Holocene climate variability deciphered from Chilika Lagoon sediments: Implication for anthropogenic activity or paleocyclones?
• High energy event post ∼1.1 Ka is recorded in the lacustrine sediments of Chilika. • Indian summer monsoon was high during the early Holocene. • CaCO 3 content and F2 values suggest the formation of barrier spit post ∼4 Ka. • High physical weathering dominated during ∼4 Ka arid period. Coastal lagoons, acting as a link between land and sea, serve as valuable archives for past climate variations, human activities, and paleo-cyclonic events. In this study, we employ a multi-proxy approach to analyze sedimentary records and uncover climatic shifts influenced by both monsoonal and non-monsoonal factors. Our analysis incorporates sediment characteristics such as grain size, magnetic susceptibility (MS), and clay mineralogy to infer high-energy conditions within the Chilika Lagoon. Additionally, we utilize Rock-Eval pyrolysis and deconvolution of flame ionization detector (FID) signals to determine the type of organic matter (OM) present. Findings reveal that during the Early Holocene, a high sand percentage and elevated MS indicate an intensified monsoon, coinciding with a dominance of terrestrial OM. However, as monsoonal intensity declined after the Early Holocene, marine OM became more prevalent, likely linked to the formation of an estuary around ∼7.7 Ka. Despite a weakening monsoon around ∼4 Ka, MS values remained high, possibly due to increased aeolian input, which transported titanomagnetite, contributing to elevated MS in the sediment record. After ∼4 Ka, the sedimentary record indicates a greater influx of terrestrial OM, likely due to the formation of a barrier spit that limited marine influence. From this period onward, monsoonal intensity gradually increased, peaking around ∼1.1 Ka, coinciding with the Medieval Warm Period. Following ∼1.1 Ka, sedimentation rates rose, accompanied by low magnetic susceptibility (MS) and high sand content. This phase also shows an increase in both terrestrial and marine OM, along with higher CaCO₃ and illite concentrations, suggesting the impact of high-energy events, possibly cyclones. The intensification of cyclonic activity after ∼1.1 Ka may be associated with a weakening of El Niño–Southern Oscillation (ENSO) intensity during this period.
Authors
- Mohd Amir
- Abdul Hameed (ORCID: https://orcid.org/0000-0002-2523-3236)
- Monalisa Mallick (ORCID: https://orcid.org/0000-0003-1249-7483)
- Nihar Ranjan Kar (ORCID: https://orcid.org/0000-0001-9128-2506)
- Pankaj Kumar (ORCID: https://orcid.org/0000-0001-7050-582X)
- Luan Carlos de Sena Monteiro Ozelim (ORCID: https://orcid.org/0000-0002-2581-0486)
- M. Venkateshwarulu
- K. Venkatesham
- Prem Chand Kisku
- Debajyoti Paul (ORCID: https://orcid.org/0000-0001-5737-3826)
- Barnita Banerjee
- Elapavalooru V.S.S.K. BABU (ORCID: https://orcid.org/0000-0002-3474-8864)
- Aurovinda Panda
- Tanveer Hassan
- Vireswar Samanta
Institutions
- University of Delhi (IN)
- National Sun Yat-sen University (TW)
- Universidade de Brasília (BR)
- National Geophysical Research Institute (IN)
- Inter-University Accelerator Centre (IN)
- Indian Institute of Technology Kanpur (IN)
- Academy of Scientific and Innovative Research (IN)
Publication Details
- Journal
- Geosystems and Geoenvironment
- Published
- 2025-04-06
- DOI
- https://doi.org/10.1016/j.geogeo.2025.100390
- Primary Topic
- Geology and Paleoclimatology Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00