Crustal Structure of the Northeast South China Sea Rifted Margin

Author:

Rodrigues de Vargas Mateus1ORCID,Tugend Julie12ORCID,Mohn Geoffroy1ORCID,Kusznir Nick3ORCID,Liang‐Fu Lin4ORCID

Affiliation:

1. Géosciences et Environnement Cergy (GEC) CY Cergy Paris Université Neuville‐sur‐Oise France

2. Commission for the Geological Map of the World Paris France

3. Department of Earth, Ocean and Ecological Sciences University of Liverpool Liverpool UK

4. Ocean Center National Taiwan University Taipei Taiwan

Abstract

AbstractWe investigate the crustal structure of the Northeastern (NE) South China Sea (SCS) rifted margin to constrain its crustal thickness and basement nature with implications for the Mesozoic and Cenozoic evolution of the SCS. First‐order interfaces interpreted from seismic reflection data were integrated into a 3D gravity inversion scheme to determine Moho depth and crustal thickness variations. A joint inversion of seismic and gravity data allowed us to determine crustal density variations along 2D profiles. The distal margin of the NE SCS is divided into two distinct crustal domains: the Southern Rift System (SRS), and the Southern High (SH). The SRS shows an extremely thinned crust on top of which thick Cenozoic sequences are observed. It is separated from the oceanic crust (∼6–8 km thick) by the SH, a comparatively thicker crustal domain (∼10–15 km thick) with significant magmatic additions. The distal NE SCS margin formed during the Cenozoic rifting of the SCS. The SH likely corresponds to a polygenic piece of crust, recording polyphase magmatic activity since the Mesozoic, with potentially significant activity during Cenozoic post‐rift time. The NE SCS margin is conjugate to Palawan whose basement is considered to be part of the exotic Luconia microcontinent that collided with Eurasia during the Late Cretaceous. Basement similarities between Palawan and the SH are highlighted, suggesting that the latter might also be part of Luconia. Our results suggest that the docking/suture zone between Eurasia and Luconia might have acted as a preferred zone for the Cenozoic rift development.

Funder

Agence Nationale de la Recherche

Publisher

American Geophysical Union (AGU)

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