NASA SBIR 2020-I Solicitation

Proposal Summary


PROPOSAL NUMBER:
 20-1- S2.05-5110
SUBTOPIC TITLE:
 Technology for the Precision Radial Velocity Measurement Technique
PROPOSAL TITLE:
 Supercontinuum Waveguides for Extreme Radial-Velocity Instrumentation
SMALL BUSINESS CONCERN (Firm Name, Mail Address, City/State/Zip, Phone)
Octave Photonics, LLC
2735 Bristlecone Court
Lafayette, CO 80026
(513) 315-3618

Principal Investigator (Name, E-mail, Mail Address, City/State/Zip, Phone)

Name:
David Carlson
E-mail:
david.carlson@octavephotonics.com
Address:
4800 Baseline Rd Suite E104-363 Boulder, CO 80303
Phone:
(720) 213-5296

Business Official (Name, E-mail, Mail Address, City/State/Zip, Phone)

Name:
Zachary Newman
E-mail:
zachary.newman@octavephotonics.com
Address:
2735 Bristlecone Ct Lafayette, CO 80026 - 0000
Phone:
(513) 315-3618
Estimated Technology Readiness Level (TRL) :
Begin: 2
End: 3
Technical Abstract (Limit 2000 characters, approximately 200 words)

We are proposing Supercontinuum Waveguides for Extreme Radial-Velocity Instrumentation (SWERVI). The SWERVI platform will be an integrated-photonics subsystem for the calibration of current and next-generation astronomical spectrographs with precision-radial velocity (PRV) sensitivity <10 cm/s. The proposed module will use nonlinear nanophotonic waveguides to efficiently and controllably broaden the optical spectrum of an input frequency comb laser, to serve as the broadband calibration source in PRV measurements. The key innovations we will demonstrate in Phase 1 include: multi-stage broadening in high-nonlinearity tantala (Ta2O5), two-channel output to support self-referencing of the frequency comb, and high-average-power handling through robust packaging. When coupled with a high-repetition-rate comb source, the SWERVI system will enable new PRV calibration sources with spectral coverage virtually anywhere in the visible and near-infrared, while reducing power consumption and complexity through photonic integration. This system addresses a critical technology gap for extreme PRV measurements to detect and study exoplanets. Beyond PRV instrumentation, further development and commercialization of this nonlinear integrated-photonics platform will enable new capabilities in terrestrial and space-borne applications, such as atmospheric spectroscopy, precision timing and navigation, and optical communications.

Potential NASA Applications (Limit 1500 characters, approximately 150 words)

The development of nonlinear supercontinuum waveguides with optical frequency combs directly addresses the Tier 2 technology gap in the measurement sensitivity of stellar radial velocities for exoplanet detection. Moreover, this technology will have synergies with other important NASA programs through integration with next-generation optical atomic clocks for satellite navigation and timing, as well as space-based spectroscopic monitoring of Earth’s atmosphere to track long-term changes in the planet’s climate.

Potential Non-NASA Applications (Limit 1500 characters, approximately 150 words)

Supercontinuum sources find use as broadband sources for photonic device testing, "white light" interferometry, and several biological imaging modalities. In particular, tantala has an extremely broad transparency window and has applications in mid infrared spectroscopy of trace gases and organic molecules. Microcombs, a closely related technology, are of great interest for optical communications.

Duration: 6

Form Generated on 06/29/2020 21:06:31