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Ultra-high resolution integrated arrayed waveguide spectrometer with reusable delay lines for exoplanet detection
Completed
TRL 5 (started at 3, targeting 5)
Description
New Integration Photonics, Inc., is proposing to develop an ultra-high resolving power (R>150,000) spectrometer based on arrayed waveguide gratings (AWGs) on a Si3N4/SiO2 photonic integrated chip (PIC). The spectrometer implements a reusable delay line (RDL), replacing the large number of waveguides in the traditional AWG, which significantly reduces the size and increases the stability of the chip. This high-resolution integrated spectrometer can be used in the detection of exoplanets based on the Precision Radial Velocity (PRV) method. The proposed photonic chip has three unique advantages to significantly improve the performance of the traditional spectrometer and increases the feasibility of chip fabrication. 1.By reducing the number of waveguides to just one, and coupling the power from single waveguide to achieve the correct power and phase distributions, the new technique eliminates the need for making large AWGs and the associated step of actively compensating the phase error. The footprint of the spectrometer can be potentially reduced by a factor of more than 100. 2. A parabolic taper will be implemented instead of a linear taper before the free propagation region (FPR) to reducing the cross-coupling, and thus the phase distribution error. 3. The photonic chip will be directly coupled to a 1-D CCD array in Phase II. To achieve this, a three-stigmatic-points compensation approach is proposed for the RDL-AWG design to realize a flat focal-plane at the output of the free propagating region. It also improves the accuracy and the uniformity of the RDL-AWG and compensates for the aberration.
Benefits
A successful completion of Phases I and II would allow the Company to claim to have realized a high resolving power integrated spectrometer. This will lead to a very compact instrument that can potentially be used in many NASA related projects. This can include sensors, lidar, laser ranging, medical and health applications. The Company will pursue opportunities with NASA for infusion in future NASA missions (including exoplanet detection).
Currently, the biggest market for on-chip spectrometers is academic labs. On-chip spectrometers may also find important applications for on-field geological measurement for mining or oil & gas. On-chip spectrometers might also find some interesting applications in pharmaceutics, food & beverages, agriculture, environment testing, medical point-of-care, consumer, and etc.
Details
| Technology area | Sensors and Instruments > Remote Sensing Instruments and Sensors > Optical Components |
| Program | Small Business Innovation Research/Small Business Tech Transfer (SBIR/STTR) |
| Lead organization | New Integration Photonics, Chevy Chase, MD |
| Start date | 2023-08-03 |
| End date | 2024-02-02 |
Project contacts
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This is early/mid-stage (TRL 5) — the most realistic path in is NASA SBIR/STTR, which funds small businesses and research institutions to develop technology aligned with NASA's needs (equity-free, phased funding). Check whether a current SBIR/STTR solicitation topic overlaps with this project's technology area, or contact the project directly (above) to ask.
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