Abstract
The Hawaiian-Emperor seamount chain in the Pacific Ocean has provided fundamental insights into hotspot generated intraplate volcanism and the long-term strength of oceanic lithosphere. However, only a few seismic experiments to determine crustal and upper mantle structure have been carried out on the Hawaiian Ridge, and no deep imaging has ever been carried out along the Emperor seamounts. Here, we present the results of an active source seismic experiment using 29 Ocean-Bottom Seismometers (OBS) carried out along a strike profile of the seamounts in the region of Jimmu and Suiko guyots. Joint reflection and refraction tomographic inversion of the OBS data show the upper crust is highly heterogeneous with P wave velocities <4–5 km s−1, which are attributed to extrusive lavas and clastics. In contrast, the lower crust is remarkably homogeneous with velocities of 6.5–7.2 km s−1, which we attribute to oceanic crust and mafic intrusions. Moho is identified by a strong PmP arrival at offsets of 20–80 km, yielding depths of 13–16 km. The underlying mantle is generally homogeneous with velocities in the range 7.9–8.0 km s−1. The crust and mantle velocity structure has been verified by gravity modeling. While top of oceanic crust prior to volcano loading is not recognized as a seismic or gravity discontinuity, flexural modeling reveals a ∼5.0–5.5 km thick preexisting oceanic crust that is overlain by a ∼8 km thick volcanic edifice. Unlike at the Hawaiian Ridge, we find no evidence of magmatic underplating.
Original language | English (US) |
---|---|
Article number | e2020JB021109 |
Journal | Journal of Geophysical Research: Solid Earth |
Volume | 126 |
Issue number | 3 |
DOIs | |
State | Published - Mar 2021 |
Keywords
- gravity and isostasy
- marine geology & geophysics
- marine seismics
- oceanic hotspots and intraplate volcanism
- seafloor morphology
ASJC Scopus subject areas
- Geophysics
- Geochemistry and Petrology
- Earth and Planetary Sciences (miscellaneous)
- Space and Planetary Science
Fingerprint
Dive into the research topics of 'Seismic Structure, Gravity Anomalies and Flexure Along the Emperor Seamount Chain'. Together they form a unique fingerprint.Datasets
-
Seismic refraction and wide-angle data along Emperor Seamounts (Northwest Pacific) from profile P02 of RV Marcus G. Langseth cruise MGL1902
Watts, A. B. (Contributor), Grevemeyer, I. (Contributor), Shillington, D. J. (Contributor), Dunn, R. A. (Contributor) & Gómez de la Peña, D. L. P. L. (Contributor), PANGAEA, Sep 30 2024
DOI: 10.1594/PANGAEA.926068, https://doi.pangaea.de/10.1594/PANGAEA.926068
Dataset