Late Miocene to Present Paleoclimatic and Paleoenvironmental Evolution of the South China Sea Recorded in the Magneto‐Cyclostratigraphy of IODP Site U1505

Author:

Nie Yunfeng123,Wu Huaichun123ORCID,Satolli Sara4ORCID,Ferré Eric C.5ORCID,Shi Meinan123,Fang Qiang123ORCID,Xu Ye6ORCID,Zhang Shihong1ORCID,Li Haiyan1ORCID,Yang Tianshui1ORCID

Affiliation:

1. State Key Laboratory of Biogeology and Environmental Geology China University of Geosciences Beijing China

2. Marine and Polar Research Center China University of Geosciences Beijing China

3. School of Ocean Science China University of Geosciences Beijing China

4. Department of Engineering and Geology University of Chieti‐Pescara Chieti Italy

5. School of Geosciences University of Louisiana at Lafayette Lafayette LA USA

6. Nanjing Institute of Geology and Palaeontology and Center for Excellence in Life and Paleoenvironment Chinese Academy of Sciences Nanjing China

Abstract

AbstractThe continuous sedimentary cores recovered at the International Ocean Discovery Program (IODP) Site U1505, Expedition 368, provide an opportunity for paleoceanography and paleoclimate reconstruction in the continental margin of the northern South China Sea (SCS). In this study, we conducted detailed rock‐ and paleomagnetic studies on 420 discrete samples from the top ∼200 m of the synthetic records of Holes U1505C and U1505D. Rock magnetic analyses indicate that low‐coercivity pseudosingle domain magnetite dominates as the primary ferromagnetic mineral of Site U1505. The magnetostratigraphic age model was constructed by correlating the interpreted polarity sequence with the Geomagnetic Polarity Time Scale 2020 with the constraints of the biostratigraphic data and the distribution probability of the age of each polarity zone provided by a Dynamic Time Warping algorithm. The Milankovitch cycles of the short eccentricity, obliquity, and precession cycles were identified in the magnetic susceptibility (MS) and natural gamma radiation (NGR) series based on paleomagnetic results. We established an ∼9 Myr high‐resolution astronomical time scale by tuning the MS and NGR records to the global oxygen isotope curves, the obliquity, and the eccentricity curves of the La2004 astronomical solution. Our new age model reveals detailed sedimentation rate variations and a ∼500 kyr hiatus across the Brunhes‐Matuyama boundary related to local tectonic activity. These results lay the foundation for understanding the paleoceanography and paleoclimate evolution of the SCS.

Funder

National Natural Science Foundation of China

Ministero dell’Istruzione, dell’Università e della Ricerca

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Atmospheric Science,Oceanography

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