Hmm, according to the last astronomy book I bought (back in 1991 or 1992), both Uranus and Neptune were speculated to have an "ocean mantle"; i.e. a rocky core surrounded by water that is many many miles deep.
Yes, exactly.
At the top of the clouds (ionosphere?) the temperature for both worlds is around 58 to 57 K. That's cold! Which leads one to speculate about the "biosphere"; i.e. the surface of the ocean; is there a hard frozen surface that is constantly cooled, or is there a tumultuous massive ocean there that is constantly whipped into a frenzy by mach 1 winds?
Note in your 2nd (Uranus) diagram, the "surface" is being designated as the interface between the gaseous atmosphere and the liquid mantle. The ocean-surface is noted as having a temperature of 2300oC (unless I am misreading the diagram). The atmospheric height above the liquid mantle in the Uranus diagram is also less than the atmospheric height in the Neptune diagram, meaning that Neptune has much more atmosphere above its liquid-mantle "surface", and therefore, higher surface pressure than Uranus.
Now, of course, a Neptunian exo-planet need not be similar to either of these.
Loose tangent; the rules as to how much pressure a starship can take would seem to allow a type S 100 ton scout to land on a Neptune or Venus, though it would be a very rough ride once you were down.
Which ruleset are you referencing?
Loose tangent 2; per my previous reference to Venus to clarify astronomical jargon, here's a cleanup processed picture from the Soviet Mariner probe;
Mariner was a NASA probe series; The corresponding Soviet program were the Venera probes. The pictures above look like they came from Venera 9 or 10.
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