Skip to main content

The world’s largest digital camera for astronomy is ready to go

Ready to scan the night sky to look for evidence of dark matter, identify near-Earth asteroids, and much more, the camera for the upcoming Vera Rubin Observatory is now complete. This is the world’s largest digital camera for astronomy, with a staggering 3,200 megapixels, and it will be placed in the Rubin Observatory in Chile.

Photograph of the camera, with one of the colour filters positioned in place.
Photograph of the camera, with one of the color filters positioned in place. Olivier Bonin/SLAC National Accelerator Laboratory

The camera is vast, weighing around 3 metric tons, making it about the same size and mass as a small car. With a huge front lens that is 5 feet across, it will be able to take incredibly detailed images of large sections of the sky. Built at the Department of Energy’s SLAC National Accelerator Laboratory (SLAC), it will be used for the Legacy Survey of Space and Time (LSST), a 10-year project to image the southern sky and spot transient objects like supernovae.

“With the completion of the unique LSST Camera at SLAC and its imminent integration with the rest of Rubin Observatory systems in Chile, we will soon start producing the greatest movie of all time and the most informative map of the night sky ever assembled,” said Director of Rubin Observatory Construction, Željko Ivezić of the University of Washington, in the statement.

The huge scale of the camera makes it incredibly powerful, able to capture a very wide field of view (meaning it can take in a large portion of the sky with each observation) and to resolve very fine detail.

“Its images are so detailed that it could resolve a golf ball from around 25 kilometers (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,” said SLAC professor and Rubin Observatory Deputy Director and Camera Program Lead Aaron Roodman.

The camera has been tested at SLAC and is now ready to be shipped to Chile, where it will be installed onto the Simonyi Survey Telescope later this year. This telescope, as part of the Rubin Observatory, is located at the top of the Cerro Pachón mountain — a location that brings some challenges to installation.

Rubin is set to begin its survey in 2025 when it will scan the sky to learn about the movements of distant galaxies to help uncover information about dark matter and other key topics in astronomy.

“More than ever before, expanding our understanding of fundamental physics requires looking farther out into the universe,” said Kathy Turner, program manager for the DOE’s Cosmic Frontier Program. “With the LSST Camera at its core, Rubin Observatory will delve deeper than ever before into the cosmos and help answer some of the hardest, most important questions in physics today.”

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Biggest stellar black hole to date discovered in our galaxy
Astronomers have found the most massive stellar black hole in our galaxy, thanks to the wobbling motion it induces on a companion star. This artist’s impression shows the orbits of both the star and the black hole, dubbed Gaia BH3, around their common centre of mass. This wobbling was measured over several years with the European Space Agency’s Gaia mission. Additional data from other telescopes, including ESO’s Very Large Telescope in Chile, confirmed that the mass of this black hole is 33 times that of our Sun. The chemical composition of the companion star suggests that the black hole was formed after the collapse of a massive star with very few heavy elements, or metals, as predicted by theory.

Black holes generally come in two sizes: big and really big. As they are so dense, they are measured in terms of mass rather than size, and astronomers call these two groups of stellar mass black holes (as in, equivalent to the mass of the sun) and supermassive black holes. Why there are hardly any intermediate-mass black holes is an ongoing question in astronomy research, and the most massive stellar mass black holes known in our galaxy tend to be up to 20 times the mass of the sun. Recently, though, astronomers have discovered a much larger stellar mass black hole that weighs 33 times the mass of the sun.

Not only is this new discovery the most massive stellar black hole discovered in our galaxy to date but it is also surprisingly close to us. Located just 2,000 light-years away, it is one of the closest known black holes to Earth.

Read more
Watch how NASA plans to land a car-sized drone on Titan
An artist's impression of NASA's Dragonfly drone.

 

A decision by NASA this week paved the way for the Dragonfly drone mission to continue to completion.

Read more
See a flyby of Io, a hellish moon with lakes of lava and an otherworldly mountain
The JunoCam instrument on NASA’s Juno captured this view of Jupiter’s moon Io — with the first-ever image of its south polar region — during the spacecraft’s 60th flyby of Jupiter on April 9.

NASA's Juno mission is best known for the gorgeous images of Jupiter that it has taken since its launch in 2011 and arrival at Jupiter in 2016. But the spacecraft hasn't only investigated the planet -- it has also studied Jupiter's many moons, like the large Ganymede and the icy Europa. Recently, the spacecraft has been making close flybys of the Jovian moon Io, which is the most volcanically active body in the solar system. And it has observed some dramatic features there, like a lake of lava and a large mountain.

Even though Jupiter (and Io) are both far from the sun, and therefore receive little heat from sunlight, Io still has high internal temperatures. That's because Jupiter is so large that its gravitational pull acts on Io and creates friction, heating it up in a process called tidal heating. Though the surface of the moon is cold, at below minus 200 degrees Fahrenheit (minus 130 degrees Celsius), the volcanoes spewing out material from the planet's hot interior can reach temperatures of thousands of degrees Fahrenheit.

Read more