BP said:Thanks GJD, nice article - but the quote above refers to a 'designation' of the end of the troposphere and the source abstract is about the Galileo probe - so I think the pressure is too low at those temps to 'liquefy hydrogen'. Google-ing didn't turn up much for me, except (for Saturn)Wikipedia said:Since the lower boundary of the atmosphere is ill-defined, the pressure level of 10 bars, at an altitude of about 90 km below the 1 bar pressure level with a temperature of around 340 K, is commonly treated as the base of the troposphere
Given the temps here the problem as I understand it (or don’t :? ) is that its not really 'liquid' so much as 'liquid-like' (supercritical liquid) - so no surface tension and its compressible like a gas, but otherwise acts like a solvent. My layman’s knowledge is useless here and the stuff I googled is confusing and contradictory.. (no nice equations/tables)http://www.britannica.com/EBchecked/topic/525169/Saturn/54280/The-interior said:Under the conditions found within the planet, hydrogen behaves as a liquid rather than a gas at pressures above about one kilobar, corresponding to a depth of 1,000 km (600 miles) below the clouds; there the temperature is roughly 1,000 K (1,340 °F, 730 °C).
Granted, the change is gradual and far from clearly defined at any point, or, come to that, observed, but the point is you don't NEED it to have kilobar pressures or thousands of Kelivin to get normal, liquid hydrogen. The phase change will happen within the mid reaches of the troposphere in localised areas.
However, why bother with all that tedious mucking about with kilo Kelvin temperatures and tens or hundreds of atmospheres to skim for liquid hydrogen? If the magic fuel processor can crack seawater to hydrogen, then filtering, chilling and compressing gaseous hydrogen to Lhyd in the tanks should be a piece of cake. Just do it up higher where the atmosphere is still H2 and all its its naughty hydrocarbon, ice, ammonia and methane buddies, but rarefied.
G.