This is a very good question I think.<br /><br />There are many different "states" of matter - superconductivity, superfluidity, ferromagnetism, diamagnetism etc etc are different phase of matter. So I think you'd be right in saying that there are more states than just solid, liquid, gas and plasma. <br /><br />Re. the gravitational compression turning plasma back into a solid state. The answer is that, yes, it can do that. That is what happens in a white dwarf, a brown dwarf or a neutron star - in these cases the material is in a different (called "degenerate") state of matter that behaves much more like a solid than like a fluid - for a white dwarf or a brown dwarf its probably most similar to a metal. Whether a subtance would be in this state or in the plasma fluid state depends on both the temperature and the density. For a star like the sun, the central temperature is about 15 million K and the density is about 160 g/cm^3 (so 160 times denser than ordinary liquid water at room temperature) - at those values the material would actually still be in the plasma state and would not be degenerate. As the sun evolves its center collapses, and the density increases. For a smaller star like the sun, at some point its temperature won't be hot enough to prevent the material at the high density from undergoing a phase change into the degenerate state, at that point the sun stops evolving and it ends its life as a white dwarf. More massive stars can have much hotter temperatures that allow them to have much higher densities. These stars can continue to collapse and evolve until they enter the neutron-matter state, or in the case of exceptionally large stars they collapse into a black hole. <br /><br />Actually, the sun will likely enter a degenerate state even before it ends up as a white dwarf - as a red giant its core becomes degenerate and undergoes a run-away nuclear reaction which gives rise to the so-called helium flash which will bring it back into the plasma state <div class="Discussion_UserSignature"> </div>