Light Emission.
|
|
|
- Phebe Bell
- 6 years ago
- Views:
Transcription
1 Light Emission
2 Radio waves are produced by electrons moving up and down an antenna. Visible light is produced by electrons changing energy states in an atom.
3 EXCITATION
4 Excitation - occurs when an electron in an atom is given energy causing it to jump to a higher orbit. This can happen through Collisions or Photon absorption (the photon absorption must exactly match the energy jump).
5 Here comes a nucleus With possible orbits for electrons e - In this configuration the atom is not excited.
6 Here comes a photon e - In this configuration the atom is not excited.
7 Now the atom is said to be excited because the electron is in a higher than normal orbit. e -
8 Now the atom is in a non-excited state again. It emitted a photon when it changed orbits. e -
9 The excited atom usually de-excites in about 100 millionth of a second. The subsequent emitted radiation has an energy that matches that of the orbital change in the atom.
10 Atomic Excitation
11 This emitted radiation gives the characteristic colors of the element involved. The atoms do not wear out. Flame Colors
12 Emission Spectra Continuous Emission Spectrum Slit White Light Source Prism Photographic Film
13 Emission Spectrum of Hydrogen Slit Discrete Emission Spectrum Film Low Density Glowing Hydrogen Gas Prism Photographic Film
14 Spectra of the Noble Gases
15 INCANDESCENCE Blue hot is hotter than white hot which is hotter than red hot. White light - all colors in the visible are present. Electron transitions occur not only in the parent atom but in adjacent atoms as well.
16 Relative Energy Brightness versus Color curve for different temperatures Peak Frequency Frequency is proportional to temperature. Frequency f T (measured in Kelvins)
17 Absorption Spectrum of Hydrogen Discrete Emission Spectrum Slit Discrete Absorption Spectrum Hydrogen Gas Film White Light Source Prism Photographic Film
18 Absorption Spectra Frequencies of light that represent the correct energy jumps in the atom will be absorbed. When the atom de-excites, it emits the same kinds of frequencies it absorbed. However, this emission can be in any direction.
19 Close inspection of the absorption spectrum of the sun reveals missing lines known as Fraunhofer lines. In 1868 a pattern of lines was observed in the solar spectrum that represented an element that had not been found on earth. It was Helium named for Helios, the sun.
20 Doppler shifts are observed in the spectra of stars. If a star is approaching, its spectra will be blue shifted. If a star is moving away, its spectra will be red shifted. Most spectra are red shifted indicating that on the average the universe is expanding.
21 FLUORESCENCE Some materials that are excited by UV emit visible. These materials are referred to as fluorescent materials.
22 Fluorescent Lamps Primary excitation - electron collisions with low pressure Hg vapor, UV given off Secondary excitation - UV photons absorbed by phosphors. Phosphors fluoresce emitting visible light. Remember that the visible light from the excited mercury vapor is also emitted.
23 PHOSPHORESCENCE Electrons get "stuck" in excited states in the atoms and de-excitation occurs at different times for different atoms. A continuous glow occurs for some time. Bioluminescence: Created by chemical reactions inside living organisms.
24 LASERS Light Amplification by Stimulated Emission of Radiation
25 Lasers produce coherent light. Coherent light is light with the same frequency and the same phase.
26 Review Questions
27 What type of spectrum would you expect to obtain if white light is shined through sodium vapor? (a) an emission spectrum of sodium (b) an absorption spectrum of sodium (c) a continuous spectrum
28 In fluorescence which has the higher energy, the radiation absorbed or the radiation of an emitted photon? (a) absorbed (b) emitted (c) they both have the same energy
29 Which phenomenon has electrons getting "stuck" in excited states? (a) incandescence (b) fluorescence (c) phosphorescence
30 What causes laser light to have all of its waves moving in the same direction? (a) the mirrors in the laser (b) the stimulated emission of the atoms to radiate in the same direction (c) atoms are lined-up in the crystal so that they emit light only in one direction Link to Chapter 27
Light Emission. Today s Topics. Excitation/De-Excitation 10/26/2008. Excitation Emission Spectra Incandescence
Light Emission Excitation Emission Spectra Incandescence Absorption Spectra Today s Topics Excitation/De-Excitation Electron raised to higher energy level Electron emits photon when it drops back down
2. Discrete means unique, that other states don t overlap it. 3. Electrons in the outer electron shells have greater potential energy.
30 Light Emission Answers and Solutions for Chapter 30 Reading Check Questions 1. At these high frequencies, ultraviolet light is emitted. 2. Discrete means unique, that other states don t overlap it.
Higher -o-o-o- Past Paper questions o-o-o- 3.4 Spectra
Higher -o-o-o- Past Paper questions 1991-2010 -o-o-o- 3.4 Spectra 1992 Q37 The diagram below shows the energy levels for the hydrogen atom. (a) Between which two energy levels would an electron transition
What are the six common sources of light?
What are the six common sources of light? Common light sources include incandescent, fluorescent, laser, neon, tungsten-halogen, and sodium-vapor bulbs. Objects that give off their own light are luminous.
PHYSICS 102N Spring Week 11 Light emission and absorption
PHYSICS 102N Spring 2009 Week 11 Light emission and absorption Accelerated charges emit electromagnetic waves *) Examples: Radio antenna: Alternating voltage drives electrons back and forth 94.9 million
hf = E 1 - E 2 hc = E 1 - E 2 λ FXA 2008 Candidates should be able to : EMISSION LINE SPECTRA
1 Candidates should be able to : EMISSION LINE SPECTRA Explain how spectral lines are evidence for the existence of discrete energy levels in isolated atoms (i.e. in a gas discharge lamp). Describe the
Laboratory Exercise. Atomic Spectra A Kirchoff Potpourri
1 Name: Laboratory Exercise Atomic Spectra A Kirchoff Potpourri Purpose: To examine the atomic spectra from several gas filled tubes and understand the importance of spectroscopy to astronomy. Introduction
Today. Spectra. Thermal Radiation. Wien s Law. Stefan-Boltzmann Law. Kirchoff s Laws. Emission and Absorption. Spectra & Composition
Today Spectra Thermal Radiation Wien s Law Stefan-Boltzmann Law Kirchoff s Laws Emission and Absorption Spectra & Composition Spectrum Originally, the range of colors obtained by passing sunlight through
Types of Spectra. How do spectrum lines form? 3/30/09. Electron cloud. Atom. Nucleus
The electron should be thought of as a distribution or cloud of probability around the nucleus that on average behave like a point particle on a fixed circular path Types of Spectra How do spectrum lines
Earlier we learned that hot, opaque objects produce continuous spectra of radiation of different wavelengths.
Section7: The Bohr Atom Earlier we learned that hot, opaque objects produce continuous spectra of radiation of different wavelengths. Continuous Spectrum Everyone has seen the spectrum produced when white
Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.
The Bohr Atom Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. 1. What is the energy of the emitted photon when an electron drops from the third
Lab: Excited Electrons
Part A: EMISSION SPECTROSCOPY Lab: Excited Electrons According to the Bohr atomic model, electrons orbit the nucleus within specific energy levels. These levels are defined by unique amounts of energy.
Review: Light and Spectra. Absorption and Emission Lines
1 Review: Light and Spectra Light is a wave It undergoes diffraction and other wave phenomena. But light also is made of particles Energy is carried by photons 1 Wavelength energy of each photon Computer
AST 105 Intro Astronomy The Solar System. MIDTERM II: Tuesday, April 5 [covering Lectures 10 through 16]
![AST 105 Intro Astronomy The Solar System. MIDTERM II: Tuesday, April 5 [covering Lectures 10 through 16]](/thumbs/78/77847540.jpg "AST 105 Intro Astronomy The Solar System. MIDTERM II: Tuesday, April 5 [covering Lectures 10 through 16]")
AST 105 Intro Astronomy The Solar System MIDTERM II: Tuesday, April 5 [covering Lectures 10 through 16] REVIEW Light as Information Bearer We can separate light into its different wavelengths (spectrum).
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
Chemistry Lecture #25: Emission Spectra
Chemistry Lecture #25: Emission Spectra We ve learned that electrons orbit the nucleus. We ve also learned that photons are a form of electromagnetic energy that has a frequency and wavelength. In today
Fingerprinting the Stars Lab
Name: Block: Fingerprinting the Stars Lab Background: Every element produces a unique fingerprint of spectral lines. By identifying the spectral features in stellar spectra, we can determine the composition
Chapter 4. Spectroscopy. Dr. Tariq Al-Abdullah
Chapter 4 Spectroscopy Dr. Tariq Al-Abdullah Learning Goals: 4.1 Spectral Lines 4.2 Atoms and Radiation 4.3 Formation of the Spectral Lines 4.4 Molecules 4.5 Spectral Line Analysis 2 DR. T. AL-ABDULLAH
EXPERIMENT 09 OBSERVATION OF SPECTRA
EXPERIMENT 09 OBSERVATION OF SPECTRA INTRODUCTION: In physics, as in very other area of study, one of the most valuable questions a student can learn to ask is, How do they know that? Thus, when you read
Experiment 3 Electromagnetic Radiation and Atom Interaction
Experiment 3 Electromagnetic Radiation and Atom Interaction B OBJECTIVES To be familiar with the relationship between emission line spectra and the energy levels of electrons in various atoms. B INTRODUCTION
Chapter 4 Spectroscopy
Chapter 4 Spectroscopy The beautiful visible spectrum of the star Procyon is shown here from red to blue, interrupted by hundreds of dark lines caused by the absorption of light in the hot star s cooler
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
Lecture5PracticeQuiz.txt
TAKEN FROM HORIZONS 7TH EDITION CHAPTER 6 TUTORIAL QUIZ 1. The difference between radiation and sound is that a. radiation exhibits the Doppler effect, whereas sound does not. b. radiation travels much
10/27/2017 [pgs ]
![10/27/2017 [pgs ]](/thumbs/82/85139288.jpg "10/27/2017 [pgs ]")
Objectives SWBAT explain the relationship between energy and frequency. SWBAT predict the behavior of and/or calculate quantum and photon energy from frequency. SWBAT explain how the quantization of energy
c = λν 10/23/13 What gives gas-filled lights their colors? Chapter 5 Electrons In Atoms
CHEMISTRY & YOU What gives gas-filled lights their colors? Chapter 5 Electrons In Atoms 5.1 Revising the Atomic Model 5. Electron Arrangement in Atoms 5.3 Atomic and the Quantum Mechanical Model An electric
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
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
Conceptual Physics Fundamentals
Conceptual Physics Fundamentals Chapter 15: QUANTUM THEORY This lecture will help you understand: The Photoelectric Effect Absorption Spectra Fluorescence Incandescence Lasers Wave-Particle Duality Particles
A World of Color. Session 2. OLLI at Illinois Spring D. H. Tracy
A World of Color Session 2 OLLI at Illinois Spring 2018 D. H. Tracy Course Outline 1. Overview, History and Spectra 2. Nature and Sources of Light 3. Eyes and Color Vision 4. Origins of Colors of Things
Experiment 24: Spectroscopy
Experiment 24: Spectroscopy Figure 24.1: Spectroscopy EQUIPMENT High Voltage Power Supply Incandescent Light Source (3) Gas Discharge Tubes: 1. Helium 2. Hydrogen 3. Unknown Element Spectrometer Felt (1)
Chemistry 212 ATOMIC SPECTROSCOPY
Chemistry 212 ATOMIC SPECTROSCOPY The emission and absorption of light energy of particular wavelengths by atoms and molecules is a common phenomenon. The emissions/absorptions are characteristic for each
X Rays must be viewed from space used for detecting exotic objects such as neutron stars and black holes also observing the Sun.
6/25 How do we get information from the telescope? 1. Galileo drew pictures. 2. With the invention of photography, we began taking pictures of the view in the telescope. With telescopes that would rotate
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
The Spectroscopy of Stars
The Spectroscopy of Stars In this activity you will use a hand held spectroscope to investigate a number of known and unknown light sources. A spectroscope is an instrument that helps to observe the spectrum
Today. Kirchoff s Laws. Emission and Absorption. Stellar Spectra & Composition. Doppler Effect & Motion. Extrasolar Planets
Today Kirchoff s Laws Emission and Absorption Stellar Spectra & Composition Doppler Effect & Motion Extrasolar Planets Three basic types of spectra Continuous Spectrum Intensity Emission Line Spectrum
APAS Laboratory { PAGE } Spectroscopy SPECTROSCOPY
SPECTROSCOPY SYNOPSIS: In this lab you will eplore different types of emission spectra, calibrate a spectrometer using the spectrum of a known element, and use your calibration to identify an unknown element.
ASTRONOMY. Chapter 5 RADIATION AND SPECTRA PowerPoint Image Slideshow
ASTRONOMY Chapter 5 RADIATION AND SPECTRA PowerPoint Image Slideshow FIGURE 5.1 Our Sun in Ultraviolet Light. This photograph of the Sun was taken at several different wavelengths of ultraviolet, which
Review: Properties of a wave
Radiation travels as waves. Waves carry information and energy. Review: Properties of a wave wavelength (λ) crest amplitude (A) trough velocity (v) λ is a distance, so its units are m, cm, or mm, etc.
What is LIGHT? Reading Question
Reading Question What is LIGHT? A. Light is a wave, like sound only much faster. B. Light is like little particles. Each one is a photon. C. Light is the absence of dark. D. A kind of energy we model with
Chapter 5 Light and Matter: Reading Messages from the Cosmos. 5.1 Light in Everyday Life. How do we experience light?
Chapter 5 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? How do we experience light?
Chapter 5 Light and Matter: Reading Messages from the Cosmos
Chapter 5 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? How do we experience light?
Duncan. Electrons, Energy, & the Electromagnetic Spectrum Notes Simplified, 2-D Bohr Model: Figure 1. Figure 2. Figure 3
Electrons, Energy, & the Electromagnetic Spectrum Notes Simplified, 2-D Bohr Model: Figure 1 Figure 2 Figure 3 Light Calculation Notes Here s how the type/form of EM radiation can be determined The amount
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
From Last Time Pearson Education, Inc.
From Last Time Light: Absorption, Emission, Transmission, Reflection, and Scattering c=λ x f E=h x f Light (electromagnetic radiation) extends from gamma rays (high E, high f, small λ) to radio waves (small
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
Light and Atoms. ASTR 1120 General Astronomy: Stars & Galaxies. ASTR 1120 General Astronomy: Stars & Galaxies !ATH REVIEW: #AST CLASS: "OMEWORK #1
ASTR 1120 General Astronomy: Stars & Galaxies!ATH REVIEW: Tonight, 5-6pm, in RAMY N1B23 "OMEWORK #1 -Due THU, Sept. 10, by 5pm, on Mastering Astronomy CLASS RECORDED STARTED - INFO WILL BE POSTED on CULEARN
We now realize that the phenomena of chemical interactions, and, ultimately life itself, are to be understood in terms of electromagnetism".
We now realize that the phenomena of chemical interactions, and, ultimately life itself, are to be understood in terms of electromagnetism". -Richard Feynman Quantum H Atom Review Radia Wave Function (1s):
Intro to Galaxies Light and Atoms - I
Astrophysics Study of Light Study of Atoms Intro to Galaxies Light and Atoms - I 1 Atomic Physics elements: substances which cannot be broken down into simpler substances atom : smallest unit of an element
Laboratory Atomic Emission Spectrum
Laboratory Atomic Emission Spectrum Pre-Lab Questions: Answer the following questions in complete sentences by reading through the Overview and Background sections below. 1. What is the purpose of the
Lights. And God said, "Let there be light"; and there was light. And God saw that the light was good; (Bible: Genesis I)
Lights Astronomy is based on observing lights from celestial bodies. And God said, "Let there be light"; and there was light. And God saw that the light was good; (Bible: Genesis I) Cat's Eye planetary
Electron Energy and Light
Why? Electron Energy and Light How does light reveal the behavior of electrons in an atom? From fireworks to stars, the color of light is useful in finding out what s in matter. The emission of light by
I understand the relationship between energy and a quanta I understand the difference between an electron s ground state and an electron s excited
NCCS 1.1.2 & 1.1.3 I understand the relationship between energy and a quanta I understand the difference between an electron s ground state and an electron s excited state I will describe how an electron
Chapter 5 Electrons In Atoms
Chapter 5 Electrons In Atoms 5.1 Revising the Atomic Model 5.2 Electron Arrangement in Atoms 5.3 Atomic Emission Spectra and the Quantum Mechanical Model 1 Copyright Pearson Education, Inc., or its affiliates.
Bright line spectrum questions
Base your answers to questions 1 and 2 on the information below and on your knowledge of chemistry. The bright-line spectra for four elements and a mixture of elements are shown in the diagram below. 1.
What are the three basic types of spectra?
Learning from Light Our goals for learning What are the three basic types of spectra? How does light tell us what things are made of? How does light tell us the temperatures of planets and stars? How do
1. Is the spectrum below a. an absorption line one b. a continuum c. an emission line one d. Doppler shifted e. unresolved
NatSci102 Due Feb. 14 Professor G. Rieke Homework on spectroscopy, colors, and light. Answers should be entered on a Scantron form given out in class. This exercise is worth 30 points (25 questions plus
Light. October 14, ) Exam Review 2) Introduction 3) Light Waves 4) Atoms 5) Light Sources
Light October 14, 2002 1) Exam Review 2) Introduction 3) Light Waves 4) Atoms 5) Light Sources Waves You know of many types of waves water, sound, seismic, etc A wave is something oscillating back and
Chapter 5 Light and Matter: Reading Messages from the Cosmos. What is light? Properties of Waves. Waves. The Electromagnetic Spectrum
Chapter 5 Light and Matter: Reading Messages from the Cosmos What is light? Light is a form of radiant energy Light can act either like a wave or like a particle (photon) Spectrum of the Sun 1 2 Waves
aka Light Properties of Light are simultaneously
Today Interaction of Light with Matter Thermal Radiation Kirchhoff s Laws aka Light Properties of Light are simultaneously wave-like AND particle-like Sometimes it behaves like ripples on a pond (waves).
Light is an important form of energy for all of us
What is Light? Light is an important form of energy for all of us it allows us to see plants rely on light for photosynthesis many chemical reactions produce light life on Earth would not exist without
Atomic Spectra. d sin θ = mλ (1)
Atomic Spectra Objectives: To measure the wavelengths of visible light emitted by atomic hydrogen and verify that the measured wavelengths obey the empirical Rydberg formula. To observe emission spectra
Unit 3. Chapter 4 Electrons in the Atom. Niels Bohr s Model. Recall the Evolution of the Atom. Bohr s planetary model
Unit 3 Chapter 4 Electrons in the Atom Electrons in the Atom (Chapter 4) & The Periodic Table/Trends (Chapter 5) Niels Bohr s Model Recall the Evolution of the Atom He had a question: Why don t the electrons
A fresh look at light: build your own spectrometer
Image courtesy of National Optical Astronomy Observatory/Association of Universities for Research in Astronomy/National Science Foundation A fresh look at light: build your own spectrometer A high-resolution
Next quiz: Monday, October 24
No homework for Wednesday Read Chapter 8! Next quiz: Monday, October 24 1 Chapter 7 Atoms and Starlight Types of Spectra: Pictorial Some light sources are comprised of all colors (white light). Other light
WAVE NATURE OF LIGHT
WAVE NATURE OF LIGHT Light is electromagnetic radiation, a type of energy composed of oscillating electric and magnetic fields. The fields oscillate perpendicular to each other. In vacuum, these waves
Spectroscopy of Various Light Sources: The Interactions between Light and Matter ASTR 170B1, Spring 2017, Lab #2. 1 Introduction.
Spectroscopy of Various Light Sources: The Interactions between Light and Matter ASTR 170B1, Spring 2017, Lab #2 DUE IN CLASS ON Thursday Sept 28! You CAN work in a group of 2, but you need only turn in
HOMEWORK - Chapter 4 Spectroscopy
Astronomy 10 HOMEWORK - Chapter 4 Spectroscopy Use a calculator whenever necessary. For full credit, always show your work and explain how you got your answer in full, complete sentences on a separate
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,
Chapter 5: Light and Matter: Reading Messages from the Cosmos
Chapter 5 Lecture Chapter 5: Light and Matter: Reading Messages from the Cosmos Light and Matter: Reading Messages from the Cosmos 5.1 Light in Everyday Life Our goals for learning: How do we experience
Chapter 28 Assignment Solutions
Chapter 28 Assignment Solutions Page 770 #23-26, 29-30, 43-48, 55 23) Complete the following concept map using these terms: energy levels, fixed electron radii, Bohr model, photon emission and absorption,
ASTR-1010: Astronomy I Course Notes Section IV
ASTR-1010: Astronomy I Course Notes Section IV Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use
Assignments. For Wed. 1 st Midterm is Friday, Oct. 12. Do Online Exercise 08 ( Doppler shift tutorial)
Assignments For Wed. Do Online Exercise 08 ( Doppler shift tutorial) 1 st Midterm is Friday, Oct. 12 Chapter 5 Light: The Cosmic Messenger Which forms of light are lower in energy and frequency than the
Light sources. Excited gas atoms are the primaty source of radiation in combustion and discharge lamps. lamps is not continuous!
Light sources Excited gas atoms are the primaty source of radiation in combustion and discharge lamps. Continuous spectrum: black body radiation Characteristic spectrum: emission lines Absorption lines
Interested in exploring science or math teaching as a career?
Interested in exploring science or math teaching as a career? Start with Step 1: EDUC 2020 (1 credit) Real experience teaching real kids! No commitment to continue with education courses Registration priority
Taking Fingerprints of Stars, Galaxies, and Other Stuff. The Bohr Atom. The Bohr Atom Model of Hydrogen atom. Bohr Atom. Bohr Atom
Periodic Table of Elements Taking Fingerprints of Stars, Galaxies, and Other Stuff Absorption and Emission from Atoms, Ions, and Molecules Universe is mostly (97%) Hydrogen and Helium (H and He) The ONLY
Lecture Outline: Spectroscopy (Ch. 4)
Lecture Outline: Spectroscopy (Ch. 4) NOTE: These are just an outline of the lectures and a guide to the textbook. The material will be covered in more detail in class. We will cover nearly all of the
P O G I L E L E C T R O N E N E R G Y A N D L I G H T
South Pasadena Honors Chemistry Name 9 Atomic Structure Period Date Why? P O G I L E L E C T R O N E N E R G Y A N D L I G H T How does light reveal the behavior of electrons in an atom? From fireworks
The Bohr Model of the Atom
Unit 4: The Bohr Model of the Atom Properties of light Before the 1900 s, light was thought to behave only as a wave. Light is a type of electromagnetic radiation - a form of energy that exhibits wave
Today in Space News: Pluto and Charon tattle on missing Kuiper Belt objects
Today in Space News: Pluto and Charon tattle on missing Kuiper Belt objects Study Points Define blackbody radiation. Draw two graphs of intensity vs wavelength for the low temperature object (reddish)
(in case you missed it yesterday ) Merger of Two Neutron Stars!
(in case you missed it yesterday ) Merger of Two Neutron Stars! https://cmns.umd.edu/news-events/features/3997 More on this later in the semester Lecture #14: Plan Light (cont d) Atomic physics Formation
The Nature of Light. Chapter Five
The Nature of Light Chapter Five Guiding Questions 1. How fast does light travel? How can this speed be measured? 2. Why do we think light is a wave? What kind of wave is it? 3. How is the light from an
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
PHYSICS 3204 PUBLIC EXAM QUESTIONS (Quantum pt.1)
PHYSICS 3204 PUBLIC EXAM QUESTIONS (Quantum pt.1) NAME: August 2009--------------------------------------------------------------------------------------------------------------------------------- 11 41.
Parallax: Space Observatories. Stars, Galaxies & the Universe Announcements. Stars, Galaxies & Universe Lecture #7 Outline
Stars, Galaxies & the Universe Announcements HW#4: posted Thursday; due Monday (9/20) Reading Quiz on Ch. 16.5 Monday (9/20) Exam #1 (Next Wednesday 9/22) In class (50 minutes) first 20 minutes: review
ATOMIC SPECTRA. To identify elements through their emission spectra. Apparatus: spectrometer, spectral tubes, power supply, incandescent lamp.
ATOMIC SPECTRA Objective: To measure the wavelengths of visible light emitted by atomic hydrogen and verify the measured wavelengths against those predicted by quantum theory. To identify elements through
EM SPECTRUM, WAVELENGTH, FREQUENCY, AND ENERGY WORKSHEET
EM SPECTRUM, WAVELENGTH, FREQUENCY, AND ENERGY WORKSHEET 1.) Look at the EM spectrum below to answer this question. As you move across the visible light spectrum from red to violet (A) Does the wavelength
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?
The Electromagnetic Spectrum
The Electromagnetic Spectrum Outcomes: http://www.avclub.com/article/marvel-made-its-own-movies-ang-lee-offered-idiosyn-204118 Qualitatively describe the electromagnetic spectrum in terms of frequency,
PH300 Spring Homework 06
PH300 Spring 2011 Homework 06 Total Points: 30 1. (1 Point) Each week you should review both your answers and the solutions for the previous week's homework to make sure that you understand all the questions
Lecture 7. Outline. ASTR 111 Section 002. Discuss Quiz 5 Light. Light travels through empty space at a speed of 300,000 km/s
Lecture 7 ASTR 111 Section 002 Outline Discuss Quiz 5 Light Suggested reading: Chapter 5.1-5.2 and 5.6-5.8 of textbook Light travels through empty space at a speed of 300,000 km/s In 1676, Danish astronomer
Chapter 5 Electrons In Atoms
Chapter 5 Electrons In Atoms 5.1 Revising the Atomic Model 5.2 Electron Arrangement in Atoms 5.3 Atomic Emission Spectra and the Quantum Mechanical Model 1 Copyright Pearson Education, Inc., or its affiliates.
Atoms and Spectra October 8th, 2013
Atoms and Spectra October 8th, 2013 Announcements Second writing assignment due two weeks from today (again, on a news item of your choice). Be sure to make plans to visit one of the open observing nights
Classification of Electromagnetic Radiation
Light and Energy Electromagnetic Radiation Radiant energy that exhibits wavelength-like behavior and travels through space at the speed of light in a vacuum. Example: The sun light, energy used in microwave
Atomic Theory C &03
Atomic Theory Part One: Flame Tests Part Two: Atomic Spectra Part Three: Applications of Spectra (optional) C12-2-02 &03 This activity will focus on the visible portion of the electromagnetic spectrum.
Experiment 7: Spectrum of the Hydrogen Atom
Experiment 7: Spectrum of the Hydrogen Nate Saffold nas2173@columbia.edu Office Hour: Mondays, 5:30-6:30PM INTRO TO EXPERIMENTAL PHYS-LAB 1493/1494/2699 Introduction The physics behind: The spectrum of
Homework on spectroscopy, colors, and light. Answers should be entered on a Scantron form given out in class. This exercise is worth 20 points.
Astr. 170B1 Due Sept. 20 Professors Rieke Homework on spectroscopy, colors, and light. Answers should be entered on a Scantron form given out in class. This exercise is worth 20 points. 1. Is the spectrum
Introduction to light Light is a form of energy called electromagnetic radiation. A chart of the electromagnetic spectrum is shown below.
Experiment: Spectroscopy Introduction to light Light is a form of energy called electromagnetic radiation. A chart of the electromagnetic spectrum is shown below. Radiowave Microwave Infrared Visible Ultraviolet
Experiment #9. Atomic Emission Spectroscopy
Introduction Experiment #9. Atomic Emission Spectroscopy Spectroscopy is the study of the interaction of light with matter. This interaction can be in the form of the absorption or the emission of electromagnetic
Light and Matter(LC)
Light and Matter(LC) Every astronomy book that I ve seen has at least one chapter dedicated to the physics of light. Why are astronomers so interested in light? Everything* that we know about Astronomical
Module 1. Illumination Engineering Basics. Version 2 EE IIT, Kharagpur 1
Module 1 Illumination Engineering Basics Version 2 EE IIT, Kharagpur 1 Lesson 2 Radiation Version 2 EE IIT, Kharagpur 2 Instructional objectives 1. State the Visible Range of light. 2. State the range