Voluntary and Involuntary Technosignatures: Which Are to Be Encountered First

Numerous methods have been tried and many more are currently being attempted to discover technosignatures of intelligent civilizations. One thing is for sure: an existing technosignature would modify its environment in detectable ways. The current study has investigated all possible voluntary and involuntary technosignatures, ranging from beacons to Dyson megastructures and from self-replicating probes to the still hypothetical stellar engines, in order to determine the extent to which these technosignatures would reveal themselves within a specified finite sphere 500 light years across, corresponding to nearly half the average thickness of our Galaxy. We then estimated the probabilities of detection of such technosignatures based on the regions, or domains, they would produce and investigated whether or not a correlation exists with the position of civilizations on the Kardashev scale. The study further explored which ones of the voluntary and involuntary technosignatures have higher detection probabilities.

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Publication Details

Journal
Astrophysical Bulletin
Published
2025-09-01
DOI
https://doi.org/10.1134/s1990341324600066
Primary Topic
Space Science and Extraterrestrial Life
Type
article
Field-Weighted Citation Impact
0.00
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article

Voluntary and Involuntary Technosignatures: Which Are to Be Encountered First

Astrophysical Bulletin
Space Science and Extraterrestrial Life
article

Voluntary and Involuntary Technosignatures: Which Are to Be Encountered First

article en

Abstract

Numerous methods have been tried and many more are currently being attempted to discover technosignatures of intelligent civilizations. One thing is for sure: an existing technosignature would modify its environment in detectable ways. The current study has investigated all possible voluntary and involuntary technosignatures, ranging from beacons to Dyson megastructures and from self-replicating probes to the still hypothetical stellar engines, in order to determine the extent to which these technosignatures would reveal themselves within a specified finite sphere 500 light years across, corresponding to nearly half the average thickness of our Galaxy. We then estimated the probabilities of detection of such technosignatures based on the regions, or domains, they would produce and investigated whether or not a correlation exists with the position of civilizations on the Kardashev scale. The study further explored which ones of the voluntary and involuntary technosignatures have higher detection probabilities.

Astrophysical BulletinVol. 80(3)
Ege University (TR)
Openalex Percentile: Top 39%
Space Science and Extraterrestrial Life
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