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The SUN.

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Presentation on theme: "The SUN."— Presentation transcript:

1 The SUN

2 What is the earth’s primary source of energy?
The Sun

3 What is the sun made of? Gas

4 3. Draw the sun and label the four main parts.

5 Photos Light

6 Sphere Ball

7 6. The photosphere is the surface of the sun. What does it do?
Radiates light from the sun

8 7. The sun’s photosphere is composed of 90%__________ and 10%_________.
Hydrogen Helium Hydrogen atoms

9 8. Chromosphere Thin layer of hot gases

10 9. Corona Outermost portion of the solar atmosphere

11 10. Solar Wind Streams of protons and electrons that boil from the corona

12 11. Sunspot Dark areas on the surface of the photosphere

13 12. Why do sunspots appear dark?
Because of their cooler temperature, 1500 k ( °F) less than the surrounding solar surface.

14 13. Prominences Huge cloudlike structures made of chromospheric gases

15 14. Solar Flare Brief outbursts of energy from a sunspot

16 Solar Flare

17 15. What do solar flares release?
Ultraviolet, radio, and X-ray radiation

18 16. What causes an Aurora? A strong solar flare

19 17. What is another name for an Aurora?
Northern and Southern Lights

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23 18. Deep in its interior, the sun produces energy by a process known as __________ _________.
Nuclear Fusion H H

24 19. What happens during the process of nuclear fusion?
Four hydrogen nuclei are converted into the nucleus of a helium atom Energy is released

25 20. What is Einstein’s equation and what does it mean?
E = mc2 The energy of an object is equal to its mass X the speed of light squared

26 LIGHT

27 1. Electromagnetic Radiation
Types of energy. Gamma rays X-rays Ultraviolet light Visible light Infrared radiation Microwaves Radio waves

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29 Longer wavelength Shorter wavelength

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31 2. Wavelength Distance from one wave crest (top) to the next.

32 3. Frequency The number of waves in a certain distance.

33 4. Electromagnetic Spectrum
Arrangement of waves according to their wavelength and frequencies.

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35 5. Speed of Light 300,000 km/s or 3.0 x 105 km/s or 3.0E5 km/s. All forms of energy waves travel at this speed.

36 How fast is the speed of light in miles per hour?
1 km per hour = _______________ mph 300,000 km per second X 60 seconds = 18,000,000 km per hour 18,000,000 km per hour X = 11,184, mph

37 6. Visible Light The band of electromagnetic radiation we can see.

38 7. Photon Stream of light particles, a small particle of light.

39 8. Radiation Pressure The force exerted by photons. Photons actually push on matter.

40 Radiation The transfer of energy (heat) through space by electromagnetic waves.

41 COLOR WAVELENGTH Violet 380-440 Blue 440-500 Green 500-560 Yellow
Table 1: Colors and Corresponding Wavelengths COLOR WAVELENGTH Violet Blue Green Yellow Orange Red

42 9. Which color has the longest wavelength?
RED 10. Which color has the highest frequency? VIOLET

43 Longer wavelength = Lower Frequency Shorter wavelength =
Higher Frequency More Energy

44 24.1 The Study of Light Spectroscopy  Absorption Spectrum
• An absorption spectrum is a continuous spectrum produced when white light passes through a cool gas under low pressure. The gas absorbs selected wavelengths of light, and the spectrum looks like it has dark lines superimposed.

45 24.1 The Study of Light Spectroscopy  Emission Spectrum
• An emission spectrum is a series of bright lines of particular wavelengths produced by a hot gas under low pressure. • When the spectrum of a star is studied, the spectral lines act as “fingerprints.” These lines identify the elements present and thus the star’s chemical composition.

46 Formation of Spectra Makes no sense without caption in book

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51 24.1 The Study of Light The Doppler Effect
 The Doppler effect is the apparent change in frequency of electromagnetic or sound waves caused by the relative motions of the source and the observer.  In astronomy, the Doppler effect is used to determine whether a star or other body in space is moving away from or toward Earth.

52 The Doppler Effect Makes no sense without caption in book

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55 Doppler effect on light


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