From Smoke to Fire: What We’re Really Looking For in the Universe ✛

Original: "Decolonizing technosignatures: Reimagining technosignatures through an Indigenist lens"
· Hilding R. Neilson
arXiv:2607.07592 · 2026-07-08 · CC BY 4.0 · 3 min
Modern searches for alien technology catch only traces of pollution, while ignoring the possibility of living in harmony with nature — an idea embedded in traditional knowledge.

In 1960, the Tatel radio telescope spent weeks listening to emptiness around Tau Ceti and Epsilon Eridani. Project Ozma was searching for technosignatures — traces of another mind at work. More than 60 years later, after thousands of exoplanets were discovered by the Kepler mission under William Borucki, we are still surrounded by silence. Our smoke detector waits faithfully for a fire. But what if the warmest hearths barely smoke?

Today’s toolkit of technosignatures includes radio astronomy (artificial emissions), megastructures that block a star’s light, and exoplanet atmosphere (industrial gases). All of these are deviations from the natural background — footprints of interference. Western science is trained to hunt anomalies. But traditional knowledge, among the Mi’kmaq for instance, sees nature not as a resource but as a relative. A technology woven into that kinship doesn’t leave scars. Like a campfire that warms you without smearing black smoke across the sky.

In 1967, graduate student Jocelyn Bell Burnell noticed a strictly periodic radio pulse. The Cambridge team half-jokingly suggested it was an alien civilization’s signal and classified the data. It turned out to be the first pulsar discovered: a spinning neutron star.

The difference is profound. Almost all technosignatures we know are forms of pollution. And pollution, as scholars of Indigenous cultures note, is colonization of the environment. So our instruments are unwittingly selecting only those civilizations that repeat the Western path. History offers a warning: when Jocelyn Bell Burnell recorded the periodic pulses of that first pulsar, their natural origin was rejected at first. The signal was code-named LGM-1 — ‘Little Green Men’. We are wired to see alien intention in any irregularity.

But what if the most sustainable societies never disturb the natural balance? Their biosignatures might gently amplify the natural background instead of fighting it. Instead of smoke over factories, a barely detectable increase in a planet’s greenery, subtle climate regulation, slow rhythms interwoven with stellar evolution. This resolves the Fermi paradox: loud species burn themselves out fast, while quiet ones slip through the noise of the cosmos unnoticed.

The Fermi paradox: if the universe is full of life, why do we see no one? Perhaps the answer lies not in the absence of civilizations, but in our habit of looking only for those who leave dirty tracks.

For science, this means a change of lens: move from looking for smoke to looking for the flame. Instead of asking ‘what is wrong?’, ask ‘what is too harmonious?’ Such a technology won’t violate the natural balance; it will join it. We will need new signal processing algorithms attuned to slow trends rather than sudden spikes. The ‘Two-Eyed Seeing’ philosophy (numerical simulation plus Indigenous knowledge) already offers concrete scenarios for non-disruptive development.

The Tatel telescope fell silent long ago, but in 1960 it listened to two stars. Today, with a new lens, we can aim our antennas at those same constellations again. But this time we will ask not ‘where is the breakdown?’ but ‘where is the quiet?’ And maybe the silence will turn out to be not emptiness, but an answer from those who learned to live without clouding the sky with smoke.

The first pulsar, discovered by Jocelyn Bell Burnell in 1967, was initially labeled LGM-1 (‘little green men’)—so strong was the expectation that any deviation from nature must be artificial.

Scientists
David Charbonneau
Concepts
technosignature search biosignatures biosignature detection seti carbon dioxide ai astrophysics radio interference artifact biomarker exoplanet characterization false alarm biology Natural Language Processing biofilm cosmic dawn magnetic signatures background galaxy merger signatures carbon footprint ecosystem ecological resilience