Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet's habitability
Mariano Battistuzzi, Lorenzo Cocola, Riccardo Claudi, Anna Caterina, Pozzer, Anna Segalla, Diana Simionato, Tomas Morosinotto, Luca Poletto,, Nicoletta La Rocca

TL;DR
This study investigates how cyanobacteria, capable of oxygenic photosynthesis, respond to M-dwarf star-like light spectra, revealing their potential to produce oxygen on exoplanets orbiting such stars, which impacts habitability assessments.
Contribution
It demonstrates that cyanobacteria can perform oxygenic photosynthesis under M-dwarf star spectra, highlighting their potential role in exoplanet habitability.
Findings
Cyanobacteria grow and photosynthesize under M-dwarf and solar spectra.
FaRLiP enables C. fritschii to harvest far-red light.
Photosynthetic activity is comparable under M-dwarf and solar conditions.
Abstract
Introduction: The search for life on distant exoplanets is expected to rely on atmospheric biosignatures detection, such as oxygen of biological origin. However, it is not demonstrated how much oxygenic photosynthesis, which on Earth depends on visible light, could work under spectral conditions simulating exoplanets orbiting the Habitable Zone of M-dwarf stars, which have low light emission in the visible and high light emission in the far-red/near-infrared. By utilizing cyanobacteria, the first organisms to evolve oxygenic photosynthesis on our planet, and a starlight simulator capable of accurately reproducing the emission spectrum of an M-dwarf in the range 350-900 nm, we could answer this question. Methods: We performed experiments with the cyanobacterium Chlorogloeopsis fritschii PCC6912, capable of Far-Red Light Photoacclimation (FaRLiP), which allows the strain to harvest…
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