Large Ultra Lightweight Monolithic Mirros for Space Missions

Technology Roadmap Sections and Deliverables

This is a technology roadmap for:

• 3LULMMFSM - Large Ultra-Lightweight Monolithic Mirros for Space Missions

Large-Ultra Lightweight Monolithic Mirrors (LULMM) also enable segmented designs for space missions - Mirrors are enabling technology for space based telescopes. Primary mirror size and quality is directly traceable to telescope performance. Every engineering advancement in space mirror technology has resulted in improved earth observation and science performance. Future large scale optical instruments for Earth Observation and Science missions will require very large primary mirrors with extreme light weighting. There has been significant technical evolution realized over the last years. However, the current level of light weighting is reaching the limit of classical techniques and decreasing optical performances due to side efforts, causing mission concepts with active correction capabilities which could be simplified by using alternative techniques for lighter and stiffer primary mirrors. The weight can be drastically reduced with designs based on a thin optical face sheets, which are attached to a stiff and lightweight support structures (e.g. honeycomb…).

Ultra precision mirrors are setting the space telescope design. Rare are the components whose design lies at such optimal crossroads between 3 major engineering fields (optical, thermal and mechanical), all the while challenging manufacturing and integration capacities in these same fields. The recent spotlight on JWST’s magnificently gigantic golden primary mirror, and the incredible pictures it helps create (figure below), has brought mirror design to the forefront of the public eye as well as the engineer’s, yet the subtle and skillful art and efforts which underlie a truly successful mirror design are not always obvious. This roadmap addresses previous, current and future needs of space mirror technologies.

Roadmap Overview

Images show the Science and Earth Observation programs from the European Space Agency (ESA) and National Aeronautics and Space Administration NASA), indicating the needs for space mirror technologies.

Some critical elements enabling the LULMM considers:

• large aperture, lowr-areal denisty and ultra-high stiff mirror substrates
• support structure
• mid/high-spatial frequency figure error
• segment-to-segment gap phasing
• mirror segment edges
• modeling and validation

Figure is showing the 5x5 Technology Matrix [Ref.1] with the position of 3LULMMFSM.

A significant amount of developments was carried out for ultra lightweight mirrors. Ball Aerospace demonstrated Beryllium mirrors with an aerial density as low as 9.8 kg/m m2. However , this was for a diameter 0.5m and without guaranteeing sufficient stiffness in order to survive the launch, similar as for the JWST where the mirrors have to be re designed with a final aerial density of 28 kg/m m2, while whilethe initial concept was aiming to achieve even below 15 kg/m m2.

A primary mirror of JWST has 6.5 meters (21 feet 4 inches) across, which is needed to measure the light from distant galaxies. Building a mirror this large was challenging, even for use on the ground. This size of the mirror had never before been launched into space, in comparison the Hubble Space Telescope 2.4 meter mirror is shown, which would be too heavy to launch into orbit for the JWST. For the JWST the stiff and light mirror was essential, thus having very lowe aerial density to enable the mission.

Technology advancements are progressing and now future must be prepared to enable areal densities less than 10 kg/m2, for large mirrors located in an optical system entrance cavity (e.g., scan mirror, primary mirror). This would enable key fac tor in the production of large monolithic mirrors (>2 meters) usable for EO and JWST successor like missions, thereby securing high resolution imaging capability for space systems in e.g., geostationary orbit.

Space community, industry and agencies are addressing this gap seeking for next technological developments to enable low aerial density, ultra-high performance mirrors [Ref. 2-5].

• GEO mid.-high resolution observation
• Science missions
• Agile flat mirrors (Fast-steering, scanners…)

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