A subset of isotopically “presolar” carbon
particles
extracted from the Murchison meteorite contain signatures expected
of particles formed in the atmosphere of red giant stars. Some of
these micron-size particles have spherical cores that show diffraction
rings from atom-thick graphene, possibly formed by solidification
of liquid carbon at low pressure. Electron phase-contrast transmission
electron microscopy (TEM) images suggest that these cores originate
from supercooled carbon droplets that formed graphene sheets on randomly
oriented 5-membered loops. In addition to presolar data, laboratory
synthesis in an “evaporating carbon oven” creates similar
core-rim structures by slow cooling of carbon vapor. In research studies,
it was shown that 5-membered loops are essential to the initiation
of carbon nanotubes on catalyst particles. In addition to offering
this experimental context, we present density functional theory (VASP)
computer simulations suggesting that 5-member loops are more likely
than 6-member loops in a solidifying carbon melt. These things suggest
that 5-member loops compete effectively as nucleation seeds for explaining
the faceted pentacones inferred from TEM images of presolar particle
cores. In that context, pent-first nucleation (along with the crowding
of growing sheets by nearby liquid atoms) may reduce the chances of
graphite layer formation and lead to unprecedented diffusion barrier
properties for this composite material.