Highly Concentrated Nebular Noble Gases in Porous Nanocarbon Separates from the Saratov (L4) Meteorite

Sachiko Amari1,*, Jun-ichi Matsuda2, Rhonda M. Stroud3, and Matthew F. Chisholm4

1McDonnell Center for the Space Sciences and the Physics Department, Washington University, St. Louis, MO 63130, USA
2Department of Earth and Space Science, Osaka University, Osaka 560-0043, Japan
3Code 6360, Naval Research Laboratory, Washington, DC 20375, USA
4Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA

The majority of heavy noble gases (Ar, Kr, and Xe) in primitive meteorites are stored in a poorly understood phase called Q. Although Q is thought to be carbonaceous, the full identity of the phase has remained elusive for almost four decades. In order to better characterize phase Q and, in turn, the early solar nebula, we separated carbon-rich fractions from the Saratov (L4) meteorite. We chose this meteorite because Q is most resistant in thermal alteration among carbonaceous noble gas carriers in meteorites and we hoped that, in this highly metamorphosed meteorite, Q would be present but not diamond: these two phases are very difficult to separate from each other. One of the fractions, AJ, has the highest 132Xe concentration of 2.1 × 10–6 cm3 STP g–1, exceeding any Q-rich fractions that have yet been analyzed. Transmission electron microscopy studies of the fraction AJ and a less Q-rich fraction AI indicate that they both are primarily porous carbon that consists of domains with short-range graphene orders, with variable packing in three dimensions, but no long-range graphitic order. The relative abundance of Xe and C atoms (6:109) in the separates indicates that individual noble gas atoms are associated with only a minor component of the porous carbon, possibly one or more specific arrangements of the nanoparticulate graphene.

Reference
Amari S, Matsuda J-I, Stroud RM and Chisholm MF (2013) Highly Concentrated Nebular Noble Gases in Porous Nanocarbon Separates from the Saratov (L4) Meteorite. The Astrophysical Journal 778:37.
[doi:10.1088/0004-637X/778/1/37]

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