CoSE Logo
CoSE AstroBotany
Lunar BLSS Bio-Infrastructure
✦ npj Microgravity Review Draft · CoSE DeepSpaceAg Series

From Dust to Bio-Infrastructure: A Mechanistic Review of Sintered Regolith Ceramics for Lunar Biogenerative Life Support Systems

First Author1,*, Second Author1,2, Collaborator Three3, and Lead Author1,4,†

1Advanced Life Support and Space Bio-Engineering Group · 2Dept. of Materials Science · 3Division of Plant Biology and Microgravity Omics · 4Center for Space Evolution (CoSE)

📌 Executive Abstract

Establishing a permanent human presence on the Moon requires closing habitat life-support loops through Biogenerative Life Support Systems (BLSS). Terrestrial resupply imposes prohibitive launch costs, while direct agricultural cultivation in unrefined lunar regolith is severely constrained by submicroscopic nanophase metallic iron ($\mathrm{npFe}^0$), abiotic generation of reactive oxygen species (ROS) via modified Fenton cascades, broken silicate dangling bonds, and sharp mineral shards that induce physical shearing and plant root apical growth arrest. Furthermore, fractional lunar gravity ($1/6\,g$) alters the Bond number, resulting in capillary entrapment, erratic nutrient transport, and pervasive root hypoxia in polydisperse regolith beds. Here, we review an alternative in-situ bio-infrastructure paradigm: transforming unrefined regolith into engineered porous ceramics via thermal sintering. High-temperature processing ($>1050^\circ\mathrm{C}$) passivates reactive geochemical interfaces by solid-solubilizing $\mathrm{npFe}^0$ into stable augite and olivine matrices, rounds grain boundaries, and enables precise control over pore throat diameters ($30\text{--}60\,\mu\mathrm{m}$). This pore architecture stabilizes matric potential ($-2.5$ to $-5.0\,\mathrm{kPa}$), ensuring continuous capillary nutrient wicking while maintaining air-filled porosity above $25\text{--}30\%$. Equivalent System Mass (ESM) lifecycle modeling reveals that the initial launch-mass investment of a sintering plant reaches parity with direct regolith cultivation within $18\text{--}22$ months, driven by $>98.5\%$ water recovery efficiency and the elimination of chemical buffers. When integrated with fungal mycoponics, microbial bioweathering, and cyclic $500^\circ\mathrm{C}$ pyrolytic substrate regeneration, sintered regolith ceramics provide a closed-loop substrate foundation for sustainable extraterrestrial habitation.

Keywords: Lunar regolith, Biogenerative Life Support Systems (BLSS), In-Situ Resource Utilization (ISRU), Porous ceramics, Microwave sintering, Nanophase iron, Microgravity hydrodynamics, Equivalent System Mass (ESM).

1. Introduction: The In-Situ Resource Utilization Imperative

Establishing an enduring human presence on the lunar surface requires transitioning from open-loop, resupply-dependent life support configurations to self-sustaining Biogenerative Life Support Systems (BLSS). Terrestrial resupply logistics impose an unsustainable launch mass burden for multi-year surface stays, where human metabolic requirements for water, oxygen, and nutrition scale linearly with crew size and mission duration. Bioregenerative architectures resolve this resupply vulnerability by harnessing photoautotrophic organisms to scrub atmospheric carbon dioxide, produce metabolic oxygen, purify wastewater via canopy transpiration, and supply fresh caloric and micronutrient biomass.

Historically, space mission architectures evaluated two distinct edaphic paradigms for extraterrestrial crop production: deploying synthetic hydroponic hardware transported from Earth, or cultivating crops directly in untreated, in-situ planetary regolith. Transporting inert hydroponic media (such as mineral rockwool, polyurethane foams, or expanded clay) and prefabricated polymeric fluid channels from Earth imposes launch mass penalties that severely limit the initial deployable agricultural canopy. Conversely, the direct edaphic use of raw lunar regolith relies on the assumption that lunar dust can serve as a functional analogue to terrestrial soil if augmented with liquid nutrients. However, pioneering botanical experiments utilizing returned Apollo specimens and high-fidelity planetary simulants demonstrate that raw lunar regolith imposes severe physiological penalties. Planetary-scale exposure to solar wind irradiation, cosmic rays, and hypervelocity micrometeorite comminution has generated a geochemically hostile matrix defined by reactive submicroscopic metallic iron, unweathered razor-sharp mineral shards, and volatile abiotic surface chemistry.

To circumvent both the launch-mass penalty of imported hardware and the biological toxicity of raw regolith, life support engineering is shifting toward an in-situ bio-infrastructure paradigm. Rather than attempting to adapt crop physiology to an inherently hostile mineral substrate, In-Situ Resource Utilization (ISRU) thermal consolidation processes can transform unrefined regolith into engineered porous ceramics. Controlled high-temperature sintering passivates reactive geochemical interfaces, rounds abrasive grain morphology, and enables the precision fabrication of hydroponic troughs, multiphase fluid-delivery wicks, and mycoponic scaffolds.

2. Physicochemical & Toxicological Interfaces of Pristine Lunar Regolith

The Moon's hyper-vacuum environment and lack of a dipolar magnetosphere expose surface minerals to unattenuated space weathering. Energetic solar wind protons reduce ferrous iron silicates, while ubiquitous micrometeorite impacts induce localized shock melting and vapor-phase condensation. These energetic phenomena generate nanophase metallic iron ($\mathrm{npFe}^0$), consisting of submicroscopic zero-valent iron droplets ($1\text{--}100\,\mathrm{nm}$ in diameter) embedded within the rims of mineral grains and dispersed through the amorphous silicate matrix of agglutinitic glasses.

When pristine lunar regolith or experimentally reduced simulants contact oxygenated aqueous solutions inside a habitat atmosphere, these surface-accessible metallic blebs trigger destructive abiotic oxidation cascades. Solvated divalent iron ions ($\mathrm{Fe}^{2+}$) dissolve from mineral boundaries, initiating modified Fenton-like catalytic cycles:

$$\mathrm{Fe}^0 + \mathrm{O}_2 + 2\mathrm{H}^+ \longrightarrow \mathrm{Fe}^{2+} + \mathrm{H}_2\mathrm{O}_2$$ $$\mathrm{Fe}^{2+} + \mathrm{H}_2\mathrm{O}_2 \longrightarrow \mathrm{Fe}^{3+} + \cdot\mathrm{OH} + \mathrm{OH}^-$$ $$\mathrm{Fe}^{2+} + \mathrm{O}_2 \longleftrightarrow \mathrm{Fe}^{3+} + \mathrm{O}_2^{\cdot-}$$

Electron paramagnetic resonance (EPR) spectroscopy alongside terephthalate hydroxylation assays confirms that reduced lunar dusts generate hydroxyl radical concentrations 5-fold to 100-fold greater than terrestrial basaltic analogs. Furthermore, mechanical crushing leaves abundant surface dangling bonds such as broken silicate radicals ($\equiv\!\mathrm{Si}\cdot$ and $\equiv\!\mathrm{Si}-\mathrm{O}\cdot$). When hydrated, these radicals homolytically split water molecules, generating sustained bursts of oxidizing species that trigger rapid lipid peroxidation in plant root cell membranes.

Figure 1: Toxicity and Passivation Mechanisms
Figure 1 | Physicochemical and toxicological interfaces of pristine versus sintered lunar regolith. Comparison of raw regolith hazards (nanophase metallic iron blebs, dangling silicate bonds, razor-sharp abrasive edges triggering Fenton-mediated oxidative stress cascades) versus high-temperature sintered ceramic bio-infrastructure (passivated crystal matrices, rounded grain boundaries, and homeostatic plant root ontogeny).
Parameter / Property Raw Lunar Regolith (Direct Cultivation) Sintered Regolith Ceramic (Engineered Substrate)
Nanophase Metallic Iron ($\mathrm{npFe}^0$) Surface-accessible blebs across grain rims ($1\text{--}100\,\mathrm{nm}$) Oxidized and incorporated into stable crystalline silicates
Aqueous ROS Generation Potential High; sustained $\cdot\mathrm{OH}$ and $\mathrm{O}_2^{\cdot-}$ generation via Fenton pathways Negligible; passivated, hydrothermally inert interface
Grain / Pore Morphometry Highly angular, sharp, micro-shearing shards Rounded, smooth, consolidated neck boundaries
Plant Transcriptomic Profile Chronic upregulation of GSTs, peroxidases, JA, and ABA stress pathways Homeostatic baseline; standard vegetative allocation
Chromosomal & Telomeric Integrity Elevated 8-oxoG lesions, accelerated telomere shortening Protected genome; absence of mineral-derived radical stress
Aqueous Solution Chemistry Uncontrolled dissolution; alkaline spikes ($\mathrm{pH}\;9.0\text{--}11.0$), P-fixation Stable $\mathrm{pH}$ control ($\mathrm{pH}\;5.8\text{--}6.2$); predictable stoichiometry

3. Materials Science & In-Situ Manufacturing Modalities

Thermal sintering between $1050^\circ\mathrm{C}$ and $1250^\circ\mathrm{C}$ transforms loose, biologically hazardous regolith into inert, structurally coherent ceramic substrates. Viscous flow of agglutinitic impact glasses and pyroxenes wets refractory minerals such as anorthite plagioclase, creating consolidated neck boundaries. Metallic $\mathrm{npFe}^0$ oxidizes and solid-solubilizes into thermodynamically stable clinopyroxenes (augite, $(\mathrm{Ca, Mg, Fe})\mathrm{SiO}_3$) and olivines ($(\mathrm{Mg, Fe})_2\mathrm{SiO}_4$), eliminating electron transfer in aqueous solution. Concurrently, atomic mass transfer rounds sharp edges, quenching reactive dangling bonds.

Microwave sintering at $2.45\,\mathrm{GHz}$ and $5.8\,\mathrm{GHz}$ provides volumetric dielectric heating. The absorbed power per unit volume ($P_v$) is described by:

$$P_v = 2\pi f \varepsilon_0 \varepsilon'' |E|^2$$

where $f$ is frequency, $\varepsilon_0$ is free space permittivity, $\varepsilon''$ is relative dielectric loss factor, and $E$ is electric field strength. The high dielectric loss tangent ($\tan\delta = \varepsilon''/\varepsilon'$) driven by $\mathrm{npFe}^0$ and ilmenite allows pristine regolith to heat rapidly from within. To prevent thermal-shock microcracking, cooling rates must be maintained strictly below $15^\circ\mathrm{C/min}$.

Figure 2: Manufacturing Modalities Radar
Figure 2 | Multi-attribute technology evaluation radar chart. Comparison of Microwave Sintering ($2.45/5.8\,\mathrm{GHz}$), Concentrated Solar Sintering (ALM), and Selective Laser Melting (SLM) across energy efficiency, mass throughput, geometric precision, thermal stress safety, and volumetric heating capability.
Modality Heating Mechanism Operating Temp. Specific Energy Resolution Primary Application
Microwave Sintering Volumetric dielectric coupling $1050^\circ\mathrm{C}\text{--}1200^\circ\mathrm{C}$ $\sim 1.2\,\mathrm{kWh/kg}$ $1\text{--}5\,\mathrm{mm}$ Volumetric growth substrates, filter blocks, pavers
Concentrated Solar (ALM) Focused solar irradiance ($1361\,\mathrm{W/m}^2$) $1100^\circ\mathrm{C}\text{--}>1400^\circ\mathrm{C}$ $0\,\mathrm{kWh}$ Electrical $2\text{--}10\,\mathrm{mm}$ Large hydroponic troughs, drainage gutters, bulk shielding
Selective Laser Melting (SLM) Focused optical laser diode ($\lambda=1064\,\mathrm{nm}$) $1200^\circ\mathrm{C}\text{--}1500^\circ\mathrm{C}$ $\sim 3.5\,\mathrm{kWh/kg}$ $50\text{--}200\,\mu\mathrm{m}$ Precision aeration nozzles, wicking pins, fluid manifolds

4. Multiphase Fluid Dynamics & Aeration in Lunar Gravity

On the lunar surface, gravitational acceleration drops to $g_L \approx 1.62\,\mathrm{m/s}^2$ ($1/6\,g$). This fundamentally lowers the dimensionless Bond number ($\mathrm{Bo}$):

$$\mathrm{Bo} = \frac{\Delta\rho \cdot g \cdot d^2}{\gamma}, \quad L_c = \sqrt{\frac{\gamma}{\rho g}}$$

where $\Delta\rho$ is density difference, $d$ is pore diameter, $\gamma$ is interfacial surface tension, and $L_c$ is capillary length. In classical bulk theory, water capillary length expands from $2.71\,\mathrm{mm}$ on Earth to $\sim 6.5\,\mathrm{mm}$ on the Moon. However, pioneering suborbital centrifuge flight data aboard Blue Origin New Shepard 29 (NS-29) by Hasenstein, Kiss, & McKay (Microgravity Science & Technology, 2026) reveals that boundary interactions in fractional gravity diverge significantly from continuum theory:

$$\frac{d^2z}{dx^2} = \frac{\rho g}{\gamma}(z - z_0) \left[ 1 + \left(\frac{dz}{dx}\right)^2 \right]^{3/2}$$
🚀 Empirical Lunar-Gravity Flight Discovery (Hasenstein et al., 2026):
  • Capillary Length Suppression: Under simulated lunar gravity ($1.76\,\mathrm{m/s}^2$), empirical water capillary length was $L_c = 4.2 \pm 0.1\,\mathrm{mm}$ ($\gamma_\mathrm{eff} \approx 30.6\,\mathrm{mN/m}$) — a $\sim 35\%$ suppression compared to theoretical bulk values ($6.5\,\mathrm{mm}$).
  • Wall Roughness & Film Thickening: Microscale surface textures override bulk fluid mechanics, producing significantly thicker boundary liquid films and rounded meniscus curvatures.
  • Glycerol as a Lunar Wetting Enhancer: A $30\%$ glycerol solution raised effective capillary length to $L_c = 5.2 \pm 0.9\,\mathrm{mm}$ ($\gamma_\mathrm{eff} \approx 50.1\,\mathrm{mN/m}$), demonstrating that biocompatible polyol adjuvants overcome boundary pinning on textured substrates.

In unsorted raw regolith, capillary suction traps water in fine micropores ($<10\,\mu\mathrm{m}$), establishing an expansive saturated zone that suffocates aerobic root respiration. Furthermore, surface dust is intrinsically hydrophobic (confirmed on Chang'e-5 samples; Zhang et al., 2025), and coarse grains ($0.5\text{--}2.0\,\mathrm{mm}$) required for root aeration exist only at multi-meter depths (Zhao et al., 2023). Sintering classified fines ($45\text{--}75\,\mu\mathrm{m}$) bypasses deep excavation by creating monodisperse pore throat diameters ($30\text{--}60\,\mu\mathrm{m}$). Governed by the van Genuchten equation:

$$\Theta(h) = \left[ 1 + (\alpha |h|)^n \right]^{-m}$$

this pore window stabilizes matric potential between $-2.5$ and $-5.0\,\mathrm{kPa}$, supporting continuous capillary wicking against fractional gravity while maintaining air-filled porosity above $25\text{--}30\%$ at field capacity.

Figure 3: Hydrodynamics and Aeration in 1/6 g
Figure 3 | Multiphase fluid dynamics and root zone aeration in fractional lunar gravity ($1/6\,g$). Interdependence of pore throat diameter ($\mu\mathrm{m}$), air-filled porosity (\%, green bars), and matric suction head ($-\mathrm{kPa}$, blue curve). The target $30\text{--}60\,\mu\mathrm{m}$ window balances wicking against root hypoxia, fully accommodating empirical boundary film thickening observed in suborbital flight data (Hasenstein et al., 2026).

5. Equivalent System Mass (ESM) & Lifecycle Economics

NASA's Equivalent System Mass ($\mathrm{ESM}$) converts hardware mass ($M$), pressurized volume ($V$), power ($P$), cooling ($C$), and crew labor ($T$) into a standardized mass metric:

$$\mathrm{ESM} = M + (V \cdot C_V) + (P \cdot C_P) + (C \cdot C_C) + (T \cdot C_T)$$

Direct regolith cultivation has a low initial launch mass ($\sim 420\,\mathrm{kg}$) but suffers severe recurring penalties from capillary water entrapment ($<80\%$ recovery efficiency), alkaline dissolution requiring $145\,\mathrm{kg/year}$ of acid buffers, and high crew dust mitigation labor. Sintered bio-infrastructure requires an automated manufacturing plant ($\sim 1850\,\mathrm{kg}$) but achieves $>98.5\%$ water recovery, stable $\mathrm{pH}$ ($5.8\text{--}6.2$), and negligible dust risks. Systems-level modeling confirms an operational breakeven horizon between $18$ and $22$ months (and $9\text{--}15$ months with surface nuclear power).

Figure 4: Cumulative ESM Trajectory
Figure 4 | Cumulative ESM lifecycle trajectory over 60 months. Comparison of direct regolith cultivation versus sintered ceramics for a nominal 6-person outpost.
Figure 5: Mission Economics Scaling
Figure 5 | Mission economics and crew scaling. Lifecycle mass comparison across 3-crew and 12-crew exploration contingents at 60 months.
Figure 9: ISRU Manufacturing and ESM Breakeven Gantt Chart
Figure 9 | Autonomous ISRU habitat outfitting, manufacturing phase-in, and ESM breakeven Gantt timeline. Chronological outfitting from cargo landing (Months 0--6) to serial sintering manufacturing (Months 3--15), canopy scaling, and the critical mass breakeven horizon at Month 18.5, yielding compounding savings (>8,000 kg net mass saved by Month 60).
3D Architecture

Figure 10 | 3D Photorealistic Progression: Shackleton Crater Rim Outpost

Moon Base 3D Render
Full Phased Architecture: Composite 4-Panel Evolution at Lunar South Pole
Figure 10 | Photorealistic 3D architectural progression of autonomous ISRU habitat manufacturing and BLSS bio-infrastructure phasing on the Shackleton Crater rim. Rendered with Blender 5.2 Cycles PBR physics under realistic low-angle polar sunlight ($5.5^\circ$) with Earth in the sky. Visualizes the progression from initial CLPS lander logistics and regolith sorting (Phase I), continuous microwave sintering plant (Phase II), pressurized Artemis habitat and glowing multi-tier LED geodesic greenhouse dome (Phase III, ESM breakeven at Month 18.5), to the mature closed-loop outpost with dual domes, pyrolytic regenerators, and bioweathering chemostats (Phase IV).

6. Closed-Loop Multitrophic Ecosystems

Crops such as dwarf wheat, potato, and soybean produce $40\text{--}60\%$ inedible lignocellulosic residue. Integrating saprotrophic fungi (\textit{Pleurotus ostreatus}, \textit{Ganoderma lucidum}) on perforated ceramic plates upcycles this residue into edible protein and $\mathrm{CO}_2$. Essential fertilizer minerals ($\mathrm{K}^+, \mathrm{Ca}^{2+}, \mathrm{Mg}^{2+}$) are replenished via microbial bioleaching in sealed external bioreactors using \textit{Sphingomonas desiccabilis} (demonstrated by ESA BioRock). Substrate biofouling is resolved through cyclic $500^\circ\mathrm{C}$ pyrolytic bake-outs:

$$\mathrm{C}_x\mathrm{H}_y\mathrm{O}_z (\text{biomass}) + \left(x + \frac{y}{4} - \frac{z}{2}\right)\mathrm{O}_2 \xrightarrow{500^\circ\mathrm{C}} x\,\mathrm{CO}_2 + \frac{y}{2}\,\mathrm{H}_2\mathrm{O} + \text{Mineral Ash}$$

The ceramic matrix emerges sterile and decarbonized for infinite re-use without structural degradation.

Figure 8: Closed-Loop Multitrophic Operational Lifecycle Gantt Chart
Figure 8 | Closed-loop multitrophic operational sequencing and substrate lifecycle schedule. A 120-day repeatable outpost schedule illustrating temporal coordination between dwarf wheat cultivation (70 days), rapid ceramic pyrolytic regeneration at 500°C (Days 71--75), staggered salad greens, saprotrophic mushroom (Pleurotus ostreatus) bioconversion (Days 71--98), and decoupled microbial bioweathering.

7. Technology Readiness Level (TRL) Maturation Roadmap

A structured three-phase development roadmap advances sintered regolith bio-infrastructure from laboratory proof-of-concept to operational lunar surface deployment:

  • Phase 1: Laboratory Formulations (2024--2026, TRL 1 $\to$ 3): Simulant dielectric characterization, multiphysics modeling, and plant transcriptomic stress elimination.
  • Phase 2: Subscale Flight Testing (2027--2030, TRL 4 $\to$ 6): Autonomous sintering payloads on CLPS landers, ISS capillary wicking validation, and microgravity bioleaching.
  • Phase 3: Operational Deployment (>2031, TRL 7 $\to$ 9): Deployment of full-scale ISRU manufacturing plants constructing vertical hydroponic arrays integrated with habitat ECLSS.
Figure 6: TRL Maturation Horizon
Figure 6 | Strategic Technology Readiness Level (TRL 1--9) maturation horizon. Progression timeline from laboratory simulant characterization to fully integrated operational lunar base bio-infrastructure.
Figure 7: Strategic TRL Maturation Gantt Chart
Figure 7 | Strategic technology maturation and multi-track development Gantt schedule (2024--2035). Parallel maturation trajectories across Track A (Sintering Physics & ISRU), Track B (Fluid Dynamics & Substrates), Track C (Agronomy & Multitrophic Loops), and Track D (Bioweathering & Substrate Lifecycle) identifying critical flight milestones.

8. Conclusions & Declarations

Transforming unrefined lunar regolith into engineered sintered ceramics provides an in-situ manufacturing pathway that resolves the fundamental toxicological, mechanical, and fluid-dynamic barriers of direct regolith agriculture. By passivating reactive metallic iron, rounding sharp grain edges, and stabilizing pore throats to $30\text{--}60\,\mu\mathrm{m}$, sintered bio-infrastructure ensures aerobic root respiration and $>98.5\%$ water recovery under $1/6\,g$. Coupled with fungal mycoponics, microbial bioweathering, and cyclic pyrolytic regeneration, sintered ceramics establish a durable, closed-loop foundation for sustained biological life support on the Moon.

Declarations

Acknowledgements: Supported by the In-Situ Resource Utilization (ISRU) and Space Life Support engineering research initiatives.

Author Contributions: F.A., S.A., C.T., and L.A. contributed to literature synthesis, modeling, manuscript writing, and review.

Competing Interests: The authors declare no competing interests.

Data & Code Availability: Complete LaTeX sources, ESM Python models, and simulation outputs are openly available in the GitHub repository at github.com/dr-richard-barker/lunar-regolith-blss-review and archived under DOI: 10.5281/zenodo.placeholder.

References

  1. Wheeler, R. M. Agriculture for space: people and places paving the way. Open Agric. 2, 14--32 (2017).
  2. Paul, A.-L., Elardo, S. M. & Ferl, R. Plants grown in Apollo lunar regolith present stress-associated transcriptomes that inform prospects for lunar exploration. Commun. Biol. 5, 382 (2022).
  3. Ming, D. W. & Henninger, D. L. Lunar Base Agriculture: Soils for Plant Growth (American Society of Agronomy, 1989).
  4. Hanford, A. J. Advanced Life Support Baseline Values and Assumptions Document. NASA/CR-2004-208941 (NASA JSC, 2004).
  5. Wheeler, R. M. Space farming contributions to agriculture on Earth and in space. NASA/TM-20230018203 (2023).
  6. Wamelink, G. W. W. et al. Crop growth and viability of seeds on Mars and Moon soil simulants. Open Agric. 4, 509--516 (2019).
  7. Atkin, J., Oliveira Santos, S. et al. Bioremediation of lunar regolith simulant through mycorrhizal fungi and plant symbioses enables chickpea to seed. Sci. Rep. 14, 8421 (2024).
  8. Hendrix, D. A., Legett, C. IV & Hurowitz, J. A. The reactivity of experimentally reduced lunar regolith simulants. Meteorit. Planet. Sci. 59, 2341--2358 (2024).
  9. Turci, F. et al. Mechanistic insight into the oxidative potential of lunar dust analogues. Astrobiology 15, 735--745 (2015).
  10. Taylor, L. A. & Meek, T. T. Microwave processing of lunar soil: properties, theory, and practice. J. Aerosp. Eng. 18, 188--196 (2005).
  11. Fateri, M. et al. Solar sintering for lunar additive manufacturing. J. Aerosp. Eng. 32, 04019084 (2019).
  12. Xi, Y., Zhang, Y. et al. Multiphysics computational model of microwave sintering of lunar regolith simulant. Coatings 16, 222 (2026).
  13. Goulas, A. & Binner, J. G. P. Process parameters development of selective laser melting of lunar regolith. Addit. Manuf. 18, 88--95 (2017).
  14. Heinse, R., Jones, S. B., Or, D. et al. Porous media water retention in microgravity: The ISS ORZS experiment. Vadose Zone J. 6, 713--722 (2007).
  15. Barbero Barcenilla, B. & Shippen, D. E. Back to the future: The intimate connection between telomere factors and stress. J. Biol. Chem. 294, 14803 (2019).
  16. Bilardo, V. J. et al. Equivalent system mass (ESM) metric modeling for surface planetary habitats. AIAA SciTech 2024-1142 (2024).
  17. Cockell, C. S. et al. Microbially-enhanced element recovery from basalt on the International Space Station. Nat. Commun. 11, 5523 (2020).

(Complete 59-entry bibliography available in `manuscript/references.bib` and in compiled PDF)