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Primary mirror segmentation for large optical telescopes: an inverse map projection approach.
Applied Optics
|October 6, 2021
Summary
This study presents three map projection methods for segmenting large telescope mirrors, offering optimal regularity, equal area, or minimized segment diameter. A compromise approach unifies these for flexible primary mirror segmentation.
Area of Science:
- Astronomy and Optical Engineering
- Large segmented-mirror telescope design
Background:
- Primary mirror segmentation is crucial for large telescope construction, impacting support, fabrication, and cost.
- Hexagonal tiling is effective for segmenting curved surfaces with specific solid angles.
Purpose of the Study:
- To present and unify three map projection-based approaches for primary mirror segmentation.
- To numerically verify the performance of these segmentation methods.
Main Methods:
- Conformal map projection for optimal local angle preservation and regularity.
- Equal-area map projection for zero area variation.
- Equidistant map projection to minimize segment circumscribed diameter.
- A novel compromise approach unifying the above methods.
Main Results:
- The conformal method offers superior regularity.
- The equal-area method ensures consistent segment area.
- The equidistant method optimizes segment size.
- The compromise approach allows for adjustable segmentation based on specific needs.
Conclusions:
- The presented map projection methods effectively segment large telescope primary mirrors.
- The study validates a scaling rule and provides insights into mirror segmentation mechanisms.
- These findings aid in the design and fabrication of advanced astronomical instruments.

