The Electromagnetic Spectrum

Similar documents
The Theory of Electromagnetism

Light and Matter(LC)

Light: Transverse WAVE

Reading for Meaning and the Electromagnetic Spectrum!

The Nature of Light. We have a dual model

Astronomy The Nature of Light

9/16/08 Tuesday. Chapter 3. Properties of Light. Light the Astronomer s Tool. and sometimes it can be described as a particle!

The Nature of Light. Chapter Five

Lecture 7. Outline. ASTR 111 Section 002. Discuss Quiz 5 Light. Light travels through empty space at a speed of 300,000 km/s

Topics Covered in Chapter. Light and Other Electromagnetic Radiation. A Subatomic Interlude II. A Subatomic Interlude. A Subatomic Interlude III

Light and Other Electromagnetic Radiation

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

Next Homework Due Oct. 9. Coming up: The Sun (Chapter 10)

HOMEWORK - Chapter 4 Spectroscopy

4. Our eyes can only see a small band of the entire spectrum of light. A) True B) False

Telescopes have Three Powers

The Sine Wave. You commonly see waves in the environment. Light Sound Electricity Ocean waves

Light carries energy. Lecture 5 Understand Light. Is light. Light as a Particle. ANSWER: Both.

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

The Electromagnetic Spectrum

ASTRONOMY. Chapter 5 RADIATION AND SPECTRA PowerPoint Image Slideshow

The nature of light. Speed of light. Nature of light. Light - a wave. EM radiation. Beyond the visible. The EM spectrum.

Grade 8 Science: Unit 3-Optics Chapter 4: Properties of Light

PHYS 160 Astronomy Test #2 Fall 2017 Version A

How do we get information about heavenly bodies when they are so far??

Chapter 5 Light: The Cosmic Messenger. Copyright 2012 Pearson Education, Inc.

Lecture Fall, 2005 Astronomy 110 1

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

Light and Geometric Optics

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

Next Homework Due March 6. Coming up: The Sun (Chapter 10)

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization

10.1 Properties of Light

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 5

Student Guide From Molecular Cores to Stars

Chapter 5 Light and Matter

Wave - Particle Duality of Light

o Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe

Light & Atoms. Electromagnetic [EM] Waves. Light and several other forms of radiation are called electromagnetic waves or electromagnetic radiation.

Chapter 5: Light and Matter: Reading Messages from the Cosmos

Light! Lecture 3, Oct. 8! Astronomy 102, Autumn 2009! Oct. 8, 2009 #1. Astronomy 102, Autumn 2009, E. Agol & J. Dalcanton U.W.

Unit 3: Optics Chapter 4. Properties of Light

Buy-back points tallied and added: 750 points bought-back. Last Withdrawal date: this friday, Oct 31st.

λ is a distance, so its units are m, cm, or mm, etc.

Modern Astronomy Review #1

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

2007 Oct 9 Light, Tools of Astronomy Page 1 of 5

The Basics of Light. Sunrise from the Space Shuttle, STS-47 mission. The Basics of Light

Name. F = ma P 2 = a 3 (M + m) P 2 = a 3. maxt = 2900 K m

Recall: The Importance of Light

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017

Atoms and Radiation electromagnetic radiation Radiation electromagnetic

Fluorescence. Incandescence. Electric. Bioluminescence Chemiluminescence. Combustion

Focusing on Light What is light? Is it a particle or a wave? An age-old debate that has persisted among scientists is related to the question, "Is

Astro 1010 Planetary Astronomy Sample Questions for Exam 2

Possible Solutions to Olbers Paradox

Chapter 4 Spectroscopy

X Rays must be viewed from space used for detecting exotic objects such as neutron stars and black holes also observing the Sun.

The Nature of Light and Matter 1 Light

AST 101 INTRODUCTION TO ASTRONOMY SPRING MIDTERM EXAM 1 TEST VERSION 1 ANSWERS NOTE: Question 20 Fixed

1) What do all waves transport from one place to another?

SNC2D PHYSICS 4/27/2013. LIGHT & GEOMETRIC OPTICS L What Is Light? (P ) What Is Light? What Is Light?

Electromagnetic Waves

Review: Properties of a wave

Producing and Harnessing Light

From Last Time Pearson Education, Inc.

ASTRO 114 Lecture Okay. What we re going to discuss today are what we call radiation laws. We ve

Doppler Shift. a. In which situation will the observer receive light that is shifted to shorter wavelengths?

Chapter 23. Light, Astronomical Observations, and the Sun

Atoms and Spectra October 8th, 2013

8-1. Chapter 8 THE DOPPLER EFFECTS OF SOUND AND LIGHT. motion. These are the classical and empirical Doppler effects of sound waves, and the

Chapter 5 Light and Matter: Reading Messages from the Cosmos. 5.1 Light in Everyday Life. How do we experience light?

Chapter 18: Studying Space Astronomy: The Original Science

Electromagnetic radiation simply a stream of photons (a bundle of energy) What are photons???

ASTR-1010: Astronomy I Course Notes Section IV

Write the electron configuration for Chromium (Cr):

Joules The units for energy are Joules=kg m 2 /s 2. Energy. Chemical Energy. Gravitational Energy. Conservation of Energy.

Astronomy 1102 Exam #1 Chapters 1,2,5,6 & 16

RADIATION and the EM Spectrum

What are the three basic types of spectra?

9/19/ Basic Properties of Light and Matter. Chapter 5: Light: The Cosmic Messenger. What is light? Lecture Outline

4.2 Properties of Visible Light Date: (pages )

Chapter 5 the nature of light

Nature of Light. Objectives. What is light What are the different forms

SECTION 3 & 4 LIGHT WAVES & INFORMATION TRANSFER

CHAPTERS: 9.1, 10.1 AND 10.2 LIGHT WAVES PROPERTIES

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

Astronomy 1143 Quiz 2 Review

ASTRONOMY 161. Introduction to Solar System Astronomy. Class 9

Studying the universe

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

The Doppler Effect ASTR1001 ASTR1001

Light The EM Spectrum

Introduction to Properties of Waves

Light. Mike Maloney Physics, SHS

Chapter 4. Spectroscopy. Dr. Tariq Al-Abdullah

Measuring Light waves

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

Astronomy 101 Test 1 Review FOUNDATIONS

Name Date Class _. Please turn to the section titled The Nature of Light.

Transcription:

The Electromagnetic Spectrum

Learning Objectives! What is Electromagnetic Radiation?! What are spectra? How could we measure a spectrum?! How do wavelengths correspond to colors for optical light? Does red or blue have the longest wavelength?! What is the speed of light? Is it infinite? How was it first measured? Can anything travel faster than light?! What is the Doppler Shift? A redshift? A blueshift? How can we use the Doppler Shift to measure the speed at which very distant objects are moving?! What are the types of Electromagnetic Radiation? Can they all penetrate the Earth s atmosphere? Can you order them by wavelength? By the energy they carry?

Light & Astronomy! Astronomers usually cannot control experiments! We get information from the objects we study (stars, planets, galaxies) by observing the light the objects emit! We use telescopes to collect the light that comes to the Earth from distant objects! To be able to extract the maximum information from the light we collect, we must understand light

Colors of the Rainbow! Newton used a prism to separate white light into its component colors! Called a spectrum! He then used a second prism to recombine the spectrum back into white light! This demonstrated that white light is a mixture of a spectrum of many colors

Particle or Wave?! How does light behave?! Huygens: light travels in the form of waves of energy! Newton: light is composed of a large number of particles

Light is a Wave!! In 1803, Thomas Young demonstrated that light travels as a wave! When light is passed through a double slit, a pattern of light and dark bands is produced! This can only be explained by wave-like behavior

How Do Colors Arise?! The color of light is determined by its wavelength! Visible light has extremely small wavelengths! Usually measured in nanometers (billionths of a meter)! Wavelengths range from 400 nm (violet light) to 700 nm (red light)! Colors, from longest wavelength to shortest: red, orange, yellow, green, blue, violet

The Speed of Light! The ancient Greeks thought the speed of light was infinite! In the 1600s Galileo realized very fast is not infinite! Galileo was the first to suggest an experiment to measure the speed of light, in which two people with lanterns signal each other! This isn t possible over distances of a few miles because of the extreme speed at which light travels Speed = 2 separation / time ~ 2 miles: 10 microseconds

The Speed of Light! In 1676, Ole Rømer saw that Io passed behind Jupiter sooner in time as the Earth got closer to Jupiter! He concluded that light from the event took longer to reach us when the Earth was farther from Jupiter! He measured that light travelled 8¼ minutes per AU! Today, we know the speed of light to be c = 3 10 8 m/s (186,000 miles per second, or 8.3 minutes per AU) June December ~16.5mins delay, extra 2AU distance

Velocity and the Doppler Effect! The Doppler Effect arises from the relative motion between an observer and a source of light (or sound)! Waves are squashed in the direction of motion! For light waves, this is called a blueshift! Waves are stretched in the direction opposite the direction of motion! For light waves, this is called a redshift

Electromagnetic Radiation! In the 1860s, James Clerk Maxwell created new theories of electricity and magnetism! These theories suggested that light is traveling electric and magnetic waves! Which is why we refer to light as electromagnetic radiation Magnetic Field Electric Field Electromagnetic wave direction

Invisible Forms of Electromagnetic Radiation! Visible light has a range of wavelengths from 400-700 nm (nanometers)! But what about light with longer or shorter wavelengths?! Maxwell s theories placed no restrictions on the possible wavelengths of light! There are types of light outside of optical or visual wavelengths (the range of wavelengths that we can see with our eyes)

Light is also a Particle!! In 1905, Einstein showed that light also behaves as a particle! Light particles are called photons! Particles, like little bullets, have energy! The energy of a photon decreases as the wavelength of the light increases! If you half the wavelength of a photon of light, you double its energy

The energy of E-M radiation that is emitted by a process depends on the atoms and molecules responsible for that process. In general, violent processes are energetic and emit short wavelengths (UV, x-rays). Gentle processes are less energetic and emit long wavelengths (IR, radio)

Opaque Atmosphere! The atmosphere blocks some wavelengths! This means that IR, UV, X-rays, gamma-rays are best observed from space or, at least, from high in our atmosphere

Important bad drawing

Next Time How Hot is a Star?