Ch. 26.1: Our Sun!
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Transcript of Ch. 26.1: Our Sun!
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Ch. 26.1: Our Sun!
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Size
1,000,000 Earths could fit inside
contains 99% of the solar system’s mass
Diameter of 1,400,000 km
If the sun were the size of a bottle cap, the largest known star would be the size of a football field!
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Distance
150,000,000 km away from Earth (average) = 1 Astronomical Unit (AU)
93,000,000 miles
Light, traveling at 300,000 km/s takes 8.5 minutes to reach Earth
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Energy
Fusion of hydrogen (H2) into helium (He) gives sun it’s energy
4 H2 atoms = 1 He atom + energy
Intense heat and pressure causes these atoms to exist in the form of plasma
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Layers
The sun’s temperature decreases from core to surface
From the surface of the sun to the outer atmosphere, the temperature increases
The sun’s layers are heated by convection
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Layers (cont.)Layer/Zone Temperature
(°C)Core 15,000,000
Radiative Zone
8,000,000
Convective Zone
1,500,000
Photosphere 6,000
Chromosphere 20,000
Corona 1,000,000-3,000,000
Sun
Sun’sAtmosphere
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Photosphere (layer 4)
surface of the sun
contains features such as sunspots and granules
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Granules
bubbles of hot gas visible on the surface of the sun
1,000 km in diameter
last about 20 minutes
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Sunspots dark spots on surface of
sun
cooler than surrounding surface
result from complications in sun’s magnetic field
sunspots go from a min to a max and back to min in 11 year cycles
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Solar Flares sudden bursts of
energy from the photosphere through the outer atmosphere
rise up suddenly in areas of sunspot activity
number of solar flares increases with the number of sunspots
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Chromosphere (layer 5) inner layer of
atmosphere
thousands of km’s off of surface
contain solar prominences dense clouds of plasma suspended over surface by magnetic fields
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Corona (layer 6) thin outer
atmosphere
1,000,000 times less bright than photosphere
only visible during solar eclipse
responsible for solar wind
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Solar Wind constant stream of electrically
charged particles from corona
fly in all directions from sun at 450 km/s
takes 2-3 days to reach Earth
solar flares & wind create auroras on Earth particles interact with Earth’s
magnetic field Northern and Southern lights
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Magnetic Storms occur when solar
flares are added to constant solar wind
auroras may be visible at mid-latitudes
electrical surges may disrupt cell phone service & damage electrical appliances