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  • Slide 1
  • How does light differ? Light Source Color Pattern seen in spectroscope Red Light Bulb Daylight Light Bulb Fluorescent Light Bright Sky DO NOT look directly at the sun. How did the colors in each light source differ? Explore how the spectroscope might be used to learn about stars. How does light differ? Light Source Color Pattern seen in spectroscope Red Light Bulb Daylight Light Bulb Fluorescent Light Bright Sky DO NOT look directly at the sun. How did the colors in each light source differ? Explore how the spectroscope might be used to learn about stars.
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  • The Big Bang by ______________.
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  • The Big Bang Read lesson 7.4 in your textbook. Then write 300 words on the topic.. _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________ _________________________
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  • Radio Waves Size: Radio waves range from the size of a water bottle to the diameter of the Earth Source Neutron Stars Radio Tower Detection Radio Satellite
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  • Microwaves Size millimeter wavelengths Sources Human Signals UHF TV Big Bang Cosmic Background Radiation Sun Supermassive Black Holes Detection Remote Sensing and Weather Simulated microwave release from supermassive blackhole Cosmic Background Radiation from the Big Bang
  • Slide 7
  • Infrared Radiation (IR) Source Heat From sun Re-radiation of Heat Warming effect on Earth Detection Spitzer Space Telescope Weather Radars Pit Vipers Infrared Cat The image on the left shows an optical view of a star forming region. The same area is shown on the right in infrared radiation. Notice how the infrared observations penetrate the obscuring cloud to reveal many new details.
  • Slide 8
  • Visible Light Source Sun and Lightbulbs Detection Telescope on the roof of RLM Building at UT McDonald Observatory Hubble Space Telescope Photo of Saturn from telescope on top of RLM at UT Hubble and Hubble photo of Jupiter
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  • Ultraviolet (UV) Source Stars (Produces sunburns and makes vitamin D) Ozone blocks UV radiation Black Lights and Electric Arcs Detection Insects NASA's Extreme Ultraviolet Explorer satellite
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  • X-Rays Source Stars Neutron stars and from object being pulled into a black hole Detection Chandra X-Ray Observatory Auroras of Jupiter Picture used overlain images from Chandra and Hubble
  • Slide 11
  • Gamma Radiation Size Wavelengths are smaller than an atom Source Supernovas Produced on Earth from Radioactive Decay and Lightning Detection Fermi Gamma Ray Space Telescope Fermi Gamma Ray Space Telescope
  • Slide 12
  • Astronomy Unit 3: Big Bang and Electromagnetic Radiation
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  • Electromagnetic Radiation and the Big Bang Astronomy Unit 3 Electromagnetic Spectrum How we know what stars are made of. The Big Bang Inflation of the Universe 13.7 Billion Years ago
  • Slide 14
  • Vocabulary electromagnetic radiation: a form of energy that travels through space as waves; called EM radiation for short electromagnetic spectrum: the variety of forms of EM radiation, such as radio waves, microwaves, visible light, and X-rays optical telescope: an instrument that uses light and lenses to study distant objects radio telescope: an instrument that collects and analyzes radio waves from stars and other objects in space observatory: a building or room that houses one or more telescopes
  • Slide 15
  • Unit 3 Vocabulary electromagnetic radiation: a form of energy that travels through space as waves; called EM radiation for short electromagnetic spectrum: the variety of forms of EM radiation, such as radio waves, microwaves, visible light, and X-rays optical telescope: an instrument that uses light and lenses to study distant objects radio telescope: an instrument that collects and analyzes radio waves from stars and other objects in space observatory: a building or room that houses one or more telescopes electromagnetic radiation: a form of energy that travels through space as waves; called EM radiation for short electromagnetic spectrum: the variety of forms of EM radiation, such as radio waves, microwaves, visible light, and X-rays optical telescope: an instrument that uses light and lenses to study distant objects radio telescope: an instrument that collects and analyzes radio waves from stars and other objects in space observatory: a building or room that houses one or more telescopes Unit 3 Vocabulary electromagnetic radiation: a form of energy that travels through space as waves; called EM radiation for short electromagnetic spectrum: the variety of forms of EM radiation, such as radio waves, microwaves, visible light, and X-rays optical telescope: an instrument that uses light and lenses to study distant objects radio telescope: an instrument that collects and analyzes radio waves from stars and other objects in space observatory: a building or room that houses one or more telescopes electromagnetic radiation: a form of energy that travels through space as waves; called EM radiation for short electromagnetic spectrum: the variety of forms of EM radiation, such as radio waves, microwaves, visible light, and X-rays optical telescope: an instrument that uses light and lenses to study distant objects radio telescope: an instrument that collects and analyzes radio waves from stars and other objects in space observatory: a building or room that houses one or more telescopes Unit 3 Vocabulary
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  • X-Ray Gamma Ultraviolet Visible Infrared Microwaves Radio Glue Here Remember only 8 dots of glue! Fold here
  • Slide 19
  • Electromagnetic Radiation
  • Slide 20
  • Electromagnetic Spectrum electromagnetic radiation: a form of energy that travels through space as waves; called EM radiation for short electromagnetic spectrum: the variety of forms of EM radiation, such as radio waves, microwaves, visible light, and X-rays
  • Slide 21
  • Electromagnetic Spectrum
  • Slide 22
  • Austins Radio Towers on Mount Larsen
  • Slide 23
  • Concepts Regarding Electromagnetic Spectrum Electromagnetic (EM) radiation is a form of energy that can travel through space. The different forms of EM radiation make up the electromagnetic spectrum. Light, radio waves, microwaves, and X-rays are all forms of EM radiation. Each form of EM radiation has a certain range of wavelengths and frequencies. All forms travel through space at the same speed, which is 3.0 10 8 meters per second. This value is called the speed of light. Stars and other objects of the universe give off visible light and other forms of EM radiation. The eyes and optical telescopes can detect the light that they give off. Other telescopes have been built to detect radio waves, microwaves, and X-rays from space. To reach Earths surface, EM radiation from space must pass through Earths atmosphere. The atmosphere distorts or blocks some of the radiation. This limits the usefulness of Earth-bound telescopes. Other telescopes, such as the Hubble Space Telescope, are aboard satellites. These telescopes can detect EM radiation from space very clearly. They produce very detailed, highly magnified images of objects in space. Scientists study the data from telescopes. This lets them learn about the distances and physical properties of stars and other components of the universe.
  • Slide 24
  • Telescopes and their Wavelengths Video: Wavelenths and Fermi
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  • All EM Radiation Travels at the speed of light. Each form of EM radiation has a certain range of wavelengths and frequencies. All forms travel through space at the same speed, which is 3.0 10 8 meters per second. This value is called the speed of light.
  • Slide 26
  • Electromagnetic Radiation meets the Earths Atmosphere Which type of EM radiation reaches the earths surface? Ultraviolet Visible Infrared Radio
  • Slide 27
  • What types of Electromagnetic radiation reach the Earths Surface? 1. 2. 3. 4. Electromagnetic Radiation What types of Electromagnetic radiation reach the Earths Surface? 1. 2. 3. 4. Electromagnetic Radiation
  • Slide 28
  • How do we know what we know about the Universe? We know what we know because these inventions. Collect this data. Which is interpreted by these scientist.
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  • Importance of Electromagnetic Radiation Astronomical Images in Different Wavelengths Electromagnetic Radiation provides the data that scientist use to understand the distances and physical properties of stars and other components of the universe. Scientist use telescopes to detect electromagnetic radiation from space. To reach Earths surface, EM radiation from space must pass through Earths atmosphere. The atmosphere distorts or blocks some of the radiation. This limits the usefulness of Earth-bound telescopes.
  • Slide 30
  • Images using different wavelengths Astronomical Images in Different Wavelengths
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  • Quarter 1 Review Stations Station2 sentences about what you learned Stamp Ballooniverse EM Spectrum Wavestown Newtonss laws Moon Phases and Why does the moon change shape? The Reason for the Seasons Station2 sentences about what you learned Stamp Ballooniverse EM Spectrum Wavestown Newtonss laws Moon Phases The Reason for the Seasons Quarter 1 Review Stations
  • Slide 33
  • Astronomy Unit Reflection What I learnedHow I learned it What I learnedHow I learned it Astronomy Unit Reflection
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  • The Reason for the Seasons The reason we have seasons is that, as the Earth revolves around the sun it is closer to the sun in the summertime; therefore, it is warmed in summer and cooler in winter. 1.Why do you think some people have this idea about the reason for the season? 2.What thinks could you do to help someone understand the scientific explanation for seasons? How would this help someone give up his or her original idea in favor of the scientific one? 3.Did you ever have similar Missed Conception at the beginning of this unit or sometime in your life? How and/or why has your thinking changed or not changed? 4.Draw the Earth during all 4 seasons. Label the seasons in the Northern and Southern Hemisphere. The Reason for the Seasons The reason we have seasons is that, as the Earth revolves around the sun it is closer to the sun in the summertime; therefore, it is warmed in summer and cooler in winter. 1.Why do you think some people have this idea about the reason for the season? 2.What thinks could you do to help someone understand the scientific explanation for seasons? How would this help someone give up his or her original idea in favor of the scientific one? 3.Did you ever have similar Missed Conception at the beginning of this unit or sometime in your life? How and/or why has your thinking changed or not changed? 4.Draw the Earth during all 4 seasons. Label the seasons in the Northern and Southern Hemisphere.
  • Slide 35
  • Moon Phases
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  • View from Earth Now draw in the correct view from the Earth for each phase using the right picture from the box. Use the diagram to explain why the Moon changes shape. Join the number to the correct name for the phase. PhaseName 1Waning crescent 2 Full moon 3 First quarter 4New moon 5Waning gibbous 6Waxing crescent 7Last quarter 8Waxing gibbous Why does the Moon change shape? 1 2 3 4 5 6 7 8 7 8 1 2 3 4 5 6 www.snapshotscience.co.uk, 2010 1 2 3 4 5 6 7 8 7 8 1 2 3 4 5 6 Shade in the parts of the moon that will get no light from the Sun in this diagram. The first one is done for you. Now draw in the correct view from the Earth for each phase using the right picture from the box. Use the diagram to explain why the Moon changes shape. Join the number to the correct name for the phase. PhaseName 1Waning crescent 2 Full moon 3 First quarter 4New moon 5Waning gibbous 6Waxing crescent 7Last quarter 8Waxing gibbous www.snapshotscience.co.uk, 2010 Why does the Moon change shape? Shade in the parts of the moon that will get no light from the Sun in this diagram. The first one is done for you.
  • Slide 37
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  • Electromagnetic Spectrum 1.What are the 6 different types of electromagnetic radiation? 2.What makes them different from one another? 3.Which type of EM radiation has the longest wavelength? 4.Which type of EM radiation has the shortest wavelength? 5.What type of radiation do supernovas produce? 6.What type of radiation do Black holes produce? 7.What type of EM radiation is a rainbow? 8.What are the colors of visible light? 9.What types of EM radiation penetrate the Earths atmosphere? 10.What type of EM radiation do the following satellites receive? FERMI CHANDRA HUBBLE 11.Tell me 3 interesting things about Electromagnetic Radiation. 1.What are the 6 different types of electromagnetic radiation? 2.What makes them different from one another? 3.Which type of EM radiation has the longest wavelength? 4.Which type of EM radiation has the shortest wavelength? 5.What type of radiation do supernovas produce? 6.What type of radiation do Black holes produce? 7.What type of EM radiation is a rainbow? 8.What are the colors of visible light? 9.What types of EM radiation penetrate the Earths atmosphere? 10.What type of EM radiation do the following satellites receive? FERMI CHANDRA HUBBLE 11.Tell me 3 interesting things about Electromagnetic Radiation. Electromagnetic Spectrum
  • Slide 39
  • Ballooniverse Purpose: to create a model that illustrates how the universe expands Materials: balloon marker tape measure (or string & ruler) Procedures: 1. Inflate your balloon until it is about 4 inches (10 cm) in diameter, but do not tie the end. 2. Using the marker, make six dots on the balloon in widely scattered locations. Label one dot "home" and the others A-E. The home dot represents the Milky Way galaxy, and the others represent galaxies formed in the early universe. 3. Without letting air out of the balloon, use the tape measure (or string & ruler) to measure the distance from home to each dot. Record the distances in the table under the heading "Measurement 1." 4. Using your tape measure (or string & ruler), determine the circumference of the balloon. Record the circumference in the table under the heading Measurement 1. 5. Inflate the balloon so that its diameter is about 4 inches (10 cm) bigger ( 20 cm). Make a prediction about the new distances from home to dots A-E. Adapted from: http://school.discoveryeducation.com/curriculumcenter/universe/activity2.html
  • Slide 40
  • Ballooniverse Conclusion/Questions: Illustrate the changes of your ballon below. 1.How did the distance from the home dot to each of the other galaxies change each time you inflated the balloon? 2. Did the galaxies near home or those farther away appear to move the greatest distance? 3. How could you use this model to simulate the Big Crunch, a time when all the galaxies might collapse in on themselves? Ballooniverse
  • Slide 41
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  • Wavestown Answer Key 1. Radio Waves Rays TV - TV reception uses radio waves Satellite Dish at Rays TV - receives movies via radio waves from a satellite Taxi - Car radio receives radio wave signals Taxi - Driver receives instructions on a CB radio which uses radio waves Radio Tower - broadcasts radio signals Large Satellite dish in field - receives radio waves from distant stars 2. Microwaves Microwave in Waves Grill - uses microwaves to cook food Disk-like antennas on tower - send microwave communications 3. Infrared Heat lamps above food in Waves Grill - use infrared waves to keep food hot Rays TV - Remote controls use infrared waves to communicate with the TV Trees, bushes, grass, and farm - vegetation reflects short infrared waves Observatory - astronomers study thermal infrared (long infrared waves) from stars 4. Visible Light Rainbow - water droplets cause white light to break apart into the colors of the rainbow Photographers studio - portrait photographers use film sensitive to visible light Observatory - astronomers look at visible light from planets and stars 5. Ultraviolet Tanning Salon - use ultraviolet waves to tan our skin sunglasses store - sunglasses protect our eyes from the ultraviolet waves Suntan lotion - protects our skin from ultraviolet waves Observatory - astronomers see some ultraviolet radiation from planets and stars 6. X-rays Dr.Bobs Health Clinic - uses x-rays to study our bones High energy x-rays are also used to treat cancer 7. Gamma Rays Dr.Bobs Health Clinic - gamma radiation is used to kill sick cells through nuclear medicine Gamma radiation is given off by nuclear explosions that occur within stars, like our sun.
  • Slide 43
  • Wavestown Introduction to the Electromagnetic Spectrum Directions: Use the descriptions below to help locate examples of electromagnetic waves in the Wavestown picture. Radio waves have the longest wavelength in the electromagnetic spectrum. These waves carry the news, ball games, and music you listen to on the radio. They also carry signals to television sets and cellular phones. Microwaves have shorter wavelengths than radio waves, which heat the food we eat. They are also used for radar images, like the Doppler radar used in weather forecasts. There are infrared waves with long wavelengths and short wavelengths. Infrared waves with long wavelengths are different from infrared waves with short wavelengths. Infrared waves with long wavelengths can be detected as heat. Your radiator or heater gives off these long infrared waves. We call these thermal infrared or far infrared waves. The sun gives off infrared waves with shorter wavelengths. Plants reflect these waves, also known as near infrared waves. Visible light waves are the only electromagnetic waves we can see. We see these waves as the colors of the rainbow. Each color has a different wavelength. Red has the longest wavelength and violet has the shortest wavelength. These waves combine to make white light. Ultraviolet waves have wavelengths shorter than visible light waves. These waves are invisible to the human eye, but some insects can see them. Of the sun's light, the ultraviolet waves are responsible for causing our sunburns. X-Rays: As wavelengths get smaller, the waves have more energy. X-Rays have smaller wavelengths and therefore more energy than the ultraviolet waves. X-Rays are so powerful that they pass easily through the skin allowing doctors to look at our bones. Gamma Rays have the smallest wavelength and the most energy of the waves in the electromagnetic spectrum. These waves are generated by radioactive atoms and in nuclear explosions. Gamma rays can kill living cells, but doctors can use gamma rays to kill diseased cells.
  • Slide 44
  • Wavestown Waves
  • Slide 45
  • Newtons Laws 1. A magician pulls a tablecloth out from under dishes and glasses on a table without disturbing them. 2. A tire is thrown outward as a car rounds a curve on a highway. 3. Rockets are launched into space using jet propulsion where exhaust accelerates out from the rocket and the rocket accelerates in an opposite direction. 4. A picture is hanging on a wall and does not move. 5. Pushing a child on a swing is easier than pushing an adult on the same swing, because the adult has more inertia. 6.A soccer ball accelerates more than a bowling ball when thrown with the same force. 7.A soccer player kicks a ball with their foot and their toes are left stinging. 8.A student leaves a pencil on a desk and the pencil stays in the same spot until another student picks it up. 9.Two students are in a baseball game. The first student hits a ball very hard and it has a greater acceleration than the second student who bunts the ball lightly. 10.For each of Newtons Laws write a hastag. Pick the best of each of the laws from your table group, write then on a post it note and place it in the designated location. Newtons 1 st Law - # Newtons 2 nd Law - # Newtons 3 rd Law - # Newtons Laws 1. A magician pulls a tablecloth out from under dishes and glasses on a table without disturbing them. 2. A tire is thrown outward as a car rounds a curve on a highway. 3. Rockets are launched into space using jet propulsion where exhaust accelerates out from the rocket and the rocket accelerates in an opposite direction. 4. A picture is hanging on a wall and does not move. 5. Pushing a child on a swing is easier than pushing an adult on the same swing, because the adult has more inertia. 6.A soccer ball accelerates more than a bowling ball when thrown with the same force. 7.A soccer player kicks a ball with their foot and their toes are left stinging. 8.A student leaves a pencil on a desk and the pencil stays in the same spot until another student picks it up. 9.Two students are in a baseball game. The first student hits a ball very hard and it has a greater acceleration than the second student who bunts the ball lightly. 10.For each of Newtons Laws write a hastag. Pick the best of each of the laws from your table group, write then on a post it note and place it in the designated location. Newtons 1 st Law - # Newtons 2 nd Law - # Newtons 3 rd Law - #
  • Slide 46
  • #Newtons1stlaw #Newtons2ndlaw #Newtons3rdlaw