COMPARISON OF CRETACEOUS VS. EOCENE GRANITOID INTRUSIONS IN NE WASHINGTON: PETROLOGY AND AL-IN-HORNBLENDE BAROMETRY
SiO2 contents overlap considerably between the Eocene (NN = 65.7 – 67.2 wt. %; HM = 55.9 – 68.6 wt. %) and Cretaceous plutons (TC =57.8 –69.6 wt. %; CS ~74 wt. %). Spidergrams for all four plutons show Ta and Nb depletions and LILE enrichments characteristic of arc magmas. REE plots, although variable, show the Eocene plutons have steeper REE slopes (La/YbN = 4.9-17.2) and smaller Eu anomalies (Eu/Eu* =1.0-0.81) than the Cretaceous plutons (La/YbN = 2.9-4.1; Eu/Eu* = 0.62-0.57). The Eocene plutons also have slightly higher Na at equivalent SiO2 contents. Al-in-hornblende barometry reveals a slightly deeper emplacement depth (1.5±0.7 Kb) for TC (~88 Ma; Todd, 1989) compared to 0.64±0.4 Kb for the NN (63.9±0.7 Ma U-Pb; Tepper unpublished data) and HM (44.5±0.9 Ma K-Ar; Barksdale, 1975). These results indicate that <~5 km of uplift have occurred in this area since ~88 Ma. We conclude that the Cretaceous and Eocene plutons were derived from similar source(s) and that any thickened crust that may have developed during the Cretaceous was in this area largely eroded by ~88 Ma.