Dissociation of CH 4 at High Pressures and Temperatures: Diamond Formation in Giant Planet Interiors?

Author:

Benedetti Laura Robin1,Nguyen Jeffrey H.2,Caldwell Wendell A.3,Liu Hongjian3,Kruger Michael4,Jeanloz Raymond35

Affiliation:

1. Department of Physics,

2. H-Division, Physics Directorate, Lawrence Livermore National Laboratory, Livermore, CA 94551, USA.

3. Department of Geology and Geophysics,

4. Department of Physics, 4747 Troost, Room 227, University of Missouri, Kansas City, MO 64110, USA.

5. Department of Astronomy and Miller Institute for Basic Research in Science, University of California, Berkeley, CA 94720, USA.

Abstract

Experiments using laser-heated diamond anvil cells show that methane (CH 4 ) breaks down to form diamond at pressures between 10 and 50 gigapascals and temperatures of about 2000 to 3000 kelvin. Infrared absorption and Raman spectroscopy, along with x-ray diffraction, indicate the presence of polymeric hydrocarbons in addition to the diamond, which is in agreement with theoretical predictions. Dissociation of CH 4 at high pressures and temperatures can influence the energy budgets of planets containing substantial amounts of CH 4 , water, and ammonia, such as Uranus and Neptune.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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