While the energy output of a miniaturized nuclear fission device is location-agnostic, the productivity of solar-powered solutions rely on solar intensity, surface temperature, and other factors that would determine where a non-nuclear outpost would be optimally located. This required modeling and accounting for a number of factors, such as how gasses and particles in the atmosphere might absorb and scatter light, which would affect the amount of solar radiation at the planet’s surface.
The winner: a photovoltaic array that uses compressed hydrogen for energy storage. At the equator, what the team calls the “carry-along mass” of such a system is about 8.3 tons versus about 9.5 tons for nuclear power. The solar-based system becomes less tenable closer to the equator at more than 22 tons, but beats out fission energy across about 50% of the Martian surface.
“I think it’s nice that the result was split pretty close down the middle,” Berliner said. “Nearer the equator, solar wins out; nearer the poles, nuclear wins.”
Such a system can employ electricity to split water molecules to produce hydrogen, which can be stored in pressurized vessels and then re-electrified in fuel cells for power. Other applications for hydrogen include combining it with nitrogen to produce ammonia for fertilizers – a common industrial-scale process.
Other technologies, like water electrolysis to produce hydrogen and hydrogen fuel cells, are less common on Earth, largely due to costs, but potentially game-changing for human occupation of Mars.
“Compressed hydrogen energy storage falls into this category as well,” noted co-lead author Anthony Abel, a chemical and biomolecular engineering PhD student at UC Berkeley. “For grid-scale energy storage, it’s not used commonly, although that is projected to change in the next decade.”
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