Ultra Low Reflectance Black Silicon for Visible to IR Light Absorption
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Matter Intelligence is proposing the development of ultra-low reflectance black silicon to enhance light absorption from the visible to infrared spectrum, specifically targeting the NASA SBIR 2025 solicitation S12.01. This project focuses on improving diffraction control in coronagraphs to achieve the extreme contrast levels necessary for the Habitable Worlds Observatory to image and characterize Earth-like exoplanets. By optimizing cryogenic etching techniques, the effort aims to achieve broadband reflectance below 0.1% across a range of 0.4µm to 20µm, building upon previous work from the Roman Space Telescope. Phase I will focus on process optimization, sample fabrication, and reflectance validation to ensure flight instrument compatibility. The technology provides significant benefits for NASA's astrophysics, Earth science, and planetary science missions by reducing stray light and improving sensor contrast. Beyond space exploration, the innovation has broad commercial and defense applications, including enhanced surveillance systems, high-efficiency infrared detectors for the semiconductor industry, and improved signal clarity for LiDAR and hyperspectral imaging in autonomous vehicles. This federal solicitation is a total small business set-aside managed by the NASA SBIR/STTR Program, with performance taking place in California.
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Place of Performance
CA, USASet-Aside
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Full Description
Benefits: Matter Intelligence’s ultra-low reflectance black silicon technology directly supports NASA’s mission directives in astrophysics by advancing diffraction control in coronagraphs for exoplanet detection. This innovation will enhance the Habitable Worlds Observatory (HWO) by improving starlight suppression, enabling the spectral characterization of Earth-like exoplanets with contrast levels <1e-10. It builds on heritage from the Roman Space Telescope’s Coronagraph Instrument (CGI), addressing the critical need for improved light absorption materials. Beyond astrophysics, this technology can benefit NASA’s Earth science missions by reducing stray light in imaging spectrometers, enhancing data accuracy for climate and atmospheric studies. Additionally, it supports planetary science by improving instrument performance for missions requiring high-contrast imaging, such as future observatories and space telescopes designed to study distant celestial objects and planetary atmospheres. Matter Intelligence’s ultra-low reflectance black silicon has broad commercialization potential across multiple industries requiring advanced light absorption and stray light suppression. In defense and aerospace, it can enhance optical systems for surveillance, target tracking, and missile defense by improving sensor contrast and reducing optical noise. The semiconductor industry can leverage this technology for advanced photolithography and high-efficiency infrared detectors. In commercial optics, it benefits high-performance cameras, telescopes, and spectrometers used in scientific research, medical imaging, and environmental monitoring. Additionally, applications in LiDAR and hyperspectral imaging for autonomous vehicles, remote sensing, and industrial inspection can improve signal clarity and accuracy. By providing a scalable, durable, and high-performance solution, this technology addresses critical needs in precision optics, sensing, and imaging markets.
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