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Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability

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 sim...

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Autores principales: Battistuzzi, Mariano, Cocola, Lorenzo, Claudi, Riccardo, Pozzer, Anna Caterina, Segalla, Anna, Simionato, Diana, Morosinotto, Tomas, Poletto, Luca, La Rocca, Nicoletta
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Frontiers Media S.A. 2023
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9941696/
https://www.ncbi.nlm.nih.gov/pubmed/36824196
http://dx.doi.org/10.3389/fpls.2023.1070359
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author Battistuzzi, Mariano
Cocola, Lorenzo
Claudi, Riccardo
Pozzer, Anna Caterina
Segalla, Anna
Simionato, Diana
Morosinotto, Tomas
Poletto, Luca
La Rocca, Nicoletta
author_facet Battistuzzi, Mariano
Cocola, Lorenzo
Claudi, Riccardo
Pozzer, Anna Caterina
Segalla, Anna
Simionato, Diana
Morosinotto, Tomas
Poletto, Luca
La Rocca, Nicoletta
author_sort Battistuzzi, Mariano
collection PubMed
description 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 far-red in addition to visible light for photosynthesis, and Synechocystis sp. PCC6803, a species unable to perform this photoacclimation, comparing their responses when exposed to three simulated light spectra: M-dwarf, solar and far-red. We analysed growth and photosynthetic acclimation features in terms of pigment composition and photosystems organization. Finally, we determined the oxygen production of the strains directly exposed to the different spectra. RESULTS: Both cyanobacteria were shown to grow and photosynthesize similarly under M-dwarf and solar light conditions: Synechocystis sp. by utilizing the few photons in the visible, C. fritschii by harvesting both visible and far-red light, activating the FaRLiP response. DISCUSSION: Our results experimentally show that an M-dwarf light spectrum could support a biological oxygen production similar to that in solar light at the tested light intensities, suggesting the possibility to discover such atmospheric biosignatures on those exoplanets if other boundary conditions are met.
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spelling pubmed-99416962023-02-22 Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability Battistuzzi, Mariano Cocola, Lorenzo Claudi, Riccardo Pozzer, Anna Caterina Segalla, Anna Simionato, Diana Morosinotto, Tomas Poletto, Luca La Rocca, Nicoletta Front Plant Sci Plant Science 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 far-red in addition to visible light for photosynthesis, and Synechocystis sp. PCC6803, a species unable to perform this photoacclimation, comparing their responses when exposed to three simulated light spectra: M-dwarf, solar and far-red. We analysed growth and photosynthetic acclimation features in terms of pigment composition and photosystems organization. Finally, we determined the oxygen production of the strains directly exposed to the different spectra. RESULTS: Both cyanobacteria were shown to grow and photosynthesize similarly under M-dwarf and solar light conditions: Synechocystis sp. by utilizing the few photons in the visible, C. fritschii by harvesting both visible and far-red light, activating the FaRLiP response. DISCUSSION: Our results experimentally show that an M-dwarf light spectrum could support a biological oxygen production similar to that in solar light at the tested light intensities, suggesting the possibility to discover such atmospheric biosignatures on those exoplanets if other boundary conditions are met. Frontiers Media S.A. 2023-02-07 /pmc/articles/PMC9941696/ /pubmed/36824196 http://dx.doi.org/10.3389/fpls.2023.1070359 Text en Copyright © 2023 Battistuzzi, Cocola, Claudi, Pozzer, Segalla, Simionato, Morosinotto, Poletto and La Rocca https://creativecommons.org/licenses/by/4.0/This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
spellingShingle Plant Science
Battistuzzi, Mariano
Cocola, Lorenzo
Claudi, Riccardo
Pozzer, Anna Caterina
Segalla, Anna
Simionato, Diana
Morosinotto, Tomas
Poletto, Luca
La Rocca, Nicoletta
Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability
title Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability
title_full Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability
title_fullStr Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability
title_full_unstemmed Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability
title_short Oxygenic photosynthetic responses of cyanobacteria exposed under an M-dwarf starlight simulator: Implications for exoplanet’s habitability
title_sort oxygenic photosynthetic responses of cyanobacteria exposed under an m-dwarf starlight simulator: implications for exoplanet’s habitability
topic Plant Science
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9941696/
https://www.ncbi.nlm.nih.gov/pubmed/36824196
http://dx.doi.org/10.3389/fpls.2023.1070359
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