August 25, 2017 - LSST’s Primary/Tertiary Mirror (M1M3) has been stored in a metal container at Tucson International Airport since its completion in 2015. Earlier this month, an LSST Telescope and Site team visited the storage site to open the container and inspect M1M3 in order to plan and prepare for upcoming hardware and electrical integration activities. The outside of the metal storage container has been inspected regularly since its arrival at the airport, but the container hasn’t been opened since May, 2015!
Although prepared for anything, once the container was opened the group encountered nothing more than a light coating of dust which was, according to Telescope and Site Optics Engineer Constanza Araujo, “No more than you’d find in a Tucson living room after a week.” The surface of the mirror has been protected from this inevitable accumulation of dust by a blue OptiCoat coating, described in this 2015 blog post, which will be removed and replaced with a clean OptiCoat coating at the end of the mirror’s storage period. The mirror won’t get its final, reflective surface coating until it arrives at Cerro Pachón.
One of the tasks completed by the team during this visit was to establish the compatibility of the load spreaders already installed on the mirror with the backing plates that will interface with the M1M3 static support system (which was described in this recent blog post). The backing plates provide a surface for the static support wire baskets to contact in the event of full compression of the static supports. The backing plates must be installed on the load spreaders before M1M3 is integrated with the mirror cell, as the back of the mirror itself will no longer be accessible afterwards.
The team also removed several panels underneath the mirror to access and map the configuration of electrical cables on M1M3. Lastly, a general inspection of the mirror’s surface, conducted by climbing up through the hole in the middle of the mirror, established that no visible damage to the mirror’s surface has occurred during storage.
This inspection of M1M3 was one of the early steps in the process of preparing it to be moved back to the Richard F. Caris Mirror Lab at the University of Arizona in May of 2018 for integration and testing with the M1M3 cell. Currently, M1M3 is scheduled to ship to Cerro Pachón by the end of 2018.
Financial support for Rubin Observatory comes from the National Science Foundation (NSF) through Cooperative Agreement No. 1258333, the Department of Energy (DOE) Office of Science under Contract No. DE-AC02-76SF00515, and private funding raised by the LSST Corporation. The NSF-funded Rubin Observatory Project Office for construction was established as an operating center under management of the Association of Universities for Research in Astronomy (AURA). The DOE-funded effort to build the Rubin Observatory LSST Camera (LSSTCam) is managed by the SLAC National Accelerator Laboratory (SLAC).
The National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 to promote the progress of science. NSF supports basic research and people to create knowledge that transforms the future.
NSF and DOE will continue to support Rubin Observatory in its Operations phase. They will also provide support for scientific research with LSST data.
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