Self-Cleaning Seals

The following methods can be used individually or in combination to generate superhydrophobic surfaces: Synthesis of novel copolyimide oxetanes with unique surface properties The technology is the synthesis of a polyimide coating or film with a modified surface chemistry shown in Figure 1. A minor amount of an oxetane reactant containing fluorine is added to the polyimide, and the oxetane preferentially migrates to the surface, enabling relatively high concentrations of fluorine at the surface, without compromising the functional performance of the bulk of the polymide coating/film. The copolymers exhibit mitigation of particle adhesion and fouling from exposure to various particulate and biological contaminants and exhibit reduced surface energy and increased surface fluorine content at extremely low oxetane loadings relative to the imide matrix (see Figure 2). Additionally, the short fluorinated carbon chains do not bioaccumulate, reducing the environmental impact of these materials. Modifying surface energy via laser ablative surface patterning This method uses a laser to create nanoscale patterns in the surface of a material to increase the hydrophobicity of the surface (see Figure 2). The benefits of hydrophobic surfaces include decreases in friction and increases in self-cleaning properties. This is an advantageous method of surface modification because it is fast and single-step, promises to be scalable, requires no chemicals, could be applied to a variety of materials, and does not require a planar surface for patterning.

Previous techniques for measuring dust accumulation, mostly de-pendent on solar cell output, were limited by their inability to distin-guish dust effects from other factors like incident radiation and radiation damage. These techniques were less effective in environ-ments with inconsistent solar flux and future missions, such as the Lunar South Pole, and lacked versatility in adapting to diverse envi-ronmental conditions. The PADS device embraces success over these challenges, and reflects enhanced features over prior iterations to also allow for space environments. Key design features begin with the customizable mechanical design of the PADS device for use in space environments, heaters with imbedded precision temperature sensors, a selected optical coating for the device coupons that are calibrated on high-fidelity thermal modeling and validated with ground-based testing to simulate the space environment of interest (including dusting with simulants representative of the planetary-body soil/regolith), and a control circuit for precision control/matching of the thermal inputs to the sensor via the heaters. Retainers with mount isolators are implemented to ensure the stacked layers within the device do not dislodge during high vibration or gravitational loads during launch. For operation, the PADS device is installed at the point of interest (e.g., space vehicle surface, extraterrestrial equipment) to quantify dust accumulation. Power and data transfer are done through cabling to the space vehicle system or can be provided standalone. A control circuit/algorithm adjusts the power to the heaters to precisely match the temperature setpoints. Ground testing in the simulated space environment conditions of interest creates a calibration plot of effec-tive emittance versus dust density, and allows determination of the degradation in emittance as the dust increases on the surface. Testing on the PADS device has been completed in a simulated lunar environment and data has been collected to enable sensor calibration for its use on the Moon. It is currently poised for integration into a lander for flight testing. Although the PADS device is intended for use in a burgeoning space industry and requisite environments – but given that the PADS device is partially comprised of programmable sensors in conjunction with optically coated coupons that can be tailored for custom use - it or its constituent components could be modified for terrestrial applications such as surface dust monitoring on photovoltaic panels or potentially combustible dust on various industrial surfaces.

State-of-the-art (SOTA) EDS technology includes the addition of a dielectric substrate, the EDS electrodes, and a dielectric cover layer. Typically, this multilayer stack-up for thermal radiator EDSs are built as a stand-alone and placed directly on top of the thermal radiator base and covered with the thermal control material. This new coating system represents an alternative EDS approach that integrates with the thermal radiator's thermal control coating system. The approach involves utilizing the thermal control coating in multiple functional capacities within the EDS configuration. The thermal control coating properties are leveraged to provide electrical insulation characteristics suitable for EDS operation while maintaining thermal performance requirements. The EDS configuration incorporates conductive elements positioned within the thermal control coating structure. The thermal control coating is applied using processes compatible with standard thermal radiator construction methods. The conductive elements are integrated during the coating application sequence. This integrated EDS approach incorporated into a thermal radiator system reduces certain components compared to SOTA EDS systems. The reduction in components offers potential benefits in system mass, thermal performance characteristics, and manufacturing complexity. The approach may reduce certain failure modes associated with interface layers and thermal expansion effects. This EDS configuration allows for enhanced flexibility in thermal radiator design parameters.

In addition to previous LOTUS coating formulations, an additional optical formulation may be applied via vacuum deposition. This coating forms a top layer and may be applied in different thicknesses that serve to enhance its hydrophobic properties. The vacuum deposited material may comprise fluorinated ethylene propylene or a similar material. This coating is transparent and can be used on optical components or any other applications requiring a clear coating.

The Astromaterials Acquisition and Curation Office (AACO) at NASA Johnson Space Center currently curates 500 milligrams of the regolith sample from the Asteroid Ryugu that was collected by the Japan Aerospace and Exploration Agency’s Hayabusa II spacecraft and returned to Earth in 2021. In September 2023, NASA’s OSIRIS-REx spacecraft returned 70 grams of regolith collected from the surface of Asteroid Bennu. These astromaterial sample collections are stored and handled in gloveboxes and desiccators that are continuously purged with ultrapure nitrogen in order to minimize contamination and alteration of extraterrestrial samples from terrestrial environments. For collaborative astromaterial sample research conducted outside of the AACO, a need emerged for a sample container system suitable for global transport, capable of maintaining the same low-oxygen envi-ronment as laboratory gloveboxes. Thus, the MCS was developed. MSC’s of different sizes (2, 4, and 8-inch sample container models) have been developed to store contact pads and bulk samples from NASA missions, including the OSIRIS-REx Asteroid Bennu mission. MCS’s are designed with seal profiles to prevent oxygen from seeping into the sample container. Additionally, the MCS uses a sample container form-factor that optimizes favorable nitrogen to oxygen gas ratios. The final prototypes were tested and verified using optochemical sensors to measure trace oxygen levels within the sealed containers. The Modular Container System (MCS) could fill a critical gap in the existing high-purity logistics and storage market in its ability to provide a passively maintained, verifiable, multi-year, glovebox-level low-oxygen environment in a portable robust form-factor. Although this technology was originally developed for astromaterial transport and storage, commercial applications may also exist in biopharmaceutical/ bio-banking, microelectronics/ semiconductor, and other industries.