An anthracite coal (Romax = 5.27%, fixed carbon = 95.5%) was deformed
in the steady state at various pressures, temperatures, and experiment
al configurations to assess the effects of stress, strain, and strain
energy on graphitization. In simple shear tests, graphite first appear
s at temperatures as low as 600 degrees C and samples tested at 900 de
grees C are predominately graphitized, as evident from optical microsc
opy, XRD, and transmission electron microscopy. The graphite is lamell
ar, has punctual hkl reflections or Debye-Scherrer (hkl) rings (triper
iodic order), and long stiff and stacked lattice fringes typical of we
ll-crystallized graphite. No graphite was formed in either hydrostatic
or coaxial tests (they remain porous and turbostratic), although incr
eased orientation of the basic structural units (BSUs) and increase in
size of molecular orientation domains (MOD), attributed to the coales
cence of neighboring pore walls, is evident in some coaxial deformed s
amples. Micro-Raman spectroscopy of deformed samples indicates the ong
oing presence of defects (band at 1350 cm(-1)), even in samples that b
y XRD and TEM prove to be mainly graphite. Results of our experiments
indicate the independence of stress and the dependence on strain and s
train energy in the formation of graphite. Samples deformed in simple
shear at 900 degrees C are more highly graphitized than a sample heate
d to 2800 degrees C (HTT) at ambient pressure. Simple shear tests, in
particular, have imparted strain energy resulting in rupturing of pore
walls, flattening of pores, and mechanical rotation of stacks of basi
c structural units (BSUs). These processes facilitate preferred parall
el orientation of pore walls, coalescence of pores and, thus, growth o
f aromatic sheets leading to the formation of graphite. We propose tha
t a major component of the activation energy required for graphitizati
on in our experiments and, by analogy in nature, is provided by strain
energy. The occurrence of natural graphite in rocks that have never b
een subjected to temperatures in excess of about 300 degrees C may be
accounted for by strain energy imparted during tectonic deformation.