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Deep Equatorial Pacific Ocean Oxygenation and Atmospheric CO2 Over The Last Ice Age


Ventilation of carbon stored in the deep ocean is thought to play an important role in atmospheric CO2 increases associated with Pleistocene deglaciations. The presence of this respired carbon has been recorded by an array of paleoceanographic proxies from various locations across the global ocean. Here we present a new sediment core from the Eastern Equatorial Pacific (EEP) Ocean spanning the last 180,000 years and reconstruct high-resolution 230Th-derived fluxes of 232Th and excess barium, along with redox-sensitive uranium concentrations to examine past variations in dust delivery, export productivity, and bottom-water oxygenation, respectively. Our bottom-water oxygenation record is compared to other similar high-resolution records from across the Pacific and in the Southern Ocean. We suggest that the deep Pacific is a site of respired carbon storage associated with periods of decreased global atmospheric CO2 concentration during the LGM, confirming the conclusions from a wealth of previous studies. However, our study is the first to show a similar relationship beyond the last glacial, extending to at least 70,000 years.


The dominant signal in global climate over the last 800,000 years is the 100-kyr co-variation of air temperature and atmospheric CO2 concentrations observed in the EPICA Antarctica ice core1. The temperature variations are likely modulated by the 100-kyr eccentricity signal and amplified by climate feedbacks which involve atmospheric CO2. The cause of atmospheric CO2 variability over late Pleistocene glacial-interglacial cycles is still debated, with a variety of explanations from changes in ocean stratification and ventilation, efficiency of the biological pump and nutrient availability, and carbonate compensation depth (see2 and references therein). One prevalent hypothesis is that there is an increased storage of respired carbon in the deep ocean during glacial maxima that is isolated from interaction with the atmosphere3,4,5,6,7. Significant ventilation of this respired carbon pool is thought to occur in the Southern Ocean and is coincident with upwelling there during the deglaciation, and on millennial timescales during the last glacial period2,4,7.

Like the Southern Ocean, the eastern equatorial Pacific Ocean (EEP) plays an important role in the global carbon cycle. Today, although the EEP is the major source of oceanic CO2 outgassed to the atmosphere8, approximately 5–10% of annual global export production occurs there9. Thus, although the EEP is a net CO2 source to the atmosphere today, it could easily have been a CO2 sink in the past, for example, if sequestering of CO2 by the biological pump were more efficient10,11.

Here we present high-resolution proxy data of bottom water oxygenation (authigenic U, see Methods), biological productivity (230Th-derived excess Ba (xsBa) flux, see Methods), and dust (230Th-derived 232Th flux, see Materials and Methods) flux from a high-sedimentation-rate core collected on the Cocos Ridge bordering the Panama Basin of the EEP (MV1014-8JC (8JC), 6°14.0′N, 86°02.6′W; 1993 m water depth). Our record spans the past 180 kyr beginning in the penultimate glacial period (Marine Oxygen Isotope stage, MIS 6). The sedimentation rate at site 8JC varies from 1.3 to 6.8 cm/kyr, giving a sub-millennial age resolution of ~300–900 yr during MIS 1–4 and a millennial age resolution of ~750–2000 yr during MIS 5 and 6 for our sampling resolution of 2 cm.

Through these records of 232Th flux, xsBa flux, and aU concentrations, we aim to better understand the relationship between changes in dust deposition, export production, and bottom water oxygenation in the glacial EEP. We compare our new record with that at the equator (MV1014-17JC11) and attempt to unravel the relative contributions of organic matter flux and bottom water oxygen concentrations to pore water redox conditions. We conclude that our EEP high resolution aU records generally reflect changes in bottom water oxygenation that waxes and wanes with the extent and reach of a deep-Pacific respired carbon pool that mirrors variations in atmospheric CO2 over the past 180 kyr. However, there are times during which differences between the authigenic uranium records in the EEP may be explained by changes in local export production and/or changes in the depth interval of the respired carbon pool.

Results and Discussion

EEP 232Th (dust) fluxes

A slowdown of the Atlantic Meridional Overturning Circulation (AMOC)12 during the Last Glacial Maximum (LGM) and Heinrich Stadial (HS) 1 is coincident with the shifting of wind belts, specifically the Intertropical Convergence Zone (ITCZ) and the westerlies of both hemispheres13. In the EEP, south of site 8JC studied here (core 17JC; Fig. 1, circle), Loveley et al.11 report evidence of increased pulses of dust (232Th fluxes; see Methods section) during the deglaciation and several HS events (climate events initiated in the North Atlantic). These pulses are interpreted to represent a link between changes in atmospheric circulation in the EEP and changes in AMOC. At site 8JC in the EEP (Fig. 1, star), there are significant increases in 230Th-derived 232Th fluxes at the Terminations of glacial stages (Fig. 2a; see Methods for age model, radiocarbon and δ18O stratigraphy). This timing is coincident with the timing of HS1 (~15 kyr, end MIS 2) and HS11 (~129–136 kyr, end MIS 6). Notably, two to three-fold increases in 230Th-derived 232Th fluxes from “baseline” interglacial values of ~1 µg cm−2 kyr−1 at HS1 and HS11 indicate a link between periods of deglaciation and increased northern hemisphere dust supplied to the EEP. Within and towards the end of MIS 4, there are two clear dust flux peaks (consistent with the timing of HS6 and HS7) with a similar 2- to 3-fold increase in 230Th-derived 232Th flux above the baseline values (Fig. 2b). The duration of these four dominant dust flux peaks (HS1, HS6, HS7, HS11) in 230Th-derived 232Th flux (~5 kyr) agree with other studies that show that the tropical Pacific records peak glacial conditions and a dustier atmosphere within short pulses during and at the end of glacial periods11,14,15.

Figure 1

Global ΔpCO2 flux and study core locations. Map created in Ocean Data View (Schlitzer, R., version 5.2.0, using ΔpCO2 flux data from Takahashi et al. (2009)8. Core locations for authigenic uranium records compared in this study are denoted on the map as follows: Subarctic North Pacific site ODP 882 (hexagon), Eastern Equatorial Pacific sites MV1014-8JC (Star) and MV1014-17JC (circle), Southern Ocean sites TN057-13/14PC (square), South Atlantic site TN057-21PC (triangle).

Figure 2

Core MV1014-8JC proxy records. (a) δ18O record from N. dutertrei as ‰VSMOW (dark blue line). (b) 230Th-normalized 232Th flux, a proxy for dust flux (green circles). Green solid line connecting data represents a three-point running mean. Dust flux peaks likely associated with HS1, 6, 7, and 11 are shown. (c) 230Th-normalized xsBa flux, a proxy for export production (purple circles). Purple solid line connecting data represents a three-point running mean. (d) Authigenic uranium, a proxy for bottom-water oxygenation (teal circles). Teal solid line connecting the data represents a three-point running mean. Ages for MIS stage boundaries and Terminations I and II from Lisiecki and Raymo, 200445 (See Methods). Seven radiocarbon ages and uncertainties plotted in red at base of figure (See Methods).

In the easternmost Equatorial Pacific, where dust fluxes are highest because of proximity to the continental margin, we compare the 8JC record with the high-resolution record from 17JC11. We are limited to comparing the two dust flux records from 0–70 kyr and 85–95 kyr (Fig. 3a) because the 17JC record spans only the past 95 kyr, and bioturbation of the Los Chocoyos ash obscures the record at 8JC between 70 and 85 kyr. For both cores, during the time intervals of comparison, values for the three highest dust peaks occur during or at the end of MIS 2 and 4, consistent with the timing of HS1, HS6, and HS7. The absolute values of the dust flux peaks in 17JC and 8JC are similar, and are about two to three times those of the baseline values (i.e., ~2–3.5 µg cm−2 kyr−1 versus ~1–1.3 µg cm−2 kyr−1 in both cores). Core 17JC clearly records 230Th-derived 232Th flux variability concurrent with the timing of several other HS events (i.e., HS 2, 4, 5, and 911). These pulses of increased dust flux in 17JC are not prominent in 8JC (HS events cannot be discerned easily in Fig. 3), likely due to the factor-of-two lower sedimentation rate at 8JC which serves to attenuate its record. Note, however, that in the 8JC record (Fig. 3a) there are, for example, several dust flux peaks in MIS3 (e.g., between HS5 and HS6) that may be associated with the pulses identified in 17JC.

Figure 3

A comparison of proxies for Eastern Equatorial Pacific cores MV1014-8JC (black symbols) and MV1014-17JC (red symbols; Loveley et al., 201711) over the past 100 kyr. (a) 232Th MARs and (b) xsBa MARs. Yellow bars represent timing of North Atlantic Heinrich Stadial (HS) events. Data affected by the Los Chocoyos ash are removed (note the greater effect of the ash in 8JC (black) because of bioturbation in this lower sedimentation rate core.

At ~6° N, site 8JC is at a position slightly south of the average annual modern-day ITCZ (~7° N16). Using the dust flux record from 17JC, it was hypothesized that increases in dust flux, coincident with the timing of several HS events, were likely associated with shifts in the ITCZ, such that the ITCZ was centered on or south of the equator during each HS event11. This reasoning was based on the similar ITCZ shifts hypothesized to explain records near or on the South American continent. The similar increases in 230Th-derived 232Th flux recorded at the more northerly 8JC site at the terminations (HS1 and HS11) and at the end of MIS 4 (HS6) argue that, if changes in the position of the ITCZ are causing the variability, then (1) southern-sourced dust must be dominating the dust delivered to both the 8JC and 17JC sites today and at other times of low dust supply, and (2) northern-sourced dust is being supplied to both sites during times of high dust delivery (consistent with HS events).

EEP xsBa fluxes

Barium enrichment in ocean sediments occurs at several locations that underlie productive surface waters in the modern ocean17. Because barite (BaSO4) constitutes most biogenically-produced barium in the ocean, fluxes of barite in marine environments have been widely used as a paleoproductivity proxy (see summary paper by18). Excess Ba (xsBa) concentrations, the portion of the total barium sedimentary signal that is produced authigenically (i.e., barite precipitation), can be estimated by subtracting the continentally-derived aluminosilicate Ba from the total sedimentary Ba (see Methods). This paleoproductivity proxy is sensitive to changing pore water redox conditions, such that sulfate-reducing conditions can lead to the remineralization of previously deposited barite and subsequent release of barium into sediment pore waters19.

At site 8JC in the EEP, the 230Th-derived xsBa flux has an average value of ~2 µg cm−2 kyr−1 and a low variability (~1.2–2.8 µg cm−2 kyr−1, Fig. 2c, data in Supporting Information). The 8JC record yields an average 230Th-derived xsBa flux approximately half that of site 17JC (average of ~ 4 µg cm−2 kyr−111,), which is located in the upwelling zone to the south in the high productivity area associated with the Pacific cold tongue region (Fig. 3b). The range of variability in xsBa fluxes at 17JC is also much higher (range of ~2–10 µg cm−2 kyr−111) than that at 8JC (Fig. 3b). The position of core 17JC beneath the high-productivity waters near the equator is probably the cause of the disparity between the xsBa fluxes at 8JC versus those at 17JC. In addition, the relationship between the xsBa fluxes and dust fluxes at 8JC are not like that at 17JC. At 17JC, there was a relationship between xsBa and dust during or near HS1, 2, 5, 6, and 7, arguing for increased export production because of increased iron fertilization by dust11,20. (Note the slight ~1-kyr offset in the xsBa peaks at H1, H2, and H5 in 17JC which has previously been explained as being due to diagenetic affects during the most severe hypoxic conditions20, i.e., authigenic uranium values greater than 5–10 ppm21). In 8JC, the prominent dust peaks at HS1, 6, and 11 are not associated with peaks in xsBa. The lack of a relationship between productivity and dust flux at 6°N, compared to that which is observed at the equator (17JC; Loveley et al.11), suggests that the increased productivity is a local effect at work only within the upwelling zone at the equator. Equatorial upwelling at 17JC (not existent at 8JC at 6°N) yields an abundant supply of nutrients to this high-nutrient, low-chlorophyll (HNLC) zone that is limited by the micronutrient, Fe. Only upon the relaxation of this Fe limitation by increased dust delivery can productivity be enhanced. Although the idea for a connection between millennial dust delivery and productivity in the eastern equatorial is controversial20,21,22, there is recent evidence suggesting that Fe-induced stimulation of nitrogen fixation can cause significant increases in export production23.

Authigenic uranium and deep ocean carbon storage in the EEP

Most important in our work here is the identification of a decoupling between the 232Th/xsBa and the authigenic uranium signals in cores 8JC and 17JC. There is no apparent or systematic relationship with HS events, for example, in either of the cores. This decoupling is clearly detected when comparing the range in values of each proxy at 8JC versus that at 17JC. Specifically, while there is a significant three- to four-fold increase in the range of the 230Th-derived xsBa fluxes at site 17JC compared to that in 8JC (Fig. 3b), there is not a similar disparity between the range of aU concentrations recorded in the two cores (Fig. 4a). Indeed, the range in aU concentrations, excluding the Holocene part of the record, is from 4–12 ppm in both 8JC and 17JC (Fig. 4a; data in Supporting Information). There are some significant temporal differences between the authigenic uranium values (Fig. 4), which we describe later, but the range in both cores is the same.

Figure 4

(a) Authigenic U records from the eastern equatorial Pacific Ocean (MV1014-8JC, black circles; MV1014-17JC, red circles). Blue bars represent times of coincident high aU and low CO2 concentrations in 17JC, 13/14PC, and 21PC. (b) Authigenic U composite record from cores TN057-13PC (10–20 kyr) and TN057-14PC (20–70 kyr) from the Southern Ocean (pink circles, Jaccard et al., 20162). (c) Authigenic U record from core TN057-21PC from the South Atlantic Ocean (green circles, authigenic U data from Sachs and Anderson, 200338; age model from Gottschalk et al., 20167). (d) Atmospheric CO2 record from Antarctic ice cores (blue circles; Bereiter et al., 20121). Southern Hemisphere Antarctic Isotope Maxima (AIM) 1–4 are shown.

Authigenic U concentrations can be a function of either the flux of reducible organic matter to the sediment24,25,26 and/or the oxygen concentrations of the overlying bottom water27,28,29. Given that the flux of reducible organic matter (i.e., the xsBa flux proxy) is significantly different at both sites, while the range in authigenic U concentrations is similar at both sites, leads us to conclude that the high aU concentrations at both sites are controlled by the low oxygen concentrations of overlying bottom waters. If the sedimentary flux of organic matter (which is higher in the zone of upwelling at 17JC) were controlling the aU concentrations in 8JC, one would expect the aU concentrations in 8JC to be significantly lower than those in 17JC. At the two sites, separated by 650 km, the general inconsistency of the productivity signals (xsBa flux, Fig. 3) versus the similar range in the authigenic U signal (Fig. 4) suggests that bottom water oxygenation, and the potential for a widespread deep respired carbon pool, is a regional feature that dominates the authigenic U record. There is no question, however, that superimposed on this “baseline,” there are various intervals (during the deglaciation and mid-MIS3) during which local changes in export production influence the authigenic U signal, which may be responding to the flux of raining reducible organic matter (i.e., export production fluxes and authigenic U concentrations vary in concert). We discuss this further below.

Substantial evidence for an increased size of the respired carbon pool in the EEP at the LGM exists in the form of observations of the deepening of oxygen-depleted waters30,31,32,33,34. Our two high-resolution aU records, one from ~6° N at 1993 m water depth (8JC, this study), and the other on the equator at 2846 m water depth (17JC[11), expands our understanding of the deepening of oxygen-depleted waters in the EEP beyond timescales of previous studies to the past 70 kyr.

Authigenic uranium concentrations at 8JC are highest during MIS 2 and 6 (Figs. 2d and 4a). Similarly, aU concentrations at 17JC are highest during MIS 2 (Fig. 4a11, no data for MIS 6). We hypothesize that at these times when aU concentrations are the highest in both cores (Fig. 4a), bottom-water oxygen concentrations are the lowest and may represent an increased extent of a respired carbon pool in the deep equatorial Pacific Ocean. However, there are specific instances within glacial times during when the records diverge. The disparities between these EEP aU records occur for ~5–10 kyr during MIS 4 and early MIS 2 (Fig. 4a). There are slight offsets during MIS3 from 38–54 kyr that are likely within the errors of both age models. Differences in the aU concentrations and trends at the two sites appear to be greatest at times when the Antarctic ice core record shows pronounced and prolonged episodes of low CO2 (180–200 ppm during MIS 2 and MIS 4; Fig. 4). The differences during these times may be due to the difference in depth between the two sites. At 2846 m water depth, core 17JC in the Panama Basin is well within the expected lower 2-km depth range associated with glacial increases in deep Pacific respired carbon storage33,34,35,36,37. However, off-equatorial site 8JC (1993 m) is slightly above the 2-km depth estimate for deep waters which show an increased glacial respired carbon storage. In this context, it is possible that the decreases in aU values at site 8JC at the same time that 17JC shows enhancement result from changes in the depth of the respired carbon pool in the EEP. That is, the site depths are telling us that, during the times of lowest CO2 concentrations, the location of the respired carbon pool moves to greater depth, and the zone of deoxygenation expands proportionally greater in the downward direction.

Importantly, the most significant decreases in aU occur at the glacial terminations, i.e., at the ends of MIS 2 (8JC and 17JC, Fig. 4a) and 6 (8JC, Fig. 2d), and likely reflect an increase in bottom water oxygen concentrations, as would be expected with a reinvigoration of deep-water ventilation. We suggest that this increased ventilation may release to the atmosphere a portion of the deep respired carbon pool, thereby increasing atmospheric CO2 concentrations.

Global changes in glacial-interglacial respired carbon storage and atmospheric CO2

Increased deep ocean respired carbon storage during the LGM, inferred using authigenic uranium concentrations, which are sensitive to changes in bottom water oxygen concentrations, has been demonstrated in the Southern2, South Atlantic7,38, and Pacific Oceans11,30,35,36,39 (Fig. 4). Increases in aU concentrations in each of these records during the most prolonged periods of low glacial atmospheric CO2 levels have been hypothesized to represent decreases in bottom water oxygen concentrations and, by inference, increased storage of respired carbon in the deep ocean at these locations.

Records from cores 8JC and 17JC present a case for multiple, repeated periods of deep ocean respired carbon storage in the EEP (previous section). There is some similarity between our records and other high-resolution, high-sedimentation-rate records from the Southern Ocean2 (TTN57-13/14PC; water depth 3700 m; Fig. 1 purple square) and the South Atlantic (TTN57-21PC; water depth 4981 m; Fig. 1 blue triangle)7,38 in Fig. 4. Specifically, the EEP, Southern Ocean, and South Atlantic aU records each demonstrate a low-frequency variability (~10–20 kyr) in aU concentrations from late MIS 4 to peak glaciation (MIS 2) (Fig. 4b–d). Note that the aU concentrations in the 8JC and 17JC EEP cores are more than 5 times higher than the highest aU concentrations observed in either TTN57-13/14PC or TTN57-21PC (Fig. 4), and is likely due to the equatorial location of these sites that have increased organic rain that might be better preserved through the shallower water column. However, the pattern of variability in the aU records from cores 8JC, 17JC, TTN57-13/14PC, and TN57-21 is such that since MIS 4, there is a general consistency between the records and the Antarctic CO2 ice core record (Fig. 4).

The South Atlantic, Southern Ocean and 17JC records have among their highest aU concentrations (lowest bottom water O2) during MIS2 and MIS4 (horizontal blue bars shown in Fig. 4a), when atmospheric CO2 is less than 200 ppm. This is not the case for the 8JC record as described above. During MIS3 when atmospheric CO2 concentrations are relatively higher during the Antarctic Isotope Maxima (AIM) 1–4 (Fig. 4d), the Southern Ocean and South Atlantic cores, within error of the age models of each, have the lowest aU concentrations (highest bottom water O2 concentrations (Fig. 4). This is what lead both Jaccard et al. (2016)2 and Gottschalk et al. (2016)7 to suggest that growth and shrinking of the respired carbon pool (as manifest by the qualitative indicator of authigenic U concentrations and deep ocean oxygenation) is associated with decreased and increased global atmospheric CO2 concentrations, respectively. During MIS3 at both EEP cores there is the suggestion of higher bottom water oxygenation during relative highs in the CO2 record (AIM 1, 3, and 4). However, during mid-MIS3, between about 45–48 kyr (AIM2 with relatively high atmospheric CO2) in both cores 17JC and 8JC, there is a clear increase in aU which is the opposite of what is observed for both the Southern Ocean and South Atlantic cores. The aU peak in both EEP cores is associated with relatively increased xsBa fluxes (Fig. 3), suggesting the influence of increased export production which may, therefore, also be playing a role in influencing the aU signal. The timing of the aU peaks in MIS3 is coincident with a significant increase in opal fluxes across the easternmost equatorial Pacific40, and suggests increased diatom production during a period of enhanced upwelling and strengthened winds. There is also evidence for increased dust fluxes in the easternmost EEP during this time (Fig. 3). Similarly, there is a peak in opal fluxes (diatom production) across the EEP during the deglaciation40 when we also observe a mismatch between the 17JC aU record (HS1; along with both increased dust and export production fluxes, Fig. 3) and the increasing atmospheric CO2 concentrations (Fig. 4).

Therefore, in the EEP the aU archives are recording a changing bottom water oxygenation pattern that is suggestive of coherent increases and decreases in long-term storage of respired carbon from ~70 kyr up to the end of MIS 2. This pattern is similar, but not identical, to that observed in the Southern and South Atlantic Ocean cores, which is thought to be associated with changing atmospheric CO2 concentrations. We believe that both EEP records reflect a general pattern of changing bottom water oxygenation concentrations and base this argument on the similarity in the range of the extremely high authigenic U concentrations at two sites that are vastly different in terms of the flux of organic matter reaching the seafloor. There is a caveat, however: there are times (mid-MIS3 and HS1) during which the EEP authigenic U records are influenced by increased export production fluxes and do not, therefore, reflect changes in a global respired carbon pool associated with those in global atmospheric CO2 concentrations. Although our aU results, along with others11,30,35,36,39,41, emphasize the importance of the deep Pacific Ocean (along with the deep Southern Ocean and the deep South Atlantic Ocean) as being a potential location for storage of respired carbon during periods of decreased global atmospheric CO2 concentrations, it is clear, given our caveats, that further studies using bottom water oxygenation proxies in conjunction with those for organic matter flux are needed to decipher the global extent of deep respired carbon storage.



Oxygen isotope analyses were performed using a Thermo Electron Kiel IV sample preparation instrument with an attached Thermo MAT 253 stable isotope ratio mass spectrometer on samples of N. dutertrei (>250 μm), and took place at the Stable Isotope Geoscience Facilities (SIGF) of Texas A&M University. Isotope values are reported in delta notation (Supporting Information Table 1) relative to the Vienna Standard Mean Ocean Water isotopic standard.

Seven radiocarbon analyses were performed on the first 100 cm of core MV1014-8JC on the planktonic foraminifer Neogloboquadrina dutertrei (>250 μm), and are reported in Supporting Information Table 2. Analyses were performed at the NOSAMS facility at the Woods Hole Oceanographic Institute. Radiocarbon ages were calibrated to calendar age using Calib 7.0 Marine1342,43 with a 400-yr reservoir age correction.

Sediments for MV1014-8JC were sampled approximately every 2 cm and analyzed for uranium, thorium, and barium isotopes using inductively coupled plasma mass spectrometry (ICP-MS) on a magnetic sector Element XR at Texas A&M University. All data appear in the Supporting Information Table 1. To prepare samples for isotope dilution analysis, 0.3–0.4 g of sediment was spiked with 229Th and 236U and then digested in a cocktail of HNO3, HClO4 and HF. Following complete sediment digestion, an aliquot was removed, diluted, and spiked with 135Ba for separate analysis. Samples for U-Th analysis were then further processed through Fe-oxyhydroxide coprecipitation and subsequent anion exchange chromatography in order to separate the Th and U. The National Institute of Standards and Technology Uranium 500 Standard (NIST U500) was used to correct for instrumental mass bias and was analyzed multiple times within each of batch of samples for which Th and U was measured.

Age models

We constructed a preliminary age model using 1) seven radiocarbon dates on N. dutertrei between 0 and 100 cm depth in core, 2) the Los Chocoyos ash (84 kyr)44 identified at 311 cm in the core, and 3) tying the 8JC δ18O record (N. dutertrei) to the LRO4 global oxygen isotope record45 via the software Analyseries46. The stage boundaries between MIS 4 and 5, and MIS 5 and 6 were the most difficult to discern, given the millennial structure in the oxygen isotope data. The age model for core MV1014-17JC was further refined from that in Loveley et al.11. Given the strong correlation between the 230Th mass accumulation rate (MAR) and Heinrich Stadial (HS) events in 17JC, the age model was refined by tuning the additional millennial scale 230Th MAR cycles between HS events to the NGRIP ice core record from 30 kyr to 95 kyr.

230Th Normalization

The ability to accurately determine past sedimentary fluxes is crucial to reliable paleoclimate reconstructions. 230Th is a particle reactive isotope and has a comparatively short residence time relative to its parent isotope 234U (tens of years versus 200–400 kyr)47,48. Scavenging of aqueous 230Th by settling particles leads to its ultimate deposition in marine sediments. The assumption that 230Th flux represents its production rate in the water column allows for the determination of sedimentary MARs. Important to the 230Th flux method is the fact that it allows for differentiation between the vertical flux form the overlying water column and the flux of sediments redistributed by bottom water currents. The latter flux can be discerned by calculating 230Th-derived sediment focusing factors (Ψ)49. The utility of focusing factors lies in their ability to measure periods of focusing and winnowing in different oceanic sedimentary environments.

230Th is preferentially scavenged by fine grain particles because they have a higher surface area to volume ratio50. There may exist, therefore, a biasing effect on the measured activities of 230Th in areas that have also been subjected to grain size biasing during redistribution processes. This would ultimately affect 230Th derived MARs as well. The potential biasing of 230Th-normalized sediment fluxes at highly focused Atlantic sites was modeled with an aim to correct for syndepositional grain size biasing50. It was determined that only sites with focusing factors (Ψ) higher than 5.9 showed significant biasing of the 230Th-derived MARs. Within the Panama Basin, previous studies show that there is no more than a 30% biasing of 230Th-normalized MARs when Ψ is less than about 451. Average focusing factors for the interval of sediment deposited within each oxygen-isotope stage (MIS 1 through 6) are consistently less than 4. The highest average focusing factor is 4.5 during MIS 2. Furthermore, xs230Th-normalized accumulation rates of proxies that are contained predominantly in the fine-grained fraction of the sediment (such as the 232Th, xsBa and authigenic U proxies used here) are not significantly sensitive to the 230Th fractionation observed during sediment redistribution processes, which seems to affect coarse-grained component accumulation rates to a greater extent52. Therefore, accumulation rates for proxies that are virtually entirely contained within the fine-grained component of the sediment can be approximated by multiplying the concentration of the proxy with the 230Th-derived MAR.

232Th Flux

Windblown dust is primarily supplied to ocean sediments from continental material, which has an average 232Th crustal concentration of 14 ppm53. The fraction of dust in sediment samples can, therefore, be estimated by dividing the sample 232Th concentration by 14 ppm. Numerous studies in the past have used 232Th as a proxy for windblown dust in the equatorial Pacific Ocean (see11, and references therein) in this way. We prefer to give the raw 232Th fluxes here rather than converting to dust fluxes so that the reader can more easily compare to previous studies in the literature which use different average dust 232Th concentration.

xsBa Flux

The association between biogenic “excess” Ba (xsBa) delivered to ocean sediment as the mineral barite17, and organic matter permits the use of xsBa fluxes as a proxy for past primary productivity17 timescales. To calculate the xsBa concentration in sediment samples, the detrital Ba component must be subtracted. This detrital, or lithogenic component is estimated by multiplying the detrital Th concentration by the average upper crustal Ba/Th ratio of 51.454. Because barite is primarily found contained in the sediment fine-grained fraction of <5 μm17, 230Th-derived xsBa fluxes are likely not biased by syndepositional sediment redistribution52.

Authigenic U Concentrations

Uranium is supplied to the sediments by the deposition of organic matter, sediment pore water redox conditions, and diffusion from higher concentrations in bottom waters to lower concentrations in pore waters55. Dissolved uranium present in pore waters exhibits similar redox behavior to iron. Near the sediment sub-oxic to anoxic boundary, iron is reduced from Fe(III) to Fe(II), and uranium, present as the highly soluble UO2(CO3)34− complex, is reduced from U(VI) to U(IV), leading to the precipitation of authigenic uranium, presumably as insoluble uranium oxide56. Authigenic uranium enrichment can, therefore, be produced by high rates of organic carbon deposition55, and/or changes in bottom water oxygenation57. Moffitt et al.21 estimate that authigenic U values greater than 5–10 ppm (such as those observed here in the EEP) represent times of severe hypoxia ([O2 concentrations < 0.5 mL/L).

Data availability

U, Th, Ba, and oxygen data will be archived at the National Oceanic and Atmospheric Administration National Centers for Environmental Information (NCEI) database upon publication and are also available as a supplement to this manuscript.


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This research was funded by NSF grant OCE-1803803 to F.M. Additional financial support was provided to F.M. by the Jane and R. Ken Williams Chair in Ocean Drilling Science, Technology, and Education. We thank L. Romero for her technical assistance in the laboratory. We are grateful to the helpful comments made by Babette Hoogakker and one  anonymous reviewer.

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F.M. designed the study. R.H. performed the U-Th and Ba isotope analyses. All authors contributed to the interpretation of the data. F.M. and R.H. wrote the manuscript, R.H., F.M., and J.E.H. prepared Figures 1–5, and F.M., R.H., J.E.H., and M.W.S. provided comments and revisions.

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Correspondence to Franco Marcantonio.

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Marcantonio, F., Hostak, R., Hertzberg, J.E. et al. Deep Equatorial Pacific Ocean Oxygenation and Atmospheric CO2 Over The Last Ice Age. Sci Rep 10, 6606 (2020).

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