← Back to NASA Technology Projects
Miniature Photonic Spectrometers and Filters for Astrophysics and Space Science
Completed
Description
This project seeks to apply our recent breakthroughs in astrophotonics - photonics applied to astronomical instrumentation - to replace the large lenses, mirrors, and gratings of conventional astronomical spectrographs with optoelectronic components borrowed from the multi-billion dollar telecommunication industry. This will reduce the mass and volume of these instruments by two to three orders of magnitudes, shorten delivery times, lower the risk, and cut the cost proportionally. Photonic instruments are also more amenable to complex light manipulation and massive multiplexing, cheaper to mass produce, easier to control, much less susceptible to vibrations and flexures, and have higher throughput. The proposed effort directly addresses one of the technology gaps identified in the 2016 Cosmic Origins Technology Report, namely the need to develop "high-performance spectral dispersion components / devices." Using private funding, we have developed photonic near-infrared (1.4 - 1.6 microns) spectrometers where the dispersing optics are replaced by miniature (~1 cubic-centimeter) arrayed waveguide gratings imprinted using buried silicon nitride (``nano-core'') technology, the leading solution for low-loss waveguides. We have also developed highly sophisticated photonics filters using complex waveguide Bragg gratings, produced on the same platform technology as the photonic spectrometers and equally small. These prototypes have been fabricated and tested using the state-of-the-art facilities of the Maryland NanoCenter and AstroPhotonics Lab, and the results of these tests have been published in refereed publications and conference proceedings. APRA funding is now needed to develop the next generation of photonics spectrometers and filters for astrophysics and space science applications. We will (1) broaden the wavelength range to 1 - 1.7 microns, (2) increase the spectral resolving power of our photonic spectrometers from R ~ 1500 to 3000, (3) experiment with the aspect ratio of the waveguide cross-section and overall design of the Braggs and arrayed waveguide gratings to make them polarization-independent, and (4) increase the overall throughput of these gratings to >70% at 1 - 1.7 microns by changing the deposition method of the cladding material (silica) and reducing the scattering losses with the use of a newly commissioned electron beam writer that delivers higher resolution (down to a few nm instead of ~8 nm). Two graduate students, already trained in the techniques relevant to this project, will lead the optimization, fabrication, and testing of these optoelectronic components. Up to three undergraduate students will also be involved with the research. A wide swath of astrophysical research, from spectroscopic studies of the distant universe to searches for biosignatures in the atmospheres of exoplanets, stands to benefit from these miniature spectrometers and filters on board future NASA balloon, CubeSat, Explorer, Probe-, Flagship-, and Surveyor class missions. The technical by-products of this effort will also offer benefits in fields far beyond astronomy, such as medicine, human science, petrochemistry, space geo-science, and quantum computing and communication. The names and contact information of five experts qualified to review this proposal were emailed directly to the two relevant Program Officers.
Benefits
The Astrophysics Research and Analysis program (APRA) supports suborbital and suborbital-class investigations, development of detectors and supporting technology, laboratory astrophysics, and limited ground-based observing. Basic research proposals in these areas are solicited for investigations that are relevant to NASA's programs in astronomy and astrophysics, including the entire range of photons, gravitational waves, and particle astrophysics. The emphasis of this solicitation is on technologies and investigations that advance NASA astrophysics missions and goals.
Details
| Technology area | Sensors and Instruments > Remote Sensing Instruments and Sensors > Detectors and Focal Planes |
| Program | Astrophysics Research and Analysis (APRA) |
| Lead organization | University of Maryland-College Park, College Park, MD |
| Start date | 2018-01-01 |
| End date | 2020-12-31 |
Project contacts
Listed on TechPort itself — the most direct way to ask about this specific project.
How to get involved
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.