Evaluation of the Allochthonous
Model for the Formation of Waulsortian Mud Mounds in
the Sacramento Mountains, South-Central New Mexico
Despite
their high potential and quality as hydrocarbon reservoirs, Waulsortian
mud-mounds remain a poorly understood Mississippian carbonate facies. The mounds
consist of mudstone cores surrounded by halos of crinoid-bryozoan
debris which offer high porosity.
Although the mechanism of mound formation is still controversial, two
end-member hypotheses are proposed: (1) biohermal
buildup and (2) allochthonous sedimentologic
buildup. Although organisms present in mounds are documented, there is no
consistent evidence for organic carbonate mud binding or precipitation. In the allochthonous
model the mound core to flank facies juxtaposition is
created by gravitational slide, glide and flow processes. These processes are associated with a
detachment surface and other predictable structural features such as
extensional structural regimes in up-dip areas, contractional
in the down-dip areas and a zone of translation of blocks connecting the up-
and down-dip regions. Systematic
evaluation of the presence or absence of these predicted features has not been
performed in areas containing Waulsortian mud-mounds
exposures. The goal of this research is
to test the allochthonous model by conducting a detailed
structural characterization of the Mississippian units in the