1. Energy from the Sun Living With a Star

3. Sun Facts The Sun is rather ordinary when it comes to stars. The Sun is rather ordinary when it comes to stars. In fact, there are 100 billion stars in our galaxy that are similar to the Sun. In fact, there are 100 billion stars in our galaxy that are similar to the Sun. What makes our star unique is that it is ours—responsible for light, heat, and life as we know it. What makes our star unique is that it is ours—responsible for light, heat, and life as we know it.

4. Learning Objectives Appreciate the scale of the Sun-Earth Appreciate the scale of the Sun-Earth The sun emits a range of energies that make up the Electromagnetic EM spectrum. The sun emits a range of energies that make up the Electromagnetic EM spectrum. The range extends beyond the visible spectrum in both directions, beyond the red and beyond the violet. ROYGBIV The range extends beyond the visible spectrum in both directions, beyond the red and beyond the violet. ROYGBIV The sun is a star that sheds a continuous flow of particles (solar wind) and electromagnetic radiation. The sun is a star that sheds a continuous flow of particles (solar wind) and electromagnetic radiation.

5. and there’s more folks… The Sun’s outer atmosphere is called the corona. The Sun’s outer atmosphere is called the corona. During solar storms, huge bursts of electromagnetic energy are emitted by solar flares During solar storms, huge bursts of electromagnetic energy are emitted by solar flares Flares are sometimes accompanied by Coronal Mass Ejections (CMES) – eruptions of particles in the corona Flares are sometimes accompanied by Coronal Mass Ejections (CMES) – eruptions of particles in the corona EM energies travel at the speed of light EM energies travel at the speed of light Some solar output is harmful Some solar output is harmful

6. Scale Model Demonstration

13. What does the Earth get from the Sun that is essential to keep us alive?

14. What evidence do you have that there is energy reaching you from the Sun?

15. Focusing on Visible Light

16. Photons Light is made up of bundles of energy called photons which travel through space. Light is made up of bundles of energy called photons which travel through space. Each color of light is made of different photon energies. Each color of light is made of different photon energies. The energy level carried by violet light is about twice as much as red light. The energy level carried by violet light is about twice as much as red light. ROYGBIV

17. Colors in Visible Light Electromagnetic Spectrum Electromagneti c energies travel at the speed of light Particles travel at less than the speed of light Particles from the Sun Slower particles Faster Particles Low EnergyVery High Energy

18. Photosphere The visible portion of the Sun. The visible portion of the Sun.

19. Random Walk For the Sun, a photon is generated at the center and makes its way to the surface. It may take up to a thousand years to get to the surface, and the form of the energy may change from X- ray to visible wavelengths. When the photon leaves the Sun, it takes eight minutes to get to us at the speed of light. For the Sun, a photon is generated at the center and makes its way to the surface. It may take up to a thousand years to get to the surface, and the form of the energy may change from X- ray to visible wavelengths. When the photon leaves the Sun, it takes eight minutes to get to us at the speed of light.

20. The 8-minute travel time to Earth by sunlight hides a thousand- year journey that actually began in the core.

21. Sir Fredrick William Herschel In 1800, Sir Fredrick William Herschel split up sunlight using a glass prism instead of a diffraction grating. Herschel's experiment was important not only because it led to the discovery of infrared light, but also because it was the first time that someone showed that there were forms of light that we cannot see with our eyes. In 1800, Sir Fredrick William Herschel split up sunlight using a glass prism instead of a diffraction grating. Herschel's experiment was important not only because it led to the discovery of infrared light, but also because it was the first time that someone showed that there were forms of light that we cannot see with our eyes.

24. Infrared Video Clips

25. ROYGBIVROYGBIVROYGBIVROYGBIV Infrared Colors in Visible Light Electromagnetic Spectrum Electromagneti c energies travel at the speed of light Particles travel at less than the speed of light Particles from the Sun Slower particles Faster Particles Low EnergyVery High Energy

26. CD ROM Play movie Infrared and Its Uses Play movie Infrared and Its Uses

27. Ultraviolet or UV Right of the violet end of the spectrum. Right of the violet end of the spectrum. Invisible to humans Invisible to humans Bees can see it Bees can see it Judging by where ultraviolet energy is located on this spectrum, do you think it has more or less energy than visible light? Judging by where ultraviolet energy is located on this spectrum, do you think it has more or less energy than visible light?

28. What have you heard about UV? Cause sunburn Cause sunburn Damage our eyes Damage our eyes Sunscreen and sunglasses block it Sunscreen and sunglasses block it

29. ROYGBIVROYGBIVROYGBIVROYGBIV Radio WavesMicrowavesInfraredUltraviolet Colors in Visible Light Electromagnetic Spectrum Electromagneti c energies travel at the speed of light Particles travel at less than the speed of light Particles from the Sun Slower particles Faster Particles Low EnergyVery High Energy

31. CD ROM Looking at various wave lengths that make up the electromagnetic spectrum. Looking at various wave lengths that make up the electromagnetic spectrum.

32. Solar Wind Particle

33. Coronal Mass Ejections CME Occasionally, a part of the Sun’s upper atmosphere (corona) erupts in a giant gust of solar storm particles called a Coronal Mass Ejection or CME Occasionally, a part of the Sun’s upper atmosphere (corona) erupts in a giant gust of solar storm particles called a Coronal Mass Ejection or CME Some CMEs are ejected outward from the Sun in the direction of Earth. Some CMEs are ejected outward from the Sun in the direction of Earth. CMEs often accompany solar flares. CMEs often accompany solar flares.

34. ROYGBIVROYGBIVROYGBIVROYGBIV Radio WavesMicrowavesInfraredUltravioletX-RaysGamma Rays Colors in Visible Light Electromagnetic Spectrum Electromagneti c energies travel at the speed of light Particles travel at less than the speed of light Particles from the Sun Slower particles Faster Particles Low EnergyVery High Energy

37. The Culprit in the Mystery Will CME, EM and solar wind knowledge help decide if the Sun caused the January disruptions in Earth? Will CME, EM and solar wind knowledge help decide if the Sun caused the January disruptions in Earth? What happened to the Sun at 3:10 on 01/25? What happened to the Sun at 3:10 on 01/25?

38. If the solar flare affected Earth in eight minutes, why did many of the mysterious events happen two days later, on 01/27? If the solar flare affected Earth in eight minutes, why did many of the mysterious events happen two days later, on 01/27?

39. Do CMEs travel at the speed of light? Do CMEs travel at the speed of light?

40. Is the Sun always sending out both EM energy and solar wind? Is the Sun always sending out both EM energy and solar wind? How fast does EM energy travel? How fast does EM energy travel? How fast does solar wind travel? How fast does solar wind travel? What happened on the Sun on 01/25? What happened on the Sun on 01/25? What happened on the Earth around 3:18? What happened on the Earth around 3:18? What happened on the Earth two days later? What happened on the Earth two days later? What do you think caused the events on 01/27? What do you think caused the events on 01/27?

41. Knowing what you know now, do you think the solar flare and CME caused the mysterious events in Activity 1? Knowing what you know now, do you think the solar flare and CME caused the mysterious events in Activity 1?