How did the Milky Way form? What constitutes 95% of the Universe that remains unseen? What insights will a detailed inventory of Solar System objects provide?
These are just a few of the questions that the U.S. National Science Foundation (NSF) and the U.S. Department of Energy (DOE) aim to explore through the Legacy Survey of Space and Time over the next decade.
At an event in Washington, D.C., the NSF–DOE Vera C. Rubin Observatory released its first imagery, showcasing cosmic phenomena captured at an unprecedented scale.
This imagery serves as a preview of Rubin Observatory's forthcoming ten-year scientific mission to explore and understand some of the Universe's biggest mysteries.
The Rubin Observatory's primary mission is the Legacy Survey of Space and Time, which will continuously scan the night sky for ten years, capturing every visible change that occurs.
After more than two decades of dedicated work, the Rubin Observatory is now located at the summit of Cerro Pachón in Chile, an ideal observing site due to its dry air and dark skies.
The observatory features an innovative 8.4-meter telescope equipped with the largest digital camera ever constructed, which provides data for a powerful processing system.
This ultra-wide, ultra-high-definition time-lapse record of the Universe will uncover a treasure trove of scientific discoveries.
The images collected will reveal asteroids, comets, pulsating stars, supernova explosions, distant galaxies, and potentially new cosmic phenomena that have never been witnessed before.
The observatory is named in honor of the pioneering U.S. astronomer Vera C. Rubin, who provided conclusive evidence for the existence of vast quantities of invisible material known as dark matter.
Understanding dark matter, dark energy, and other significant cosmic mysteries is central to the Rubin Observatory's mission.
Dark energy refers to the mysterious force that appears to be causing galaxies in the Universe to move away from one another at an accelerating rate.
Though dark matter and dark energy together comprise 95% of the Universe, their properties remain largely unknown.
Rubin will take approximately a thousand images of the Southern Hemisphere sky every night, allowing it to cover the entire visible Southern sky every three to four nights.
Through this approach, it will identify millions of unseen asteroids, comets, and interstellar objects.
The Rubin Observatory is a game changer for planetary defense, as it will be able to detect far more asteroids than ever before, potentially identifying some that may pose a risk to Earth or the Moon.
The observatory operates as a joint program of NSF's NOIRLab and the DOE's SLAC National Accelerator Laboratory. NOIRLab is managed by the Association of Universities for Research in Astronomy (AURA).
Rubin Observatory also aims to enhance public engagement through an online platform, developed by a team of astronomers, educators, and web design experts.
This platform will provide educators and students worldwide with tools and activities, enabling them to interact with a selection of Rubin Observatory data.
Additionally, the First Look images from Rubin Observatory have been shared with more than 300 public and private watch parties hosted by partner institutions, planetariums, observatories, museums, libraries, amateur astronomy societies, schools, and universities worldwide.