Micro-Slit Collimators for X-ray/Gamma-ray Imaging, Phase II

Building on the success of our Phase I efforts, Mikro Systems, Inc. (MSI) proposes to advance the state-of-the-art in high resolution, high-aspect-ratio X-ray/gamma-ray collimator fabrication by reducing slit pitch by a factor of ~2, from 35 microns to 20 microns, using an innovative hybrid micro-machining technology. Fine grids having high-aspect-ratio (>50:1) and made from dense materials are the enabling components for solar and astrophysical imaging missions requiring high angular and/or spectral resolution at X-ray/gamma-ray energies. Instruments for these missions are severely constrained by size and mass considerations, and any technology that allows a reduction of size and/or mass without reducing image quality would contribute significantly to NASA's ongoing instrumentation development. Angular resolution is a function of the grid-pitch and distance between grids in a bi-grid collimator. Consequently, this advance in technology will have a significant effect on the angular resolution and/or instrument length and mass of grid-based optics required for x-ray and gamma-ray imaging in space. In Phase I, MSI demonstrated the technical feasibility of producing collimator grids with pitch as fine as 16 microns.

This is a mature technology (TRL 7+) — the realistic path in is usually NASA's Technology Transfer Program: licensing an existing NASA patent, or a Space Act Agreement to use NASA facilities/expertise directly. NASA also runs a startup licensing program with no upfront fee for companies formed to commercialize a specific NASA technology.

None of these are guaranteed paths for this specific project — TechPort itself doesn't have an "apply" button. Reaching out to the contact(s) above with a specific question is usually the fastest way to find out what's actually open.