No Snowball Cycles at the Outer Edge of the Habitable Zone for Habitable Tidally Locked Planets

Planets orbiting within the habitable zones of M stars are prime targets for future observations, which motivates a greater understanding of how tidal locking can affect planetary habitability. In this Letter we will consider the effect of tidal locking on limit cycling between snowball and warm cli...

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Veröffentlicht in:	Astrophysical journal. Letters 2019-12, Vol.887 (1), p.L3
Hauptverfasser:	Checlair, Jade H., Salazar, Andrea M., Paradise, Adiv, Menou, Kristen, Abbot, Dorian S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Activated carbon Astrobiology Carbon cycle Carbon dioxide Circumstellar habitable zone Climate models Cycles Exoplanet astronomy Exoplanet atmospheres Exoplanets Global climate Global climate models Habitability Habitable planets Irradiation Locking M stars Outgassing Planetary rotation Planets Three dimensional models Tidal effects Warm climates Weathering
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