Orbital Forcing and Evolution of the Southern African Monsoon From Late Miocene to Early Pliocene

Author:

de Azevedo Allana Queiroz1ORCID,Jiménez‐Espejo Francisco J.23ORCID,Bulian Francesca45,Sierro Francisco J.4ORCID,Tangunan Deborah6,Takashimizu Yasuhiro7ORCID,Albuquerque Ana Luiza S.1ORCID,Kubota Kaoru3ORCID,Escutia Carlota2,Norris Richard D.8ORCID,Hemming Sidney R.9,Hall Ian R.6ORCID

Affiliation:

1. Programa de Pós‐Graduação em Geoquímica Universidade Federal Fluminense Rio de Janeiro Brazil

2. Instituto Andaluz de Ciencias de la Tierra Consejo Superior de Investigaciones Científicas‐Universidad de Granada Armilla Spain

3. Japan Agency for Marine‐Earth Science and Technology (JAMSTEC) Yokosuka Japan

4. Department of Geology Universidad de Salamanca Salamanca Spain

5. Groningen Institute of Archeology University of Groningen Groningen The Netherlands

6. School of Earth and Environmental Sciences Cardiff University Cardiff UK

7. Mathematical and Natural Sciences Niigata University Niigata Japan

8. Scripps Institution of Oceanography University of California San Diego San Diego CA USA

9. Department of Earth and Environmental Sciences Lamont‐Doherty Earth Observatory New York NY USA

Abstract

AbstractThe late Miocene‐early Pliocene (7.4‐4.5 Ma) is a key interval in Earth's history where intense reorganization of atmospheric and ocean circulation occurred within a global cooling scenario. The Southern African monsoon (SAFM) potentially played an important role in climate systems variability during this interval. However, the dynamics of this important atmospheric system is poorly understood due to the scarcity of continuous records. Here, we present an exceptional continuous late Miocene to early Pliocene reconstruction of SAFM based on elemental geochemistry (Ca/Ti and Si/K ratios), stable isotope geochemistry (δ18O and δ13C recorded in the planktonic foraminiferaOrbulina universa), and marine sediment grain size data from the International Ocean Discovery Program (IODP) Site U1476 located at the entrance of the Mozambique Channel. Spectral characteristics of the Si/K ratio (fluvial input) was used to identify the main orbital forcing controlling SAFM. Precession cycles governed precipitation from 7.4 to ∼6.9 Ma and during the early Pliocene. From ∼6.9 to ∼5.9 Ma, the precession and long eccentricity cycles drove the SAFM. The major Antarctic ice sheet expansion across this interval appear to influence the isotopic records ofO. universaimprinting its long‐term variability signal as a response to the ocean and atmospheric reorganization. Precession cycles markedly weakened from 5.9 to 5.3 Ma, almost the same period when the Mediterranean Outflow Water ceased. These findings highlight important teleconnections among the SAFM, Mediterranean Sea, and other tropical regions.

Funder

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior

Ministerio de Ciencia e Innovación

Universidad de Granada

Universidad de Salamanca

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Atmospheric Science,Oceanography

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