Researchers at the SETI Institute modeled how plasma turbulence and stellar activity near a transmitting planet can broaden an originally ultra‑narrow radio signal, spreading its power across frequencies so it slips below narrowband detection thresholds. They built a practical framework by calibrating against spacecraft transmissions in our solar system and extrapolating to other stellar types, finding M‑dwarf systems are particularly likely to wash out narrowband technosignals.
— If true, the result implies many past null results are observational artifacts and that SETI search strategies and resource allocation should be revised to account for stellar environment effects.
EditorDavid
2026.03.09
100% relevant
SETI Institute study led by Dr. Vishal Gajjar; framework calibrated on spacecraft radio transmissions; specific finding that M‑dwarfs (≈75% of Milky Way stars) are prone to signal broadening.
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