After two decades of work, scientists and engineers at the Department of Energy's SLAC National Accelerator Laboratory and their collaborators are celebrating the completion of the Legacy Survey of Space and Time (LSST) Camera.
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As the heart of the Vera C. Rubin Observatory, the 3,200-megapixel camera will help researchers observe our universe in unprecedented detail. Over 10 years, it will generate an enormous trove of data on the southern night sky that researchers will mine for new insights into the universe.
That data will aid in the quest to understand dark energy, which is driving the accelerating expansion of the universe, and the hunt for dark matter, the mysterious substance that makes up about 85% of the matter in the universe.
Researchers also have plans to use Rubin data to better understand the changing night sky, the Milky Way galaxy, and our own solar system.
To achieve that goal, the SLAC team and its partners built the largest digital camera ever constructed for astronomy. The camera is roughly the size of a small car and weighs about 3,000 kilograms (3 metric tons), and its front lens is more than 5 feet across—the largest lens ever made for this purpose.
Another 3-foot-wide lens had to be specially designed to maintain shape and optical clarity while also sealing the vacuum chamber that houses the camera's enormous focal plane.
That focal plane is made up of 201 individual custom-designed CCD sensors, and it is so flat that it varies by no more than a tenth the width of a human hair. The pixels themselves are only 10 microns wide.
Still, the camera's most important feature is its resolution, which is so high it would take hundreds of ultra-high-definition TVs to display just one of its images at full size, said SLAC professor and Rubin Observatory Deputy Director and Camera Program Lead Aaron Roodman.
"Its images are so detailed that it could resolve a golf ball from around 15 miles away, while covering a swath of the sky seven times wider than the full moon. These images with billions of stars and galaxies will help unlock the secrets of the universe."
Now that the LSST Camera is complete and has been thoroughly tested at SLAC, it will be packed up and shipped to Chile and driven up 8,900-foot-high Cerro Pachón in the Andes, where it will be hoisted atop the Simonyi Survey Telescope later this year.
Once it's up and running, the camera's essential purpose is to map the positions and measure the brightness of a vast number of night-sky objects. From that catalog, researchers can infer a wealth of information.
Perhaps most notably, the LSST Camera will look for signs of weak gravitational lensing, in which massive galaxies subtly bend the paths light from background galaxies take to reach us.
Weak lensing reveals something about the distribution of mass in the universe and how that's changed over time, which will help cosmologists understand how dark energy is driving the expansion of the universe.
Scientists also want to study patterns in the distribution of galaxies and how those have changed over time, identifying clusters of dark matter and spotting supernovae, all of which can help further understanding of dark matter and dark energy alike.
The same images that reveal details of distant galaxies will help researchers study something closer to home: our own Milky Way galaxy.
Many of its stars are small and faint, but with the LSST Camera's sensitivity, researchers expect to produce a far more detailed map of our galaxy, yielding insights into its structure and evolution as well as the nature of stars and other objects within it.
Even closer to home, researchers are hoping to create a far more thorough census of the many small objects in our solar system.
According to Rubin Observatory estimates, the project may increase the number of known objects by a factor of 10, which could lead to a new understanding of how our solar system formed and perhaps help identify threats from asteroids that get a little too close to the planet.
Finally, Rubin scientists will look at how the night sky is changing—for example, how stars die or how matter falls into supermassive black holes at the centers of galaxies.
Among the partner labs that contributed expertise and technology are Brookhaven National Laboratory, which built the camera's digital sensor array; Lawrence Livermore National Laboratory, which with its industrial partners designed and built lenses for the camera; and the National Institute of Nuclear and Particle Physics at the National Center for Scientific Research (IN2P3/CNRS) in France, which contributed to sensor and electronics design and built the camera's filter exchange system, which will allow the camera to home in on six separate bands of light from the ultraviolet to infrared.
A key feature of the camera's optical assemblies are its three lenses, one of which at 1.57 meters (5.1 feet) in diameter is believed to be the world's largest high-performance optical lens ever fabricated. ■