Goal: To understand how light is used to understand what humankind has discovered about astronomy. Objectives: 1)To learn the Properties of light 2)To.

Slides:



Advertisements
Similar presentations
Lecture 7 ASTR 111 – Section 002.
Advertisements

During the past few decades, scientists have discovered smaller sub- atomic particles that create the electrons, protons, and neutrons of an atom. As they.
Radiation:.
Radiation and Spectra Chapter 5
Unlocking Light The key to understanding the Cosmos.
Life always offers you a second chance. It’s called tomorrow.
Spectroscopy. Spectroscopy is complex - but it can be very useful in helping understand how an object like a Star or active galaxy is producing light,
ASTRONOMY 161 Introduction to Solar System Astronomy Class 9.
The Light Fantastic! Astronomy relies on messages from all kinds of light.
PHYS 206 Matter and Light At least 95% of the celestial information we receive is in the form of light. Therefore we need to know what light is and where.
Chapter 5 Light and Matter: Reading Messages from the Cosmos
Unit 4 Atomic Physics and Spectra. The Electromagnetic Spectrum.
The Nebular Theory, Matter, and Light 1. 1.Terrestrial, Jovian, and dwarf planets 2. 2.Nebular theory 3. 3.Matter – atoms and molecules 4. 4.Kinetic and.
Test #1, Wednesday, Feb 10 I will post a review for Test 1 in the A101 homepage under the link to “Lectures” this week. I will tell you the topics to review.
ISP Astronomy Gary D. Westfall1Lecture 6 The Nature of Light Light and other forms of radiation carry information to us from distance astronomical.
The Nature of Light In Astronomy II. The Earth’s atmosphere absorbs most of EM spectrum, including all UV, X ray, gamma ray and most infrared. We have.
Astronomy Picture of the Day. Possible First Pic of Extrasolar Planet
Aim: How to distinguish electrons in the excited state DO NOW: PREPARE FOR QUIZ. 10 MIN.
Quantum Mechanics.  Write what’s in white on the back of the Week 10 Concept Review  Then, answer the questions on the front Your Job.
Goal: To understand electromagnetic waves. Objectives: 1) to learn that the term electromagnetic wave is scarier sounding than it actually is 2) to understand.
Electromagnetic Radiation
© 2010 Pearson Education, Inc. Light and Matter: Reading Messages from the Cosmos.
Blackbody Radiation & Atomic Spectra. “Light” – From gamma-rays to radio waves The vast majority of information we have about astronomical objects comes.
Properties of Matter Our goals for learning: What is the structure of matter? What are the phases of matter How is energy stored in atoms?
Creating Light. Light as a Wave Light (or electromagnetic radiation), can be thought of as either a particle or a wave. As a wave, light has a wavelength,
Blackbody Radiation And Spectra. Light is a form of _______. Why is this important? With very few exceptions, the only way we have to study objects in.
Spectral Analysis of Stars Astronomy. Energy Through Space Energy is transmitted through space as electromagnetic waves. The movement of these waves through.
Many scientists found Rutherford’s Model to be incomplete  He did not explain how the electrons are arranged  He did not explain how the electrons were.
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.
Light as Messenger.
Energy Energy is a property that enables something to do work
Properties of Light.
How do colors in a spectrum help us understand stars? Image from
The SUN.
Donna Kubik PHYS162 Fall, Because of its electric and magnetic properties, light is called electromagnetic radiation. It consists of perpendicular,
What Can Spectroscopy Tell Us?. Atom or Molecular Fingerprints Every atom or molecule exists in its own unique energy state. This energy state is dependent.
EARTH SCIENCE Prentice Hall EARTH SCIENCE Tarbuck Lutgens 
Lecture 9 Stellar Spectra
Energy Levels & Photons Atomic & Nuclear Lesson 2.
The Nature of Light A Prism “Breaks Up” White Light When white light passes through a prism a spectrum is formed.
Physics and the Quantum Mechanical Model
Electrons and the Electromagnetic Spectrum Table Team Review — DEFINE in your own words ‘Electromagnetic radiation’. LIST three examples.
Bellwork What is the majority of the volume of an atom?
Light 1)Exam Review 2)Introduction 3)Light Waves 4)Atoms 5)Light Sources October 14, 2002.
Electromagnetic Spectrum. Different Types of Light  Light is a form of energy  It travels in waves  Also called Electromagnetic Radiation  Some Electromagnetic.
Section 5.3.  Neon advertising signs are formed from glass tubes bent in various shapes. An electric current passing through the gas in each glass tube.
Exam #1 Approaching 1 st Exam will be in four days (Friday, Sept. 18) – Chapters closed book/notes exam 40 questions, multiple choice, no calculators.
1 CHAPTER 13: Electrons in the Atom. 2 Quantum Mechanical Model of the Atom and Ernest Schrodinger The model of the atom was developed based on the study.
Aim: How to distinguish electrons in the excited state
What is light? Light can act either like a wave or like a particle Particles of light are called photons.
Tools of Modern Astronomy
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 2 Light and Matter.
Light and Matter Astronomy 315 Professor Lee Carkner Lecture 6.
Electron As a Particle and Wave Electrons get excited when energy is absorbed by using heat or electrical energy Electrons get excited when energy is absorbed.
C-4 Atomic Structure The nucleus and the moving electrons.
Chapter 5 Light: The Cosmic Messenger. 5.1Basic Properties of Light and Matter Light: electromagnetic waves 1. Velocity (c = speed of light), wavelength.
Physics and the Quantum Mechanical Model.  Light consists of waves  A wave cycle begins at zero, increases to its highest value (crest), returns to.
Starlight What is it? What does it tell us? Write down all notes in RED.
Chapter 24 Video Field Trip: Fireball Write down five facts from the video!
NATS From the Cosmos to Earth Light as a Wave For a wave, its speed: s = l x f But the speed of light is a constant, c. For light: l x f = c The.
Life always offers you a second chance. It’s called tomorrow.
Starter 1.Where are most asteroids located? 2.Describe the structure of a comet. 3.Where do short period comets come from? What about long period comets?
The Study of Light.
Cool, invisible galactic gas (60 K, f peak in low radio frequencies) Dim, young star (600K, f peak in infrared) The Sun’s surface (6000K, f peak in visible)
Unit 3.  Much of the information we get in astronomy is carried by “light”.
Objectives: To learn the Properties of light
Matter All matter is composed of atoms.
Electromagnetic Spectrum
Light and The Electromagnetic Spectrum
Light and Matter Chapter 2.
Presentation transcript:

Goal: To understand how light is used to understand what humankind has discovered about astronomy. Objectives: 1)To learn the Properties of light 2)To understand how the 3 different types of spectra are created. 3)Play the GUESS THE GAS CONTEST!!!

Properties of light Light can act like either a particle or a wave. Most commonly acts like a wave. Like waves you are familiar with, light waves have a wavelength and energy. Energy = a constant * speed of light / wavelength

Which of the following would NOT emit light waves? Dentist X-ray machine An outgoing radio tower Radar machine The night side of the moon Neon sign All of the above emit light None of these emit light

Spectrum of Electromagnetic Radiation RegionWavelength (Angstroms) Wavelength (centimeters) Frequency (Hz) Energy (eV) Radio> 10 9 > 10< 3 x 10 9 < Microwave x x Infrared x x x Visible x x x x Ultraviolet x x x X-Rays x x Gamma Rays< 0.1< > 3 x > 10 5

A radio wave is sent out from planet earth. How long will it take that radio wave to travel to Alpha Centauri B (4.3 light years away) A) a little over 1 year B) a little over 2 years C) a little over 4 years D) a little over 8 years E) this radio wave can’t possibly get there.

How is light created? Light is created by electrons changing energy states – to conserve energy. So, to understand light, you have to understand the atom. Atoms are made of a nucleus (with + charged protons and uncharged neutrons) and shells of – charged electrons. Much like different distances from an object creates a difference gravitational energy, so to does the distance from a nucleus. However, there are only certain specific allowed energy states in an atom.

Spectra, meet the spectra! There are 3 types of spectra: 1) continuous – a smooth light curve with no breaks and light at all wavelengths 2) absorption – a continuum which has parts taken out (kind of like a hockey goalie). 3) emission – either a continuum with emission added to it, or just a series of special lines.

Condescend Light Bulb Take the spectral glasses and take a look at the Condescend light bulb. What type of spectrum would you classify this as? A) Continuous B) Absorption C) Emission

Blackbody Spectrum – continuous All objects which absorb most of the light which passes through them emit energy as a “blackbody”. The shape of the blackbody spectrum is always the same. The strength of the spectrum (i.e. how much light it emits) and the peak wavelength of the spectrum depend on the temperature of the object.

Windex What type of spectrum does this produce? A) Continuous B) Absorption C) Emission

Absorption Spectrum As you can see, the Windex creates a spectrum where you have a continuous portion, but a huge chunk is taken out. This chunk is absorbed by the Windex. The Windex, not surprising, is blue because of the light it absorbs.

Absorption spectra in Astronomy Windex is a solution of very complex molecules though, and in Astronomy most Absorption spectra are created by gasses of a few atoms and few molecules. Therefore, most Absorption spectra in Astronomy consist of thin dark lines, or thin areas where most of the energy is removed at just a few wavelengths. Any “thin” substance which is in front of a continuous light source will produce an absorption spectrum IF it is cooler than the continuous source.

Absorption – our use When you find an emission or absorption spectrum, you know what the makeup of the gas or material that emitted it. Each element and each molecule have their own specific energies they can emit. This is a fingerprint of the gas. This is why we know the sun is made of mostly H and He.

Fluorescent lights What type of spectrum does this produce? A) Continuous B) Absorption C) Emission

Fluorescent lights This is emission. The electrons in the gas get “excited” by the energy put through the gas. The electrons then “cascade” down to emit several photons of light. One is a optical photon. There are different specific energy states, and the lines are produced by the different combinations of energy states (starting/ending). Any thin gas will produce an emission spectrum if you JUST look at the gas. Any thin gas which is HOTTER than a background continuous source will ALSO produce emission features!

Guess the gas contest! For each of the following tubes you may find it helpful to draw the pattern of light. You will guess which gas is in each tube. Anyone who can get all of them gets a bonus 5 points! Everyone who turns in with guesses and patterns on all tubes gets the normal points. If you can get all but 1 I will give you a bonus 3 points. If you get 4 of 6 you get 1 bonus point.

Conclusion We examined the properties of light. We discovered the method of creating light. We discovered the different spectrum and explored how to create each one of them (and therefore what we can use them for). We looked at some gasses and found what most of them were from the light they emitted.