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Journal of the Geological Society; 2007; v. 164; issue.5; p. 1065-1072;
DOI: 10.1144/0016-76492006-193
© 2007 Geological Society of London

Discussion

Discussion on Pleistocene calcified cyanobacterial mounds, Perachora peninsula, central Greece: a controversy of growth and historyGeological Society, London, Special Publications, Vol. 255, 2006, 53–69

J.E. Andrews1, M.R. Leeder2, C. Portman3, P.J. Rowe4, J. Smith5, S. Kershaw6 & Li Guo7

1 1 University of East Anglia, School of Environmental Sciences, Norwich NR4 7TJ, UK (e-mail: j.andrews{at}uea.ac.uk)
2 2 University of East Anglia, School of Environmental Sciences, Norwich NR4 7TJ, UK (e-mail: j.andrews{at}uea.ac.uk)
3 3 University of East Anglia, School of Environmental Sciences, Norwich NR4 7TJ, UK (e-mail: j.andrews{at}uea.ac.uk)
4 4 University of East Anglia, School of Environmental Sciences, Norwich NR4 7TJ, UK (e-mail: j.andrews{at}uea.ac.uk)
5 5 University of East Anglia, School of Environmental Sciences, Norwich NR4 7TJ, UK (e-mail: j.andrews{at}uea.ac.uk)
6 6 Department of Geography and Earth Sciences, Brunel University, Kingston Lane, Uxbridge UB3 8PH, UK (e-mail: stephen.kershaw{at}brunel.ac.uk)
7 7 CASP, Department of Earth Sciences, Cambridge University, 181a Huntingdon Road, Cambridge CB3 0D, UK


    Introduction
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
J. E. Andrews, M. R. Leeder, C. Portman, P. J. Rowe & J. Smith write: we were very interested to read Kershaw & Guo's (2006) analysis of the conflicting views on the growth and history of Pleistocene cyanobacterial mounds (bioherms) from the Perachora peninsula in the eastern Gulf of Corinth rift, central Greece. A new field guide to this classic geological area and these spectacular exposures will soon be available (Leeder et al. 2007) and the issues we debate below have an important bearing on regional uplift rates, the role of faulting, and the environmental conditions required for cyanobacterial calcification. We welcome Kershaw & Guo's (2006) fair and balanced account of competing hypotheses for bioherm evolution, and particularly commend and accept their new interpretation of the cavity-dwelling, pendant coralline algae. However, we dispute the more fundamental basis of their interpretations and take this opportunity to discuss them further.

  In the vicinity of Cape Heraion (Perachora peninsula) uplifted Pleistocene shorelines of marine isotope stage (MIS) 5a/c, MIS 5e, MIS 7a/c and MIS 7e age have been mapped (Leeder et al. 2005), and where possible U/Th dated using coral aragonite (Vita-Finzi 1993; Dia et al. 1997; Leeder et al. 2005). The upper part of a prominent terrace, at c. +25 to +30 m above modern sea level, is composed of marine bioclastic marls and carbonates of proven MIS 5e age (Vita-Finzi 1993; Leeder et al. 2005). However, directly below these sediments is a horizon of spectacular bioherms, up to 10 m high (Fig. 1) constructed by calcified cyanobacteria (Rivularia haematites) and coralline algae (Lithophyllum pustulatum). There is controversy regarding the age, stratigraphic relations and environment of formation of these bioherms. They have variously been interpreted as brackish lake deposits forming immediately before the Palaeotyrrhenian (i.e. just before MIS 7; Richter et al. 1979); as brackish water deposits forming in shallow seawater during MIS 5e (Portman et al. 2005); or as freshwater structures forming in an MIS 6 lowstand ‘Lake Corinth’ (Kershaw & Guo 2003, 2006). Attempts to date the bioherms directly by the U–Th method, and therefore corroborate these age speculations, have been problematic. However, the combined dataset assembled by Portman et al. (2005) most strongly supports formation of this horizon of bioherms early in MIS 5e.


Figure 1
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Fig. 1.  Spectacular bioherms at Cape Heraion, here down-faulted by about 10 m from the 25 m terrace (after Portman et al. 2005). In our opinion these giant microbial structures formed very rapidly, early in MIS 5e.

 
The principal problem we have with the interpretations of Kershaw & Guo (2006) is that they recognize only a single stratigraphic horizon of bioherms, the bases of which they find at present-day elevations of –1 to +40 m relative to modern sea level, the difference in elevation being caused by faulting. Our interpretation is different. Although we recognize the elevations recorded, the role of local minor faulting (Leeder et al. 2005, fig. 6a) and the sites illustrated by Kershaw & Guo (2006; figs 3–6), we have carefully mapped two stratigraphic levels of bioherms. The upper level, not considered in our paper (Portman et al. 2005), which detailed development of the lower level bioherms (in our opinion of MIS 5e age), has mound bases at about +40 m today (Kershaw & Guo 2006, fig. 4), c. 20 m above the tops of the lower bioherms. We interpret these upper bioherms as deposits formed during MIS 7 and our detailed mapping of the associated raised marine terrace in the western part of the Perachora Peninsula (Leeder et al. 2005) confirms this. These bioherms are more lithified, and appear much more pitted and corroded by karstic weathering, than the lower ones. At Heraion they are fairly small (typically <5 m high) but with a clear core of calcified Rivularia fabrics overgrown by encrusting marine boundstones. At Heraion they also have a distinctive grey-weathering calcarenite incorporated into their bases, a sediment never seen in the lower bioherm bases. Although we have not yet successfully dated the framework or flowstone speleothem calcites from these older bioherms, their unfaulted elevations are entirely consistent with marine shoreline deposits mapped locally at +35 to +42 m (hereafter c. +40 m) that contain corals dated to MIS 7a/c (Leeder et al. 2005).

Our interpretation of the stratigraphy has a major bearing on the required uplift rates discussed by Kershaw & Guo (2006), because their preferred non-marine interpretation for the bioherms leaves them with the impossible dilemma of having lacustrine bioherms far too high for deposition in the waters of lowstand (MIS 6) Lake Corinth. Their only escape from this is to speculate that uplift rates were two or three times the widely published rates, carefully worked out by accurate mapping and radiometric dating in this western part of the Perachora peninsula (Leeder et al. 2005, fig. 6 and table 2). Regardless of any subsidence of the Rion sill controlling the lowstand level of pre MIS 3 glacial Lake Corinth episodes, they ignore the independently mapped shoreline data at +40 m for the MIS 7a/c highstand. If the MIS 6 lowstand (Lake Corinth) was –60 m and the MIS 7a/c highstand deposits are now at c. +40 m it is impossible to uplift the bioherms at a greater rate than the highstand shoreline of MIS 7a/c without an unproven system of faults that must have been uplifting the bioherms relative to the shoreline deposits. Also, in unfaulted areas, for example, the Heraion car park area west of the prominent NW–SE-trending fault that dissects the tip of the peninsula (Leeder et al. 2005, fig. 6a), the MIS 7 shoreline would have to be >50 m above the tops of the lower bioherms at +20 to +25 m, requiring MIS 7a/c shoreline deposits at +70 to +75 m. As the MIS 7a/c highstand deposits are proven here at c. +40 m (Leeder et al. 2005) we are forced to conclude that their uplift model is wrong. Recognition that the mounds at +40 m are likely to be of MIS 7 age resolves all of these problems and allows uplift to occur at published rates calculated from dated mapped shorelines.

If Kershaw & Guo accept our interpretation that there are two stratigraphic levels of bioherms, and if they stick with their interpretation that the bioherms formed in Lake Corinth during lowstands, they would presumably propose that the lower mounds formed during MIS 6 and the upper mounds during MIS 8? This poses more difficulties with their suggestion that uplift rates were two or three times those calculated from mapped and dated palaeoshorelines. For example, an uplift rate of 0.6 mm a–1 would put the tops of the lower (their MIS 6) bioherms at the observed modern elevation of +24 m, but would also put the tops of the upper (their MIS 8) bioherms at about +155 m, much higher than the observed elevations of about +35 to +45 m. The only way they can avoid this problem and explain the stratigraphy we have mapped without a series of huge and unproven faults (>100 m downthrow) is to have highly variable uplift rates; that is, uplift rates before MIS 6 at about 0.3 mm a–1, which then double after MIS 6, to uplift the whole two-level bioherm stratigraphy as a single block. We find such an uplift history highly implausible.

We also have difficulty with the new suggestion by Kershaw & Guo (2006) that all of the conglomerate–breccia fabrics seen in these bioherms are part of a cave-fill stratigraphy that is genetically associated with faulting of the bioherms during growth. In their interpretation, caves are excavated in the bioherms only where faults have cut through the bioherm framework to expose a softer, erodible core. We are not aware of a single field locality where evidence for this interpretation is available: nowhere have we seen an unequivocal fault plane cutting bioherm framework and being draped by later bioherm growth. Further, no coherent fault structures cutting bioherms were mapped by Kershaw & Guo, who took their structural data directly from Morewood & Roberts (1999). We do agree that at some localities there are boulders and cobbles, some of which are well rounded (Fig. 2) presumably by wave action, and some of which are clearly part of a cave-fill stratigraphy. However, there is no compelling evidence that these caves were anything other than either growth cavities between bioherm framework or, in some cases, sea caves excavated on the coast as part of the complex sea-level changes that these sediments preserve. Indeed, at some of the upper bioherm localities (MIS 7a/c age in our interpretation) well-rounded boulders of former bioherm framework are clearly banked against the bases of the bioherms and associated with small sea-cave notches. We interpret these as wave-modified peri-mound talus in the intertidal to shallow subtidal zone. Moreover, contrary to comments by Kershaw & Guo (2006), there is clear field evidence (Fig. 2) that some of the breccia–conglomerate facies formed by collapse of bioherm framework in the early stages of bioherm growth (Portman et al. 2005) and that the main phase of Rivularia growth, to form the giant bioherms, followed on. We do, however, concede that this breccia–conglomerate facies is local and not widespread as implied by Portman et al. (2005).


Figure 2
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Fig. 2.  Photograph showing two generations of boulders (breccia–conglomerate facies) in the lower bioherms below the prominent +25 m terrace at Heraion. Vertical field of view is c. 10–12 m. Arrow A shows a large boulder (>2 m long axis) of bioherm framework, which is overgrown by subsequent bioherm growth to the cliff top. This relationship demonstrates collapse of bioherm framework early in growth, followed by the main phase of Rivularia growth, to form the giant bioherms. Arrow B shows smaller wave-rounded boulders that post-date bioherm framework growth as part of a cave fill unrelated to faulting.

 
A corollary of not recognizing the MIS 7 age of the upper mounds is that Kershaw & Guo (2006) mix up observations made from sediments that formed about 100 ka apart. Although this does not seriously compromise the main elements of their cave-fill story it does explain why they notice that ‘differences occur between mounds in the degree to which components are preserved’. Their cave fills described at +40 m (their fig. 4) are, in our opinion, MIS 7a/c events, whereas those from the lower mounds (their fig. 5) are MIS 5e events. What we find intriguing is that the MIS 7a/c deposits contain a number of the facies elements, such as the Rivularia-dominated bioherms, cave fills, pendant coralline algae and dripstone speleothems, that are seen again in the MIS 5e bioherms. This suggests to us that the conditions that promoted Rivularia-bioherm growth, and their subsequent history, were repeated a number of times during the late Pleistocene history of the area.

The main objection that Kershaw & Guo (2006) have about the lower bioherms forming in an MIS 5e near-coastal setting (Portman et al. 2005) is that Rivularia haematites is known to grow only in freshwater or brackish conditions today. We do not see the dilemma here: Portman et al. (2005) stated very clearly that Rivularia calcification requires at least 60% freshwater input from submarine springs, and that makes the water salinity during bioherm calcification not more than 15 p.s.u.: brackish by anybody's standards. Neither did Portman et al. (2005) interpret the stable oxygen isotope values as ‘marine’: they interpreted them, in conjunction with other geochemical data, as disequilibium values, caused by the rapid degassing of CO2 from the spring water. Perhaps Kershaw & Guo (2006) have misled themselves about marine indicators by quoting from conference abstracts that represented unfinished, in-progress work by a graduate student? Portman et al. (2005), is a peer reviewed paper that represented, in 2005, our most up-to-date interpretation, and one that clearly superseded any earlier unpublished interpretations.

What we, and others (Richter et al. 1979), find much more difficult to accept, in the non-marine model of Kershaw & Guo (2003, 2006), is the requirement that the marine (albeit euryhaline) coralline alga Lithophyllum pustulatum penetrated metres into the dark interiors of a pre-existing bioherm framework. Lithophyllum growth and photosynthesis in a gloomy submarine cave is one thing, but inside a dark bioherm framework quite another. As far as we can see, Kershaw & Guo (2006) have no answer to this problem either. We prefer the much simpler explanation (Richter et al. 1979; Portman et al. 2005) that the coralline algae within the bioherm framework encrusted crypts in the growing bioherms. With a marine alga as part of the growing framework the bioherms had to form in a coastal setting, albeit of low salinity because of submarine spring discharge.

Although we are pleased that Clive Portman's in-progress conference presentations, where he first suggested that the bioherms contain a history of sea-level changes during marine isotope stage 5e, have been taken up by Kershaw & Guo (2006), there is not yet any hard evidence that the regressive events occurred during the sustained highstand of MIS 5e, and this is why we refrained from asserting this in our earlier study (Portman et al. 2005). Chronology, combined with stratigraphic evidence, is critical to a correct interpretation of events, and the alpha spectrometric U-series date of 127.1 +13.6/–12.2 ka (1{sigma}) (Portman et al. 2005) from the speleothem-flowstones that coat the outer surfaces of Kershaw & Guo's ‘pendant coralline dripstones’ strongly suggests (although it does not prove) formation early in MIS 5e, before the sustained MIS 5e highstand (Portman et al. 2005). We are currently following this up with high-precision U/Th dating and strongly suspect that the sea-level history recorded in these sediments occurred early in MIS 5e as described, for example, by Esat et al. (1999) and Thompson & Goldstein (2005). We are pleased to note that Kershaw & Guo (2006) find two horizons of dripstone speleothem, an observation confirmed by our own fieldwork, and one that might imply two regressive events, potentially consistent with the early MIS 5e Barbados coral data (Thompson & Goldstein 2005). In our opinion, the highstand sediment package is the rather friable bioclastic sediment with coralline–algal and serpulid mounds (Richter et al. 1979) that clearly postdates the bioherms, cave fills and speleothems (above a minor discontinuity; Portman et al. 2005, fig. 6). We have not yet found any evidence for regressive events within this highstand sediment package.

Finally, Kershaw & Guo (2006) have no evidence or credible model to contest the geochemical data presented by Portman et al. (2005). They are forced to explain the unusually high Mg and oxygen isotope values in the bioherm framework as due to some unusual form of diagenesis that ‘inherited’ marine values from the basement limestones, even though this should result in lower Mg values and negative oxygen isotope values (Veizer 1983; James & Choquette 1990). Failing this, they invoke diagenesis caused by seawater immersion of the bioherms during the subsequent MIS 5e highstand. This is testable, because marine aragonite cements, which clearly formed from MIS 5e highstand seawater, are not found within the bioherm frameworks, but occur only as late-stage cavity fills that post-dated both bioherm and speleothem-flowstone formation (Richter et al. 1979; Portman et al. 2005). There is no evidence that a substantial volume of highstand seawater penetrated into the bioherms. Even if pervasive seawater diagenesis had occurred, the geochemical constraints would require total neomorphism of the framework to reset elemental and stable isotope data to high values, without affecting the Sr-isotope composition. This we cannot accept. We know that neomorphism of the bioherm frameworks occurred, but we contend that it was mostly syndepositional or very early diagenetic (Portman et al. 2005). Kershaw & Guo (2006) apparently see a more substantial alteration, an observation incompatible with the geochemical data. A possible explanation is perhaps that they have mixed up observations from the two levels of bioherms. We certainly agree that in the older (in our opinion MIS 7a/c) bioherms, cementation of void space and more extensive neomorphism and alteration of primary fabrics has occurred, but in our paper (Portman et al. 2005) we described fabrics and made geochemical analyses only from the lower, younger, better preserved bioherms.

In conclusion, we see no new information or argument in the study by Kershaw & Guo (2006) that precludes formation of the (stratigraphically lower) bioherms during MIS 5e in shallow seawater associated with submarine freshwater spring flow from faults. Indeed, all of the available evidence assembled so far is consistent with this interpretation, with the added advantage that the uplift rates require no special pleading. We agree that freshwater flow would need to be sustained during bioherm growth, but we do not know how fast these structures calcified. Kershaw & Guo (2003) suggested a 2000 year growth history, but we have no concrete evidence; calcification and growth could have been much faster and without the spring water chemistry data it is impossible to be certain. We have to be prepared to accept that highly unusual circumstances allowed construction of these giant bioherms by Rivularia haematites, structures that may be, in Kershaw & Guo's (2006) own words, ‘unique in the Phanerozoic record’.

12 December 2006

Steve Kershaw & Li Guo reply: The discussion by Andrews et al. of our work on cyanobacterial mounds (which they call bioherms) in the Perachora Peninsula (Figs 1–4) provides a further demonstration of the complexity of these interesting deposits. Andrews et al. begin by reference to our ‘fair and balanced account’, but afterwards seem to ignore our extensive discussion of an MIS 5e age for the mounds. Instead, they focus a robust criticism on the alternative interpretation of an MIS 6 age. Their statements about an ‘impossible dilemma’ and ‘only escape’ in relation to variable uplift rates simply reiterate the discussion by Kershaw & Guo (2006). However, since the publication of our study (Kershaw & Guo 2006) we have realized that the variable uplift problem may be resolved if the behaviour of both the Rion Sill and the Isthmus of Corinth (at the western and eastern ends of the Gulf of Corinth respectively; see Fig. 5) are considered, as discussed below. Also, in our view there is poor evidence for two levels of mounds invoked by Andrews et al., but there is evidence of a higher and possibly older mound level. Therefore we address their discussion, with additional observations.


Figure 5
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Fig. 5.  Late Quaternary sea-level curve (modified from Kershaw & Guo 2006) showing pathways of uplift of the relevant components. The four sloping lines at 0.23 mm a represent the averaged uplift (from Leeder et al. 2005) of the surface on which mounds sit, the MIS 5e terrace top, the proposed MIS 7a/c terraces and the mound near Heraion lighthouse (up to their current positions of at c. +15 m, c. +25 m, proposed c. +40 m and c. +55 m, respectively). Uplift of late Quaternary marine sediments in the Isthmus of Corinth (IC) and two interpretations of the behaviour of the Rion Sill (RS) are shown. The interplay between these two barriers probably created a lake in the Gulf during MIS 6. The inset map shows the locations of IC, RS and the Perachora Peninsula (PP). The significance of the various possible pathways of terrace uplift is discussed in the text.

 

    Behaviour of barriers.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
The depth of the Rion Sill controls the marine connection through the western entrance to the Gulf of Corinth, and the sill subsided through the Quaternary. The sill's subsidence rate may have been much faster than the value previously used by Kershaw & Guo (2003), and is here based on a calculated 0.7 mm a–1 uplift rate on the Psathopyrgos fault, the hanging wall of which includes the Rion Sill, by Houghton et al. (2003). McNeill & Collier (2004) suggested a minimum uplift:subsidence ratio of 1:2 for active faults in the Gulf of Corinth, so that 1.4 mm a–1 subsidence should accompany 0.7 mm a–1 uplift, as plotted in Figure 5. However, even if subsidence and uplift on a fault are equal (a 1:1 ratio, the likely minimum), to allow the known MIS 5a deposits on the Perachora Peninsula (Fig. 5), the Rion Sill presents a major barrier at the western end of the gulf until the last interglacial highstand (G. Roberts, pers. comm.). The sill is generally considered to be –65 m, but this is uncertain, and does not account for sediments deposited on the sill during the late Quaternary; thus the sill's bedrock would be deeper. A suggested current depth of c. –85 m for the bedrock sill would be needed to permit the observed MIS 5a deposits in the Perachora Peninsula (Fig. 5). If this new interpretation is correct, then the first time the Rion Sill was overtopped by Mediterranean seawater was during MIS 5e, if it was subsiding at 0.7 mm a–1. Prior to MIS 5e, access of the sea into the Gulf was via the Isthmus of Corinth rather than the Rion Sill.

The Isthmus of Corinth uplifted through the Late Quaternary approximately along the lines plotted in Figure 5. Deposits dated at c. 205 ka on the Gulf of Corinth side of the Isthmus are currently at a maximum of c. +60 m and rising at a minimum uplift rate of 0.3 mm a–1, according to Collier (1990). Figure 5 suggests that this rate of uplift would not quite permit flooding of the Gulf during MIS 5e and 7, but if the uplift rate was slightly higher, then the Isthmus would have been overtopped during MIS 5e. In fact, corals were found by McNeill & Collier (2004, table 1) in the Gulf of Corinth at 230 ka and older; also, Collier & Thompson (1991) recorded 205 ka oolitic sediments at +100 m. Therefore, if the Rion Sill was a land barrier before MIS 5e, the uplift rate of the Isthmus of Corinth must have been at least 0.5 mm a–1, plotted in Figure 5. Thus, during at least the later part of MIS 6, the Isthmus was a land barrier and the Gulf of Corinth was a lake.

Thus Figure 5 shows that the surface of Lake Corinth during MIS 6 can have been higher than previously interpreted, governed by the Isthmus of Corinth, and allowed lacustrine growth of Rivularia mounds. This interpretation removes the need for a variable uplift rate and negates the criticism by Andrews et al. However, fluctuations in lake level towards the end of MIS 6 would be required to generate the caves in Rivularia mounds prior to MIS 5e flooding.


    Mound levels, faults and shorelines.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
Andrews et al. identified two levels of bioherms (lower, MIS 5; upper, MIS 7a/c); we interpreted only one layer of Rivularia mounds because they are similar. The degree of erosion varies across the mound field probably because of variation in exposure, so physical appearance is not a clear indication of relative age. Both upper and lower mounds have the same order of cave fills (non-marine arrow marine arrow non-marine arrow marine), and this would be remarkable if they are of different ages (discussed below). Also, differences in sedimentary material in the lower portions of mounds, referred to by Andrews et al., may relate to lithological variation of the underlying Heraion marl, and do not necessarily show that the mounds are of different ages. The marl dips gently, and Portman et al. (2005, p. 443) noted some facies variation.

We did not ignore uplifted shorelines, but did not recognize any in the study area (Figs 3 and 4), where breaks of slope are vegetation-covered. For example, the +25 m terrace on the northern side of the peninsula tip is backed by a tree-covered slope that we assumed covered a fault (Fig. 3). On the ground, a palaeoshoreline is not recognizable, and this line was mapped as a fault by Morewood & Roberts (1999). Also, the ‘MIS 7a/c’ age of the upper terrace seems to be based on a few uranium-series dated corals near Vouliagmeni Lake, c. 1.6 km east of the end of the Heraion road (Leeder et al. 2005, table 2). One sample, from Dia et al. (1997), was collected at +30 m, yet corals were inferred by Leeder et al. (2005) to relate to a possible MIS 7a/c shoreline at +35–42 m; the terrace itself does not have a confirmed MIS 7a/c age. Furthermore, in the absence of precise biological sea-level indicators, terraces with a notch at their apparent inner margin do not necessarily record past sea levels; terraces can store debris that may be used by turbulent water to erode a notch below sea level, as observed in modern settings (e.g. Antonioli et al. 2003). This raises a question about the reliability of the use of notches to define the ‘MIS 7a/c’ terrace as a sea-level indicator.


Figure 3
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Fig. 3.  View looking east from near the lighthouse at Heraion of the MIS 5e and (interpreted) 7a/c terraces and cliffs near the west end of Perachora Peninsula. The locations of Figures 1 and 2 are indicated, plus the mapped MIS 5e shoreline of Leeder et al. (2005). The area of broken ground in the foreground and vegetation cover make the identification of palaeo-shorelines subjective in this area. The minor fault mapped by Leeder et al. (2005, fig. 6a) lies at the far end of the broken ground where it meets the MIS 5e terrace. The uplifted block from which the view in Figure 4 was photographed is on the right-hand edge.

 
North of the western end of paved road is an extensive area of broken ground (Fig. 3), the eastern edge of which terminates at the +25 m terrace, coinciding with the northern portion of a NNE–SSW-trending minor fault mapped by Leeder et al. (2005, fig. 6a). The broken ground is rich in damaged Rivularia mounds, but there is little inter-mound sediment, and this damage may be due to human quarrying, although this was not confirmed by local archaeologists. Any faults and/or palaeoshorelines north of the paved road are obscured by this deposit. Furthermore, although Leeder et al. (2005, fig. 6a) continued the NNE–SSW minor fault south to the western side of Heraion harbour, the fault is not apparent on the ground, and was not shown in detailed mapping by Morewood & Roberts (1997). Instead, two east–west faults in the Heraion harbour area (one of them a major fault) controlled topography in the area of the Heraion archaeological site (Fig. 4), together with a NW–SE-trending normal fault located further east. The latter is not recognizable north of the road; it marks the western boundary of an uplifted block on the south coast of Perachora Peninsula upon which sits St. Nicholas Church; the northern boundary of that block is an east–west fault south of the road. Therefore we differ from Leeder et al. (2005) about the location and influence of minor faults at the tip of Perachora Peninsula, and this is important for interpretation of relative heights and displacements of the mounds. Furthermore, Andrews et al. referred to the car parking area at the western end of the peninsula as being unfaulted (Figs 3 and 4). However, north and south of the road, downfaulting in some places and uplifting in others occurs in close proximity; this draws into question just what portions of the rock mass are behaving in a predictable manner, and why we should believe that the central portion rose at a steady rate through the Late Quaternary. However, below, in an attempt at a balanced discussion, we evaluate the history of the mound sequence if MIS 5e and 7a/c shorelines and mounds are valid.


Figure 4
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Fig. 4.  View of the end of Perachora Peninsula looking west from St. Nicholas Church. The proposed MIS 7a/c terrace of Leeder et al. (2005) is shown and the location of the uppermost eroded coralline-dominated mound is 50 m east of the lighthouse. The NE–SW fault mentioned in the text lies directly in front of and below the area shown in the photograph. This fault controls the eastern end of the mini-graben structure in which the Heraion archaeological site lies. The minor fault mapped by Leeder et al. (2005, fig. 6a) supposedly passes through the far edge of the archaeological site and cuts the prominent east–west fault that dissects the end of the peninsula. It should be noted also that the sharp margins of the triangular end of the peninsula are defined by coastal-bounding faults. Other faults, especially the Xylokastro Fault, are interpreted in submarine rocks between the end of the peninsula and the south coast of the Gulf of Corinth visible in the distance.

 

    Coincidences.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
A fascinating aspect of the Rivularia mounds is the seemingly unlikely coincidence of three features: (1) mound growth during a non-marine stage (MIS 6), or possibly one or two marine stages (MIS 7a/c and 5e), of the Quaternary sea-level curve; (2) episodes of expulsion of groundwater interpreted by Kershaw & Guo (2003) and Portman et al. (2005) to have forced mound formation; (3) terraces that were probably no more than 10 m below water level, the depth range of Lithophyllum pustulatum (see Kershaw et al. 2005, pp. 176–177). Then the mounds were exposed to form caves, and resubmerged twice in the sea to receive two layers of apparently marine material (interbedded with non-marine deposits) in caves. Many mounds were encrusted by two episodes of pendent corallines (presumed coeval with the marine cave fills). In the case of the lower mounds, Portman et al. (2005) interpreted this sequence to have been completed during the MIS 5e transgression, and affected by minor sea-level fluctuations prior to the MIS 5e peak, although they seem not to have recognized the complexity of cave-fill stratigraphy. The mound phase was completed before caves formed, and therefore before pendent corallines (composed of only Lithophyllum pustulatum) grew. Although L. pustulatum presumably grew in low-salinity environments within the mounds (noted by Andrews et al.), it is debatable whether the (later) pendent corallines also grew in low-salinity water; so far no proven fully marine fossils are associated with them. If they did grow in brackish water, then the pluvial phase (invoked by Portman et al. (2005) as the primary forcing of expelled groundwater) must have ended or declined, because mounds stopped growing; this suggests lessening or termination of expulsion of groundwaters. However, there is remaining uncertainty about the longevity of diluted seawater, and therefore of the processes that forced it. If expulsion continued at a lower rate, seawater may have stayed dilute long enough to generate the pendent corallines in caves. Altogether, if Andrews et al. are correct, there is a complex sequence to fit into the brief period of submergence of the terrace in rising sea-level prior to the peak of MIS 5e (see Fig. 5). In contrast, there is more time to develop the sequence if the mounds are MIS 6 age, and the pendent corallines grew during MIS 5e, as interpreted by Kershaw & Guo (2006).

It is remarkable that caves in both ‘MIS 7a/c’ and ‘5e’ mounds contain two sets of deposits in the same order; these are of variable thickness up to c. 50 cm, and some are represented by only shelly encrustations on hard surfaces. The two generations of pendent corallines in caves on the north coast (Kershaw & Guo 2006, fig. 6) lie just above the cut terrace of Heraion marl, c. 10 m below the depositional MIS 5e terrace at +25 m. The base of ‘MIS 7a/c’ mounds is a further 15 m higher (at +40 m), so that sea-level variations would have needed to be at least 25 m, prior to the MIS 5e peak, to flood both sets of caves at the same time. The lower three of four lines plotted with an uplift rate of 0.23 mm a–1 in Figure 5 show that this probably did not occur, but confirmation of two different episodes of caves and cave fills will require dating the fills, and perhaps faunal analysis of shell debris. If dating reveals similar ages, then it follows that ‘MIS 5e’ and ‘7a/c’ mounds were the same age and have been displaced by faulting, as interpreted by Kershaw & Guo (2006). We repeat that there are no confirmed MIS 7a/c dates on the terrace attributed to that age by Leeder et al. (2005).


    Mounds, faults and caves.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
Kershaw & Guo (2006) interpreted caves to have formed where faults cut mounds. However, Andrews et al. stated: ‘nowhere have we seen an unequivocal fault plane cutting bioherm framework and being draped by later bioherm growth’. First, we did not say that later bioherm growth draped cut surfaces of mounds; in fact, in general terms, we interpreted the caves to have formed after the mound growth phase was completed (Kershaw & Guo 2006, pp. 61–62). Second, we agree that it would be hard to demonstrate a fault cutting a mound at all sites, because the caves indicate erosion of the rocks. Nevertheless, we argue that caves exposed in cut mounds on the western end of the +25 m terrace in Figure 3 are due to fault-breaks, and coincide with the minor fault mapped by Leeder et al. (2005, fig. 6a). In other places, perhaps mounds broke open as a result of gravitational stresses created by unevenness in the substrate caused by faulting (perhaps even earthquake shock), not requiring exact coincidence of mounds and faults.

Andrews et al. also noted that ‘there is no evidence that these caves were anything other than... growth cavities between bioherm framework‘. We have not observed any cavities that can be confidently interpreted as growth cavities, but many mounds have large central hollows. In our opinion these are secondary, and curved roofs following the growth banding would be expected if roof-collapse followed weakness lines defined by banding (see photographs in the paper by Kershaw & Guo 2006).

If Rivularia mounds grew on a single level, then it is possible that some faults became active before completion of the mound phase. The large rounded boulder of Rivularia conglomerate shown by Andrews et al. (Fig. 2, arrow A) may have rolled down from the upfaulted part of the mound field and then been used as a substrate by the later part of mound growth, at least partly consistent with one interpretation by Portman et al. (2005, p. 458). The other boulder (Fig. 2, arrow B) is a later addition derived either from cave fill (of a mound that has since completely collapsed), or could also have rolled down (it is difficult to be sure for an inaccessible item high on a cliff). Hence there is no need to invoke two separate mound levels.


    Other structures.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
Kershaw & Guo (2006) noted an even higher (and therefore possibly older) mound remnant at c. +55 m at the tip of the peninsula, on the western end of the hilltop east of Heraion lighthouse (Fig. 4). This mound contains pendent corallines in cavities. If the hilltop was uplifted relative to adjacent land, then this mound could be the same age as lower mounds. However, otherwise, if a steady uplift rate of 0.23 mm a–1 is applied, ending at +55 m (the uppermost of the four lines in Fig. 5), this site would have been above sea level during MIS 5e but perhaps within reach of MIS 7 (see Leeder et al. 2005, fig. 6a inset) or MIS 9, if the mound grew in marine conditions. Work so far shows this mound is dominated by corallines, with Rivularia as only a minor component; it therefore differs from the ‘MIS 5e’ and ‘7a/c’ mounds. Thus the complexity of the facies system at Heraion did not produce uniform mounds. Although Andrews et al. comment that mound growth and associated facies seem to have been ‘repeated a number of times’, currently there is potential evidence for MIS 5e, 7 or 9 only if the mounds are marine and all of different ages. In that case, Rivularia calcification theoretically could also have occurred in freshwater during MIS 6, and would now be at least 10 m below modern sea-level (with a 0.3 mm a–1 uplift rate), encrusting the steep cliff of the coastal-bounding faults. As far as we know, there has been no exploration of this possibility. If mounds grew in the sea, we would also expect Holocene mounds during the known mid-Holocene pluvial phases that affected the Mediterranean region, as mentioned by Kershaw et al. (2005) and Kershaw & Guo (2006). They would now be uplifted above sea level, but none have been recognized. Did they fail to form because of insufficient groundwater expelled up the faults during the Holocene, or because they needed a lake to grow?

Terraces with marine deposits are well known to have formed in response to the c. 100 ka Milankovitch eccentricity cycle that drove eustatic sea-level changes throughout the Quaternary. Figure 5 shows that the MIS 5e terrace was flooded by the sea during only the peak portion of the curve. The other two Milankovitch cyclicities, which forced smaller-scale sea-level changes (obliquity, 41 ka; precession, 19–23 ka) are both too long-ranging to account for water-level changes leading to the complex deposits in this peak part of the curve. Therefore sub-Milankovitch-scale sea-level changes may be interpreted if the sequence was completed before the MIS 5e highstand. However, if the mounds grew in a lake during MIS 6, then the problem of time constraints is removed; but if two levels of mounds exist (which would therefore need two lakes at different times), then earlier mounds in an MIS 8 lake can be accommodated in Figure 5, but depend on the uplift rates in the Isthmus of Corinth and Perachora Peninsula in earlier times (not constructed in Fig. 5).


    History and alteration of mound fabric.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
We agree that less than half of the mound frame is constructed by recognizable R. haematites (see Portman et al. 2005, p. 445), and that some of the material we had previously identified as strongly altered R. haematites is instead clotted micritic (?microbial) fabric. All the samples of R. haematites we studied had some alteration, which is gradational, so that strongly altered portions resemble the clotted micrite. Certainly we agree that the encrusting L. pustulatum would need light to grow, and had envisaged a more open frame of R. haematites for encrustation by L. pustulatum. It remains a curious fact that R. haematites is encrusted by L. pustulatum and never the other way around. This arrangement supposes that mounds were built layer by layer during short pulses of groundwater expulsion to calcify the R. haematites, then a brief respite to allow L. pustulatum encrustation, followed by restarting of R. haematites growth during the next groundwater pulse. Layer boundaries within mounds should have R. haematites encrusting L. pustulatum, but as far as we are aware that has not been discovered. Nevertheless, growth of L. pustulatum in the MIS 6 lake is not precluded by the penecontemporaneous growth of Rivularia and L. pustulatum; the latter can grow in very low salinities of the northern Caspian Sea (see Kershaw & Guo 2003), and it is possible that the MIS 6 lake did not become completely fresh. Therefore, in our opinion, the growth of Rivularia in a lacustrine setting is not precluded by its intimate relationship with L. pustulatum.

Micrite and encrusting coralline alga L. pustulatum are apparently not altered, in contrast to Rivularia, reinforcing the interpretation of Kershaw & Guo (2003) that alteration was early. Andrews et al. strongly reject any later recrystallization of the fabric. However, we wish we could share their conviction that a carbonate system, composed of a diverse and intricate assemblage of calcified organic and inorganic elements, subjected to an unusual geochemical environment, would be unquestionable for secure geochemical investigation. We emphasize that the Perachora mounds have two unique components: giant Rivularia mounds, and pendent coralline algae composed of a single (euryhaline) species. Also, strontium isotope ratios in the Gulf of Corinth are lower than those of normal seawater in the Late Quaternary (Dia et al. 1997; see McArthur et al. 2001). Dia et al. (1997) suggested that one reason for low Sr ratios is incomplete connection between the Gulf of Corinth and the open ocean during the last few highstands. However, they preferred a model of diagenetic alteration, and emphasized apparent alteration of visibly and mineralogically pristine coral aragonite. Overall, any arguments about diagenesis involving strontium isotopes are suspect and cannot be safely applied to these sediments.


    Referencing of abstracts.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
Andrews et al. noted that one University of East Anglia (UEA) abstract was work in progress, and did not reflect their later views. Although Portman et al. (2005) currently do not consider the mounds to have been influenced by mid-5e fall, if supporting evidence later emerges then their earlier abstract will justly credit the UEA group as the first to recognize it.


    Conclusion.
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
Independent work by both the UEA and Brunel groups has revealed different aspects of the Heraion mounds. Consideration of published coral dates interpreting the behaviour of the Rion Sill and Isthmus of Corinth removes the need for a variable uplift rate model and does not preclude a lacustrine setting for the mounds. We repeat that the mound outcrops lie in the confluence of several fault strands (see maps in the various papers referenced herein, and Figs 3 and 4 of this Discussion). The status of these faults is uncertain (see Leeder et al. 2005), and we have also shown above that there seem to be differences of opinion about the relative importance of some faults. Thus, much depends on the faults behaving in a predictable manner, and on whether two levels of mounds exist or not. The Perachora mounds may well contain more surprises than the pendent coralline algae we discovered. Therefore, until proved otherwise, we see no reason to abandon our published view that the non-marine interpretation is more likely, with only one layer of mounds, plus a possible older mound level represented by a single remnant near Heraion lighthouse.


    Acknowledgements
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 
We thank G. Roberts for discussion of aspects of the Perachora mounds.

29 March 2007


    References
 TOP
 Introduction
 Behaviour of barriers.
 Mound levels, faults and...
 Coincidences.
 Mounds, faults and caves.
 Other structures.
 History and alteration of...
 Referencing of abstracts.
 Conclusion.
 Acknowledgements
 References
 

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