← Back to NASA Technology Projects

Vortex Coronagraph High Contrast Demonstrations

Completed TRL 3 (started at 3, targeting 4)

Description

Our objective is to carry out critical performance demonstrations of the optical vortex coronagraph, by extending our previous work to deeper contrasts, broader bandwidths, and segmented apertures. Our specific goals are demonstrations of broadband pseudo-starlight rejection with a clear aperture at the 10e-10 level (first for 10% bandwidth, and then 20%) on JPL's HCIT-2 testbed, and also to carry out complementary high-contrast demonstrations on a segmented aperture testbed. We plan to carry out initial vortex mask and polarizer/quarter-wave-plate characterization on existing test facilities available to us at JPL and Caltech, including a polarizing microscope, a Muller Matrix Imaging Polarimeter, and cross-polarization spectroscopy in the existing Infrared Coronagraphic Testbed at JPL (which also operates in the visible). Muller matrix imaging and cross-polarization spectroscopy are extremely valuable initial evaluation tools that can immediately characterize a vortex's quality, thereby allowing us to better focus on the best vortices in the HCIT-2 facility. Likewise, the High Contrast Segmented Testbed at Caltech will allow initial testing of apodizers and segmented pupil configurations, prior to final tests in JPL's Decadal Segmented Testbed (DST). The HCIT and DST would thus only be used for final deep coronagraphic testing of already vetted vortex masks and apodizers, thus minimizing chamber time and cost, and maximizing efficiency and chamber sharing. Due to their small inner working angle and high throughput, optical vortex coronagraphs are of great interest to potential NASA coronagraphic missions such as Exo-C, HabEx, and LUVOIR, as well as to forthcoming large ground-based telescopes. Indeed, the vortex coronagraph is the primary coronagraphic mode selected by the Habex design study. Moreover, a broadband vortex coronagraph is also planned for the NASA-funded balloon project Picture-C. The vortex coronagraph thus has a very prominent role in NASA's exoplanet plans.

Benefits

The Strategic Astrophysics Technology program (SAT) supports focused development efforts for key technologies to the point at which they are ready to feed into major missions in the three science themes of the Astrophysics Division: Exoplanet Exploration, Cosmic Origins, and the Physics of the Cosmos. This program is specifically designed to address middle technology readiness level (TRL) "gaps" between levels 3 and 6: the maturation of technologies that have been established as feasible, but which are not yet sufficiently mature to incorporate into flight missions without introducing an unacceptable level of risk. NASA does not require a data management plan for proposals to SAT.

Details

Technology areaSensors and Instruments > Remote Sensing Instruments and Sensors > Optical Components
ProgramStrategic Astrophysics Technology (SAT)
Lead organizationCalifornia Institute of Technology, Pasadena, CA
Start date2018-10-01
End date2025-09-30

Project contacts

Listed on TechPort itself — the most direct way to ask about this specific project.

How to get involved

This is early/mid-stage (TRL 3) — 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.

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.