Heat treatment procedure of the Aluminium 6061-T651 for the Ariel Telescope mirrors

The Atmospheric Remote-Sensing Infrared Exoplanet Large Survey (Ariel) is the M4 mission adopted by ESA's Cosmic Vision program. Its launch is scheduled for 2029. The purpose of the mission is the study of exoplanetary atmospheres on a target of similar to 1000 exoplanets. Ariel scientific payload consists of an off-axis, unobscured Cassegrain telescope. The light is directed towards a set of photometers and spectrometers with wavebands between 0.5 and 7.8 mu m and operating at cryogenic temperatures. The Ariel Space Telescope consists of a primary parabolic mirror with an elliptical aperture of 1.1 center dot 0.7 m, followed by a hyperbolic secondary, a parabolic collimating tertiary and a flat-folding mirror directing the output beam parallel to the optical bench; all in bare aluminium. The choice of bare aluminium for the realization of the mirrors is dictated by several factors: maximizing the heat exchange, reducing the costs of materials and technological advancement. To date, an aluminium mirror the size of Ariel's primary has never been made. The greatest challenge is finding a heat treatment procedure that stabilizes the aluminium, particularly the Al6061T651 Laminated alloy. This paper describes the study and testing of the heat treatment procedure developed on aluminium samples of different sizes (from 50mm to 150mm diameter), on 0.7m diameter mirror, and discusses future steps.

Automated summary

The Atmospheric Remote-Sensing Infrared Exoplanet Large Survey (Ariel) is a mission under the Cosmic Vision program of the European Space Agency. It aims to study the atmospheres of approximately 1000 exoplanets. The mission will use an off-axis, unobscured Cassegrain telescope with photometers and spectrometers operating at cryogenic temperatures. The challenge lies in developing a heat treatment procedure to stabilize the aluminium mirrors, particularly the Al6061T651 Laminated alloy.