Habitability And Sub Glacial Liquid Water On Planets Of M-dwarf Stars
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A long-standing issue in astrobiology is whether planets orbiting the most abundant type of stars, M-dwarfs, can support liquid water and eventually life.
A new study shows that subglacial melting may provide an answer, significantly extending the habitability region, in particular around M-dwarf stars, which are also the most promising for biosignature detection with the present and near-future technology.
Amri Wandel
Comments: 6 pages, 2 figures, Nature Communications
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Popular Physics (physics.pop-ph)
Cite as: arXiv:2303.04474 [astro-ph.EP] (or arXiv:2303.04474v1 [astro-ph.EP] for this version)
Submission history
From: Amri Wandel
[v1] Wed, 8 Mar 2023 09:46:57 UTC (1,296 KB)
https://arxiv.org/abs/2303.04474
Astrobiology