Paleomagnetism of the Southern Crescent Formation, Olympic Peninsula, Washington
Megan Young
The mechanism of curvature for the Crescent Formation has been a subject of debate since the geology of the Olympic
Peninsula was first studied. The Crescent Formation is an extraordinarily large swath of basalts that lies along the
northern, eastern, and southeastern sides of the Olympic Peninsula. Although it is grouped as part of the Coast Range
basalts, recent paleomagnetic studies of the northern part of the Crescent Formation suggest that it has a regional
tectonic history distinct from other Coast Range basalts to the south. Previous attempts at paleomagnetic studies in
the southern Crescent Formation have not yielded stable paleomagnetic directions. The majority of cores obtained for
this study possessed stable magnetic directions, but scatter within each site is large. Comparison of the site mean
directions with the expected middle Eocene pole for North America (82.8° north latitude, 170.4° east longitude)
suggests that the sites have undergone some tilting and rotation, although the large directional scatter within each
site prevents an accurate measurement of the amount of rotation and tilt. The inclinations and declinations obtained
from the sites show different directions of rotation within a small area and also show inclinations inconsistent with
any plausible model of regional deformation. These inconsistencies suggest that the areas sampled contain more
structural complexities than simple bedding tilt, and that the site mean directions may reflect local, rather than
regional, deformation and rotation.
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