We believe iGEM can advance the cause of recycling in space.
As space exploration ventures beyond Earth orbit toward the Moon and Mars, mission planners face a critical constraint: resupply cost increases exponentially with distance. For the International Space Station (ISS), which orbits just 400 km above Earth, resupply costs roughly $10,000–$20,000 per kilogram. For future deep-space missions to Mars—requiring 6–9 months of transit—resupply becomes logistically impractical and economically prohibitive. A crewed Mars mission lasting 2–3 years will generate an estimated 7.5–8 tons of solid waste for a four-person crew—all of which currently cannot be recycled and must either be stored (consuming valuable habitat volume) or discarded.
The ISS itself provides a concrete example. Four astronauts generate approximately 2,500 kg of trash per year, or roughly two trash cans per week. The ISS accumulates up to 2 tonnes of rubbish on board for a total of 12 tonnes per year, and this garbage is typically collected and loaded into cargo spacecraft bound for atmospheric re-entry, where it burns up on descent. While this solves the on-station storage problem, it wastes a valuable resource and creates atmospheric pollution.
When spacecraft and orbital waste re-enter Earth's atmosphere at thousands of degrees Celsius, they release not only carbon dioxide and water vapor—which are harmless—but also metal oxides and combustion products from polymers like PET. After end of life, satellites and rocket stages reenter Earth's atmosphere and inject a substantial amount of their matter into the mesosphere and lower thermosphere. Recent research has documented significant and even dominant injection of several metal elements regularly used in spacecraft compared to natural injection by meteoroids, posing substantial risks of long-term adverse effects on the atmosphere such as ozone depletion, radiative effects and changes in cloud formation.
For plastic waste specifically, combustion at re-entry temperatures (>1000°C) releases particulates and volatile organic compounds. A future Mars program with multiple resupply missions could contribute measurably to this pollution—a burden that should be minimized through recycling rather than disposal.
On Earth, PET recycling relies on two primary pathways, each with significant limitations for space:
Mechanical Recycling:
Mechanical recycling requires heating plastic to 285°C and high pressure for extrusion, followed by pelletization and polycondensation at elevated temperatures. A major drawback of mechanical recycling is the degradation of PET properties with each cycle, leading to a decrease in elasticity and viscosity, resulting in recycled polymer losing value and eventually being sent to landfills after several cycles. This process consumes significant energy and requires heavy industrial equipment—incompatible with the mass and power constraints of spacecraft.
Chemical Recycling (Industrial Standard):
The most mature industrial method is glycolysis. Glycolysis is widely adopted by major companies like DuPont, Dow Chemicals, and Shell Polyester for large-scale PET recycling, and it offers the mildest operating conditions among chemical recycling methods, operating at lower cost and lower volatility of solvents. However, glycolysis typically requires temperatures between 180–250°C and the use of catalysts or high pressures. Alternative chemical methods like methanolysis demand even harsher conditions: conventional methanolysis processes typically require harsh conditions exceeding 200°C and 2–4 MPa pressure.
Why These Fail in Space:
There is a critical temperature gap: industrial recycling operates at 180–285°C, while safe spacecraft operations typically stay below 50°C.
We propose SynPETic, a system that closes this gap by harnessing biological catalysts—enzymes—to depolymerize PET at mild temperatures and pressures, making it safe and efficient for space-based recycling.
Our solution combines three engineered proteins into a multi-enzyme complex inspired by nature's cellulosomes—catalytic machines found in cellulase-producing bacteria that degrade cellulose through coordinated enzyme action.
Three Engineered Proteins:
When ICCG-DoT and TfCa-DoG act independently in solution, their reaction products mix inefficiently:
By fusing both enzymes to complementary dockerin/cohesin domains and loading them onto the ScafGVT scaffold, we achieve spatial co-localization: the intermediate product (MHET) released by ICCG-DoT is immediately adjacent to TfCa-DoG, enabling substrate channeling and more efficient sequential conversion:
PET → [ICCG-DoT] → MHET → [immediately adjacent TfCa-DoG] → TPA + EG
(much faster cascade)
Prior iGEM projects have explored PETase expression and basic enzyme assays. Several commercial efforts (e.g., Carbios in France, Quantumscape) focus on thermophilic variants or traditional chemical catalysis.
Our contribution is unique in three ways:
Wet Lab:
Composite Part:
Measurement:
For Space Missions
For Earth