A 'failed' Runaway Moist Greenhouse: Need help to model...

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SUMMARY

This discussion focuses on modeling an Earth-sized exoplanet with a 'failed' Runaway Moist Greenhouse scenario. The planet, approximately 1.1g in gravity, features a slightly smaller core than Earth, a thicker mantle and crust, and is located near the inner edge of the habitable zone of an Early-K-type star. Key geological features include a Large Igneous Province (LIP) that has outgassed CO2 and H2O, contributing to a basic nitrogen atmosphere. The discussion emphasizes the need for precise pressure and temperature conditions across the lowlands and atop the LIP to understand the planet's inhospitable environment.

PREREQUISITES
  • Understanding of planetary geology and exoplanet modeling
  • Knowledge of atmospheric science, particularly regarding greenhouse effects
  • Familiarity with the concept of Large Igneous Provinces (LIPs)
  • Basic principles of gravitational effects on planetary features
NEXT STEPS
  • Research atmospheric modeling techniques for exoplanets
  • Explore the implications of Large Igneous Provinces on planetary atmospheres
  • Study the effects of gravity on geological formations and tectonics
  • Investigate the characteristics of Early-K-type stars and their habitable zones
USEFUL FOR

Planetary scientists, atmospheric researchers, and astrophysicists interested in exoplanetary conditions and geological modeling will benefit from this discussion.

Nik_2213
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I'm trying to model an Earth-sized exo-planet, ~1.1g, with 'failed' Runaway Moist Greenhouse...
Slightly smaller core than Earth's, with thicker mantle and crust. So, larger than Earth, but not by much.
Sitting near inner-edge of 'Hab Zone' of Early-K-type star, orange-ish rather than Sol's yellow.
Day length ~31 hours due 'solar tides'.
There's sufficient magnetic field to prevent rapid atmospheric 'stripping' as happened on Mars...
Due timing of system's 'Late Heavy Bombardment' equivalent, the planet is 'mostly arid', no vast oceans, just enough for a few 'seas' and Great Lakes.
If was cool enough for such...
And, without ample water to help lubricate tectonics, no 'Terran' multiplicity of subduction zones.
Just one (1) big 'hotspot'. A 'Large Igneous Province'. Think Mars' Olympus complex. Not so tall, though as, despite thicker crust, limited by ~1.1 g gravity.
Still, enough to build 'Shield' the size of Australia, with sundry dormant cones and caldera, some smoking / fizzing vents...
The 'LIP' has out-gassed enough CO2 and H2O to top-up basic N2 'atmosphere' and start planet towards a 'Runaway Moist Greenhouse'.
The lowlands' water evaporated to salt flats and brine pools, think Med's 'Messinian' period, briskly bootstrapping 'Runaway'...
But, then the supply of water ceased, the 'Runaway' stalled...

Okay, another big eruptive 'pulse' from the 'LIP' might provide enough extra atmospheric CO2 + H2O to 'Go the Distance', turn planet to a 'Lesser Venus'.
But, for now, the summits of the cones and rims atop 'LIP' are still 'condensing'.
The volcanic sulphur has long-since washed out of atmosphere.
There are many springs, even a few streams draining acidic pools and volcanic lakes. These run down-hill, either soak in or simply evaporate...
Hmm...
I need pressure & temperature across lowlands to be 'dire', utterly inhospitable, yet conditions atop LIP to be 'condensing' at not more than 2~~3 Bar.
Yes, 'SCUBA ' range, perhaps with a partial Heliox mix...

Sorry, I've tried to 'Do the Math', but it keeps beating me: Is there an 'Atmospheric Scientist' in the room ??
 
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