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Super Resolving Astronomical Targets by Leveraging Quantum Measurements
Completed
Description
For approximately the past 150 years the resolution of astronomical measurements has been constrained to the diffraction limit of the collecting aperture or synthesized aperture. Achieving high-resolution imagery of stars or probing extended structures meant either building a bigger telescope or going towards aperture synthesis through interferometry. Recent advances in the field of quantum measurements have shown that incoherent sources, such as stellar companions, lends themselves to a specific kind of modal analysis that can achieve sub-diffraction limited estimates on the separation of the two objects down to theoretically zero separation. By decomposing light into an orthogonal basis, such as Hermite-Gaussian modes, the underlying mode structure provides information to the observer not readily available in a classical measurement scheme. The intent of this proposal is to further develop and demonstrate a bench-top setup showing the method used to probe the underlying mode structure, referred to as mode-selective sum frequency generation, and its applicability to astronomical imaging. Of special interest in furthering the TRL is understanding the range of applicability of the modal analysis technique, the broadband nature of the measurement schemes, development of efficient parameter extraction algorithms, and the interface to the telescope.
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 |
| Program | Astrophysics Research and Analysis (APRA) |
| Lead organization | Ball Aerospace & Technologies Corporation, Boulder, CO |
| Start date | 2022-07-01 |
| End date | 2025-06-30 |
Project contacts
Listed on TechPort itself — the most direct way to ask about this specific project.
- Brian D Baker
- Brian A Hicks
- Courtney L Coe
- Jennifer Lee
- Laurent A Pueyo
- Remi Soummer
- Tyler Mccracken
- Yuping Huang
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.