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images in the ultra-violet (UV), Visible (Vis) and Infra-Red (IR) regimes. Analysis of the Vis and UV (multi-spectral) images will provide sufficient signal to detect the NEO, while analysis of the IR image in conjunction with the UV and Vis images will provide information about its size. Within NASA’s Technology Area Breakdown Structure (TABS) nomenclature, this project is addressing TA08, Science Instruments, Observatories and Sensor Systems. We were able to demonstrate a lightweight multi-spectral imager and are currently commercializing this technology.