16 - 21 June 2024
Yokohama, Japan
Conference 13100 > Paper 13100-11
Paper 13100-11

Hyperpolishing off-axis mirror’s with nanoparticles slurries for the next generation of space exoplanets imagers

16 June 2024 • 14:05 - 14:20 Japan Standard Time | Room G214, North - 2F

Abstract

The stressed-mirror polishing process has been successfully deployed for the manufacturing of Nancy Grace Roman Space Telescope coronagraph mirrors. This process combines a simple warping system with an optimized (more complex) thickness distribution of the mirror’s substrates allowing to warp them into the required Off Axis Parabola’s parameters. This way, the polishing process uses full-sized tools, avoiding the generation of undesired high spatial frequency sub-aperture tool marks. The smoothness of the surface is then worked with a super-polishing process, lowering the roughness down to a few Angstroms. The research we present is done in the frame of the post-RST technology maturation roadmap. The Habitable Worlds Observatory requirements are so drastic that we must push the performance of the stressed mirror polishing process to gain on the roughness. Together with chemical scientists, we work on the production of nanoparticle slurries with the goal to go below the angstrom in terms of roughness. In this talk, we present the nanoparticles production process, the results obtained on the mirror’s prototypes we produced and the roadmap for the production of hyperpolished OAPs.

Presenter

Houda Bellahsene
Lab. d'Astrophysique de Marseille (France), Institut Charles Gerhardt Montpellier (France)
Houda Bellahsene is a chemist, PhD students, applying her skills to the development of optical fabrication process towards ultra-polished astronomical mirrors, in the frame of the maturity increase of technologies for future large space telescopes such as the Habitable Worlds Observatory.
Application tracks: Astrophotonics
Presenter/Author
Houda Bellahsene
Lab. d'Astrophysique de Marseille (France), Institut Charles Gerhardt Montpellier (France)
Author
Lab. d'Astrophysique de Marseille (France)
Author
Institut Charles Gerhardt Montpellier (France)
Author
Institut Charles Gerhardt Montpellier (France)
Author
Lab. d'Astrophysique de Marseille (France)
Author
Institut Charles Gerhardt Montpellier (France)