Environmental Science From Space

Size: px
Start display at page:

Download "Environmental Science From Space"

Transcription

1 Environmental Science From Space Remote Sensing and the Electromagne9c Spectrum Note: All images from NASA unless otherwise noted

2 Remote Sensing = learning about an object or phenomenon without touching, usually using satellites or airplanes h@p://

3

4

5 Videos LandSat video: Terra orbit anima9on: Watch live broadcast of LandSat:

6 Landsat 7 h@p://science.hq.nasa.gov/kids/imagers/ems/infrared.html Band Bandwidth (nm) Radia:on Blue Green Red Near Infrared 5 1,550-1,750 Shortwave Infrared 6 10,400-12,500 Thermal Infrared 7 2,090-2,350 Shortwave Infrared

7

8

9

10

11 LandSat Spectral Signatures Band Bandwidth (nm) Radia:on Blue Green Red Near Infrared 5 1,550-1,750 Shortwave Infrared 6 10,400-12,500 Thermal Infrared 7 2,090-2,350 Shortwave Infrared BUILDINGS WATER TREES ROCKS

12 Pixels & RGB Codes = 255,0,0 = 0,255,0 = 0,0,255 =255,255,255 = 0,0,0 = 255,0,255?,?,?? = 0,255,255

13 ACTIVITY: Crea9ng & Interpre9ng Remote Sensing Images (Derived from NASA s Remote Sensing Math)

14 Key to Pixels Feature Symbol Color RGB Code Sky Water Ice Land Plants

15 Key to Pixels Feature Symbol Color RGB Code Sky S Black 0,0,0 Water W Blue 0,0,1 Ice I White 1,1,1 Land L Brown 1,1,0 Plants P Green 0,1,0

16

17

18

19 Reviewing Waves (λ) = distance from any point on a wave to an iden9cal point on the next wave (f) = number of cycles or vibra9ons per unit of 9me (1 Hz = 1/s) (v) = distance/9me = * Speed of light (c) in vacuum = 3.8 x 10 8 m/s (186,000 miles/second)

20 Problem #1: Visible Light Which color has the longest wavelength? Which color has the highest frequency? Which color has the highest speed?

21 We can only see a small amount of the light that surrounds us all the 9me. h@p://science.hq.nasa.gov/kids/imagers/ems/index.html

22 Radio Waves Carry TV, AM & FM radio, cell phone, & other communica9on signals Used by radio telescopes to study radia9on by objects in space Carbon Monoxide (CO) gases in our Milky Way galaxy

23 Problem #2: Radio What s the frequency of your favorite radio sta9on? Calculate its wavelength.

24 Microwaves Heat food by making molecules rotate fast Used to detect & measure distance to objects, such as airplanes & weather, with radar sarakwatch.com

25 Microwaves Credit: NASA/WMAP Science Team

26 Infrared Waves Image of Phoenix (AZ) with near infrared as red Wikipedia Heat used to determine temperature of objects Uses Keeping food, spaces, animals warm (heat lamps) TV remote signal Firefigh9ng use to detect warm- blooded animals Remote sensing Determine temperature of land, water Map clouds, vegeta9on

27 ems/07_infraredwaves.html

28 Infrared Imaging What object is in the image below?

29 Visible Light Only wavelengths we can see Sources: sun, light bulbs Uses Human vision Photosynthesis of plants Remote sensing: map height of mountains, trees, clouds, etc.

30 Laser Al:metry (LiDAR) Where are the tallest trees? Outside Davenport, north of Santa Cruz Credit: NASA Earth Observatory/Image by Jesse Allen and Robert Simmon/Based on data from Michael Lefsky. height- map.html

31 Problem #3: Technology Choose one of the following devices Bluetooth (2400 MHz) GPS ( MHz) Wi- Fi (5 GHz) What wavelength is this? What type of radia9on is this? Garmin.com Wikipedia

32 Ultraviolet Light Causes sunburn Par9ally blocked by ozone in atmosphere Astronomers use to study stars Bees can see UV! UV image of Earth taken from Moon

33 Hubble Space Telescope spiral galaxy Messier_100 stars forming in the Eagle Nebula Wikipedia

34 X- Rays Image bones & teeth for medicine Astronomers use to study very hot objects such as stars, supernova & black holes

35 Gamma Rays Sources: Radioac9ve atoms Nuclear explosions Lightning strikes Supernova explosions (death of star) Black holes Uses: Detect spread of cancer Kill cancer cells Scan shipping containers for security Detect elements on other planets

36 Mapping Vegeta:on North America seasonal NDVI anima9on: h@p:// Normalized Difference Vegeta9on Index NDVI = (NIR Red) / (NIR + Red)

37 Problem #4: Mapping Vegeta:on red red Calculate NDVI for the healthy tree. Calculate NDVI for the stressed tree. Normalized Difference Vegeta9on Index NDVI = (NIR Red) / (NIR + Red) h@p://earthobservatory.nasa.gov/ Experiments/ICE/panama/panama_ex2.php

38 Vegeta:on Index Products NASA Earth Observatory

39 h@p://landsat.gsfc.nasa.gov/

40 Ac:vity: Remote Sensing of Barro Colorado Island NASA s Rainforest at the Crossroads h@p://earthobservatory.nasa.gov/experiments/ice/panama/

41

Which type of electromagnetic wave has a wavelength longer than that of yellow light? A. Infrared radiation C. X-rays B. Gamma Rays D.

Which type of electromagnetic wave has a wavelength longer than that of yellow light? A. Infrared radiation C. X-rays B. Gamma Rays D. Which type of electromagnetic wave has a wavelength longer than that of yellow light? A. Infrared radiation C. X-rays B. Gamma Rays D. UV Rays Science Starter! 10.14-15.13! THE UNIVERSE AND ELECTROMAGNETIC

More information

ELECTROMAGNETIC SPECTRUM All waves travel the SAME speed (the speed of light) 300,000 km/sec (186,000 miles/sec) in a vacuum

ELECTROMAGNETIC SPECTRUM All waves travel the SAME speed (the speed of light) 300,000 km/sec (186,000 miles/sec) in a vacuum ELECTROMAGNETIC SPECTRUM All waves travel the SAME speed (the speed of light) 300,000 km/sec (186,000 miles/sec) in a vacuum 10 4 Hz 10 6 Hz 10 8 Hz 10 12 Hz 10 14 Hz 10 16 Hz 10 18 Hz 1 million 1 trillion

More information

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

Chapter 26. Objectives. Describe characteristics of the universe in terms of time, distance, and organization Objectives Describe characteristics of the universe in terms of time, distance, and organization Identify the visible and nonvisible parts of the electromagnetic spectrum Compare refracting telescopes

More information

Chapter 4 - Light. Name: Block:

Chapter 4 - Light. Name: Block: Chapter 4 Notes: Light Name: Block: Properties of Waves Waves are a repeating disturbance or movement that energy through matter or space without causing any displacement of material Features of a wave:

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

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

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

Light is an important form of energy for all of us

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

More information

Electromagnetic Spectrum ANSWER ALL OF THE FOLLOWING USING THE WEB SITES LISTED. http://missionscience.nasa.gov/ems/index.html Introduction to The Electromagnetic Spectrum 1) Electromagnetic energy travels

More information

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

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 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 light a wave or a stream of particles?" Very noteworthy

More information

ELECTROMAGNETIC WAVES ELECTROMAGNETIC SPECTRUM

ELECTROMAGNETIC WAVES ELECTROMAGNETIC SPECTRUM VISUAL PHYSICS ONLINE MODULE 7 NATURE OF LIGHT ELECTROMAGNETIC WAVES ELECTROMAGNETIC SPECTRUM When white light passes through a prism, it spreads out into a rainbow of colours, with red at one end and

More information

Electromagnetic Waves. Electromagnetic Spectrum. Electromagnetic Spectrum. Electromagnetic Waves. CH 27-Physics (B) Fall, 2010

Electromagnetic Waves. Electromagnetic Spectrum. Electromagnetic Spectrum. Electromagnetic Waves. CH 27-Physics (B) Fall, 2010 Electromagnetic Waves Electromagnetic Spectrum CH 27-Physics (B) Fall, 2010 Electric and magnetic fields always exist When ever one is. the other is The fields can exist in a... They are at. o to each

More information

Name Class Date. What two models do scientists use to describe light? What is the electromagnetic spectrum? How can electromagnetic waves be used?

Name Class Date. What two models do scientists use to describe light? What is the electromagnetic spectrum? How can electromagnetic waves be used? CHAPTER 16 12 SECTION Sound and Light The Nature of Light KEY IDEAS As you read this section, keep these questions in mind: What two models do scientists use to describe light? What is the electromagnetic

More information

wave Electromagnetic Waves

wave Electromagnetic Waves What is a wave? A wave is a periodic disturbance in a solid, liquid or gas as energy is transmitted. A wave is characterized by its wavelength, frequency, and amplitude Light waves don t require a medium

More information

Frequency: the number of complete waves that pass a point in a given time. It has the symbol f. 1) SI Units: Hertz (Hz) Wavelength: The length from

Frequency: the number of complete waves that pass a point in a given time. It has the symbol f. 1) SI Units: Hertz (Hz) Wavelength: The length from Frequency: the number of complete waves that pass a point in a given time. It has the symbol f. 1) SI Units: Hertz (Hz) Wavelength: The length from the one crest of a wave to the next. I. Electromagnetic

More information

Light The EM Spectrum

Light The EM Spectrum Light The EM Spectrum 1 Spectrum of Electromagnetic Radiation Region Wavelength (Angstroms) Wavelength (centimeters) Frequency (Hz) Energy (ev) Radio > 10 9 > 10 < 3 x 10 9 < 10-5 Microwave 10 9-10 6 10-0.01

More information

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

Electromagnetic radiation simply a stream of photons (a bundle of energy) What are photons??? Electromagnetic radiation simply a stream of photons (a bundle of energy) What are photons??? no mass travel in a wave like pattern move at the speed of light contain a certain amount (or bundle) of energy

More information

#1 - Electromagnetic Spectrum Intro

#1 - Electromagnetic Spectrum Intro Go here for text on each section https://docs.google.com/viewer?a=v&pid=sites&srcid=zgvmyxvsdgrvbwfpbnxhbxltzwxiexloc3njaw VuY2V8Z3g6NjQxNzhiMGI3ZGI5ZjQ1Yw #1 - Electromagnetic Spectrum Intro https://www.youtube.com/watch?v=lwfjpc-rsxw&index=1&list=pl09e558656ca5df76

More information

Electromagnetic Radiation (EMR)

Electromagnetic Radiation (EMR) Electromagnetic Radiation (EMR) It is kind of energy with wave character ( exactly as sea waves ) that can be characterized by : Wavelength ( ) : The distance between two identical points on the wave.

More information

4.2 Properties of Visible Light Date: (pages )

4.2 Properties of Visible Light Date: (pages ) 4.2 Properties of Visible Light Date: (pages 144-149) Visible light is a mixture of all the colours of the rainbow. A prism refracts light separating the colours. A second prism can recombine the colours

More information

Electromagnetic Waves

Electromagnetic Waves ELECTROMAGNETIC RADIATION AND THE ELECTROMAGNETIC SPECTRUM Electromagnetic Radiation (EMR) THE ELECTROMAGNETIC SPECTRUM Electromagnetic Waves A wave is characterized by: Wavelength (λ - lambda) is the

More information

Astronomy Universe: all of space and everything in it

Astronomy Universe: all of space and everything in it Astronomy Universe: all of space and everything in it Most (90%) of the universe is made up of: dark matter: stuff we think is there due to amount of mass we think is there but is not detected by the instruments

More information

Chapter 17, Electromagnetic Waves Physical Science, McDougal-Littell, 2008

Chapter 17, Electromagnetic Waves Physical Science, McDougal-Littell, 2008 SECTION 1 (PP. 553-558): ELECTROMAGNETIC WAVES HAVE UNIQUE TRAITS. Georgia Standards: S8P4a Identify the characteristics of electromagnetic and mechanical waves; S8P4d Describe how the behavior of waves

More information

An x-ray image of teeth. Can you see the filling?

An x-ray image of teeth. Can you see the filling? X-Rays APA National Aeronautics and Space Administration, Science Mission Directorate. (2010). X-Rays. Retrieved December 12, 2012, from Mission:Science website: http://missionscience.nasa.gov /ems/11_xrays.html

More information

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

Name Date Class _. Please turn to the section titled The Nature of Light. Please turn to the section titled The Nature of Light. In this section, you will learn that light has both wave and particle characteristics. You will also see that visible light is just part of a wide

More information

Electromagnetic Spectrum

Electromagnetic Spectrum Lesson 2 Electromagnetic Spectrum visible ultraviolet x-rays gamma-rays frequency wavelength electromagnetic spectrum radio microwaves infrared Vocabulary Source:

More information

Solution 3: A glass prism deviates the violet light most and the red light least.

Solution 3: A glass prism deviates the violet light most and the red light least. EXERCISE- 6 (A) Question 1: Name three factors on which the deviation produces by a prism depends and state how does it depend on the factors stated by you. Solution 1: The deviation produced by the prism

More information

The Universe. 3. Base your answer to the following question on The diagram below represents the bright-line spectrum for an element.

The Universe. 3. Base your answer to the following question on The diagram below represents the bright-line spectrum for an element. A) B) The Universe 1. According to the Big Bang theory, which graph hest represents the relationship between time and the size of the universe from the beginning of the universe to the present? C) D) 2.

More information

wave speed (metre/second, m/s) = distance (metre, m) / time (second, s) v = x/t_ Universal physics

wave speed (metre/second, m/s) = distance (metre, m) / time (second, s) v = x/t_ Universal physics Topic 1 Visible light and the Solar System 1.1 Describe how ideas about the structure of the Solar System have changed over time, including the change from the geocentric to the heliocentric models and

More information

TELESCOPES POWERFUL. Beyond the Book. FOCUS Book

TELESCOPES POWERFUL. Beyond the Book. FOCUS Book FOCUS Book POWERFUL TELESCOPES Why do we need telescopes in order to observe stars that are very far away? Why do stars look bright in the sky while most galaxies, which have billions of stars, are too

More information

Chapter 25. Electromagnetic Waves

Chapter 25. Electromagnetic Waves Chapter 25 Electromagnetic Waves EXAM # 3 Nov. 20-21 Chapter 23 Chapter 25 Powerpoint Nov. 4 Problems from previous exams Physics in Perspective (pg. 836 837) Units of Chapter 25 The Production of Electromagnetic

More information

Astronomy beyond the visible Beatriz García, Ricardo Moreno, Rosa M. Ros

Astronomy beyond the visible Beatriz García, Ricardo Moreno, Rosa M. Ros Astronomy beyond the visible Beatriz García, Ricardo Moreno, Rosa M. Ros International Astronomical Union Comm 46 Universidad Tecnológica Nacional, Mendoza (Argentina) Colegio Retamar, Madrid (España)

More information

Name Class Date. Circle the letter of the best answer for each question.

Name Class Date. Circle the letter of the best answer for each question. Skills Worksheet Directed Reading B Section: The Electromagnetic Spectrum CHARACTERISTICS OF EM WAVES 1. At what speed do EM waves travel in a vacuum? a. 3,000,000 km/s b. 3,000,000 km/min c. 300,000 km/s

More information

Electromagnetic Radiation (EMR)

Electromagnetic Radiation (EMR) Electromagnetic Radiation (EMR) It is kind of energy with wave character ( exactly as sea waves ) that can be characterized by : Wavelength ( ) : The distance between two identical points on the wave.

More information

The Nature of Light. We have a dual model

The Nature of Light. We have a dual model Light and Atoms Properties of Light We can come to understand the composition of distant bodies by analyzing the light they emit This analysis can tell us about the composition as well as the temperature

More information

Todays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors

Todays Topics 3/19/2018. Light and Telescope. PHYS 1403 Introduction to Astronomy. CCD Camera Makes Digital Images. Astronomical Detectors PHYS 1403 Introduction to Astronomy Light and Telescope Chapter 6 Todays Topics Astronomical Detectors Radio Telescopes Why we need space telescopes? Hubble Space Telescopes Future Space Telescopes Astronomy

More information

Sunlight is a combination of light-waves of various frequencies. Some

Sunlight is a combination of light-waves of various frequencies. Some 96 The Electromagnetic Spectrum r e a d i n g Sunlight is a combination of light-waves of various frequencies. Some of the frequencies can be seen and some cannot be seen by the human eye. The reading

More information

Scale the Universe. Exploring your Universe from Inner to Outer Space. Linda L. Smith NASA Astrophysics Educator Ambassador

Scale the Universe. Exploring your Universe from Inner to Outer Space. Linda L. Smith NASA Astrophysics Educator Ambassador Scale the Universe Exploring your Universe from Inner to Outer Space Linda L. Smith NASA Astrophysics Educator Ambassador lsmith@paulsboro.k12.nj.us 1 The Booklet This book is organized into 3-stand-alone

More information

Properties of Waves. Before You Read. What are the features of a wave?

Properties of Waves. Before You Read. What are the features of a wave? Properties of Waves Textbook pages 134 143 Before You Read Section 4.1 Summary In this section, you will find out about waves, such as water waves, sound waves, and radio waves. On the lines below, list

More information

Light is an electromagnetic wave (EM)

Light is an electromagnetic wave (EM) What is light? Light is a form of energy. Light travels in a straight line Light speed is 3.0 x 10 8 m/s Light is carried by photons Light can travel through a vacuum Light is a transverse wave Light is

More information

Collecting Light. In a dark-adapted eye, the iris is fully open and the pupil has a diameter of about 7 mm. pupil

Collecting Light. In a dark-adapted eye, the iris is fully open and the pupil has a diameter of about 7 mm. pupil Telescopes Collecting Light The simplest means of observing the Universe is the eye. The human eye is sensitive to light with a wavelength of about 400 and 700 nanometers. In a dark-adapted eye, the iris

More information

Let there be light THE CAUSES OF ELECTROMAGNETIC RADIATION

Let there be light THE CAUSES OF ELECTROMAGNETIC RADIATION Let there be light THE CAUSES OF ELECTROMAGNETIC RADIATION Learning Target I can construct an explana/on of the Big Bang theory based on astronomical evidence of light spectra, mo/on of distant galaxies,

More information

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

9/16/08 Tuesday. Chapter 3. Properties of Light. Light the Astronomer s Tool. and sometimes it can be described as a particle! 9/16/08 Tuesday Announce: Observations? Milky Way Center movie Moon s Surface Gravity movie Questions on Gravity from Ch. 2 Ch. 3 Newton Movie Chapter 3 Light and Atoms Copyright (c) The McGraw-Hill Companies,

More information

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth)

days to rotate in its own axis km in diameter ( 109 diameter of the Earth ) and kg in mass ( mass of the Earth) The Sun - It is located at the centre of our solar system with all planets and objects (comets and asteroids) revolving around it Page 1 of 6 - It s gravitational pull keeps the planets and other objects

More information

PRINCIPLES OF REMOTE SENSING. Electromagnetic Energy and Spectral Signatures

PRINCIPLES OF REMOTE SENSING. Electromagnetic Energy and Spectral Signatures PRINCIPLES OF REMOTE SENSING Electromagnetic Energy and Spectral Signatures Remote sensing is the science and art of acquiring and analyzing information about objects or phenomena from a distance. As humans,

More information

Taking Fingerprints of Stars, Galaxies, and Other Stuff. The Bohr Atom. The Bohr Atom Model of Hydrogen atom. Bohr Atom. Bohr Atom

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

More information

Lecture Outlines. Chapter 5. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 5. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 5 Astronomy Today 8th Edition Chaisson/McMillan Chapter 5 Telescopes Units of Chapter 5 5.1 Optical Telescopes 5.2 Telescope Size 5.3 Images and Detectors 5.4 High-Resolution Astronomy

More information

3. The very long ones are called waves, and the very short ones are called waves.

3. The very long ones are called waves, and the very short ones are called waves. NASA Mission: Science Introduction to the Electromagnetic Spectrum Web Quest Directions: Load the following website which will discuss the electromagnetic spectrum in detail. http://missionscience.nasa.gov/ems/01_intro.html

More information

Chapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Chapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Learning Objectives Upon completing this chapter you should be able to: 1. Classify the

More information

Topic 8: Beyond Light

Topic 8: Beyond Light Topic 8: Beyond Light The Sun is the most abundant source of direct natural light on the Earth. There are other forms of energy, invisible, that are also supplied by this source. The tiny band of visible

More information

Cosmic Microwave Background Radiation

Cosmic Microwave Background Radiation Base your answers to questions 1 and 2 on the passage below and on your knowledge of Earth Science. Cosmic Microwave Background Radiation In the 1920s, Edwin Hubble's discovery of a pattern in the red

More information

Unit 3: Optics Chapter 4. Properties of Light

Unit 3: Optics Chapter 4. Properties of Light Unit 3: Optics Chapter 4 Properties of Light There are many types of light sources... Fluorescence Incandescence Electric Bioluminescence Chemiluminescence Combustion The Nature of Light Pythagoras A Greek

More information

= λ. Topics for Today. Clicker Q: Radio Waves. Radios. Light Pollution. Problems in Looking Through Our Atmosphere

= λ. Topics for Today. Clicker Q: Radio Waves. Radios. Light Pollution. Problems in Looking Through Our Atmosphere ASTR 1040 Accel Astro: Stars & Galaxies Prof. Juri Toomre TA: Nick Featherstone Lecture 5 Tues 30 Jan 07 zeus.colorado.edu/astr1040-toomre toomre Topics for Today Twinkle and absorption by our atmosphere

More information

Background: The Electromagnetic Spectrum

Background: The Electromagnetic Spectrum Background: The Electromagnetic Spectrum Wavelength (λ) in meters wavelength decreasing 10 4 10 2 10 0 10-2 10-4 10-6 10-8 10-10 10-12 10-14 microwaves ultraviolet Gamma rays Radio waves AM 10 4 Shortwave

More information

Newton s Laws of Motion

Newton s Laws of Motion Newton s Laws of Motion #1: A body continues at rest or in uniform motion in a straight line unless acted upon by a force. Why doesn t the soccer ball move on its own? What causes a soccer ball to roll

More information

Properties of Thermal Radiation

Properties of Thermal Radiation Observing the Universe: Telescopes Astronomy 2020 Lecture 6 Prof. Tom Megeath Today s Lecture: 1. A little more on blackbodies 2. Light, vision, and basic optics 3. Telescopes Properties of Thermal Radiation

More information

Taking fingerprints of stars, galaxies, and interstellar gas clouds

Taking fingerprints of stars, galaxies, and interstellar gas clouds - - Taking fingerprints of stars, galaxies, and interstellar gas clouds Absorption and emission from atoms, ions, and molecules Periodic Table of Elements The universe is mostly hydrogen H and helium He

More information

Light and Geometric Optics

Light and Geometric Optics By the end of this week I will be able to... label a diagram of a wave Solve word problems using the wave equation identify the types of radiation on the EM spectrum explain how light behaves like a wave

More information

ASTR 2310: Chapter 6

ASTR 2310: Chapter 6 ASTR 231: Chapter 6 Astronomical Detection of Light The Telescope as a Camera Refraction and Reflection Telescopes Quality of Images Astronomical Instruments and Detectors Observations and Photon Counting

More information

Visions of the Universe. Four Centuries of Discovery. Future. Visions

Visions of the Universe. Four Centuries of Discovery. Future. Visions Visions of the Universe ~ Four Centuries of Discovery Future Visions Future Visions Table of Contents - Exhibit Overview... 3 Science Background... 4 Science Misconceptions... 6 Glossary... 8 Related Educational

More information

Earth s Atmosphere & Telescopes. Atmospheric Effects

Earth s Atmosphere & Telescopes. Atmospheric Effects Earth s Atmosphere & Telescopes Whether light is absorbed by the atmosphere or not depends greatly on its wavelength. Earth s atmosphere can absorb certain wavelengths of light so much that astronomers

More information

Waves and Space Exploration Review (PS.4, PS.5, ST.1 and ESS.8)

Waves and Space Exploration Review (PS.4, PS.5, ST.1 and ESS.8) Waves 1. What causes waves? 2. Define wave. Label each below as longitudinal or transverse 3. 4. Label the crest, trough, wavelength and amplitude of the wave below. 9. In the diagram above, four complete

More information

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe

Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe Formation of the Universe & What is in Space? The Big Bang Theory and components of the Universe The Big Bang Theory The Big Bang Theory The Big Bang Theory is the most widely accepted scientific explanation

More information

Stars, Galaxies, and the Universe

Stars, Galaxies, and the Universe Stars, Galaxies, and the Universe Chapter Test A Multiple Choice Write the letter of the correct answer on the line at the left. 1. What is a giant ball of hot gases that undergo nuclear fusion? a. a planet

More information

FCAT REVIEW Physical Science: Force and Energy

FCAT REVIEW Physical Science: Force and Energy FCAT REVIEW Physical Science: Force and Energy Force and Motion A force is a push or pull that starts, stops, or changes the direction of an object. Some examples of contact forces are gravity and friction.

More information

Astronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe.

Astronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe. Astronomy Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe. Universe = everything that exists Disclaimer: Astrology is NOT science!!!

More information

How to Measure and Record Light Spectrograph. The Photographic plate now obsolete Turbulence

How to Measure and Record Light Spectrograph. The Photographic plate now obsolete Turbulence PHYS 1411 Introduction to Astronomy Light and Telescope Chapter 6 Chapter 6 topics we have covered so far Radiation Information from Space Wave properties, light as a wave and particle, Electromagnetic

More information

Taking fingerprints of stars, galaxies, and interstellar gas clouds. Absorption and emission from atoms, ions, and molecules

Taking fingerprints of stars, galaxies, and interstellar gas clouds. Absorption and emission from atoms, ions, and molecules Taking fingerprints of stars, galaxies, and interstellar gas clouds Absorption and emission from atoms, ions, and molecules 1 Periodic Table of Elements The universe is mostly hydrogen H and helium He

More information

Fluorescence. Incandescence. Electric. Bioluminescence Chemiluminescence. Combustion

Fluorescence. Incandescence. Electric. Bioluminescence Chemiluminescence. Combustion Fluorescence Incandescence Electric Bioluminescence Chemiluminescence Combustion Pythagoras A Greek philosopher Believed light was beams of tiny particles The eyes could detect these particles and see

More information

Red Hot, Blue Hot: Mapping the Invisible Universe

Red Hot, Blue Hot: Mapping the Invisible Universe Red Hot, Blue Hot: Mapping the Invisible Universe Activity Guide Originally developed by Marni Berendsen for the Night Sky Network Adapted by Anna Hurst 2006, Astronomy from the Ground Up Astronomical

More information

Light and Telescopes

Light and Telescopes Light and Telescopes Astronomy 1 Elementary Astronomy LA Mission College Spring F2015 Quotes & Cartoon of the Day We find them smaller and fainter, in constantly increasing numbers, and we know that we

More information

Modern Astronomy Review #1

Modern Astronomy Review #1 Modern Astronomy Review #1 1. The red-shift of light from distant galaxies provides evidence that the universe is (1) shrinking, only (3) shrinking and expanding in a cyclic pattern (2) expanding, only

More information

Science 30 Unit C Review Outline GCCHS. Negatively charged Positively charged Coulomb Conductor Electric potential difference

Science 30 Unit C Review Outline GCCHS. Negatively charged Positively charged Coulomb Conductor Electric potential difference Science 30 Unit C Review Outline GCCHS Negatively charged Positively charged Coulomb Conductor Electric potential difference volt voltage Insulator Test body Gravitational field Field lines Solar wind

More information

AST 101 Intro to Astronomy: Stars & Galaxies

AST 101 Intro to Astronomy: Stars & Galaxies AST 101 Intro to Astronomy: Stars & Galaxies Telescopes Mauna Kea Observatories, Big Island, HI Imaging with our Eyes pupil allows light to enter the eye lens focuses light to create an image retina detects

More information

Light. Transverse electromagnetic wave, or electromagnetic radiation. Includes radio waves, microwaves, infra-red, visible, UV, X-rays, and gamma rays

Light. Transverse electromagnetic wave, or electromagnetic radiation. Includes radio waves, microwaves, infra-red, visible, UV, X-rays, and gamma rays Light Transverse electromagnetic wave, or electromagnetic radiation Includes radio waves, microwaves, infra-red, visible, UV, X-rays, and gamma rays The type of light is determined purely by wavelength.

More information

1. Using, scientists can use a few smaller telescopes to take images with the. 2. To double the resolving power of a telescope, you must.

1. Using, scientists can use a few smaller telescopes to take images with the. 2. To double the resolving power of a telescope, you must. Chapter 5 Telescopes Multiple Choice Questions 1. Using, scientists can use a few smaller telescopes to take images with the same resolution as a much larger telescope. A. Satellite telescopes B. Charge-coupled

More information

Chapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc.

Chapter 19 Reading Quiz Clickers. The Cosmic Perspective Seventh Edition. Our Galaxy Pearson Education, Inc. Reading Quiz Clickers The Cosmic Perspective Seventh Edition Our Galaxy 19.1 The Milky Way Revealed What does our galaxy look like? How do stars orbit in our galaxy? Where are globular clusters located

More information

1. The symbols below represent the Milky Way galaxy, the solar system, the Sun, and the universe.

1. The symbols below represent the Milky Way galaxy, the solar system, the Sun, and the universe. Name Date 1. The symbols below represent the Milky Way galaxy, the solar system, the Sun, and the universe. 4. The diagram below illustrates three stages of a current theory of the formation of the universe.

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

Light: Transverse WAVE

Light: Transverse WAVE Light Longitudinal WAVES Light: Transverse WAVE Light: Particle or wave Photon The Wave Nature of Light 1. Unlike other branches of science, astronomers cannot touch or do field work on their samples.

More information

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

Grade 8 Science: Unit 3-Optics Chapter 4: Properties of Light Grade 8 Science: Unit 3-Optics Chapter 4: Properties of Light Key Terms: Microscope, telescope, amplitude, crest, energy, force, frequency, hertz, medium, transverse wave, trough, wave, wavelength, reflection,

More information

Tools of Astronomy Tools of Astronomy

Tools of Astronomy Tools of Astronomy Tools of Astronomy Tools of Astronomy The light that comes to Earth from distant objects is the best tool that astronomers can use to learn about the universe. In most cases, there is no other way to study

More information

Discussion Review Test #2. Units 12-19: (1) (2) (3) (4) (5) (6)

Discussion Review Test #2. Units 12-19: (1) (2) (3) (4) (5) (6) Discussion Review Test #2 Units 12-19: (1) (2) (3) (4) (5) (6) (7) (8) (9) Galileo used his observations of the changing phases of Venus to demonstrate that a. the sun moves around the Earth b. the universe

More information

Chapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Chapter 5. Telescopes. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Chapter 5 Telescopes Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Tools of the Trade: Telescopes The Powers of a Telescope Collecting Power Bigger telescope,

More information

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

Lecture 6: The Physics of Light, Part 1. Astronomy 111 Wednesday September 13, 2017 Lecture 6: The Physics of Light, Part 1 Astronomy 111 Wednesday September 13, 2017 Reminders Star party tonight! Homework #3 due Monday Exam #1 Monday, September 25 The nature of light Look, but don t

More information

UNIT E: SPACE EXPLORATION

UNIT E: SPACE EXPLORATION UNIT E: SPACE EXPLORATION S C I E N C E 9 1 Science 9 Unit E Section 3.0 OPTICAL TELESCOPES, RADIO TELESCOPES, AND OTHER TECHNOLOGIES ADVANCE OUR UNDERSTANDING OF SPACE SECTI ON 3.0 Science 9 Unit E Section

More information

1. The most important aspects of the quantum theory.

1. The most important aspects of the quantum theory. Lecture 5. Radiation and energy. Objectives: 1. The most important aspects of the quantum theory: atom, subatomic particles, atomic number, mass number, atomic mass, isotopes, simplified atomic diagrams,

More information

Astronomical Tools. Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes

Astronomical Tools. Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes Astronomical Tools Optics Telescope Design Optical Telescopes Radio Telescopes Infrared Telescopes X Ray Telescopes Gamma Ray Telescopes Laws of Refraction and Reflection Law of Refraction n 1 sin θ 1

More information

CHAPTER 28 STARS AND GALAXIES

CHAPTER 28 STARS AND GALAXIES CHAPTER 28 STARS AND GALAXIES 28.1 A CLOSER LOOK AT LIGHT Light is a form of electromagnetic radiation, which is energy that travels in waves. Waves of energy travel at 300,000 km/sec (speed of light Ex:

More information

Newton s Law of Gravity. Isaac Newton ( ) Newton s Law of Gravity. Newton s Laws of Motion. Newton s Laws of Motion 2/17/17

Newton s Law of Gravity. Isaac Newton ( ) Newton s Law of Gravity. Newton s Laws of Motion. Newton s Laws of Motion 2/17/17 Isaac Newton (1642-1727) English physicist and mathematician Studied motion, light, and gravity Newton puts all the pieces together Key idea: Mass Mass is the amount of matter in an object NOT the same

More information

LIFE CYCLE OF A STAR

LIFE CYCLE OF A STAR LIFE CYCLE OF A STAR First stage = Protostar PROTOSTAR Cloud of gas and dust many light-years across Gravity tries to pull the materials together Eventually, at the center of the ball of dust and gas,

More information

Inaugural University of Michigan Science Olympiad Tournament

Inaugural University of Michigan Science Olympiad Tournament Inaugural University of Michigan Science Olympiad Tournament The test may be taken apart. Ties will be broken based on predetermined questions and quality of response. Remote Sensing Test length: 50 Minutes

More information

Chapter 17 Practice Questions KEY

Chapter 17 Practice Questions KEY Chapter 17 Practice Questions KEY 1. Long wavelength Medium wavelength Short wavelength 1. Long wavelength Radio, Microwave Medium wavelength Infrared, Visible, Ultraviolet Short wavelength X ray, gamma

More information

Unit 5 Physical Science Radioactivity Answer Key

Unit 5 Physical Science Radioactivity Answer Key Unit 5 Physical Science Radioactivity Answer Key Page 198 1. True 2. False: The higher the frequency is, the higher the energy is. 3. True 4. False: Energy increases as frequency increases. 5. False: The

More information

Directed Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past?

Directed Reading. Section: Viewing the Universe THE VALUE OF ASTRONOMY. Skills Worksheet. 1. How did observations of the sky help farmers in the past? Skills Worksheet Directed Reading Section: Viewing the Universe 1. How did observations of the sky help farmers in the past? 2. How did observations of the sky help sailors in the past? 3. What is the

More information

National 3 Waves and Radiation

National 3 Waves and Radiation What is a wave? National 3 Waves and Radiation 1. Wave Properties The basic definition Waves are a way of transporting energy from one place to another. They do this through some form of vibration. We

More information

Review: Properties of a wave

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.

More information

Chapter 21: Stars Notes

Chapter 21: Stars Notes Branches of Earth Science Chapter 21: Stars Notes Astronomy: The study of planets, stars, and other objects in space. Lithosphere: the land masses of earth o Litho means rock Hydrosphere: waters of the

More information

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

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

More information

Useful Formulas and Values

Useful Formulas and Values Name Test 1 Planetary and Stellar Astronomy 2017 (Last, First) The exam has 20 multiple choice questions (3 points each) and 8 short answer questions (5 points each). This is a closed-book, closed-notes

More information

ANSWER KEY. Stars, Galaxies, and the Universe. Telescopes Guided Reading and Study. Characteristics of Stars Guided Reading and Study

ANSWER KEY. Stars, Galaxies, and the Universe. Telescopes Guided Reading and Study. Characteristics of Stars Guided Reading and Study Stars, Galaxies, a the Universe Stars, Galaxies, and the Universe Telescopes Use Target Reading Skills Check student definitions for accuracy. 1. Electromagneticradiationisenergythatcan travel through

More information