NASA's Langley Research Center has built a very small spectrometer by integrating a differential linear Fresnel lens onto an imaging chip. NASA is using the lens/chip in a very small spectrometer that will be mounted on the tires of a rover to analyze soil on the Moon or Mars. The spectrometer is useful for space-constrained applications. It combines good resolution with small size and potentially reduced manufacturing costs. The ultra-compact integration of the spectrometer is enabled by the use of an optimized Fresnel grating. Since Fresnel imaging works as valid focal points of spectrum within the short optical distance, the shorter optical path length required (compared to a traditional Fraunhofer lens) enables the small size. Further, the evolution to a differentially linear Fresnel lens (instead of circular Fresnel) avoids the need for aperture slit driver electronics and moving parts, and simplifies manufacturing. The linear Fresnel gratings lend themselves to mass production via plastic injection molding or nano-imprint lithography. NASA is seeking partners to develop the spectrometer for commercial applications.

(a) Shown are various types of Fresnel gratings (zone-plates), (b) 3D configuration of a conventional Fraunhofer spectrometer, and (c) a linear Fresnel spectrometer.

The Fresnel spectrometer was built by adding a Fresnel grating onto a tiny sensor array microchip. A half linear Fresnel grating was mounted vertically on one end of a linear imaging sensor. The Fresnel spectrometer uses a gradient line grating with changing gaps and widths. The angle between the imaging detector surface and the grating is 90 degrees. The resolution of the current iteration is 20 nm with a spectral range of 200 nm to 1200 nm. Resolution is dependent on the number of gratings. Theoretically, if the number of gratings approaches 200, the resolution would be less than 5 nm.

The figure shows an actual photo of the linear imaging sensor array chip (Hamamatsu S8378-256Q) that became a platform for building the first prototype linear Fresnel spectrometer. This chip has 256 active pixels in 25-m pitch and 0.5-mm height, spectral response range of 200 to 1,000 nm, and maximum operating clock frequency of 500 kHz. Instead of building a spectrometer by putting a detector into a box, NASA built the spectrometer onto the detector chip itself.

NASA has developed a technology demonstrator of the basic spectrometer. In addition to the spectrometer, NASA has a software algorithm to acquire spectrum data and convert it to actionable information. This technology has potential applications in agriculture, automobiles, drug enforcement, food processing, healthcare, personal protection, and textile manufacturing.

NASA is actively seeking licensees to commercialize this technology. Please contact The Technology Gateway at This email address is being protected from spambots. You need JavaScript enabled to view it. to initiate licensing discussions. Follow this link for more information: here .

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This article first appeared in the August, 2017 issue of Tech Briefs Magazine.

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