Fingerprinting the Stars Lab

Size: px
Start display at page:

Download "Fingerprinting the Stars Lab"

Transcription

1 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 and temperature of stars. You will see two kinds of spectra, a continuous spectrum (rainbow) and a line spectra (either bright or dark lines at specific colors). A continuous spectrum- light emitted by anything that is very hot and dense (stars). This rainbow of light of all energies is created because hot, dense objects contain many loose electrons which can emit photons of any energy. A line Spectrum- result of bound electrons in atoms jumping between energy levels. It takes the right amount of energy to move between an energy level. This amount of energy is a certain color of light. In this lab we will use a special lamp that sends a strong current through the substance that triggers it to emit its signature line spectrum. This special lamp is called a discharge lamp and it holds a glass tube filled with gas. When the discharge lamp is turned on the electrons then get excited causing the gas to glow. Procedure: 1. Look at the light in the room through the spectroscope. Describe what you see. Include the colors observed AND the corresponding number. 2. Which color has the longest wavelength? 3. Which color has the shortest wavelength? 4. In the darkened classroom you will see several light sources. Each light source produces light by passing a very high voltage through a gas such as neon, hydrogen, mercury, water vapor etc. Record the name of the chemical element providing the light. On the spectra data sheet draw the lines you see. Try to place the lines as accurately as you can in each color range. You may wish to try to match the color with colored pencils.

2

3 The following pages contain information about the spectra of specific elements and the spectra of 5 stars. Worksheet 1 contains the spectra for 7 elements commonly found in star. These spectra do not show colors, however light at the 4000 angstrom end of the spectrum is violet and light at the 6800 angstrom end of the spectrum is red. Worksheet 2 shows the spectra from 5 different stars. Obviously, stars are made of a variety of elements. Use these worksheets to answer the following questions. 5. What elements are in each star? Check the box is that element is present. Star 1 Hydrogen Iron Neon Sodium Lithium Magnesium Helium Star 2 Star 3 Star 4 Star 5 6. What elements are in every star? 7. Based on your knowledge of star formation, explain why all stars contain that/those element(s). 8. What stars contain all seven elements? 9. Make a prediction about the size and temperature of the star that contain all of the elements. Conclusion: 10. How is it possible for scientists to know the composition of stars without traveling to the star? 11. True or false, every gas has a unique sent of spectral lines that help identify the gas.

4 12. Predict what would happen to the spectral lines if this discharge lamp were moving away from you similar to how galaxies are moving away from each other. Hint: do not just put the lines will get fainter. Conclusion: For Honors Only 13. Write a one paragraph conclusion about this lab activity. In other words, what can you conclude about the visible spectrum of different stars and gases? Remember, a conclusion is a new idea or concept that you learned from analyzing the data available. Defend your conclusion with data obtained in the lab activity.

5

6

Student Lab Investigation

Student Lab Investigation Student Lab Investigation Prediction: You have seen that white light has a definite spectrum. Would you predict that different colors of light have different spectra from each other? Will they be different

More information

Laboratory Atomic Emission Spectrum

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

More information

Fingerprinting the Stars Lab (Sarah Hansen & Monica Valluri)

Fingerprinting the Stars Lab (Sarah Hansen & Monica Valluri) Fingerprinting the Stars Lab (Sarah Hansen & Monica Valluri) Introduction Every element produces a unique fingerprint of spectral lines. By identifying the spectral features in stellar spectra, we can

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

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. 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

More information

Observation of Atomic Spectra

Observation of Atomic Spectra Observation of Atomic Spectra Introduction In this experiment you will observe and measure the wavelengths of different colors of light emitted by atoms. You will first observe light emitted from excited

More information

Bright line spectrum questions

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.

More information

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

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

More information

Laboratory Exercise. Atomic Spectra A Kirchoff Potpourri

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

More information

Visible spectrum 1. Spectroscope. Name:

Visible spectrum 1. Spectroscope. Name: Name: Visible spectrum 1 You know by now that different atoms have different configurations of electrons. You also know that electrons generate electromagnetic waves when they oscillate (remember that

More information

ACTIVITY 2 Exploring Light Patterns

ACTIVITY 2 Exploring Light Patterns Name: Class: SOLIDS & Visual Quantum Mechanics LIGHT ACTIVITY 2 Exploring Light Patterns Goal We will continue to investigate the properties of LEDs and the incandescent lamp by observing and exploring

More information

Electron Energy and Light

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

More information

Pre-Lab Exercises Lab 2: Spectroscopy

Pre-Lab Exercises Lab 2: Spectroscopy Pre-Lab Exercises Lab 2: Spectroscopy 1. Which color of visible light has the longest wavelength? Name Date Section 2. List the colors of visible light from highest frequency to lowest frequency. 3. Does

More information

Chapter 8. Spectroscopy. 8.1 Purpose. 8.2 Introduction

Chapter 8. Spectroscopy. 8.1 Purpose. 8.2 Introduction Chapter 8 Spectroscopy 8.1 Purpose In the experiment atomic spectra will be investigated. The spectra of three know materials will be observed. The composition of an unknown material will be determined.

More information

INSIDE LAB 5: Spectroscopic Identification of Gaseous Elements

INSIDE LAB 5: Spectroscopic Identification of Gaseous Elements INSIDE LAB 5: Spectroscopic Identification of Gaseous Elements OBJECTIVE: To examine the light emitted by glowing gases in order to identify the elements that compose the gases. DISCUSSION: If a gas is

More information

CSUS Department of Chemistry Experiment 9 Chem. 1A

CSUS Department of Chemistry Experiment 9 Chem. 1A CSUS Department of Chemistry xperiment 9 Chem. 1A xp. 9 PR-Lab ASSIGNMNT Name: Lab Section (1) Use equation (2) [see the discussion on the next page] to calculate the energies of the ten lowest states

More information

Introduction to light Light is a form of energy called electromagnetic radiation. A chart of the electromagnetic spectrum is shown below.

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

More information

Electron Energy and Light

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

More information

Physics Lab #2: Spectroscopy

Physics Lab #2: Spectroscopy Physics 10263 Lab #2: Spectroscopy Introduction This lab is meant to serve as an introduction to the science of spectroscopy. In this lab, we ll learn about how emission and absorption works, and we ll

More information

Duncan. Electrons, Energy, & the Electromagnetic Spectrum Notes Simplified, 2-D Bohr Model: Figure 1. Figure 2. Figure 3

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

More information

Lab: Excited Electrons

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.

More information

Atomic Theory C &03

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.

More information

ACTIVITY 1. Exploring Light from Gases

ACTIVITY 1. Exploring Light from Gases Name: WAVES of matter Class: Visual Quantum Mechanics ACTIVITY 1 Exploring Light from Gases Goal We will view the colors of light which are emitted by different gases. From these patterns of light we gain

More information

APAS Laboratory { PAGE } Spectroscopy SPECTROSCOPY

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.

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

Sun Building Activity 2 The Signature of the Stars

Sun Building Activity 2 The Signature of the Stars Sun Building The Signature of the Stars Rainbows reveal that white light is a combination of all the colours. In 1666, Isaac Newton showed that white light could be separated into its component colours

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

Chemistry 212 ATOMIC SPECTROSCOPY

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

More information

Color. 3. Why are the color labels in the table above plural (i.e., Reds rather than Red )?

Color. 3. Why are the color labels in the table above plural (i.e., Reds rather than Red )? NS D3 Electron Energy and Light Name From fireworks to stars, the color of light is useful in finding out what s in matter. The emission of light by hydrogen and other atoms has played a key role in understanding

More information

What are the six common sources of light?

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.

More information

Light Emission.

Light Emission. Light Emission www.physics.sfasu.edu/friedfeld/ch29lec.ppt Radio waves are produced by electrons moving up and down an antenna. Visible light is produced by electrons changing energy states in an atom.

More information

Atomic Spectra Introduction

Atomic Spectra Introduction Atomic Spectra Introduction: Light and all other electromagnetic radiation is energy that is emitted in the form of waves. Thus light behaves like a wave, and the energy of light varies with the wavelength

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

Atomic Emission Spectra

Atomic Emission Spectra Atomic Emission Spectra Objectives The objectives of this laboratory are as follows: To build and calibrate a simple meter-stick spectroscope that is capable of measuring wavelengths of visible light.

More information

PHYSICS 116 SPECTROSCOPY: DETERMINATION OF THE WAVELENGTH OF LIGHT

PHYSICS 116 SPECTROSCOPY: DETERMINATION OF THE WAVELENGTH OF LIGHT Name Date Lab Time Lab TA PHYSICS 116 SPECTROSCOPY: DETERMINATION OF THE WAVELENGTH OF LIGHT I. PURPOSE To use a diffraction grating to investigate the spectra produced by several unknown gas discharge

More information

EXPERIMENT 09 OBSERVATION OF SPECTRA

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

More information

Emission Spectroscopy

Emission Spectroscopy Objectives Emission Spectroscopy Observe spectral lines from a hydrogen gas discharge tube Determine the initial and final energy levels for the electronic transitions associated with the visible portion

More information

Experiment 3 Electromagnetic Radiation and Atom Interaction

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

More information

2. Why do the discharge tubes get hot after running for a period of time?

2. Why do the discharge tubes get hot after running for a period of time? EXPERIIMENT #2 FLAME TESTS Note: Experiments #2 and #3 can be completed together in a single lab period (90 minutes). A combined data sheet for the two labs can be found after Experiment #3. Discussion:

More information

Using the spectrometer

Using the spectrometer MATERIALS LIST Investigation 13.1 Stars and Spectroscopy 4 Spectrometer (also known as a spectroscope) 4 Colored pencils 4 Incandescent light source ChAPTER 13 The Universe How can we use a spectrometer

More information

high energy state for the electron in the atom low energy state for the electron in the atom

high energy state for the electron in the atom low energy state for the electron in the atom Atomic Spectra Objectives The objectives of this experiment are to: 1) Build and calibrate a simple spectroscope capable of measuring wavelengths of visible light. 2) Measure several wavelengths of light

More information

Unit 3 Atomics Repair Problems

Unit 3 Atomics Repair Problems 1. What is the charge of the nucleus in an atom of oxygen-17? A) 0 B) 2 C) +8 D) +17 2. A neutral atom contains 12 neutrons and 11 electrons. The number of protons in this atom is A) 1 B) 11 C) 12 D) 23

More information

EM SPECTRUM, WAVELENGTH, FREQUENCY, AND ENERGY WORKSHEET

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

More information

Parallax: Space Observatories. Stars, Galaxies & the Universe Announcements. Stars, Galaxies & Universe Lecture #7 Outline

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

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

Emission of Light: Discharge Lamps & Flame Tests 1

Emission of Light: Discharge Lamps & Flame Tests 1 Emission of Light: Discharge Lamps & Flame Tests 1 Objectives At the end of this activity you should be able to: o Describe how discharge lamps emit photons following electrical excitation of gaseous atoms.

More information

ATOMIC SPECTRA. To identify elements through their emission spectra. Apparatus: spectrometer, spectral tubes, power supply, incandescent lamp.

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

More information

Higher -o-o-o- Past Paper questions o-o-o- 3.4 Spectra

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

More information

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] 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).

More information

hf = E 1 - E 2 hc = E 1 - E 2 λ FXA 2008 Candidates should be able to : EMISSION LINE SPECTRA

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

More information

History of the Universe Unit Tracking Sheet

History of the Universe Unit Tracking Sheet Name Period Mrs. Coates Earth Science History of the Universe Unit Tracking Sheet Learning Target Question Example Date Target was Taught in Class The Big Bang Theory explains how the universe formed The

More information

THE DIFFRACTION GRATING SPECTROMETER

THE DIFFRACTION GRATING SPECTROMETER Purpose Theory THE DIFFRACTION GRATING SPECTROMETER a. To study diffraction of light using a diffraction grating spectrometer b. To measure the wavelengths of certain lines in the spectrum of the mercury

More information

5.3. Physics and the Quantum Mechanical Model

5.3. Physics and the Quantum Mechanical Model Chemistry 5-3 Physics and the Quantum Mechanical Model Neon advertising signs are formed from glass tubes bent in various shapes. An electric current passing through the gas in each glass tube makes the

More information

The relationship between these aspects is described by the following equation: E = hν =

The relationship between these aspects is described by the following equation: E = hν = 1 Learning Outcomes EXPERIMENT A10: LINE SPECTRUM Upon completion of this lab, the student will be able to: 1) Examine the line spectrum of the hydrogen atom. 2) Calculate the frequency and energy of the

More information

UNIT 4: The Periodic Table! Lesson 4.1: Bright-Line Spectra. Protons Neutrons Electron

UNIT 4: The Periodic Table! Lesson 4.1: Bright-Line Spectra. Protons Neutrons Electron Name: Date: Chemistry ~ Ms. Hart Class: Anions or Cations DO NOW: About Neon-20 UNIT 4: The Periodic Table! Lesson 4.1: Bright-Line Spectra Amount of each Mass of each Protons Neutrons Electron Location

More information

Instructor Resources

Instructor Resources SPECTROSCOPY Quantitative Analysis with Light Instructor Resources Learning Objectives The objectives of this experiment are to: identify band and line spectra, and relate the physical state of a light-emitting

More information

2. Discrete means unique, that other states don t overlap it. 3. Electrons in the outer electron shells have greater potential energy.

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.

More information

1. Is the spectrum below a. an absorption line one b. a continuum c. an emission line one d. Doppler shifted e. unresolved

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

More information

What can laser light do for (or to) me?

What can laser light do for (or to) me? What can laser light do for (or to) me? Phys 1020, Day 15: Questions? Refection, refraction LASERS: 14.3 Next Up: Finish lasers Cameras and optics 1 Eyes to web: Final Project Info Light travels more slowly

More information

For instance, for a particular star cluster, these data were derived:

For instance, for a particular star cluster, these data were derived: Astronomy 100 Name(s): Exercise 5: The H-R diagram and spectroscopy A very basic correlation using the color index By the 1920 s, various astronomers had evidence that the temperature of a star was also

More information

Name: Partner(s): 1102 or 3311: Desk # Date: Spectroscopy Part I

Name: Partner(s): 1102 or 3311: Desk # Date: Spectroscopy Part I Name: Partner(s): 1102 or 3311: Desk # Date: Spectroscopy Part I Purpose Investigate Kirchhoff s Laws for continuous, emission and absorption spectra Analyze the solar spectrum and identify unknown lines

More information

Atomic Spectra for Atoms and Ions. Light is made up of different wavelengths

Atomic Spectra for Atoms and Ions. Light is made up of different wavelengths Atomic Spectra for Atoms and Ions What will you be doing in lab next week? Recording the line spectra of several different substances in discharge tubes. Recording the line spectra of several ions from

More information

The Electromagnetic Spectrum

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,

More information

Intro to Galaxies Light and Atoms - I

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

More information

Atomic Physics Worksheet. between 4000 and 5000 Angstroms ( nanometers): between 6500 and 7500 Angstroms ( nanometers):

Atomic Physics Worksheet. between 4000 and 5000 Angstroms ( nanometers): between 6500 and 7500 Angstroms ( nanometers): Atomic Physics Worksheet 1. Which of the gas samples shows an emission line with a wavelength between 4000 and 5000 Angstroms (400-500 nanometers): between 6500 and 7500 Angstroms (650-750 nanometers):

More information

What is LIGHT? Reading Question

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

More information

Physics and the Quantum Mechanical Model

Physics and the Quantum Mechanical Model chemistry 1 of 38 Mechanical Model Neon advertising signs are formed from glass tubes bent in various shapes. An electric current passing through the gas in each glass tube makes the gas glow with its

More information

Homework on spectroscopy, colors, and light. Answers should be entered on a Scantron form given out in class. This exercise is worth 20 points.

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

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

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

Experiment 12: SPECTROSCOPY: EMISSION & ABSORPTION

Experiment 12: SPECTROSCOPY: EMISSION & ABSORPTION Sample Experiment 12: SPECTROSCOPY: EMISSION & ABSORPTION Purpose: Emission and absorption spectroscopy is to be explored from different perspectives in a multipart experiment. Part I: Certain elements

More information

Astronomy 101 Lab: Spectra

Astronomy 101 Lab: Spectra Name: Astronomy 101 Lab: Spectra You will access your textbook in this lab. Pre-Lab Assignment: In class, we've talked about different kinds of spectra and what kind of object produces each kind of spectrum.

More information

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 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

More information

Atomic Spectra: Energy, Light, and the Electron

Atomic Spectra: Energy, Light, and the Electron Atomic Spectra: Energy, Light, and the Electron Introduction: An atom consists of a nucleus, containing protons and neutrons, and tiny electrons, which move around the nucleus. Picture a beehive where

More information

Spectroscopy. Materials Diffraction grating Grating tube Spectrometer Incandescent light source

Spectroscopy. Materials Diffraction grating Grating tube Spectrometer Incandescent light source Name: Date: Spectroscopy Hazards: The power supply used to run the lights is HIGH VOLTAGE. You should not need to change any tubes, but if you do please call the instructor over for assistance, and turn

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

Electrons, Energy, & the Electromagnetic Spectrum Notes Simplified, 2-D Bohr Model: Figure 2. Figure 3 UNIT 4 - ELECTRONS & ELECTRON ARRANGEMENT

Electrons, Energy, & the Electromagnetic Spectrum Notes Simplified, 2-D Bohr Model: Figure 2. Figure 3 UNIT 4 - ELECTRONS & ELECTRON ARRANGEMENT Electrons, Energy, & the Electromagnetic Spectrum Notes Simplified, 2-D Bohr Model: Figure 1 UNIT 4 - ELECTRONS & ELECTRON ARRANGEMENT Figure 2 Figure 3 The energy is released as electromagnetic radiation.

More information

Planetary Science: Investigations 9-10 I-Check Quiz STUDY GUIDE- ANSWER KEY Name HR Date

Planetary Science: Investigations 9-10 I-Check Quiz STUDY GUIDE- ANSWER KEY Name HR Date 1. How are different types of radiation arranged along the electromagnetic spectrum? A. By how fast they travel incorrect answer B. By their sources incorrect answer C. By the amount of energy they carry

More information

Why do the lights in Times Square differ from sunlight?

Why do the lights in Times Square differ from sunlight? Work hard. Be nice. Name: KIPP NYC College Prep Period: UNIT 3: Electrons Date: General Chemistry Lesson 1: Bright- Line Spectra By the end of today, you will have an answer to: Do NOW: Why do the lights

More information

TWINKLE, TWINKLE LITTLE STAR HOW ASTRONOMERS KNOW WHAT YOU ARE. View the white lights in the room with the diffraction glasses. What do you see?

TWINKLE, TWINKLE LITTLE STAR HOW ASTRONOMERS KNOW WHAT YOU ARE. View the white lights in the room with the diffraction glasses. What do you see? Name Partner(s) Section Date TWINKLE, TWINKLE LITTLE STAR HOW ASTRONOMERS KNOW WHAT YOU ARE Since journeys to the stars are not possible at this time, astronomers use every source of information available

More information

Emission Spectrum of Atomic Gases. Prelab Questions

Emission Spectrum of Atomic Gases. Prelab Questions Emission Spectrum of Atomic Gases Prelab Questions Before this coming to this lab, please review your text for the physics of the spectrum of visible light and of diffraction grating spectrometer.. Which

More information

Experiment 7: Spectrum of the Hydrogen Atom

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

More information

Spectrum of Hydrogen. Physics 227 Lab

Spectrum of Hydrogen. Physics 227 Lab Introduction In today's lab you will be dealing with an area of physics called quantum mechanics. The only quantum mechanical idea that you will be using today is that electrons in an atom can exist only

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

Collegiate Institute for Math and Science Day 57: December 9, 2016 Room 427

Collegiate Institute for Math and Science Day 57: December 9, 2016 Room 427 Unit 2: Atomic Concepts Outline Name: Period: Date: 1. The modern model of the atom has evolved over a long period of time through the work of many scientists. Dalton s Model: Elements are made of atoms

More information

Arrangement of Electrons in the Atom

Arrangement of Electrons in the Atom Arrangement of Electrons in the Atom Bohr s Study of Atomic Spectra When white light is passed through a prism, the white light is broken up into an array of colours. This spread of colours is called a

More information

Today is Thursday, March (!) 1 st, 2018

Today is Thursday, March (!) 1 st, 2018 In This Lesson: Atomic Emissions (Lesson 2 of 4) Stuff You Need: Calculator Today is Thursday, March (!) 1 st, 2018 Pre-Class: [choose one] What is white light? How are fireworks made to be different colors?

More information

Multiple Choice Identify the letter of the choice that best completes the statement or answers the question.

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

More information

Experiment 24: Spectroscopy

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)

More information

The Emission Spectra of Light

The Emission Spectra of Light The Emission Spectra of Light Objectives: Theory: 1.... measured the wavelength limits of the color bands in the visible spectrum, 2.... measured the wavelengths of the emission lines of the hydrogen Balmer

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

THE SPECTRUM OF A STAR

THE SPECTRUM OF A STAR THE SPECTRUM OF A STAR Overview: Stars can be classified by using the general shape and specific lines of their spectra. Objectives: The student will: perform a simple analysis of spectral lines to classify

More information

SPECTROSCOPY: A KEY TO ELEMENTAL IDENTITY

SPECTROSCOPY: A KEY TO ELEMENTAL IDENTITY AME PARTERS SECTIO DATE SPECTROSCOPY: A KEY TO ELEMETAL IDETITY This activity is designed to introduce visible light spectroscopy as a means of identifying elements and providing information on atomic

More information

What are the energies (J) and wavelengths (in nm) for these colors? Color Energy wavelength. Rev. F11 Page 1 of 5

What are the energies (J) and wavelengths (in nm) for these colors? Color Energy wavelength. Rev. F11 Page 1 of 5 Exp. 8 Pre Lab ASSIGNMENT Name: Lab Section Score: / 10 (1) Use the equations [see the discussion on the next page] to calculate the energies of the 6 lowest states for the hydrogen atom, and enter your

More information

The Spectroscopy of Stars

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

More information

NORTHERN ILLINOIS UNIVERSITY PHYSICS DEPARTMENT. Physics 211 E&M and Quantum Physics Spring Lab #9: Diffraction Spectroscopy

NORTHERN ILLINOIS UNIVERSITY PHYSICS DEPARTMENT. Physics 211 E&M and Quantum Physics Spring Lab #9: Diffraction Spectroscopy NORTHERN ILLINOIS UNIVERSITY PHYSICS DEPARTMENT Physics 211 E&M and Quantum Physics Spring 2018 Lab #9: Diffraction Spectroscopy Lab Writeup Due: Mon/Wed/Thu/Fri, April 30/ May 2/3/4, 2018 Background All

More information

Experiment 9. Emission Spectra. measure the emission spectrum of a source of light using the digital spectrometer.

Experiment 9. Emission Spectra. measure the emission spectrum of a source of light using the digital spectrometer. Experiment 9 Emission Spectra 9.1 Objectives By the end of this experiment, you will be able to: measure the emission spectrum of a source of light using the digital spectrometer. find the wavelength of

More information

DIFFRACTION GRATING. OBJECTIVE: To use the diffraction grating in the formation of spectra and in the measurement of wavelengths.

DIFFRACTION GRATING. OBJECTIVE: To use the diffraction grating in the formation of spectra and in the measurement of wavelengths. DIFFRACTION GRATING OBJECTIVE: To use the diffraction grating in the formation of spectra and in the measurement of wavelengths. THEORY: The operation of the grating is depicted in Fig. 1 on page Lens

More information

Spectrometers. Materials: Easy Spectrometer. Old CD Razor Index card Cardboard tube at least 10 inches long

Spectrometers. Materials: Easy Spectrometer. Old CD Razor Index card Cardboard tube at least 10 inches long Spectrometers Overview: Spectrometers (spectroscopes) are used in chemistry and astronomy to measure light. In astronomy, we can find out about distant stars without ever traveling to them, because we

More information

Tuesday, August 27, Stellar Astrophysics

Tuesday, August 27, Stellar Astrophysics Stellar Astrophysics Policies No Exams Homework 65% Project 35% Oral Presentation 5% More on the project http://myhome.coloradomesa.edu/ ~jworkman/teaching/fall13/396/ syllabus396.pdf You need to self

More information