3.8 Proceedings Paper

FEA Testing the Pre-Flight Ariel Primary Mirror

出版社

SPIE-INT SOC OPTICAL ENGINEERING
DOI: 10.1117/12.2629815

关键词

Space Telescope; Ariel mission; aluminum mirror; optical test; FEA

资金

  1. Italian Space Agency (ASI) [2021-5-HH.0]
  2. National Institute for Astrophysics (INAF)

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Ariel is an ESA mission that aims to study exoplanets. It will orbit in the lagrangian point L2 and survey 1000 exoplanets simultaneously in visible and infrared wavelengths. The challenging scientific goals of Ariel require unprecedented engineering efforts, especially in designing the primary mirror with high accuracy. Some tests on a prototype mirror revealed unexpected deformation, leading to the need for numerical simulations to identify and understand the errors and guide future testing campaigns.
Ariel (Atmospheric Remote-sensing Infrared Exoplanet Large-survey) is an ESA M class mission aimed at the study of exoplanets. The satellite will orbit in the lagrangian point L2 and will survey a sample of 1000 exoplanets simultaneously in visible and infrared wavelengths. The challenging scientific goal of Ariel implies unprecedented engineering efforts to satisfy the severe requirements coming from the science in terms of accuracy. The most important specification - an all-Aluminum telescope - requires very accurate design of the primary mirror (M1), a novel, off-set paraboloid honeycomb mirror with ribs, edge, and reflective surface. To validate such a mirror, some tests were carried out on a prototype - namely Pathfinder Telescope Mirror (PTM) - built specifically for this purpose. These tests, carried out at the Centre Spatial de Liege in Belgium - revealed an unexpected deformation of the reflecting surface exceeding a peek-to-valley of 1 mu m. Consequently, the test had to be re-run, to identify systematic errors and correct the setting for future tests on the final prototype M1. To avoid the very expensive procedure of developing a new prototype and testing it both at room and cryogenic temperatures, it was decided to carry out some numerical simulations. These analyses allowed first to recognize and understand the reasoning behind the faults occurred during the testing phase, and later to apply the obtained knowledge to a new M1 design to set a defined guideline for future testing campaigns.

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