THE INSTRUMENT
Rubin's 8.4-meter mirror feeds the largest digital camera ever built — 3.2 gigapixels, the size of a small car. A single exposure covers 40 times the area of the full moon. The whole southern sky is reimaged every three to four nights.
WHY A SURVEY, NOT A TARGET
Traditional telescopes point at one object on request. Rubin does the opposite: it stares at everything, all the time, building a time-lapse of the universe. The science isn't in any single image — it's in the differences between tonight's image and last week's.
THE NAMESAKE
Vera Rubin's 1970s observations of galaxy rotation curves showed stars at the edges of galaxies orbiting as fast as those near the center — physically impossible unless vast invisible mass surrounded them. Her work made dark matter undeniable. The telescope bearing her name is built to map exactly that invisible structure.
DARK ENERGY, THE TARGET
Roughly 68% of the universe is dark energy — the unknown force accelerating cosmic expansion. Rubin will measure how galaxy clusters grew over billions of years, and the growth rate constrains what dark energy actually is. This is the single largest open question in physics.
INTERSTELLAR VISITORS
Until 2017, no object from outside the solar system had ever been observed. Then ʻOumuamua appeared, followed by comet Borisov in 2019. Rubin is expected to find dozens per year — a sample size that turns interstellar objects from curiosities into a population to study.
THE DATA FIREHOSE
Every night Rubin generates ~20 terabytes of images and roughly 10 million alerts — notifications that something in the sky changed. No human can review that volume; the pipeline is built around machine classifiers that route alerts to brokers for follow-up within 60 seconds.