Abstract
Relative abundance of planktic foraminifera from Eastern Arabian Sea (EAS) deep-sea sediment Core SK291/GC17 suggests surface water palaeoceanographic shifts in the EAS during ~25–3.5 calibrated kilo years before present (cal ky BP). The chronology of the studied core is established based on fifteen AMS 14C dates derived from a mixed planktic foraminiferal assemblage and using the ‘Bacon R’ statistical package. Between ~21 and 19 ky BP, the mixed-layer oligotrophic planktic foraminifera, such as
INTRODUCTION
The monsoonal winds play a crucial role in driving upwelling in the Eastern Arabian Sea (EAS) along the western coast of India. In this region, due to the impact of strong Indian Summer Monsoonal winds, nutrient-rich subsurface water comes up to the surface (Wyrtki, 1973). Back in 1985, Zhang conducted the first detailed study about the spatial distribution of living planktic foraminiferal assemblages in the water column of the EAS (~10°N–15°N), which revealed higher planktic foraminiferal abundance, mainly in the upper water column. The variation in the abundance and assemblage of living planktic foraminifera in the EAS seemed to be driven more by upwelling rather than seasonal changes in temperature and salinity (Zhang, 1985). Later on, Naidu et al. (1992) observed a decreasing trend of
STUDY AREA
The deep-sea core sediment (Core SK291/GC17) was collected from off the coast of Goa, EAS (15°07.64′N;72°56.69′E), at a water depth of ~182 m (Figure 1) during the Sagar Kanya expedition number 291 ORV. In the EAS, upwelling generated by the ISM spans from the southernmost margin of the western Indian coastline (~8°N) to the offshore sector of Goa (~15°N) (Rao et al., 2008; Smitha et al., 2008). This process is accompanied by a seasonal shoaling of the thermocline during summer and its subsequent deepening in winter (Antoine et al., 1996).
(a) Chlorophyll a concentration in the EAS in the summer and winter seasons. Maps are prepared using chlorophyll data from NASA Aqua-MODIS Level 3 (https://oceandata.sci.gsfc.nasa.gov/l3/ ) (NASA Goddard Space Flight Centre, Ocean Biology Processing Group, 2023), downloaded from https://oceancolor.gsfc.nasa.gov , in SeaDAS 9.0.1 (NASA Goddard Space Flight Centre, Ocean Biology Processing Group, 2023). (b) A zoomed-in site map showing the bathymetric contours based on ETOPO1 Global Relief Model (Amante & Eakins, 2009). Base map prepared in Ocean Data View software (Schlitzer, Reiner, Ocean Data View, https://odv.awi.de , 2022). (c) Summer monsoon wind vectors from July to September 2017 (Data Set: CCMP monthly v2 (Atlas et al., 2011). Asia-Pacific Data Research Centre (APDRC) Live Access Service (LAS8.6) (https://apdrc.soest.hawaii.edu/las86/ )). The location of Core SK291/GC17 is shown with a solid black square, and the nearby site locations are marked with blue-coloured circles.
In the offshore waters of Goa, a mature stage of upwelling was observed during the peak and waning stages of the ISM (Habeebrehman et al., 2008). Weak to moderately intense upwelling is reported along the coastal sector between Mangalore and Goa, spanning approximately 13°N to 15°N and is mainly confined to the coastal belt (Smitha et al., 2008). As a consequence of ISM wind-induced upwelling, a higher chlorophyll a concentration is seen in summer months, whereas a low chlorophyll a concentration is witnessed during winter months (Figure 1). Additionally, the existence of an intermediate nepheloid layer was found to be associated with high microbial metabolic rates in the EAS (Naqvi et al., 1993) and a benthic nepheloid layer was observed at ~70 m depth on the inner shelf off the Goa coast (Desa et al., 2005). Earlier studies based on the clay mineralogy and sediment transport from the western continental shelf of India suggest long-distance transport of fine-grained sediment along the shelf. In contrast, cross-shelf transport is relatively much less (Ramaswamy & Nair, 1989).
MATERIAL AND METHODOLOGY
A total of 137 samples from the top 1.78 m Core SK291/GC17 (subsampled at 1 cm intervals from top to 100 cm and subsampled at 2 cm intervals from 100 to 178 cm) were analysed to investigate the planktic foraminiferal assemblage. Sediment samples were processed using the method mentioned in Saravanan et al. (2019). The relative abundance studies of major planktic foraminifera species were obtained from an aliquot of around 300 individuals from the >149 µm size fraction (Saravanan et al., 2019). As Peeters et al. (1999) stated that most planktic foraminifera species with a size greater than 149 µm reach the adult stage of ontogeny in the Arabian Sea, we preferred to use this size fraction for our study. Moreover, this standard method has been followed by previous researchers to study planktic foraminiferal assemblages in the western (e.g., Gupta et al., 2003; Ivanova et al., 2003; Naidu & Malmgren, 1995) as well as the EAS (Ivanova et al., 2003; Naik et al., 2017; Saravanan et al., 2020). However, one of the shortcomings of using the >149 µm fraction is the underestimation of both small and large planktic foraminiferal species (Peeters et al., 1999). The taxonomy and census counting of planktic foraminiferal species were performed under a stereo zoom microscope following the methods of Kennett and Srinivasan (1983) and Hemleben et al. (2012). The updated nomenclature of planktic foraminifera species was carried out by using the online database ‘Mikrotax’ (Huber et al., 2017;
The age model for Core SK291/GC17 was established based on 15 14C dates using a mixed planktic foraminiferal assemblage (Majumder, Gupta, Kumar, et al., 2022; Majumder et al., 2024). The raw dates were run in ‘R’ using the ‘Bacon R’ package (Blaauw, 2010; Blaauw & Christen, 2013; Blaauw et al., 2018; R Core Team, 2013). The ‘Bacon R’ package uses an in-built Marine20 calibration curve (Heaton et al., 2020). To account for regional correction, ∇R = 84 ± 51 years (Southon et al., 2002) was applied before running the age-depth model. The mean age per sample is ~120 years. The raw and calibrated ages (see Supplemental Table S1) and the age-depth model discussed by Majumder et al. (2024) are discussed in detail.
RESULTS AND DISCUSSION
In Core SK291/GC17, the major planktic foraminifera species identified and counted are
Box and whisker plot showing the range of relative abundance and mean values of planktic foraminiferal species in Core SK291/GC17, from ~25,000 to 3,500 cal yr BP. Solid grey circles represent the outliers.
Temporal variation in planktic foraminiferal relative abundances
The widespread occurrence of
Schulz et al. (2002) found the highest abundance and flux of
Relative abundance of planktic foraminifera from Core SK291/GC17: (a) Globigerina bulloides (Majumder et al., 2024), (b) Globigerinita glutinata , (c) Oligotrophic group of planktic foraminifera (Globigerinoides ruber + Trilobatus spp.), and (d) Pulleniatina obliquiloculata (Majumder, Gupta, Sanyal, et al., 2022). (e) δ13C (‰, VPDB) of G. ruber in Core SK291/GC17 (Majumder et al., 2024). (f) δ18O (‰, VPDB) of speleothem MWS-2 from Mawmluh cave (Jaglan et al., 2021). (g) G. bulloides (%) in ODP 723A, western Arabian Sea (Gupta, 2008). (h) Relative sea level (m) curve (De Boer et al., 2014) and July solar insolation curve at 65°N (Berger & Loutre, 1991) are shown at the top. Five-point running averages are shown with thick lines (except the topmost panel). Mean values are shown with dotted horizontal lines. The cold intervals are marked with light grey bars, and the warm interval is marked with a light orange bar. The radiocarbon-dated horizons are marked with inverted black triangles.
The second most abundant species in Core SK291/GC17 (Figure 2) is
The most frequent planktic foraminifer in the studied core was
Variability in oligotrophic surface waters off Goa was inferred from the distribution of
In the studied core, though with a low mean abundance (~2.5%),
From ~6.0 to 3.5 kyr BP, the relative population of
Upwelling along the western coast of India
Relative abundance of G. bulloides from different locations along the western continental margin of India. (a) SSD004-GC03, southernmost EAS (Singh et al., 2022), (b) Core SK291/GC15, EAS (Saravanan et al., 2019), (c) Core SK291/GC17, EAS (Majumder et al., 2024), (d) ABP25/02, northern EAS (Gupta et al., 2011). Five-point running averages are shown with thick lines. The cold intervals are marked with light grey bars, and the warm interval is marked with a light orange bar. The radiocarbon-dated horizons are marked with inverted black triangles.
CONCLUSIONS
Relative abundances of planktic foraminiferal records from the studied Core from EAS suggest a substantial shift in surface palaeoceanographic conditions from ~25.0 to 3.50 kyr BP. Between ~21.0 and 19.0 kyr BP, which concurs with the LGM, the oligotrophic, mixed-layer planktic foraminifera like
The SEM images of (1) Globigerinita glutinata (Umbilical view), (2) Orbulina universa (Side view), (3) Trilobatus sacculifer (Umbilical view), (4) Trilobatus sacculifer (Spiral view), (5) Globigerinoides ruber (Umbilical view), (6) Globigerinoides ruber (Spiral view), (7) Globigerina bulloides (Umbilical view), (8) Globigerina bulloides (Spiral view), from Core SK291/GC17.
The SEM images of (1) Globorotalia menardii (Umbilical view), (2) Globorotalia menardii (Spiral view), (3) Globigerinella siphonifera (Side view), (4) Globigerinella siphonifera (Apertural view), (5) Pulleniatina obliquiloculata (Side view), (6) Pulleniatina obliquiloculata (Apertural view), (7) Neogloboquadrina dutertrei (Umbilical view), (8) Neogloboquadrina dutertrei (Spiral view), from Core SK291/GC17.
Footnotes
Acknowledgements
The authors express their gratitude to NCPOR, Goa, for supplying the samples used in this investigation, collected during the Sagar Kanya research cruise SK291. We are thankful to A.D. Singh for his assistance in the taxonomic identification of planktic foraminifera. A.K.G. also acknowledges the support received from ANRF, New Delhi, through the Sir J. C. Bose Fellowship (Grant No. JBR/2021/000019).
Data Availability Statement
All datasets produced from Core SK291/GC17 and used in this study are available through the Zenodo digital repository (Majumder et al., 2025). Previously published information includes the relative abundance of
Declaration of Conflicting Interests
The authors declared no potential conflicts of interest with respect to the research, authorship and/or publication of this article.
Funding
The authors disclosed receipt of the following financial support for the research, authorship and/or publication of this article: JM gratefully acknowledges the Council of Scientific and Industrial Research (CSIR), New Delhi, for awarding the fellowship (SPM-06/081(0258)/2017-EMR-I). AKG appreciates the support received through the Sir J. C. Bose Fellowship (JBR/2021/000019), funded by the Anusandhan National Research Foundation (ANRF), Department of Science and Technology, Government of India, which facilitated this research.
Supplemental Material
References
Supplementary Material
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