As you descend into the atmosphere of Jupiter, you'll encounter the cloudtops at right around 1 atm (coincidence). The temperature there is way cold, about 160 K. Over the next 100 km or so, the temperature inceases at about 2 K/km but the pressure is building up as well. The atmosphere is mostly H2 and He, of course. As you go deeper and the pressure increases, this gas just gets denser and denser without ever becoming a liquid because it is above its critical temperature.
I don't have the depths available to me here, but as the pressure builds, the gas becomes much denser than water and, at even deeper, becomes a metal. Once again, it isn't really a liquid, gas or solid; just a supercritical fluid. A little hard to imagine. That big hunk of hydrogen metal is where Jupiter gets its immense magnetic field.
Near the center is a little Earth-sized silicate rocky core, but the "atmosphere" around it is a very hot, super high P metallic H2/He material. Not really a solid, but much denser than a liquid. The exact depths and compositions aren't really known because we don't know much about the behavior of hydrogen at those temperatures and, especially, pressures.