Wild internet rumors speculated that the newly discovered interstellar visitor was an active extraterrestrial spacecraft scanning our solar system; forty-two radio telescope dishes listened across eleven gigahertz of frequencies and heard only total cosmic silence. Published in The Astronomical Journal by the SETI Institute, this rigorous investigation proves that if 3I/ATLAS were broadcasting an alien radio signal, its transmitter power would have to be weaker than a standard handheld walkie-talkie.

Whenever an object enters our solar system from another star, the mystery captures the world's imagination. When 3I/ATLAS was discovered traveling at tremendous speed on an alien trajectory, scientists and the public wondered: could this interstellar voyager be an active technological probe sent by an alien civilization?
The SETI Institute aimed forty-two radio telescope dishes at the passing visitor, scanning millions of radio channels simultaneously across the microwave spectrum. The array listened for artificial narrow-band radio beeps, calculating that if the object had a radio transmitter even ten times weaker than an ordinary smartphone, the telescopes would have caught it instantly.
The search yielded absolute radio silence, confirming that 3I/ATLAS is a completely natural cosmic iceberg. By demonstrating the speed of modern SETI technosignature defense networks, by setting strict physical limits on alien artifacts, and by maintaining rigorous scientific skepticism, planetary defense astronomy protects empirical truth.
A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array
In 2025 July, the third-ever interstellar object, 3I/ATLAS, was discovered on its ingress into the solar system. Similar to the NASA Voyager missions sent in 1977, science probes by extraterrestrial life (“artifact technosignatures”) could be sent to explore other stellar systems like our own. In this campaign, we used the SETI Institute’s Allen Telescope Array to observe 3I/ATLAS from 1–9 GHz. We detected nearly 74 million narrowband hits in 7.25 hr of data using the newly developed search pipeline bliss. We then blanked hits by frequency and drift rate to mitigate radio frequency interference in our dataset, narrowing the dataset down to ∼2 million hits. These hits were further filtered by the localization code NBeamAnalysis, and the remaining 211 hits were visually inspected in the time-frequency domain. We did not find any signals worthy of additional follow-up. Accounting for the Doppler drift correction and given the nondetection, we are able to set an effective isotropic radiated power upper limit of 10–110 W on radio technosignatures from 3I/ATLAS across the frequency and drift rate ranges covered by our survey.
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