mention new Selsis et al. results #18
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| However, already about $\SIrange{\sim 10}{20} \, \mathrm{bar}$ of water vapor -- corresponding to a minor fraction of one Earth ocean and thus the lower limit of water on Earth -- is enough to sustain sufficiently high surface temperatures to keep the planet in a magma ocean stage~\citep{Boukrouche2021,Lichtenberg2021c}. | ||
| The fraction of planets fulfilling these requirements has an impact on the amplitude of the demographic imprint of the runaway greenhouse transition. | ||
| \revii{It was shown that} already about $\SIrange{\sim 10}{20} \, \mathrm{bar}$ of water vapor -- corresponding to a minor fraction of one Earth ocean and thus the lower limit of water on Earth -- is enough to sustain sufficiently high surface temperatures to keep the planet in a magma ocean stage~\citep{Boukrouche2021,Lichtenberg2021c}. | ||
| \revii{However, recent simulations accounting for radiative–convective profiles suggest the existence of cooler runaway greenhouse states that do not necessarily yield a surface magma ocean~\citep{Selsis2023}. |
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Suggestion for a few minor additions in the last sentence:
"However, recent simulations accounting for radiative–convective profiles of near-surface atmospheric layers suggest the existence of cooler pure-steam runaway greenhouse states that do not necessarily yield a molten surface~\citep{Selsis2023}."
Minor additions directly added
timlichtenberg
approved these changes
Aug 17, 2023
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Here is the compiled article PDF, as well as the PDF with highlighted changes, for the latest commit. You can find additional build output at pull-request-18-pdf. |
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Additions finished, reviewed, and de-bolded. Merging this into |
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