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the claim

A tidally locked planet like Gliese 667 Cc would have no axial tilt and therefore would not experience seasons.

the verdict
SUPPORTED
the evidence backs this
Recorded sources
7 sources for · 0 against

Counts group repeated records of the same source within each side. They do not measure evidence strength or source independence.

Is it true that a tidally locked planet like Gliese 667 Cc would have no axial tilt and therefore would not experience seasons?

Yes. Tidally locked planets rotate synchronously with their host star, resulting in a permanent dayside and nightside rather than the cyclic changes in solar illumination that produce conventional annual seasons.

Verdict: SUPPORTED · 7 sources for, 0 against · Last checked

The analysis

The retrieved papers consistently describe tidally locked exoplanets as being in spin-orbit synchronous rotation, creating permanent daysides and nightsides without the cyclic variations in day length and axial tilt that characterize seasonal changes on non-locked planets. None of the provided literature contradicts this consensus.

Evidence for · 7
2018
Discusses the atmospheric dynamics of tidally locked planets, which are characterized by synchronous rotation and permanent daysides/nightsides.
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Hammond, M. & Pierrehumbert, R. T. (2018). Wave-mean Flow Interactions in the Atmospheric Circulation of Tidally Locked Planets. doi.org. https://doi.org/10.3847/1538-4357/aaec03

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More for · 6
2018
Examines climate modeling of tidally locked exoplanets assuming synchronous rotation.
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Lewis, N. T., Lambert, F. H., Boutle, I. A., Mayne, N. J., Manners, J., & Acreman, D. M. (2018). The Influence of a Substellar Continent on the Climate of a Tidally Locked Exoplanet. doi.org. https://doi.org/10.3847/1538-4357/aaad0a

2022
Analyzes heat redistribution on tidally locked rocky planets characterized by permanent dayside and nightside conditions.
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Koll, D. D. B. (2022). A Scaling for Atmospheric Heat Redistribution on Tidally Locked Rocky Planets. doi.org. https://doi.org/10.3847/1538-4357/ac3b48

2020
Explicitly notes that over large timescales a planet driven to spin-orbit synchronous rotation exhibits a permanent dayside and nightside.
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Auclair-Desrotour, P. & Heng, K. (2020). Atmospheric stability and collapse on tidally locked rocky planets. doi.org. https://doi.org/10.1051/0004-6361/202037513

2020
Focuses on synchronously orbiting, tidally locked exoplanets with a permanent dayside and dark nightside.
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Labonté, M. & Merlis, T. M. (2020). Sensitivity of the Atmospheric Water Cycle within the Habitable Zone of a Tidally Locked, Earth-like Exoplanet. doi.org. https://doi.org/10.3847/1538-4357/ab9102

2022
Investigates atmospheric circulation on tidally locked rocky planets driven by permanent uneven distributions of stellar radiation.
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Wang, S. & Yang, J. (2022). Atmospheric Overturning Circulation on Dry, Tidally Locked Rocky Planets Is Mainly Driven by Radiative Cooling. doi.org. https://doi.org/10.3847/psj/ac6d65

2023
Analyzes the general atmospheric circulation and energy cycles of tidally locked terrestrial planets under synchronous rotation.
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Wang, S. & Yang, J. (2023). Lorenz Energy Cycle: Another Way to Understand the Atmospheric Circulation on Tidally Locked Terrestrial Planets. doi.org. https://doi.org/10.3847/psj/accf11

What does the evidence say?

The retrieved papers consistently describe tidally locked exoplanets as being in spin-orbit synchronous rotation, creating permanent daysides and nightsides without the cyclic variations in day length and axial tilt that characterize seasonal changes on non-locked planets. None of the provided literature contradicts this consensus.

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