the sun

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The Sun NASA photograph, Skylab, 10 December 1973

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The Sun. NASA photograph, Skylab, 10 December 1973. Sun Facts. Mass 1.989 × 10 30 kg (99.9% of Solar system) Diameter 1.39 million km (109 times Earth) Surface Temperature 6000K Energy Output 3.826 × 10 36 W. Spectrum of the Sun. Source: McMath-Pierce Solar Observatories. Layers. - PowerPoint PPT Presentation

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Page 1: The Sun

The Sun

NASA photograph, Skylab, 10 December 1973

Page 2: The Sun

Sun Facts

• Mass 1.989 × 1030 kg (99.9% of Solar system)• Diameter 1.39 million km (109 times Earth)• Surface Temperature 6000K• Energy Output 3.826 × 1036 W

Page 3: The Sun

Spectrum of the Sun

Source: McMath-Pierce Solar Observatories

Page 4: The Sun

Layers

Source: Gribbin & Gribbin, From Here to Infinity, 2008, p. 68

Page 5: The Sun

Sun’s corona

Source: Koen van Gorp

Page 6: The Sun

Density

Source: Arny & Schneider, Explorations, p.314.

Page 7: The Sun

Fusion in the Core

Source: Seeds, Horizons: Exploring the Universe

Net reaction: 4 p+ 4He + 2 e+ + 2 + 2

Page 8: The Sun

Surface

• Granules– convection cells– Around 1000 km across– Typically last about 10 minutes

Source: NOAO

Page 9: The Sun

Sunspots• Relatively cool surface region • Associated with magnetic disruptions

Source: Vacuum Tower Telescope, National Solar Observatory

Page 10: The Sun

Sun’s Magnetic Field

• Sun’s interior (plasma) conducts electric current

• Sun rotates: faster at equator than poles

Page 11: The Sun

Gas circulation

Source: Solar and Heliospheric Observatory (SOHO)

Page 12: The Sun

Solar Cycle

Source: Solar and Heliospheric Observatory (SOHO)

Page 13: The Sun

Solar cycle

• Magnetic field reverses every ~11 yr

Source: Gribbin & Gribbin, From Here to Infinity, 2008, p. 72