Solar prominence - PowerPoint PPT Presentation

The Sun

The Sun. Properties. M = 2 X 10 30 kg = 300,000 M Earth R = 700,000 km &gt; 100 R Earth 70% H, 28% He T = 5800 K surface, 15,000,000 K core. Structure. Sun’s Atmosphere. Sun’s Atmosphere. Solar Wind – stream of particles blown out from the sun Corona

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Chapter 23

Chapter 23. Our Solar System. Our Solar System. Historical Astronomy – Wandering Stars. Greeks watched the stars move across the sky and noticed five “stars” that wandered around and did not follow the paths of the normal stars. They called them Wander Stars “planets”.

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563 views • 28 slides

Chapter 23

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446 views • 28 slides

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