Biosignature False Positives in Potentially Habitable Planets around M Dwarfs: The Effect of UV Radiation from One Flare Article Swipe
Arturo Miranda-Rosete
,
Antígona Segura
,
Edward W. Schwieterman
·
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/acebec
YOU?
·
· 2025
· Open Access
·
· DOI: https://doi.org/10.3847/1538-4357/acebec
Many past studies have predicted the steady-state production and maintenance of abiotic O 2 and O 3 in the atmospheres of CO 2 -rich terrestrial planets orbiting M dwarf stars. However, the time-dependent responses of these planetary atmospheres to flare events—and the possible temporary production or enhancement of false-positive biosignatures therein—has been comparatively less well studied. Most past works that have modeled the photochemical response to flares have assumed abundant free oxygen, like that of the modern or Proterozoic Earth. Here we examine in detail the photochemical impact of the UV emitted by a single flare on abiotic O 2 /O 3 production in prebiotic, CO 2 -dominated atmospheres of M dwarf planets with CO 2 levels ranging from 3% to 80% of 1 bar. We find that a single flare generally destroys O 2 and O 3 over short timescales while modestly enhancing their column densities over intermediate timescales. We simulate the spectral observables of both the steady-state atmosphere and time-dependent spectral response over the flare window for both emitted and transmitted light spectra. Over the course of the flare, the O 3 UV Hartley band is decreased by a maximum of 47 ppm. In both emitted and transmitted light spectra, the 9.65 μ m O 3 band is hidden by the overlapping 9.4 μ m CO 2 band for all scenarios considered. Overall, we find that the possible enhancements of abiotic O 3 due to a single flare are small compared to O 3 ’s sensitivity to other parameters such as CO 2 and H 2 O abundances or the availability of reducing gases such as H 2 .
Related Topics
Concepts
Physics
Flare
Astrophysics
Astronomy
Planet
Planetary habitability
Astrobiology
Radiation
Circumstellar habitable zone
Exoplanet
Optics
Metadata
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- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-4357/acebec
- OA Status
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- References
- 105
- Related Works
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https://doi.org/10.3847/1538-4357/acebecDigital Object Identifier
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Biosignature False Positives in Potentially Habitable Planets around M Dwarfs: The Effect of UV Radiation from One FlareWork title
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articleOpenAlex work type
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enPrimary language
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2025Year of publication
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2025-08-01Full publication date if available
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Arturo Miranda-Rosete, Antígona Segura, Edward W. SchwietermanList of authors in order
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https://doi.org/10.3847/1538-4357/acebecPublisher landing page
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goldOpen access status per OpenAlex
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https://doi.org/10.3847/1538-4357/acebecDirect OA link when available
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Physics, Flare, Astrophysics, Astronomy, Planet, Planetary habitability, Astrobiology, Radiation, Circumstellar habitable zone, Exoplanet, OpticsTop concepts (fields/topics) attached by OpenAlex
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| abstract_inverted_index.M | 28, 111 |
| abstract_inverted_index.O | 13, 16, 99, 134, 137, 183, 207, 234, 245, 259 |
| abstract_inverted_index.a | 94, 129, 191, 238 |
| abstract_inverted_index.m | 206, 217 |
| abstract_inverted_index./O | 101 |
| abstract_inverted_index.3% | 120 |
| abstract_inverted_index.47 | 194 |
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| abstract_inverted_index.UV | 91, 185 |
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| abstract_inverted_index.is | 188, 210 |
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| abstract_inverted_index.to | 39, 66, 121, 237, 244, 249 |
| abstract_inverted_index.we | 82, 226 |
| abstract_inverted_index.μ | 205, 216 |
| abstract_inverted_index.80% | 122 |
| abstract_inverted_index.9.4 | 215 |
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| abstract_inverted_index.spectral | 154, 163 |
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| abstract_inverted_index.false-positive | 49 |
| abstract_inverted_index.time-dependent | 33, 162 |
| cited_by_percentile_year | |
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| institutions_distinct_count | 3 |
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| citation_normalized_percentile.is_in_top_10_percent | False |