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Extreme Water Loss and Abiotic O(2) Buildup on Planets Throughout the Habitable Zones of M Dwarfs

We show that terrestrial planets in the habitable zones of M dwarfs older than ∼1 Gyr could have been in runaway greenhouses for several hundred million years following their formation due to the star's extended pre-main sequence phase, provided they form with abundant surface water. Such prolo...

पूर्ण विवरण

में बचाया:
ग्रंथसूची विवरण
में प्रकाशित:Astrobiology
मुख्य लेखकों: Luger, R., Barnes, R.
स्वरूप: Artigo
भाषा:Inglês
प्रकाशित: Mary Ann Liebert, Inc. 2015
विषय:
ऑनलाइन पहुंच:https://ncbi.nlm.nih.gov/pmc/articles/PMC4323125/
https://ncbi.nlm.nih.gov/pubmed/25629240
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1089/ast.2014.1231
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