Evidence map›Paper›PMID 36824196›Full record

ArticleFrontiers in plant science2023

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

Abstract read
In one paragraph

Article in Frontiers in plant science, 2023. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 9 papers.

0numbers the graph read from it
0cells of the map it votes in
9citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

9 citing papers in PubMed.

  1. Review
  2. Article
  3. Article
  4. Article
  5. Frontiers in microbiology · 2025
    Article
  6. Article
  7. Far-red light photoacclimation in a desertFrontiers in microbiology · 2024
    Article
  8. Article
  9. Transcriptomic and photosynthetic analyses ofFrontiers in plant science · 2023
    Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

9 authors.

Mariano BattistuzziDepartment of Biology, University of Padua, Padua, Italy.
Lorenzo CocolaNational Council of Research of Italy, Institute for Photonics and Nanotechnologies (CNR-IFN), Padua, Italy.
Riccardo ClaudiNational Institute for Astrophysics, Astronomical Observatory of Padua (INAF-OAPD), Padua, Italy.
Anna Caterina PozzerDepartment of Biology, University of Padua, Padua, Italy.
Anna SegallaDepartment of Biology, University of Padua, Padua, Italy.
Diana SimionatoDepartment of Biology, University of Padua, Padua, Italy.
Tomas MorosinottoDepartment of Biology, University of Padua, Padua, Italy.
Luca PolettoNational Council of Research of Italy, Institute for Photonics and Nanotechnologies (CNR-IFN), Padua, Italy.
Nicoletta La RoccaDepartment of Biology, University of Padua, Padua, Italy.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

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 Results: Both cyanobacteria were shown to grow and photosynthesize similarly under M-dwarf and solar light conditions: 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.

Indexed as

biosignaturescyanobacterialaboratory simulationslight acclimationM-dwarf spectrumoxygenic photosynthesis

Identifiers

PMID36824196
PMCPMC9941696

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.