Discs around 0.1 M⊙ M-dwarfs form all their planetesimals within the 26Al half-life, so the resulting planetesimals—and likely rocky planets—are dehydrated and volatile-poor.
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Planetesimal Formation Across the Stellar Mass Spectrum and its Influence on Exoplanet-Inherited Volatile Budgets
Discs around 0.1 M⊙ M-dwarfs form all their planetesimals within the 26Al half-life, so the resulting planetesimals—and likely rocky planets—are dehydrated and volatile-poor.