Rubin will #CaptureTheCosmos in exquisite detail starting in 2026 🌌 Funded by @NSF and @DOEScience. Para español: instagram.com/rubin_observat…

Cerro Pachon, Chile
A new view of a familiar field 🤩 Meet NSF–DOE Rubin Observatory's breathtaking view of the renowned COSMOS field🌀✨ rubinobservatory.org/news/ru… 🧵
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Zoom in for millions of galaxies 🌌 This is NSF–DOE Rubin Observatory’s view of the Virgo Cluster, a bustling neighborhood of galaxies in various shapes, sizes, & colors. In all, there are over 10 million galaxies in this view 🤯 🎥: NSF–DOE Rubin Observatory/NOIRLab/SLAC/AURA
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Not everything in the Universe glows… This spooky season, we're exploring the darker corners of NSF–DOE Rubin's Observatory's view of the Trifid and Lagoon Nebulae. 🌌 Dark nebulae are dense clouds of gas and dust that block the light from behind, creating inky silhouettes
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🔎 A few spots to find: 1️⃣ Barnard 85: Splits the bright Trifid Nebula into three distinct sections, giving it its name. 2️⃣ Barnard 89: A particularly dark patch of dust lurking among the stars. 3️⃣ Barnard 302 and 303: These dust clouds trace a winding, dragon-like shape🐉
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📷: NSF–DOE Rubin Observatory/NOIRLab/SLAC/AURA
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We recently had a couple of very special visitors at NSF–DOE Rubin Observatory: Andean condors! 🦅 They're some of the largest flying birds on Earth, with wingspans more than 10 feet (3 m). Soaring with air currents, they can go huge distances while barely flapping their wings!
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A night at NSF–DOE Rubin Observatory✨ Beneath the Milky Way, Rubin shares the scene with the Large and Small Magellanic Clouds and the faint red Cobold Nebula. Over the next decade, Rubin will scan this sky over and over, building an ever-deeper view of the changing Universe🌌
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Spooky vibes for spooky month👻🌌 The more you look at this region of NSF–DOE Rubin Observatory’s Ocean of Stars, the more emerges. Wispy galactic cirrus veils stars & distant galaxies, while thousands of spiral galaxies, smooth galaxies, & more lurk in the depths.
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While mountains give us high-altitude dark skies, they disrupt smooth airflow, forcing the air to break into turbulent pockets. This atmospheric jitter is called "seeing." NSF–DOE Rubin Observatory was intentionally built where coastal airflow passes smoothly over the ridge.
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It's October 3rd, so we're wearing pink! 🌸 On Cerro Pachón in Chile, nature puts on its own show during twilight, painting the sky and NSF–DOE Rubin Observatory in glowing pink. We can't really enforce a dress code for the cosmos, but the Chilean skies clearly got the memo.
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If galaxies had signature dance moves, this one's would be the spiral swirl 💃🌀 Meet Z 36-24, a barred spiral galaxy with two swirly arms. Bars are a common feature in spiral galaxies, where the arms connect to a straight bar of stars across its center.
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Z 36-24 is in the COSMOS field, one of the most studied patches of sky. NSF–DOE Rubin Observatory's deep view reveals hundreds of thousands of galaxies here. By repeatedly observing the sky, Rubin will help scientists track huge populations of active galaxies over time.
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Explore this galaxy (and many more!) in Skyviewer: skyviewer.app/explorer?targe… 📷: NSF–DOE Rubin Observatory/NOIRLab/SLAC/AURA
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Not a bad office view🌌 In this image of NSF–DOE Rubin Observatory, we see the Milky Way plus the ghostly glow of zodiacal light caused by sunlight reflecting off dust in the Solar System. Zodiacal light is super faint, but Cerro Pachón's dark skies make it possible to see!🌌
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"Let's just take a closer look." Famous last words. NSF–DOE Rubin Observatory images reveal stars, nebulae, and a mindblowing number of distant galaxies hiding in the background. So go ahead. Zoom in. You might want to clear your schedule. ➡️ skyviewer.app
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Choose your favorite NSF–DOE Rubin Observatory palette!🎨 Rubin sees a wider range of colors than our eyes, & when mapped to colors we see: 🔴 Redder galaxies are farther 🔵 Blue stars are hotter 🌈 In the Trifid & Lagoon Nebulae, pink traces hydrogen while blue shows hot stars
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Welcome to Chile, @SLACLab LSST Camera team colleagues! They arrived from California last week for scheduled camera work during NSF–DOE Rubin Observatory’s planned engineering downtime. This engineering period will last about three weeks in total.
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Planned engineering periods are common in ground-based astronomy, especially in winter when the weather is less favorable. During this time, teams will do maintenance and other work that keeps the observatory running smoothly during the rest of the year! 🔧🔭
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📸: NSF–DOE Rubin Observatory/NOIRLab/SLAC/AURA/T. Lange
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Imagine looking up and watching a star suddenly lose 99% of its light. These stars are a rare type of variable star called an R Coronae Borealis. They suddenly puff out huge clouds of dust, blocking nearly all their light for months before returning to normal.
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We can't see inside stars — we really can only observe the light coming from their surfaces. But when a star changes in brightness, it can reveal clues about what's happening deep inside. That's why scientists are so interested in variable stars!
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NSF–DOE Rubin Observatory will detect ~100 million variable stars during its 10-year survey, helping scientists uncover why some stars stay steady for billions of years while others rewrite the rules! 🎥: NSF–DOE Rubin Observatory/NOIRLab/SLAC/AURA
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