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Palomar Habitable Zone Planet Finder (PARVI)

Completed TRL 3 (started at 3, targeting 5)

Description

Diffraction limited high resolution spectrograph for Doppler measurements of the host stars of extrasolar planets. This may enable the design of highly stable, high resolution spectrographs for astrophysics missions.

PARVI will couple to the Palm 3000 adaptive optics system at the Hale telescope at Palomar. It will conduct Doppler measurements of late type stars in search of low mass planetary companions. It may conduct follow-up activities for NASA TESS mission.

Benefits

Follow up measurements of exoplanets found with the NASA TESS mission.

Develops technologies that are pertinent to future missions currently being studied such as HabEx and LUVOIR.

Details

Technology areaSensors and Instruments > Remote Sensing Instruments and Sensors > Detectors and Focal Planes
ProgramCenter Independent Research & Development: JPL IRAD (JPL IRAD)
Lead organizationJet Propulsion Laboratory, Pasadena, CA
Start date2016-10-01
End date2019-09-01

Project contacts

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How to get involved

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