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Credit: Rubinobs/Noirlab/Slac/NSF/Doe/Aura/b. Quint
A main milestone with the Vera C. Rubin Observatory was reached by installing the enormous list of the telescope – the last optical component that is required before the start of the last test phase.
The LSS camera (car size), recently installed on Vera C. Rubin Observatory, is the largest digital camera that records detailed images of the sky of the southern hemisphere over a decade.
“The installation of the LSST camera at the telescope is a triumph of science and engineering,” said Harriet Kung, acting director of the Ministry of Science of the Energy Ministry in an explanation. “We look forward to seeing the unprecedented pictures that this camera is created.”
The NSF -Doe Vera C. Rubin Observatory team installs the LSST camera in the Simonyi Survey Telescope in March 2025 | Credit: Rubinobs/Noirlab/Slac/NSF/Doe/Aura/b. Quint
The telescope is financed by the US National Science Foundation and the US Ministry of Health and according to Dr. Vera C. Rubin named, an American astronomer whose work provided strong evidence of the existence of dark matter. Together with her colleague Kent Ford, Rubin observed that the stars on the outer edges moved as quickly as those near the center in the numerous galaxies they examined. This was unusual, since according to Newton’s physics and Kepler, laws of the planetary movement should continue to circle the center of a gravitational system more slowly due to the weaker gravitational suit.
After taking all visible matter into account, the gravitational force of the observed mass was not sufficient to keep these rapidly moving stars bound to the galaxy. Without an additional mass that delivers additional gravitational tendencies, the galaxies should fly apart. This discrepancy led to the conclusion that an invisible form of the mass, which is now known as a dark matter, gave it together.
After its namesake, the ruby telescope examines the secrets of dark energy and dark matter with the latest technology. Its state -of -the -art mirror design, the highly sensitive camera, the quick survey speed and the advanced computer infrastructure represent breakthroughs in their respective fields.
The NSF -Doe Vera C. Rubin Observatory team installs the LSST camera in the Simonyi Survey Telescope in March 2025 | Credit: Rubinobs/Noirlab/Slac/NSF/Doe/Aura/b. Quint
Every few nights it will examine the entire sky and create an “ultra-wide, ultra-high-definition time-lapse record of the universe” adds the explanation. Each picture is so solid that displaying 400 ultra -high definition television screens is required.
“This unique film will bring the night sky to life and bring a treasure trove of discoveries: asteroids and comets, pulsating stars and supernova explosions,” says the Observatory website.
While the LSST camera is a technical miracle, its installation was equally difficult. In March 2025, the Summit team used a vertical platform elevator after months of testing in the Clean Room of Rubin Observatory to move the camera onto the telescopic floor. A custom lifting device then positioned it carefully and for the first time attached it to the telescope.
The NSF -Doe Vera C. Rubin Observatory team installs the LSST camera in the Simonyi Survey Telescope in March 2025 | Credit: Rubinobs/Noirlab/Slac/NSF/Doe/Aura/b. Quint
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“The assembly of the LSST camera on the Simonyi telescope was an effort for intensive planning and teamwork in the entire execution of observatories and millimeter precision,” said Freddy Muñoz, mechanical group leadership of Rubin Observatory. “The LSST camera to observe that you take your place in the telescope is a proud moment for all of us.”
In the coming weeks, the service programs and systems of the LSST camera will be connected and tested. Soon it will be ready to take detailed pictures of the night sky. The ruby telescope in Cerro Pachón, Chile, under construction is expected to see the first light in 2025.