Solar Energy: Falling Prices, Improving Efficiencies

 | Jul 21, 2013 03:11AM ET

I am a solar energy enthusiast. The energetic parts of the universe are clustered around stars. We sit here on this dusty ball of rock and water, heated continually by the Sun. The difference between when we face toward our local star and when we face away from it is — in the most literal sense — day and night. Our lives on Earth are already solar-powered; the plants (and plant-eating animals) we eat get their energy from photosynthesis. The trees and other biomass we have used for energy for much of our history, as well as the fossil fuel reserves we use today are forms of stored solar energy from earlier organisms that died and were trapped under the Earth. Wind energy and tidal energy are perturbations of dynamical systems heated by solar energy. Even the nuclear energy we use extracted from fissionable uranium and plutonium is stored from supernovae in early stars that exploded and pushed the complex elements — including the carbon, nitrogen and oxygen in our bodies — out across the universe.

It is not so much a question of whether we use solar energy, but whether we use direct solar energy, or some derivative form. As our civilisation has advanced and grown, we have had to tap into larger sources to meet the demand for cheap and easily-accessible energy. Our technological sophistication and understanding of basic physics and chemistry has had to grow with our energy hunger to take advantage of different forms of energy; windmills, steam engines, oil refineries, cold water reactors and photovoltaic panels, and so on. In the long run, it is a mathematical certainty that to sustain our civilisation at present levels, or to grow and increase energy consumption we must transition to renewable energy both because quantities of fossil fuels and star fuels like uranium and plutonium on Earth are finite.