The Scientists used lasers and X-rays to study liquid carbon, which forms under extreme heat and pressure.
The atomic structure resembles diamond, not a simple liquid, reshaping our understanding.
This discovery aids the planetary science, fusion energy research, and material science by revealing carbon’s behaviour under conditions found in planets and fusion reactors.
Liquid carbon refers to carbon in a liquid state, which is not naturally stable under normal temperature and pressure conditions.
The Carbon typically exists in solid forms like graphite, diamond, or as agas (CO₂) when oxidised.
Carbon does not melt under normal pressure; it transitions directly from solid to gas (sublimation), making lab-based liquid-phase studies almost impossible.
To create liquid carbon, extreme conditions are required, like pressures over 10 million times Earth’s atmosphere and temperatures around 4,500°C.
Traditional methods fail because no material can withstand these conditions without melting.
Liquid carbon atoms have 4 neighbouring atoms each, mirroring the diamond’s structure (but in liquid form).
This challenges earlier assumptions of a simpler liquid structure.
The structure is complex and ordered, akin to water’s hydrogen-bonded network but with covalent bonds.
The experiment has narrowed down carbon’s melting point under high pressure, resolving discrepancies in past theoretical models.
Liquid carbon exists in the cores of the giant planets (e.g., Neptune, Uranus) and white dwarf stars.
Understanding its behaviour improves the very models of the planetary formation and dynamics.
Inertial confinement fusion (a clean energy concept) uses carbon-rich materials.