Silicon Production for Solar Panels

Overview

Silicon (Si) is the foundation of local solar panel production on Mercury.

Parameter Value
Feedstock Quartz sand SiO₂ (20% of Mercury’s crust)
Method Aluminothermic reduction
Si consumption ~70 t per 1 solar panel complex (35,000 m²)
Application Solar panels (18% efficiency)

Aluminothermic Reduction

Problem: The traditional method (SiO₂ + C → Si + CO₂) requires carbon, which Mercury lacks.

Solution: Aluminothermy — reduction using aluminum.

3SiO₂ + 4Al → 3Si + 2Al₂O₃
Advantage Description
Local aluminum From MRE electrolysis slag (see Distillation)
No carbon import Full autonomy
Byproduct Al₂O₃ (corundum) → ceramics, abrasives

Stoichiometry: - Per 1 kg silicon: 1.3 kg aluminum - Byproduct: 2.4 kg corundum (Al₂O₃)


Production Chain

Stage Process Materials Note
1 Quartz sand (SiO₂) Local 20% of Mercury’s crust
2 Aluminum MRE slag Already produced
3 Aluminothermy Local Solar furnace, 2000°C
4 Zone melting Purification to solar grade
5 Czochralski method Quartz crucible Ingot ∅150 mm
6 Wire cutting Diamond wire (Earth) 200 μm wafers
7 P/B diffusion Phosphorus + Boron (Earth) p-n junction
8 Screen printing Local aluminum Contacts
9 SiNx deposition Nitrogen (Earth) + Silane Anti-reflection
10 Module assembly Local aluminum No glass needed (vacuum)

Material Balance

For 35,000 m² of panels (1 complex):

Parameter Value
Import from Earth ~210 kg (consumables)
Local aluminum ~90 tons
Silicon ~70 tons
Corundum (byproduct) ~170 tons → ceramics
Finished panel mass ~120 tons

See Also

  • Production — energy supply and solar panels
  • Distillation — aluminum production for aluminothermy
  • MRE — magnetic separation of elements