The principal isoprenoid hydrocarbons in flash pyrolysates from immature ke
rogens are prist-1-ene and, to a lesser extent, prist-2-ene. The precise or
igin of these compounds is still a matter of debate. Chemical degradation e
xperiments performed on a sulfur-rich kerogen in this study show that at le
ast two precursors can generate pristenes during pyrolysis of sulfur-rich k
erogens: ether-bound precursors, probably tocopherols, and a sulfur-bound p
recursor. From pyrolysis experiments performed on mixtures of isolated kero
gens with different clay minerals, it is concluded that prist-2-ene is like
ly formed by the double-bond isomerization of prist-1-ene. This isomerizati
on of prist-1-ene into prist-2-ene depends on the amount of protons availab
le for the formation of the intermediate carbonium ion. These protons can b
e derived from acidified aluminosilicates (e.g, the clay minerals montmoril
lonite or kaolinite) in the rock or from inorganic acids (e.g. HI, HCl). Th
e degree of isomerization depends on the amount of protons available relati
ve to the total organic carbon content. (C) 2001 Elsevier Science B.V. All
rights reserved.