The Thin Lens! s parallel
More informationPHYS 1020 LAB 7: LENSES AND OPTICS. Pre-Lab
PHYS 1020 LAB 7: LENSES AND OPTICS Note: Print and complete the separate pre-lab assignment BEFORE the lab. Hand it in at the start of the lab. Pre-Lab Start by reading the entire prelab and lab write-up.
More informationTOPICS Recap of PHYS110-1 lecture Physical Optics - 4 lectures EM spectrum and colour Light sources Interference and diffraction Polarization
TOPICS Recap of PHYS110-1 lecture Physical Optics - 4 lectures EM spectrum and colour Light sources Interference and diffraction Polarization Lens Aberrations - 3 lectures Spherical aberrations Coma, astigmatism,
More informationThere 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
Chapter 25 Optical Instruments Some Topics in Chapter 25 Cameras The Human Eye; Corrective Lenses Magnifying Glass Telescopes Compound Microscope Aberrations of Lenses and Mirrors Limits of Resolution
More informationWaves & Oscillations
Physics 42200 Waves & Oscillations Lecture 33 Geometric Optics Spring 2013 Semester Matthew Jones Aberrations We have continued to make approximations: Paraxial rays Spherical lenses Index of refraction
More informationPhysics II. Chapter 23. Spring 2018
Physics II Chapter 23 Spring 2018 IMPORTANT: Except for multiple-choice questions, you will receive no credit if you show only an answer, even if the answer is correct. Always show in the space on your
More informationLecture 2: Geometrical Optics. Geometrical Approximation. Lenses. Mirrors. Optical Systems. Images and Pupils. Aberrations.
Lecture 2: Geometrical Optics Outline 1 Geometrical Approximation 2 Lenses 3 Mirrors 4 Optical Systems 5 Images and Pupils 6 Aberrations Christoph U. Keller, Leiden Observatory, keller@strw.leidenuniv.nl
More informationAberrations of a lens
Aberrations of a lens 1. What are aberrations? A lens made of a uniform glass with spherical surfaces cannot form perfect images. Spherical aberration is a prominent image defect for a point source on
More informationChapter 28. Reflection and Refraction
Chapter 28 Reflection and Refraction Light takes the path from one point to another that is a. quickest. b. shortest. c. closest to a straight line. d. None of these. Light takes the path from one point
More informationChapter 36. Image Formation
Chapter 36 Image Formation Image of Formation Images can result when light rays encounter flat or curved surfaces between two media. Images can be formed either by reflection or refraction due to these
More informationPhys 531 Lecture 9 30 September 2004 Ray Optics II. + 1 s i. = 1 f
Phys 531 Lecture 9 30 September 2004 Ray Optics II Last time, developed idea of ray optics approximation to wave theory Introduced paraxial approximation: rays with θ 1 Will continue to use Started disussing
More informationVery short introduction to light microscopy and digital imaging
Very short introduction to light microscopy and digital imaging Hernan G. Garcia August 1, 2005 1 Light Microscopy Basics In this section we will briefly describe the basic principles of operation and
More informationGeometrical Optics Optical systems
Phys 322 Lecture 16 Chapter 5 Geometrical Optics Optical systems Magnifying glass Purpose: enlarge a nearby object by increasing its image size on retina Requirements: Image should not be inverted Image
More informationLecture 2: Geometrical Optics. Geometrical Approximation. Lenses. Mirrors. Optical Systems. Images and Pupils. Aberrations.
Lecture 2: Geometrical Optics Outline 1 Geometrical Approximation 2 Lenses 3 Mirrors 4 Optical Systems 5 Images and Pupils 6 Aberrations Christoph U. Keller, Leiden Observatory, keller@strw.leidenuniv.nl
More informationOption G 2: Lenses. The diagram below shows the image of a square grid as produced by a lens that does not cause spherical aberration.
Name: Date: Option G 2: Lenses 1. This question is about spherical aberration. The diagram below shows the image of a square grid as produced by a lens that does not cause spherical aberration. In the
More informationPhysics 1202: Lecture 19 Today s Agenda
Physics 1202: Lecture 19 Today s Agenda Announcements: Team problems today Team 12: Kervell Baird, Matthew George, Derek Schultz Team 13: Paxton Stowik, Stacey Ann Burke Team 14: Gregory Desautels, Benjamin
More informationLecture 21. Physics 1202: Lecture 21 Today s Agenda
Physics 1202: Lecture 21 Today s Agenda Announcements: Team problems today Team 14: Gregory Desautels, Benjamin Hallisey, Kyle Mcginnis Team 15: Austin Dion, Nicholas Gandza, Paul Macgillis-Falcon Homework
More information"Internet Telescope" Performance Requirements
"Internet Telescope" Performance Requirements by Dr. Frank Melsheimer DFM Engineering, Inc. 1035 Delaware Avenue Longmont, Colorado 80501 phone 303-678-8143 fax 303-772-9411 www.dfmengineering.com Table
More informationChapter 23. Geometrical Optics: Mirrors and Lenses and other Instruments
Chapter 23 Geometrical Optics: Mirrors and Lenses and other Instruments HITT 1 You stand two feet away from a plane mirror. How far is it from you to your image? a. 2.0 ft b. 3.0 ft c. 4.0 ft d. 5.0 ft
More informationCHARA Collaboration Review New York 2007 CHARA Telescope Alignment
CHARA Telescope Alignment By Laszlo Sturmann Mersenne (Cassegrain type) Telescope M2 140 mm R= 625 mm k = -1 M1/M2 provides an afocal optical system 1 m input beam and 0.125 m collimated output beam Aplanatic
More informationChapter 18 Optical Elements
Chapter 18 Optical Elements GOALS When you have mastered the content of this chapter, you will be able to achieve the following goals: Definitions Define each of the following terms and use it in an operational
More informationClassical Optical Solutions
Petzval Lens Enter Petzval, a Hungarian mathematician. To pursue a prize being offered for the development of a wide-field fast lens system he enlisted Hungarian army members seeing a distraction from
More informationG1 THE NATURE OF EM WAVES AND LIGHT SOURCES
G1 THE NATURE OF EM WAVES AND LIGHT SOURCES G2 OPTICAL INSTRUMENTS HW/Study Packet Required: READ Tsokos, pp 598-620 SL/HL Supplemental: Hamper, pp 411-450 DO Questions p 605 #1,3 pp 621-623 #6,8,15,18,19,24,26
More informationAstrophotography Basics
Astrophotography Basics Cameras, Acquisition, and Processing John Carter April, 2018 Art, Science, Hobby Astrophotography ingredients. The focus of astrophotography can be as an art form, or it can be
More informationPHYSICS OPTICS. Mr Rishi Gopie
OPTICS Mr Rishi Gopie Ray Optics II Images formed by lens maybe real or virtual and may have different characteristics and locations that depend on: i) The type of lens involved, whether converging or
More informationDr. Todd Satogata (ODU/Jefferson Lab) Monday, April
University Physics 227N/232N Mirrors and Lenses Homework Optics 2 due Friday AM Quiz Friday Optional review session next Monday (Apr 28) Bring Homework Notebooks to Final for Grading Dr. Todd Satogata
More informationGemini 8m Telescopes Instrument Science Requirements. R. McGonegal Controls Group. January 27, 1996
GEMINI 8-M Telescopes Project Gemini 8m Telescopes Instrument Science Requirements R. McGonegal Controls Group January 27, 1996 GEMINI PROJECT OFFICE 950 N. Cherry Ave. Tucson, Arizona 85719 Phone: (520)
More information25 cm. 60 cm. 50 cm. 40 cm.
Geometrical Optics 7. The image formed by a plane mirror is: (a) Real. (b) Virtual. (c) Erect and of equal size. (d) Laterally inverted. (e) B, c, and d. (f) A, b and c. 8. A real image is that: (a) Which
More informationUseful Optics Information
Massachusetts Institute of Technology Department of Earth, Atmospheric, and Planetary Sciences 12.409 Observing Stars and Planets, Spring 2002 Handout 7 week of February 25, 2002 Copyright 1999 Created
More informationEarly Telescopes & Geometrical Optics. C. A. Griffith, Class Notes, PTYS 521, 2016 Not for distribution.
Early Telescopes & Geometrical Optics C. A. Griffith, Class Notes, PTYS 521, 2016 Not for distribution. 1 1.2. Image Formation Fig. 1. Snell s law indicates the bending of light at the interface of two
More informationChapter 36. Image Formation
Chapter 36 Image Formation Notation for Mirrors and Lenses The object distance is the distance from the object to the mirror or lens Denoted by p The image distance is the distance from the image to the
More informationPhysics 1C. Lecture 25B
Physics 1C Lecture 25B "More than 50 years ago, Austrian researcher Ivo Kohler gave people goggles thats severely distorted their vision: The lenses turned the world upside down. After several weeks, subjects
More informationTelescope Basics by Keith Beadman
Telescope Basics 2009 by Keith Beadman Table of Contents Introduction...1 The Basics...2 What a telescope is...2 Aperture size...3 Focal length...4 Focal ratio...5 Magnification...6 Introduction In the
More informationECEN 4606, UNDERGRADUATE OPTICS LAB
ECEN 4606, UNDERGRADUATE OPTICS LAB Lab 2: Imaging 1 the Telescope Original Version: Prof. McLeod SUMMARY: In this lab you will become familiar with the use of one or more lenses to create images of distant
More informationChapter 23. Light Geometric Optics
Chapter 23. Light Geometric Optics There are 3 basic ways to gather light and focus it to make an image. Pinhole - Simple geometry Mirror - Reflection Lens - Refraction Pinhole Camera Image Formation (the
More informationGEOMETRICAL OPTICS AND OPTICAL DESIGN
GEOMETRICAL OPTICS AND OPTICAL DESIGN Pantazis Mouroulis Associate Professor Center for Imaging Science Rochester Institute of Technology John Macdonald Senior Lecturer Physics Department University of
More informationc v n = n r Sin n c = n i Refraction of Light Index of Refraction Snell s Law or Refraction Example Problem Total Internal Reflection Optics
Refraction is the bending of the path of a light wave as it passes from one material into another material. Refraction occurs at the boundary and is caused by a change in the speed of the light wave upon
More informationChapter 23. Mirrors and Lenses
Chapter 23 Mirrors and Lenses Mirrors and Lenses The development of mirrors and lenses aided the progress of science. It led to the microscopes and telescopes. Allowed the study of objects from microbes
More informationSpectroscopy in the UV and Visible: Instrumentation. Spectroscopy in the UV and Visible: Instrumentation
Spectroscopy in the UV and Visible: Instrumentation Typical UV-VIS instrument 1 Source - Disperser Sample (Blank) Detector Readout Monitor the relative response of the sample signal to the blank Transmittance
More informationChapter 34: Geometrical Optics (Part 2)
Chapter 34: Geometrical Optics (Part 2) Brief review Optical instruments Camera Human eye Magnifying glass Telescope Microscope Optical Aberrations Phys Phys 2435: 22: Chap. 34, 31, Pg 1 The Lens Equation
More informationSecrets of Telescope Resolution
amateur telescope making Secrets of Telescope Resolution Computer modeling and mathematical analysis shed light on instrumental limits to angular resolution. By Daniel W. Rickey even on a good night, the
More informationChapter 25 Optical Instruments
Chapter 25 Optical Instruments Units of Chapter 25 Cameras, Film, and Digital The Human Eye; Corrective Lenses Magnifying Glass Telescopes Compound Microscope Aberrations of Lenses and Mirrors Limits of
More informationPhysics 1230: Light and Color
Physics 1230: Light and Color Exam 4 cancelled: Exam extra credit assignment will be due Wed. at 5PM Extra credit to improve exam scores! HW9: Due today, Monday, 5PM FCQ at end of lecture. Lecture 13:
More informationConverging and Diverging Surfaces. Lenses. Converging Surface
Lenses Sandy Skoglund 2 Converging and Diverging s AIR Converging If the surface is convex, it is a converging surface in the sense that the parallel rays bend toward each other after passing through the
More informationOPTICS LENSES AND TELESCOPES
ASTR 1030 Astronomy Lab 97 Optics - Lenses & Telescopes OPTICS LENSES AND TELESCOPES SYNOPSIS: In this lab you will explore the fundamental properties of a lens and investigate refracting and reflecting
More informationScaling relations for telescopes, spectrographs, and reimaging instruments
Scaling relations for telescopes, spectrographs, and reimaging instruments Benjamin Weiner Steward Observatory University of Arizona bjw @ asarizonaedu 19 September 2008 1 Introduction To make modern astronomical
More informationNotation for Mirrors and Lenses. Chapter 23. Types of Images for Mirrors and Lenses. More About Images
Notation for Mirrors and Lenses Chapter 23 Mirrors and Lenses Sections: 4, 6 Problems:, 8, 2, 25, 27, 32 The object distance is the distance from the object to the mirror or lens Denoted by p The image
More informationLecture 3: Geometrical Optics 1. Spherical Waves. From Waves to Rays. Lenses. Chromatic Aberrations. Mirrors. Outline
Lecture 3: Geometrical Optics 1 Outline 1 Spherical Waves 2 From Waves to Rays 3 Lenses 4 Chromatic Aberrations 5 Mirrors Christoph U. Keller, Leiden Observatory, keller@strw.leidenuniv.nl Lecture 3: Geometrical
More informationMore problems for Chapter 12 of Introduction to Wave Phenomena (Hirose- Lonngren) θ =.
More problems for Chapter 1 of Introduction to Wave Phenomena (Hirose- Lonngren). In the 18-th century, Bradley observed apparent change in angular location of distant stars by " when the earth is moving
More informationOptical Systems: Pinhole Camera Pinhole camera: simple hole in a box: Called Camera Obscura Aristotle discussed, Al-Hazen analyzed in Book of Optics
Optical Systems: Pinhole Camera Pinhole camera: simple hole in a box: Called Camera Obscura Aristotle discussed, Al-Hazen analyzed in Book of Optics 1011CE Restricts rays: acts as a single lens: inverts
More informationExercise 8: Interference and diffraction
Physics 223 Name: Exercise 8: Interference and diffraction 1. In a two-slit Young s interference experiment, the aperture (the mask with the two slits) to screen distance is 2.0 m, and a red light of wavelength
More informationPresented by Jerry Hubbell Lake of the Woods Observatory (MPC I24) President, Rappahannock Astronomy Club
Presented by Jerry Hubbell Lake of the Woods Observatory (MPC I24) President, Rappahannock Astronomy Club ENGINEERING A FIBER-FED FED SPECTROMETER FOR ASTRONOMICAL USE Objectives Discuss the engineering
More informationThe New. Astronomy. 2 Practical Focusing
The New 2 Practical Focusing Astronomy CCD cameras represent some pretty fancy technology, but in some ways they are just like ordinary cameras. As with a traditional film camera, the difference between
More informationAperture and Digi scoping. Thoughts on the value of the aperture of a scope digital camera combination.
Aperture and Digi scoping. Thoughts on the value of the aperture of a scope digital camera combination. Before entering the heart of the matter, let s do a few reminders. 1. Entrance pupil. It is the image
More informationProblems with filters can have the strangest causes
Problems with filters can have the strangest causes If you switch from simple astrophotography to more difficult fields of activity and start working with different filters, correctors and systems, you
More informationPrac%ce Quiz 7. 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.
Prac%ce Quiz 7 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. D B cameras zoom lens covers the focal length range from 38mm to 110
More informationPotential benefits of freeform optics for the ELT instruments. J. Kosmalski
Potential benefits of freeform optics for the ELT instruments J. Kosmalski Freeform Days, 12-13 th October 2017 Summary Introduction to E-ELT intruments Freeform design for MAORY LGS Free form design for
More informationDefinition of light rays
Geometrical optics In this section we study optical systems involving lenses and mirrors, developing an understanding o devices such as microscopes and telescopes, and biological systems such as the human
More informationa simple optical imager
Imagers and Imaging a simple optical imager Here s one on our 61-Inch Telescope Here s one on our 61-Inch Telescope filter wheel in here dewar preamplifier However, to get a large field we cannot afford
More informationCOURSE NAME: PHOTOGRAPHY AND AUDIO VISUAL PRODUCTION (VOCATIONAL) FOR UNDER GRADUATE (FIRST YEAR)
COURSE NAME: PHOTOGRAPHY AND AUDIO VISUAL PRODUCTION (VOCATIONAL) FOR UNDER GRADUATE (FIRST YEAR) PAPER TITLE: BASIC PHOTOGRAPHIC UNIT - 3 : SIMPLE LENS TOPIC: LENS PROPERTIES AND DEFECTS OBJECTIVES By
More informationOptical Design of the SuMIRe PFS Spectrograph
Optical Design of the SuMIRe PFS Spectrograph Sandrine Pascal* a, Sébastien Vives a, Robert H. Barkhouser b, James E. Gunn c a Aix Marseille Université - CNRS, LAM (Laboratoire d'astrophysique de Marseille),
More informationPHYS 160 Astronomy. When analyzing light s behavior in a mirror or lens, it is helpful to use a technique called ray tracing.
Optics Introduction In this lab, we will be exploring several properties of light including diffraction, reflection, geometric optics, and interference. There are two sections to this lab and they may
More informationIntroduction. Geometrical Optics. Milton Katz State University of New York. VfeWorld Scientific New Jersey London Sine Singapore Hong Kong
Introduction to Geometrical Optics Milton Katz State University of New York VfeWorld Scientific «New Jersey London Sine Singapore Hong Kong TABLE OF CONTENTS PREFACE ACKNOWLEDGMENTS xiii xiv CHAPTER 1:
More information