
Congrats is due our FEMAP support customer, the Giant Magellan Telescope Organization. GMTO is on a bit of a hiring spree as their planned 2025 activation date comes closer.
We introduced some of their team into the world of FEMAP with access to our customized resources, including our popular Starting Fresh webinar which covers model organization; our Best Practices seminar that gives an excellent overview on key touchpoints within FEMAP; and our Principals of Vibration seminar covering various vibration-based analysis techniques.
The GMTO is part of a slew of telescopes slated to come online in the 2020s. Other telescopes underway include the succinctly-named Thirty Meter Telescope, the not-so-creatively-named European Extremely Large Telescope, and the okay-this-name-thing-is-getting-out-of-hand Overwhelmingly Large Telescope, which has since been cancelled and folded into the EELT project.
GMTO recently did a lengthy interview with Engineering.com, where they discuss the project, the team, the mirror casting process and their testing process. The GMT will be made of seven primary mirror segments, each 8.4 m (27.6 ft.) in diameter. According to Patrick McCarthy, Operations VP, that size is the magic size gleaned from hard-won lessons a few decades ago:
“What we leaned in the 1980s and ‘90s is that there’s a maximum size you can make any individual mirror; in practice, it appears to be about 8 or 9 meters in diameter. Some of that is set by the physics of glass and how uniformly you can allow it to cool without building up internal strains, and some of it is practical issues, such as how can you pick up a piece of glass that big and take it to a mountaintop without it breaking just by the fact of you lifting it and it sagging under its own gravity.”
The mirrors are made in small batches in Japan out of borosilicate glass, with very low thermal expansion and very uniform thermal expansion from piece to piece.
For the full article please visit Engineering.com