Abstract
Do you like getting something for nothing? Everybody likes getting things for free. How about getting energy and power for free? The Sun sends us free energy every second and all we have to do is collect it. Taking advantage of free energy can reduce our dependence on fossil fuels, which are harmful to our environment. In this science fair project, you will work with a solar panel, which is a collector of free energy, and investigate how varying the angle of the solar panel, and thus the amount of light it absorbs, affects the solar panel's output power.Objective
To investigate the effect of the angle of incident light on the output power of a solar panel and determine which angle of incidence produces the most output power.
Introduction
Did you know that the core of the Sun is a series of constant nuclear explosions that turn hydrogen into energy? The temperature in the core of the Sun reaches almost 27 million°F, and the Sun produces 3.8x1026 watts (W) of power and 1.4x1031 joules (J) of energy every hour!
![]() Figure 1. Shown here is a composite image of multiple solar flares, which are hot eruptions, on the Sun. (JAXA, 2008.) |
The Sun provides energy to the Earth in the form of radiated heat and light. The energy that the Earth receives is called insolation. Insolation can be expressed in the units of watts per square meter (W/m2) or kilowatt-hours per square meter (kWh/m2) per day. Of the insolation that arrives at the Earth's upper atmosphere, about half is reflected back into space. The remainder—approximately 50%—of the insolation is absorbed by Earth's oceans and landmass. This means that the Earth is continuously absorbing 89 petawatts! Insolation plays a huge role in many of Earth's functions; for instance, it powers the water cycle and is responsible for almost all of the Earth's renewable energy sources, such as wind and wave energy. There is more than enough free solar energy available to power human energy needs.
Insolation is affected by Earth's atmosphere and the angle of incidence of sunlight on the atmosphere. On a clear day at sea level, when the Sun's rays hit perpendicular to the Earth's surface, we receive 1000 W/m2 of insolation. Because Earth is round, the Sun strikes the surface at different angles, from 0 degrees to 90 degrees. At lower degrees, the insolation travels longer through the atmosphere and becomes scattered and diffuse; whereas at higher degrees, there is less atmosphere to travel through, so more of the Sun's energy hits Earth. The tilt of Earth's axis also affects the amount of insolation reaching the Earth.
![]() Figure 2. This is the average annual insolation on the Earth's surface. (Wikipedia, 2008.) |
So now you know that the angle of sunlight affects the amount of insolation and power that is absorbed by Earth. But how do we capture and use the insolation? There are many ways of doing this, and this science fair project will allow you to investigate one of those ways: photovoltaic devices.
A photovoltaic device, or solar cell, is a semiconductor device. It is used to convert light into electricity. When a packet of light, called a photon, hits the surface of the solar cell, it is absorbed by the semiconductor. When the photon is absorbed, it creates electrons and holes in the semiconductor. The movement of electrons is electrical current. The amount of electrical current created depends on the amount of insolation, or the number of photons, that hits the surface of the solar cell. Electrical current is proportional to the power that the solar cell delivers.
In this science fair project, you will investigate the output power of a solar panel (a collection of solar cells) as a function of the angle of incoming light (the angle of incidence). Measuring the angle of incoming light is a bit tricky, so you will be changing the angle of incident light by changing the angle of the solar panel. You will model how the Sun interacts with the Earth. Check out this science fair project and get something for nothing!
Terms, Concepts and Questions to Start Background Research
Bibliography
The following websites will give you interesting information on the Sun and solar energy:
The United States Department of Energy's websites have good information and factual links:
This website explains the difference between power and energy:
Materials and Equipment
Experimental Procedure
| Figure 3. This is a schematic of three ways that the solar panel can be placed. (a) The panel at 0 degrees. (b) The panel at 90 degrees, and (c) the panel at an unknown but calculable angle, η. |
| Figure 4. Calculating σ is the first step in finding the angle of the solar panel. The value b is the height of the solar panel, while a is the length. |
Equation 1:
| σ = tan-1 | ( | b a | ) |
|
Equation 2:
| 180 degrees = η + 90 degrees + σ |
Equation 3:
| η = 180 degrees − 90 degrees − σ |
Equation 4:
| η = 90 degrees − tan-1 | ( | b a | ) |
Figure 5. Measuring open-circuit voltage and short-circuit current. |
Equation 5:
| Solar panel maximum output power | = | Short-circuit current × Open-circuit voltage |
| Poutput | = | ISC × VOC |
|
| Solar Panel Angle | b | a | σ | η | VOC | ISC | Solar Panel Output Power |
| Angle #1 | Trial 1: | Trial 1: | |||||
| Trial 2: | Trial 2: | ||||||
| Trial 3: | Trial 3: | ||||||
| Average: | Average: | ||||||
| Angle #2 | Trial 1: | Trial 1: | |||||
| Trial 2: | Trial 2: | ||||||
| Trial 3: | Trial 3: | ||||||
| Average: | Average: | ||||||
| Angle #3 | Trial 1: | Trial 1: | |||||
| Trial 2: | Trial 2: | ||||||
| Trial 3: | Trial 3: | ||||||
| Average: | Average: | ||||||
| Lamp position= | |||||||
Variations
Credits
Michelle Maranowski, PhD, Science Buddies
Last edit date: 2008-07-26 23:00:00
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