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Detecting the entropy of exoplanets in the context of the Acta Universi hypothesis represents the next great challenge for astronomy. This will require: • New technologies (quantum sensors, interferometry) • New missions (space observatories) • New analysis methods (machine learning, correlation analysis) But the potential reward is huge: the discovery and study of life in the universe is not through chemical traces, but through its fundamental manifestation — entropic complexity in the universal AU field. The time to start is now. The first steps can already be taken with the analysis of existing data and the development of detector prototypes. By 2030-2040, we may have the first real data on the AU entropy of other worlds.
YASHCHENKO D. 2026. ENTROPY OF EXOPLANETS: DETECTION METHODS IN THE CONTEXT OF ACTA UNIVERSI. PREPRINTS.RU. https://doi.org/10.24108/preprints-3114447
