Abstract
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 (Formula presented.) 10 t of carry-along mass, outperforming alternatives over ∼50% of Mars’ surface.
| Original language | English |
|---|---|
| Article number | 868519 |
| Journal | Frontiers in Astronomy and Space Sciences |
| Volume | 9 |
| DOIs | |
| Publication status | Published - 27 Apr 2022 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
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SDG 13 Climate Action
Keywords
- climate model
- human exploration mission
- mars
- photovoltaics
- radiative transfer
- technoeconomic analysis
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