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NASA Contributions to LISA: Space-based Gravitational Wave Laser Technology Development Project for the LISA Mission
Completed
TRL 4 (started at 3, targeting 6)
Description
LISA uses laser light to make measurements of the distance between pairs of spacecraft. In order to reach the required precision of picometers (1pm = 10-12m), the LISA lasers must carefully control both their intensity and their wavelength. In addition, the lasers have to operate for an extended period in the harsh environment of space. NASA is developing a prototype LISA laser system to meet these challenging requirements. The LISA laser utilizes the same non-planar ring oscillator (NPRO) technology employed by ground-based gravitational wave detectors like LIGO but in a customized package that is optimized for spaceflight. The laser is stabilized to a frequency reference cavity similar to the one which flew on the NASA-German GRACE-FO mission.
Benefits
Develop enabling technology for the LISA mission US contribution to the LISA mission led by ESA
Details
| Technology area | Sensors and Instruments > Remote Sensing Instruments and Sensors > Lasers |
| Program | Physics of the Cosmos (PCOS) |
| Start date | 2017-05-01 |
| End date | 2023-12-31 |
How to get involved
This is early/mid-stage (TRL 4) — 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.