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Alien Radio Hum: How to Eavesdrop on Distant Civilizations ⚡ экспресс

Original: "Isolating Broadband Radio Technosignatures (BRaTs): A Framework for Detecting Planetary-Scale Leakage"
· Michael A. Garrett
arXiv:2605.10212 · 2026-05-11 · CC BY 4.0 · ⏱ 1 min · Instrumentation
Instead of narrow radio beacons, scientists propose hunting for the persistent techno-hum that resembles our own internet chatter.
Abstract

Traditional SETI methods focus on narrow-band electromagnetic beacons, yet our own technological development shows a shift to distributed broadband digital networks. Strict bandwidth filtering in most surveys risks missing the aggregate emission of technological civilizations, misclassifying it as unstructured noise. The possibility of detecting such planetary broadband radio technosignatures (BRaTs) via a hierarchical observing scheme is explored. In the first stage, wide-field surveys with next-generation arrays (SKA and its precursors) select candidates, after which very long baseline radio interferometry (VLBI) performs high-precision confirmation. Broadband emission is virtually insensitive to Doppler drift, enabling lengthy 'SETI deep fields' and increasing the detectable volume for leaks from Kardashev Type I civilizations to up to 100 pc.

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For decades, the search for extraterrestrial intelligence was waiting for quiet whistles from space. But our own technosphere has created a continuous radio background—like the hum of a vast metropolis. If nearby stars have sensitive antennas, they already hear this noise. SETI is now learning to pick up similar "noisy cities" on other planets.

The method has two stages: a quick sky survey for bright radio spots, then a detailed examination with a network of antennas. A technogenic source is identified by its anomalous radio brightness (it "shines" in radio like an overheated object, but without real heat), lack of circular polarization, and scintillation in cosmic irregularities. The final test is synchronous motion with the star. These observations will complement the exoplanet data from the Kepler mission William Borucki.

The first pulsar, discovered by Jocelyn Bell Burnell, was mistaken for an alien signal and named LGM-1 ("little green men"). Today, astronomers purposefully hunt for technogenic hum, not pulsars.

🎯 If a narrow radio beacon is a lone whistle in the night, then a planet's technogenic hum resembles the cacophony of a big city: a mix of conversations, engines, and music across all frequencies.

🎬 In Carl Sagan's novel "Contact," aliens sent a complex narrow signal. The new approach suggests we're more likely to pick up the unintended noise of their technology—the same kind our own internet traffic generates.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Tags
exoplanet spectroscopy cosmic dust
Laws
Doppler effectKepler's third lawMaxwell's equationsPlanck's lawPlanck–Einstein relationWien's displacement law
Original: arXiv:2605.10212 · CC BY 4.0 · bridge42worlds