How Solar Panels Work
Solar panels convert sunlight into electricity through the photovoltaic effect. When photons from sunlight hit silicon cells in a panel, they knock electrons loose, creating a flow of direct current (DC) electricity. An inverter then converts this DC power into alternating current (AC) that your home can use. The average US household consumes about 10,632 kilowatt-hours (kWh) of electricity annually, according to the Energy Information Administration (EIA). A typical residential solar system needs to generate this amount—or more if you want to offset future rate increases. Modern solar panels operate at 20-23% efficiency, meaning they convert roughly one-fifth of the sunlight hitting them into usable electricity. The National Renewable Energy Laboratory (NREL) reports that the average US home needs a 7-11 kW system to meet its annual needs, depending on location and energy consumption. Here's a real-world example: A home in Phoenix, Arizona receives about 5.7 peak sun hours daily, while Seattle gets around 3.5 hours. This means the same 10 kW system produces roughly 18,000 kWh annually in Phoenix but only 11,000 kWh in Seattle. Location matters enormously. Grid-tied systems—which make up about 95% of residential installations—remain connected to your local utility. Excess power flows back to the grid, earning you credits through net metering programs. Off-grid systems require battery storage and are typically 3-5 times more expensive, making them practical only for remote properties without utility access.