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Did WISE detect Dyson Spheres/Structures around Gaia-2MASS-selected stars?

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arxiv 2409.11447 v1 pith:HKV2KEH2 submitted 2024-09-17 astro-ph.IM physics.pop-ph

Did WISE detect Dyson Spheres/Structures around Gaia-2MASS-selected stars?

classification astro-ph.IM physics.pop-ph
keywords dsmsadvancedwiseappearcataloguecivilizationdysonenough
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Soon after the release of the WISE all-sky catalogue of 500 million mid-infrared (IR) objects, suggestions were made that it could be used to search for extrasolar devices constructed by an advanced civilization to convert a significant fraction of their host star's luminosity into useful work: "technostructures", "megastructures" or "Dyson spheres/structures", hereafter DSMs, whose inevitable waste heat would be seen by WISE at mid-IR wavelengths. However, a trawl of several million potentially-habitable Gaia-detected stars for mid-IR-excess signatures is fraught with danger, due to both noise from such a large sample and, more importantly, confusion with the emission from dusty background galaxies. In light of a recent claim of seven potential DSMs in MNRAS, a brief rebuttal appeared on arXiv. Further to this response, the relevance of WISE-detected galaxies is discussed in more detail, leading to a seemingly tight limit on the number and lifetime of DSMs, and indeed intelligent worlds, in the ~600-pc-radius region patrolled by Gaia. However, the detectability of DSMs is questioned: a DSM might extinguish its star at optical/near-IR wavelengths, and thus either not appear or appear anomalously faint in a stellar catalogue. Moreover, a civilization advanced enough to construct a DSM is likely to be advanced enough to use countermeasures to mask its presence from us.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Project Hephaistos -- IV. James Webb Space Telescope Observations of Two Dyson Sphere Candidates

    astro-ph.GA 2026-07 accept novelty 6.5

    JWST/MIRI data attribute the mid-IR excess of Hephaistos candidates D and E to background galaxies at z≈0.9 (Hot-DOG-like) and z≈0.4 (dusty starburst), not to Dyson spheres or debris disks.