Rubin Observatory Achieves Another Major Milestone: Reflective Coating of the 8.4-meter Primary/Tertiary Mirror Built at the Richard F. Caris Mirror Lab

Seventeen years ago, under the UArizona football stadium, technicians at the Richard F. Caris Mirror Lab began carefully hand-loading borosilicate glass into the enormous furnace that would cast two colossal, concentric mirrors in a 51,900-pound mirror blank—the first time a combined primary and tertiary mirror had ever been produced on such a large scale. On April 27, 2024—after a meticulous multi-year process of polishing and a five-week ocean voyage to Chile—the 8.4-meter Primary/Tertiary Mirror (M1M3) for the Vera C. Rubin Observatory received a brilliant reflective coat of protected silver: an essential step on its path toward capturing light from the distant cosmos. When installed, the mirrors from Steward Observatory’s Richard F. Caris Mirror Lab will help provide the widest, fastest, and deepest views of the night sky ever observed from Earth.

 

The Vera C. Rubin Observatory is a next-generation astronomical facility under construction in Chile funded by the U.S. National Science Foundation (NSF) and the U.S. Department of Energy (DOE). The successful coating of the 8.4-meter primary/tertiary mirror paves the way for the installation of the glass mirrors on the Simonyi Telescope, bringing Rubin Observatory ever closer to revolutionizing the fields of astronomy and astrophysics with its 10-year Legacy Survey of Space and Time (LSST) beginning in 2025. “This milestone represents not just an incredible feat of engineering, but also an important step towards a transformative new era of scientific advancement” said Edward Ajhar, NSF Program Director for Rubin Observatory.

 

Rubin Observatory’s primary/tertiary mirror — the only one in the world exactly like it — is an integral component of the telescope’s optical system, which also includes a 3.4-meter secondary mirror and the LSST Camera, the  largest digital camera in the world. Fabrication of the mirror began before the rest of the Rubin Observatory components, enabled by major gifts from the Charles Simonyi Fund for Arts and Sciences and from Microsoft founder Bill Gates. The 8.4-meter mirror is made up of two optical surfaces, each with a different curvature, combined into one large structure about as wide as a tennis court. Integrating the two mirrors in this way reduced the engineering and control complexity for the telescope while maintaining its excellent light collecting capacity. The mirror was fabricated over a period of seven years at the Richard F. Caris Mirror Lab (RFCML), of the University of Arizona, Tucson, AZ, beginning in 2007. In 2015, the completed mirror was moved to a secure storage area, and in early 2019 it was shipped to the summit facility on Cerro Pachón. 

 

“This moment, having a completed primary/tertiary mirror, has been decades in the making, starting with the gift of funding by Richard F. Caris to buy the glass from Ohara Corporation that was used to make the mirror blank. Everyone at RFCML and the University of Arizona that have been involved in this project are thrilled that our work on this unique mirror will soon contribute to the success of such an incredible scientific instrument,”said Professor Buell T. Jannuzi, Head of the Department of Astronomy and Director of Steward Observatory at the University of Arizona.

 

The mirror coating process was carried out safely and efficiently by a skilled team using a state-of-the-art, onsite coating chamber built specifically for Rubin Observatory by VON ARDENNE in Deggendorf, Germany. The 128-ton coating chamber, installed on the maintenance floor of the observatory facility, uses a technique called magnetron sputtering to coat mirrors to precise specifications. This technique gives Rubin the flexibility to coat the telescope mirrors with aluminum, silver, or even a combination of both during any coating run. The coating chamber can also be configured for either of Rubin Observatory’s differently-sized mirrors — it was also used to coat the 3.4-meter secondary mirror with protected silver in mid-2019. To coat the 8.4-meter primary/tertiary mirror, the lower half of the coating chamber was removed and the mirror’s vacuum-sealed support structure — called the mirror cell — acted as the base of the chamber.

 

“We’re thrilled that this very specialized piece of equipment has contributed to achieving the scientific requirements for both of Rubin Observatory’s mirrors,” said Norman Müller, project manager at VON ARDENNE, Germany. “Meeting the very demanding homogeneity requirements was definitely a challenge. But we were able to succeed thanks to our extensive experience in building vacuum coating equipment for large surfaces.”

 

The Rubin coating team, led by Tomislav Vucina, conducted extensive testing to determine the final coating “recipe” — the precise mixture of elements that make up the coating layers, with the goal of achieving the best possible combination of reflectivity and durability. To verify the performance of the chosen mixture, the team coated a steel stand-in mirror that has also been used for testing the telescope mount and other observatory components. After confirming the mixture met the defined requirements, they repeated the process using the glass mirror. 

 

First, the team applied an adhesion layer of nickel-chromium (NiCr) to the glass mirror blank. Then, they applied the reflective layer of silver (Ag). This reflective layer is incredibly thin — the amount of silver used to coat the entire 8.4-meter surface (64 grams) would form a ball about the size of a cherry tomato. After the application of the reflective layer, the mirror received another NiCr adhesion layer, and a final layer of silicon nitride (Si3N4) to protect the reflective coating from dust and other environmental contaminants. “This outer layer needs to be thick enough that it’s not worn off by cleaning,” said Vucina, “but not so thick that it absorbs too many photons and prevents the mirror from meeting Rubin’s scientific requirements.”

 

The process of coating the mirror took about 4 ½ hours. After the coating was complete, and to ensure that all the requirements were met, the mirror was moved out of the chamber to a nearby space where — the following day — Vucina and his team conducted a series of tests: reflectivity, adhesion, pinhole, and cosmetic.  After analyzing  the results of those tests, they declared the coating a success. “This was a very well-conducted project from every angle,” said Vucina, “thanks to a combination of careful planning and the technical skills of our excellent team.”

 

With its dazzling new coat, Rubin’s primary/tertiary mirror is an important step closer to capturing light from distant celestial objects. “We’re extremely excited that both mirrors are now coated and will be installed on the telescope very soon,” said Sandrine Thomas, Deputy Director for Rubin Construction. “The combined reflectivity of these mirrors will enable Rubin to detect very faint and far-away objects, leading to great science!”

 

About Rubin

 

Vera C. Rubin Observatory is a groundbreaking new astronomy observatory under construction on Cerro Pachón in Chile, with first light expected in early 2025. It’s named after astronomer Vera Rubin, who provided the first convincing evidence for the existence of dark matter. The 8.4-meter telescope at Rubin Observatory, equipped with the largest digital camera in the world, will take enormous images of the southern hemisphere sky, covering the entire sky every few nights. Rubin will do this over and over for 10 years, creating a timelapse view of the Universe that’s unlike anything we’ve seen before. Rubin Observatory’s 10-year survey is called the Legacy Survey of Space and Time (LSST).

 

Learn more about the Vera C. Rubin Observatory here.

 

 

More information

 

Vera C. Rubin Observatory is a Federal project jointly funded by the US National Science Foundation (NSF) and the US Department of Energy (DOE) Office of Science, with early construction funding received from private donations through the LSST Discovery Alliance. The NSF-funded Rubin Observatory Project Office for construction was established as an operating center under the 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 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 via NSF NOIRLab and DOE’s SLAC.