Tag: Rubin Observatory

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This asteroid is spinning fast enough to set a record

Illustration: Fast-spinning asteroid surrounded by other space rocks
An artist’s conception zeroes in on asteroid 2025 MN45. (Credit: NSF-DOE Vera C. Rubin Observatory / NOIRLab / SLAC / AURA / P. Marenfeld)

Astronomers say they’ve found an asteroid that spins faster than other space rocks of its size.

The asteroid, known as 2025 MN45, is nearly half a mile (710 meters) in diameter and makes a full rotation every 1.88 minutes, based on an analysis of data from the Vera C. Rubin Observatory. “This is now the fastest-spinning asteroid that we know of, larger than 500 meters,” University of Washington astronomer Sarah Greenstreet said today at the American Astronomical Society’s winter meeting in Phoenix.

Greenstreet, who serves as an assistant astronomer at the National Science Foundation’s NOIRLab and heads the Rubin Observatory’s working group for near-Earth objects and interstellar objects, is the lead author of a paper in The Astrophysical Journal Letters that describes the discovery and its implications. It’s the first peer-reviewed paper based on data from Rubin’s LSST Camera in Chile.

2025 MN45 is one of more than 2,100 solar system objects that were detected during the observatory’s commissioning phase. Over time, the LSST Camera tracked variations in the light reflected by those objects. Greenstreet and her colleagues analyzed those variations to determine the size, distance, composition and rate of rotation for 76 asteroids, all but one of which are in the main asteroid belt between the orbits of Mars and Jupiter. (The other asteroid is a near-Earth object.)

The team found 16 “super-fast rotators” spinning at rates ranging between 13 minutes and 2.2 hours per revolution — plus three “ultra-fast rotators,” including 2025 MN45, that make a full revolution in less than five minutes.

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Astronomers hail observatory’s debut — and look ahead

Zeljko Ivezic with picture of Rubin Observatory
University of Washington astronomer Zeljko Ivezic talks about the Rubin Observatory in front of a photo of Rubin. (GeekWire Photo / Alan Boyle)

It’s been more than two decades since the University of Washington helped kick off the effort to get the Vera C. Rubin Observatory built in Chile — and now that it’s finished, UW astronomers are gearing up to get in on the first decade of discoveries.

The university’s role in the past, present and future of the Rubin Observatory and its 10-year Legacy Survey of Space and Time, or LSST, literally took center stage in front of a packed house at UW’s Kane Hall on June 26.

UW astronomer Zeljko Ivezic, who served as director of Rubin construction and is shifting his focus to his role as head of science operations for LSST, recalled the night of April 15, when Rubin’s first test images came in for fine tuning.

“We were all so happy, and we are still happy,” he said. “We had been dreaming about this night for two decades, and it finally arrived. And not only that, we quickly obtained beautiful data, but also we continued to do so, and every new image was better and better. The observatory is performing beyond all our expectations.”

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Rubin Observatory makes discoveries in its debut

This image shows a small section of the Rubin Observatory’s view of the Virgo Cluster, including two spiral galaxies at lower right, three merging galaxies at upper right, several groups of distant galaxies and many stars in our own Milky Way galaxy. Click for a larger version of the image. (Credit: NSF-DOE Vera C. Rubin Observatory)

After more than 20 years of planning and construction, astronomers celebrated the release of the first images from the Vera C. Rubin Observatory today — and also registered hundreds of the first discoveries from the world’s newest eye on the sky.

University of Washington astronomer Mario Juric, a member of the Rubin team and director of UW’s DiRAC Institute, said that discovery data for 2,104 previously undetected small bodies in the solar system were reported to the Minor Planet Center early today.

Those small bodies include 2,015 main-belt asteroids, nine trans-Neptunian objects and seven near-Earth objects. (But don’t worry: None of those NEOs has a chance of hitting Earth anytime soon.)

“The over 2,100 asteroids we discovered are impressive, but just a drop in the bucket relative to what’s coming. We’ll have moments where we find over 20,000 in a single night, more than the entire world presently finds in a year,” Juric told me in an email.

“By sometime next year Rubin will double the number of known asteroids, then continue to discover hundreds of new comets, the remaining few dwarf planets, and maybe even a new planet in our solar system,” he said. “This will be the most comprehensive census of our planetary home in history.”

During today’s “First Look” briefing in Washington, D.C., astronomers explained the science behind their scan for asteroids — and showed off eye-pleasing imagery that included a colorful wide-angle view of the Trifid and Lagoon nebulas in the constellation Sagittarius, galactic closeups gleaned from the observatory’s survey of the Virgo Cluster, and a zooming video scan of the same region of the sky.

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Rubin Observatory throws a party to reveal first pictures

Long-exposure image of Rubin Observatory against night sky filled with star trails
A long-exposure image shows the Rubin Observatory beneath star trails. (Credit: Hernan Stockebrand via Rubin Observatory)

After more than 20 years of planning and construction, the Vera C. Rubin Observatory is ready for its grand opening, and the world is invited.

The observatory in the foothills of the Chilean Andes features a monster of a telescope, with an 8.4-meter-wide (28-foot-wide) mirror, coupled with what’s said to be the world’s largest digital camera.

It will survey the night sky every night for at least 10 years, producing about 20 trillion bytes of data every 24 hours. It would take you more than three years of watching Netflix, or over 50 years of listening to Spotify, to use that amount of data, according to the Rubin team.

The first images and videos are due to be unveiled on June 23, during a “First Look” webcast that will be shared online and at more than 300 in-person watch parties across the globe.

What will the images look like? Mario Juric knows, but he isn’t telling.

“I cannot tell you what’s on them, but I can tell you we just finished them, and they look amazing,” Juric, a member of the Rubin team and the director of the University of Washington’s DiRAC Institute, says on the Fiction Science podcast. “I did not spend a day doing what I was supposed to be doing, because I just spent it browsing through the images. … I could teach an entire class by just zooming in on different parts of this image and explaining what this object is.”

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Software predicts a bonanza of solar system discoveries

Visualization of Rubin Observatory's solar system observations
A computer visualization maps small bodies in the solar system that are expected to be observed by the Rubin Observatory during its 10-year sky survey. Red indicates near-Earth objects, gold indicates main-belt asteroids, light purple indicates Jupiter Trojan asteroids, and deep blue indicates trans-Neptunian objects. The left image looks down from above the ecliptic plane, and the right image provides a side view. (Credit: Kurlander et al. / Sorcha.space / Univ. of Washington)

A new type of computer simulation predicts that the Vera C. Rubin Observatory in Chile will discover millions of previously undetected objects in the solar system over the course of the coming decade.

The discovery campaign, which is due to begin in earnest later this year, should expand the known small-body populations in the solar system by a factor of four to nine, said University of Washington astronomer Mario Juric, a member of the research team behind the open-source Sorcha simulation software.

“With this data, we’ll be able to update the textbooks of solar system formation and vastly improve our ability to spot — and potentially deflect — the asteroids that could threaten Earth,” Juric said today in a news release.

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Astronomers process test images at Rubin Observatory

Rubin Observatory's LSST Camera
The Rubin Observatory’s LSST Camera is the size of a small car. (Credit: Rubin Observatory / NOIRLab / SLAC / NSF / DOE / AURA / F. Munoz)

The Vera C. Rubin Observatory in Chile has begun generating test images of the night sky, thanks to the Simonyi Survey Telescope and its giant camera as well as a data management team that includes scientists from the University of Washington.

Team members started taking on-sky engineering data with Rubin’s LSST Camera on April 15, according to an update posted to an online forum for the Rubin Observatory research community by Keith Bechtol, a physicist at the University of Wisconsin at Madison.

“The Data Management system successfully transported and processed the 3-gigapixel images at the US Data Facility within about a minute of acquisition,” Bechtol wrote. “The distributed Rubin team was jubilant, taking a few moments to celebrate the first few data acquisitions, and then quickly got back to work.”

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Rubin Observatory’s monster telescope takes shape

Rubin Observatory telescope mount assembly
The Simonyi Survey Telescope now has its mirrors and a camera in place. (Credit: Rubin Observatory)

The Vera C. Rubin Observatory’s 8.4-meter Simonyi Survey Telescope in Chile has now been equipped with all three of its mirrors, plus a camera for good measure.

Last week’s installation of the telescope’s combined primary/tertiary mirror represented a major milestone in the observatory’s 15-year-long design and construction effort.

“We have a telescope!” the observatory team declared in updates posted to Instagram, Threads, BlueSky and X / Twitter.

The wide-field survey telescope, which is named after Microsoft software pioneer Charles Simonyi, is expected to shed light on astronomical mysteries ranging from the nature of dark energy and dark matter to the potential existence of an as-yet-unseen “Planet X” in the far reaches of our solar system.

The telescope’s 8.4-meter-wide (27.5-foot-wide) primary/tertiary mirror makes use of a continuous surface with different curvatures that are designed to optimize image resolution inside a relatively compact support structure. The 3.4-meter-wide (11-foot-wide) secondary mirror was installed in July.

When it’s fully up and running, the Simonyi Survey Telescope is expected to generate 20 terabytes of data every night. But the current version of the telescope isn’t yet ready for prime time.

“This iteration has the commissioning camera — a smaller 144-megapixel version of Rubin’s huge, 3,200-megapixel camera — which is used for testing and troubleshooting,” the observatory team noted. “Rubin’s LSST Camera, the biggest digital camera in the world that will #CaptureTheCosmos in science operations, will be installed early next year after our summit staff complete the next round of tests.”

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Get a wide-angle view of the Simonyi Survey Telescope

Simonyi Survey Telescope at the Rubin Observatory
The Vera C. Rubin Observatory’s Simonyi Survey Telescope will make use of an 8.4-meter primary mirror and an 3.5-meter secondary mirror. Note the size of the support structure compared with the size of the workers on the platform. (Credit: Rubin Observatory / NSF / AURA / F. Munoz Arancibia)

Hubble. Webb. Chandra. Spitzer. Rubin. Roman. And now, Simonyi.

With the ramping up of the Simonyi Survey Telescope at the Vera C. Rubin Observatory in Chile, Microsoft software architect Charles Simonyi joins a select group of scientists and technologists, policymakers and philanthropists who have had world-class telescopes and observatories named after them.

But here’s the thing: Technically speaking, the Simonyi Survey Telescope isn’t named after Charles Simonyi alone.

“The idea was to create something that carries the family name, and I was more thinking about my dad, Simonyi Károly,” Charles Simonyi told GeekWire, using the Hungarian manner of speech for personal names. “He was a professor at Budapest University. He wrote a wonderful book called ‘The Cultural History of Physics,’ which is available now in English at Amazon.”

Simonyi said his father was best-known for his work in popularizing science, “to make science understandable to the great public.” The physicist’s son arguably had an even greater impact on our computer-centric society by taking a leading role in creating Word, Excel and other tools for Microsoft’s Office suite of applications back in the 1980s. Four decades later, Word is still the world’s most widely used word processing software, and Excel is the most widely used spreadsheet.

Now the Simonyi Survey Telescope promises to have a similarly transformative and long-lasting impact on astronomy. Built at the Rubin Observatory on the edge of Chile’s Atacama Desert, one of the driest places on Earth, the telescope will survey the full sky every three nights, generating about 20 terabytes of raw data daily.

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Asteroid hunters make 27,500 new finds in old data

Asteroid orbital tracks
This visualization shows trajectories for scores of asteroids. (B612 Asteroid Institute / UW Dirac Institute / OpenSpace Project)

A team of asteroid hunters that includes researchers at the University of Washington says it has identified 27,500 new, high-confidence asteroid discovery candidates — not by making fresh observations of the night sky, but by sifting through archives of astronomical data.

The weeks-long database search was conducted by the Asteroid Institute, a program of the nonprofit B612 Foundation, in partnership with UW’s DiRAC Institute and Google Cloud.

The two institutes developed a program called THOR, which stands for “Tracklet-less Heliocentric Orbit Recovery.” THOR runs on a cloud-based, open-source platform known as ADAM (“Asteroid Discovery Analysis and Mapping”). The program can analyze the positions of millions of moving points of light observed in the sky over a given period of time, and link those points together in ways that are consistent with orbital paths.

Google Cloud’s Office of the CTO collaborated with the Asteroid Institute to fine-tune its algorithms for Google Cloud. The project analyzed 5.4 billion observations drawn from the NOIRLab Source Catalog Data Release 2.

“What is exciting is that we are using electrons in data centers, in addition to the usual photons in telescopes, to make astronomical discoveries,” Ed Lu, executive director of the Asteroid Institute, said in a news release.

Most of the 27,500 asteroid discovery candidates are in the main belt, between the orbits of Mars and Jupiter. But the candidates also include more than 100 apparent near-Earth asteroids.

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Asteroid-hunting algorithm passes a tricky test

Bird's eye view showing orbital paths for Earth and asteroid 2022 SF289 at closest approach
A bird’s-eye view of the solar system shows the orbital path for Earth in blue and the projected orbit for the asteroid known as 2022 SF289 at its closest approach in green. Orbits of Venus and Mars are shown in orange and red. (Credit: Joachim Moeyens / UW / OpenSpace)

A new technique for finding potentially hazardous asteroids before they find us has chalked up its first success.

In this case, the asteroid isn’t expected to threaten Earth anytime in the foreseeable future. But the fact that the technique — which uses a new computer algorithm called HelioLinc3D — actually works comes as a confidence boost as astronomers get set to step up the asteroid hunt with the Vera C. Rubin Observatory in Chile.

The University of Washington’s DiRAC Institute will play a leading role in analyzing the data from the Rubin Observatory, and HelioLinc3D is meant to make the job easier.

It’ll be another couple of years before the Rubin Observatory starts surveying the skies, but researchers put HelioLinc3D to the test by feeding it data from the NASA-funded Asteroid Terrestrial-impact Last Alert System, or ATLAS.

During the July 18 test run, the algorithm combined fragments of ATLAS data from four nights of observations to identify an asteroid that had been previously missed.

The asteroid, designated 2022 SF289 and described in a Minor Planet Electronic Circular, is thought to be about 600 feet wide. That’s wide enough to cause widespread destruction on Earth in the event of an impact. The good news is that projections of 2022 SF289’s orbital path show it staying 140,000 miles away from Earth at its closest. Nevertheless, the space rock fits NASA’s definition of a potentially hazardous asteroid because of its estimated size and the fact that it can come within 5 million miles of our planet.

UW researcher Ari Heinze, the principal developer of HelioLinc3D, said the algorithm’s success should carry over to the Rubin Observatory’s future database.

“By demonstrating the real-world effectiveness of the software that Rubin will use to look for thousands of yet-unknown potentially hazardous asteroids, the discovery of 2022 SF289 makes us all safer,” Heinze said in a news release.

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