Extended Habitability of Exoplanets Due to Subglacial Water
Considering subglacial liquid water, a significant extension of the classical Habitable Zone is obtained. Elaborating on the model of Wandel it is shown how an atmosphere and liquid water could survive on tidally locked planets closely orbiting an M-dwarf host, extending the Habitable Zone boundary...
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| Hlavní autor: | |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
IOP Publishing
2023-01-01
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| Edice: | The Astronomical Journal |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/1538-3881/ad0045 |
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