Environmental Science From Space

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

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

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

Chapter 4 - Light. Name: Block:

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 Name HR Date

Light is an important form of energy for all of us


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

ELECTROMAGNETIC WAVES ELECTROMAGNETIC SPECTRUM

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

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

wave Electromagnetic Waves

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

Light The EM Spectrum

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

#1 - Electromagnetic Spectrum Intro

Electromagnetic Radiation (EMR)

4.2 Properties of Visible Light Date: (pages )

Electromagnetic Waves

Astronomy Universe: all of space and everything in it

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

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

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

Electromagnetic Spectrum

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

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

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

TELESCOPES POWERFUL. Beyond the Book. FOCUS Book

Chapter 25. Electromagnetic Waves

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

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

Electromagnetic Radiation (EMR)

The Nature of Light. We have a dual model

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

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

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

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

Light is an electromagnetic wave (EM)

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

Let there be light THE CAUSES OF ELECTROMAGNETIC RADIATION

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

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

PRINCIPLES OF REMOTE SENSING. Electromagnetic Energy and Spectral Signatures

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

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

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

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

Topic 8: Beyond Light

Cosmic Microwave Background Radiation

Unit 3: Optics Chapter 4. Properties of Light

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

Background: The Electromagnetic Spectrum

Newton s Laws of Motion

Properties of Thermal Radiation

Taking fingerprints of stars, galaxies, and interstellar gas clouds

Light and Geometric Optics

ASTR 2310: Chapter 6

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

Earth s Atmosphere & Telescopes. Atmospheric Effects

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

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

Stars, Galaxies, and the Universe

FCAT REVIEW Physical Science: Force and Energy

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

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

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

Fluorescence. Incandescence. Electric. Bioluminescence Chemiluminescence. Combustion

Red Hot, Blue Hot: Mapping the Invisible Universe

Light and Telescopes

Modern Astronomy Review #1

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

AST 101 Intro to Astronomy: Stars & Galaxies

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

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

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

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

Light: Transverse WAVE

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

Tools of Astronomy Tools of Astronomy

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

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

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

UNIT E: SPACE EXPLORATION

1. The most important aspects of the quantum theory.

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

CHAPTER 28 STARS AND GALAXIES

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

LIFE CYCLE OF A STAR

Inaugural University of Michigan Science Olympiad Tournament

Chapter 17 Practice Questions KEY

Unit 5 Physical Science Radioactivity Answer Key

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

National 3 Waves and Radiation

Review: Properties of a wave

Chapter 21: Stars Notes

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

Useful Formulas and Values

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

Transcription:

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

Remote Sensing = learning about an object or phenomenon without touching, usually using satellites or airplanes h@p://www.nasa.gov/centers/langley/news/factsheets/remotesensing.html

Videos LandSat video: h@p://landsat.gsfc.nasa.gov/about/ Terra orbit anima9on: h@p://earthobservatory.nasa.gov/experiments/ice/panama/panama_mov2.php Watch live broadcast of LandSat: h@p://earthnow.usgs.gov/

h@p://landsat.gsfc.nasa.gov/ Landsat 7 h@p://science.hq.nasa.gov/kids/imagers/ems/infrared.html Band Bandwidth (nm) Radia:on 1 450-515 Blue 2 525-605 Green 3 630-690 Red 4 750-900 Near Infrared 5 1,550-1,750 Shortwave Infrared 6 10,400-12,500 Thermal Infrared 7 2,090-2,350 Shortwave Infrared

h@p://missionscience.nasa.gov/ems/09_visiblelight.html

LandSat Spectral Signatures Band Bandwidth (nm) Radia:on 1 450-515 Blue 2 525-605 Green 3 630-690 Red 4 750-900 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

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

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

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

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

1 2 3 4 5 6 7 8 9 1 2 3 4 5 6 7 8

1 2 3 4 5 6 7 8 9 1 2 3 4 5 6 7 8

h@p://science.hq.nasa.gov/kids/imagers/ems/index.html

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)

Problem #1: Visible Light Which color has the longest wavelength? Which color has the highest frequency? h@p://science.hq.nasa.gov/kids/imagers/ems/index.html Which color has the highest speed?

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

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

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

Microwaves Heat food by making molecules rotate fast Used to detect & measure distance to objects, such as airplanes & weather, with radar h@p://science.hq.nasa.gov/kids/imagers/ems/micro.html sarakwatch.com

Microwaves Credit: NASA/WMAP Science Team h@p://missionscience.nasa.gov/ems/06_microwaves.html

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 Ra@lesnakes use to detect warm- blooded animals Remote sensing Determine temperature of land, water Map clouds, vegeta9on

h@p://www.osdpd.noaa.gov/ml/ocean/sst/sst_50km.html h@p://missionscience.nasa.gov/ ems/07_infraredwaves.html

Infrared Imaging What object is in the image below?

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.

Laser Al:metry (LiDAR) Where are the tallest trees? Outside Davenport, north of Santa Cruz www.nps.edu/faculty/olsen/student_theses/11sep_harmon.pdf Credit: NASA Earth Observatory/Image by Jesse Allen and Robert Simmon/Based on data from Michael Lefsky. h@p://www.nasa.gov/topics/earth/features/forest- height- map.html

Problem #3: Technology Choose one of the following devices Bluetooth (2400 MHz) GPS (1575.42 MHz) Wi- Fi (5 GHz) What wavelength is this? What type of radia9on is this? Garmin.com Wikipedia

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

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

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

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

Mapping Vegeta:on 3-2- 1 North America seasonal NDVI anima9on: h@p://www.nasa.gov/topics/earth/features/obscure_data.html Normalized Difference Vegeta9on Index NDVI = (NIR Red) / (NIR + Red) 4-3- 2

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

Vegeta:on Index Products NASA Earth Observatory

4 3 2 4 3 2 h@p://landsat.gsfc.nasa.gov/ 4-3- 2

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