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Title: Siliceous sponge spicule dissolution: in field experimental
evidences from temperate and tropical waters
Article Type: Research Paper
Keywords: Siliceous spicules, spicule dissolution, marine sponges,
seawater temperature
Corresponding Author: Prof. Giorgio Bavestrello,
Corresponding Author's Institution: University of Genova
First Author: Marco Bertolino
Order of Authors: Marco Bertolino; Riccardo Cattaneo-Vietti; Maurizio
Pansini; Chiara Santini; Giorgio Bavestrello
Published in Estuarine, Coastal and Shelf Science
(2017) Vol. 184, pp 46-53
DOI: 10.1016/j.ecss.2016.10.044
Abstract: Sponge siliceous spicules are considered a sink in the silica
balance of the oceans as their dissolution rate seems to be negligible,
but no field data are available about this process. Aim of this study
was a first evaluation of the quantitative dissolution rates of some
demosponge and hexactinellid spicules (collected in different
localities at different latitudes), left at sea for six months in two
localities characterised by different water average temperatures:
Mediterranean Sea and Celebes Sea.
The effects of silica dissolution on the experimented spicules, studied
by SEM analysis, resulted in an enlargement of the axial canal
sometimes resulting in empty spicules. While in demosponges the axial
canal wall of eroded spicules was perfectly smooth or slightly rough,
the hexactinellid Rossella racovitzae showed a cavernous, well
recognizable pattern of dissolution.
The dissolution rates were determined evaluating the decrease in outer
diameter and in the expansion of the axial channel of about 300
spicules for each considered species and locality. The spicules from
the Mediterranean Geodia cydonium did not show any detectable
dissolution in both sites, while those from Tethya citrina showed a
loose of silica of about 23% in the Mediterranean and 47% in the
Celebes Sea. Paratetilla bacca from the Red Sea decreased the silica
content of about 30% in both the localities. Tetilla leptoderma from
Mar del Plata lost about 8% and 42% of silica respectively in
Mediterranean and Celebes Sea. Finally, the hexactinellid spicules from
the Antarctic Rossella racovitzae showed highest dissolution rates in
both the experimented sites (37% and 66% in the Mediterranean and
Celebes Sea, respectively).
The different levels of dissolution can be related to the different
taxonomic position as well as to the temperatures at which the spicules
have been deposed and exposed. In fact, spicules from the same species
showed a dissolution rate generally higher in tropical waters than in
Mediterranean.
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Siliceous sponge spicule dissolution: in field experimental evidences from temperate and tropical
waters
Marco Bertolino1, Riccardo Cattaneo-Vietti2, Maurizio Pansini1, Chiara Santini1, Giorgio Bavestrello1
1
Dipartimento di Scienze della Terra, dell’Ambiente e della Vita, Università di Genova, Corso Europa
26, 16132 Genova
2
Dipartimento di Scienze della Vita e dell’Ambiente, Università Politecnica delle Marche, Via Brecce
Bianche 60131 Ancona
Key word: Siliceous spicules, spicule dissolution, marine sponges, seawater temperature.
Abstract
Sponge siliceous spicules are considered a sink in the silica balance of the oceans as their dissolution
rate seems to be negligible, but no field data are available about this process. Aim of this study was a
first evaluation of the quantitative dissolution rates of some demosponge and hexactinellid spicules
(collected in different localities at different latitudes), left at sea for six months in two localities
characterised by different water average temperatures: Mediterranean Sea and Celebes Sea.
The effects of silica dissolution on the experimented spicules, studied by SEM analysis, resulted in an
enlargement of the axial canal sometimes resulting in empty spicules. While in demosponges the axial
canal wall of eroded spicules was perfectly smooth or slightly rough, the hexactinellid Rossella
racovitzae showed a cavernous, well recognizable pattern of dissolution.
The dissolution rates were determined evaluating the decrease in outer diameter and in the expansion of
the axial channel of about 300 spicules for each considered species and locality. The spicules from the
Mediterranean Geodia cydonium did not show any detectable dissolution in both sites, while those
from Tethya citrina showed a loose of silica of about 23% in the Mediterranean and 47% in the Celebes
Sea. Paratetilla bacca from the Red Sea decreased the silica content of about 30% in both the
localities. Tetilla leptoderma from Mar del Plata lost about 8% and 42% of silica respectively in
Mediterranean and Celebes Sea. Finally, the hexactinellid spicules from the Antarctic Rossella
racovitzae showed highest dissolution rates in both the experimented sites (37% and 66% in the
Mediterranean and Celebes Sea, respectively).
The different levels of dissolution can be related to the different taxonomic position as well as to the
temperatures at which the spicules have been deposed and exposed. In fact, spicules from the same
species showed a dissolution rate generally higher in tropical waters than in Mediterranean.
Introduction
Siliceous sponge spicules are among the most fascinating skeletal features of marine invertebrates. In
the last three decades, an impressive amount of work was dedicated to the elucidation of spicule
structure and mechanism of silica deposition, also with applicative purposes (e.g. Müller et al., 2006,
2007a, 2007b). Biogenic silica (bSi) precipitated by sponges (but also by diatoms, radiolarian and
silicoflagellates) is in the form of opal-A which is highly disordered and almost completely amorphous
(DeMaster, 2003).
In spite of the wide interest in spicule formation, very few data are available about the role of siliceous
sponges in the silica balance of the oceans (Maldonado et al., 2005, 2010). When sponges decay, their
spicules become free in the environment and a certain proportion of bSi is sunk for a relevant span of
time, because dissolution rate is considered low (Maldonado et al., 2005; Gutt et al., 2013).
The first attempt to study these siliceous structures lost in the sediments was due to Rützler and
McIntyre (1978), who evaluated the amount of spicules present in the coralline sand from Carrie Bow
Key (Belize). Those spicules showed, on their surface, a typical pitting pattern of dissolution that was
artificially replicated in laboratory by treating spicules coming from living specimens with hydrofluoric
acid 1 N. This peculiar kind of spicule erosion pattern was already been described from Jamaica and
tentatively attributed to some biological agents (Land, 1976).
More recently, sponge spicules have been shown to be a component, although with variable amounts,
of the sediments of some coastal areas all around the world (Inoue, 1985; Bavestrello et al., 1996;
Andri et al., 2001; Bertolino et al., 2012; Chu et al., 2011). Moreover, also the sediments entrapped
inside the Mediterranean coralligenous concretions, with an estimated age of thousands of years,
include several spicules. Although these structures are sometimes deeply etched and damaged, they are
still recognisable and, in several cases, allowed the identification of the original old sponge assemblage
(Bertolino et al., 2014).
On the other hand, Maldonado et al. (2005) demonstrated in lab that free spicules re-dissolve into
silicic acid at far slower rates than those recorded for diatom frustules, thus determining a bSi sink.
This phenomenon is particularly intense in some geographic areas, mainly polar waters (CattaneoVietti et al., 2000; Van Wagoner et al., 1989) where spicules can produce impressive mats as thick as
1.5 m (Koltun, 1968; Gutt, 2007) but no quantitative data are until now available about their dissolution
rates.
The aim of this research is to evaluate, by means of SEM and morphometric analysis, the fate of free
spicules deriving from different sponge species coming from different latitudes, left for six month at
sea both in temperate and tropical localities.
Materials and Methods
The spicular material used in the field experiments came from different species (Geodia cydonium
(Jameson, 1811), Tethya citrina Sarà & Melone, 1965, Paratetilla bacca (Selenka, 1867), Tetilla
leptoderma Sollas, 1886, and Rossella racovitzae Topsent, 1901) collected around the world (Tab. 1).
Spicules were obtained from dry specimens by dissolving their tissues in boiling nitric acid. The
spicules were further cleaned by rinsing several times in distilled water and then dried at 50 °C.
Small packs, containing 1 g of spicules from each sponge specimen, were prepared using plankton nets
(50 m mesh). Two sets of packs (each one in triplicate) were then left for six months in superficial
sediments of two localities characterised by different water average temperatures: a detritic bottom of
the north-Mediterranean (Paraggi Bay, 15 m depth) (from June to December 2013) and a coralline
sandy bottom of Celebes Sea (Banka Is. North Sulawesi, Indonesia, 10 m depth) (from July 2014 to
January 2015). The average water temperatures at the sites of the field tests were 18.4 °C and 28.2 °C,
respectively for the north-Mediterranean and the Celebes Sea. The packs were fixed to plastic pegs and
covered by about 1 cm of sediments.
After the permanence at sea, the content of each pack was dried and weighted.
To describe possible changes in the spicular morphological features due to the putative dissolutive
processes, SEM and light microscopy preparations were made before and after the permanence at sea.
For the morphometric analysis, three microscopy slides were prepared for each spicule pack, before
and after the field tests. For each slide, the external and axial canal diameters of 100 spicules were
measured. From these data the average surface of the annular spicule section was calculated as
difference between the surface referred to the spicular diameter and the surface of the axial canal (Fig.
1).
A gross estimation of the total dissolution was obtained, for each species and locality, by calculating
the percent variation of the spicular average section vs the section of the untreated spicules.
Statistical analyses were carried out to test for significance of differences in the average spicular and
axial channel diameters as well as the annular surface of the spicule section among the three considered
conditions (NT=No Treatment, M=Treatment in the Mediterranean Sea, I=Treatment in Celebes Sea)
for each of the 5 species separately. As the normal distribution of data after a square roottransformation was verified by the Shapiro-Wilk’s test, a one-way analysis of variance (ANOVA) was
performed followed by a Tukey's pairwise comparison. Analyses were performed using PAST for
Windows version 1.91 (Hammer et al., 2001).
Results
SEM analysis has shown evident morphological changes between untreated and treated spicules,
mainly due to the enlargement of their axial canal. While the external surface remained smooth in all
tested spicules in both experimental sites, without any evident mark of etching, the inner canal showed
different levels and patterns of dissolution (Figs. 2, 3).
In Geodia cydonium, the axial canal of treated trienes maintained the original triangular shape, with a
slight enlargement in comparison to untreated spicules (Fig. 2A-C). No morphological differences were
recognisable between spicules tested in the two localities. In the strogyloxeas of Tethya citrina (Fig.
2D), a huge enlargement of the canal (Fig. 2E, F) occurred in both sites after six months of permanence
at sea and the canal wall showed a rough surface (Fig. 2F). Similar results occurred for Paratetilla
bacca (Fig. 2G-I) and Tetilla leptoderma (Fig. J-M) although in these two species the canal wall
remained perfectly smooth (Fig. 2I, M).
In the spicules of the hexactinellid Rossella racovitzae (Fig. 3A), the small square axial canal (Fig. 3B)
showed a huge enlargement (Fig. 3 C-D), sometimes resulting in the formation of “empty” spicules
(Fig. 3E). The wall of the canal was heavy etched, with a characteristic cavernous pattern of dissolution
(Fig. 3F).
To evaluate the silica dissolution, the weight loss of the total amount of the tested spicules resulted
unsuitable due to high loss of spicules through the plankton net probably under the effect of the water
movement. However, the morphometric analysis of the average spicule thickness, of the axial canal
diameter and of the estimated annular spicule section, indicated different intensity of dissolution
according to the different seawater temperatures to which they were tested (Fig. 4).
The spicules of the atlanto-mediterranean demosponge G. cydonium, after six months of permanence at
sea in both sites, were not subjected to reduction of the spicular thickness (Fig. 4A; Tabs. 2, 3), while
the diameter of the axial canal showed an increasing with significant differences in the two tested
temperatures (Fig. 4B; Tabs. 2, 3). The calculated transversal surface of the spicules was not subjected
to significant variations after the permanence in both sites (Fig. 4C; Tabs. 2, 3) resulting in a slight
percent of silica dissolution (3.9 and 7.5%, respectively in the Mediterranean and Celebes sites) (Fig.
4D).
The strongyloxeas of the Mediterranean demosponge T. citrina, showed a significantly decreasing of
their thickness in the spicules tested in Mediterranean and Celebes Sea (Fig. 4A; Tabs 2, 3) as well as a
significant increasing of axial canal diameter between treated and untreated spicules (Fig. 4B; Tabs. 2,
3). The spicular annular section showed a progressive reduction from spicules untreated, treated in
Mediterranean and in Celebes Sea (Fig. 4C; Tabs 2, 3) resulting in an estimated silica lost of about 23%
in the Mediterranean and 47% in the Celebes Sea (Fig. 4D).
The variation of all recorded spicular parameters in P. bacca from Dalahk Is (Red Sea) were significant
in untreated vs treated spicules, while no significant differences were recorded between spicules tested
in Mediterranean and Celebes Sea. From these data, it was possible to estimate a silica dissolution of
about 30% (Fig. 4; Tabs. 2, 3).
In T. leptoderma from Mar del Plata, the main recorded differences were observed after the treatment
in the tropical waters, producing a silica dissolution of about 40% while no differences were recorded
between untreated material and spicules experimented in the Mediterranean Sea (Fig. 4; Tabs. 2, 3).
Finally the spicules from the Antarctic hexactinellid R. racovitzae showed highest dissolution rates in
both the experimented sites (37 and 66% in the Mediterranean and Celebes Sea, respectively) due to
significant reductions of the external diameter and significant increasing of the axial canals (Fig. 4;
Tabs. 2, 3).
Discussion
Forty years ago Rützler & McIntyre (1978), in their seminal paper about the presence of sponge
spicules in Caribbean sediments, quantified the amount of siliceous spicules and described, through
SEM imagining, their peculiar pattern of dissolution in natural conditions. Although numerous other
papers have identified spicules in sediments of several marine or fresh-water basins (Inoue, 1985;
Bavestrello et al., 1996; Andri et al., 2001; Bertolino et al., 2012; Chu et al., 2011), no field data are
until now available about their natural dissolution rates and about the environmental factors affecting
this process. The amount of silica up-taken by sponges is not negligible in the global silica balance and
therefore a clarification of its turnover is necessary for a correct estimation of the bSi balance of the
ocean (Kamatani, 1971).
Sponge spicules are more resistant to dissolution, particularly in comparison with diatoms (Maldonado
et al., 2005; Kamatani, 1971): Maldonado et al. (2005), in fact, found no detectable dissolution of
demosponge spicules and a 5% of dissolution in hexactinellid spicules after 8 months of lab
experiments at room temperature, in contrast to a severe dissolution of the diatom frustules. On this
base, several authors considered the silica uptake of the sponges as a sink of available silica from the
marine system (Maldonado et al., 2005, 2010; Chu, 2011).
Here we demonstrate, through field experiments that, although with differences among different
species, the dissolution rate of spicules lost in the sediments is not negligible. Among the tested
spicules, only those of G. cydonium, in fact, showed a slight dissolution rate, while all other spicules
lost, in 6 months, from 8 to 37% of their volume in temperate waters, and from 34 to 66% in tropical
ones. In particular, in the tested conditions, the spicules of the hexactinellid Rosella racovitzae,
dissolve at a rate significantly faster that of all the tested demosponges.
The recorded total dissolved silica resulted both from a reduction of the external diameter and an
enlargement of the axial canal. While the erosion of the external surface was always homogeneous,
without any marks of etching in all tested spicules, the enlargement of the axial canal resulted in
different types of dissolution process with different microtextures, according to the examined species.
The phenomenon is particularly evident in the hexactinellid R. racovitzae, in which the wall of the axial
canal showed a cavernous etching pattern. On the contrary, in the demosponge spicules, the axial canal
is slightly etched in Tethya or completely smooth in Paratetilla and Tetilla. These differences could be
related to the complex, not homogeneous silica deposition around the axial filament (Mueller et al.,
2007b; 2009).
From a compositional point of view, it is already stated that the spicules of demosponges and
hexactinellids are very similar (Standford, 2003): both are composed almost completely by silica,
deposed around a central axial filament which harbours the silicatein. Nevertheless, the recorded
differences in IR spectra between the spicules of the two classes (Standford, 2003) were considered
related to different molecular configurations, involving Si-O-Si or other linkages, that may result in
different dissolution patterns. This structural difference could result in the higher dissolution rates of
the hexactinellid R. racovitzae in comparison with the demosponges, at both tested temperatures.
It was already stated that the solubility of bSi is highly temperature dependent (Lawson et al., 1978;
Kamatani, 1982) and this laboratory evidence was supported by ecological observations: spicules from
living specimens of Tethya, collected in a marine cave from Oman (Persian Gulf) characterised by very
warm waters, showed deep marks of dissolution already inside the living sponges (Bavestrello et al.,
1996)). The significant differences recorded in the two tested localities confirmed the role of the water
temperature on the silica dissolution: spicules from the same species showed in Mediterranean the
maximal dissolution rate which was about the minimum in tropical waters.
These results indicate that the sponge spicules, and in particular those from hexactinellids, can play a
significant role in the sinking process of silica only in cold waters, supporting the geographic
differences of the presence of spicules in sediments (Kamatani, 1971; Kratz et al., 1991; Conley and
Schelske, 1993). For example, in the Antarctic Ocean, where the cold waters prevent the silica
dissolution, sponge spicules can form thick mats (Koltun, 1968; Gutt et al., 2013; Bonci et al., 1989;
Barthel, 1992), while at Tropics, with comparable sponge biomasses, spicule mats were never recorded.
The evidence that the spicules of several Mediterranean species are completely dissolved in a couple of
years is not in agreement with the finding of recognisable spicules, although partially etched, in
sediment buried in the Posidonia oceanica mat with an estimated age of tens of years (Bertolino et al.,
2012) or in sediments included in the growing coralligenous conglomerate, datable thousands of years
(Bertolino et al., 2014). Probably, the peculiar features of these habitats, characterised by high
concentration of organic matter, anoxic conditions and low pH values, were able to preserve bSi from
the dissolution process.
Although other researches will be necessary at this subject, our results seem to suggest that the
dissolution rate can be related to the temperature at which the spicule was formed. It is already known
that the sponge spicule size varies along a latitudinal gradient, suggesting an inverse relationship with
water temperature and silica deposition (Topsent, 1917; Hentschel, 1929; Hartman, 1958; Simpson,
1978; Hooper, 1991) and this trend was attributed to a more efficient entrapment of silicon rather than
to effects upon silicon transport (Simpson, 1978). In our experiment, the spicules of two related
demosponges, P. bacca and T. leptoderma, respectively secreted in warm and cold waters, showed
different patterns of dissolution. Those from the warm waters of the southern Red Sea dissolved at the
Mediterranean temperature, while those secreted in the cold south Atlantic waters, significantly
dissolved only in the tropical condition, suggesting a more compact and resistant structure in spicules
coming from cold waters.
However, also the role of the silica concentration in the waters cannot be ignored to determine different
structures of the silica secreted, considering that, both at global (Treguer et al., 1995) and local level,
according to the seasonal cycles (Stone, 1970), the silica concentration in the seawater is inversely
correlated with the temperature, a condition which could play a major role in determining the
morphological and structural characteristics of the spicule.
Acknowledgments
We would like to thank Dr. Marzia Bo for the helpful suggestions. This study was financially supported
by COFIN-PRIN and SIR projects (Italian Ministry of Research, MIUR).
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Figure legends
Figure 1 – The spicule dissolution was evaluated by measuring the annular surface of the spicule
section before (A, B) and after (C, D) a six month of permanence in the field. a-b, external diametr; a’b’, diameter of the axial canal.
Figure 2 – A-C, Geodia cydonium. A-B, Trienes showing the axial canal of normal size before the
treatment and (C) slightly enlarged after the permanence at sea. D-F, Tethya citrina. D, Untreated
fractured strogyloxea showing the small axial canal). E-F, Enlarged axial canals after the field test.
While the external surface remains smooth (E), the wall of the axial canal shows a rough pattern of
dissolution (F). G-I Paratetilla bacca. G, Untreated triaene; H, enlargement of the axial canal after the
treatment (H); I, the perfectly smooth wall of the axial canal. J-M, Tetilla leptoderma, J, untreated
triaene, L-M, different stages of the enlargement of the axial canal after the permanence at the sea.
Figure 3 – Rossella racovitzae. A, untreated spicules; B, section of an untreated spicule showing the
normal size of the axial canal. C-D, spicules of the mat with an enlarged axial canal after the
permanence in the sea. E-F, spicules with the enlarged canal wall characterised by a cavernous etching
pattern.
Figure 4 – Average external diameter (A); average diameter of the axial canal (B), average annular
surface of the spicule section (C) of 300 spicules per species and per site. Black bars, untreated
spicules; grey bars, spicules left for six month in the Mediterranean; white bars, spicules left for six
month in the Celebes Sea. D, estimated percent dissolution of the spicules tested in Mediterranean
(grey bars) and Celebes Sea (white bars) vs untreated spicules.
Table(s)
Click here to download Table(s): Bertolino et al., Table 1.docx
Tab. 1 – Tested species, localities of collection with depth and temperature range of the localities of
collection; spicule types
Class
Species
Demospongiae Geodia
cydonium
Locality
North
Depth
SWT
(m)
(°C)
Adriatic 20
7 - 25
Sea
Spicule type
Oxeas
Orto-Anatriaenes
(Mediterranean)
Demospongiae Tethya
citrina
North
Adriatic 30
7 - 25
Strongyloxea
Sea
(Mediterranean)
Demospongiae Paratetilla
bacca
Dalhak Is. (Red 6
26 - 32
Sea)
Oxeas
Anatriaenes
Protriaenes
Demospongiae Tetilla
leptoderma
Mar del Plata 360
8
(SW Atlantic)
Oxeas
Anatriaenes
Protriaenes
Hexactinellida
Rossella
Ross
racovitzae
(Antarctica)
Sea 200
-1.5
Oxeas
Table(s)
Click here to download Table(s): Bertolino et al., Table 2.docx
Tab. 2 – Average values (± SE) of external spicule diameter, axial canal diameter and surface of the
annulus of the spicule section after and before six months of permanence at sea in temperate and
tropical localities.
Species
Geodia cydonium
Tethya citrina
Paratetilla bacca
Tetilla leptoderma
Rossella racovitzae
Treatment
untreated
External
diameter
(μm)
24,59 ± 0,70
Axial canal
diameter
(μm)
1,21 ± 0,03
Annular section
surface
2
(μm )
589,98 ± 30,52
6 months Medit
24,12 ± 0,71
1,41 ± 0,03
566,86
± 30,51
6 month Celebes 23,52 ± 0,76
1,71 ± 0,05
545,33
± 33,53
untreated
21,54 ± 0,38
3,17 ± 0,09
381,97
± 13,12
6 months Medit
19,03 ± 0,28
3,84 ± 0,09
293,81
± 9,18
6 month Celebes 15,91 ± 0,23
4,14 ± 0,08
201,01
± 6,34
untreated
35,25 ± 0,67
3,67 ± 0,15
1046,45 ± 36,48
6 months Medit
30,05 ± 0,51
5,98 ± 0,20
743,13
± 24,88
6 month Celebes 29,16 ± 0,41
5,58 ± 0,16
694,43
± 18,49
untreated
20,97 ± 0,84
1,09 ± 0,04
479,21
± 42,92
6 months Medit
19,70 ± 0,63
1,38 ± 0,05
459,46
± 29,24
6 month Celebes 16,20 ± 0,46
1,33 ± 0,05
278,47
± 19,66
untreated
12,72 ± 0,36
0,99 ± 0,04
151,34
± 10,07
6 months Medit
10,40 ± 0,22
1,63 ± 0,05
95,54
± 5,03
2,14 ± 0,05
51,77
± 2,25
6 month Celebes 7,97
± 0,13
Table(s)
Click here to download Table(s): Bertolino et al., Table 3.docx
Tab 3 - Results of the one-way ANOVA tests.
Effect of treatment on the spicule external diameter for each species (Fig. 4A). NT=Untreated, M=Mediterranean Sea, I=Celebes Sea
Comparison
Geodia cydonium
Between groups
Within groups
Total
Tethya citrina
Between groups
Within groups
Total
Paratetilla bacca
Between groups
Within groups
Total
Tetilla leptoderma
Between groups
Within groups
Total
Rossella racovitzae
Between groups
Within groups
Total
df
F
p
2
865
867
0.6455
p=ns
(NT=M=I)
2
1025
1027
89.66
p<0.001
(NT>M>I)
2
974
976
28.7
p<0.001
(NT>M=I)
2
1033
1035
16.81
p<0.001
(NT=M>I)
2
1035
1037
120.4
p<0.001
(NT>M>I)
Effect of treatment on the spicule axial canal diameter for each species (Fig. 4B). NT= Untreated, M=Mediterranean Sea, I= Celebes Sea
Comparison
Geodia cydonium
Between groups
Within groups
Total
Tethya citrina
Between groups
Within groups
Total
Paratetilla bacca
Between groups
Within groups
Total
Tetilla leptoderma
Between groups
Within groups
Total
Rossella racovitzae
Between groups
Within groups
Total
df
F
p
2
865
867
51.72
p<0.001
(NT<M<I)
2
1025
1027
29.07
p<0.001
(NT<M=I)
2
974
976
38.37
p<0.001
(NT<M=I)
2
1033
1035
5.631
p<0.01
(NT<M=I)
2
1035
1037
88.51
p<0.001
(NT<M<I)
Effect of treatment on the spicule annular section surface for each species (Fig. 4C). NT= Untreated, M=Mediterranean Sea, I= Celebes Sea
Comparison
Geodia cydonium
Between groups
Within groups
Total
Tethya citrina
Between groups
Within groups
Total
Paratetilla bacca
Between groups
Within groups
Total
Tetilla leptoderma
Between groups
Within groups
Total
Rossella racovitzae
Between groups
Within groups
Total
df
F
p
2
865
867
0.7229
p=ns
(NT=M=I)
2
1025
1027
99.84
p<0.001
(NT>M>I)
2
974
976
38.57
p<0.001
(NT>M=I)
2
1033
1035
15.59
p<0.001
(NT=M>I)
2
1035
1037
124
p<0.001
(NT>M>I)
Figure(s)
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Figure(s)
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Figure(s)
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Figure(s)
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