Slowpoke Star: A New Way to Search for Aliens ✛ ✦

Original: "Stellar J-Harvesting: a novel angular momentum technosignature and first search in the Kepler field"
· Sahin Torlakcik
arXiv:2607.07781 · 2026-07-08 · CC BY 4.0 · 1 min
An unusually slow-spinning star could signal an advanced civilization siphoning its energy.

A child’s spinning top loses rotational energy and slows down on its own; hooked to a generator, it decelerates much faster. Astronomers look for the same effect in stars: unusually slow rotation could betray alien technology. After digging through the Kepler telescope archive, which spent years measuring brightness (photometry) and monitoring planets around 6725 sun-like stars, scientists found two “slowpokes” whose rotation lagged far behind the evolutionary norm. But one is slowed by an unseen companion, and the other’s data were smeared by a neighboring star. No techno-signatures were found, but a limit was set: such harvesters appear no more than once per 2000 stars. The method’s main asset is stealth: it doesn’t hunt for heat but catches hidden deceleration. Future surveys with spectroscopy (chemical makeup), radio observations, and interferometry (ultra-sharp imaging) will sift millions of stars, accounting for star formation and metallicity (heavy-element fraction). Twist: to leave a noticeable trace, a civilization would need to extract 94% of the rotational energy, like braking the Sun to a halt in a billion years. The idea is fueled by the work of founding fathers: William Borucki (Kepler mission) and Subrahmanyan Chandrasekhar (stellar evolution).

To give themselves away, alien engineers would have to extract 94% of a star’s rotational energy — roughly like braking the Sun to a standstill in a time a hundred times shorter than its age.

E_{\text{rot}} = \frac{1}{2} k M_{\star} R_{\star}^2 \Omega_{\star}^2
E_rot - rotational energy, k - dimensionless moment of inertia (~0.059 for the Sun), M, R - mass and radius of the star, Ω - angular velocity.
P_{\text{new}} = P_{\text{old}} (1 - f)^{-1/2}, \quad \Delta \log P = -\frac{1}{2} \log_{10}(1 - f)
Allows calculation of the observed rotational slowdown from a known fraction of extracted energy.
Scientists
Subrahmanyan ChandrasekharArthur EddingtonNikolai Shakura
Concepts
technosignature search JWST kepler telescope astrophysical signal detection stellar spectroscopy james webb space telescope jwst red sources stellar archaeology binary star detection axion detection neutron stars technosignatures