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The SETI Institute Searched For Signs of Technology From 3I/ATLAS—a New Paper Reveals What They Found

6 June 2026 at 15:06


Astronomers from around the world were fascinated last year when 3I/ATLAS, the third interstellar object ever observed passing through our Solar System, was discovered.

The SETI Institute was one of the many organizations that examined the unusual interstellar object, conducting a comprehensive search for any signs that it might be producing technological signals.

Using the Allen Telescope Array (ATA) at the Hat Creek Radio Observatory in Northern California, SETI researchers scanned a broad range of radio frequencies in search of potential evidence of extraterrestrial technology associated with 3I/ATLAS. The data that came back was clear: no signs of artificial signals. As most astronomers expected, 3I/ATLAS is most likely a natural comet. 

“We searched for narrowband signals across a broad range of spectrum: 1–10 GHz. We can do this efficiently due to the ATA’s ability to record and search billions of channels at a time,” says Dr. Sofia Sheik, lead author of a new paper describing the SETI Institute’s work, in an email to The Debrief.
3I/ATLAS
The interstellar comet 3I/ATLAS (Image Credit: International Gemini Observatory/NOIRLab/NSF/AURA/Shadow the Scientist)

Observations of interstellar objects have become more common in recent years, due to advances in telescopic technologies available to astronomers. Discovered last July, 3I/ATLAS is only the third confirmed interstellar visitor to enter our Solar System, preceded by 1I/ʻOumuamua in 2017, and 2I/Borisov in 2019. 

These rare discoveries help astronomers understand the materials in our cosmic backyard. By analyzing the composition of these objects, scientists can gain a deeper understanding of how planetary systems develop and evolve throughout the galaxy.

The Research 

The majority of recent astronomical observations indicate that 3I/ATLAS is a natural object, albeit one that exhibited some unusual qualities. However, the possibility remains that we may one day find a technological artifact from an intelligent civilization; it is equally possible that at some point, aliens may also discover a spacecraft of Earthly origin. 

“Eventually, our own Voyager spacecraft will be extraterrestrial artifacts in other stellar systems,” Sheik told The Debrief. “Given that, it is important that we understand the natural distribution of interstellar objects so that we will be able to identify any anomalies that could one day be signs of an artificial interstellar object.”

The SETI research team studied 3I/ATLAS for over seven hours using the ATA, searching radio frequencies from 1 to 9 gigahertz. This range is especially important because it can detect narrowband radio signals, which are rarely produced by natural space phenomena and are often considered possible signs of technological activity.

Researchers found 74 million narrowband signals, but after filtering out human interference and motion-matched sources, only about 200 remained. These were later confirmed to come entirely from Earth-based technology or satellites.

“To be clear, we did not detect any radio signals from 3I/ATLAS. We ruled out the presence of signals down to power levels comparable with everyday appliances: for example, we definitely would have picked up a cell tower or a radio station equivalent had it been on the surface of 3I/ATLAS,” Sheik said.

In other words, no technosignatures were detected. The SETI observation ruled out signals stronger than approximately 10 to 110 watts across the observed frequencies (comparable to the power consumption of a household appliance).

3I/ATLAS trajectory
NASA diagram showing the trajectory of the interstellar object 3I/ATLAS (Image Credit: NASA).

The Origins of 3I/ATLAS

For a time, there was a considerable amount of speculation over whether 3I/ATLAS could represent something more than just a natural object. Among the proponents of such ideas, theoretical physicist Avi Loeb emerged as one of the most visible supporters of the possibility that the interstellar object displayed anomalous qualities that could point to technological origins. 

Last July, shortly after the object’s discovery, Loeb predicted on his Medium page that 3I/ATLAS may be one of two things: a comet possessing a smaller core with a radius less than 400 meters, or “an object that favored a radial orbit into the inner solar system,” meaning that it may also be a larger object compared to its predecessors. Indeed, further observations of the object eventually suggested that 3I/ATLAS appears to be significantly larger than ‘Oumuamua or Borisov was.

Loeb also suggested in a podcast interview that 3I/ATLAS might not be following a random trajectory, but rather that its current motion could be understood as “directed” toward the inner solar system.

“That obviously opens the door for it being technological, because who would target the inner solar system?” said Loeb during an interview. 

 

In an email to The Debrief, Loeb shared his thoughts on the recent SETI findings.

“Radio communication is an old technology, which was recently accompanied by optical laser communication in NASA’s Artemis II mission to the Moon,” Loeb said. “Lasers might replace radio communication in our future space missions, and there is no guarantee that they would operate at the frequencies scanned in this study.”

“To save power, a technological transmitter might beam its signal in the direction of the receiver (rather than Earth) and might only transmit sporadically,” Loeb added.

Last September, Loeb also looked at another fairly remote possibility: that the famous “Wow!” signal might be somehow related to 3I/ATLAS.

“Interestingly, the anomalous ‘Wow! Signal’ detected on August 15, 1977, came from a direction which is separated by only 9 degrees from the arrival direction of 3I/ATLAS into the inner Solar System, but a similar signal was never detected again,” Loeb told The Debrief. 

The Search for Interstellar Objects 

For Sheik and the team, while 3I/ATLAS did not display any obvious signatures that could be associated with technosignatures, it still provided a significant learning opportunity.

“The results from 3I/ATLAS show how realistic it is to detect a signal with the technology we have today,” said co-author Valeria Garcia Lopez. “That is why it is important to keep searching for technosignatures, even from objects we might not expect to have signals.”

Additionally, this project highlighted the ATA’s ability to respond quickly to new discoveries. Observations began less than 24 hours after the discovery of 3I/ATLAS was announced, showcasing the telescope’s flexibility and preparedness. 

“One of the ATA’s advantages is being able to get quickly on-source to follow up on new and exciting discoveries, which was showcased in the 3I/ATLAS observations,” Sheik told The Debrief. “3I/ATLAS was announced on July 1st, and the ATA began observations on July 3rd.”
With ongoing advancements in technology, future observations of similar interstellar objects should become more frequent.
“For sources that might be changing quickly, this kind of rapid follow-up is essential to get early data and context for later observations with other observatories,” Sheik added.

Chrissy Newton is a PR professional and the founder of VOCAB Communications. She currently appears on The Discovery Channel and Max and hosts the Rebelliously Curious podcast, which can be found on YouTube and on all audio podcast streaming platforms. Follow her on X: @ChrissyNewton, Instagram: @BeingChrissyNewton, and chrissynewton.com. To contact Chrissy with a story, please email chrissy @ thedebrief.org.

The LHC is on turning on again! What does that mean?

5 July 2022 at 18:20

Deep underground, on the border between Switzerland and France, the Large Hadron Collider (LHC) is starting back up again after a 4 year hiatus. Today, July 5th, the LHC had its first full energy collisions since 2018.  Whenever the LHC is running is exciting enough on its own, but this new run of data taking will also feature several upgrades to the LHC itself as well as the several different experiments that make use of its collisions. The physics world will be watching to see if the data from this new run confirms any of the interesting anomalies seen in previous datasets or reveals any other unexpected discoveries. 

New and Improved

During the multi-year shutdown the LHC itself has been upgraded. Noticably the energy of the colliding beams has been increased, from 13 TeV to 13.6 TeV. Besides breaking its own record for the highest energy collisions every produced, this 5% increase to the LHC’s energy will give a boost to searches looking for very rare high energy phenomena. The rate of collisions the LHC produces is also expected to be roughly 50% higher  previous maximum achieved in previous runs. At the end of this three year run it is expected that the experiments will have collected twice as much data as the previous two runs combined. 

The experiments have also been busy upgrading their detectors to take full advantage of this new round of collisions.

The ALICE experiment had the most substantial upgrade. It features a new silicon inner tracker, an upgraded time projection chamber, a new forward muon detector, a new triggering system and an improved data processing system. These upgrades will help in its study of exotic phase of matter called the quark gluon plasma, a hot dense soup of nuclear material present in the early universe. 

 

A diagram showing the various upgrades to the ALICE detector (source)

ATLAS and CMS, the two ‘general purpose’ experiments at the LHC, had a few upgrades as well. ATLAS replaced their ‘small wheel’ detector used to measure the momentum of muons. CMS replaced the inner most part its inner tracker, and installed a new GEM detector to measure muons close to the beamline. Both experiments also upgraded their software and data collection systems (triggers) in order to be more sensitive to the signatures of potential exotic particles that may have been missed in previous runs. 

The new ATLAS ‘small wheel’ being lowered into place. (source)

The LHCb experiment, which specializes in studying the properties of the bottom quark, also had major upgrades during the shutdown. LHCb installed a new Vertex Locator closer to the beam line and upgraded their tracking and particle identification system. It also fully revamped its trigger system to run entirely on GPU’s. These upgrades should allow them to collect 5 times the amount of data over the next two runs as they did over the first two. 

Run 3 will also feature a new smaller scale experiment, FASER, which will study neutrinos produced in the LHC and search for long-lived new particles. 

What will we learn?

One of the main goals in particle physics now is direct experimental evidence of a phenomena unexplained by the Standard Model. While very successful in many respects, the Standard Model leaves several mysteries unexplained such as the nature of dark matter, the imbalance of matter over anti-matter, and the origin of neutrino’s mass. All of these are questions many hope that the LHC can help answer.

Much of the excitement for Run-3 of the LHC will be on whether the additional data can confirm some of the deviations from the Standard Model which have been seen in previous runs.

One very hot topic in particle physics right now are a series of ‘flavor anomalies‘ seen by the LHCb experiment in previous LHC runs. These anomalies are deviations from the Standard Model predictions of how often certain rare decays of the b quarks should occur. With their dataset so far, LHCb has not yet had enough data to pass the high statistical threshold required in particle physics to claim a discovery. But if these anomalies are real, Run-3 should provide enough data to claim a discovery.

A summary of the various measurements making up the ‘flavor anomalies’. The blue lines and error bars indicate the measurements and their uncertainties. The yellow line and error bars indicates the standard model predictions and their uncertainties. Source

There are also a decent number ‘excesses’, potential signals of new particles being produced in LHC collisions, that have been seen by the ATLAS and CMS collaborations. The statistical significance of these excesses are all still quite low, and many such excesses have gone away with more data. But if one or more of these excesses was confirmed in the Run-3 dataset it would be a massive discovery.

While all of these anomalies are gamble, this new dataset will also certainly be used to measure various known entities with better precision, improving our understanding of nature no matter what. Our understanding of the Higgs boson, the top quark, rare decays of the bottom quark, rare standard model processes, the dynamics of the quark gluon plasma and many other areas will no doubt improve from this additional data.

In addition to these ‘known’ anomalies and measurements, whenever an experiment starts up again there is also the possibility of something entirely unexpected showing up. Perhaps one of the upgrades performed will allow the detection of something entirely new, unseen in previous runs. Perhaps FASER will see signals of long-lived particles missed by the other experiments. Or perhaps the data from the main experiments will be analyzed in a new way, revealing evidence of a new particle which had been missed up until now.

No matter what happens, the world of particle physics is a more exciting place when the LHC is running. So lets all cheers to that!

Read More:

CERN Run-3 Press Event / Livestream Recording “Join us for the first collisions for physics at 13.6 TeV!“

Symmetry Magazine “What’s new for LHC Run 3?”

CERN Courier “New data strengthens RK flavour anomaly“

CERN Physicists Observe New Exotic Particle

25 May 2026 at 22:15
An artist’s impression of the Bc*+ meson. Image credit: Daniel Dominguez / CERN.

Physicists with the ATLAS Collaboration at CERN’s Large Hadron Collider (LHC) have observed the Bc*+ meson, an excited version of the Bc+ meson -- both consist of a charm quark and a bottom antiquark.

The post CERN Physicists Observe New Exotic Particle appeared first on Sci.News: Breaking Science News.

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