Thermocline state change in the eastern equatorial Pacific during the late Pliocene/early Pleistocene intensification of Northern Hemisphere glaciation
- 1Institute of Earth Sciences, Heidelberg University, 69120 Heidelberg, Germany
- 2Institute of Geosciences, Goethe University Frankfurt, 60438 Frankfurt, Germany
Correspondence: Kim Alix Jakob (firstname.lastname@example.org)
The late Pliocene/early Pleistocene intensification of Northern Hemisphere glaciation (iNHG) ∼2.5 million years ago (marine isotope stages, MIS, 100–96) stands out as an important tipping point in Earth's climate history, which strongly influenced oceanographic and climatic patterns including trade wind and upwelling strength in the eastern equatorial Pacific (EEP). The thermocline depth in the EEP, in turn, plays a pivotal role in the Earth's climate system: small changes in its depth associated with short-term climate phenomena such as the El Niño–Southern Oscillation can affect surface-water properties and the ocean–atmosphere exchange. However, thermocline dynamics in the EEP during the iNHG still remain unclear. While numerous studies have suggested a link between a thermocline shoaling in the EEP and Northern Hemisphere ice growth, other studies have indicated a stable thermocline depth during the iNHG; consequently, a causal relationship between thermocline dynamics and ice-sheet growth has been excluded. In light of these contradictory views, we have generated geochemical (planktic foraminiferal δ18O, δ13C and Mg ∕ Ca), sedimentological (sand accumulation rates) and faunal (abundance data of thermocline-dwelling foraminifera) records for Ocean Drilling Program Site 849 located in the central region of the EEP. Our records span the interval from ∼2.75 to 2.4 Ma (MIS G7–95), which is critical for understanding thermocline dynamics during the final phase of the iNHG. Our new records document a thermocline shoaling from ∼2.64 to 2.55 Ma (MIS G2–101) and a relatively shallow thermocline from ∼2.55 Ma onwards (MIS 101–95). This indicates a state change in thermocline depth at Site 849 shortly before the final phase of the iNHG. Ultimately, our data support the hypothesis that (sub-)tropical thermocline shoaling may have contributed to the development of large Northern Hemisphere ice sheets.
The onset and intensification of Northern Hemisphere glaciation during the late Pliocene and early Pleistocene (∼3.6–2.4 Ma; Mudelsee and Raymo, 2005) is part of a long-term cooling trend following the mid-Piacenzian warm period. The glacial corresponding to marine isotope stage (MIS) G6 (∼2.7 Ma) is often considered to mark the onset of large-scale glaciation in the Northern Hemisphere, as it is characterized by the first occurrence of ice-rafted debris in the North Atlantic Ocean (Bartoli et al., 2006; Bailey et al., 2013). The first culmination in Northern Hemisphere ice buildup occurred at ∼2.5 Ma as documented by the first three large-amplitude (∼1 ‰ in the benthic δ18O record) glacial–interglacial cycles (MIS 100–96) that indicate substantial waxing and waning of ice sheets (Lisiecki and Raymo, 2005). At that time, ice rafting became widespread across the North Atlantic Ocean (Shackleton et al., 1984; Naafs et al., 2013). This so-called “intensification of Northern Hemisphere glaciation” (iNHG) represents an important tipping point in Earth's climate history. It strongly influenced oceanographic and climatic patterns worldwide, affecting, for example, the amount of biological production in the eastern equatorial Pacific Ocean (EEP) (Etourneau et al., 2010; Jakob et al., 2016) – a region that exerts a strong influence on the Earth's climate system through its effects on the global carbon and nutrient cycles (e.g., Schlitzer, 2004; Takahashi et al., 2009).
Within the EEP, the position of the thermocline in the water column bears important consequences for the Earth's climate system. Today, it is poised at shallow depths. As a consequence, small changes in its depth through east–west tilting regulated by short-term climate phenomena such as the El Niño–Southern Oscillation can affect surface-water properties and ocean–atmosphere exchange processes (Fedorov et al., 2004; Ma et al., 2013). In general, proxy records and modeling results consistently document a long-term shoaling of the thermocline in the EEP and other (sub-)tropical upwelling regions throughout the Plio-Pleistocene (Wara et al., 2005; Fedorov et al., 2006; Steph et al., 2006a, 2010; Dekens et al., 2007; Ford et al., 2012). However, the dynamics of the thermocline in the EEP and its potential links to the iNHG currently remained enigmatic. Some studies have inferred that the thermocline depth reached a critical threshold at ∼3 Ma, which allowed trade winds to deliver cool waters from below the thermocline to the surface in (sub-)tropical upwelling regions such as the EEP (Fedorov et al., 2006; Dekens et al., 2007). The timing led to the hypothesis that thermocline shoaling and the development of the EEP “cold tongue” (Wyrtki, 1981) were necessary preconditions for the iNHG, as they reduced poleward atmospheric heat transport (Cane and Molnar, 2001). However, other studies only identified fundamental shifts in the thermocline depth prior to ∼3.5 Ma (Wara et al., 2005; Steph et al., 2006a, 2010; Ford et al., 2012), which would imply that the thermocline depth in the EEP did not play an important role in the development of large-scale glaciation in the Northern Hemisphere. In light of these contradictory views, and to ultimately shed new light on potential links between low-latitude thermocline dynamics and high-latitude ice-sheet buildup, we investigated thermocline state changes for Ocean Drilling Program (ODP) Site 849 in the EEP during the final phase of the late Pliocene/early Pleistocene iNHG (∼2.75 to 2.4 Ma, MIS G7–95).
2.1 The eastern equatorial Pacific
The EEP has considerable relevance for the Earth's atmospheric and marine carbon budget (Toggweiler and Sarmiento, 1985; Takahashi et al., 2009), and simultaneously exerts strong control on oceanographic and climatic circulation patterns (Fedorov and Philander, 2000; Pennington et al., 2006). Today, as a part of the tropical Pacific Walker circulation, westward-blowing trade winds induce a year-round upwelling of cold waters from below the thermocline to the surface in the EEP. This results in a thin, nutrient-enriched and relatively cold (∼23 ∘C; Locarnini et al., 2013) mixed layer, the so-called EEP “cold tongue” (Wyrtki, 1981) (Fig. 1a, b). In today's oceans, this upwelling system supports more than 10 % of the global biological production (Pennington et al., 2006). Relatively high primary productivity rates result in exceptionally high sedimentation rates, which have amounted to up to 3.0 cm kyr−1 during the past 5 Myr (Mayer et al., 1992; Mix et al., 1995).
The EEP stands out as an ideal natural laboratory for studying the dynamics of the tropical thermocline: the shallow depth of the thermocline in the present-day EEP upwelling system (∼50 m; Wang et al., 2000) (Fig. 1c) means that even small changes in its depth can affect surface-water properties, such as temperature or nutrient content, which can be ideally reconstructed from sediments underneath the “cold tongue”. Thereby, the high sedimentation rates allow for the acquisition of proxy records at a high temporal resolution compared to areas outside the EEP upwelling zone.
2.2 ODP Site 849
To reconstruct changes in the thermocline depth in the EEP we focused on sediments from ODP Leg 138 Site 849 (coordinates: 0∘11′ N, 110∘31′ W; present-day water depth: 3851 m; Mayer et al., 1992) (Fig. 1a, b). This site was selected because of (i) its position within the equatorial “cold tongue”, west of the East Pacific Rise in the open ocean, which makes it less prone to continental influence compared to sites east of the East Pacific Rise (Mix et al., 1995); (ii) the good preservation of foraminifera (Jakob et al., 2016, 2017) despite the fact that the present-day water depth at Site 849 is close to the lysocline (Adelseck and Anderson, 1978; Berger et al., 1982); and (iii) the high sedimentation rates (2.7 cm kyr−1 for our study interval; Jakob et al., 2017) with continuous sedimentation (Mayer et al., 1992).
The geochemical and faunal records generated in this study (for details see Sect. 4) are based on the planktic foraminiferal species Globigerinoides ruber (white, sensu stricto), Globorotalia crassaformis, Globorotalia menardii and Globorotalia tumida; the presumed calcification depths of these species in the EEP, as briefly elaborated upon in the following, are compiled in Fig. 1c. Globigerinoides ruber generally inhabits and calcifies in the mixed layer and is typically considered to represent surface-water conditions (Fairbanks et al., 1982; Wang, 2000; Dekens et al., 2002; Steph et al., 2009, and references therein). Globorotalia menardii and Globorotalia tumida are found in the EEP at depths of ∼25–70 and ∼50–125 m, respectively, typically in intermediate-thermocline waters (Fairbanks et al., 1982; Watkins et al., 1998; Faul et al., 2000). Globorotalia crassaformis inhabits the bottom of the thermocline (Niebler et al., 1999; Regenberg et al., 2009; Steph et al., 2009, and references therein), and has a rather constant calcification depth as opposed to other deep-dwelling foraminiferal species (Cléroux and Lynch-Stieglitz, 2010). Whilst its exact calcification depth in the EEP remains unclear, δ18O values of G. crassaformis from the (sub-)tropical Atlantic and the Caribbean Sea suggest that this species typically calcifies at water depths between ∼400 and 800 m (Steph et al., 2006b, 2009; Regenberg et al., 2009; Cléroux et al., 2013).
To reconstruct the thermocline depth for the final phase of the late Pliocene/early Pleistocene iNHG from ∼2.75 to 2.4 Ma (MIS G7–95), we integrate new and previously published proxy records from ODP Site 849 (Fig. 1; Table 1). In particular, we combine planktic (both sea surface- and thermocline-dwelling) foraminiferal geochemical (δ18O, δ13C and Mg ∕ Ca) proxy records with sedimentological (sand accumulation rates) and faunal (abundance data of thermocline-dwelling foraminiferal species) information.
4.1 Sample material
To obtain geochemical, faunal and sedimentological information for Site 849, 374 samples were investigated along the primary shipboard splice (Mayer et al., 1992) from cores 849C-7H-1-80 cm to 849C-7H-2-21 cm and 849D-6H-5-102 cm to 849D-7H-5-57 cm (77.02–67.78 m composite depth, m c.d.). Based on the age model of Jakob et al. (2017), this interval spans from ∼2.75 to 2.4 Ma (MIS G7–95). Samples with a volume of 20 cm3 were investigated at 2 cm intervals, which yielded a temporal resolution of ∼750 years. The sample material was dried, weighed and washed over a 63 µm sieve.
Foraminiferal geochemical records (δ18O, δ13C and Mg ∕ Ca) of the deep-thermocline-dwelling species G. crassaformis and the surface-dwelling species G. ruber, as well as sand accumulation rates were generated from the full sample set (with a temporal resolution of ∼750 years). From these measurements surface to thermocline δ18O, δ13C and Mg ∕ Ca gradients were calculated. Abundance counts of both deep-thermocline- (G. crassaformis) and intermediate-thermocline-dwelling species (G. menardii and G. tumida) were conducted every 20 cm (with a temporal resolution of ∼ 7.5 kyr).
For G. crassaformis, we generated new δ18O, δ13C and Mg ∕ Ca records, except for the interval from ∼2.65 to 2.4 Ma for which δ13C values had already been published by Jakob et al. (2016). For this purpose, an average of 15 individuals per sample was picked from the 315 to 400 µm fraction. This size fraction was selected to keep ontogenetic effects as small as possible (Elderfield et al., 2002; Friedrich et al., 2012) but at the same time to allow for a sufficient number of G. crassaformis tests per sample. Moreover, the 315–400 µm fraction ensured the highest comparability to previous geochemical records of this species (e.g., Karas et al., 2009; Jakob et al., 2016). Tests for δ18O and Mg ∕ Ca analyses were cracked, homogenized and split into two subsamples. For G. crassaformis, both sinistral- and dextral-coiling specimens occur at Site 849; geochemical data were preferentially measured on tests with the most abundant coiling direction (sinistral). However, sinistral-coiling specimens do not occur continuously across our study interval. Thus, dextral-coiling tests were used for some intervals (in particular from ∼2.46 to 2.43 Ma (69.84–69.04 m c.d.) and from ∼2.51 to 2.50 Ma (70.85–70.68 m c.d.)). The occurrence of dextral- versus sinistral-coiling G. crassaformis specimens is random rather than following a specific cyclicity. Separate measurements of geochemical parameters (δ13C, δ18O, Mg ∕ Ca) on sinistral- and dextral-coiling specimens from the same samples have demonstrated that the reconstructed values are independent of the coiling directions (see also Jakob et al., 2016).
The number of G. crassaformis individuals in the investigated size fraction (315–400 µm) was too low to allow for geochemical analyses in specific intervals. These intervals were from 2.68 to 2.65 Ma (75.39–74.65 m c.d. corresponding to MIS G3) and from 2.73 to 2.69 Ma (77.02–75.79 m c.d. corresponding to MIS G7–G5). We decided not to fill these gaps using another size fraction because (i) this might have biased our Mg ∕ Ca and stable isotope records due to ontogenetic effects (Elderfield et al., 2002; Friedrich et al., 2012), and (ii) the abundance of G. crassaformis specimens <315 µm was also too low for geochemical analyses in most of the samples where the 315–400 µm G. crassaformis size fraction was absent (see Sect. 5.4.2 for details).
For G. ruber, the previously published Mg ∕ Ca-based sea-surface temperature (SST) and δ18O datasets of Jakob et al. (2017) were augmented by δ13C data, except for the interval from ∼2.65 to 2.4 Ma for which δ13C values have already been published by Jakob et al. (2016). For this purpose, an average of 12 specimens was picked from the 250–315 µm size fraction (i.e., the fraction also used in Jakob et al., 2016). An overview of all geochemical datasets evaluated in this study is presented in Table 1.
4.2 Analytical methods
4.2.1 Foraminiferal preservation
The preservation of planktic foraminiferal (G. crassaformis and G. ruber) tests used for geochemical analyses was examined using scanning electron microscope (SEM) images of selected specimens from both glacial and interglacial intervals. Close-up views were taken using a LEO 440 SEM at the Institute of Earth Sciences, Heidelberg University.
4.2.2 Stable isotope analyses
Oxygen and carbon isotopes of G. ruber and G. crassaformis were analyzed using a Thermo Finnigan MAT253 gas source mass spectrometer equipped with a Gas Bench II at the Institute of Geosciences, Goethe University Frankfurt. Values are reported relative to the Vienna Pee Dee Belemnite (VPDB) standard through the analysis of an in-house standard calibrated to NBS-19. The precision of the δ18O and δ13C analyses is better than 0.08 and 0.06 ‰ (at 1σ level), respectively. δ13C values of G. ruber reported herein were adjusted for the species-specific offset from equilibrium precipitation via the addition of +0.94 ‰ (Spero et al., 2003), while measured δ18O values of G. ruber were considered to approximate equilibrium precipitation (Koutavas and Lynch-Stieglitz, 2003) and were not adjusted. For G. crassaformis we simply report the measured values, as laboratory investigations on δ13C and δ18O fractionation for this species are still lacking.
4.2.3 Mg ∕ Ca analyses
Samples of G. crassaformis for Mg ∕ Ca analyses were carefully cleaned to remove clay minerals, organic material and re-adsorbed contaminants following the protocol of Barker et al. (2003) but omitting reductive cleaning. However, for selected samples reductive cleaning was also applied (see Sect. 5.2); a mixture of hydrazine, ammonium hydroxide and ammonium citrate was used as a reductive reagent. Analyses were carried out with an Agilent 720 inductively coupled plasma-optical emission spectrometer at the Institute of Earth Sciences, Heidelberg University. Reported Mg ∕ Ca values were normalized relative to the ECRM 752-1 standard reference value of 3.762 mmol mol−1 (Greaves et al., 2008). To ensure instrumental precision, an internal consistency standard was monitored at least every 20 samples. Based on replicate measurements, a standard deviation for Mg ∕ Ca of ±0.02 mmol mol−1 (corresponding to ±0.12 ∘C) was obtained. To identify possible contamination by clay particles or diagenetic coatings that might affect foraminiferal Mg ∕ Ca ratios (Barker et al., 2003), elemental ratios of Al ∕ Ca, Fe ∕ Ca and Mn ∕ Ca were screened (see Sect. 5.2).
4.2.4 Paleotemperature reconstruction
Species-specific conversions of Mg ∕ Ca to temperature for G. crassaformis were only calibrated based on samples from the Atlantic Ocean (Anand et al., 2003; Regenberg et al., 2009; Cléroux et al., 2013). These equations yield the same trend and amplitudes when applied to G. crassaformis Mg ∕ Ca values from Site 849, but differ with regard to absolute values (Fig. 2). We converted Mg ∕ Ca ratios of G. crassaformis into temperature following the species-specific equation of Cléroux et al. (2013) for the following two reasons: (i) the selected calibration is based on specimens with a grain size of 355–425 µm, which matches the size fraction used in our study (315–400 µm) better than the other available equations; and (ii) the Mg ∕ Ca range of G. crassaformis from Site 849 (∼1–3 mmol mol−1) fits best to the calibration range (∼1–2 mmol mol−1) of the equation from Cléroux et al. (2013) compared to the other equations.
As the equation of Cléroux et al. (2013) is based on oxidative and reductive cleaning of foraminiferal tests, and only oxidative cleaning has been applied to Site 849 samples, the measured Mg ∕ Ca values had to be reduced by 10 % (Barker et al., 2003). The pooled uncertainty in the temperature record is ±0.94 ∘C (analytical error of ±0.02 mmol mol−1, corresponding to ±0.12 ∘C, and a calibration error of ±0.82 ∘C; Cléroux et al., 2013).
4.2.5 Abundance counts
Following the approach of Sexton and Norris (2008), abundance counts of deep-thermocline-dwelling (G. crassaformis, both sinistral- and dextral-coiling specimens) and intermediate-thermocline-dwelling (G. tumida and G. menardii) species (Fig. 1c) were generated for the >250 µm size fraction of Site 849 samples. The >250 µm size fraction was split down to at least 400 individual planktic foraminifera using a microsplitter. Abundance counts were converted to mass accumulation rates using linear sedimentation rates and dry bulk density data (calculated from high-resolution GRAPE density shipboard measurements, IODP JANUS database; Mayer et al., 1992) following the methodology described in Jakob et al. (2016).
4.2.6 Sand accumulation rates
The sand accumulation rates available for the MIS G1–95 (∼2.65–2.4 Ma) interval from Site 849, as presented in Jakob et al. (2016), were extended back to MIS G7 (∼2.75 Ma) in this study. They were calculated using linear sedimentation rates, dry bulk density data (calculated from high-resolution GRAPE density shipboard measurements, IODP JANUS database; Mayer et al., 1992) and the portion of the >63 µm sand fraction following the approach described in Jakob et al. (2016).
5.1 Foraminiferal test preservation at Site 849
Shipboard investigations on core catchers originally reported a poor preservation of planktic foraminiferal tests at Site 849 (Mayer et al., 1992). However, these observations do not apply to the samples from our study interval. Instead, SEM images of both glacial and interglacial G. crassaformis and G. ruber specimens consistently show well-preserved fine features such as delicate spines, pore channels and a layered wall structure, in addition to a lack of secondary calcite or crusts on test surfaces (Fig. 3). This indicates that test preservation is consistently sufficient for the acquisition of high-quality geochemical data for both species throughout the study interval. A low planktic foraminiferal fragmentation index (Jakob et al., 2017) and large numbers of well-preserved, although typically less resistant, specimens such as Globigerinoides (Dittert et al., 1999) (Fig. 3g–l) further confirms this interpretation, and indicates that dissolution has not considerably affected foraminiferal tests.
5.2 Assessment of contamination and diagenetic effects on Mg ∕ Ca ratios of G. crassaformis
Al ∕ Ca, Fe ∕ Ca and Mn ∕ Ca ratios >0.1 mmol mol−1 are typically considered to indicate the presence of detrital clay, Fe-rich coatings and Mn-rich overgrowth, respectively. Such contamination might have biased the measured Mg ∕ Ca ratios (Barker et al., 2003). In most of our samples the content of Al was below the detection limit, arguing against the presence of detrital clay. With the exception of a few samples, Fe ∕ Ca values also do not exceed the critical value of 0.1 mmol mol−1, which indicates no contamination by Fe-rich overgrowth (Fig. 4a). The lack of a statistically significant correlation between Mg ∕ Ca and Fe ∕ Ca ratios (r2=0.17, p<0.01) further supports this finding.
However, measured Mn ∕ Ca ratios were above the 0.1 mmol mol−1 threshold, which might indicate Mn-rich overgrowth on the analyzed tests (Fig. 4b). Reductive cleaning (in addition to the standard cleaning procedure applied to Site 849 samples; see Sect. 4.2.3) performed on selected samples shows ∼40–45 % lower Mn ∕ Ca values compared to values derived from oxidative cleaning alone. This indicates that at least two different Mn phases coexist on G. crassaformis test surfaces. A similar observation has been made for the thermocline-dwelling species Neogloboquadrina dutertrei from the nearby ODP Site 1240, located in the Panama Basin. In this study, Mn-rich phases not removed through oxidative cleaning are hypothesized to arise from “kutnahorite-like” carbonates or Mn oxyhydroxide (Pena et al., 2005) – Mn phases that may also exist on G. crassaformis test surfaces at Site 849. Indeed, our data show a weak correlation between the Mg ∕ Ca and Mn ∕ Ca ratios for G. crassaformis samples (r2=0.44, p<0.01), which might indicate a bias of the measured Mg ∕ Ca ratios due to a Mn-rich overgrowth. However, we note that SEM images argue against the existence of any kind of overgrowth (Fig. 3). Diagenetic overgrowth usually has a Mg ∕ Mn ratio of ∼0.1 mol mol−1 (Barker et al., 2003, and references therein). If an unrealistically high Mg ∕ Mn ratio of 1 in the diagenetic overgrowth is assumed, this might change temperature estimates by ∼0.5 ∘C on average; however, we note that this would not affect the overall shape of the Mg ∕ Ca-based temperature record (Fig. 4c, d). Therefore, we conclude with reasonable certainty that early diagenetic overprinting has no significant impact on the interpretation of our data, although we cannot rule out the possibility of diagenetic changes in G. crassaformis tests because of significantly enriched Mn ∕ Ca ratios.
5.3 Geochemical records of G. crassaformis and G. ruber at Site 849
In warm tropical waters, where seasonal climate variability is low, geochemical signatures of the investigated foraminiferal species are typically considered not to be seasonally biased (Lin et al., 1997; Tedesco et al., 2007; Mohtadi et al., 2009; Jonkers and Kučera, 2015). At Site 849, seasonal temperature variability is presently ∼0.4 ∘C (i.e., SST of ∼24 ∘C during summer (June) versus ∼23.6 ∘C during winter (January)). The same seasonal amplitude (∼0.4 ∘C) prevails at 20 m water depth (Locarnini et al., 2013), i.e., the assumed mean depth habitat of the investigated species G. ruber (Wang, 2000; see also Sect. 3). Further, we suggest that seasonality decreases as water depth increases; therefore it should be <0.4 ∘C at the calcification depth of G. crassaformis. Thus, because of the low seasonal temperature variability, it is reasonable to assume that all geochemical data derived from Site 849 (Figs. 5–8) reflect mean annual conditions.
5.3.1 Stable isotope data
The δ18O record of G. crassaformis varies between 0.91 and 2.79 ‰ throughout the study interval (∼2.75–2.4 Ma) (Fig. 5b). The lowest values correspond to interglacials and the highest values are associated with glacials. With a mean value of 2.01 ‰, δ18O values of G. crassaformis (this study) are 2.78 ‰ higher on average than those of G. ruber (Jakob et al., 2017), indicating cooler and/or more saline waters at the calcification depth of G. crassaformis (bottom of the thermocline) compared to that of G. ruber (surface waters) (Fig. 1c; see Sect. 3 for details). In theory, a deeper calcification depth of G. crassaformis than of G. ruber should result in a lower δ13C signature in G. crassaformis tests than in those from G. ruber, as the amount of organic matter remineralization and the associated release of light 12C into the surrounding water typically increases with water depth (Deuser and Hunt, 1969; Kroopnick, 1985). Indeed, ∼1.86 ‰ lower δ13C values were recorded for G. crassaformis (mean: 0.46 ‰) than for G. ruber (mean: 2.32 ‰; Jakob et al., 2016; this study) (Fig. 5c). In general, δ13C values of G. ruber and G. crassaformis fluctuate between minima of 1.36 and 0 ‰ during glacials and maxima of 2.97 and 0.97 ‰ during interglacials, respectively (Jakob et al., 2016; this study) (Fig. 5c). It has been shown in a former study that the glacial–interglacial foraminiferal δ13C pattern at Site 849 during the iNHG is strongly controlled by the amount of primary productivity in the Southern Ocean, which is highest during interglacials (high δ13C) and lowest during glacials (low δ13C) (Jakob et al., 2016).
5.3.2 Mg ∕ Ca-based temperature data
Mg ∕ Ca values of G. crassaformis vary between 0.82 and 3.02 mmol mol−1 (this study), and are 1.43 mmol mol−1 lower on average than Mg ∕ Ca ratios of G. ruber from the same site and time interval (Jakob et al., 2017) (Fig. 5d). Temperatures reconstructed from G. crassaformis Mg ∕ Ca values cover a range from 1.0 to 11.6 ∘C. Thus, sub-thermocline temperatures at Site 849 derived from G. crassaformis are 19 ∘C lower on average than SSTs as reflected by G. ruber (∼22–27 ∘C; Jakob et al., 2017) (Fig. 5d). To bring the G. crassaformis-based temperatures of this study into a broader temporal and geographical context, we compare this record to a number of other relevant datasets:
The temperature range reconstructed based on G. crassaformis at Site 849 is close to temperatures inferred for the same species and time interval at Deep Sea Drilling Project (DSDP) Site 214 in the tropical eastern Indian Ocean (∼8–10 ∘C; Karas et al., 2009) (Figs. 1a, 6). Available Mg ∕ Ca-based thermocline temperature records from the eastern Pacific for the ∼2.75–2.4 Ma interval capture ranges of ∼17–22.5 ∘C (ODP Site 1241, G. tumida-based; Steph et al., 2006a), ∼18–21 ∘C (Site 1241, N. dutertrei-based; Groeneveld et al., 2014) and ∼15.5–17.5 ∘C (Site 849, G. tumida-based; Ford et al., 2012) (Figs. 1a, b and 6). In comparison to thermocline temperature records from Site 1241 (Steph et al., 2006a; Groeneveld et al., 2014) our new G. crassaformis-based temperatures appear to be relatively low. However, this discrepancy can likely be explained by different calcification depths of the investigated species (which means that different temperatures are reflected; Cléroux et al., 2013) and differences in the oceanographic setting of the investigated sites (i.e., Site 849 in the “cold tongue” versus Site 1241 in the “warm pool” with, for example, a modern-day SST difference of ∼3 ∘C; Locarnini et al., 2013; see also Sect. 5.4.1). The record from Site 849 by Ford et al. (2012) is of low temporal resolution (with only six datapoints across our study interval) such that peak (both glacial and interglacial) temperatures are probably not captured. Therefore, a comparison to this record is not robust enough to warrant further discussion.
The EEP upwelling system is mainly fed by waters derived from the Southern Ocean (e.g., Tsuchiya et al., 1989). However, relatively warm SSTs in the Southern Ocean during our study interval (∼10.5–17 ∘C at ODP Site 1090, Martínez-Garcia et al., 2010; Fig. 1a, – a site accepted as the best end-member of Southern Ocean waters, Billups et al., 2002; Pusz et al., 2011) are difficult to reconcile with substantially lower temperatures recorded in thermocline waters at EEP Site 849 (∼1–11.6 ∘C; this study) and Indian Ocean Site 214 (∼8–10 ∘C; Karas et al., 2009). Together, these datasets imply strong cooling of Southern Ocean surface waters either when being downwelled and transported to the lower latitudes and/or through mixing with cold (presently ∼0 ∘C; Craig and Gordon, 1965) Antarctic Bottom Waters.
Thermocline temperatures of the Last Glacial Maximum are expected to be substantially colder than those of the Plio-Pleistocene transition (Ford et al., 2012). However, in comparison to tropical east Pacific thermocline temperatures of the Last Glacial Maximum (on average ∼14–16 ∘C), which are derived from Mg ∕ Ca data of G. tumida from Site 849 (Ford et al., 2015) and N. dutertrei from Sites 08JC and 17JC (Hertzberg et al., 2016) (Fig. 1a), deep-thermocline temperatures of G. crassaformis at Site 849 from the ∼2.75 to 2.4 Ma interval appear to be too low. We suggest that different calcification depths of the investigated species may explain this discrepancy (Cléroux et al., 2013).
Finally, we notice that modern bottom-water temperatures at our study site of ∼1.5 ∘C (Locarnini et al., 2013) overlap the deep-thermocline temperature range as reconstructed from G. crassaformis-based Mg ∕ Ca data. However, very low G. crassaformis-based temperatures of ∼1 ∘C are derived from a single data point, while temperatures typically higher than 2–3 ∘C, even during prominent iNHG glacials, can be better reconciled with present-day bottom-water temperatures.
5.4 Thermocline development in the easternequatorial Pacific
5.4.1 Geochemical evidence
Variations in the vertical temperature gradient within the upper water column allow for the effective monitoring of shifts in the thermocline depth, with a small temperature difference between surface and thermocline waters indicating a deep thermocline and vice versa (e.g., Steph et al., 2009; Nürnberg et al., 2015). Absolute values of surface to thermocline temperature gradients can be reconstructed from the Mg ∕ Ca-based temperature gradient derived from surface-dwelling and thermocline-dwelling foraminiferal species. In addition, the δ18O gradient provides information on relative changes in the surface to thermocline temperature gradient (as opposed to absolute estimates derived from the Mg ∕ Ca gradient). This is because salinity might also play a role in controlling the δ18O values of foraminifera inhabiting different depths. The effect of global ice volume (i.e., the third factor beside temperature and salinity that affect foraminiferal δ18O; Ravelo and Hillaire-Marcel, 2007) should be identical. For gradient calculations, G. ruber is ideally suited as a surface-water recorder since it is one of the shallowest-dwelling species among modern planktic foraminifera (Bé, 1977); G. crassaformis appears to be one of the most promising recorders of the deep thermocline due to its rather constant calcification depth compared to other deep dwellers (Cléroux and Lynch-Stieglitz, 2010). This approach (i.e., G. ruber to G. crassaformis gradient calculation) has already successfully been applied by previous studies that have investigated changes in the surface-water structure and the thermocline through time (e.g., Karas et al., 2009; Bahr et al., 2011).
The δ18O- and Mg ∕ Ca-based temperature gradients between G. ruber and G. crassaformis at Site 849 show no glacial–interglacial cyclicity (Fig. 7b), indicating that the thermocline depth was unaffected by varying glacial versus interglacial climatic conditions. This observation is in line with previous modeling efforts (Lee and Poulsen, 2005) and proxy-based (both geochemical and faunal) studies from EEP “cold tongue” ODP Sites 846 and 849 that cover the same time interval (Bolton et al., 2010; Jakob et al., 2017). However, it contradicts geochemical data (i.e., the surface to thermocline (Globigerinoides sacculifer to N. dutertrei) Mg ∕ Ca-based temperature gradient) derived from Site 1241 located in the east Pacific “warm pool”, which shows glacial–interglacial variations in thermocline depth for MIS 100–96 (Groeneveld et al., 2014) (Fig. 8). Therefore, we hypothesize that thermocline depth underwent a different evolution on the glacial–interglacial timescale in regions inside (Sites 846 and 849) and outside (Site 1241) the “cold tongue”. Further, water column stratification and thermocline depth at Site 1241 has been shown to be affected by glacioeustatic closures of the Central American Seaway that temporally occurred during MIS 100–96 (Groeneveld et al., 2014), perhaps due to upwelling intensification (Schneider and Schmittner, 2006). In contrast, Site 849 appears to be unaffected by such changes, as shown by sand accumulation rate based data on export production (Jakob et al., 2016). Hence, it is likely that Site 1241 reflects a more local signal as opposed to the open ocean, quasi-global signal reported at Site 849 due to its position west of the East Pacific Rise (Mix et al., 1995).
On longer timescales, the δ18O gradient at Site 849 decreased by ∼1 ‰ from ∼2.64 to 2.55 Ma (MIS G2–101), and remained relatively constant throughout the remainder of our study interval (∼2.55–2.38 Ma; MIS 101–95) (Fig. 7b). The Mg ∕ Ca-based temperature gradient shows the same overall pattern as the δ18O gradient (i.e., a ∼5 ∘C increase from ∼2.64 to 2.55 Ma, and a constant value of ∼20 ∘C from ∼2.55 to 2.38 Ma) (Fig. 7b). We interpret the decrease in the δ18O gradient and the increase in the Mg ∕ Ca-based temperature gradient from ∼2.64 to 2.55 Ma as representing a shoaling of the thermocline. From that time onwards, constant δ18O and Mg ∕ Ca-based temperature gradients suggest that the thermocline remained relatively shallow throughout the final phase of the late Pliocene/early Pleistocene iNHG until ∼2.38 Ma. In general, the shoaling trend of the thermocline revealed by our records agrees with the overall long-term shoaling trend of the thermocline in the EEP observed throughout the Plio-Pleistocene (Fedorov et al., 2006; Steph et al., 2006a, 2010; Dekens et al., 2007; Ford et al., 2012), although substantial thermocline shoaling is restricted to the ∼2.64–2.55 Ma period rather than occurring continuously throughout the entire investigated time interval (Fig. 8). However, our data do not confirm previous datasets indicating that most prominent thermocline shoaling occurred prior to ∼3.5 Ma (Wara et al., 2005; Steph et al., 2006a, 2010; Ford et al., 2012). Geochemical data from Site 1241 even reveal a transient thermocline deepening for the ∼2.7–2.5 Ma interval (Steph et al., 2006a) (Fig. 8), which also cannot be confirmed by our records from Site 849 and supports the fact that Site 1241 might reflect a more local signal (see above). Other records used to infer thermocline evolution in the east Pacific for this interval lack the required temporal resolution (∼10–30 kyr, Wara et al., 2005; Dekens et al., 2007; and Ford et al., 2012, versus ∼0.75–3 kyr, Steph et al., 2006a and this study) to resolve transient thermocline changes as observed at Site 1241, if they exist.
5.4.2 Faunal and sedimentological evidence
Based on our data, the overall abundances of the deep-thermocline-dwelling species G. crassaformis at Site 849 were relatively low when the thermocline was relatively deep (i.e., prior to ∼2.55 Ma as indicated by the δ18O and Mg ∕ Ca-based temperature gradients) (Fig. 7c). More specifically, G. crassaformis was only present in substantially reduced numbers or was even completely absent between ∼2.73 and 2.64 Ma (MIS G7–G2; with the exception of MIS G4, ∼2.69–2.68 Ma). Since ∼2.64 Ma, i.e., when the thermocline started to shoal, relative G. crassaformis abundances increased markedly from <5 to ∼10–35 %; consequently, representatives of this taxon are continuously present throughout the remainder of the study interval. The increase of G. crassaformis abundances occurs at the expense of the intermediate-thermocline-dwelling species G. menardii and G. tumida, which decline from ∼30 to 75 % to only ∼5 to 65 % (Fig. 7c). This observation suggests that prior to the final phase of the late Pliocene/early Pleistocene iNHG, when the thermocline was relatively deep, the living conditions for the deep-thermocline-dwelling species G. crassaformis were unfavorable. At the same time, low G. crassaformis abundances allowed intermediate-thermocline-dwelling species (such as G. menardii and G. tumida) to dominate the planktic foraminiferal assemblages. However, we note that the thermocline depth is most probably not the sole factor regulating G. crassaformis abundances. This is because this species only reaches low percentages within modern planktic foraminiferal assemblages in the EEP (typically <1 % in core-top samples; Prell, 1985), although the present-day thermocline is relatively shallow.
In general, G. crassaformis reaches highest abundances in oxygen-depleted waters (Jones, 1967; Kemle von Mücke and Hemleben, 1999), while other environmental factors including temperature, salinity or nutrient availability are markedly less important (Cléroux et al., 2013). The oxygen content of deep waters (and accordingly the abundance of G. crassaformis) is typically closely coupled to surface-water productivity (with a lower oxygen level and higher G. crassaformis abundances in deeper waters when surface-water productivity is high) (Wilson et al., 2017). Therefore, we hypothesize that primary productivity at Site 849 prior to ∼2.64 Ma (MIS G2) was relatively low (with the exception of MIS G4). Low primary productivity led to a reduction of organic matter remineralization and related oxygen consumption in deeper waters. An elevated oxygen content in deeper waters implies, in turn, low G. crassaformis abundances. Such a scenario is supported by the sand accumulation rate based primary productivity record from Site 849 (Jakob et al., 2016; this study), which clearly indicates low productivity rates prior to ∼2.64 Ma when the thermocline was relatively deep compared to after ∼2.64 Ma when the thermocline became shallow (Fig. 7b, d).
As outlined above, on longer timescales primary productivity at Site 849 appears to be coupled to variations in the thermocline depth. The observed long-term trend in primary productivity is overprinted by a clear glacial–interglacial cyclicity, particularly during the final phase of iNHG (MIS 100–96); however, the position of the thermocline remained constant along the obliquity (i.e., 41 kyr) band (Fig. 7b, d). Notably, the accumulation rates of G. crassaformis, G. menardii and G. tumida perfectly capture the pattern derived by the sand accumulation rate based productivity record (Fig. 7c, d). This suggests that the abundances of deep- and intermediate-thermocline-dwelling foraminiferal species are coupled to the strength of the biological pump and can be used as a tracer for primary productivity at Site 849.
The relatively high δ13C gradient for MIS G4–G2, as it emerges from our data (Fig. 7d), confirms the interpretation of Jakob et al. (2016) for MIS G1–95, which was that low-amplitude productivity changes prior to MIS 100 were mainly driven by the nutrient content within the upwelled water mass as long as the thermocline was relatively deep (as reflected by a low thermocline to surface temperature gradient prior to ∼2.55 Ma, MIS 101; Fig. 7b, d). High-amplitude productivity changes resulting from upwelling intensification played an important role from MIS 100 onward (Jakob et al., 2016). At the same time, the thermocline became relatively shallow (as reflected by the large thermocline to surface temperature gradient since ∼2.55 Ma (MIS 101) at Site 849; Fig. 7b, d). This is unlikely to be a coincidence, but rather suggests that the thermocline depth reached a critical threshold at that time. Prior to this, relatively warm and nutrient-poor waters from above the thermocline upwelled at EEP Site 849. Consequently, primary productivity rates were low. However, when the thermocline became shallow enough, trade winds could deliver cooler, nutrient-enriched waters from below the thermocline to the surface, which allowed primary productivity to increase. This scenario is supported by the observation that lower SSTs have prevailed at Site 849 during glacials since MIS 100 (Jakob et al., 2017) (Fig. 5d). Moreover, temporal closures of the Central American Seaway might have additionally promoted generally increasing upwelling and therefore primary productivity rates since MIS 100 (Schneider and Schmittner, 2006; Groeneveld et al., 2014).
Our findings imply a marked effect of long-term thermocline state change on primary productivity at the studied site. In particular, when thermocline shoaling reached a critical threshold, primary productivity increased, thereby removing CO2 from the surface ocean. Thermocline shoaling appears to be a consistent feature in the EEP throughout the Plio-Pleistocene (although the timing and magnitude varies between different studies which may be related to the different approaches used for thermocline reconstruction or different localities and local oceanography). Considering that the entire EEP substantially contributes to global biological production in the present-day oceans (Pennington et al., 2006), the observed coupling between thermocline state change and primary productivity (if this behavior is similar across the entire EEP “cold tongue”) is of major importance for the Earth's climate; it may have favored global cooling and the subsequent early development of large ice sheets in the Northern Hemisphere. At the same time, as suggested in previous studies, the formation of the “cold tongue” through thermocline shoaling might have additionally preconditioned the iNHG by reducing atmospheric heat transport from the tropics to the poles (Cane and Molnar, 2001).
We integrate new and previously published foraminiferal-based geochemical, faunal and sedimentological records from ODP Site 849 (∼2.75–2.4 Ma, MIS G7–95) to reconstruct changes in the thermocline depth during the late Pliocene/early Pleistocene iNHG. Our data document a shoaling of the thermocline at Site 849 from ∼2.64 to 2.55 Ma, while it remained relatively shallow until ∼2.38 Ma. This implies that major changes in thermocline depth occurred shortly before the final phase of the late Pliocene/early Pleistocene iNHG (i.e., prior to MIS 100–96). This finding, which is in line with former studies (Fedorov et al., 2006; Dekens et al., 2007), supports the hypothesis that (sub-)tropical thermocline shoaling was a precondition to allow the development of large ice sheets in the Northern Hemisphere (Cane and Molnar, 2001). At the same time, our new data contradict studies that have documented substantial shifts in thermocline depth in the EEP only prior to ∼3.5 Ma (Wara et al., 2005; Steph et al., 2006a, 2010; Ford et al., 2012). Our new records also suggest low primary productivity rates during periods when the thermocline is relatively deep prior to ∼2.64 Ma (MIS G2). In turn, the relatively shallow thermocline associated with low SSTs after ∼2.55 Ma allowed primary productivity to increase during prominent iNHG glacials (MIS 100–96) and, perhaps, by removing CO2 from ocean–atmosphere exchange processes, to further stimulate Northern Hemisphere ice-sheet growth.
The data associated with this paper are provided in the Supplement (Tables S1 to S4).
The supplement related to this article is available online at: https://doi.org/10.5194/cp-14-1079-2018-supplement.
The project was designed by OF, KAJ and JP. KAJ and CS carried out the Mg ∕ Ca analyses; JF and KAJ performed the stable isotope analyses. KAJ wrote the manuscript with input from all co-authors.
The authors declare that they have no conflict of interest.
Richard Norris provided invaluable support regarding foraminiferal taxonomy.
Sven Hofmann and Silvia Rheinberger are thanked for the stable isotope and
Mg ∕ Ca analyses, respectively. André Bahr provided support with the
Mg ∕ Ca sample preparation. Hans-Peter Meyer and Alexander Varychev
provided SEM assistance. Jani L. Biber, Verena Braun, Jakob Gänzler,
Barbara Hennrich, Karsten Kähler and Tobias Syla helped with the processing
of sediment samples. Comments and suggestions by the editor Luc Beaufort and two
anonymous reviewers are highly appreciated. This research used samples
provided by the Ocean Drilling Program, which was sponsored by the US
National Science Foundation and participating countries under the management
of Joint Oceanographic Institutions, Inc. Funding for this study was provided
by the German Research Foundation (DFG; grant FR2544/6 to Oliver Friedrich
and grant PR651/15 to Jörg Pross). Further, we acknowledge financial support
from the DFG within the funding program Open Access Publishing, from the
Baden-Württemberg Ministry of Science, Research and the Arts and from
Edited by: Luc Beaufort
Reviewed by: two anonymous referees
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