<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">IJG</journal-id><journal-title-group><journal-title>International Journal of Geosciences</journal-title></journal-title-group><issn pub-type="epub">2156-8359</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ijg.2014.58071</article-id><article-id pub-id-type="publisher-id">IJG-48340</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>EARTH &amp; ENVIRONMENTAL SCIENCES</subject></subj-group></article-categories><title-group><article-title>Late Pleistocene Climatic Changes in Central Brazil Indicated by Freshwater Sponges</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Vanessa</surname><given-names>de Souza Machado</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Cecilia</surname><given-names>Volkmer-Ribeiro</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Roberto</surname><given-names>Iannuzzi</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Museu de Ciências Naturais (MCN), Funda??o Zoobotanica do Rio Grande do Sul (FZB), Porto Alegre, Brasil</addr-line></aff><aff id="aff3"><addr-line>Departamento de Paleontologia e Estratigrafia, Instituto de Geociências, UFRGS, Porto Alegre, Brasil</addr-line></aff><aff id="aff1"><addr-line>Programa de Pós-gradua??o em Geociências, Instituto de Geociências, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre, Brasil</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>biologavsm@gmail.com(VDSM)</email>;<email>cvolkmer1427@gmail.com(CV)</email>;<email>roberto.iannuzzi@ufrgs.br(RI)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>24</day><month>07</month><year>2014</year></pub-date><volume>05</volume><issue>08</issue><fpage>799</fpage><lpage>815</lpage><history><date date-type="received"><day>9</day>	<month>May</month>	<year>2014</year></date><date date-type="rev-recd"><day>5</day>	<month>June</month>	<year>2014</year>	</date><date date-type="accepted"><day>1</day>	<month>July</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
	The Cemitério Palaeolake deposit in Catalao, Goiás State, Brazil, comprises a single, complete lacustrine sequence, dated from less than 27,500 ± 4000 yr B.P. to more than 51,780 ± 400 <sup>14</sup>C yr<sup> </sup>B.P. The unprecedented presence of spongillite and diatomite layers in this deposit was investigated using spicules of continental sponges as proxy data for environmental and climate reconstruction, which was relatively extensive for the ages examined. From the analysis of the sedimentary features and the associations of spicules preserved in the deposit, it was possible to reconstruct the evolution of the limnic system. Five developmental stages were thus identified, corresponding to the installation (lotic and erosion phase), establishment and development of the lake and its colmatation, the latter correlating to the Last Glacial Maximum (LGM). Moreover, based on the ecological requirements of the sponge species identified in the deposit, it was possible to infer the likely weather patterns related to respective phases of the lake. The presence of the sponge species Corvoheteromeyenia australis, presently recorded only from southern South America, indicated that polar incursions originating from the Antarctic were frequent during the last glacial period and might have played a notable role in what is now central Brazil. However, for a short time, drier and hotter weather conditions might have predominated, as suggested by the presence of the species Corvomeyenia thumi. 
</p></abstract><kwd-group><kwd>Spongillites</kwd><kwd> Lacustrine Palaeoenvironment</kwd><kwd> Palaeoclimate</kwd><kwd> Central Brazil</kwd><kwd> Late Pleistocene</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Palaeoenvironmental and palaeoclimatic reconstructions of the Late Pleistocene, particularly in the central region of Brazil, have been proposed based on the analyses of lake sediments containing pollen, spores and microalgal spectra [<xref ref-type="bibr" rid="scirp.48340-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.48340-ref8">8</xref>] . However, several worldwide reports produced on lentic quaternary sediments suggest the use of freshwater sponge spicules as a diagnostic tool in palaeo interpretations [<xref ref-type="bibr" rid="scirp.48340-ref9">9</xref>] -[<xref ref-type="bibr" rid="scirp.48340-ref13">13</xref>] . In this respect, extensive studies have been conducted in South America [<xref ref-type="bibr" rid="scirp.48340-ref14">14</xref>] -[<xref ref-type="bibr" rid="scirp.48340-ref18">18</xref>] .</p><p>Spongillites and diatomites are evidences that natural environmental conditions can maximize the production of aquatic organisms with silicious supporting structures and generate large deposits of biosilicious rocks, formed in the case of the spongillites from sponge spicules [<xref ref-type="bibr" rid="scirp.48340-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref19">19</xref>] , and in that diatomites from diatoms frustules [<xref ref-type="bibr" rid="scirp.48340-ref20">20</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref21">21</xref>] . Studies on these deposits, particularly in freshwater lentic environments, are typically rare, although they have indicated their unique and preferred characteristics in relation to various contexts, including geomorphology [<xref ref-type="bibr" rid="scirp.48340-ref22">22</xref>] -[<xref ref-type="bibr" rid="scirp.48340-ref27">27</xref>] , palaeoenvironment [<xref ref-type="bibr" rid="scirp.48340-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref22">22</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref26">26</xref>] -[<xref ref-type="bibr" rid="scirp.48340-ref28">28</xref>] , palaeoclimate [<xref ref-type="bibr" rid="scirp.48340-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref27">27</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref29">29</xref>] , and, in the case of diatomite, even orbitals [<xref ref-type="bibr" rid="scirp.48340-ref30">30</xref>] . However, to date, deposits of diatomites and spongillites have not been recorded in the same basin.</p><p>The Cemit&#233;rio Palaeolake deposit in Catal&#227;o, Goi&#225;s State, Brazil was dated from less than 27,500 &#177; 4000 yr BP to more than 51,780 &#177; 400 <sup>14</sup>C yr BP [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] . It therefore constitutes the oldest dated deposit in central Brazil, where few such deposits are dated at over 40,000 yr BP [<xref ref-type="bibr" rid="scirp.48340-ref1">1</xref>] -[<xref ref-type="bibr" rid="scirp.48340-ref8">8</xref>] . The study of the Cemit&#233;rio Palaeolake has revealed the occurrence of facies rich in sponge spicules [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] , and fully preserved gemmules [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] produced by the same sponge community related to the spongillite deposits [<xref ref-type="bibr" rid="scirp.48340-ref19">19</xref>] and currently typical of lakes in the Cerrado Biome [<xref ref-type="bibr" rid="scirp.48340-ref33">33</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref34">34</xref>] , Metania spinata (Carter, 1881), Dosilia pydanieli Volkmer-Ribeiro (1992), Heterorotula fistula Volkmer-Ribeiro and Motta (1995), Corvomeyenia thumi (Traxler, 1895), Radiospongilla amazonensis Volkmer-Ribeiro and Maciel (1983) and Trochospongilla variabilis Bonetto and Ezcurra de Drago (1973), but added also Corvoheteromeyenia australis (Bonetto and Ezcurra de Drago, 1966). Machado and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] also detected rare spicules from species more typical of lotic environments in the Cemit&#233;rio Palaeolake, including Corvospongilla seckti Bonetto and Ezcurra Drago (1966), Oncosclera navicella (Carter, 1881) and Eunapius fragilis (Leidy, 1851).</p><p>However, the Cemit&#233;rio Palaeolake is remarkable because of its intercalated facies of spongillites and diatomites. Thus, this paper examines the environment related to the formation of these two bio-siliceous deposits, as well as their relationship with the other facies in the palaeolake, extracting from these analyses palaeoenvironmental and palaeoclimatic interpretations that are unprecedented for the ages obtained.</p></sec><sec id="s2"><title>2. Study Area</title><p>The Cemit&#233;rio Palaeolake outcrop (18˚08'S; 47˚08'W) is constituted by a continuously exposed lacustrine deposit, formed in a depression at the northern part of the Catal&#227;o I Carbonatite Complex (<xref ref-type="fig" rid="fig1">Figure 1</xref>). The sedimentary rocks lie discordantly on the dome of magmatic carbonatite [<xref ref-type="bibr" rid="scirp.48340-ref35">35</xref>] . The outcrop consists of a 27 km<sup>2</sup> sub-cir- cular plateau, with the NS and EW axes measuring 6 and 5.5 km, respectively. The average elevation is 900 m, rising 100 m above the surrounding land.</p><p>The rocks of the Catal&#227;o region are included in the igneous province of the Upper Parana&#237;ba, lying between the Paran&#225; and S&#227;o Francisco basins [<xref ref-type="bibr" rid="scirp.48340-ref36">36</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref37">37</xref>] (<xref ref-type="fig" rid="fig1">Figure 1</xref>). In this same region is an elongated structure extending NW-SE, known as the Upper Parana&#237;ba Arch, in which uplifting began in the early Cretaceous and intensified during the late Cretaceous. This igneous basin was established as a result of intense mafic-ultramafic alkaline and ultrapotassic magmatism generating intrusive (dikes, pipes, diatremes, and plutonic complexes) and extrusive (lava and pyroclastic) bodies. According to Gibson and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref36">36</xref>] , the alkaline rocks in this province include, among others, kamafugites, kimberlite, lamproite, and carbonatite complexes. The carbonatite complexes of the Upper Parana&#237;ba include Catal&#227;o I and II at the northernmost end of the Province in the state of Goi&#225;s and Salitre I and II, Arax&#225;, Tapira, and Serra Negra in the state of Minas Gerais (<xref ref-type="fig" rid="fig1">Figure 1</xref>). Of particular note is the Serra Negra dome, which contains a lake of the same name and a rich current deposit of sponge spicules in the bottom sediments [<xref ref-type="bibr" rid="scirp.48340-ref34">34</xref>] .</p><p>Sand lenses of Layer # 16 from Section 2, upper interval of the Cemit&#233;rio Palaeolake outcrop, have previously been dated using thermo-luminescence (TL) and optically stimulated luminescence (OSL) [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] . The TL resulted in an age of 34,700 &#177; 5000 yr BP, whereas that obtained using OSL was 27,500 &#177; 4000 yr BP. Radiocarbon dating of the basal-most layer (Layer # 5 from Section 1) indicated an age of more than 53,780 years <sup>14</sup>C yr BP for a fragment of fossil wood and 51,780 &#177; 400 <sup>14</sup>C yr BP for a fern frond [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] . In addition to these, in layer subsequent to the base (Layer # 2 from Section 2), radiocarbon dating of an angiosperm leaf obtained an age from 48,333 &#177; 400 years <sup>14</sup>C yr BP [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] (<xref ref-type="fig" rid="fig1">Figure 1</xref> and <xref ref-type="fig" rid="fig2">Figure 2</xref>).</p><fig id="fig1"><label>Figure 1</label><caption><p> Geological map of the Alto Parana&#237;ba Igneous Province, signaling the alkaline-carbonatite plutonic complex of Catal&#227;o I (Catal&#227;o, Goi&#225;s, central Brazil). Adapted from [37] </p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\2621c5d7-84b4-4230-bc42-598d3ad8f0d6.png"/></fig></sec><sec id="s3"><title>3. Materials and Methods</title><p>Samples removed from each of the 21, 19, and 13 layers of Sections 1, 2, and 3, respectively, were deposited and catalogued in the Porifera Collection of Museu de Ci&#234;ncias Naturais da Funda&#231;&#227;o Zoobot&#226;nica do Rio Grande do Sul (MCN/FZB) under numbers MCN-POR nr 8147 to 8200 [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] . Permanent slides were produced and mounted for taxonomic identification of the sponge spicules following as in [<xref ref-type="bibr" rid="scirp.48340-ref38">38</xref>] .</p><p>Fragments of the spongillites and diatomites from the Palaeolake were also mounted on supports and placed in a SEM (Philips Model XL20) at the Centro de Microscopia da Universidade Luterana do Brasil (ULBRA- RS). All the SEM supports containing the studied materials were then included in the respective previously catalogued materials. The presence of abundant sponge gemmoscleres was detected and identified using optical microscopy to examine the permanent slides catalogued in the MCN. The specific identifications were made according to [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] . Drawings of the gemmoscleres were prepared using Camera Clara to illustrate the dif- ferent species identified. These new analyses allowed us to refine the relative quantification proposed by [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] by differentiating the facies formed by spicules from the sponge skeletons from others containing, in addition, the spicules of the gemmules.</p><p>All the layers/sediments obtained from the Cemit&#233;rio Palaeolake sections were classified according to both the particle size and organic matter (OM) content at the Centro de Estudos Costeiros e Oceanogr&#225;ficos da Universidade Federal do Rio Grande do Sul (CECO-UFRGS). To establish particle size, the coarse sediments were separated using a set of 1-mm &#216; sieves [<xref ref-type="bibr" rid="scirp.48340-ref39">39</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref40">40</xref>] ; whereas for fine sediments, the small particle sedimentation method in a liquid medium, according to [<xref ref-type="bibr" rid="scirp.48340-ref41">41</xref>] was used. These results were compared to the descriptions of these same layers performed in situ [<xref ref-type="bibr" rid="scirp.48340-ref42">42</xref>] . This allowed us to pinpoint facies containing clasts and thus propose the precise textural classification of each layer from the Cemit&#233;rio Palaeolake. The combustion-based OM elimination method was used [<xref ref-type="bibr" rid="scirp.48340-ref43">43</xref>] to determine the OM content in the fine sediments (silt and clay). Layer # 14 from Section 1 and Layers # 12 and # 15 from Section 2 had previously been analysed for particle size and OM content [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] .</p></sec><sec id="s4"><title>4. Results</title><sec id="s4_1"><title>4.1. Textural Classification</title><p>The result of the granulometric analysis and the corresponding textural classification of the facies from each of</p><fig id="fig2"><label>Figure 2</label><caption><p> Profile of Section 1 (meters) illustrating from left to right: the results of the textural classification; the percentage of organic matter; the occurrence of the spicules of each sponge species, according to their category and abundance; figures of the gemmoscleres with occurrence in this section. Abbreviations: A, argillite; S, siltstone; Af, fine sandstone; Am, medium sandstone; Ag, coarse sandstone; C, conglomerate/diamictite. Adaptated from [31] [32] </p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\6a1f55bb-2d3b-4764-8390-fc6832eba41f.png"/></fig><p>the three sections taken from the Cemit&#233;rio Palaeolake is shown in <xref ref-type="table" rid="table1">Table 1</xref> and illustrated in the distinct profiles shown in Figures 2-4. The ternary diagram in <xref ref-type="fig" rid="fig5">Figure 5</xref> shows that most of the facies from the palaeolake were formed from a fine matrix in the silt fraction, including those layers presenting clasts (<xref ref-type="table" rid="table1">Table 1</xref>). The latter were classified as diamictites (Layer # 1, 6 and 8 from Section 1; Layers # 1, 5, 7, 11 and 14 from Section 2; Layers # 2, 3, 5/6 and 12/13 from Section 3). Only Layer # 2/3 from Section 1 presented higher percentages of sand, and was thus classified as a sandy conglomerate. Two layers presented higher percentages of clay and were classified as silt-mudstone, Layer # 7 from Section 1 and Layer # 10 from Section 3. In contrast, most of the facies from the palaeolake showed higher percentages of silt and were thus characterized as siltstones (Layers # 4, 9, 11, 12/13, 14, 15, 16 and 17/18 from Section 1; Layers # 2, 3, 4, 6, 8, 9, 10, 12 and 13 from Section 2; Layers # 1 and 11 from Section 3).</p><p>The layers formed predominantly of sponge spicules and others formed by diatom frustules, respectively spongillites and diatomites occurred in three Sections of the Cemit&#233;rio Palaeolake (<xref ref-type="table" rid="table1">Table 1</xref>, Figures 2-4). The spongillites were identified in Layer # 10 from Section 1, Layer # 15 from Section 2, and Layer # 8 (<xref ref-type="fig" rid="fig6">Figure 6</xref>(a), <xref ref-type="fig" rid="fig6">Figure 6</xref>(b)) from Section 3. Whilst the diatomites occurred in Layer # 5 from Section 1, Layer # 16 from</p><table-wrap id="table1"  position="float"><object-id pub-id-type="pii">Table 1</object-id><label>Table 1</label><caption><p>. Results of the sedimentologic analysis of the layers of the Sections 1, 2 and 3 of the Cemit&#233;rio Palaeolake, Catal&#227;o, GO: Organic matter (OM) and Granulometry (Gravel: absent = 0, minerals clasts = 1, organic clasts = 2). The results allowed the proposal of the textural classification for each layer</p></caption><table><thead><tr><th align="center" valign="middle"  rowspan="2"  >Layers</th><th align="center" valign="middle"  rowspan="2"  >OM (%)</th><th align="center" valign="middle"  colspan="4"  >Granulometry</th><th align="center" valign="middle"  rowspan="2"  >Textural classification</th></tr></thead><tbody><tr><td align="center" valign="middle" >Gravel</td><td align="center" valign="middle" >Sandy (%)</td><td align="center" valign="middle" >Silty (%)</td><td align="center" valign="middle" >Clay (%)</td></tr><tr><td align="center" valign="middle"  colspan="7"  >Section 1</td></tr><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >12.40</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >17.15</td><td align="center" valign="middle" >64.05</td><td align="center" valign="middle" >18.80</td><td align="center" valign="middle" >Diamictite of silty matrix</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >21.70</td><td align="center" valign="middle" >1, 2</td><td align="center" valign="middle" >57.41</td><td align="center" valign="middle" >31.83</td><td align="center" valign="middle" >7.30</td><td align="center" valign="middle"  rowspan="2"  >Sandy Conglomerate</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >7.50</td><td align="center" valign="middle" >1, 2</td><td align="center" valign="middle" >34.06</td><td align="center" valign="middle" >25.74</td><td align="center" valign="middle" >25.87</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >44.90</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.24</td><td align="center" valign="middle" >92.00</td><td align="center" valign="middle" >7.97</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >19.10</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.20</td><td align="center" valign="middle" >54.34</td><td align="center" valign="middle" >45.45</td><td align="center" valign="middle" >Diatomite</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >12.50</td><td align="center" valign="middle" >1,2</td><td align="center" valign="middle" >0.21</td><td align="center" valign="middle" >63.00</td><td align="center" valign="middle" >36.79</td><td align="center" valign="middle" >Diamictite of silty-clayey matrix</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >13.70</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >41.00</td><td align="center" valign="middle" >58.78</td><td align="center" valign="middle" >Silty argillite</td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >32.60</td><td align="center" valign="middle" >1, 2</td><td align="center" valign="middle" >21.34</td><td align="center" valign="middle" >65.36</td><td align="center" valign="middle" >13.30</td><td align="center" valign="middle" >Diamictite of silty matrix</td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >23.60</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.11</td><td align="center" valign="middle" >78.61</td><td align="center" valign="middle" >21.28</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >34.20</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.19</td><td align="center" valign="middle" >83.31</td><td align="center" valign="middle" >16.50</td><td align="center" valign="middle" >Spongillite</td></tr><tr><td align="center" valign="middle" >11</td><td align="center" valign="middle" >41.10</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.03</td><td align="center" valign="middle" >88.65</td><td align="center" valign="middle" >11.32</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >12</td><td align="center" valign="middle" >20.20</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.24</td><td align="center" valign="middle" >80.11</td><td align="center" valign="middle" >19.65</td><td align="center" valign="middle"  rowspan="2"  >Siltstone</td></tr><tr><td align="center" valign="middle" >13</td><td align="center" valign="middle" >23.80</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.23</td><td align="center" valign="middle" >80.45</td><td align="center" valign="middle" >19.32</td></tr><tr><td align="center" valign="middle" >14</td><td align="center" valign="middle" >15.30</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.51</td><td align="center" valign="middle" >73.30</td><td align="center" valign="middle" >26.19</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >15</td><td align="center" valign="middle" >29.20</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.73</td><td align="center" valign="middle" >83.79</td><td align="center" valign="middle" >16.14</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >16</td><td align="center" valign="middle" >62.10</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.19</td><td align="center" valign="middle" >85.94</td><td align="center" valign="middle" >13.87</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >17</td><td align="center" valign="middle" >37.00</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.11</td><td align="center" valign="middle" >84.05</td><td align="center" valign="middle" >15.84</td><td align="center" valign="middle"  rowspan="2"  >Siltstone</td></tr><tr><td align="center" valign="middle" >18</td><td align="center" valign="middle" >26.80</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.10</td><td align="center" valign="middle" >70.52</td><td align="center" valign="middle" >29.37</td></tr><tr><td align="center" valign="middle"  colspan="7"  >Section 2</td></tr><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >10.65</td><td align="center" valign="middle" >1</td><td align="center" valign="middle" >15.41</td><td align="center" valign="middle" >61.93</td><td align="center" valign="middle" >22.66</td><td align="center" valign="middle" >Diamictite of silty-clayey matrix</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >32.50</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.28</td><td align="center" valign="middle" >76.15</td><td align="center" valign="middle" >23.57</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >19.90</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.32</td><td align="center" valign="middle" >73.66</td><td align="center" valign="middle" >26.02</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >38.95</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.22</td><td align="center" valign="middle" >86.27</td><td align="center" valign="middle" >13.50</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >41.70</td><td align="center" valign="middle" >1, 2</td><td align="center" valign="middle" >0.85</td><td align="center" valign="middle" >82.28</td><td align="center" valign="middle" >16.87</td><td align="center" valign="middle" >Diamictite of silty matrix</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >37.50</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.19</td><td align="center" valign="middle" >83.32</td><td align="center" valign="middle" >16.49</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >36.60</td><td align="center" valign="middle" >1, 2</td><td align="center" valign="middle" >0.49</td><td align="center" valign="middle" >81.56</td><td align="center" valign="middle" >17.95</td><td align="center" valign="middle" >Diamictite of silty matrix</td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >75.60</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.41</td><td align="center" valign="middle" >90.10</td><td align="center" valign="middle" >9.48</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >28.50</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.41</td><td align="center" valign="middle" >77.73</td><td align="center" valign="middle" >21.85</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >48.80</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.95</td><td align="center" valign="middle" >90.64</td><td align="center" valign="middle" >8.41</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >11</td><td align="center" valign="middle" >34.15</td><td align="center" valign="middle" >1, 2</td><td align="center" valign="middle" >0.25</td><td align="center" valign="middle" >82.21</td><td align="center" valign="middle" >17.54</td><td align="center" valign="middle" >Diamictite of silty matrix</td></tr><tr><td align="center" valign="middle" >12</td><td align="center" valign="middle" >29.70</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.15</td><td align="center" valign="middle" >75.68</td><td align="center" valign="middle" >24.17</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >13</td><td align="center" valign="middle" >56.70</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >1.03</td><td align="center" valign="middle" >87.93</td><td align="center" valign="middle" >11.03</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >14</td><td align="center" valign="middle" >21.30</td><td align="center" valign="middle" >1, 2</td><td align="center" valign="middle" >0.26</td><td align="center" valign="middle" >71.32</td><td align="center" valign="middle" >28.41</td><td align="center" valign="middle" >Diamictite of silty-clayey matrix</td></tr><tr><td align="center" valign="middle" >15</td><td align="center" valign="middle" >34.05</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.90</td><td align="center" valign="middle" >80.34</td><td align="center" valign="middle" >18.76</td><td align="center" valign="middle" >Spongillite</td></tr><tr><td align="center" valign="middle" >16</td><td align="center" valign="middle" >30.55</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.02</td><td align="center" valign="middle" >73.20</td><td align="center" valign="middle" >26.78</td><td align="center" valign="middle" >Diatomite</td></tr><tr><td align="center" valign="middle"  colspan="7"  >Section 3</td></tr><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >28.95</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.36</td><td align="center" valign="middle" >76.46</td><td align="center" valign="middle" >23.18</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >09.65</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >4.01</td><td align="center" valign="middle" >51.39</td><td align="center" valign="middle" >44.60</td><td align="center" valign="middle" >Diamictite of silty-clayey matrix</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >17.05</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >11.01</td><td align="center" valign="middle" >69.51</td><td align="center" valign="middle" >19.48</td><td align="center" valign="middle" >Diamictite of silty-clayey matrix</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >24.25</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.11</td><td align="center" valign="middle" >70.68</td><td align="center" valign="middle" >29.20</td><td align="center" valign="middle" >Diatomite</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >11.25</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >9.95</td><td align="center" valign="middle" >68.44</td><td align="center" valign="middle" >21.61</td><td align="center" valign="middle"  rowspan="2"  >Diamictite of silty-clayey matrix</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >13.35</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >5.82</td><td align="center" valign="middle" >68.99</td><td align="center" valign="middle" >25.18</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >23.40</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.16</td><td align="center" valign="middle" >68.97</td><td align="center" valign="middle" >30.87</td><td align="center" valign="middle" >Diatomite</td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >33.25</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.02</td><td align="center" valign="middle" >82.88</td><td align="center" valign="middle" >17.10</td><td align="center" valign="middle" >Spongillite</td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >28.05</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.29</td><td align="center" valign="middle" >62.69</td><td align="center" valign="middle" >37.02</td><td align="center" valign="middle" >Diatomite</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >13.75</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.16</td><td align="center" valign="middle" >47.81</td><td align="center" valign="middle" >52.03</td><td align="center" valign="middle" >Silty argillite</td></tr><tr><td align="center" valign="middle" >11</td><td align="center" valign="middle" >16.85</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0.13</td><td align="center" valign="middle" >69.20</td><td align="center" valign="middle" >30.67</td><td align="center" valign="middle" >Siltstone</td></tr><tr><td align="center" valign="middle" >12</td><td align="center" valign="middle" >30.75</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >0.03</td><td align="center" valign="middle" >84.67</td><td align="center" valign="middle" >15.30</td><td align="center" valign="middle"  rowspan="2"  >Diamictite of silty matrix</td></tr><tr><td align="center" valign="middle" >13</td><td align="center" valign="middle" >28.50</td><td align="center" valign="middle" >2</td><td align="center" valign="middle" >0.68</td><td align="center" valign="middle" >74.08</td><td align="center" valign="middle" >25.24</td></tr></tbody></table></table-wrap><fig id="fig3"><label>Figure 3</label><caption><p> Profile of Section 2 (meters) illustrating from left to right: the results of the textural classification; the percentage of organic matter; the occurrence of the spicules of each sponge species, according to their category and abundance; figures of the gemmoscleres with occurrence in this section. Abbreviations: A, argillite; S, siltstone; Af, fine sandstone; Am, medium sandstone; Ag, coarse sandstone; C, conglomerate/diamictite. Legend as Figure 2. Adaptated from [31] [32] </p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\95bdd813-9eb9-4bf4-b3ad-b65847cbc8b4.png"/></fig><fig id="fig4"><label>Figure 4</label><caption><p> Profile of Section 3 (meters) illustrating from left to right: the results of the textural classification; the percentage of organic matter; the occurrence of the spicules of each sponge species, according to their category and abundance; figures of the gemmoscleres with occurrence in this section. Abbreviations: A, argillite; S, siltstone; Af, fine sandstone; Am, medium sandstone; Ag, coarse sandstone; C, conglomerate/diamictite. Legend as Figure 2. Adaptated from [31] [32] </p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\47f5e929-6dfd-4517-badb-4e32c00ee57a.png"/></fig><p>Section 2 and Layers # 4, 7 (<xref ref-type="fig" rid="fig6">Figure 6</xref>(c), <xref ref-type="fig" rid="fig6">Figure 6</xref>(d)), and 9 from Section 3. It should be noted that none of the layers of spongillites presented diatom frustules, whereas there were numerous sponge spicules in the diatomites. The ternary diagram (<xref ref-type="fig" rid="fig5">Figure 5</xref>) also showed that the layers of spongillites and diatomites were associated with the fine fraction of the sediments, as illustrated in the profiles in Figures 2-4.</p></sec><sec id="s4_2"><title>4.2. Analysis of the Sponge Spicules</title><p>The facies that contained abundant spicules from the skeleton of sponges (megascleres and microscleres) and</p><fig id="fig5"><label>Figure 5</label><caption><p> Ternary diagram showing the granulometric relation between sandy/silt/clay in the layers from Sections 1, 2 and 3 of the Cemit&#233;rio Palaeolake. The circle indicates a single layer with higher percentages of sand, Layer # 2/3 from Section 1. The arrows indicate the layers with higher clay contents, Layer # 7 from Section 1 and Layer # 10 from Section 3</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\e46e0cab-5edf-4b2d-a67a-a5b34e5c97c9.png"/></fig><fig id="fig6"><label>Figure 6</label><caption><p> SEM images of the spongillite (a) (b) and diatomite (c) (d), respectively, Layer # 7 and 8 from Section 3. (a) (b): Sponges megascleres; (c) (d): Diatom frustules</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\97d17694-9fbc-4310-8624-d065cec2b913.png"/></fig><p>also from the gemmules (gemmoscleres) consisted of siltstone (Layer # 11 from Section 1; Layers # 3, 4 and 12 from Section 2), diamictites (Layer # 11 from Section 2; Layers # 2 and 13 from Section 3), and spongillites (Layer # 15 from Section 2; Layer # 8 from Section 3). Gemmoscleres of Dosilia pydanieli, Corvohetero- meyenia australis, Radiospongilla amazonensis, and Trochospongilla variabilis occurred in all of these facies (Figures 2-4). However, gemmoscleres of Corvomeyenia thumi and Metania spinata occurred only in the Layers # 11, 12, and 15 from Section 2 and Layer # 2 from Section 3 (<xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>). It should be noted that M. spinata occurred also with skeletal spicules throughout the three studied profiles from the Cemit&#233;rio Palaeolake [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] , whereas the megascleres of C. thumi were restricted to precisely the same layers where its gemmoscleres occurred (<xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>). Heterorotula fistula which was only registered in Section 2 [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] occurred also with its megascleres and gemmoscleres (<xref ref-type="fig" rid="fig3">Figure 3</xref>).</p><p>The facies that contained only abundant spicules from the skeleton of sponges were siltstones (Layers # 9 and 14 from Section 1; Layer # 13 from Section 2; Layer # 11 from Section 3), diamictites (Layer # 6 from Section 1; Layer # 14 from Section 2; Layers # 3, 6 and 12 from Section 3), diatomites (Layer # 5 from Section 1; Layer #16 from Section 2; Layers # 4, 7 and 9 from Section 3), and only one of silt-mudstone (Layer # 10 from Section 3) (Figures 2-4). The spongillites from Layer # 10 from Section 1 (<xref ref-type="fig" rid="fig2">Figure 2</xref>) also showed a predominance of megascleres and microscleres.</p></sec><sec id="s4_3"><title>4.3. OM</title><p>The results with respect to the organic content of the different rocks from the Cemit&#233;rio Palaeolake, in addition to the levels previously characterized by [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] (Layer # 14 from Section 1 and Layers # 12 and 15 from Section 2), are presented in <xref ref-type="table" rid="table1">Table 1</xref> and illustrated in Figures 2-4. In Section 1, two peaks of OM were recorded, one in Layer # 4 and another in Layer # 16. In Section 2, Layers # 8, 10, and 13 stand out, whereas in Section 3, the highest levels were detected in Layer # 8. However, when the three profiles from the Cemit&#233;rio Palaeolake were compared, the boxplot graph (<xref ref-type="fig" rid="fig7">Figure 7</xref>) showed that Sections 1 and 2 had the greatest variation in OM, from 7.50% to 62.10% and from 10.65% to 75.60% (<xref ref-type="fig" rid="fig2">Figure 2</xref> and <xref ref-type="fig" rid="fig3">Figure 3</xref>), respectively. The graph also showed that most of the layers from Section 2 had high levels of OM (28% - 40%), whereas in Sections 1 and 3, the percentage of OM was less than 30% in most of the layers (<xref ref-type="fig" rid="fig7">Figure 7</xref>).</p></sec><sec id="s4_4"><title>4.4. Correlation of the Three Sections from the Paleolake</title><p>On the basis of the sedimentary features and the association of the preserved sponge spicules, it was possible to correlate the three sections from the Cemit&#233;rio Palaeolake (<xref ref-type="fig" rid="fig8">Figure 8</xref>). The deposit thickest sequence was detected in Section 1, where it reached approximately 26.5 m in height (<xref ref-type="fig" rid="fig2">Figure 2</xref>). On the basis of the dating provided by [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] , it became clear that the base of this Palaeolake was mainly exposed in Section 1 and consisted of diamictites (Layer # 1) overlaid by a sandy conglomerate (Layer # 2/3), with a combined thickness of approximately 6 m (<xref ref-type="fig" rid="fig2">Figure 2</xref>). The basal diamictites in both Sections 1 and 2 were characterized by the presence of clasts of exclusively mineral origin (<xref ref-type="table" rid="table1">Table 1</xref>). Sponge spicules from five species of both lentic and lotic environments were also observed in both layers (<xref ref-type="fig" rid="fig8">Figure 8</xref>).</p><fig id="fig7"><label>Figure 7</label><caption><p> Boxplot Graph showing the variation of organic matter in the Sections 1, 2 and 3 of the Cemit&#233;rio Palaeolake deposit</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\945eba06-9c26-4184-9be1-a5c0695115a0.png"/></fig><fig id="fig8"><label>Figure 8</label><caption><p> Lithostratigraphic profiles of the Cemit&#233;rio Palaeolake, Catal&#227;o, Goi&#225;s, illustrating the correlation among the three analyzed sections (dashed line), the corresponding palaeoclimatic interpretations and geomorphological steps of the dome structure erosion (a-b, after [44] ), taking to formation of the basin and its final colmatation (c-f; modified from [45] )</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-2800795x\4384c8f0-9119-44c1-a2c1-c8c3eed62dc7.png"/></fig><p>The upper part of the basal portion of Section 1 was lost during the recovery procedures. A layer of siltstone followed, with high levels of OM and presence of sponge spicules exclusively from a lentic environment (Layer # 4, <xref ref-type="fig" rid="fig2">Figure 2</xref>). Similar features occurred in Layer # 1 from Section 3, allowing these two sections to be correlated (<xref ref-type="fig" rid="fig8">Figure 8</xref>).</p><p>The subsequent layers in Section 1 corresponded to two diamictites separated by a layer of silt-mudstone (Layers # 6, 7 and 8; <xref ref-type="fig" rid="fig2">Figure 2</xref>). Alternating layers of diamictites and siltstones characterized the longest sequence in Section 2 (Layers 2 - 15; <xref ref-type="fig" rid="fig3">Figure 3</xref>). The diamictites in these two sequences, from Sections 1 and 2, presented clasts of both mineral and organic origin (<xref ref-type="table" rid="table1">Table 1</xref>), allowing for a correlation to be made between these two sections. This correspondence was also confirmed by the considerable decrease in spicules in both sections.</p><p>The correlation found between Layers # 11 to 15 from Section 2 and Layer # 2 from Section 3 is based on the occurrence of C. thumi, which is restricted to these layers (<xref ref-type="fig" rid="fig8">Figure 8</xref>).</p><p>Field observations [<xref ref-type="bibr" rid="scirp.48340-ref42">42</xref>] indicated two guide levels between Sections 1 and 3. The first consists of a thin layer of spongillites between two layers of diatomites, occurring in Layers # 7, 8, and 9 from Section 3 (<xref ref-type="fig" rid="fig2">Figure 2</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>) and juxtaposed to that of the diamictites in Layer # 8 from Section 1 (<xref ref-type="fig" rid="fig8">Figure 8</xref>). The second corresponds to a paleosols facies sampled at Section 1 (Layer # 14; <xref ref-type="fig" rid="fig2">Figure 2</xref>) and top of Section 3 (<xref ref-type="fig" rid="fig8">Figure 8</xref>).</p></sec></sec><sec id="s5"><title>5. Discussion</title><p>The ages provided by [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] for Sections 1 and 2 of the Cemit&#233;rio Palaeolake, together with the sedimentary features and associated spicules, suggest the existence of five distinct phases of climatic regimes that influenced the nature of the deposit from the base to the top (<xref ref-type="fig" rid="fig8">Figure 8</xref>).</p><sec id="s5_1"><title>5.1. Phases I and II</title><p>Phase I, which was older than 51,780 <sup>14</sup>C yr BP [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] , was formed during high levels of precipitation, as indicated by the diamictites and also by the conglomerates, favouring flows of unselected sediments resulting from the erosion of the dome and that accumulated in the areas with less steep slopes (<xref ref-type="fig" rid="fig8">Figure 8</xref>(a)). Machado and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref34">34</xref>] demonstrated that a similar process is occurring in the dome of the Serra Negra, which exhibits a centripetal drainage system that accumulates in the centre. Phase I can be taken as the intermediate step of erosion of dome structures as described by [<xref ref-type="bibr" rid="scirp.48340-ref44">44</xref>] . The incorporation of organic clasts during this phase (<xref ref-type="fig" rid="fig2">Figure 2</xref> and <xref ref-type="fig" rid="fig8">Figure 8</xref>) indicates a change from an arid to a humid climate. Thus, the occurrence of higher pluviosity favoured the formation of a lotic system, forming a layer of sandy conglomerate, which retained sponge spicules from lotic environments.</p><p>Phase II, which was dated from 51,780 &#177; 400 <sup>14</sup>C yr BP [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] , features a shallow lake system with free permanent water coverage, intense illumination in the water column, scattered macrophytes, and stable water levels (<xref ref-type="fig" rid="fig8">Figure 8</xref>(b), <xref ref-type="fig" rid="fig8">Figure 8</xref>(c)), as indicated by the diatomite layer containing the skeletal spicules of sponges from lacustrine environments [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] . Machado and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref34">34</xref>] demonstrated the presence of abundant megascleres and microscleres in the bottom sediments of the actual lake on the Serra Negra Dome and attributed this to the perennial nature of this lake. Volkmer-Ribeiro and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref26">26</xref>] reported that the predominant species of sponges in the diatomite rocks in the northeast region of Brazil are those that occur in shallow lakes exposed to full sunlight and limited water movement.</p><p>Corvoheteromeyenia australis, for the first time identified in a spongillite-forming community, is endemic to South America and was described from living material collected in Argentina [<xref ref-type="bibr" rid="scirp.48340-ref46">46</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref47">47</xref>] . Its occurrence in the Cemit&#233;rio Palaeolake, from Phase I, and its absence in the current Serra Negra Lake [<xref ref-type="bibr" rid="scirp.48340-ref34">34</xref>] , indicates that a colder climate prevailed in central Brazil during the formation of the Cemit&#233;rio Palaeolake.</p><p><xref ref-type="table" rid="table2">Table 2</xref> provides a comparison of palaeoclimatic interpretations of the developmental stages of the Palaeolake</p><table-wrap id="table2"  position="float"><object-id pub-id-type="pii">Table 2</object-id><label>Table 2</label><caption><p>. Interpretations of the climatic evolution along the 5th phases detected in the Cemit&#233;rio Palaeolake, compared with those already presented for central/southeast Brazil</p></caption><table><thead><tr><th align="center" valign="middle" >Age</th><th align="center" valign="middle" >F</th><th align="center" valign="middle" >Facies</th><th align="center" valign="middle" >Interpretation</th><th align="center" valign="middle" >Bibliographic comparison</th></tr></thead><tbody><tr><td align="center" valign="middle" >&gt; 51,780 &#177; 400 <sup>14</sup>C yr BP.</td><td align="center" valign="middle" >I</td><td align="center" valign="middle" >Layers # 1 and 2/3  from Section 1; Layer # 1 from Section 2</td><td align="center" valign="middle" >Cold and rainy</td><td align="center" valign="middle" >A cold and dry climate between 40,000 and 50,000 yr BP in Salitre [2] .</td></tr><tr><td align="center" valign="middle" >51,780 &#177; 400 <sup>14</sup>C yr BP.</td><td align="center" valign="middle" >II</td><td align="center" valign="middle" >Layers # 4 and 5  from Section 1;  Layer # 1 from  Section 3</td><td align="center" valign="middle" >Cold and wet</td><td align="center" valign="middle" >An increase in moisture at low temperatures as from 45,000 yr BP in Salitre and Serra Negra [1] [2] .</td></tr><tr><td align="center" valign="middle" >Between 34,700 &#177; 5000  and 48,333 &#177; 370 <sup>14</sup>C yr BP.</td><td align="center" valign="middle" >III</td><td align="center" valign="middle" >Layers # 6, 7 and 8  from Section 1;  Layers # 2 - 15  from Section 2;  Layers # 2 and 3  from Section 3</td><td align="center" valign="middle" >Seasonal and gradually warming</td><td align="center" valign="middle" >A slow decrease in vegetation as from 36,700 yr BP in S&#227;o Paulo [8] ; Seasonality during this period in Serra Negra [1] ; Stable water levels in the Salitre basin between 33,000 and 40,000 yr BP [2] . However, both records [1] [2]  reported an increase in temperature during this period. A more seasonal climate is suggested from 28.300 to 32,000 yr BP in Crom&#237;nia [3] [4] .</td></tr><tr><td align="center" valign="middle" >Between 27,500 &#177; 4000 and 34,700 &#177; 5000 yr BP.</td><td align="center" valign="middle" >IV</td><td align="center" valign="middle" >Layers # 9-14  from Section 1;  Layers # 16 from Section 2; Layers # 4 - 13 from Section 3</td><td align="center" valign="middle" >Cold and wet</td><td align="center" valign="middle" >Expansion of the Atlantic forest and high humidity in the period between 28,225 and 30,400 yr BP, in the region of S&#227;o Paulo [8] ; Presence for the Crom&#237;nia deposit of a shallow lake surrounded by open countryside with a wetter and probably cooler period between 20,000 and 27,000 yr BP, when compared to the present [3] [4] ; The same was indicated for &#193;guas Emendadas between 21,000 and 24,000 yr BP [6] . Higher rainfall in a slightly cooler and less seasonal climate between 26,206 and 28,166 yr BP [27] .</td></tr><tr><td align="center" valign="middle" >&lt;27,500 &#177; 4000 yr BP.</td><td align="center" valign="middle" >V</td><td align="center" valign="middle" >Layers # 15 - 18 from Section 1</td><td align="center" valign="middle" >Cold and dry</td><td align="center" valign="middle" >Colder and drier conditions in southern and southeastern Brazil during the Last Glacial Maximum (LGM), as from 25,000 yr BP [2] [5] .</td></tr></tbody></table></table-wrap><p>with other records produced for central Brazil. The oldest dating available for this region was presented by [<xref ref-type="bibr" rid="scirp.48340-ref2">2</xref>] , through the analysis of pollen and algae deposited in the Serra do Salitre, MG, alkaline carbonatite dome, which is similar to those of the Cemit&#233;rio Palaeolake and the Serra Negra Lake (<xref ref-type="fig" rid="fig1">Figure 1</xref>). The authors based their arguments on a correlation with a deposit studied precisely in the Serra Negra Lake [<xref ref-type="bibr" rid="scirp.48340-ref1">1</xref>] , and with the oldest dating of 42,000 yr BP, and indicated a cold and dry climate between 40,000 and 50,000 yr BP. In both the Salitre and Serra Negra deposits, that phase was followed by a change in the landscape as from 45,000 yr BP. The increase in tree pollen, with the occurrence of some originating from colder climates, suggests an increase in moisture at low temperatures. The proposed sequence for Phases I and II of the Cemit&#233;rio Palaeolake does not differ from the palaeo-interpretation, although the results presented for Phase I suggest that an increase in rainfall and humidity began at a time earlier than 51,780 <sup>14</sup>C yr BP. A record submitted by [<xref ref-type="bibr" rid="scirp.48340-ref8">8</xref>] obtained from the coastal mountains, in this case in S&#227;o Paulo, showed that the Atlantic Forest expanded in the same region during the last 100,000 yr BP, thus confirming the occurrence of wetter periods during the late Pleistocene, as was also indicated in the deposits from central Brazil.</p><p>To explain the colder temperature during the late Pleistocene, several authors have suggested that polar incursions from the south might have been more frequent during that period [<xref ref-type="bibr" rid="scirp.48340-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref8">8</xref>] . Furthermore, Ledru and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref8">8</xref>] also suggested that these incursions had a significant impact on the climate of South America during the last glacial period. This would explain the presence of C. australis in the Cemit&#233;rio Palaeolake as well as its bio-geographical position today, with its occurrence restricted to southern South America.</p></sec><sec id="s5_2"><title>5.2. Phase III</title><p>Phase III, dated from just under 34,700 &#177; 5000 to 48,333 &#177; 370 <sup>14</sup>C yr BP [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] , is characterized by an alternating sequence of siltstones and diamictites, as seen mainly in Section 2, Layers # 2 to 15, where there was still a layer of spongillite in the top layer (<xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig8">Figure 8</xref>). This alternation indicates the presence of periods of heavy rainfall that caused mudslides (diamictites), intercalated with long periods of lacustrine sedimentation (siltstones and spongillite). In fact, Machado and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] indicated the rare occurrence of sponge spicules typical of lotic environments, whereas spicules from sponges typical of lakes were abundant (<xref ref-type="fig" rid="fig3">Figure 3</xref>). However, the layers of siltstone in Section 2 were distinguished from the other facies in the Cemit&#233;rio Palaeolake deposit by the high levels of OM (<xref ref-type="fig" rid="fig7">Figure 7</xref>) as well as by the abundance of spicules, there included gemmoscleres (<xref ref-type="fig" rid="fig3">Figure 3</xref>).</p><p>Gemmules are asexual reproductive structures produced by particularly continental sponges, during periods of adversity such as dry periods [<xref ref-type="bibr" rid="scirp.48340-ref48">48</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref49">49</xref>] . However, the specific identification of the gemmoscleres from the Cemit&#233;rio Palaeolake revealed that Layers # 11, 12, and 15 from Section 2 and Layer # 2 from Section 3, on top of Phase III, were unique in showing that the entire sponge community of the Palaeolake, including the species C. thumi, was in the process of forming gemmules (<xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>). The latter species only occurred during periods of drastic reduction in the water column and encrusted substrates very near the water surface, as was seasonally observed by [<xref ref-type="bibr" rid="scirp.48340-ref50">50</xref>] in the seasonal lakes of the Marac&#225; Island that, with the exception of H. fistula, contained the same community of sponges detected in Phase III. Volkmer-Ribeiro and Turcq [<xref ref-type="bibr" rid="scirp.48340-ref38">38</xref>] report this species as an excellent palaeoenvironmental indicator. Moreover, several studies of columns of sediment from the Serra dos Caraj&#225;s, Par&#225;, have used the presence of C. thumi gemmoscleres to define successive stages of drought during the Holocene [<xref ref-type="bibr" rid="scirp.48340-ref16">16</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref17">17</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref51">51</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref52">52</xref>] . Machado and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] detected fully preserved gemmules of C. thumi precisely in Layers # 12 and 15 from Section 2, thus corroborating with the proposed interpretation. Furthermore, C. thumi also indicates an increase in temperature during the development of Phase III, with warmer dry seasons, at least when compared with the other phases of the Cemit&#233;rio Palaeolake. Interestingly, Heterorotula fistula was restricted to Section 2 [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] and was the most abundant species among diatomites from the northeast of Brazil [<xref ref-type="bibr" rid="scirp.48340-ref26">26</xref>] .</p><p>This fluctuation in water level during Phase III of the Cemit&#233;rio Palaeolake explains the higher organic levels, between 28% and 40%, in the layers of Section 2 (<xref ref-type="fig" rid="fig7">Figure 7</xref>). These levels were similar to those detected in the sediments from the current Serra Negra Lake, with just over 30% OM [<xref ref-type="bibr" rid="scirp.48340-ref34">34</xref>] . However, an abundance of spicules from the skeletal structure of the sponges, which are suggestive of continuous sponge production allowed by permanent water levels as indicated for the Serra Negra Lake, only occurred in a thin layer of siltstone at the top of Phase III (Layer # 13; <xref ref-type="fig" rid="fig3">Figure 3</xref>), and so, for a very short period of time. The high altitudes common to Cemit&#233;rio Palaeolake and Serra Negra Lake indicate that the peaty sediments in Phase III of the palaeolake (<xref ref-type="fig" rid="fig8">Figure 8</xref>(d)) were produced during a similar microclime, although more seasonal than the actual one acting on Serra Negra Lake.</p><p>The palaeoenvironmental and palaeoclimatic interpretations presented for Phase III of the Cemit&#233;rio Palaeolake can be compared with those proposed by [<xref ref-type="bibr" rid="scirp.48340-ref8">8</xref>] (<xref ref-type="table" rid="table2">Table 2</xref>), who suggested that a slow decrease in vegetation occurred from 36,700 yr BP. This period could be correlated with the sequence of Phases II and III of the Cemit&#233;rio Palaeolake. In this sense, the retraction of the forest could have been caused by the occurrence of successive periods of drought. De Oliveira [<xref ref-type="bibr" rid="scirp.48340-ref1">1</xref>] also inferred the occurrence of seasonality in the Serra Negra deposit during this period. In contrast, Ledru and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref2">2</xref>] reported more stable water levels in the Salitre basin between 33,000 and 40,000 yr BP and suggested the higher altitude of Salitre in relation to Serra Negra might account for this difference. However, these authors cited a gap in the Salitre record, followed by the formation of a peat bog, just over 32,000 yr BP. Both records [<xref ref-type="bibr" rid="scirp.48340-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref2">2</xref>] reported an increase in temperature, as proposed in the present study for Phase III of the Palaeolake. Likewise, a more seasonal climate, similar to the current one, was suggested by [<xref ref-type="bibr" rid="scirp.48340-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref4">4</xref>] in profiles collected from a vereda (Buritizal) at a height of 710 m in the region of Crom&#237;nia, Goi&#225;s. These authors emphasized that prior to 32,400 yr BP, a vereda and a gallery forest existed on the site and the surrounding area was occupied by a wooded Cerrado. Barberi and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref6">6</xref>] , who analysed pollen obtained from a vereda on the top of a plateau (1040 m) in &#193;guas Emendadas, near the city of Brasilia, suggested that peat deposition began in the area 30,480 yr BP (<xref ref-type="table" rid="table2">Table 2</xref>).</p></sec><sec id="s5_3"><title>5.3. Phase IV</title><p>Phase IV, which has been dated to be between 27,500 &#177; 4000 and 34,700 &#177; 5000 yr BP [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] , includes the longest sequences in Sections 1 (Layers # 9 to 14, <xref ref-type="fig" rid="fig2">Figure 2</xref>) and 3 (Layers # 4 to 13; <xref ref-type="fig" rid="fig4">Figure 4</xref>), and the diatomite from Section 2 (Layer # 16; <xref ref-type="fig" rid="fig3">Figure 3</xref>) (<xref ref-type="fig" rid="fig8">Figure 8</xref>). Diatomites and siltstones with abundant spicules from the skeletal structure of the sponges are typical facies in this phase and indicate a basin covered with free permanent water, intense illumination in the water column, and scattered macrophytes (<xref ref-type="fig" rid="fig8">Figure 8</xref>(e)), as was also described in Phase II. Fluctuations in the water column which also occurred during this phase are documented in the spongillite as well as in the layers with abundant spicules and gemmoscleres. However, these periods could not be compared to those described for Phase III. The absence of C. thumi and, moreover, of gemmoscleres from M. spinata indicate that the reductions were minimal and short, indicating the predominance of a wetter and less seasonal climate. The formation of diamictites in Section 3 is noteworthy, as observed during this phase (<xref ref-type="fig" rid="fig4">Figure 4</xref> and <xref ref-type="fig" rid="fig8">Figure 8</xref>). However, these are distinct from the other diamictites formed in the Palaeolake because the clasts exclusively consisted of OM [<xref ref-type="bibr" rid="scirp.48340-ref42">42</xref>] . Accordingly, this observation confirmed the presence of lighter rainfall during this period, thus favouring the leaching of the lighter, organic, clasts into the basin.</p><p>Concurrent with Phase IV of the Cemit&#233;rio Palaeolake (<xref ref-type="table" rid="table2">Table 2</xref>), [<xref ref-type="bibr" rid="scirp.48340-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref2">2</xref>] signalled a hiatus in the Salitre and Serra Negra deposits that was probably due to local events, since the result for this phase of the Cemit&#233;rio Palaeolake indicated the existence of a period with permanent water levels and, therefore, wetter conditions. Such results conform also those of [<xref ref-type="bibr" rid="scirp.48340-ref8">8</xref>] , who recorded the expansion of the Atlantic forest and high humidity during the period between 28,225 and 30,400 yr BP, in the region of S&#227;o Paulo. Moreover, the records submitted for the Crom&#237;nia deposit [<xref ref-type="bibr" rid="scirp.48340-ref3">3</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref4">4</xref>] indicated a retraction of arboreal and shrub elements in the region from 28,300 to 32,000 yr BP, followed by substitution of the vereda by a shallow lake surrounded by open countryside. This suggests a wetter and probably cooler period between 20,000 and 27,000 yr BP, compared to the present. For the profile studied in the vereda peat bog in &#193;guas Emendadas [<xref ref-type="bibr" rid="scirp.48340-ref6">6</xref>] between 24,000 and 25,790 yr BP, pollen grains and algal remains indicate the presence of a marsh surrounded by patches of open Cerrado and gallery forest on top of the plateau. In addition, between 21,000 and 24,000 yr BP, the vegetation was denser than that of the present period, with abundant aquatic plants and some trees from cooler climates, suggesting a wetter and probably cooler climate. In more lowland terrains in central Brazil, Almeida and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref27">27</xref>] presented the results of palaeoenvironmental interpretations in spongillite deposits from the region of Jo&#227;o Pinheiro, MG (average altitude of 560 to 600 m). According to the composition of the identified spicules and sponge community, the authors described the development of these palaeo-basins to be from 28,166 yr BP. At an earlier period, they suggested the basin was formed over a slight depression in the terrain, giving rise to a shallow lake and initially favouring diatoms. This phase was followed by a period that was more favourable to sponge settlement, mainly by M. spinata, without the formation of gemmules, which led the authors to suggest that concurrent with the deepening of the pond, there was a higher rainfall in a slightly cooler and less seasonal climate. Later, for the period between 26,206 and 26,656 yr BP, due to the presence of gemmoscleres, the authors reported a reduction in the water level and suggested periods of intermittent short droughts and rainy seasons, although without heavy downpours. Thus, these results also corroborate those presented for Phase IV of the Cemit&#233;rio Palaeolake. Almeida and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref27">27</xref>] reported an age between 13,887 and 14,495 yr BP for the layers of “pure” spongillite deposits from Jo&#227;o Pinheiro, thus impeding any correlation with spongillite deposits from the Cemit&#233;rio Palaeolake.</p></sec><sec id="s5_4"><title>5.4. Phase V</title><p>Phase V covered the period of less than 27,500 &#177; 4000 yr BP [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] and is characterized by siltstone facies sampled only at the top of Section 1, Layers # 15 to 18 (<xref ref-type="fig" rid="fig2">Figure 2</xref> and <xref ref-type="fig" rid="fig8">Figure 8</xref>). The volume of OM increased, whereas sponge spicules decreased until they completely disappeared. This phase witnessed the complete filling of the basin (<xref ref-type="fig" rid="fig8">Figure 8</xref>(f)) and can be correlated with the Last Glacial Maximum (LGM), which occurred between 11,000 and 25,000 yr BP, as indicated by [<xref ref-type="bibr" rid="scirp.48340-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref5">5</xref>] , where colder and drier conditions prevailed in southern and central Brazil (<xref ref-type="table" rid="table2">Table 2</xref>).</p></sec></sec><sec id="s6"><title>6. Genesis of Bio-Siliceous Accumulations</title><p>The layers of spongillites in southeastern Brazil [<xref ref-type="bibr" rid="scirp.48340-ref19">19</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref26">26</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref27">27</xref>] were thick and, at the base, contained spicules of M. spinata, with contributions from D. pydanieli and H. fistula and, above, in the transition to the layer of peat, T. variabilis and R. amazonensis. In the top, peaty layer, there were also spicules from C. thumi and gemmoscleres from all six species. The layers of spongillites in the Cemit&#233;rio Palaeolake deposit were thin and contained C. australis [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] , whereas C. thumi and H. fistula only occurred in the spongillites in Layer # 15 from Section 2 (<xref ref-type="fig" rid="fig3">Figure 3</xref>), which also contain an exceptional amount of whole gemmules [<xref ref-type="bibr" rid="scirp.48340-ref32">32</xref>] . Volkmer-Ribeiro and Motta [<xref ref-type="bibr" rid="scirp.48340-ref19">19</xref>] attributed the existence of the most basal layer of the spongillite deposits to a deeper palaeo-envi- ronment with a greater abundance of submerged macrophytes, the preferred substrate of M. spinata [<xref ref-type="bibr" rid="scirp.48340-ref33">33</xref>] , which did not occur during the evolution of the Cemit&#233;rio Palaeolake. The absence of diatoms in the spongillite layers, as also observed in the Cemit&#233;rio Palaeolake, is a typical feature of such deposits, precisely because the abundance of macrophytes prevents light, which is essential for photosynthetic organisms such as diatoms, from penetrating the body of water. However, the presence of sponge spicules is common in layers of diatomites [<xref ref-type="bibr" rid="scirp.48340-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref23">23</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref26">26</xref>] . Thus, the alternating layers of diatomites and spongillites in the Cemit&#233;rio Palaeolake deposit indicates variations in the permanence of water levels, causing the establishment of a greater or lesser degree of macrophytic vegetation and, concomitantly, more or less light penetration.</p><p>The decrease in the availability of water from Phase I to Phase II, which favoured diatoms imparted a significant effect on the characteristics of the lentic environment inside the Catal&#227;o I dome. This interpretation has previously been inferred for shallow basins, remarkable for the accumulation of diatoms in northeastern Brazil [<xref ref-type="bibr" rid="scirp.48340-ref26">26</xref>] Moreover, Moyle and Dolley [<xref ref-type="bibr" rid="scirp.48340-ref22">22</xref>] reported that the areas of diatomites in continental U.S.A. were also associated with small lake systems formed by the clogging of lotic systems. Almeida and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref27">27</xref>] , when comparing sponge species present in two profiles of lakes with spongillite deposits in the region of Jo&#227;o Pinheiro, MG, confirmed the results reported by [<xref ref-type="bibr" rid="scirp.48340-ref26">26</xref>] and added that, in the case of karst environments, the process of forming palaeolakes that favour the production of diatoms occurred due to the slow dissolution of carbonate rock, without the immediate establishment of macrophytes, but instead a shallow sheet of water exposed to the sun. In the case of spongillites, the karst process would involve the undermining of the bottom of lakes, thus generating initially deeper basins. There is no doubt that the intense lotic environments during Phase I (<xref ref-type="fig" rid="fig8">Figure 8</xref>(a)), contributed to the large volume of water and, consequently, to the increased physical and chemical weathering at the bottom of the lake, which is typical of karstic lakes, as also noted by [<xref ref-type="bibr" rid="scirp.48340-ref31">31</xref>] .</p><p>The availability of silica is important in the formation of sponge spicules [<xref ref-type="bibr" rid="scirp.48340-ref53">53</xref>] , as well as that of diatomic algae [<xref ref-type="bibr" rid="scirp.48340-ref22">22</xref>] . Machado and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref34">34</xref>] highlighted the high levels of silica dissolved in the water of the Serra Negra Lake (8 to 32 mg/L) and showed that these were derived from the rocks in the volcanic dome. Pisera and S&#225;ez [<xref ref-type="bibr" rid="scirp.48340-ref23">23</xref>] , who described Ephydatia chileana from gemmules fully preserved in the diatomite layer within alluvial-lacustrine deposits from the Late Miocene Quillagua Formation, in the Atacama region of Chile, attributed the high silica content in the lake environment to the volcanic origin of the sediments, thus encouraging the development of diatoms and freshwater sponges. Moreover, Moyle and Dolley [<xref ref-type="bibr" rid="scirp.48340-ref22">22</xref>] indicated that diatomite deposits in North American were generally associated with volcanic terrains, which supplied the silica needed for the skeletal development of diatoms. Barbosa and colleagues [<xref ref-type="bibr" rid="scirp.48340-ref37">37</xref>] reported that the Igneous Province of Upper Parana&#237;ba are rich in silicate rocks. Given that the pyroclastic deposits and lavas of this Province also covered large areas of the Mata Corda Group [<xref ref-type="bibr" rid="scirp.48340-ref36">36</xref>] [<xref ref-type="bibr" rid="scirp.48340-ref54">54</xref>] , it was reasonable for us to infer that these rocks were, and still are, an important source of silica for the surrounding aquatic environments, as are those of the Areado Group, as indicated by [<xref ref-type="bibr" rid="scirp.48340-ref55">55</xref>] . The rocks of the Igneous Province of the Alto Paranaiba are located between the Paran&#225; and S&#227;o Francisco Basins, one of the most important watersheds in Brazil (<xref ref-type="fig" rid="fig1">Figure 1</xref>).</p><p>Hilgen and Krijgsman [<xref ref-type="bibr" rid="scirp.48340-ref30">30</xref>] , who studied the Tripoli diatomite formation in three distinct deposits in Sicily, Italy, astronomically dated at 7005 Ma, highlighted the intercalated occurrence of homogeneous marls/clays, diatomites, and layers of sapropels, and noted a very strong relationship between the sapropels and diatomites, relating the availability of nutrients in the sapropel as being of paramount importance for the intense production of diatomic algae and thus formation of diatomites. Accordingly, the reduction in the water column during the formation of the spongillites in the Cemit&#233;rio Palaeolake favoured the accumulation of OM and nutrient supply for consumption by the diatoms, as new rainfall occurred. Moyle and Dolley [<xref ref-type="bibr" rid="scirp.48340-ref22">22</xref>] stated that nutrients such as phosphates and nitrates were made available in the water column when organisms died and decomposed on the lake bottom. This would explain the presence of diatomites and spongillites in the Cemit&#233;rio Palaeolake, and their intercalation, as in the case of Layers # 7, 8, and 9 from Section 3 or even the sequence of spongillites followed by diatomites in Section 2 (Layers # 15 and 16) (<xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>).</p><p>Regarding the need of diatoms for light, the formation of diatomites was linked to the wetter phases of the Cemit&#233;rio Palaeolake (Phases II and IV), which suggested greater cloud cover and less sun exposure. However, photosynthetic organisms such as diatom algae would not have produced such deposits without full light hitting the water column of the Palaeolake. In this regard, Hilgen and Krijgsman [<xref ref-type="bibr" rid="scirp.48340-ref30">30</xref>] highlighted a very clear correlation between the depositional periods of sapropels and diatomites with the patterns of maximum insolation and minimum precession, particularly in the Northern Hemisphere. The formation sequence of the two diatomite facies dated in the Cemit&#233;rio Palaeolake (Phase II and IV, <xref ref-type="fig" rid="fig8">Figure 8</xref>), corresponded to a periodicity of approximately 22,000 yr, which coincided with the complete precession cycle of approximately 20,000 yr prior [<xref ref-type="bibr" rid="scirp.48340-ref56">56</xref>] . Berger and Loutre [<xref ref-type="bibr" rid="scirp.48340-ref56">56</xref>] produced figures for the astronomical parameters of the Earth’s orbit, eccentricity, obliquity, and precession in the Quaternary. In terms of the precession cycle, the illustrations provided by the authors showed maximum values shortly before 50,000 yr BP. Around 30,000 yr BP, the precession values were increasing and reached their maximum just before 20,000 yr BP. Thus, in the case of frequent clouds and shorter sun exposure, the occurrence of an orbital event that increased solar intensity in the Southern Hemisphere such as during maximum precession, could have favoured the formation of the diatomites during Phases II an IV in the Cemit&#233;rio Palaeolake.</p></sec><sec id="s7"><title>7. Final Remarks</title><p>The results of the analysis of the freshwater sponge spicules from the Cemit&#233;rio Palaeolake deposit were highly significant towards not only the reconstitution of palaeoenvironments, but particularly those of palaeoclimates. At least two species could be here highlighted as good climatic indicators. Corvoheteromeyenia australis, which is now restricted to southern South America, stands out as an indicator of colder and wetter weather. Accordingly, the data suggest that polar incursions originating in Antarctica were common during the late Pleistocene and may have played a notable role in the humidity of central Brazil during the period &gt; 51,780 &#177; 400 <sup>14</sup>C yr BP until the beginning of the LGM, when drier conditions began to predominate. Corvomeyenia thumi is again confirmed as a sponge species indicator of environments subjected to marked seasonal droughts. In the case of the Cemit&#233;rio Palaeolake, the restriction of the presence of this species a little before 34,700 &#177; 5000 yr BP, at the upper part of Phase III, suggests the occurrence of a more seasonal climate.</p><p>The Cemit&#233;rio Palaeolake stands out as a remarkable deposit, if not unique one in Brazil and in the world, to illustrate the formation of spongillites and diatomites in a same basin. The present study disclosed also environmental conditions, at Phase II and IV, which were more favourable for diatoms as demonstrated by their more voluminous facies. In spite of the fact that the spongillites of the Palaeolake were distinct from other spongillite deposits in the country, the Cemit&#233;rio Palaeolake was also seen to favour the establishment of communities of sponges common to the Cerrado Biome. In this sense, the karst processes that led to the formation of small palaeo-basins in central Brazil during the Quaternary, and that are still operating, as in the current Serra Negra Lake, enabled/enable the formation of lakes under environmental conditions that have favoured the continued existence of a unique sponge community from at least 51,780 &#177; 400 <sup>14</sup>C yr BP.</p></sec><sec id="s8"><title>Acknowledgements</title><p>V. S. Machado acknowledges the Brazilian Research Council “Conselho Nacional de Desenvolvimento Cient&#237;fico e Tecnol&#243;gico” (CNPq) for the Ph.D. fellowship. C. Volkmer-Ribeiro acknowledges CNPq for granting of the Universal Project (Process 481555/2009-9). R. Iannuzzi acknowledges CNPq for research fellowship granted (Process PQ305687/2010-7 and PQ309211/2013-1). The authors are indebted to an anonymous referee for the critical comments on the manuscript.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.48340-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">DE OLIVEIRA, P.E. (1992) A PALYNOLOGICAL RECORD OF LATE QUATERNARY VEGETATIONAL AND CLIMATIC CHANGE IN SOUTHEASTERN BRAZIL. PH.D. 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