Space is Colder Than We Hoped express

Original: "WISE/CatWISE Constraints on Dysonian Waste-Heat Technosignatures in Nearby Galaxies"
arXiv:2601.07297v2 · 2026-01-12 · CC BY 4.0 · 1 min
Astronomers conducted the largest search for thermal traces of extraterrestrial civilizations among thousands of galaxies and found nothing but a chill.

📄 Showing the "Simple" version — "Advanced" is not ready yet. Add it to favorites to help prioritize it.

Any device, from a toaster to a smartphone, heats up when operating. This is the inevitable result of energy conversion — there's always a heat trace left, like a hot stove burner after cooking. The law of entropy applies to galaxies too: if advanced civilizations live there, reprocessing the light of entire stars, they should 'glow' with infrared heat — like a kitchen where something is stewing around the clock.

Astronomers pointed the heat-sensing WISE telescope at thousands of neighboring galaxies. Using photometry — measuring brightness in different shades of thermal radiation — they compared the actual glow with what ordinary old stars produce. Natural 'hot spots', like dust around black holes, were excluded in advance. The result: not a single galaxy showed a clear excess.

Our planet is cooling almost without a trace: Earth converts only 0.04% of sunlight into artificial heat — thousands of times less than what the authors were looking for.
WISE's sensitivity is enough to notice the heat from a megastructure encircling a star within a few light-years. But even that heat isn't there.

The strict conclusion: no more than 0.016% of nearby galaxies can contain civilizations that turn at least a fifth of starlight into heat. The universe seems suspiciously cool, like a kitchen after the residents have moved out, leaving us in solitude.

Original abstract

as written by the authors arXiv:2601.07297v2

We search for galaxy-scale (Dysonian) waste heat in the mid-infrared using WISE. Starting from the 2MASS Redshift Survey (2MRS), we cross-match to CatWISE2020 and AllWISE, apply standard MIR AGN/starburst vetoes (Stern, Assef R90, Jarrett), and treat W1 and W2 as stellar baselines and W3 and W4 as constraining bands. For each galaxy and for blackbody waste heat temperatures T=150-600 K, we convert W3/W4 photometry into conservative 3-sigma per-galaxy upper limits on the bolometric waste heat luminosity using the WISE bandpass (RSR) color correction. The resulting distributions have median caps of ~(5-9) x 10^8 L_sun across T=150-600 K. Aggregated at the population level, the one-sided 95% upper bound on the fraction of nearby galaxies that could host waste heat above a given threshold monotonically decreases with threshold and asymptotes to ~1/6500 at high thresholds (set by the sample size). Sensitivity transitions from W4 at T <= 200K to W3 at T >= 300K. Interpreted with the AGENT formalism, a fiducial Milky Way like stellar luminosity L_=3 x 10^10 L_sun implies typical per galaxy caps of alpha = L_wh/L_ <= 1.7-2.9% over T=150-600 K (e.g., alpha <= 1.8% at T=300 K). At T ~= 300K, no more than f_95 ~= 1.61 x 10^-4 (~= 0.0161%) of nearby galaxies can host KIII-scale systems reprocessing >= 21% of a Milky Way-like stellar luminosity into ~ 300K waste heat.

The temperature of 300 Kelvin they were looking for is a comfortable 27°C. Remarkably, the human body radiates about as much heat as a 100-watt light bulb. From a galactic civilization, however, they expected a glow hundreds of trillions of times more powerful.

The search for engineering structures of alien races is a popular sci-fi plot. For example, in Ivan Efremov's novel 'Andromeda Nebula', the characters find a vanished civilization by its residual radiation.

Scientists
Fritz ZwickyJacob BekensteinWilliam BoruckiSubrahmanyan ChandrasekharWilhelm WienAdam Riess
Concepts
wolf rayet star waste heat miri hot gas cosmic microwave background measurement infrared james webb space telescope Chandrasekhar limit white dwarf Outgoing longwave radiation Niño 4 microwave rubidium vapor