CWY004 · Patent Family

Satellite & Deep Space
Materials Platform

Five MOF formula families engineered for extreme space environments — radiation shielding, life support, propulsion catalysis, water harvesting, and thermal management for Mars, Lunar, and orbital missions.

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Space is Hostile

The Extreme Demands
of Space Environments

Spacecraft and satellites operate in some of the most extreme conditions imaginable: temperatures swinging from -270°C in deep space to +250°C in direct sunlight, constant bombardment by cosmic rays and solar radiation, vacuum conditions, microgravity, and atomic oxygen erosion in low Earth orbit. Conventional materials fail. MOFs don't.

500°C
Thermal stability of Zr/Gd MOFs
7000
m²/g max surface area
0.2
g/cm³ minimum MOF density
Z=64
Gd atomic no. — neutron shielding
☢️
Cosmic Radiation
Cosmic rays, solar flares, and high-energy gamma rays damage electronics, degrade materials, and pose lethal risks to astronauts. Traditional lead/aluminium shielding is prohibitively heavy.
🌡️
Extreme Temperatures
Thermal cycling from -270°C to +250°C causes material fatigue and structural failure. Electronics need precise thermal management across this entire range.
💨
Life Support Gas Management
Producing and recycling breathable air in closed spacecraft — O₂ supply, CO₂ removal, humidity control — requires compact, lightweight, and highly selective materials.
🚀
Propulsion Efficiency
Reducing fuel mass is critical to mission economics. Compact H₂ and CH₄ storage, propellant decomposition catalysis, and in-situ fuel generation from Mars atmosphere are all key needs.
CWY004 Patent — Five MOF Formula Families

Materials Engineered for
Space from the Ground Up

Each formula family in CWY004 addresses one or more critical satellite/spacecraft needs. Together they form a complete materials toolkit for the next generation of space missions.

Formula I · Lanthanide MOFs
[MₓLy(H₂O)z]·n(S) · M = Gd³⁺, Hf⁴⁺
Gadolinium & Hafnium
Radiation Shielding
⬡ Gd(III), Hf(IV)

Flagship radiation protection MOFs. Gadolinium (Z=64) has the highest neutron capture cross-section of any element and strongly absorbs gamma rays. Hafnium has a high X-ray and γ-ray attenuation coefficient, superior to conventional Zr. Gd-MOFs thermally stable to 500°C in vacuum; resistant to oxidation. Hf-MOFs show strong thermal resistance under extreme UV radiation and superior mechanical strength in microgravity. 32 linker systems including pyrene, anthracene, and naphthalene tetracarboxylate series.

Neutron + γ-ray shieldingZ=64 (Gd)500°C stable32 ligand variantsMars ISRU catalyst
I
Formula II · Zirconium MOFs
[ZrₓLyOz(OH)w]·n(S) · UiO-66/67/MOF-808
Zr-MOF: Structural Workhorse
of Space Materials
⬡ Zr(IV)

The most thermally, chemically, and mechanically stable MOF family. UiO-66, UiO-67, and MOF-808 withstand -200°C to 500°C, cosmic radiation, vacuum, and atomic oxygen. Strong Zr-O bonds (Young's modulus ~20 GPa) prevent structural failure. MOF-808 provides high H₂ storage; UiO-66/67 for CO₂ removal and O₂ management. Nanocomposite Zr-MOF coatings self-heal from micrometeoroid damage. 16 linker variants including terphenyl, azido, and bromo-functionalised series.

~20 GPa Young's modulus-200°C to 500°CSelf-healing coatingsH₂ storage16 ligand variants
II
Formula III · Zinc MOFs
[ZnₓLy(H₂O)z]·n(S) · MOF-5, ZIF-8 class
Lightweight High-Porosity
Gas Storage & Separation
⬡ Zn(II)

Exceptionally lightweight (density as low as 0.2 g/cm³) with surface areas >4000 m²/g. ZIF-8 provides remarkable CO₂ selectivity for air revitalisation. Thermal stability to 550°C. Photocatalytic activity with TiO₂/graphene composites for solar-driven water splitting and H₂ generation. ZIF composites combined with aerogels and polymers create radiation-resistant coatings for LEO satellite exteriors. Resists atomic oxygen corrosion — a critical failure mode in low Earth orbit. 3 btb/terphenyl linker variants.

0.2 g/cm³ density>4000 m²/g550°C stableAO corrosion resistantH₂ photocatalysis
III
Formula IV · Fe/Cr MOFs
[MₓLyOz(OH)w]·n(S) · M = Fe²⁺/³⁺, Cr³⁺, Ni, Co, Mn
Catalytic & Magnetic
Propulsion MOFs
⬡ Fe(II/III), Cr(III), Ni(II), Co(II), Mn(II)

Fe-MOFs (MIL-101, PCN-250, MIL-88B) possess intrinsic magnetic properties for magnetically controlled spacecraft components. MIL-101(Fe) enables CO₂ to CH₄ conversion for onboard power. MIL-88B(Fe) catalyses hydrazine decomposition for efficient satellite thrusters. Cr-MOFs (MIL-101(Cr), MIL-100(Cr)) have ~4000–4500 m²/g porosity and catalyse CO₂ hydrogenation to CH₄ for Martian ISRU. Porphyrin linkers (C₂₀H₁₄N₄) provide enhanced catalytic and electronic properties. 16 ligand variants for Cr, Ni, Co, Mn; 11 azobenzene variants for Fe.

Magnetic propulsionN₂H₄ decompositionCO₂→CH₄ ISRU~4500 m²/gPorphyrin linker
IV
Formula V · Zeolitic Imidazolate Frameworks (ZIFs) for Space
[M(Im)ₓ]·n(S) · M = Zn²⁺, Co²⁺, Fe²⁺, Cu²⁺
ZIFs: The All-Around Space Performer
⬡ Zn(II), Co(II/III), Fe(II), Cu(II)

ZIFs combine the best properties of zeolites and MOFs in a single material uniquely suited to space. Thermal stability to 550°C; structural integrity under vacuum, microgravity, and mechanical stress during launch (high G-force). High porosity (up to 90% free volume) enables compact H₂ and CH₄ fuel storage. ZIF membranes enable gas separation for ISRU on Mars — CO₂ from the Martian atmosphere can be separated and converted to CH₄ for fuel. ZIF-67 provides O₂ adsorption for life support systems. ZIF-8 efficiently scrubs CO₂ from spacecraft cabins. Hydrophobic nature and chemical stability protect against atomic oxygen erosion in LEO. 11 imidazolate ligand variants including methylimidazolate, trimethyl, and pentamethylbenzimidazolate.

550°C stable90% free volumeMars CO₂ ISRUO₂ life supportAO resistant11 ligand variantsHigh G-force resistant
V
Mission Applications

From Low Earth Orbit
to Mars

Radiation
Spacecraft Shielding

Gd-MOF coatings for neutron and gamma-ray absorption. Hf-MOF for X-ray and solar radiation. Cr-MOF composites for cosmic ray protection. All lighter and more effective than conventional Pb/Al shielding.

Life Support
Air Revitalisation

ZIF-8 and UiO-66 for CO₂ scrubbing from cabin air. Ni-MOF-74 and Co-MOF-74 for O₂ storage and release. Compact, regenerable, and mass-efficient vs. LiOH canister systems.

Propulsion
Fuel Storage & Generation

MOF-808 (Zr) for high-capacity H₂ storage. ZIF membranes for CH₄ storage. MIL-88B(Fe) and MIL-100(Cr) for hydrazine decomposition. NH₂-MIL-125(Ti) for photocatalytic H₂ from water.

ISRU
Mars In-Situ Resource Use

ZIF membranes separate CO₂ from Mars atmosphere (95% CO₂). Gd-MOF and Cr-MOF catalysts convert CO₂ to CH₄ (Sabatier reaction) for propellant. Hf-MOF water splitting for O₂ and H₂.

Thermal
Thermal Management

Zr-MOFs adsorb and desorb water as phase-change materials to regulate heat in electronic components. ZIF-8 thermal insulation coatings manage extreme temperature swings from -200°C to +250°C.

Water
Water Harvesting

Hf-MOFs with hydrophilic properties capture and condense water from trace atmospheric moisture. Critical for long-duration missions. Prevents moisture damage to electronics and provides drinking water for astronauts.

Mission Profiles

Optimised for Every
Mission Type

LOW EARTH ORBIT (LEO)

Primary MOFs: ZIF-8 (AO resistance), Zr-UiO (structural durability), Cr-MIL-101 (gas management). Key threats: atomic oxygen erosion, thermal cycling, micrometeorites. ZIF hydrophobicity and Zr-MOF self-healing coatings are specifically engineered for LEO operating conditions.

GEOSTATIONARY (GEO) / DEEP SPACE

Primary MOFs: Gd-MOF + Hf-MOF (intense radiation environment), Zr-MOF (extreme thermal). Deep space missions face unfiltered cosmic rays and solar particle events — Gd's neutron capture and Hf's X-ray attenuation provide layered shielding unachievable with conventional materials.

LUNAR MISSIONS

Primary MOFs: Zn-MOFs (lightweight, O₂/H₂ storage), Ni/Co-MOFs (energy storage, fuel cells), Hf-MOF (water splitting for LOX/LH₂). The lunar surface lacks a magnetosphere — radiation shielding and in-situ resource utilisation for water and oxygen are mission-critical needs.

MARS MISSIONS

Primary MOFs: Gd-MOF (CO₂→CH₄ ISRU catalyst), ZIF membranes (CO₂ separation from 95% CO₂ Martian atmosphere), UiO-66(Ti/Zr) (H₂ from water for fuel), Ni-MOF-74 (life support O₂). Mars ISRU is the single biggest enabler of cost-effective crewed missions — MOFs are central to it.

Technical Reference

Platform Specifications

MOF Formula Families — CWY004
FamilyMetal(s)Primary Use
Lanthanide (I)Gd(III), Hf(IV)Radiation shielding, ISRU
Zirconium (II)Zr(IV)Structural, thermal, H₂ storage
Zinc (III)Zn(II)Lightweight gas storage, LEO coatings
Fe/Cr/Ni/Co/Mn (IV)Fe, Cr, Ni, Co, MnPropulsion catalysis, energy storage
ZIF (V)Zn, Co, Fe, CuAll-round: gas, ISRU, shielding
Key Performance Parameters
PropertyBest-in-Class MOFValue
Thermal stabilityZIF-8 / ZIF-67Up to 550°C
Mechanical strengthZr-UiO series~20 GPa Young's modulus
Surface areaMIL-101 (Cr)~4000–4500 m²/g
DensityZn-MOF-50.2 g/cm³
Neutron shieldingGd-MOFHighest capture cross-section
H₂ adsorptionNi-MOF-74~6 wt%
CO₂ adsorption (Ni)Ni-MOF-74>40 wt%
Free volume (ZIF)ZIF-8Up to 90%

License the Satellite
Materials Platform

Full synthesis protocols and characterisation data available under NDA. Ideal for aerospace primes, satellite manufacturers, and space agencies.