The model explored star temperatures from 2300K to 5800K, representing cool M-dwarfs to Sun-like stars. By varying antenna size and absorption peaks, they determined the most efficient configurations for each stellar environment.
This study builds on recent experiments showing some organisms can grow under simulated M-dwarf light. It provides a theoretical framework explaining why certain life forms might thrive or struggle in these conditions.
Botany One /
npub1jr…xvtkn
2024-09-19 03:30:01
in reply to nevent1q…2g5g
Author Public Key
npub1jreqk3srdhyzw4y4pyah0vezxnngtyru0teydhyzwnnrepy59z0srxvtknPublished at
2024-09-19 03:30:01Event JSON
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