GROWTH FAULTING WITHIN THE PENNSYLVANIAN HERMOSA GROUP, COAL BANK PASS – MOLAS PASS, SAN JUAN MOUNTAINS, COLORADO
In order to more accurately constrain the activity of the Snowdon Fault, a stratigraphic section within the syncline was measured and compared to multiple sections across the faults. There is roughly 10 meters of thickness difference in the lower third of each section. The top of this growth faulted interval is correlated to the top of sequence 3 of Gianniny, and Miskell-Gerhardt, (2009). The lack of deformation between the syncline section and the Coal bank Hill section (Spoelhof, 1974) above this bed indicates that the fault became inactive before sequence 4 deposition. Up section, in sequence 10 and 11 the Snowdon Fault was reactivated during deposition. The beds of sequence 10 and 11 are much thicker and become clastically dominated across the Snowdon Fault to the north. These beds transition from paleosols and thin shallow water carbonates on the Engineer section to thick mud dominated carbonates and thick clastic packages on the syncline section; which may indicate a fault controlled paleo-valley.
Comparing the Coal Bank Hill section to the Engineer section across of the Coal bank fault, there is roughly 30 meters of thickness difference in the lower third of the section. This difference also disappears by the base of sequence 4. This indicates that the Coal Bank Fault was also active during sequence 1 through sequence 3 deposition of the Hermosa Group.
This study helps to distinguish Pennsylvanian syndepositional faulting from post-depositional Laramide faulting and builds on the previous work of Baars and See, 1967, Girdley, 1969, Spoelhof, 1974, Evans, 2002, and Thomas, 2007.