Arid terrestrial planets with less than roughly 20-50% of Earth's ocean water mass cannot sustain a balanced carbon cycle, leading to runaway CO2 buildup and uninhabitable conditions even inside the habitable zone.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Stellar winds from young weak-lined T Tauri stars compress exoplanet magnetospheres to sizes significantly smaller than Earth's, with sizes increasing as stellar activity decays with age.
citing papers explorer
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Carbon Cycle Imbalances on Arid Terrestrial Planets with Implications for Venus
Arid terrestrial planets with less than roughly 20-50% of Earth's ocean water mass cannot sustain a balanced carbon cycle, leading to runaway CO2 buildup and uninhabitable conditions even inside the habitable zone.
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Interaction between Winds from Weak-lined T Tauri Stars with Exoplanetary Magnetospheres
Stellar winds from young weak-lined T Tauri stars compress exoplanet magnetospheres to sizes significantly smaller than Earth's, with sizes increasing as stellar activity decays with age.