Physics Hour Examination Light and Optics - Version 1

Size: px
Start display at page:

Download "Physics Hour Examination Light and Optics - Version 1"

Transcription

1 Physics Hour Examination Light and Optics - Version 1 How Do We See Colors? Warning: Multiple Choice questions may have more than one correct answer. They are graded 3 points of each correct answer circled and minus 1 point for each wrong answer circled. : Reci Section 8:30 11:00 12:00 Physical Constants: Electric charge of the electron = e = 1.6 x C Speed of light = c =3 x 10 8 m/s Mass of the electron = me = 9.1 x kg Planck's constant = h = 6.63 x Js = 4.14 x evs Electron volt of energy = 1eV = 1.6 x J Situation No. Maximum Pts Earned Total 100 Bonus 3 10 Bonus 3 20 Grand Total 130

2 Situation 1: Circle the letter in front of every correct answer. (3 points for each correct answer, -1 for each wrong answer, then scaled to 18 points max.) The eye can detect wavelengths that range from 400 nm to 700 nm, where 1 nm = 10-9 m. The color of this visible light ranges from violet at 400 nm to red at 700 nm. This range closely matches the wavelength range of maximum emission from the sun. The relationship between the wavelength of light and the energy of each quantum is E = hc/λ where h is Planck's constant, c is the speed of light in a vacuum, and λ is the wavelength. Another form of this equation is E = 1240/λ where λ is in nm and E is in ev (electron volts). Light can be emitted when atoms make transitions from excited states to lower-energy states. Each quantum of emitted light carries energy equal to the difference between the energies of the states involved. For the emitted light to be visible, it is necessary that the states involved be separated by the proper energies. Visible light arises from atomic transitions between energy levels separated by approximately 1.78 to 3.10 ev. For example, assume that the energy levels of a hypothetical atom are the following: Energy Level ev Energy Level ev Energy Level ev Energy Level ev Energy Level ev Energy will be emitted when an atom makes a transition from a higher to a lower energy level, but visible light will result only when those energies fall within the prescribed range. Light is also emitted from a hot object by a process called blackbody radiation. The most intense wavelength, λ max, of blackbody radiation is given by Wien's displacement law, λ max = 2.9 x 10 6 / T, where T is in kelvins and λ max is in nm. 1. The most intense wavelength emitted by the sun is 480 nm. What is the approximate temperature of a blackbody that emits its most intense radiation at the same wavelength? A. 4,100 K B. 6,000 K C. 7,200 K D. 9,000 K 2. What is the maximum number of emission lines of visible light that could be observed in the spectrum of the hypothetical atom described in the passage? A. 1 B. 2 C. 5 D A blackbody appears white when its temperature is approximately 6,000 K. Which of the following statements explains the color of light emitted at this temperature? A. The object is not hot enough to emit red light. B. The object is too hot to emit blue light. C. White light is the most common wavelength being emitted. D. The object is emitting some light from all colors of the visible spectrum. 4. What is the wavelength of the light emitted when the hypothetical atom described in the passage makes a transition from Energy Level 4 to Energy Level 3? A. 477 nm B. 525 nm C. 600 nm D. 658 nm 5. As the power input to a light bulb decreases, the brightness decreases. How does the color of the emitted light change? A. The emitted spectrum shifts to longer wavelengths. B. The emitted spectrum shifts to shorter wavelengths. C. The most intensive light shifts to lower energy. D. The spectrum does not change. Page 2 of 5

3 Situation 2: Circle the letter in front of every correct answer. (3 points for each correct answer, -1 for each wrong answer, then scaled to 27 points max.) Flexible endoscopes are used extensively in medicine to visualize 6.For the best image quality, the internal structures such as the respiratory tract, stomach, and colon. The following conditions should be met. advantage of a flexible endoscope over a rigid endoscope is that it can A. The core of the fibers must not bend and thus go around corners. This means less discomfort for the absorb a significant amount of light. B. The cladding must have a higher patient and the endoscope can be advanced farther into the cavity of optical density than the core. interest. C. Light rays must be incident on the An endoscope has a number of channels, e.g. for irrigation, suctioning, core-cladding interface at angles of surgical manipulation, illumination, and imaging. Below is a incidence greater than the critical diagrammatic representation of the imaging components of a relatively angle. simple flexible endoscope. D. The endoscope must not be bent too acutely. 7.The critical angle of the corecladding interface is given by A. critical angle = sin -1 (n cladding /n core ) B. critical angle = sin -1 (n core /n cladding ) C. critical angle = sin -1 (1/n core ) D. critical angle = sin -1 (1/n cladding ) 8.If each fiber core is 1 mm in diameter, n core is 1.50, and n cladding is 1.20, what is the minimum length of light-absorbing material required at the ends of the fibers to prevent refraction of light into the cladding? A. 1 mm B mm C. 1.5 mm D. 2 mm 9. The effect of lens 1 is A. to possibly reduce overall chromatic aberration B. to produce a virtual, erect, and diminished image that is the object for lens 2 C. create a wider field of view D. to invert the image of the object Lens 1 focal length is -2 cm. Lens 2 focal length is 1 cm. Lens 3 can be easily removed and replaced with another lens. Also, the distance between lens 3 and the end of the optical fibers can be adjusted. Each optical fiber consists of a cylindrical core surrounded by a cladding. Light enters one end of a fiber and is total internally reflected repeatedly until it exits the fiber at the opposite end. 10.When light has travelled the length of the optical fibers it exits the ends of them and passes through lens 3, which acts like a magnifying glass. If an observer chooses a lens of 50 diopters, how far should lens 3 be from the end of the optical fibers to form an image at infinity? A. 2.0 cm B. 2.5 cm C. 3.0 cm D. 3.5 cm Page 3 of 5

4 Situation 3: (25 points) As a part of your job as an Olympic drug-testing expert, you have been asked to make a judgment on an Olympic athlete whose body fluid has been given an analysis using a standard spectrophotometer. A calibration curve of the appropriate body fluid was first taken, and then the body fluid of the athlete containing an unknown amount of a possible drug was taken. The data and the curves for both analyses are shown below. wavelength Calibration Unknown nm rel. intensity rel. intensity Spectrophotomete Calib Unknown Solu Wavelength (a) (15 points) You have found from the standard table of concentrations of drugs in this bodily fluid, that the forbidden drug, Neosynepherin, has a maximun absorption at about 575 nm and has an optical density as a function of concentation give by the equation OD(Neosynepherin) = 3.14 * (concentration of Neosynepherin in gm/liter of body fluid) Estimate the concentration of Neosynepherin in the body fluid of this athlete. Show your work. (b) (10 points) It is believed that 200 parts per million of Neosynepherin will enhance the performance of an athlete. Knowing that one liter of body fluid has a mass of 1000 gm, do you think the athlete should be ejected from the Olympic games? Explain your answer. Bonus points: (10 points) Select an appropriate graph and show the transmission of the body fluid containing the unknown drug as a function of wavelength. Label the axes. Show your work. Page 4 of 5

5 Situation 4: (30 points, 10 points for each correct answer and its explanation) As a part of your job as a health care provider, you have been asked to come up with a plan to help Americans pay for their health care costs. You have been presented with the following data: The cost of gall bladder surgery in the United States is given below: Year Cost 1950 $ $ $ $ $ $ 803* The Medicare Program went into effect in $ $ $ $ $ $ 4900 From these data, or an appropriate graph, estimate, and explain the process you use to make your estimate (a) when will gall bladder surgery cost twice as much as it did in 1980? Show your work. (b) the present annual percentage change in the cost of gall bladder surgery. Show your work. (c) the cost of gall bladder surgery near the end of your lifetime say, in the year Show your work. Bonus (20 points) Select an appropriate graph and show these data as linear function(s). Label the axes. Page 5 of 5

Chapter 24 Photonics Question 1 Question 2 Question 3 Question 4 Question 5

Chapter 24 Photonics Question 1 Question 2 Question 3 Question 4 Question 5 Chapter 24 Photonics Data throughout this chapter: e = 1.6 10 19 C; h = 6.63 10 34 Js (or 4.14 10 15 ev s); m e = 9.1 10 31 kg; c = 3.0 10 8 m s 1 Question 1 Visible light has a range of photons with wavelengths

More information

Core Concept. PowerPoint Lectures to accompany Physical Science, 8e. Chapter 7 Light. New Symbols for this Chapter 3/29/2011

Core Concept. PowerPoint Lectures to accompany Physical Science, 8e. Chapter 7 Light. New Symbols for this Chapter 3/29/2011 PowerPoint Lectures to accompany Physical Science, 8e Chapter 7 Light Copyright The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Core Concept Light is electromagnetic radiation

More information

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information

Properties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information Concepts: Properties of Electromagnetic Radiation Chapter 5 Electromagnetic waves Types of spectra Temperature Blackbody radiation Dual nature of radiation Atomic structure Interaction of light and matter

More information

School. Team Number. Optics

School. Team Number. Optics School Team Number Optics Physical Optics (30%) Proceed to the laser shoot (40%) when your team number is called. 1. What are the four colors used in the CMYK color model? (2 points) 2. Muscae Volitantes

More information

The Nature of Light I: Electromagnetic Waves Spectra Kirchoff s Laws Temperature Blackbody radiation

The Nature of Light I: Electromagnetic Waves Spectra Kirchoff s Laws Temperature Blackbody radiation The Nature of Light I: Electromagnetic Waves Spectra Kirchoff s Laws Temperature Blackbody radiation Electromagnetic Radiation (How we get most of our information about the cosmos) Examples of electromagnetic

More information

A system of two lenses is achromatic when the separation between them is

A system of two lenses is achromatic when the separation between them is L e c t u r e 1 5 1 Eyepieces Single eye lens in a telescope / microscope produces spherical and chromatic aberrations. The field of view is also narrow. The eye lens is replaced by a system of lenses

More information

5.At what speed is a particle traveling if its kinetic energy is three times its rest energy? A) 0.879c B) 0.918c C) 0.943c D) 0.

5.At what speed is a particle traveling if its kinetic energy is three times its rest energy? A) 0.879c B) 0.918c C) 0.943c D) 0. 1.Two identical light waves, A and B, are emitted from different sources and meet at a point P. The distance from the source of A to the point P is L A ; and the source of B is a distance L B from P. Which

More information

VISIBLE LIGHT. L 32 Light and Optics [2] Seeing through the window. Windows behaving as mirrors. Seeing through a window

VISIBLE LIGHT. L 32 Light and Optics [2] Seeing through the window. Windows behaving as mirrors. Seeing through a window L 32 Light and Optics [2] Measurements of the speed of light The bending of light refraction Total internal reflection Dispersion Dispersion Rainbows Atmospheric scattering Blue sky and red sunsets Mirrors

More information

A) n L < 1.0 B) n L > 1.1 C) n L > 1.3 D) n L < 1.1 E) n L < 1.3

A) n L < 1.0 B) n L > 1.1 C) n L > 1.3 D) n L < 1.1 E) n L < 1.3 1. A beam of light passes from air into water. Which is necessarily true? A) The frequency is unchanged and the wavelength increases. B) The frequency is unchanged and the wavelength decreases. C) The

More information

EA Notes (Scen 101), Tillery Chapter 7. Light

EA Notes (Scen 101), Tillery Chapter 7. Light EA Notes (Scen 101), Tillery Chapter 7 Light Introduction Light is hard to study because you can't see it, you only see it's effects. Newton tried to explain the energy in a light beam as the KE of a particle

More information

A small object is placed a distance 2.0 cm from a thin convex lens. The focal length of the lens is 5.0 cm.

A small object is placed a distance 2.0 cm from a thin convex lens. The focal length of the lens is 5.0 cm. TC [66 marks] This question is about a converging (convex) lens. A small object is placed a distance 2.0 cm from a thin convex lens. The focal length of the lens is 5.0 cm. (i) Deduce the magnification

More information

Physics 1CL OPTICAL SPECTROSCOPY Spring 2010

Physics 1CL OPTICAL SPECTROSCOPY Spring 2010 Introduction In this lab, you will use a diffraction grating to split up light into the various colors which make up the different wavelengths of the visible electromagnetic spectrum. You will assemble

More information

U n 3 n Ba Kr (D) Br (C) Kr (B) Rb (E) 94 37

U n 3 n Ba Kr (D) Br (C) Kr (B) Rb (E) 94 37 1984 36. The critical angle for a transparent material in air is 30. The index of refraction of the material is most nearly (A) 0.33 (B) 0.50 (C) 1.0 (D) 1.5 (E) 2.0 37. An object is placed as shown in

More information

Physics 1252 Sec.A Exam #1A

Physics 1252 Sec.A Exam #1A Physics 1252 Sec.A Exam #1A Instructions: This is a closed-book, closed-notes exam. You are allowed to use a clean print-out of your formula sheet, any scientific calculator, and a ruler. Do not write

More information

AST 102 chapter 5. Radiation and Spectra. Radiation and Spectra. Radiation and Spectra. What is light? What is radiation?

AST 102 chapter 5. Radiation and Spectra. Radiation and Spectra. Radiation and Spectra. What is light? What is radiation? 5 Radiation and Spectra 1 Radiation and Spectra What is light? According to Webster: a.something that makes vision possible b.the sensation aroused by stimulation of the visual receptors c.electromagnetic

More information

PHYS General Physics II Lab The Balmer Series for Hydrogen Source. c = speed of light = 3 x 10 8 m/s

PHYS General Physics II Lab The Balmer Series for Hydrogen Source. c = speed of light = 3 x 10 8 m/s PHYS 1040 - General Physics II Lab The Balmer Series for Hydrogen Source Purpose: The purpose of this experiment is to analyze the emission of light from a hydrogen source and measure and the wavelengths

More information

Physics 1161: Lecture 22

Physics 1161: Lecture 22 Physics 1161: Lecture 22 Blackbody Radiation Photoelectric Effect Wave-Particle Duality sections 30-1 30-4 Everything comes unglued The predictions of classical physics (Newton s laws and Maxwell s equations)

More information

PHSC 3033: Meteorology Atmospheric Optics

PHSC 3033: Meteorology Atmospheric Optics PHSC 3033: Meteorology Atmospheric Optics Hot Radiating Objects Imagine a piece of metal placed in a hot furnace. At first, the metal becomes warm, although its visual appearance doesn't change. As it

More information

SECTION 3 & 4 LIGHT WAVES & INFORMATION TRANSFER

SECTION 3 & 4 LIGHT WAVES & INFORMATION TRANSFER SECTION 3 & 4 LIGHT WAVES & INFORMATION TRANSFER Light Waves Light is a type of energy that travels as waves. Light is different than other waves because it does not need matter to travel. Light waves

More information

Blackbody Radiation EX-9920 ScienceWorkshop Page 1 of 8. Blackbody Radiation

Blackbody Radiation EX-9920 ScienceWorkshop Page 1 of 8. Blackbody Radiation Blackbody Radiation EX-9920 ScienceWorkshop Page 1 of 8 EQUIPMENT Blackbody Radiation INCLUDED: 1 Prism Spectrophotometer Kit OS-8544 1 Optics Bench (60 cm) OS-8541 1 Spectrophotometer Accessory Kit OS-8537

More information

AS 101: Day Lab #2 Summer Spectroscopy

AS 101: Day Lab #2 Summer Spectroscopy Spectroscopy Goals To see light dispersed into its constituent colors To study how temperature, light intensity, and light color are related To see spectral lines from different elements in emission and

More information

THE ELECTROMAGNETIC SPECTRUM. (We will go into more detail later but we need to establish some basic understanding here)

THE ELECTROMAGNETIC SPECTRUM. (We will go into more detail later but we need to establish some basic understanding here) What is color? THE ELECTROMAGNETIC SPECTRUM. (We will go into more detail later but we need to establish some basic understanding here) Light isn t just white: colors is direct evidence that light has

More information

Lecture 15 Notes: 07 / 26. The photoelectric effect and the particle nature of light

Lecture 15 Notes: 07 / 26. The photoelectric effect and the particle nature of light Lecture 15 Notes: 07 / 26 The photoelectric effect and the particle nature of light When diffraction of light was discovered, it was assumed that light was purely a wave phenomenon, since waves, but not

More information

DAY LABORATORY EXERCISE: SPECTROSCOPY

DAY LABORATORY EXERCISE: SPECTROSCOPY AS101 - Day Laboratory: Spectroscopy Page 1 DAY LABORATORY EXERCISE: SPECTROSCOPY Goals: To see light dispersed into its constituent colors To study how temperature, light intensity, and light color are

More information

The Spectrophotometer and Atomic Spectra of Hydrogen Physics 246

The Spectrophotometer and Atomic Spectra of Hydrogen Physics 246 The Spectrophotometer and Atomic Spectra of Hydrogen Physics 46 Introduction: When heated sufficiently, most elements emit light. With a spectrometer, the emitted light can be broken down into its various

More information

2. The figure shows the path of a portion of a ray of light as it passes through three different materials. Note: The figure is drawn to scale.

2. The figure shows the path of a portion of a ray of light as it passes through three different materials. Note: The figure is drawn to scale. 1. The bending of light as it moves from one medium to another with differing indices of refraction is due to a change in what property of the light? A) amplitude B) period C) frequency D) speed E) color

More information

Thermal Radiation By: Prof. K M Joshi

Thermal Radiation By: Prof. K M Joshi Thermal Radiation By: Prof. K M Joshi Radiation originate due to emission of matter and its subsequent transports does not required any matter / medium. Que: Then what is the nature of this transport???

More information

Exam 4--PHYS 151--Spring 2017

Exam 4--PHYS 151--Spring 2017 Name: Exam 4--PHYS 151--Spring 2017 Multiple Choice Identify the choice that best completes the statement or answers the question. 1. Electromagnetic radiation is caused by a. electricity b. radioactive

More information

Prof. Jeff Kenney Class 5 June 1, 2018

Prof. Jeff Kenney Class 5 June 1, 2018 www.astro.yale.edu/astro120 Prof. Jeff Kenney Class 5 June 1, 2018 to understand how we know stuff about the universe we need to understand: 1. the spectral analysis of light 2. how light interacts with

More information

Test 4 Preparation Questions

Test 4 Preparation Questions Test 4 Preparation Questions A1. One joule of work is required to move a one-coulomb point charge from point A to point B in a uniform electric field. This indicates that (A) the resistance between points

More information

The Structure of the Atom

The Structure of the Atom CHAPTER 5 The Structure of the Atom 5.4 Light and Spectroscopy 460 370 BC 1808 1870 1897 1910 1925 Today Democritus Atomism Dalton Modern atomic theory Crookes Cathode rays Thomson Discovery of the electron

More information

Exp. P-6 Blackbody Radiation

Exp. P-6 Blackbody Radiation Exp. P-6 Blackbody Radiation Updated Feb 2019 by A. Azelis, M. Hohlmann Equipment Prism Spectrophotometrer Kit Optics Bench (60 cm) Spectrophotometer Accessory Kit Aperture Bracket High Sensitivity Light

More information

SPECTROSCOPY PRELAB. 2) Name the 3 types of spectra and, in 1 sentence each, describe them.

SPECTROSCOPY PRELAB. 2) Name the 3 types of spectra and, in 1 sentence each, describe them. NAME: SPECTROSCOPY PRELAB 1) What is a spectrum? 2) Name the 3 types of spectra and, in 1 sentence each, describe them. a. b. c. 3) Use Wien s law to calculate the surface temperature of the star Alnilam

More information

Physics 1252 Section Exam #1D

Physics 1252 Section Exam #1D Thu, 09 February 2017 Name: Physics 1252 Section 36501 Exam #1D Instructions: This is a closed-book, closed-notes exam. You are allowed to use a clean print-out of your formula sheet, any scientific calculator,

More information

Physics 1252 Section Exam #1E

Physics 1252 Section Exam #1E Thu, 09 February 2017 Name: Physics 1252 Section 36501 Exam #1E Instructions: This is a closed-book, closed-notes exam. You are allowed to use a clean print-out of your formula sheet, any scientific calculator,

More information

LIGHT. Question. Until very recently, the study of ALL astronomical objects, outside of the Solar System, has been with telescopes observing light.

LIGHT. Question. Until very recently, the study of ALL astronomical objects, outside of the Solar System, has been with telescopes observing light. LIGHT Question Until very recently, the study of ALL astronomical objects, outside of the Solar System, has been with telescopes observing light. What kind of information can we get from light? 1 Light

More information

1. Newton's Laws provide a good description of the flight of a baseball because:

1. Newton's Laws provide a good description of the flight of a baseball because: 1. Newton's Laws provide a good description of the flight of a baseball because: Solution: Newton's laws can be used provided that the velocities are small compared to c (so that relativistic effects can

More information

The Essential Exponential! Mathematical Modeling IN Beginning Physics. Robert G. Fuller and Vicki L. Plano Clark University of Nebraska Lincoln

The Essential Exponential! Mathematical Modeling IN Beginning Physics. Robert G. Fuller and Vicki L. Plano Clark University of Nebraska Lincoln The Essential Exponential! Mathematical Modeling IN Beginning Physics Robert G. Fuller and Vicki L. Plano Clark University of Nebraska Lincoln Poster Abstract: Mathematical Modeling in Beginning Physics

More information

PHYS 160 Astronomy Test #2 Fall 2017 Version A

PHYS 160 Astronomy Test #2 Fall 2017 Version A PHYS 160 Astronomy Test #2 Fall 2017 Version A I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. A blackbody emits all of its radiation

More information

Modern Physics Laboratory MP2 Blackbody Radiation

Modern Physics Laboratory MP2 Blackbody Radiation Purpose MP2 Blackbody Radiation In this experiment, you will investigate the spectrum of the blackbody radiation and its dependence on the temperature of the body. Equipment and components Tungsten light

More information

DISPERSION VERY SHORT ANSWER QUESTIONS. Two identical prisms made of the same material placed with their based on opposite sides (of the

DISPERSION VERY SHORT ANSWER QUESTIONS. Two identical prisms made of the same material placed with their based on opposite sides (of the DISPERSION VERY SHORT ANSWER QUESTIONS Q-1. What will be the spectrum of sun during a total solar eclipse? Q-2. Why the secondary rainbow is always fainter than the primary rainbow? Q-3. Two identical

More information

COLLEGE OF ENGINEERING PUTRAJAYA CAMPUS FINAL EXAMINATION TRIMESTER 1, 2010/2011

COLLEGE OF ENGINEERING PUTRAJAYA CAMPUS FINAL EXAMINATION TRIMESTER 1, 2010/2011 COLLEGE OF ENGINEERING PUTRAJAYA CAMPUS FINAL EXAMINATION TRIMESTER 1, 2010/2011 PROGRAMME SUBJECT CODE : Foundation in Engineering : PHYF144 SUBJECT : Physics 3 DATE : October 2010 TIME VENUE : 2 hours

More information

UNIT-5 EM WAVES UNIT-6 RAY OPTICS

UNIT-5 EM WAVES UNIT-6 RAY OPTICS UNIT-5 EM WAVES 2 Marks Question 1. To which regions of electromagnetic spectrum do the following wavelengths belong: (a) 250 nm (b) 1500 nm 2. State any one property which is common to all electromagnetic

More information

where c m s (1)

where c m s (1) General Physics Experiment 6 Spectrum of Hydrogen s Emission Lines Objectives: < To determine wave lengths of the bright emission lines of hydrogen. < To test the relationship between wavelength and energy

More information

Physics 202 Final (Monday, December 12) Fall 2016 (Saslow) White Version

Physics 202 Final (Monday, December 12) Fall 2016 (Saslow) White Version Physics 202 Final (Monday, December 12) Fall 2016 (Saslow) White Version Name (printed) Lab Section(+2 pts) Name (signed as on ID) Show all work. Partial credit may be given. Answers should include the

More information

Preview from Notesale.co.uk Page 1 of 38

Preview from Notesale.co.uk Page 1 of 38 F UNDAMENTALS OF PHOTONICS Module 1.1 Nature and Properties of Light Linda J. Vandergriff Director of Photonics System Engineering Science Applications International Corporation McLean, Virginia Light

More information

Physics 11 Exam 3 Spring 2016

Physics 11 Exam 3 Spring 2016 Physics 11 Exam 3 Spring 2016 Name: Circle the BEST Answer 1 Electromagnetic waves consist of A) compressions and rarefactions of electromagnetic pulses. B) oscillating electric and magnetic fields. C)

More information

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics Physics 111.6 MIDTERM TEST #4 March 8, 2001 Time: 90 minutes NAME: STUDENT NO.: (Last) Please Print (Given) LECTURE SECTION (please

More information

Chapter 33: ELECTROMAGNETIC WAVES 559

Chapter 33: ELECTROMAGNETIC WAVES 559 Chapter 33: ELECTROMAGNETIC WAVES 1 Select the correct statement: A ultraviolet light has a longer wavelength than infrared B blue light has a higher frequency than x rays C radio waves have higher frequency

More information

Conceptual Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson VI October 3, 2017

Conceptual Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson VI October 3, 2017 Conceptual Physics Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson VI October 3, 2017 https://arxiv.org/abs/1711.07445 L. A. Anchordoqui (CUNY)

More information

2. Determine the excess charge on the outer surface of the outer sphere (a distance c from the center of the system).

2. Determine the excess charge on the outer surface of the outer sphere (a distance c from the center of the system). Use the following to answer question 1. Two point charges, A and B, lie along a line separated by a distance L. The point x is the midpoint of their separation. 1. Which combination of charges will yield

More information

FALL 2004 Final Exam, Part A

FALL 2004 Final Exam, Part A Physics 152 FALL 2004 Final Exam, Part A Roster No.: Score: 23 pts. possible Exam time limit: 2 hours. You may use a calculator and both sides of 2 sheets of notes, handwritten only. Closed book; no collaboration.

More information

Optics in a Fish Tank Demonstrations for the Classroom

Optics in a Fish Tank Demonstrations for the Classroom Optics in a Fish Tank Demonstrations for the Classroom Introduction: This series of demonstrations will illustrate a number of optical phenomena. Using different light sources and a tank of water, you

More information

Practical 1P4 Energy Levels and Band Gaps

Practical 1P4 Energy Levels and Band Gaps Practical 1P4 Energy Levels and Band Gaps What you should learn from this practical Science This practical illustrates some of the points from the lecture course on Elementary Quantum Mechanics and Bonding

More information

Activity: Cosmic Colors and Spectroscopy

Activity: Cosmic Colors and Spectroscopy 1 Activity: Cosmic Colors and Spectroscopy Background: The energy of a photon of light depends on the wavelength (frequency) of the light higher frequency f = higher energy E = shorter wavelength λ) red

More information

Laboratory Exercise. Quantum Mechanics

Laboratory Exercise. Quantum Mechanics Laboratory Exercise Quantum Mechanics Exercise 1 Atomic Spectrum of Hydrogen INTRODUCTION You have no doubt been exposed many times to the Bohr model of the atom. You may have even learned of the connection

More information

EXPERIMENT 18 THE PHOTOELECTRIC EFFECT

EXPERIMENT 18 THE PHOTOELECTRIC EFFECT 220 18-1 I. THEORY EXPERIMENT 18 THE PHOTOELECTRIC EFFECT When light or other electromagnetic waves of sufficiently high frequency fall on a metal surface, they cause electrons to be emitted by the surface.

More information

Practical 1P4 Energy Levels and Band Gaps

Practical 1P4 Energy Levels and Band Gaps Practical 1P4 Energy Levels and Band Gaps What you should learn from this practical Science This practical illustrates some of the points from the lecture course on Elementary Quantum Mechanics and Bonding

More information

INFRAMET. 2.1 Basic laws

INFRAMET. 2.1 Basic laws tel: 048 60844873, fax 48 6668780. Basic laws.. Planck law All objects above the temperature of absolute zero emit thermal radiation due to thermal motion of the atoms and the molecules. The hotter they

More information

EXPERIMENT 17: Atomic Emission

EXPERIMENT 17: Atomic Emission EXPERIMENT 17: Atomic Emission PURPOSE: To construct an energy level diagram of the hydrogen atom To identify an element from its line spectrum. PRINCIPLES: White light, such as emitted by the sun or an

More information

MIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova

MIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova MIDTERM 3 REVIEW SESSION Dr. Flera Rizatdinova Summary of Chapter 23 Index of refraction: Angle of reflection equals angle of incidence Plane mirror: image is virtual, upright, and the same size as the

More information

NOTES: 5.3 Light and Atomic Spectra (more Quantum Mechanics!)

NOTES: 5.3 Light and Atomic Spectra (more Quantum Mechanics!) NOTES: 5.3 Light and Atomic Spectra (more Quantum Mechanics!) Light WAVE or PARTICLE? Electromagnetic Radiation Electromagnetic radiation includes: -radio waves -microwaves -infrared waves -visible light

More information

Preview. Atomic Physics Section 1. Section 1 Quantization of Energy. Section 2 Models of the Atom. Section 3 Quantum Mechanics

Preview. Atomic Physics Section 1. Section 1 Quantization of Energy. Section 2 Models of the Atom. Section 3 Quantum Mechanics Atomic Physics Section 1 Preview Section 1 Quantization of Energy Section 2 Models of the Atom Section 3 Quantum Mechanics Atomic Physics Section 1 TEKS The student is expected to: 8A describe the photoelectric

More information

Seat Number. Print and sign your name, and write your Student ID Number and seat number legibly in the spaces above.

Seat Number. Print and sign your name, and write your Student ID Number and seat number legibly in the spaces above. Physics 123A Final Spring 2001 Wednesday, June 6 Name last first initial Seat Number Signature Student Number Print and sign your name, and write your Student ID Number and seat number legibly in the spaces

More information

10. A Kelvin thermometer and a Fahrenheit thermometer both give the same reading for a certain sample. The corresponding Celsius temperature is: A)

10. A Kelvin thermometer and a Fahrenheit thermometer both give the same reading for a certain sample. The corresponding Celsius temperature is: A) Physics 223 practice final exam, Form X!! Fall 2017 Name Write your answers (one per question) on a Scantron form (882E) using a pencil. Write your name above. Return this exam with your scantron upon

More information

Lecture 12. Measurements in Astronomy. Using Light. ASTR 111 Section 002. In astronomy, we need to make remote and indirect measurements

Lecture 12. Measurements in Astronomy. Using Light. ASTR 111 Section 002. In astronomy, we need to make remote and indirect measurements Lecture 12 ASTR 111 Section 002 Measurements in Astronomy In astronomy, we need to make remote and indirect measurements Think of an example of a remote and indirect measurement from everyday life Using

More information

LIGHT. A beam is made up of several rays. It maybe parallel, diverging (spreading out) or converging (getting narrower). Parallel Diverging Converging

LIGHT. A beam is made up of several rays. It maybe parallel, diverging (spreading out) or converging (getting narrower). Parallel Diverging Converging LIGHT Light is a form of energy. It stimulates the retina of the eye and produces the sensation of sight. We see an object when light leaves it and enters the eye. Objects such as flames, the sum and stars

More information

Physics 23 Fall 1998 Lab 4 - The Hydrogen Spectrum

Physics 23 Fall 1998 Lab 4 - The Hydrogen Spectrum Physics 3 Fall 998 Lab 4 - The Hydrogen Spectrum Theory In the late 800's, it was known that when a gas is excited by means of an electric discharge and the light emitted is viewed through a diffraction

More information

Physics 25 Exam #4 December 2, 2008 Dr. Alward Page 1

Physics 25 Exam #4 December 2, 2008 Dr. Alward Page 1 1. Light with a wavelength of 589 nm in a vacuum strikes the surface of an unknown liquid at an angle of 31.2 with respect to the normal to the surface. If the light travels at a speed of 1.97 10 8 m/s

More information

Unit 4 Parent Guide: Waves. What is a wave?

Unit 4 Parent Guide: Waves. What is a wave? Unit 4 Parent Guide: Waves What is a wave? A wave is a disturbance or vibration that carries energy from one location to another. Some waves require a medium to transmit the energy whereas others can travel

More information

General Physics II Summer Session 2013 Review Ch - 16, 17, 18

General Physics II Summer Session 2013 Review Ch - 16, 17, 18 95.104 General Physics II Summer Session 2013 Review Ch - 16, 17, 18 A metal ball hangs from the ceiling by an insulating thread. The ball is attracted to a positivecharged rod held near the ball. The

More information

The Quantum Model of the Hydrogen Atom

The Quantum Model of the Hydrogen Atom Physics 109 Science 1 Experiment 1 1 The Quantum Model of the Hydrogen Atom In this experiment you will use a spectrometer to determine the wavelengths of the visible lines of atomic hydrogen. The goal

More information

Name: Class: Date: Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.

Name: Class: Date: Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. Name: Class: Date: AP REVIEW 3 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.. For a mass hanging from a spring, the maximum displacement the

More information

Chapter 26: Properties of Light

Chapter 26: Properties of Light Lecture Outline Chapter 26: Properties of Light This lecture will help you understand: Electromagnetic Waves The Electromagnetic Spectrum Transparent Materials Opaque Materials Seeing Light The Eye Electromagnetic

More information

PHYSICS. Ray Optics. Mr Rishi Gopie

PHYSICS. Ray Optics. Mr Rishi Gopie Ray Optics Mr Rishi Gopie Ray Optics Nature of light Light is a form of energy which affects the human eye in such a way as to cause the sensation of sight. Visible light is a range of electromagnetic

More information

Chapter 5 Light and Matter: Reading Messages from the Cosmos. How do we experience light? Colors of Light. How do light and matter interact?

Chapter 5 Light and Matter: Reading Messages from the Cosmos. How do we experience light? Colors of Light. How do light and matter interact? Chapter 5 Light and Matter: Reading Messages from the Cosmos How do we experience light? The warmth of sunlight tells us that light is a form of energy We can measure the amount of energy emitted by a

More information

Chapter 5 Light and Matter

Chapter 5 Light and Matter Chapter 5 Light and Matter Stars and galaxies are too far for us to send a spacecraft or to visit (in our lifetimes). All we can receive from them is light But there is much we can learn (composition,

More information

The Death of Classical Physics. The Rise of the Photon

The Death of Classical Physics. The Rise of the Photon The Death of Classical Physics The Rise of the Photon A fundamental question: What is Light? James Clerk Maxwell 1831-1879 Electromagnetic Wave Max Planck 1858-1947 Photon Maxwell's Equations (1865) Maxwell's

More information

Gen. Phys. II Exam 4 - Chs. 27,28,29 - Wave Optics, Relativity, Quantum Physics Apr. 16, 2018

Gen. Phys. II Exam 4 - Chs. 27,28,29 - Wave Optics, Relativity, Quantum Physics Apr. 16, 2018 Gen. Phys. II Exam 4 - Chs. 27,28,29 - Wave Optics, Relativity, Quantum Physics Apr. 16, 2018 Rec. Time Name For full credit, make your work clear. Show formulas used, essential steps, and results with

More information

DISPERSION AND SPECTRA CHAPTER 20

DISPERSION AND SPECTRA CHAPTER 20 CHAPTER 20 DISPERSION AND SPECTRA 20.1 DISPERSION As mentioned earlier, the refractive index of a material depends slightly on the wavelength of light. The relation between the two may be approximately

More information

Radiation in the Earth's Atmosphere. Part 1: Absorption and Emission by Atmospheric Gases

Radiation in the Earth's Atmosphere. Part 1: Absorption and Emission by Atmospheric Gases Radiation in the Earth's Atmosphere Part 1: Absorption and Emission by Atmospheric Gases Electromagnetic Waves Electromagnetic waves are transversal. Electric and magnetic fields are perpendicular. In

More information

Explain how Planck resolved the ultraviolet catastrophe in blackbody radiation. Calculate energy of quanta using Planck s equation.

Explain how Planck resolved the ultraviolet catastrophe in blackbody radiation. Calculate energy of quanta using Planck s equation. Objectives Explain how Planck resolved the ultraviolet catastrophe in blackbody radiation. Calculate energy of quanta using Planck s equation. Solve problems involving maximum kinetic energy, work function,

More information

Telescopes: Portals of Discovery

Telescopes: Portals of Discovery Telescopes: Portals of Discovery How do light and matter interact? Emission Absorption Transmission Transparent objects transmit light Opaque objects block (absorb) light Reflection or Scattering Reflection

More information

Recall: The Importance of Light

Recall: The Importance of Light Key Concepts: Lecture 19: Light Light: wave-like behavior Light: particle-like behavior Light: Interaction with matter - Kirchoff s Laws The Wave Nature of Electro-Magnetic Radiation Visible light is just

More information

Stellar Astrophysics: The Continuous Spectrum of Light

Stellar Astrophysics: The Continuous Spectrum of Light Stellar Astrophysics: The Continuous Spectrum of Light Distance Measurement of Stars Distance Sun - Earth 1.496 x 10 11 m 1 AU 1.581 x 10-5 ly Light year 9.461 x 10 15 m 6.324 x 10 4 AU 1 ly Parsec (1

More information

Final Exam, Part A. December 12, Score:

Final Exam, Part A. December 12, Score: Physics 152 December 12, 2005 Final Exam, Part A Roster No.: Score: Exam time limit: 2 hours. You may use a calculator and both sides of TWO sheets of notes, handwritten only. Closed book; no collaboration.

More information

ASTRO Fall 2012 LAB #7: The Electromagnetic Spectrum

ASTRO Fall 2012 LAB #7: The Electromagnetic Spectrum ASTRO 1050 - Fall 2012 LAB #7: The Electromagnetic Spectrum ABSTRACT Astronomers rely on light to convey almost all of the information we have on distant astronomical objects. In addition to measuring

More information

Chapter 38. The End of Classical Physics

Chapter 38. The End of Classical Physics Chapter 38. The End of Classical Physics Studies of the light emitted by gas discharge tubes helped bring classical physics to an end. Chapter Goal: To understand how scientists discovered the properties

More information

Chapter 37 Early Quantum Theory and Models of the Atom. Copyright 2009 Pearson Education, Inc.

Chapter 37 Early Quantum Theory and Models of the Atom. Copyright 2009 Pearson Education, Inc. Chapter 37 Early Quantum Theory and Models of the Atom Planck s Quantum Hypothesis; Blackbody Radiation Photon Theory of Light and the Photoelectric Effect Energy, Mass, and Momentum of a Photon Compton

More information

LECTURE 23: LIGHT. Propagation of Light Huygen s Principle

LECTURE 23: LIGHT. Propagation of Light Huygen s Principle LECTURE 23: LIGHT Propagation of Light Reflection & Refraction Internal Reflection Propagation of Light Huygen s Principle Each point on a primary wavefront serves as the source of spherical secondary

More information

How does your eye form an Refraction

How does your eye form an Refraction Astronomical Instruments Eyes and Cameras: Everyday Light Sensors How does your eye form an image? How do we record images? How does your eye form an image? Refraction Refraction is the bending of light

More information

Light and Matter: Reading Messages from the Cosmos. White light is made up of many different colors. Interactions of Light with Matter

Light and Matter: Reading Messages from the Cosmos. White light is made up of many different colors. Interactions of Light with Matter Chapter 5 Lecture The Cosmic Perspective Light and Matter: Reading Messages from the Cosmos 5.1 Light in Everyday Life Our goals for learning: How do we experience light? How do light and matter interact?

More information

Physics 202 Final Exam May 14, 2012

Physics 202 Final Exam May 14, 2012 ID CODE: D Physics 202 Final Exam May 14, 2012 Name:... Student ID:... Section:... TA (please circle): Deepak Agarwal Nicholas Brewer Raghvendra Chaubey Todd Garon Yutao Gong Andrew Loveridge Abhishek

More information

Write the electron configuration for Chromium (Cr):

Write the electron configuration for Chromium (Cr): Write the electron configuration for Chromium (Cr): Energy level Aufbau Principle Atomic orbital Quantum Hund s Rule Atomic number Electron Configuration Whole number Pauli Exlcusion Principle Quantum

More information

EXPERIMENT NO. 4. Thermal Radiation: the Stefan-Boltzmann Law

EXPERIMENT NO. 4. Thermal Radiation: the Stefan-Boltzmann Law 1 EXPERIMENT NO. 4 Thermal Radiation: the Stefan-Boltzmann Law References: Physics for Scientists and Engineers, Serway and Jewett. Sections 40.1 An Introduction to Thermal Physics, Schroeder, Section

More information

Last Name: First Name Network-ID

Last Name: First Name Network-ID Last Name: First Name Network-ID Discussion Section: Discussion TA Name: Turn off your cell phone and put it out of sight. Keep your calculator on your own desk. Calculators cannot be shared. This is a

More information

1. Waves and Particles 2. Interference of Waves 3. Wave Nature of Light

1. Waves and Particles 2. Interference of Waves 3. Wave Nature of Light 1. Waves and Particles 2. Interference of Waves 3. Wave Nature of Light 1. Double-Slit Eperiment reading: Chapter 22 2. Single-Slit Diffraction reading: Chapter 22 3. Diffraction Grating reading: Chapter

More information

Experiment 4 Radiation in the Visible Spectrum

Experiment 4 Radiation in the Visible Spectrum Experiment 4 Radiation in the Visible Spectrum Emission spectra can be a unique fingerprint of an atom or molecule. The photon energies and wavelengths are directly related to the allowed quantum energy

More information

Chapter 1. Blackbody Radiation. Theory

Chapter 1. Blackbody Radiation. Theory Chapter 1 Blackbody Radiation Experiment objectives: explore radiation from objects at certain temperatures, commonly known as blackbody radiation ; make measurements testing the Stefan-Boltzmann law in

More information