Lateral constraint for thin glass shell: analysis of the requirements and conceptual design for a segmented active mirror

TL;DR

This paper analyzes the physical constraints and design considerations for a segmented active mirror in large space telescopes, focusing on the lateral constraint requirements for thin glass shells under acceleration conditions.

Contribution

It provides a detailed analysis of the acceleration environment and proposes conceptual design considerations for a lateral constraint system for segmented active mirrors.

Findings

Acceleration environment impacts on mirror stability analyzed

Design requirements for shell retention system identified

Qualitative discussion on potential constraining solutions

Abstract

The latest high-performance telescopes for deep space observation employ very large primary mirrors that are made of smaller segments, like the JWST which employs monolithic beryllium hexagonal segments. A very promising development stage of these systems is to make them active and to operate on their reflective surfaces to change their shape and compensate for aberrations as well as to perform a very precise alignment. This is possible by employing a reference body that stores actuators to modify the shape of the shell, like in the SPLATT project where voice coil actuators are used. However, the lack of physical contact between the main body and shell places, along with the many advantages related to the physical decoupling of the two bodies, some concerns related to the retaining of the shell under all the possible acceleration conditions affecting the system during the mission lifetime. This paper aims to study the acceleration environment affecting the spacecraft during its lifetime and to use it as a baseline for operational requirements of a retaining system for the shells. Any solution is selected in this paper to leave complete freedom for the development of a constraining system, just some are qualitatively discussed.