paper

Project Hephaistos I. Upper limits on partial Dyson spheres in the Milky Way

arXiv:2201.11123 · doi:10.1093/mnras/stac280

Abstract

Dyson spheres are hypothetical megastructures built by advanced extraterrestrial civilizations to harvest radiation energy from stars. Here, we combine optical data from Gaia DR2 with mid-infrared data from AllWISE to set the strongest upper limits to date on the prevalence of partial Dyson spheres within the Milky Way, based on their expected waste-heat signatures. Conservative upper limits are presented on the fraction of stars at G 21 that may potentially host non-reflective Dyson spheres that absorb 1 - 90 of the bolometric luminosity of their host stars and emit thermal waste-heat in the 100 - 1000 K range. Based on a sample of stars within 100 pc, we find that a fraction less than could potentially host 300 K Dyson spheres at 90 completion. These limits become progressively weaker for less complete Dyson spheres due to increased confusion with naturally occurring sources of strong mid-infrared radiation, and also at larger distances, due to the detection limits of WISE. For the stars within 5 kpc in our Milky Way sample, the corresponding upper limit on the fraction of stars that could potentially be 300 K Dyson spheres at 90 completion is .

Accepted for publication in MNRAS

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