Nick,
Firstly emission temperature is to the 1/4 power of the temperature. So 0.05 watts works out as 30.64 K effective temperature - ignoring opacity issues. If the heat-flow is higher, from radioactives or gravitational energy, then the effective temperature is, of course, higher too. A 1 watt heat-flow means a 64.8 K effective temperature - enough to keep even nitrogen from chilling out as puddles at 1 bar.
Thus hydrogen actually remaining stable as ice or liquid requires very low heat-flows from a planet's interior - if it is big enough to capture any during formation that is. I'd say if it's big enough to retain a significant free hydrogen atmosphere then it'll be warm enough to keep it all gaseous, with the consequent stratified atmosphere.
Space/Science » in reply to It depends whether it is IMPORTANT or not
au contraire
The whole thread (39 posts)
- Regarding earthlike planets
- re: Resonance
- ejection
- life on ejected planets
- re: life on ejected planets. - Ejected planets is one thing...
- Monitoring globular star clusters
- life on ejected planets
