The Emperor seamounts form part of the hotspot generated Hawaiian-Emperor seamount chain in the Pacific Ocean. The fixed hotspot hypothesis (Morgan, 1971) suggests the chain formed at a deep mantle hotspot presently located off the southeast flank of Hawai'i, in the vicinity of Loih'i seamount. Differences in orientation between the Hawaiian Ridge and the Emperor seamounts have been attributed to changes in the direction of absolute motion of the Pacific plate from more northerly during 50-83 Ma to more westerly during 0-50 Ma (Morgan, 1971). Paleomagnetic data from Deep Sea Drilling Project (DSDP) drill and sample sites, however, suggest that while the Hawaiian Ridge, which includes the Hawaiian Islands, formed close to the present day latitude of Loih'i, paleolatitudes progressively increase from ∼2° at Koko, through ∼8° at Suiko, to ∼19° at Detroit indicating that the Hawaiian hotspot may have migrated south during emplacement of the Emperor seamounts rather than stayed fixed (Tarduno et al., 2003). Subsequent studies have suggested that the Hawaiian-Emperor seamount chain formed by some combination of changed Pacific plate motions and hotspot wander (