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Why the Interstellar Visitor 3I/ATLAS Remains Silent on the Radio

Original: "Periodic Radio Technosignature Search toward 3I/ATLAS with FAST"
arXiv:2607.01666v1 · 2026-07-02 · CC BY · ⏱ 2 min · Instrumentation Exoplanets Galaxies
Astronomers checked radio waves from an object from another star system but heard no artificial signals.
Abstract

The interstellar object 3I/ATLAS is a 'visitor' from another star system. Scientists tried to pick up periodic radio signals from it using the giant FAST telescope—think of it as listening in, hoping to catch signs of intelligent life. But they found nothing resembling an artificial signal. Maybe it's just a rock, silently roaming through space?

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Imagine you're trying to hear a faint alarm clock from one room when an orchestra is playing loudly. If you set up several microphones, you can catch the difference: the alarm clock's sound will be louder in the nearest microphone. That's roughly how the method used to observe the interstellar object 3I/ATLAS worked — an unusual comet that flew in from another star system. The giant FAST radio telescope, with its multiple beams as 'ears', listened to the ether for a long time, and mathematical processing, akin to separating mixed voices in a recording, searched for rhythmic notes.

Natural radio sources can also pulse. For example, pulsars — ultra-dense neutron stars — spin and send out pulses like cosmic lighthouses. They were discovered by Jocelyn Bell Burnell.

Alas, no artificial signals were found. Analysis based on entropy — a measure of how much energy is concentrated in the desired beam rather than smeared everywhere — showed that all suspicious bursts turned out to be either terrestrial interference or random noise. If there is a radio beacon operating on 3I/ATLAS, its power is no more than 0.146 watts — weaker than a flashlight bulb. The search was conducted at frequencies where hydrogen emits (21 centimeters) — this spectral fingerprint is considered a common language for interstellar communication.

3I/ATLAS is far from the first interstellar wanderer. Before it came 'Oumuamua and Comet Borisov. Unlike distant exoplanets, these objects zip by quite close, and scientists can study their emissions in detail. According to the theory of James Clerk Maxwell, radio waves travel at the speed of light, so we hear them almost instantaneously.

🎯 A signal separation method, akin to breaking a cocktail down into its ingredients, was invented in 1927, but astronomers could apply it only with the advent of powerful computers.

🎬 The plot of Arthur C. Clarke’s novel ‘Rendezvous with Rama’ describes an encounter with an interstellar object that turns out to be an alien spaceship. The real 3I/ATLAS, alas, remains silent for now.

S_{\min} \approx \frac{(S/N)_{\min} \mathrm{SEFD}}{\sqrt{n_{\mathrm{pol}} \Delta\nu_{\mathrm{ch}} T_{\mathrm{obs}}}} \sqrt{\frac{\delta}{1-\delta}}
Minimum detectable flux density for a periodic signal. Here SEFD is the system equivalent flux density, (S/N)_min is the threshold signal-to-noise ratio, n_pol is the number of polarizations, Δν_ch is the channel width, T_obs is the observation time, δ is the signal duty cycle.
\mathrm{EIRP} = 4\pi d^2 S_{\min} \Delta\nu
Equivalent isotropic radiated power of the transmitter. Shows what power an isotropic transmitter at distance d must emit to produce the observed flux density S_min in bandwidth Δν.
Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
hydrogen pulsar exoplanet comet spectroscopy entropy neutron star speed of light
Laws
second law of thermodynamicsDoppler effectprinciple of constancy of the speed of lightBekenstein-Hawking entropyKepler's third lawmass–energy equivalence
Original: arXiv:2607.01666v1 · CC BY · bridge42worlds