The New 8.4-meter Simonyi Survey Telescope in Chile | Vera C. Rubin Observatory
The 8.4-meter Simonyi Survey Telescope features a unique three-mirror design. This gives the telescope an exceptionally wide field of view, while maintaining a compact shape that allows it to move quickly across the sky. The design and construction of Rubin Observatory took more than a decade.
The Simonyi Survey Telescope is named after Charles Simonyi's family, in recognition of his significant gift early in the construction phase in support of the design, development, and fabrication of the telescope’s primary mirror.
A team of engineers and technicians at SLAC National Accelerator Laboratory constructed the LSST Camera.
The focal plane consists of 189 charge-coupled device (CCD) sensors arranged on 21 “rafts” for a combined 3200 megapixels.
Every night, Rubin Observatory’s intricate data network, designed and built by a distributed team of data management experts, will move 20 terabytes of data from the summit of Cerro Pachón in Chile to the US Data Facility and then to other data processing facilities around the world.
Rubin Observatory is supported by funding from the US National Science Foundation (NSF) and the US Department of Energy (DOE). Rubin Observatory is operated by NSF’s NOIRLab and SLAC National Accelerator Laboratory.
Credit: RubinObs/NOIRLab/SLAC/NSF/DOE/AURA/H. Stockebrand
Release Date: Oct. 28, 2024
#NASA #Astronomy #Space #Science #VeraRubinObservatory #SimonyiSurveyTelescope #Telescope #OpticalTelescope #LSSTCamera #CCD #Cosmos #Universe #CerroPachón #Chile #NOIRLab #NSF #AURA #DOE #SLAC #UnitedStates #STEM #Education
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