A central question surrounding possible human exploration of Mars is whether crewed missions can be supported by available technologies using in situ resources. Here, we show that photovoltaics-based power systems would be adequate and practical to sustain a crewed outpost for an extended period over a large fraction of the planet's surface. Climate data were integrated into a radiative transfer model to predict spectrally-resolved solar flux across the Martian surface. This informed detailed balance calculations for solar cell devices that identified optimal bandgap combinations for maximizing production capacity over a Martian year. We then quantified power systems, manufacturing, and agricultural demands for a six-person mission, which revealed that photovoltaics-based power generation would require <10 t of carry-along mass, outperforming alternatives over ~50% of Mars' surface.
Main TextLong-duration space missions or continuously-occupied extraterrestrial outposts require Earthindependent power and chemical supply. Mars has an abundance of in situ resources, including (sub)surface water ice (1) and carbon and nitrogen in atmospheric CO 2 and N2 (2). Efficient conversion of these resources to reduced forms of hydrogen, nitrogen, and carbon would represent an enabling step towards sustaining a permanent human presence in space. In analogy to the proposed terrestrial "Hydrogen Economy", molecular hydrogen (H2) can be used as a platform molecule for energy storage, on-demand power supply, and as a reactant driving CO2 and N2 (bio)chemical reduction on Mars (3-5).Water electrolysis with selective catalysts can drive water reduction to H2 on cathode surfaces. This technology is attractive for space manufacturing applications since reactions can proceed at high rates at