3.6       Seawater evolution

 

Biogenic carbonates fulfil two of the requirements of a sedimentary dating tool: they are fairly resistant to diagenetic alteration, and since they are secreted directly from seawater by the organism, they contain no detrital fraction. Unfortunately, the negligible Rb content of carbonates precludes application of the conventional Rb)Sr dating method. However, calibration of the seawater Sr isotope evolution path would allow the ‘initial’ 87Sr/86Sr isotope ratios of carbonates to be used as an indirect dating tool. In the following section we will assess the realisation of this concept, as well as the application of Sr isotopes as an oceanographic tracer.

 

 

3.6.1    Measurement of the curve

 

Interest in the strontium isotope composition of seawater dates back to Wickman (1948). He argued that decay of 87Rb to 87Sr in crustal rocks over geological time, and its subsequent release into the hydrosphere by erosion, should lead to a 25% increase in seawater Sr isotope composition over the last 3 Byr. This model was tested by Gast (1955), who analysed carbonates of various ages as a means of characterising the evolution of seawater through geological time. However, he found that any natural variations were of the same order as the analytical errors of 87Sr/86Sr analysis pertaining at that time (ca. 0.004), thus refuting Wickman’s model. Evidently the average crustal Rb/Sr ratio assumed by Wickman was an over-estimate.

 

            Resolution of the actual extent of seawater Sr isotope variation through time had to wait 15 years for the advent of more precise mass spectrometry. Peterman et al. (1970) measured the 87Sr/86Sr composition of macro-fossil shell carbonates with an order of magnitude improvement in precision (" 0.0005, 2F). They found a total isotopic range of 0.0022 (4 H analytical error), which would have been imperceptible using earlier equipment. Peterman et al. showed that, contrary to Wickman’s prediction, seawater Sr isotope ratio actually decreased during the Paleozoic, reaching a minimum during the Mesozoic before rising quickly to a maximum at the present day.

 

            In order to avoid the effects of post-depositional alteration, Peterman et al. rejected any recrystallised shell material, which they claimed to be able to recognise visually. The possibility of Sr exchange between matrix and un-recrystallised shells was rendered unlikely by the good compositional agreement between different shells in a bed. A mixture of different types of molluscs was used (belemnites, bivalves and brachiopods). Since no variation was seen between such classes at the present day, they were assumed to behave in the same way as fossils.

 

            Additional data were collected by Dasch and Biscaye (1971) and Veizer and Compston (1974) from different types of sample material. Dasch and Biscaye used Cretaceous-to-Recent pelagic foraminifera, whereas Veizer and Compston analysed ‘sedimentary carbonate’ (in other words not macro-fossil carbonate) to test its reliability for the determination of seawater Sr isotope ratios. In both cases the authors found general agreement with the data of Peterman et al. (1970). This implies global homogenisation of seawater Sr, which can be attributed to the very long residence time of Sr in seawater (ca. 2.5 Myr; Hodell et. al., 1990) compared with the average mixing time of oceanic water (ca. 1.6 kyr; section 14.1.7). However, Veizer and Compston recognised that ‘sedimentary carbonate’ is more susceptible to post-depositional exchange with pore-waters. They argued that since detrital grains would normally have radiogenic Sr isotope signatures, post-depositional exchange would normally be expected to raise 87Sr/86Sr ratios. Therefore the minimum Sr isotope ratio found at any given time should be the most reliable guide to contemporaneous seawater composition.

 

            While the analysis of whole-rock carbonate provides fewer constraints on post-depositional processes, it provides more opportunity for sampling, and is essential for Precambrian carbonates. Using the principles outlined above, Veizer and Compston (1976) made a reconnaissance study of the Sr isotope evolution of Precambrian seawater. They found uniformly unradiogenic Sr isotope ratios in Archean carbonates, with values only slightly elevated over contemporaneous upper mantle (Fig. 3.23). However, there was a substantial rise in Sr isotope ratio during the Proterozoic, reaching a maximum in the early Cambrian which was similar to the present-day composition.

Fig. 3.23. Sr isotope composition of marine carbonates over the last 3.5 Byr, from which the isotopic evolution of seawater is deduced (shaded band). After Veizer and Compston (1976).

 

            A major expansion of the seawater Sr data set was achieved by Burke et al. (1982), who presented 786 isotopic analyses of marine carbonates, phosphates and evaporites, with good coverage of all of Phanerozoic time except the Lower Cambrian (Fig. 3.24). In addition, work by Derry et al. (1989), Asmerom et al. (1991) and Kaufman et al. (1993) extended the curve back to the Late Proterozoic. In the absence of fossil material, the latter studies were made principally on whole-rock carbonates, which are susceptible to contamination by fluid-borne Sr during post-depositional alteration. Therefore, Sr was extracted from bulk carbonates by leaching with dilute acetic acid, to reduce the amount of contamination from detrital phases containing radiogenic Sr.

Fig. 3.24. Sr isotope data for Phanerozoic carbonates. Solid line indicates the lower bound of most of the data, which is the most probable seawater Sr composition. After Burke et al. (1982).

 

            Following the wide-ranging study of Burke et al. (1982), subsequent work was generally devoted to improving precision on small segments of the curve. This requires material to be well-dated stratigraphically and carefully screened before analysis in order to exclude the possibility of post-depositional alteration. In Paleozoic rocks, this screening is best achieved chemically. Brand and Veizer (1980) showed that open-system diagenesis of carbonates is accompanied by a decrease in Sr/Ca ratio and an increase in Mn content (Fig. 3.25). However, Mn-enriched calcite can be detected by cathodoluminescence, so that sections of shell can be screened for alteration before sample analysis. Popp et al. (1986) showed that samples of brachiopod shell prepared in this way gave more reliable results than whole brachiopod shells (which were sometimes contaminated by unradiogenic Sr) or whole-rock carbonates (which were usually contaminated by radiogenic Sr).

Fig. 3.25. Summary of diagnostic chemical changes which occur during the diagenetic alteration of carbonates. Boxes represent primary fields. After Brand and Veizer (1980).

 

            The use of high quality brachiopod shells and belemenites from around the world allowed  Veizer et al. (1999) to present a complete Sr evolution curve for the Mesozoic and Paleozoic, based on 1450 new analyses. They utilised the interior shell layers from brachiopods and single laminae of belemnites, and much of their material showed excellent preservation of textures on a sub-micron scale, as demonstrated by examination under the scanning electron microscope (SEM). This study therefore represents a successor to that of Burke et al. (1982) in giving an overview of seawater Sr evolution between 100 and 500 Myr ago.

 

            Construction of a very precise seawater Sr isotope evolution curve for the last 100 Myr was made easier by the availability of numerous Deep Sea Drilling Project (DSDP) cores. These cores provide overlapping continuous sections with well preserved microfossils such as foraminifera. Relatively constant sedimentation rates in these sections are used to interpolate between biostratigraphic and magnetostratigraphic calibration points. This avoids the age uncertainty involved in correlating short stratigraphic sections from different localities.

 

            Two different sampling approaches have been adopted for DSDP core material. DePaolo (1986) made a study on a single DSDP hole reaching back to the Early Miocene, but with duplicate analysis of all samples to improve analytical precision. In his approach, bulk samples of foram)nano-fossil ooze were analysed by direct acetic acid leaching of washed whole-rock samples. This necessitates a correction for post-depositional exchange, in order to determine original seawater compositions. These corrections were based on the analysis of pore waters. However, pore waters displayed relatively small deviations in 87Sr/86Sr from the carbonate fraction (< 0.0001), and were also found to have Sr contents an order of magnitude lower (Richter and DePaolo, 1987). Hence it was argued that corrections for Sr exchange were smaller than mass spectrometric reproducibilities.

 

            In the other approach (Hess et al., 1986), hand-picked whole foram tests were analysed. These were screened for secondary alteration by SEM examination and chemical analysis (e.g. Mn and Sr content). Fig. 3.26 shows data from eight partially overlapping DSDP sections. Slight scatter is seen, but much of this can be attributed to analytical error rather than diagenetic effects. In selected samples from two sites, pore-waters had very similar isotope ratios to forams. At one other site, pore waters were somewhat more radiogenic, but there was no evidence that the foram data had been perturbed. Most subsequent studies have also employed hand-picked forams. Since less than 50 ng of Sr is now needed for a precise analysis, this may be possible on a few or even a single foram. As an additional precaution, Martin and Macdougall (1991) were able to break open large Cretaceous forams to examine them by SEM for internal calcite growth.

Fig. 3.26. Plot of Sr isotope ratio against age for forams from eight DSDP holes (distinguished by symbol shape). Solid symbols and crosses indicate most reliable data; open symbols may be slightly disturbed. After Hess et al. (1986).

 

            The high-precision seawater Sr isotope evolution curve can be used as a stratigraphic dating tool, with a (conservative) precision as good as 0.5 Myr for periods of rapid Sr isotope evolution, but as bad as 2 Myr during periods of slow isotopic evolution. This precision cannot compete with biostratigraphic dating in the Cretaceous and Tertiary periods, but it may be useful for calibration of un-fossiliferous borehole sections (e.g. Rundberg and Smalley, 1989; McArthur et al., 2001).

 

            An interesting observation by Hess et al. (1986) in their Cretaceous)Tertiary data set was a ‘spike’ in seawater Sr isotope ratio at the so-called ‘K)T boundary’ (Fig. 3.26). They speculated as to whether a meteorite impact could have released sufficient Sr, either from the bolide or the terrestrial impact ejecta, to explain this peak. If the spike in 87Sr is attributed to a meteorite, it is critical to demonstrate that it occurred at exactly the correct stratigraphic level. Martin and Macdougall (1991) collected data from four widely spaced localities around the world which appeared to support the model. However, detailed analysis of sample suites close to the K)T boundary in Denmark and Antarctica failed to find such a spike (McArthur et al., 1998). Instead, the data of McArthur et al. (1998) fitted the lower bound of the more-scattered older data (Fig. 3.27), suggesting that the elevated values in these older studies reflect diagenetic alteration, despite the precautions taken to exclude this effect.

Fig. 3.27. Variation of Sr isotope ratio in the vicinity of the K-T boundary, showing data of McArthur et al. on macro-fossils and leached chalk ( !) in comparison with data from Martin and Macdougall, 1991 ( " ). After McArthur et al. (1998).

 

            To examine this problem further, MacLeod et al. (2001) studied Sr isotope variation in a section across the K)T boundary in a DSDP hole off Florida. Because this section is close to the impact site, the spherulitic K-T boundary horizon here is 10 cm thick, and can therefore be studied in more detail. Bulk carbonates from the spherulitic layer itself are radiogenic, due to Sr exchange with silicate phases (Fig. 3.28). However, to test for global seawater Sr variations, MacLeod et al. analysed the isotopic compositions of two different groups of foraminifera in the vicinity of the boundary. The results (Fig. 3.28) showed that forams found only above the boundary (Tertiary taxa) generally had more radiogenic Sr than those that straddled the boundary (Cretaceous taxa).

 

            MacLeod et al. considered two alternative explanations for these observations. One is that the Tertiary taxa (solid symbols in Fig. 3.28) were more susceptible to contamination by overgrowths because they have thinner tests. However, an analysis of such overgrowths suggested that this might lower rather than increase the 87Sr/86Sr ratio (Fig. 3.28). The other explanation is that the Tertiary strata were contaminated by Cretaceous forams reworked elsewhere from below the boundary and then carried into the section as clastic sediment. The fact that the drill hole comes from part way down the continental slope makes this a significant possibility. This would imply that the Tertiary taxa best represent the composition of seawater Sr after the impact, and hence that a very small (0.00003) increase in seawater 87Sr/86Sr ratio occurred across the boundary. This suggests that the impact event at the boundary did have a small effect on seawater Sr. However, this evidence needs to be tested at a site less susceptible to sedimentary reworking.

Fig. 3.28. Variation in St isotope ratio in different sample types at the K-T boundary, from a DSDP site off Florida. ( " ) = Cretaceous foram taxon; ( ! ) = Tertiary foram taxon; ( <> ) = dolomite rhomb overgrowths; ( + ) = bulk carbonate; ( x ) = silicate. After MacLeod et al. (2001).

 

            Neogene seawater evolution has provided a challenge to geochemists to find the most short-term variations in Sr isotope evolution which can be documented. In early work on this question, Hodell et al. (1990) determined a smooth evolution curve. However, Dia et al. (1992) and Clemens et al. (1993) claimed to observe changes in 87Sr/86Sr, correlated with d 18O, with a periodicity of about 0.1 Myr (Fig. 3.29 a, b, c). This was surprising, in view of the long seawater residence of Sr. However, subsequent work by Henderson et al., (1994) and Clemens et al., 1995) failed to reproduce these cycles in three drill cores (including two used in the original work). Instead, the new data fell on a linear evolution path defined by Hodell et al. (1990). Hence, the apparent periodicity in the earlier work is attributed to analytical artefacts and does not reflect seawater Sr isotope evolution.

 

            For the data of Dia et al. (1992), the analytical artefact was apparently a breakdown in the accuracy of the fractional correction. Thus, Clemens et al. (1995) were able to reproduce the temporal periodicity using a linear-law fractionation correction, but this also generated a positive correlation between 88Sr/86Sr and fractionation-corrected 87Sr/86Sr ratio, indicative of a fractionation bias (section 2.2.3). After correction of this bias, the periodicity disappeared (Fig. 3.29d). The data of Clemens et al. (1993) were not subject to this bias, since the more accurate exponential law was used. However, Henderson et al. (1994) showed that only eight of 75 samples analysed by Clemens et al. (1993) lay outside 2F (95%) confidence limits from the linear evolution path of Hodell et al. (1990). Since four outliers would be expected at this confidence limit, the apparent periodicity in this data set is probably not statistically significant (Fig. 3.29b).

 

Farrell et al. (1995) carried out a study with similar sampling density and analytical precision to the above work, but using 455 samples extending over the past 6 Myr. These data constrain the seawater evolution curve to an average confidence limit of " 0.00002 (2F). The curve shows undulations with a 1 – 2 Myr periodicity which are realistic reflections of changing Sr fluxes, given a 2.5 Myr residence time of Sr in the ocean system.

Fig. 3.29. Comparison between seawater Sr and oxygen isotope data for the past 400 kyr. a) oxygen isotope record; b) data of Clemens et al. (1993) expressed by 2F error limits; c, d) data of Dia et al. (1991) and Henderson et al. (1994) on the same drill core. Modified after Henderson et al. (1994).

 

 

3.6.2    Modelling the fluxes

 

The first model for the Sr isotopic composition of seawater was constructed by Faure et al. (1965) to explain the present-day Sr isotope ratio of the North Atlantic. They suggested that there was a balance between the supply of unradiogenic Sr by erosion of young volcanics, radiogenic Sr from old crustal rocks, and Sr of intermediate composition from the erosion of carbonates. This model was adopted by Peterman et al. (1970) to explain the rise and fall of seawater Sr isotope ratio during the Phanerozoic. Armstrong (1971) supplemented this model, suggesting that peaks in seawater Sr isotope ratio during the Carboniferous and Tertiary periods were due to enhanced glacial erosion of old shields with elevated 87Sr contents (Fig. 3.30). However, in other ways the model remained largely unchallenged.

Fig. 3.30. Illustration of a glacial)erosional model to explain the seawater Sr evolution curve of Peterman et al. (shaded band). After Armstrong (1971).

 

            A major advance in modelling seawater Sr evolution was the proposal of Spooner (1976) that the unradiogenic Sr flux was due to submarine hydrothermal exchange with basaltic crust, rather than sub-aerial erosion of basic rock. Spooner calculated that the hydrothermal flux must be six times the magnitude of the river water Sr flux. However, this was based on high estimates of the isotopic composition of run-off (0.716) and hydrothermally buffered water (0.708). Subsequent analysis of hydrothermal vent waters from the East Pacific Rise (Albarede et al., 1981) indicated much less radiogenic compositions. Albarede et al. estimated the flux of hydrothermally recycled Sr as less than one-quarter of the flux due to continental run-off. This model predicted an average Sr isotope composition of between for run-off between 0.710 and 0.711, in good agreement with major rivers such as the Amazon (Brass, 1976). The magnitudes of present-day Sr fluxes were further refined by Palmer and Edmond (1989), who measured the Sr budget and isotope composition of  hydrothermal vent fluids and of most of the world’s major rivers. Taken together, the complete data set of Palmer and Edmond led to an estimated  global river flux of 3.3 H 1010 mol Sr per year, with 87Sr/86Sr of 0.7119, and an ocean ridge hydrothermal Sr flux of about one-half this magnitude, with 87Sr/86Sr of 0.7035.

 

            The recognition of competing riverine and hydrothermal fluxes raises the question of how these fluxes interacted in the past to cause variations in seawater isotope ratio with time. Spooner (1976) assumed that the hydrothermal Sr flux was fairly constant over time. Therefore, he attributed the increase in 87Sr/86Sr since the Cretaceous principally to an increase in continental exposure (and hence Sr run-off) over the last 85 Myr (Fig. 3.31). In contrast, Albarede et al. (1981) argued that a drop in the ocean ridge Sr exchange flux from a Mesozoic value nearly four times higher was more important than a rise in the flux of continental run-off. However, these two effects are difficult to separate, since they are bound together as a system. A drop in spreading rate causes ridge collapse and a consequent fall in sea-level, so that continental exposure should increase as hydrothermal buffering of seawater decreases.

Fig. 3.31. Plot of seawater Sr isotope composition over the last 85 Myr against % continental flooding (relative to the present land area). After Spooner (1976).

 

            In addition to run-off and hydrothermal exchange, two other fluxes have been proposed to control seawater Sr. One which has been widely accepted, although small in size, is the Sr released from ocean floor carbonates by diagenetic recrystallisation (Elderfield and Gieskes, 1982). This is estimated at about 10% of the run-off flux and tends to dampen isotopic fluctuations because it recycles old seawater Sr.

 

            Another proposed flux is the sub-surface outflow of continental groundwater, from below the water table, into the sea (Fig. 3.32). This flux was termed ‘run-out’ by Chaudhuri and Clauer (1986), who proposed that it could explain seawater Sr isotope fluctuations that are not in harmony with variations in sea-level. For example, run-out would be affected by the length of the continental perimeter as well as the extent of continental uplift, so plate tectonic configurations which form super-continents would be characterised by low run-out, whereas fragmented continents (such as those existing at the present day) should be characterised by high run-out. This model attributes the rising Sr isotope ratio during the early Cretaceous (despite rising sea-level) to progressive continental break-up at that time.

Fig. 3.32. Simplified circulation model for the present day seawater Sr budget. Modified after DePaolo (1987).

 

            Chaudhuri and Clauer suggested that the run-out (continental groundwater) Sr flux could be almost as large as the riverine run-off flux. This proposal has received very little attention over subsequent years, but a similar model was recently proposed by Basu et al. (2001) based on studies of groundwater flow in the Bengal Fan. Basu et al. cited evidence that this groundwater flux could supply as much strontium to the sea as the riverine Sr flux of the Ganges-Brahmaputra system. If this flux was extrapolated world-wide, it might imply a doubling of the continental Sr flux, as proposed by Chaudhuri and Clauer (1986). This would have a fairly dramatic effect on calculations of global Sr fluxes, including a reduction of the estimated oceanic residence time of Sr to 2 Myr. However, our present knowledge of groundwater Sr fluxes is too poor to further constrain the importance of this process.

 

 

3.6.3    The effects of Himalayan erosion

 

            The best opportunity to study the interaction of competing fluxes in the buffering of seawater Sr is during periods of rapid change in isotope ratio with time. The Tertiary represents one such period, which is characterised by an overall trend of increasing Sr isotope ratio, on which several smaller steps are superimposed. These variations can be represented in terms of the rate of change of Sr isotope ratio with time (Fig. 3.33).

 

            Raymo et al. (1988) attributed the general trend of seawater evolution over the last 40 Myr to increased rates of uplift of the Himalayas, Tibet and Andes. This could have caused a substantial increase in the supply of radiogenic Sr to the oceans, since the rivers which rise in these regions (Ganges-Brahmaputra, Yangtze and Amazon) together supply 20% of the total solid load to the oceans. On the other hand, changes in the hydrothermal Sr flux are not thought to have occurred during the Neogene, since ocean spreading rates have been nearly uniform during this time.

Fig. 3.33. Representation of seawater Sr isotope variation in the last 100 Myr in terms of the rate of change per million years. After Richter et al. (1992).

 

            Additional evidence for the control of seawater Sr by Himalayan erosion rates was provided by Richter et al. (1992). Ar)Ar thermochronology was used to date the sudden unroofing of the Quxu granite pluton, corresponding to a period of exceptionally rapid erosion of the Tibetan plateau. The timing of this event, which began 20 Myr ago, matches exactly with the peak rate of change in the seawater Sr isotope record (Fig. 3.33). However, Harris (1995) claimed that there was no evidence in the Bengal Fan for increased Himalayan erosion 20 Myr ago. Instead, he suggested that the inferred 87Sr spike in river water at that time was due to the exposure and chemical weathering of meta-sedimentary rocks with a large budget of leachable 87Sr.

 

            In order to reach a better understanding of how variations in riverine Sr influence seawater Sr, Palmer and Edmond (1989) made the first comprehensive study of the Sr budget of the world’s rivers. This revealed an inverse relationship between isotope ratio and concentration (Fig. 3.34a) which was attributed to mixing between radiogenic Sr from silicate weathering and less radiogenic Sr from carbonate weathering. The Ganges and Brahmaputra, which drain the Himalayan uplift, lie off the general trend. However, within the drainage basin of the Ganges, its tributaries themselves display a mixing line, although with a steeper slope than the other rivers (Fig. 3.34b).

Fig. 3.34. Plot of Sr isotope ratio against reciprocal of Sr concentration. a) For the world’s major rivers; b) for tributaries of the Ganges. After Palmer and Edmond (1989).

 

            Further examination of these data (Palmer and Edmond, 1992) showed that the mixing line for the Ganges system had a more elevated intercept (Sr isotope ratio) than for other rivers of the world, as well as a steeper trend. Palmer and Edmond attributed this pattern to the presence of carbonate rocks in the Ganges watershed with abnormally radiogenic Sr isotope ratios. They speculated that these carbonates had become enriched in radiogenic Sr by exchange with the surrounding very radiogenic silicate rocks.  

 

            Subsequent to this work, more detailed studies have been made of the rivers draining the High Himalayas, which are tributaries to the Indus and Ganges-Brahmaputra  river systems. For example, Blum et al. (1998) analysed river water, rock outcrops, and river-bed sands from the Raikot watershed in northern Pakistan. They showed that river and stream waters define a positive trend on a plot of Sr isotope ratio against Ca/Sr ratio (Fig. 3.35). This trend runs from the composition of marbles and marble sands at the unradiogenic end, to a radiogenic end-member with a much higher Ca/Sr ratio than silicate rocks. Blum et al. speculated that this unknown end-member might be calcite that had inherited its radiogenic Sr during hydrothermal alteration of the surrounding silicate rocks.

Fig. 3.35. Plot of Sr isotope ratio against Ca/Sr ratio for samples from the Raikot river watershed, northern Pakistan. ( ! ) = waters; ( + ) = silicate rocks; ( " ) = carbonate rocks; boxes = proposed end-members. After Blum et al. (1998).

 

            Further study (Jacobson and Blum, 2000) identified disseminated calcite interstitially within silicates, at grain boundaries, and in fracture fillings. This calcite makes up less than 0.5% of the orthogneissic rocks in the Raikot watershed, but appears to dominate the Sr budget of streams draining this terrain. Similar conclusions about the role of carbonate dissolution were reached by English et al. (2000), based on a study of the Seti watershed in western Nepal. In addition, carbonates in the Seti watershed have also been proposed as a source of radiogenic osmium in Himalayan rivers (Pierson-Wickmann et al., 2002).

 

            An alternative explanation for recent increases in the Sr isotope signature of seawater is the onset of Tertiary glaciation, as originally proposed by Armstrong (1971). Hodell et al. (1990) revived this model, attempting to link inflections in the Tertiary Sr isotope evolution path to glacial advances and retreats, and this type of argument has been examined in several subsequent papers. The basis of this model is that glaciation creates rock flour, which is then more susceptible to chemical weathering than in situ crystalline rocks.

 

            Blum and Erel (1995) attempted to quantify the amount of radiogenic Sr that could be released by glacial erosion. In order to do this, they used ammonium acetate leaching to analyse the isotopic composition of exchangeable Sr in glacial moraines. Weathered soils from six moraines in the Wind River Range, Wyoming, displayed a negative correlation between the isotopic composition of leachable Sr and the age of the soil (Fig. 3.36). Most notably, a very radiogenic 87Sr/86Sr ratio of 0.795 was obtained by leaching soil from the youngest (400 yr old) moraine. Blum and Erel used these data to argue that a spike of radiogenic Sr is released by weathering of moraines immediately after glaciation. Modelling of this spike suggested that it could yield an incremental increase in 87Sr/86Sr of 0.00005 for each 100 kyr glacial cycle of the Quaternary period, thus reproducing (within error) the seawater evolution curve for this interval.

Fig. 3.36. Sr isotope ratio in ammonium acetate soil leachates plotted against the geological age of the moraines on which the soils were formed. After Blum and Erel (1995).

 

            The glacial erosion model was further developed by Jacobson et al. (2002), who showed that this could also be a facet of Himalayan erosion. Analysis of exchangeable Sr from weathered moraines, together with the carbonate and silicate fractions, showed that a carbonate fraction as low as 1% by weight could nevertheless supply as much as 90% of soluble Sr to streams that are tributaries to the Indus River system. Although these observations may not be applicable to the whole Himalayan drainage system, they do show that the two competing explanations for Tertiary seawater Sr isotope evolution may be facets of a single model.

 

 

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