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Our Sun.

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Presentation on theme: "Our Sun."— Presentation transcript:

1 Our Sun

2 The Sun Largest object in the solar system
The sun has 99% of all mass in the solar system It is low density—similar to gas giants The sun controls motions of all objects in the solar system Planets Comets Asteroids

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4 Layers of the Sun

5 Layers of the sun Core is the innermost layer
It is more dense than lead, but not solid It is the site of nuclear fusion 18,000,000 oF! Photosphere is lowest layer of Sun’s atmosphere 400 km thick It is the visible layer of the sun Thought of as the “surface of the sun” 10,000 oF

6 Chromosphere is the middle layer of Sun’s atmosphere
Visible only with filters as a red aura Corona is the top most layer of Sun’s atmosphere Visible only during a solar eclipse 1.7 t0 3.5 million oF Extends several million km above chromosphere

7 Other features of the Sun
Solar wind is gas flowing outward from Sun at high speeds 400 km/s Charged particles from the wind are trapped in Van Allen belts and can be seen as aurora borealis: “northern lights” Solar flares are eruptions of radiation Prominence are large jets of gas (loops)

8 Northern Lights as seen from Earth

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10 How Northern Lights Work

11 Sunspots Sunspots are dark spots on Sun’s surface
Sun’s magnetic field breaks through photosphere Appear darker because of cooler temp.

12 Close up of sunspot

13 Solar Prominences

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16 The Sun’s Energy Nuclear fusion of Hydrogen into Helium
Not all of Sun’s energy reaches Earth because of the atmosphere Our sun is “middle aged” having converted half of its Hydrodgen

17 Visible light Spectrum is the arrangement of visible light based on wavelength Violet is the shortest wavelength Red is the longest wavelength 3 types of light Absorption Emission Continuous


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