Tectonic synthesis of the Olympic Mountains segment of the Cascadia wedge,using two-dimensional thermal and kinematic modeling of thermochronological ages
Ge. Batt et al., Tectonic synthesis of the Olympic Mountains segment of the Cascadia wedge,using two-dimensional thermal and kinematic modeling of thermochronological ages, J GEO R-SOL, 106(B11), 2001, pp. 26731-26746
A fully coupled two-dimensional kinematic and thermal model of a steady sta
te accretionary wedge, constrained by an extensive data set of fission trac
k and (U-Th)/He ages for apatite and zircon, is here used to investigate th
e development of the Olympic Mountains segment of the Cascadia accretionary
wedge. The model has two main free parameters: (epsilon) over dot(max), th
e maximum rate of erosion for a generic erosion function operating at the t
op of the wedge, and alpha, the distribution of sedimentary accretion into
the wedge. The best fit values for (epsilon) over dot(max), and alpha and t
heir confidence limits are determined through an iterative search of parame
ter space. This study represents the first time that such inversion methods
have been used to quantify the thermal-kinematic evolution of an accretion
ary wedge. Our results suggest that horizontal transport plays an important
role in the exhumation trajectories experienced by material passing throug
h the Cascadia wedge. At a 95% confidence interval, 80 to 100% of the sedim
entary sequence from the subducting Juan de Fuca Plate has been accreted at
the front of the wedge offshore of the Olympics over the past 14 m.y. This
frontally accreted material must then traverse the entire width of the wed
ge prior to its eventual exposure in the Olympic forearc high. Assessed in
this two-dimensional framework, the fission track and (U-Th)/He age data se
ts from the Olympic Mountains are all best fit by (epsilon) over dot(max) o
f 0.9-1.0 mm yr(-1), despite variation in the timescales relevant to Mounta
ins are all best fit by the three chronometers. This result supports the hy
pothesis that the Olympic Mountains segment of the Cascadia accretionary we
dge has been in a flux steady-state since similar to 14 Ma. The demonstrati
on of a flux balance across the Cascadia margin also suggests that margin-p
arallel transport has not had a significant role in driving uplift of the O
lympic Mountains.