How insights into 'supercritical fluids' could help us understand the interior of the giant gas planets
The temperature and pressure inside Jupiter range from about -100°C near the edge to about 15,000°C and 50m times the Earth's atmospheric pressure in the middle. Saturn, Uranus and Neptune are similar pressure cookers. As we descend into Jupiter, we may see matter in the gas state, in the liquid state and in another, less well-known state, called the "supercritical fluid" state.
Understanding supercritical fluids is not only important for planetary scientists, it is also used in industrial processes such as power generation and food processing.
When we boil water on Earth, it changes "phase" going from a liquid to a gas state. This is due to a sudden dramatic change in the density and other properties called a "phase transition". However, if you squeezed water to 1,000 times atmospheric pressure and then heated it while keeping the pressure on, you would no longer observe boiling as such. The water molecules would whizz around with more energy, and the density would gradually go down, but there would be no sudden boiling (phase transition). This is what constitutes the supercritical fluid state – it's neither a liquid nor a gas.
Exactly how liquids and supercritical fluids behave has caused scientists to scratch their heads for decades. But new research has shed light on this problem, raising hopes that we can soon gain a much better understanding of what goes on deep inside the giant gas planets.