Extrasolar Planets

Will Solar Panels Work at Proxima Centauri?

Solar panel technology has advanced significantly in recent years, to the point where solar energy is the fastest-growing renewable power source. The solar panels we have today are a by-product of those used in space. If you want to power a satellite or crewed spacecraft, there are only two ways: solar energy or nuclear power. Of the two, only solar energy isn’t limited by the amount of fuel you bring on board. As we contemplate traveling to other star systems, this raises the question: will solar panels work near other stars?

Solar panels generate an electric voltage through what is known as the photoelectric effect. The effect was first discovered in the 1800s when scientists noticed that charged metallic planets could give off electrons when exposed to ultraviolet light. This led to the discovery that light consisted of quantum particles known as photons. Soon afterward there were some examples of using the effect to generate electric power, but the first true solar cells didn’t appear until the mid-1900s.

Since then research has focused on making solar cells lighter, cheaper, and more efficient. Modern solar panels can harness not just ultraviolet light, but also visible and in some cases infrared. But all of these designs are built to harness the Sun, which gives off most of its light in the green range and emits plenty of ultraviolet light. But most exoplanets orbit red dwarf stars, which have a peak brightness in the red or infrared and emit little ultraviolet. If we want to visit nearby planetary systems, such as the Proxima Centauri system, then we’ll need to have solar panels capable of harnessing red dwarf starlight.

That’s the topic of a recent study in Scientific Reports. The authors look at the efficiency of solar panels under a range of stellar spectra, particularly comparing the Sun and Proxima Centauri. Their study focuses on organic photovoltaics (OPVs), which are both light and flexible. This would allow solar panels to be applied to large solar sails, which is a common design element for early interstellar probes.

Theoretical photovoltaic performance limits for the different stellar types. Credit: Schopp, et al

OPVs are a young technology, but they have an advantage over more established silicon-based cells in that they can be tuned to different wavelengths. The efficiency of a solar cell and the wavelengths from which it derives the most energy are based on what is known as the band gap. Essentially, electrons bound to the cell material must capture enough energy from photons to jump across the band gap into the conduction band, where they can then flow as electric current. Using different organic materials, we can adjust the band gap to best suit the light available.

The team found that while a wider band gap works well for sunlight, the light of Proxima Centauri would require a narrow band gap. For example, a simulated wide band gap solar cell has a theoretical efficiency of 18.9% for sunlight, but only 0.9% for Proxima Centauri. In contrast, a narrow band gap model has a theoretical efficiency of 12.6% for Proxima Centauri.

So solar panels could generate electricity from red dwarf stars. But one major disadvantage remains. Since red dwarfs produce much less light than the Sun, even with a good efficiency individual solar cells wouldn’t produce nearly the amount of energy we can gather from the Sun. Interstellar solar panels would need to be significantly larger, which would greatly increase their weight and cost. But it is possible, and further materials research may find even more efficient methods of generating electricity from light.

Reference: Schopp, Nora, et al. “Interstellar photovoltaics.” Scientific Reports 13.1 (2023): 16114.

Brian Koberlein

Brian Koberlein is an astrophysicist and science writer with the National Radio Astronomy Observatory. He writes about astronomy and astrophysics on his blog. You can follow him on YouTube, and on Twitter @BrianKoberlein.

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