The role of plume-lithosphere interaction in Hawaii-Emperor chain formation

Paleolatitudes of volcanic rocks reveal that prominent changes in volcanic trend of the Hawaii-Emperor hotspot chain represent meridional migration of the magma source. However, models assuming latitudinal plume migration fail to explain the observed age distribution, rock composition, and erratic p...

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Published inNature communications Vol. 15; no. 1; pp. 6571 - 10
Main Authors Xie, Shijie, Cao, Zebin, Liu, Lijun, Yang, Dinghui, Liu, Mengxue, Li, Yanchong, Qi, Rui
Format Journal Article
LanguageEnglish
Published London Nature Publishing Group UK 03.08.2024
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Summary:Paleolatitudes of volcanic rocks reveal that prominent changes in volcanic trend of the Hawaii-Emperor hotspot chain represent meridional migration of the magma source. However, models assuming latitudinal plume migration fail to explain the observed age distribution, rock composition, and erratic paleolatitude changes of the oldest Emperor seamounts. Here we use data-assimilation models to better reproduce the Hawaii-Emperor hotspot track by systematically considering plate reconstruction, plume-lithosphere interaction, and simplified melt generation and migration. Our results show that plate drag and plume-ridge interaction are both important in explaining the observed seamount ages. These shallow dynamic processes could account for 50% of the observed paleolatitude’s secular reduction and erratic variations over time, where the necessary southward migration of the Hawaiian plume root is significantly less than previously thought. We conclude that plume-lithosphere interaction represents a common mechanism in affecting hotspot track, and has important implications in understanding mantle dynamics and plate reference frames. Plume-ridge interaction modulates plume-lithosphere interaction and leads to hotspot track deviations and paleolatitude offsets in multiple hotspot chains, according to 3D data assimilation models focused on the Hawaii-Emperor hotspot track.
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ISSN:2041-1723
2041-1723
DOI:10.1038/s41467-024-51055-9