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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ALT A dense field of countless pinpoint stars fills the frame against the deep black of space, creating a fine, grainy texture like fine sand spread across a smooth table. Dozens of particularly bright stars in blue, yellow, and orange glitter across the scene like jewels.
Wispy, grayish clouds of galactic dust drift across the center and right sides of the image, appearing soft and powder-like against the dark background.
Scattered throughout the entire scene are stars and faint objects in shades of blue, yellow, and red. Some appear as sharp, solid points, while others are soft, diffuse smudges. Zooming in reveals that many of these tiny, faint smudges scattered between the stars are actually distant galaxies, varying from smooth, pebble-like blobs to faint, stretched lines.
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
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
ALT Wide starfield with pink and blue nebulae, including the Lagoon and Trifid Nebulae, with three white numbered boxes marking regions.
🔎 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🐉
ALT Colorful nebula in a dense star field, with a glowing pink core, blue gas clouds, and dark dust lanes branching outward.
ALT Pink and white glowing nebula filled with stars, with wispy gas clouds and dark dust lanes swirling across space.
ALT Pink and blue nebula clouds fill a star-dense sky, threaded with dark dust lanes and scattered bright stars.
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!
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🌌
ALT A stunning night sky showcasing the vibrant, colorful Milky Way galaxy arching above a boot-shaped observatory on a hill, with countless stars and cosmic dust visible in the clear atmosphere.
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.
ALT Vast star field with numerous bright stars and distant galaxies of various shapes, sizes, and colors. On the left, a ghostly haze of galactic cirrus drifts like cotton candy.
ALT A wide, panoramic view of a dense field of countless tiny, pinpoint stars filling the entire frame like fine dust. Wispy, faint, grayish-brown clouds of galactic cirrus drift across the scene, creating a patchy texture over the dark background. Several brighter stars stand out across the field, most notably a large blue star on the upper right surrounded by a glowing halo, along with a few other scattered blue and orange stars. A white rectangle at upper center highlights a specific area.
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.
ALT Observatory perched atop a rocky mountain with layered hills fading into the distance under a golden sunset sky.
ALT Sunset casting warm orange light over high desert mountains with an observatory perched on a ridge at left.
ALT Rubin Observatory perched atop its mountain summit site on Cerro Pachón. The observatory is boot-shaped at lower left with long white service building extending left and silver dome sticking up. The dome's vertical slit is open, revealing the telescope in the blackness within. The night sky is peppered with the pinpricks of stars. The Little Beehive Cluster of stars is a denser collection of pinpricks to the upper right of the observatory.
ALT Illustration showing smooth ocean air flowing over a mountain, with turbulence forming on the mountain's opposite side. Two insets show the impact of turbulence on an image of a star: without turbulence the star is sharp, while with turbulence it's blurred. Text reads "A site chosen for steady air. Smooth, stable air flows in from the ocean..then gets disrupted by mountains, creating turbulence."
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.
ALT Large observatory with open dome on rocky terrain under a pink and purple twilight sky.
ALT A large boot-shaped observatory on the left and small cylindrical dome on the right, both perched on rocky hills under a vibrant pink and purple sunset sky.
ALT Boot-shaped observatory building against a gradient sky transitioning from orange up to deep purple.
ALT White astronomical observatory dome with closed shutter against a pink and blue twilight sky with pink sunset clouds.
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.
ALT Spiral galaxy with bright core and swirling arms surrounded by numerous distant stars and galaxies in deep space.
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.
ALT Vast star field with countless stars and galaxies scattered across a dark cosmos with wispy clouds of interstellar dust filling the scene. There's a small white square highlighting a specific galaxy left of center.
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!🌌
ALT Large boot-shaped observatory building under a clear star-filled night sky on a mountain. The glowing band of the Milky Way stretches low and parallel to the horizon on the left, while the faint, barely-there haze of zodiacal light stretches diagonally up and right.
"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
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
ALT Dense starfield with faint clouds of interstellar dust, filled with white, orange, and blue stars. A few brighter blue and orange stars stand out. A horizontal palette bar at the bottom shows blue, gray, orange, brown, and cream swatches.
ALT A large pink-red nebula cloud with dark dust lanes at center-left and a smaller blue-pink nebula upper right in a dense, tan Milky Way star field. Bottom palette strip shows pink, slate blue, orange, tan, and brown swatches.
ALT Deep field packed with faint galaxies and stars. A few bright blue and orange foreground stars stand out among thousands of galaxies of varying shapes, sizes, and colors. A color palette strip at bottom shows black, dark blue, beige, tan, and gray swatches.
ALT Deep field packed with faint galaxies and stars. Bright blue and orange foreground stars show diffraction spikes. Large elliptical galaxies cluster at left and right amid thousand of other galaxies of varying shapes, sizes, and colors. A color palette strip runs along the bottom showing tan, light blue, bright blue, red, and black.
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.
ALT A "selfie" from two workers wearing helmets and safety vests using Rubin's primary mirror. They're standing on a metal platform with metal structural beams reflected behind them.
ALT Five workers wearing safety gear inside Rubin's dome next to a curved concrete wall.
ALT A person in red safety gear and yellow helmet laying on a platform while working on Rubin's giant digital camera.
ALT Two people working on computers in an office with safety hard hats and high-visibility vests nearby.
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! 🔧🔭
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.
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!
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