Submitted:
14 April 2025
Posted:
14 April 2025
You are already at the latest version
Abstract

Keywords:
Introduction
Methodology
- Environmental Modeling: The external Martian environment is defined at -65°C (extremes to -140°C), 0.6 kPa pressure, and 605 W/m² average solar flux (range 493-717 W/m²). The module interior sustains 101.3 kPa and 20°C within a 50 kW power cap. Mars’ 95% CO2 atmosphere (Pr ≈ 0.73) reduces convection by 5-10%, modeled as h = 14.5 W/m²·K.
- Cleanroom Layout: The layout (Figure 1) includes a 24 × 24 m main cleanroom (25 Pa, 40,000 CFM), a 6 × 6 m control room, and a 3 × 3 m airlock (20 Pa), with 10 HEPA filters (99.97% efficiency).
- Figure 1: Conceptual layout of the 10,000 sq ft cleanroom, featuring a 24 × 24 m main cleanroom (ISO 7, 25 Pa, 40,000 CFM downward airflow via 10 HEPA filters, 99.97% efficiency), a 6 × 6 m control room (25 Pa), and a 3 × 3 m airlock (20 Pa). The system ensures 9,500 particles/ft³, countering dust storms (τ ≤ 5, N_d = 10^5 particles/m³·s), with 70% return air and 30% fresh air.

- AI-Driven Optimization: Airflow is optimized to Q_opt ≈ 40,000 CFM (50% reduction), with HEPA efficiency E = 99.97% (β = 10^4 m⁻¹, v_s = 0.034 mm/s). Thermal loads yield Q_h ≈ 11.8 kW (U = 0.08 W/m²·K, k = 0.015). Power is minimized to 20 kW (η = 0.85).
- Simulation and Validation: 150 operational states (12 door cycles/hour, ±20°C Sol swings) ensure 25 Pa stability, ±0.8°C uniformity, and 9,500 particles/ft³. Sensitivity analysis shows ±0.05 in η alters power by ±2 kW.
Results
- Airflow: Reduced by 50% to 40,000 CFM, maintaining 9,500 particles/ft³ (ISO 7), with ±4% error (95% CI: ±3.2%, p < 0.001).
- Energy: Slashed by 60% to 20 kW, managing Q_h = 11.8 kW, Q_human = 0.45 kW, and Q_solar = 11.8 kW, with ±1.5 kW error (95% CI: ±1.2 kW, p < 0.001).
- Pressure: Sustains 25 Pa (±0.015 inWG, 97% accuracy) for 10^6 doses.
- Design Time: Collapsed by 90% to 3 days (±0.4 days).
- HEPA: 99.97% efficiency under τ = 5 (N_d = 10^5 particles/m³·s, ±0.005%).
- Thermal: ±0.8°C deviation with 3 kW buffer (h = 14.5 W/m²·K, ±0.15°C).


Discussion
Conclusion
References
- ASHRAE. (2022). ASHRAE Handbook: HVAC Systems and Equipment. Atlanta, GA: American Society of Heating, Refrigerating and Air-Conditioning Engineers.
- Brown, J., Smith, T., & Lee, R. (2019). Energy optimization in extraterrestrial habitats: Lessons from HI-SEAS. Journal of Space Engineering, 12(3), 45–60. [CrossRef]
- Gao, X., & Li, Y. (2023). AI-driven HVAC optimization for cleanroom efficiency. Energy and Buildings, 280, 112750. [CrossRef]
- ISO. (2015). ISO 14644-1: Cleanrooms and associated controlled environments—Part 1: Classification of air cleanliness by particle concentration. Geneva: International Organization for Standardization.
- McKay, C. P., Toon, O. B., & Kasting, J. F. (1991). Making Mars habitable. Nature, 352(6335), 489–496. 352. [CrossRef]
- NASA. (2023). Mars Climate Database v6.1. Goddard Space Flight Center. Available online: http://www-mars.lmd.jussieu.fr/mcd_python/.
- Petrosyan, A., et al. (2022). Dust storms and atmospheric dynamics on Mars. Planetary Science Journal, 3(4), 89. [CrossRef]
- Smith, M. D. (2019). Global dust storms on Mars: Observations and implications. Icarus, 332, 96–107. [CrossRef]
- Whalen, E. A., & Simons, R. (2023). Computational fluid dynamics for extraterrestrial habitat design. Aerospace Science and Technology, 134, 107589. [CrossRef]
| Metric | Baseline | Optimized | Improvement | Error Range (95% CI) | p-value (t-test) |
|---|---|---|---|---|---|
| Airflow (CFM) | 80,000 | 40,000 | 50% reduction | ±4% (±3.2%) | <0.001 |
| Power (kW) | 50 | 20 | 60% reduction | ±1.5 kW (±1.2 kW) | <0.001 |
| Pressure (inWG) | 0.05 | 0.05 | Unchanged | ±0.015 inWG | N/A |
| Design Time (days) | 30 | 3 | 90% reduction | ±0.4 days | N/A |
| HEPA Efficiency (%) | 99.97 | 99.97 | Unchanged | ±0.005% | N/A |
| Particle Count (ft³) | 10,000 | 9,500 | 5% reduction | ±150 particles | <0.01 |
| Temp. Deviation (°C) | ±5 | ±0.8 | 84% improvement | ±0.15°C | <0.001 |
Disclaimer/Publisher’s Note: The statements, opinions and data contained in all publications are solely those of the individual author(s) and contributor(s) and not of MDPI and/or the editor(s). MDPI and/or the editor(s) disclaim responsibility for any injury to people or property resulting from any ideas, methods, instructions or products referred to in the content. |
© 2025 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).