Hydrobiologia 517: 1–13, 2004. © 2004 Kluwer Academic Publishers. Printed in the Netherlands. 1 On the celestite-secreting Acantharia and their effect on seawater strontium to calcium ratios Patrick De Deckker Department of Earth and Marine Sciences, The Australian National University, Canberra ACT 0200, Australia E-mail: [email protected] Received 27 April 2003; in revised form 16 August 2003; accepted 10 September 2003 Key words: Acantharia, sarcodine protozoan, strontium sulfate, Indian Ocean, coral palaeothermometry, seawater chemistry Abstract Significant variations in the Sr/Ca in waters from the eastern Indian Ocean in the vicinity of Australia, both from the surface and from shallow depth profiles, are documented. The strontium sulfate-secreting protozoans Acantharia, which are common in the upper 400 m of the oceans, especially at low latitudes, contribute substantially to changes in the Sr/Ca of oceanic waters by extracting Sr for the formation of their skeletons. Below such depths, these organisms dissolve and the Sr/Ca of seawater regains its ‘conservative’ nature. This mechanism accounts for some of the variability of the Sr/Ca near the surface of the ocean, but this may still be found at depth as surface waters become entrained at greater depths. It is argued here that the noted Sr/Ca variations may explain discrepancies between coral data sets from different parts of the oceans, and calls for caution when reconstructing sea-surface temperatures from the Sr/Ca of corals. Introduction Acantharians are common inhabitants in all oceans. This unique group of sarcodine protozoans secretes a skeleton made of the mineral celestite, SrSO4 . Because seawater is grossly undersaturated with respect to this mineral, the remains of these planktonic organisms readily dissolve and are very rarely encountered as fossils. Hence, the study of acantharians has been neglected by geologists and palaeoceanographers, although these organisms are among the most abundant members of the plankton in the oceans (Beers et al., 1975; Bishop et al., 1977; Michaels, 1988), frequently surpassing that of the calcareous test-forming foraminiferans. Acantharian numbers in the equatorial Atlantic Ocean can reach up to 744 specimens m−3 , compared to a value of 105 m−3 at high latitudes (Bottazzi, 1978; Bottazzi & Andreoli, 1982). In the North Pacific Central Gyre, Michaels (1988) counted 16 specimens per litre in the upper 20 m of the water column, but numbers dropped down to 10 between 40 m to 120 m. In comparison, foraminifers amounted to less than 1 specimen per litre in the upper 80 m of these samples (Michaels, 1988). Commonly, the maximum density of acantharians in the oceans is found between 50 and 200 m, but figures vary between studies, and the type of mesh size for plankton sampling devices can substantially affect results; even the nature of the preservative used is important as some selectively dissolve acantharian spicules (Beers & Stewart, 1970). Also, to undergo gametogenesis, some acantharians migrate to depths between 300 and 400 m (Bottazzi, 1978). With respect to seasonal abundance, the pioneering taxonomic and ecological observations of Schewiakoff (1926) for the Bay of Naples showed that these organisms are especially abundant from late spring to the beginning of autumn. In addition, studies from the seas around Italy identified that salinity is also a controlling factor in the abundance of acantharians (Bottazzi, 1978), with high specimen counts even at salinities up to 38.3% (Bottazzi & Andreoli, 1978). During the two Australian cruises in the eastern Indian Ocean, on board the RV Franklin, numer- 2 ous acantharian specimens were recovered from surface plankton tows at the sites where water samples and CTD profiles were obtained. The abundance of the acantharians collected was on average 100 times higher than the live foraminifers and radiolarians; acantharian densities were consistent with other oceans (Beers et al., 1975; Bishop et al., 1977; Bottazzi & Andreoli, 1982; Michaels et al., 1995). Acantharians were most abundant between latitudes 14◦ and 25◦ S. The aim of this paper is to present chemical analyses of water samples collected during the 2 cruises and also document the presence of acantharians collected at the same stations. Material and methods During two cruises with the RV Franklin in the eastern Indian Ocean in late 1995 [Fr10/95] and early 1996 [Fr2/96], numerous surface plankton samples were collected. The plankton samples were collected by towing a circular plankton net, 40 cm in diameter and with a 150 µm mesh, through the surface of the ocean for approximately 1 km. About 4 m3 of water passed through the plankton nets. No quantitative effort was made to estimate the number of plankton species per volume of water sampled, although it is estimated that approximately 125 m3 of surface water were sampled. Once the towing was completed, the plankton sample was immediately filtered through a small 10 cm diameter net (mesh 60 µm) and rinsed thoroughly with distilled water to get rid of any remaining sea water (to prevent a flocculant from forming once ethanol is added to the sample, and also to prevent dissolution of the acantharians as seawater is undersaturated with respect to celestite – see Discussion later). The samples were then preserved in 100% ethanol. Water samples were collected from both the ocean surface and depth profiles. The water samples used for chemical analyses were filtered through a 0.45 µm Millipore membrane using a peristaltic pump, acidified with a few drops of ultrapure HNO3 . The seawater samples were all analysed on a Perkin Elmer Elan 6000 ICP-MS, with the use of a Perkin Elmer FIAS 2000 (used as an online auto-diluter) and a Perkin Elmer AS-90 auto-sampler. Two sets of samples and standards were prepared. Both sets of samples and standards were analysed for Ca42,43,44, Sr86,87,88, Ba134,135, Sc45 and Y89 . The first set comprised a 1 in 10 dilution of the original samples and stand- ards, the second set was prepared as the first, but included spikes of internal standards of Sc45 and Y89 , resulting in end concentrations of 9 and 0.9 mg l−1 , respectively, in every sample and standard. A further 1 to 10 dilution was carried out for all samples and standards using a Perkin Elmer FIAS 2000 running as an online auto-diluter, feeding directly into a Ryton Cross Flow Nebulizer/Spray Chamber attached to a Perkin Elmer Elan 6000 ICP-MS. Artificial seawater was used to make up the analytical standards; these were also crossed-checked against natural seawaters spiked with Ca, Sr and Ba standards to determine analytical performance of the technique. In the first set of samples, Sc and Y concentrations proved to be low [less than 20 µg/l], but raw counts were still used as minor corrections for Sc45 and Y89 concentrations in the results from the analysis of the second set of samples. The results of the second set of samples were used only, as the corrected internal standards, Sc45 for Ca44 and Y89 for Sr88 , could be used to correct for matrix interference, instrument drift and short-term noise in the second analysis on the analyses of interest. A further 8 sub-samples were analysed as duplicates, and 6 sub-samples were analysed using Methods of Standard addition on both a Perkin Elmer Elan 6000 ICP-MS and a Perkin Elmer 3100 Atomic Absorption Spectrometer, as cross-checks on the original analysis. Considering ICP-MS analysis is not the ‘favoured’ technique for the analysis of seawater, this technique showed considerable promise. However, errors associated with large dilutions (this was partially corrected for with the addition of internal standards at the beginning of the dilution stages), and the production of a suitable standard solution, matrixmatched to the samples, continued to cause small problems. All samples with standards greater than 5% were re-analysed. Results A total of 65 surface water samples was analysed from the region between 108◦ E and 13◦ E and 12◦ S and 32◦ S and their location are shown in Fig. 1a. Note that none of the surface samples were taken in less than 50 km from the Australian coastline to prevent possible ‘contamination’ from likely fluvial sources. A broad range of salinities was encountered spanning from S = 33.69 to S = 35.91 and those values are schematically contoured in Fig. 1b. Variations were also noted for Ca and Sr measurements, and again the 3 Figure 1. Maps of the eastern Indian Ocean adjacent to Western Australia showing the location of the sea-surface samples (dots) taken during the two Franklin cruises in December 1995 (= Fr10/95) and February–March 1996 (= Fr2/96) (1a) and the location of the rivers which contribute to continental outflow, especially during the monsoonal season. 1(b) shows the salinity contouring based on the data obtained during the 2 cruises; 1(c) displays the contouring for Sr/Cl (as µg/g); 1(d) the measured molar Sr/Ca values in mmol/mol; 1(e) and 1(f) display the contouring for Ca and Sr in ppm respectively. Chlorinity values used in 1c were obtained using the relationship of S() = 1.80655 Cl() (Chester, 1990). Salinity values were obtained by conductivity measurements while at sea, and recalibrated later by CSIRO personnel. The location of the 3 sites with CTD profiles displayed in Fig. 2 is shown by black crosses in the above map. values are schematically contoured in Figs 1e, f. Ratios of Sr/Cl as well as Sr/Ca were also computed and are displayed in the same fashion in Figs 1c, d. Water samples from three CTD [conductivity-temperaturedepth] profiles were selected for chemical analyses and the Sr/Ca results are presented against salinity in Figs 2a–c. All data used for the present paper are available on the Springer server. Discussion Surface waters Surface water data from these Franklin cruises show a typical patchiness with respect to all measured elements, either tabled singly or displayed as ratios such as Sr/Ca or Cl/Sr (Figs 1a–f). The latter ratio was used to determine whether a relationship could be found between salinity and the concentration of Sr. This could not be found. Patchiness of Sr values in upper waters in the oceans had already been documented in Renard’s (1985) review, and more recently for several 4 Figure 1(b). (Continued.) sites adjacent to the Hawaiian islands where corals grow (de Villiers et al., 1995). Close examination of the location of the major rivers bordering the Western Australian coast (Fig. 1a) shows no obvious links between chemical and salinity variations found offshore (Figs 1b–f), despite the fact that half of the water samples were collected in December 1995 when three cyclonic depressions occurred in the region with substantial rainfall, and river discharge ensuing. Equally, no link was found in February–March 1996 when the rest of the water samples were taken. Overall, salinity displays lower values at the lowest latitudes and highest salinities are recorded near 28◦ –30◦ S where evaporation is highest in the region. Nevertheless, salinity values ≥ 34.6 are noticeable on the northwest shelf and these correspond also to the overall high Sr/Ca values. A possible explanation being that very likely fine needles of CaCO3 may precipitate due to the high salinities and temperatures at the end of the ‘dry’ [=austral winter] season caused by some supersaturation in CaCO3 . However, this hypothesis requires testing as a comparison between the plots for salinity (Fig. 1b) and Cl/Sr (Fig. 1c) show no obvious similarity with Sr/Ca (Fig. 1d). Depth profiles Characteristically, in some profiles obtained using conductivity-temperature-depth [CTD] equipment, Sr/Ca ratios also show a systematic depletion of Sr in the upper portion of the water column (see 5 Figure 1(c). (Continued.) Figs 2a–c). This pattern is reminiscent of profiles from the Atlantic (McKenzie, 1964; Brass & Turekian, 1972, 1974; Bernstein et al., 1987) and Pacific (Brass and Turekian, 1973, 1974; Brass, 1980) Oceans, and the same was recently found also by Müller & De Deckker (2003) from a region near Tasmania and New Zealand at the confluence of the Indian, Pacific and Southern Oceans. More importantly, de Villiers (1999) concluded from her work in the Atlantic and Pacific Oceans that ‘seawater Sr and Sr/Ca exhibit spacial gradients of 2–3% globally with the deep ocean enriched relative to the surface’. This is investigated further below by attempting to determine the cause of seawater Sr/Ca variability. However, despite the lowest values recognized near the surface in all three CTD profiles (for explanation see Discussion below), another phenomenon showing a variation in the Sr/Ca with depth is noticeable. Examination of the salinity–temperature profiles for the 3 CTD sites (Station Fr2/95-36 at 14◦ 48.68 S 114◦ 16.37 E; Station Fr10/95-39 at 28◦ 44.35 S 112◦ 47.89 E; station Fr10/95-28 at 20◦ 01.93 S 112◦ 43.37 E) help identify the various water masses encountered in the region. Importantly are (1) the Indonesian Throughflow water (= ITF in Fig. 3) which is characteristically of low salinity, (2) the Indian Central Water (= ICW in Fig. 3) which is at the other extreme with its highest salinity, and (3) the other two water masses the Subtropical South Indian water (= SSIW in Fig. 3) and the South Indian Central Water (= SICW in Fig. 3). The latter two water masses are intermediary between the ITF and the ICW. It is noteworthy that the ICW, recognized in Fig. 2c at Station Fr10/95-28 between ∼200 and 300 m water depth, also has a high 6 Figure 1(d). (Continued.) Sr/Ca as for the other 2 profiles below the surficial Sr/Ca-‘depleted’ layer. The surprising feature, however, is that below the ICW lens at Station Fr10/95-28, Sr/Ca return to low values; these waters belong to watermasses (SSIW and SICW) that originated at the surface at higher latitudes, and at the time of their formation, may also have been ‘depleted’ in Sr/Ca and remained as such. The acantharian skeleton and seawater Sr/Ca The acantharian skeleton is made of fine SrSO4 needles/spicules and rapidly becomes dismantled upon death once the protoplasm decomposes, falls through the water column [probably fairly rapidly due to its high (3.96) specific density] and consequently dissolves readily (Beers et al., 1975). Acantharians are rare or non existent below 1500 m as recognised from trap studies (Beers & Stewart, 1970). This explains the change in the Sr composition of seawater as acantharians utilise a substantial amount of Sr in the upper parts of the water column where they live and secrete their test, but this element is returned into solution once spicules dissolve while they sink. Several studies have alluded to the substantial uptake of Sr by acantharians from their ambient waters. Estimates for one acantharian vary between 20.6 µg cm−2 yr−1 (Bernstein et al., 1987) and 22 to 40 µg cm−2 yr−1 (Brass, 1980). Again, estimates vary between the amount of Sr acantharian skeletons contain; 0.2 nmol (Bishop et al., 1977) and between 5–49 nmol (Bernstein et al., 1987) based on mean weights. Assuming a mean value of 20 nmol of Sr, an acantharian specimen would require 0.76 µg of Sr to fabricate its acicu- 7 Figure 1(e). (Continued.) lar skeleton; for an average number of 10 specimens per litre at anyone time, up to 7.6 µg of Sr would be taken from the ambient seawater. As an example, with 2 acantharian generations per year, and an average residence time of 25 years for the upper waters in the ocean, an acantharian population would have extracted 380 µg of Sr from 1 l of seawater over those years. By this process, the Sr can be extracted from the original water sample, provided there is no mixing with underlying waters, and explains the 5% areal and vertical variations of Sr/Ca in the upper 400 m of the water column. de Villiers (1999) discussed the characteristic depletion of Sr variations in the upper few hundred metres in her samples form the Atlantic and Pacific Oceans with respect to deeper horizons below. She concluded that the dissolution of acantharians contrib- ute to a significant increase in the upper part of the ocean [below the horizon near the surface which is depleted in Sr as a result of Sr uptake from acantharians], but that also a secondary influence is caused by calcium carbonate cycling. It is suggested here that different upper-ocean water masses may, in fact, also have Sr/Ca values as illustrated in Fig. 2c for the profile which displays an obvious correlation between salinity and Sr/Ca. It may be that partially-evaporated seawater may have chemically evolved differently, such that aragonite needles may have precipitated at high salinities [and high temperatures], thus forcing a ‘partial’ depletion in Sr values. Such a phenomenon could be expected on the northwest shelf of Australia where intense evaporation does frequently occur and high salinities are generated. 8 Plate 1. SEM photos of acantharians collected in plankton tows during the RV Franklin cruises in the eastern Indian Ocean. Collection stations with coordinates are listed after the identification. (A) Acanthocolla cruciata Haeckel with spicules partly broken (Fr2/96–19; 15◦ 00.12 S 110◦ 29.80 E); B, F: Acanthostaurus purpurascens Haeckel (Fr2/96-26; 21◦ 59.76 S 107◦ 42.71 E); C: Phyllostaurus siculus Haeckel with shrunk protoplasm still visible (Fr2/96-18); D: Amphibelone hydrotomica Haeckel with juvenile planktonic foraminifers stuck in between the spicules (Fr2/96-18); E: Coleapsis vaginata Haeckel (Fr2/96-26). Note scale bars for all specimens represent 50 µm and the background which consisted of carbon tape has been artificially erased. 9 Plate 2. SEM photos of acantharians collected in plankton tows during the RV Franklin cruises in the eastern Indian Ocean. Same remarks about collection stations as for Plate 1. (A), (B) Diploconus aff. fasces Haeckel (note juvenile planktonic foraminifers for relative scale) (Fr2/96-19); (C) Amphibelone anomala Haeckel (Fr2/96-19; 26◦ 59.68 S 109◦ 29.68 E); D: Acanthospira spiralis Haeckel with possible radiolarian stuck among the spicules and with some shrunk protoplasm still visible (Fr2/96-36; 14◦ 48.68 S 114◦ 16.37 E); (E) Phyllostaurus siculus Haeckel with shrunk protoplasm still visible and a juvenile planktonic foraminifer adhering to some of the spicules (Fr2/96-36); (F) possible early stage of Pleuraspis costata Müller with some protoplasm also visible (Fr2/96-19). Note scale bars for all specimens represent 50 µm and the background which consisted of carbon tape has been artificially erased. 10 Figure 3. Temperature-salinity profiles obtained with CTD equipment for the 3 stations discussed in the text (36 = Fr2/96-36; 39 = Fr10/95-39; 28 = Fr10/95-28]. The various watermasses of relevance to the discussion in this paper are labeled on these profiles. These are: ITF for Indonesian Throughflow; SSIW for Subtropical South Indian Water; SICW for South Indian Central Water; ICW for Indian Central Water (nomenclature after Fieux et al., 1996). Implications of seawater Sr/Ca Figure 2. Continuous salinity profiles measured by CTD (bold line) and Sr/Ca (in mmol mol−1 ) (thin line with dots showing the depths of sampling using Niskin bottles) taken for 3 selected sites during the two Franklin cruises (see text for more details) to show the characteristic depletion in Sr in at least the upper 200 m of the ocean, and the increase at various levels down to 1000 m where acantharians would completely dissolve. Note the broad range of salinities resulting from the sampling of different water masses, and the different depths displayed for those profiles. In particular, note the relationship in (2c) between salinity and the Sr/Ca measured at station Fr10/95-28. The residence times for calcium and strontium in today’s oceans have been estimated to be of the order of 1.1 × 106 and 4.9 × 106 years, respectively (Martin & Whitfield, 1983; Chester, 1990) and, consequently, the ratio of these two elements has been considered by many to be constant for the entirety of the Quaternary. This assumption led to the use of Sr/Ca fluctuation detected in the skeleton of modem and fossil corals as a proxy for sea-surface temperature changes in tropical oceans (Smith et al., 1979; Beck et al. 1992; McCulloch et al., 1994; Min et al., 1995; Beck et al., 1997; Alibert & McCulloch, 1997; McCulloch et al., 1999; Schrag, 1999). Nevertheless, there have been ample published accounts documenting significant variations in either Sr, or in the Sr/Ca and Sr/Cl ratios of seawater in the open oceans (Andersen et al., 1970; Brass & Turekian, 1972, 1973, 1974; Bernstein et al. 1987; Bernstein et al., 1992; de Villiers et al., 1994; de Villiers, 1999). These findings have been ignored by most of those using the coral Sr/Ca as a palaeothermometer. These contradicting views need resolving, especially since there are now several claims for substantial sea-surface temperature differences between the present and previous episodes of the Late Quaternary (e.g., for the Last Glacial Maximum) (Guilderson et al., 1994), or younger episodes (Beck et al., 1992, 11 1997) that are in conflict with sea-surface temperature reconstructions using other proxy methods such as foraminiferal faunal assemblages (CLIMAP, 1981; Anderson et al., 1989; Martinez et al., 1997) or Uk37 analyses from the remains of calcareous nannoplankton (Bard et al., 1997). Here, additional chemical analyses of seawater samples from the eastern Indian Ocean are presented and these identify that the Sr/Ca of waters at the surface and through profiles is again not constant throughout in an oceanic region where corals live. Seawater Sr/Ca and coral palaeothermomet Plate 3. SEM photos of acantharians collected in plankton tows during the RV Franklin cruises in the eastern Indian Ocean. Same remarks about collection stations as for Plate 1. (A) Acanthostaurus purpurascens Haeckel with some shrunk protoplasm visible and a smaller acantharian adhering to some of its spicules (Fr2/96-19); (B) Amphibelone hydrotomica Haeckel (Fr2/96-15; 23◦ 44.23 S 108◦ 31.91 E); C: Amphilithium clavarium var. lanceolatum Schewiakoff with several planktonic foraminifers and one radiolarian adhering to numerous other ancantharian spicule debris; one dinoflagellate is also visible at the opposite end of the debris amalgamate (Fr2/96-36). Note scale bars for all specimens represent 50 µm and the background which consisted of carbon tape has been artificially erased. The analytical data presented here seriously question the validity of using the Sr/Ca of fossil corals in reconstructions of past sea-surface temperatures, because calculated temperature shifts (Beck et al., 1992; Guilderson et al., 1994; Min et al., 1995; Beck et al., 1997; Schrag, 1999; McCulloch et al., 1999) all assume a constant or near-constant Sr/Ca for the water in which the corals grew. The present study, in addition to others mentioned above, shows that the Sr/Ca of seawater, especially in the realm where corals grow, cannot be accepted to be constant through time and space. It is noteworthy that the several sites and periods for which fossil corals have been analysed represent locations – and periods of time – during which salinity may have changed as a result of reduced precipitation. For example, the ‘postulated’ substantial temperature drop (6.5 ◦ C) at Vanuatu (Beck et al., 1992, 1997) appears to coincide with the occurrence of a significant period of aridity registered in northern Australia at a similar latitude (De Deckker et al., 1991), implying a possible reduction of runoff from the island that could cause a change in the Sr/Ca but not necessarily a change of sea-surface temperature (SST). Foraminifer assemblages from nearby ODP core 828 (Martinez et al., 1997), detect a shift of summer SST of no more that 1 ◦ C over the last 20 Ka, challenging the coral Sr/Ca evidence (Beck et al., 1997). Similarly, for the Barbados coral (Guilderson et al., 1994) which grew during the Last Glacial Maximum (= LGM), a reconstructed SST (e.g., a drop of 5 ◦ C compared to today) may be misleading because of much more arid conditions in the region. So far, no lacustrine cores have returned LGM sediments from the island, very likely due to the extreme dry conditions there during the LGM. The postulated decrease in precipitation is confirmed for adjacent areas in the Caribbean (Bradbury et al. 1981) and could have 12 caused the increase in the salinity and δ18 O of the ambient waters that was originally interpreted as resulting from an SST drop (Guilderson et al., 1994). In addition, at the LGM 1.2 must be added to the salinity to adjust for the fall in global sea level. Similarly, an increase of the Sr/Ca of seawater by 3% (due to a change in the supply of local Sr-depleted continental waters) near the coast where corals usually grow, or a lack of local acantharian productivity, for example, would have registered as a 5 ◦ C temperature drop by the coral Sr/Ca palaeothermometer. Modelling studies (Stoll & Schrag, 1998) on the effect of sea level changes during the Quaternary also postulate that Sr in seawater would have changed during periods of low sea levels. No quantitative measurements have so far been made to verify these models but they support the argument that the basis of coral Sr/Ca thermometry for parts of the Quaternary ought to be looked at more closely. Conclusion This paper argues that acantharians, despite their small size, play an important role in the Sr depletion in the upper few hundred metres of the ocean’s water column. It is argued also that if such ‘Sr-depleted’ waters eventually ‘sink’ or become covered by the water masses, the Sr depletion may remain at greater depths. Such a phenomenon may perhaps be used to actually trace the origin of a water mass. Despite the lack of uniformity in the Sr/Ca of sea water near the surface as shown in this paper, the coral Sr/Ca thermometer remains a very powerful tool for demonstrating secular variations and for recent times’ reconstructions (e.g., the last millennium) as oceanic conditions for that time frame would have changed little. Nevertheless, several studies have identified that the temperature equation using the Sr/Ca in the same species of coral varies from place to place (de Villiers et al., 1994; Beck et al., 1997; Alibert & McCulloch, 1997), showing that oceanic Sr/Ca varies between sites. However, in order to extend past SST reconstructions for periods of the record which registered significantly different conditions – the extreme being during the LGM – such as salinity changes (which could affect acantharian productivity levels (effectively changing the Sr/Ca of seawater locally), light intensity, depth of the nutricline, wind-induced turbulence and mixing of the surface layer of the ocean) caution is definitely warranted. A number of proxies, used together at the same site – such as corals and other methods/organisms – are essential before inferring substantial sea-surface temperature changes at low latitudes during the LGM. Acknowledgements I am thankful to the captains and crew of the Australian National Facility RV Franklin for facilitating the collection of all samples in the eastern Indian Ocean, and the numerous colleagues who helped while at sea, and for several ARC grants to support this work. I benefited from the insight of Dr D. Nürnberg (Geomar, Kiel) who suggested that acantharians play a role in the uptake of Sr in the oceans. He also provided key references and commented on an earlier draft of the manuscript. Mr F. Krikowa of the University of Canberra performed the analyses presented here. Dr T. Corrège provided some cross-checking analyses by ICP-MS. Very profitable discussions with Michael Shelley during the early stages of writing of this paper helped improve the clarity of the arguments and text. Mr C. Hilliker drew the figures and Mr A. Sadekov helped with the photographs. Dr R. Barwick was also provided much valuable advice with the illustrations. I am also grateful to Dr E. Gliozzi who managed to obtain an original of the publication and plates of the important and outstanding work of W. Schewiakoff from the Zoological Station in Naples through negotiations with the librarian there. References Alibert, C. & M. T. McCulloch, 1997. 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