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Building a Space Station – Potential Paths

December 16, 2025 by Stilgar

Continuing my rabbit hole which started with traveling to Mars, I pivoted to building space stations for 100, 1000, 100K, 1 Million, and 10 Million people. My rationale was that a large space-based population would be independent of earth and drive growth of space-related activities and expansion. Essentially, a large population outside of earth would be a catalyst of chatGPT like investments and potential, rather than just be an outpost of human endeavours driven by a few people on earth.

One of the key pre-requisites from my perspective was that the quality of life should be equal to that of earth, which means – living on the surface of the moon or mars is off-the-table as they have different gravity. This essentially leaves you with creating space habitats that can mimic 1 g earth gravity. Apparently, if you have large space station that rotates once per minute (or even less), you won’t notice the dizzying (or Coriolis effect).

The 1 g earth gravity requirement, 1 RPM, and having radiation dose same as earth (~2.4 – 3 mSv annual) requirement leads to a significant requirement on the size of the space ship. A 0.5 RPM has an even more requirement on the space ship tonnage.

This large tonnage requirement is driven by the necessity to shield people from radiation. There were essentially the following options to provide shielding in space

  1. Lunar Regolith
  2. Wet Lunar Crete (Lunar Regolith + Water Ice + Binder + Neutron Absorber)
  3. Hybrid Shielding: Wet Lunar Crete + Magnetic Shielding

For my research, I moved forward with Hybrid Active/Passive Shielding, and this had an estimate mass of 31.7 million tons giving a dose of ~3 – 3.5 mSv per year.

Summary of My Conversation


Shielding Use-Case Comparison for 1,000-Person Habitat

Shielding ScenarioRequired Areal DensityTotal Habitat Mass (Estimate)Annual Dose (vs. Earth Avg. 3.0 mSv/year)Key Trade-Offs
1. Hybrid Active/Passive5 t / square meter Wetcrete + 2.0 T Magnet31.7 Million Tonsapprox 3.0-3.5 mSv/year(Earth-Equivalent)Pros: Lowest mass, best safety. Cons: Doubles operational power (approx 1.0 MW for cooling), requires highly complex cryogenic system, high risk from single point of failure (magnet quench).
2. Enhanced Passive10 t/m^2 Lunar Wetcrete (Pure Passive)54.0 Million Tonsapprox 3.2-3.6 mSv/year (Slightly Above Earth)Pros: Simple, reliable operation (no active magnet). Cons: Highest mass (requires doubling lunar mining output), fails to guarantee true Earth-equivalent safety, extreme structural load on the hull.
3. Baseline Passive10 t/m^2 Pure Lunar Regolith (No Hydrogen)54.0 Million Tonsapprox 5.0 mSv/year (High Exposure)Pros: Simple technology, no power needed for shielding. Cons: Highest mass, Fails to meet safety goal due to overwhelming secondary neutron production. Requires settlers to accept career-limiting doses.

Conclusion on Trade-Offs

The three scenarios represent a choice between three engineering drivers: Mass, Safety, and Complexity/Power.

1. The Mass Trade-Off (Scenario 1 vs. 2)

  • Hybrid Shielding (31.7 Mt) chooses mass efficiency by accepting the long-term operational cost of the magnetic system. It requires 22.3 million fewer tons of material than the pure passive method.
  • Enhanced Passive Shielding 54.0 Mt chooses operational simplicity (no complex power plant for the magnet) by accepting a massive upfront construction cost and a major increase in lunar resource mobilization.

2. The Safety Trade-Off (Scenario 3 vs. 4)

  • The comparison between Pure Regolith approx 5.0 mSv/year) and Lunar Wetcrete (approx 3.5 mSv/year at $10 t/m^2) shows that simply adding mass is not enough. The key to effective passive shielding is the inclusion of light elements (water/hydrogen) to moderate (slow down) secondary neutrons. Without it, the dose actually gets worse as the shield gets thicker.

3. The Optimal Balance (Scenario 1)

The Hybrid Active/Passive (Wetcrete + Magnet) system is the only one that efficiently achieves the goal of near-Earth radiation safety (approx 3.0 mSv/year) while keeping the total mass within a manageable, albeit astronomical, range. It fundamentally solves the GCR problem by using deflection (physics) rather than brute force (mass).

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