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Solar Power
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The Sun The Sun’s surface is called the photosphere is 10,000 Fahrenheit. The temperature at the core, or very middle, of the Sun, is about 27 million Fahrenheit. The sun is only important to our solar system. There are over 100 billion stars in the milky way.
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The Sun Is a G2 dwarf star that is 4.6 billion years old
It will burn for another 4.6 billion years The sun is only important to our solar system. There are over 100 billion stars in the milky way.
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The Sun The sun is the closest star to Earth and is million kilometers (92.96 million miles) away The sun rotates on its axis once every Earth days or hours The sun is only important to our solar system. There are over 100 billion stars in the milky way.
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The Sun Approximately 109 planet Earths would fit on the surface of the sun More than one million planet Earths would fit inside of the sun. The sun is only important to our solar system. There are over 100 billion stars in the milky way.
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The Sun 100,000,000,000 tons of dynamite would have to be detonated every second to match the energy produced by the sun The sun is only important to our solar system. There are over 100 billion stars in the milky way.
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The Sun
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How could we utilize the Sun?
The sun is a renewable energy resource. Just a tiny fraction of the Sun's energy that hits the Earth (around a hundredth of a millionth of a percent) is enough to meet all our power needs many times over. In fact, every minute, enough energy arrives at the Earth to meet our demands for a whole year if only we could harness it properly.
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Solar Green House Sun’s short waves go in
Infrared rays cannot get back out Warm air rises from the ground Air collectors heat the ambient air and circulate it around
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Envelope Homes Utilizes convection Passive (no moving parts)
Air collectors heat the ambient air and circulate it around
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Envelope Homes Trombe Walls
Sun goes through glass and is absorbed by the absorber Air collectors heat the ambient air and circulate it around
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Parabolic Dish Reflects rays of the sun to a focal point
Hydronic collectors heat a fluid called a hydronic fluid and then used in heat exchangers or stored in tanks. Water can also be superheated into steam and create electricity.
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Parabolic Trough Reflects rays of the sun to a focal point
Hydronic collectors heat a fluid called a hydronic fluid and then used in heat exchangers or stored in tanks. Water can also be superheated into steam and create electricity.
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Solar Hot Water Water is heated Stored in tanks
Hydronic collectors heat a fluid called a hydronic fluid and then used in heat exchangers or stored in tanks. Water can also be superheated into steam and create electricity.
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Photovoltaic Cells A solar electric system that converts visible sunlight directly into electricity Light hits a silicon or cadmium sulfide and creates a positive and negative charge. Cell acts as a small battery
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Photovoltaic Cells
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Connecting to the Grid
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Solar Thermal Energy Conversion
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What is it? Solar thermal electric energy generation concentrates the light from the sun to create heat, and that heat is used to run a heat engine, which turns a generator to make electricity. The working fluid that is heated by the concentrated sunlight can be a liquid or a gas. Different working fluids include water, oil, salts, air, nitrogen, helium, etc.
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What is it? Different engine types include steam engines, gas turbines, Stirling engines, etc. All of these engines can be quite efficient, often between 30% and 40%, and are capable of producing 10’s to 100’s of megawatts of power. Heat can be stored during the day and then converted into electricity at night.
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Major Solar Thermal Industry Players
eSolar Brightsource Abengoa
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2 types of Solar Thermal Collection
Line Focus Point Focus
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Line Focus Less Expensive Technically less difficult Not as efficient
250° C or 482° F
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Point Focus Series of mirrors surrounding a central tower.
500° C or 932° F
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Point Focus
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Point Focus
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References c “Solar System Exploration: Sun.” NASA.gov. June 11, Accessed: June 10, 2009. d “Sun: The Center of It All.” NationalGeographic.com. Accessed: June 10, 2009.
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