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The Solar System The Sun.

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Presentation on theme: "The Solar System The Sun."— Presentation transcript:

1 The Solar System The Sun

2 Objectives Describe the basic structure and composition of the sun
Explain how the sun generates energy Describe the surface activity of the sun, and identify how this activity affects Earth

3 Did You Know??? 1) 99% of the solar systems mass is concentrated in the sun. 2) Mass: 333,060 X Earth (1,989,100 x 10¹² kg) 3) The temperature of the center of the sun is 26,999,540 oF 4) The surface temperature of the sun is about 11,000 oF 5) Diameter: 1,392,648 km 6) Composition: hydrogen and helium 7) Distance from the sun (average): 150 million km (1 AU) Source -

4 The Sun

5 The Sun

6 The Structure of the Sun

7 Parts of the Sun Corona – The outer layer of the sun’s atmosphere
Chromosphere – Thin area below the corona Photosphere – The visible part of the sun we see from earth Convection Zone – Area where gasses circulate Radioactive Zone – Dense region below the Convection Zone Core – Center of the sun where energy is produced

8 The Structure of the Sun

9 Parts of the Sun

10 Is the Sun burning?????? For many years scientists thought the sun burned fuel to generate energy The Sun does NOT burn fuel If the sun was burning it would only last for 10,000 years before it ran out of fuel

11 Nuclear Fusion Nuclear Fusion – The process where 2 or more nuclei join together (fuse) During this process, a massive amount of energy is created  Albert Einstein proved this with his famous formula E = mc2 Energy = mass . speed of light2

12 Nuclear Fusion Because of the high temperatures and pressure of the sun, Nuclei of Hydrogen, which would normally repel each other are smashed together creating helium. This creates a massive amount of energy

13 Nuclear Fusion of the Sun

14 Solar Activity Sunspots – A dark area of the photosphere of the sun that is cooler than the surrounding areas It also has a strong magnetic field Sunspots last about 11 years

15 Sunspots

16 Solar Activity Solar Flares – Regions of extremely high temperatures
Solar flares can extend several thousand kilometers within minutes Solar flares usually occur near sunspots They can interrupt radio communication on Earth

17 Solar Flares

18 Solar Flares

19 Solar Flares

20 Solar Flares

21

22 Earth’s Magnetic Field

23 Solar Flares and Earth

24 Review The photosphere is the visible part of the sun on the earth
The Sun is not burning, it creates energy through nuclear fusion The sun’s nuclear fusion comes from changing hydrogen into helium Sunspots are colder spots on the suns surface Solar Flares are hot spots that shoot out from the sun Earths magnetic field and atmosphere protect it from the sun


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