• Media type: E-Article
  • Title: Dissociation of Methane into Hydrocarbons at Extreme (Planetary) Pressure and Temperature
  • Contributor: Ancilotto, F.; Chiarotti, G. L.; Scandolo, S.; Tosatti, E.
  • imprint: American Society for the Advancement of Science, 1997
  • Published in: Science
  • Language: English
  • ISSN: 0036-8075; 1095-9203
  • Keywords: Reports
  • Origination:
  • Footnote:
  • Description: <p>Constant-pressure, first-principles molecular dynamic simulations were used to investigate the behavior of methane at high pressure and temperature. Contrary to the current interpretation of shock-wave experiments, the simulations suggest that, below 100 gigapascals, methane dissociates into a mixture of hydrocarbons, and it separates into hydrogen and carbon only above 300 gigapascals. The simulation conditions (100 to 300 gigapascals; 4000 to 5000 kelvin) were chosen to follow the isentrope in the middle ice layers of Neptune and Uranus. Implications on the physics of these planets are discussed.</p>