<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>1647-581X</journal-id>
<journal-title><![CDATA[Comunicações Geológicas]]></journal-title>
<abbrev-journal-title><![CDATA[Comunicações Geológicas]]></abbrev-journal-title>
<issn>1647-581X</issn>
<publisher>
<publisher-name><![CDATA[LNEG - Laboratório Nacional de Energia e Geologia]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1647-581X2009000100006</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Assumptions and problems with Fe-Mg garnet - biotite diffusion based petrological cooling rates: a case study in granulites and migmatites fromcentral Ribeira Fold Belt, SE Brazil]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Santos]]></surname>
<given-names><![CDATA[T. M. Bento dos]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Munhá]]></surname>
<given-names><![CDATA[J. M. U.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Tassinari]]></surname>
<given-names><![CDATA[C. C. G.]]></given-names>
</name>
<xref ref-type="aff" rid="A03"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Fonseca]]></surname>
<given-names><![CDATA[P. E.]]></given-names>
</name>
<xref ref-type="aff" rid="A02"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,LNEG - Laboratório Nacional de Energia e Geologia  ]]></institution>
<addr-line><![CDATA[Amadora ]]></addr-line>
<country>Portugal</country>
</aff>
<aff id="A02">
<institution><![CDATA[,Universidade de Lisboa Departamento de Geologia Centro de Geologia]]></institution>
<addr-line><![CDATA[Lisboa ]]></addr-line>
<country>Portugal</country>
</aff>
<aff id="A03">
<institution><![CDATA[,Universidade de São Paulo Instituto de Geociências ]]></institution>
<addr-line><![CDATA[São Paulo ]]></addr-line>
<country>Brazil</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>00</month>
<year>2009</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>00</month>
<year>2009</year>
</pub-date>
<numero>96</numero>
<fpage>83</fpage>
<lpage>100</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://scielo.pt/scielo.php?script=sci_arttext&amp;pid=S1647-581X2009000100006&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.pt/scielo.php?script=sci_abstract&amp;pid=S1647-581X2009000100006&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://scielo.pt/scielo.php?script=sci_pdf&amp;pid=S1647-581X2009000100006&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[The São Fidelis - Santo António de Pádua sector of central Ribeira Fold Belt is mainly composed of migmatites, granulites and blastomylonites. Application of two contrasting methodologies to obtain petrological cooling rates based on Fe-Mg diffusion between garnet and respective biotite inclusions proved unfruitful. This was mainly due to: a) high dispersion of results caused by open-system behaviour; and b) narrow closure temperature variation caused by garnet reequilibration at high temperatures followed by very fast cooling. The obtained results are mainly qualitative but in broad agreement with previously obtained thermochronological results based on integration of multiple isotopic systems.]]></p></abstract>
<abstract abstract-type="short" xml:lang="pt"><p><![CDATA[O sector São Fidelis - Santo António de Pádua, pertencente à zona central da Faixa Ribeira, é fundamentalmente composto por migmatitos, granulitos e blastomilonitos. A aplicação de diferentes metodologias com o objectivo de obter taxas de arrefecimento baseadas na difusão Fe-Mg entre granada e respectivas inclusões de biotite revelou-se infrutífera. Tal deve-se fundamentalmente a: a) elevada dispersão dos resultados causada pela existência de um sistema aberto; b) estreita variação das temperaturas de fecho do sistema causada por re-homogeneização da granada a altas temperaturas seguida de arrefecimento muito rápido. Os resultados obtidos são fundamentalmente qualitativos, mas estão de acordo com resultados termocronológicos previamente obtidos baseados na integração de múltiplos sistemas isotópicos.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Petrological cooling rates]]></kwd>
<kwd lng="en"><![CDATA[Fe-Mg diffusion]]></kwd>
<kwd lng="en"><![CDATA[Ribeira Fold Belt]]></kwd>
<kwd lng="pt"><![CDATA[Taxas de arrefecimento petrológicas]]></kwd>
<kwd lng="pt"><![CDATA[Difusão Fe-Mg]]></kwd>
<kwd lng="pt"><![CDATA[Faixa Ribeira]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p><b>Assumptions and problems with Fe-Mg garnet &#8211; biotite diffusion based    petrological cooling rates: a case study in granulites and migmatites fromcentral    Ribeira Fold Belt, SE Brazil </b></p>     <p><b>T. M. Bento dos Santos*<sup>1</sup>; J. M. U. Munh&aacute;**; C. C. G. Tassinari***    &amp; P. E. Fonseca**</b></p>     <p>&nbsp;</p>      <p>* LNEG &#8211; Laboratório Nacional de Energia e Geologia, Estrada da Portela    &#8211; Zambujal &#8211; Alfragide, 2720-866 Amadora, Portugal (<sup>1</sup>Corresponding    author: <a href="mailto:telmo.santos@ineti.pt">telmo.santos@ineti.pt</a>). </p>     <p>** Centro/Departamento de Geologia, Universidade de Lisboa, Edifício C6, 3º,    Campo Grande, 1749-016 Lisboa, Portugal. <a href="mailto:jmmunha@fc.ul.pt">jmmunha@fc.ul.pt</a>;    <a href="mailto:pefonseca@fc.ul.pt">pefonseca@fc.ul.pt</a>. </p>     <p>*** Instituto de Geociências, Universidade de São Paulo, Rua do Lago, 562 &#8211;    Butantã, CEP: 05508-080, São Paulo, Brazil. <a href="mailto:ccgtassi@usp.br">ccgtassi@usp.br</a>.  </p>     <p>&nbsp;</p>      <p><i>Abstract</i></p>     <p>The São Fidelis &#8211; Santo António de Pádua sector of central Ribeira Fold    Belt is mainly composed of migmatites, granulites and blastomylonites. Application    of two contrasting methodologies to obtain petrological cooling rates based    on Fe-Mg diffusion between garnet and respective biotite inclusions proved unfruitful.    This was mainly due to: a) high dispersion of results caused by open-system    behaviour; and b) narrow closure temperature variation caused by garnet reequilibration    at high temperatures followed by very fast cooling. The obtained results are    mainly qualitative but in broad agreement with previously obtained thermochronological    results based on integration of multiple isotopic systems. </p>     <p><i>Keywords: </i>Petrological cooling rates; Fe-Mg diffusion; Ribeira Fold    Belt. </p>      ]]></body>
<body><![CDATA[<p>&nbsp;</p>      <p><i>Resumo</i></p>     <p>O sector São Fidelis &#8211; Santo António de Pádua, pertencente à zona central    da Faixa Ribeira, é fundamentalmente composto por migmatitos, granulitos e blastomilonitos.    A aplicação de diferentes metodologias com o objectivo de obter taxas de arrefecimento    baseadas na difusão Fe-Mg entre granada e respectivas inclusões de biotite revelou-se    infrutífera. Tal deve-se fundamentalmente a: a) elevada dispersão dos resultados    causada pela existência de um sistema aberto; b) estreita variação das temperaturas    de fecho do sistema causada por re-homogeneização da granada a altas temperaturas    seguida de arrefecimento muito rápido. Os resultados obtidos são fundamentalmente    qualitativos, mas estão de acordo com resultados termocronológicos previamente    obtidos baseados na integração de múltiplos sistemas isotópicos.</p>      <p><i>Palavras-chave:</i> Taxas de arrefecimento petrológicas; Difusão Fe-Mg;    Faixa Ribeira. </p>      <p>&nbsp;</p>     <p>&nbsp;</p>      <p><b>1. INTRODUCTION</b></p>      <p>Previous works in central Ribeira Fold Belt (RFB) established age constraints    for the Brasiliano orogeny and tectonic evolution of the belt (e.g.: CORDANI    <i style='mso-bidi-font-style:normal'>et a</i>l., 1973; MACHADO <i style='mso-bidi-font-style:normal'>et al</i>., 1996; SCHMITT <i style='mso-bidi-font-style:normal'>et al</i>., 2004; 2008; HEILBRON &amp; MACHADO,    2003; BENTO DOS SANTOS <i style='mso-bidi-font-style:normal'>et al</i>., 2007;    FONSECA <i style='mso-bidi-font-style:normal'>et al</i>., 2008). However, there    are few thermochronological studies (BENTO DOS SANTOS <i style='mso-bidi-font-style:normal'>et    al</i>., 2008; FONSECA <i style='mso-bidi-font-style:normal'>et al</i>., 2008; SCHMITT <i style='mso-bidi-font-style:normal'>et al</i>., 2004) that accurately depict the    geodynamic evolution and quantitatively constrain the cooling rates of central    RFB.</p>      <p>This work provides new petrological cooling rates, which can be determined from analysis of diffusional zoning in metamorphic minerals (SPEAR &amp; PARRISH, 1996). Here, petrological cooling rates based on Fe-Mg diffusion between garnet and biotite inclusions for the studied granulites and migmatites are presented. The obtained results are then compared with geochronological cooling rates previously obtained in the study area (BENTO DOS SANTOS <i style='mso-bidi-font-style:normal'>et al</i>., 2008).</p>      <p>Several authors tried to use mineral diffusion mechanisms in order to determine cooling rates (e.g.: DODSON, 1973; LASAGA <i style='mso-bidi-font-style:normal'>et al</i>., 1977; EHLERS <i style='mso-bidi-font-style:normal'>et al</i>., 1994; SPEAR &amp; PARRISH, 1996). These authors assumed that diffusion induced by compositional variation in the garnet-biotite interface is a function of Kd<sub>(</sub><sub>Mg/Fe)</sub><sup>Garnet-Biotite</sup> in response to thermal changes, such as cooling during the retrograde path. During cooling garnet is enriched in Fe/(Fe+Mg), whereas biotite inclusions become poorer. When temperature drops below closure temperature, diffusion becomes negligible. The diffusive process is limited by the rate of diffusion in garnet, because D<sub>Fe/Mg</sub><sup>Biotite</sup><sup> </sup>&gt;&gt; D<sub>Fe/Mg</sub><sup>Garnet</sup> and mass balance determines that diffusive flows (rate of cation transfer in the mineral interface) between garnet and biotite must be the same. Therefore, Fe/(Fe+Mg) variations will be a functionof biotite inclusion size or garnet/biotite proportion. This implies that Fe/(Fe+Mg) results in garnet and biotite inclusions can be transformed in its respective apparent closure temperature and cooling rates can be obtained (Fig. 1). The used methodologies only consider diffusion between garnet and respective biotite inclusions and exclude garnet &#8211; matrix biotite interface diffusive processes, because it is very likely that the latter had open-system behaviour. Besides, most matrix biotite is affected or was formed by net-transfer reactions that include consumption of garnet rims. Therefore, it is unreasonable to use garnet and matrix biotites to model cation diffusion based petrological cooling rates.</p>      ]]></body>
<body><![CDATA[<p>&nbsp;</p>      <p><img src="/img/revistas/cg/n96/n96a06f1.jpg" width="568" height="496"></p>      
<p>Fig. 1 &#8211; Schematics showing how composition of biotite inclusions are    dependent of respective size and how their Fe/Mg composition can be transformed    in petrological cooling rates using the SPEAR &amp; PARRISH (1996) methodology.    Garnet&#8217;s core composition is used with the FERRY &amp; SPEAR (1978) thermometer    in order to obtain apparent closure temperatures. CHAKRABORTY &amp; GANGULLY    (1992) &#8211; C&amp;G (1992) &#8211; diffusion coefficients are used to depict    the petrological cooling rates. In this example, cooling rates range from 1    &#8211; 1000ºC/Ma (modified from SPEAR &amp; PARRISH, 1996).</p>      <p>&nbsp;</p>     <p>This work explores the referred assumptions that allow petrological cooling    rates to be applied to natural systems, as well as the potential pitfalls regarding    these methodologies, namely the difficulty in assuring that open-system behaviour    did not take place in complex orogenic belts, such as the RFB. Therefore, this    article is a critic work to the applied methodologies and also a first attempt    to constrain petrological cooling rates in the RFB.</p>     <p>&nbsp;</p>        <p><b>2. GEOLOGICALSETTING AND FIELD OBSERVATIONS </b></p>      <p>The RFB extends over 1,500 km along the SE Brazilian coast from southern Bahia State to Uruguay, through Espírito Santo, Rio de Janeiro, Minas Gerais, São Paulo and Paraná States (CORDANI, 1971). The RFB is a NE-SW trending (south and central sectors) and NNE-SSW trending (northern sector) Neoproterozoic mobile belt (CORDANI <i>et al</i>., 1973) formed during the Brasiliano Orogeny as outcome of the collision between the São Francisco and West Congo cratons, from which resulted Western Gondwana at around 670 &#8211; 480 Ma ago (TROUW <i>et. al</i>., 2000; SCHMITT <i>et al</i>., 2008) (Fig. 2a). </p>      <p>&nbsp;</p>      <p><img src="/img/revistas/cg/n96/n96a06f2.jpg" width="492" height="350"></p>      
]]></body>
<body><![CDATA[<p><a href="#f2">Fig. 2</a><a name="topf2"></a> &#8211;a) Central Ribeira Fold    Belt (square) in the Western Gondwana amalgamation context (modified from TROUW    <i>et al</i>., 2000). SF: São Francisco Craton; Co: Congo Craton; further abbreviations    as in TROUW <i>et al. </i>(2000); b) Main regional structures from Central Ribeira    Fold Belt and the Além Paraíba &#8211; Pádua Shear system (Modified from VAUCHEZ    <i>et al.</i>, 1994).</p>      <p>&nbsp;</p>     <p>The RFB constitutes a very complex orogenic zone composed of several geological    units, commonly separated by deep dextral shears, being the studied São Fidelis    &#8211; Santo António de Pádua (SFSAP) sector located inside the Além Paraíba    &#8211; Santo António de Pádua Shear (APPS) system (Fig. 2b). This megashear    system deformed the area rocks imposing a NE trending transpressive shear deformation    (FONSECA <i>et al</i>., 2008) associated with long-term HT/LP metamorphism (BENTO    DOS SANTOS <i>et al</i>., 2008). </p>     <p>According to TROUW <i>et al</i>. (2000), the RFB can be divided in four major    lithologic associations: a) reworked Archean to Paleoproterozoic basement rocks    composed of metavolcanic-sedimentary sequences, granodioritic orthogneisses    and intermediate granulites; b) a deformed meta-sedimentary sequence composed    of pelitic schists and high grade migmatitic paragneisses with quartzite, calc-silicate    and amphibolite intercalations; c) molasic sedimentary basins; and d) widespread    granitoid intrusive bodies with different tectonic settings, from pre-to post-collision    stages of the Brasiliano orogenic system (CAMPOS NETO &amp; FIGUEIREDO, 1995;    TROUW <i>et. al</i>., 2000; PEDROSA SOARES &amp; WIEDMANN-LEONARDOS, 2000).  </p>     <p>HEILBRON &amp; MACHADO (2003) and VALLADARES <i>et al</i>. (2008) divided the    central RFB into four tecto-nic/lithologic/geochronological domains as <i>klippen</i><i>    </i>thrusted against the São Francisco Craton. According to these authors, the    central sector of RFB includes from NW to SE: a) the Occidental Domain, a pre-1.8    Ga passive margin succession, considered to be the reworked margin of the São    Francisco Craton (basement rocks); b) the Paraíba do Sul <i>klippe</i>, composed    of amphibolite facies orthogneisses and meta-sediments; c) the Oriental Domain,    comprising the Rio Negro Magmatic arc (TUPINAMBÁ, 1999) and fore-arc and back-arc    meta-sedimentary sequences; and d) the Cabo Frio Terrane (SCHMITT <i>et al</i>.,    2008), an allochthonous terrane belonging to the West Congo Craton.</p>     <p>Regarding the RFB tectonic evolution, a dominant ensialic evolution with important crustal reworking has been favoured (CORDANI <i>et al</i>., 1973), although subordinated oceanic crust subduction (and obduction) and continental accretion have also been considered (PEDROSA SOARES &amp; WIEDMANN-LEONARDOS, 2000; PEDROSA SOARES <i>et al</i>., 2001). Within the central part of the belt, in the Rio de Janeiro state, HEILBRON <i>et al</i>. (1993) and MACHADO <i>et al</i>. (1996) proposed that the tectonometamorphic evolution of the Brasiliano Orogeny should be divided in: a) collision period (590 &#8211; 563 Ma) in which occurred the main deformation phases and metamorphism, with reworking and partial melting of older continental basement rocks and emplacement of several granitoid bodies; b) post-collision period at 535 &#8211; 520 Ma, corresponding to major dextral shear zones and retrograde metamorphism; c) post-tectonic period of orogenic collapse with emplacement of late granitic plutons at 490 Ma ago (BENTO DOS SANTOS <i>et al</i>., 2007). </p>      <p>The studied area, the SFSAP sector, is located in the central-north part of    the RFB in northern Rio de Janeiro State (SE Brazil) and SE to the APPS main    shear (near Santo António de Pádua) (<a href="#topf2">Fig. 2</a><a name="f2"></a>    and 3). The SFSAP sector underwent complex polyphase ductile deformation, with    thrusting dominantly to ESE, followed by NNE-SSW sub-horizontal dextral shearing    that produced the elongated mineral fabric observed in the studied rocks (BASCOU    <i>et al</i>., 2002; FONSECA <i>et al</i>., 2008). In the studied area three    main deformation phases can be observed. As outlined by FONSECA <i>et al</i>.    (2008), the earliest deformation event (D<sub>1</sub>) corresponds to high temperature    (ductile) thrusts (250°, 55-70° NW), that were mostly erased by the main syn-    to post-metamorphic peak D<sub>2 </sub>event. This corresponds to the dextral    megashear APPS system (50-65°, 70-85° NW). Finally, a D<sub>3 </sub>fragile/brittle    event is simultaneous with reactivation of D<sub>2 </sub>conjugated fault systems    (290-320°, subvertical). </p>      <p>&nbsp;</p>      <p><img src="/img/revistas/cg/n96/n96a06f3.jpg" width="545" height="339"></p>      
<p>Fig. 3 &#8211;a) Location of the studied São Fidelis &#8211; Santo António de Pádua sector in central Ribeira Fold Belt, northern Rio de Janeiro State, SE Brazil (Modified from TROUW <i>et al.</i>, 2000; HEILBRON &amp; MACHADO, 2003). Lithologic domains are presented as in HEILBRON &amp; MACHADO, 2003; b) Simplified geological map of the São Fidelis &#8211; Santo António de Pádua sector showing the main lithologic units and structures present.</p>      ]]></body>
<body><![CDATA[<p>&nbsp;</p>     <p>Intense granulite facies metamorphism produced generalized migmatization and    granitoid production by partial melting of paragneisses. Outcrops in the area    comprise the referred migmatites, granulites and blastomylonites that resulted    from late retrogression of the other rock types. Migmatites (Fig. 4a-b) show    a clear separation of gneissic paleosome and aplitic or pegmatitic neosome (Migmatite    terminology as recommended by WIMMENAUER &amp; BRYHNI, 2007).</p>      <p>&nbsp;</p>      <p><img src="/img/revistas/cg/n96/n96a06f4.jpg" width="553" height="429"></p>      
<p>Fig. 4 &#8211;a) Garnet migmatites with clear separation of gneissic paleosome    and aplitic neosome. b) Homogeneous undeformed migmatites with granitic/diatexitic    aspect. c) Elongated granulite massif (circle evidences a person for scale purposes).    d) Blastomylonitic occurrence with plagioclase neoblasts. </p>      <p>&nbsp;</p>     <p>These rocks present gneissic foliation and banding, as well as clear evidences    of late deformation and retrogression. These are associated with large elongated    or rounded, undeformed and homogeneous granitic to migmatitic batholiths (diatexites),    that represent a more advanced stage of anatexis of the migmatites. Marbles    are occasionally interlayered in the migmatites as decametric to kilometric    thick bands or small metric pockets. In the study area, granulites range from    charnockites (s. s.) (Fig. 4c) to enderbites (basic granulites) that crop out    as elongated NE-SW trending massifs and are overthrusted onto the migmatites    during D<sub>2 </sub>and D<sub>3 </sub>deformation phases (FONSECA <i>et al</i>.,    2008). </p>     <p>Blastomylonites resulted from the deformation and retrogression of the other    rock types in areas closer to the APPS main shears (Fig. 4d). They represent    the deformed and retrogressed equivalents of the granulites (mainly) and of    the migmatites.</p>     <p>&nbsp;</p>     <p><b>3. PETROGRAPHY</b></p>     ]]></body>
<body><![CDATA[<p>Petrographic observations and a mineral chemistry synthesis for the studied    rocks are provided in this section with the exception of garnet and biotite    mineral chemistry that will be provided with more detail below. </p>     <p><b>3.1. Migmatites</b></p>     <p>Paleosome commonly comprises a g + bi + q + pl (X<sub>an</sub> = 0.26 &#8211;    0.43; X<sub>or</sub> = 0.01 &#8211; 0.04) + ksp (X<sub>ab</sub> &lt; 0.1; X<sub>an</sub>    &lt; 0.01) ± mt ± sill ± ilm (Mineral abbreviations according to POWELL &amp;    HOLLAND, 1999) gneissic association, whereas the neosomatic fraction consists    of a g + bi + pl (X<sub>an</sub>= 0.27 &#8211; 0.42; X<sub>or</sub>= 0.01 &#8211;    0.04) + q + ksp (X<sub>ab</sub> &lt; 0.1; X<sub>an</sub> &lt; 0.01) ± sill ±    ap mineral association (Fig. 5a). Migmatites do not show significant compositional    difference between paleosome and neosome, including for garnets and biotites    (see below). The granolepidoblastic texture present in both paleosome and neosome,    largely defined by the biotite + quartz association, is commonly obliterated    by coarse grained, sometimes centimetric, subhedral or rounded poikiloblastic    garnet, plagioclase and K-feldspar granoblasts. They frequently have matrix    mineral inclusions, such as biotite, quartz and magnetite. These megablasts    are usually deformed, bent or cracked and show recrystallized rims. The garnet    &#8211; plagioclase &#8211; K-feldspar granoblastic assemblage represents the    metamorphic peak paragenesis of the migmatites, possibly with small amounts    of quartz and residual biotite. </p>     <p>&nbsp;</p>     <p><a name="f5"></a></p>          <p><img src="/img/revistas/cg/n96/n96a06f5.jpg" width="539" height="608"></p>      
<p><a href="#topf5">Fig. 5</a> &#8211; Petrographic observations of the studied    rocks: a) Migmatite paleosome with a garnet megablast surrounded by a granolepidoblastic    matrix. b) Deformed and sheared migmatite neosome with retrogressed biotite    + quartz + sillimanite assemblage. c) Isotropic granulites showing an orthopyroxene    megablast surrounded by late biotite. d) Deformed and sheared granulites showing    fine grained mylonitic granolepidoblastic texture. e) Coarse grained enderbite    with some amphibolitization of the peak garnet + clinopyroxene assemblage. f)    Profuse equigranular mylonitic texture with abundant finely recrystallized mineral    grains in blastomylonites. </p>      <p>&nbsp;</p>     <p>The presence of biotite and sillimanite at garnet rims is a clear evidence    of retrogression by garnet consumption. Symplectitic biotite + quartz + sillimanite    growth after garnet is a common feature of these rocks. In some cases, these    migmatites are intensively sheared, originating a fine grained mylonitic banding    with abundant sillimanite (<a name="topf5"></a><a href="#f5">Fig. 5b</a>). </p>     <p><b>3.2. Granulites </b></p>     ]]></body>
<body><![CDATA[<p>Isotropic charnockites (s. s.) show a medium to coarse sized granoblastic texture    with megablastic (sometimes centimetric) subhedral g + pl (X<sub>an</sub><sub>    </sub>= 0.29 &#8211; 0.51; X<sub>or</sub><sub> </sub>= 0 &#8211; 0.03) + ksp    (X<sub>ab</sub><sub> </sub>&lt; 0.1 and X<sub>an</sub><sub> </sub>&lt; 0.01)    + opx (X<sub>en</sub><sub> </sub>= 0.39 &#8211; 0.48; X<sub>wo</sub><sub> </sub>&lt;    0.03) assemblage. Bi + q + mt + ilm + ap + zrc are only present as diffuse,    rarely orientated, matrix minerals (<a name="topf5"></a><a href="#f5">Fig. 5c</a>). Biotites are frequently included    in garnet and rarely in orthopyroxene mega-blasts. Bi + q symplectites are common    around garnet and pyroxene rims, revealing that the retrometamorphic path involved    significant deformation with decompression. </p>     <p>Some granulites are extensively sheared and retrogressed, showing a fine grained    mylonitic or cataclastic texture with g + bi + pl + q + ksp + opx (relic) ±    ap ± hb (X<sub>Mg</sub><sub> </sub>= 0.35 &#8211; 0.65) mineral assemblage (<a name="topf5"></a><a href="#f5">Fig.    5d</a>). Metamorphic peak minerals (pl + ksp + q + opx + g) are intensively deformed,    fractured, grinded and replaced by an amphibolite facies assemblage of bi +    hb. </p>     <p>Enderbites are banded, medium to coarse grained and have a subhedral g + pl    (X<sub>an</sub><sub> </sub>= 0.29 &#8211; 0.51; X<sub>or</sub><sub> </sub>=    0 &#8211; 0.03) + opx (X<sub>en</sub><sub> </sub>= 0.41 &#8211; 0.44; X<sub>wo</sub><sub>    </sub>&lt; 0.02) + cpx (X<sub>en</sub><sub> </sub>= 0.30 &#8211; 0.35; X<sub>wo</sub><sub>    </sub>= 0.42 &#8211; 0.48) metamorphic peak paragenesis. This assemblage is    often replaced by the hb (X<sub>Mg</sub><sub> </sub>= 0.35 &#8211; 0.65) + pl    (X<sub>an</sub><sub> </sub>= 0.29 &#8211; 42; X<sub>or</sub><sub> </sub>= 0    &#8211; 0.03) ± bi amphibolite facies assemblage (<a name="topf5"></a><a href="#f5">Fig. 5e</a>).</p>     <p><b>3.3. Blastomylonites </b></p>     <p>Migmatites and granulites are profusely deformed and retrogressed in the near    region of Santo António de Pádua, centre of the APPS system. There, it is very    difficult to determine if the observed rocks were granulites or migmatites because    of the blastomylonitic transformation they experienced. Therefore, the broad    term blastomylonite is employed. </p>     <p>Petrographic features indicate that they are equivalent to their undeformed    counterparts, with the exception of having a profuse equigranular mylonitic    texture and finely recrystallized mineral grains (<a name="topf5"></a><a href="#f5">Fig.    5f</a>). Mineralogical replacement of metamorphic peak assemblage progresses    in the same way as previously stated for migmatites and granulites, but in blastomylonites    there are only remnants of the high grade paragenesis. Therefore, the typical    mineral assemblage of blastomylonites is pl (X<sub>an</sub>= 0.17 &#8211; 0.55;    X<sub>or</sub>= 0.01 &#8211; 0.02) + bi + q + ksp (X<sub>ab</sub><sub> </sub>&lt;    0.22; X<sub>an</sub><sub> </sub>&lt; 0.01) with some small relics of the high    temperature minerals, such as garnet, orthopyroxene (X<sub>en</sub><sub> </sub>=    0.41 &#8211; 0.44; X<sub>wo</sub><sub> </sub>&lt; 0.02) or clinopyroxene (X<sub>en</sub><sub>    </sub>= 0.30 &#8211; 0.35; X<sub>wo</sub><sub> </sub>= 0.42 &#8211; 0.48).</p>     <p>&nbsp;</p>     <p><b>4. GARNET AND BIOTITE MINERAL CHEMISTRY </b></p>     <p>Samples were prepared for the different types of analyses at the Instituto    de Geociências da Universidade de São Paulo (IGc-USP) and at the Departamento    de Geologia da Faculdade de Ciências da Universidade de Lisboa (DG-FCUL). </p>     <p>Mineral composition data were determined on carbon coated polished thin sections    using a JEOL JXA 733 wavelength dispersive Electron Microprobe, at the Centro    de Geologia da Faculdade de Ciências da Universidade de Lisboa (CeGUL). Minerals    were analysed with an acceleration voltage of 15 kV and a current of 25 nA,    using a beam of 5 mm. Both natural and synthetic silicates were used as standards.    Errors are typically below 1.5 wt% for major elements. </p>     ]]></body>
<body><![CDATA[<p>An extensive mineral chemistry study on garnets, biotite inclusions in garnets    and matrix biotites was performed in the studied rocks, namely major element    analyses of rim &#8211; core &#8211; rim (RCR) profiles in garnets and garnet    &#8211; biotite interface (GBI) profiles in garnets. These results were obtained    in granulites and in the paleosomes (mainly) of migmatites. However, no significant    compositional variation was found for paleosomes and neosomes of the migmatite    samples.</p>      <p>The following mineral chemistry data on garnets and biotites is summarized    due to the extensive number of chemical analyses performed in both garnet and    biotite (over 2500 and over 1800 analyses, respectively). Examples of RCR profiles    of the studied garnets are provided in Fig. 6 as a synthesis. GBI profiles in    garnets and summarized analyses of biotite inclusions are provided in the petrological    cooling rates section.</p>     <p>&nbsp;</p>      <p><a href="/img/revistas/cg/n96/n96a06f6.jpg" target="_blank">Fig. 6</a>    &#8211; Examples of compositional RCR profiles in garnets from migmatites (Fig.    6a-b) and granulites (Fig. 6c-d). Xalm is always plotted in the main axis (at    the left), whereas Xspss, Xpy and Xgr are plotted in the secondary axis (at    the right). Fig. 6a shows a typical zoning pattern for garnet (as described    in the text), increasing substantially the Fe/(Fe+Mg) values in the core area    due to the proximity of a biotite inclusion; Fig. 6b shows a rare RCR profile    where garnet does not present the expect results, which is probably due to garnet    consumption or some other heterogeneity; Fig. 6c shows a typical diffusive RCR    profile for garnet with a zoning pattern where Fe and Mn decreases and Mg increases    from rim to core; Fig. 6d shows the same zoning pattern, but only in one rim.  </p>      
<p>&nbsp;</p>     <p>Mineral chemistry results for blastomylonites are presented as a synthesis    in order to be compared with their undeformed equivalents. However, due to the    extensive shearing and metamorphic recrystallization that characterize these    rocks, no attempt to obtain petrological cooling rates in blastomylonites was    performed.</p>     <p><b>4.1. Garnets </b></p>     <p>Garnets are almandine-rich in all rock types, with X<sub>alm</sub> always higher    than 0.54 and always with Mg-richer cores compared to the rims. All rock types    show the same zoning pattern from core (Mg-richer) to rim (Fe-richer), but display    very different range of values, namely X<sub>alm</sub> =0.61 to 0.75 and X<sub>py</sub>    = 0.07 to 0.21 for granulites, X<sub>alm</sub> = 0.54 to 0.77 and X<sub>py</sub>    = 0.07 to 0.37 for migmatites and X<sub>alm</sub> = 0.59 to 0.77 and X<sub>py</sub>    = 0.11 to 0.19 for blastomylonites. Migmatites do not show significant compositional    difference between paleosome and neosome. They present the highest pyrope contents    and variable grossular contents ranging from X<sub>gr</sub> = 0.01 to 0.27.    Although the highest value of X<sub>gr</sub> is present in a migmatite, granulites    are normally richer in calcium, with X<sub>gr</sub> ranging from 0.02 to 0.22.    Spessartine contents are always low (normally X<sub>spss</sub> &lt; 0.1), reaching    a maximum of 0.13 in granulites and migmatites. Examples of compositional RCR    profiles of garnets from both rock types are provided in <a href="/img/revistas/cg/n96/n96a06f6.jpg" target="_blank">Fig.    6a-d</a>.</p>     
<p><b>4.2. Biotites</b></p>     <p>Granulites have matrix biotites with X<sub>Mg</sub> ranging from 0.39 to 0.55    and high TiO<sub>2</sub> contents ranging from 3.8 to 6.3 wt%. Migmatites show    a great range of X<sub>Mg</sub> contents ranging from 0.36 to Fe-poor matrix    biotites with X<sub>Mg</sub> = 0.76, whereas TiO<sub>2</sub> contents range    between 3.7 to 4.5 wt%. This X<sub>Mg</sub> range is observable in both paleosome    and neosome. Blastomylonites show X<sub>Mg</sub> values similar to granulites    (0.39 to 0.55) and TiO<sub>2</sub> contents ranging from 4.9 &#8211; 5.8 wt%.    Fe/Mg composition and size of biotite inclusions in garnet from migmatites and    granulites are synthesized in Tables 1a-f and will be further discussed below.</p>     ]]></body>
<body><![CDATA[<p>&nbsp;</p>     <p><a name="t1a"></a></p>     <p><b><a href="#topt1a">TABLE 1a</a></b></p>     <p>Garnet and respective biotite inclusions composition of migmatite 341a used    for the application of the SPEAR &amp; PARRISH (1996) method. Also present is    the dimension of each biotite inclusion and garnet&#8217;s core composition.    The latter was used together with each biotite Fe/Mg value to obtain each apparent    closure temperature using the FERRY &amp; SPEAR (1978) geothermometer.</p>     <p><img src="/img/revistas/cg/n96/n96a06t1a.jpg" width="444" height="294"></p>     
<p>&nbsp;</p>     <p><b><a href="#topt1a">TABLE 1b</a></b></p>     <p>Garnet and respective biotite inclusions composition of migmatite 13a used    for the application of the SPEAR &amp; PARRISH (1996) method. Also present is    the dimension of each biotite inclusion and garnet&#8217;s core composition.    The latter was used together with each biotite Fe/Mg value to obtain each apparent    closure temperature using the FERRY &amp; SPEAR (1978) geothermometer.</p>     <p><img src="/img/revistas/cg/n96/n96a06t1b.jpg" width="445" height="293"></p>     
<p>&nbsp;</p>     ]]></body>
<body><![CDATA[<p><b><a href="#topt1a">TABLE 1c</a></b></p>     <p>Garnet and respective biotite inclusions composition of granulite 24E-1 used    for the application of the SPEAR &amp; PARRISH (1996) method. Also present is    the dimension of each biotite inclusion and garnet&#8217;s core composition.    The latter was used together with each biotite Fe/Mg value to obtain each apparent    closure temperature using the FERRY &amp; SPEAR (1978) geothermometer.</p>     <p><img src="/img/revistas/cg/n96/n96a06t1c.jpg" width="390" height="323"></p>     
<p>&nbsp;</p>     <p><b><a href="#topt1a">TABLE 1d</a></b></p>     <p>Garnet and respective biotite inclusions composition of granulite 24E-2 used    for the application of the SPEAR &amp; PARRISH (1996) method. Also present is    the dimension of each biotite inclusion and garnet&#8217;s core composition.    The latter was used together with each biotite Fe/Mg value to obtain each apparent    closure temperature using the FERRY &amp; SPEAR (1978) geothermometer.</p>     <p><img src="/img/revistas/cg/n96/n96a06t1d.jpg" width="395" height="304"></p>     
<p>&nbsp;</p>     <p><b><a href="#topt1a">TABLE 1e</a></b></p>     <p>Garnet and respective biotite inclusions composition of granulite 36Cb-1 used    for the application of the SPEAR &amp; PARRISH (1996) method. Also present is    the dimension of each biotite inclusion and garnet&#8217;s core composition.    The latter was used together with each biotite Fe/Mg value to obtain each apparent    closure temperature using the FERRY &amp; SPEAR (1978) geothermometer.</p>     ]]></body>
<body><![CDATA[<p><img src="/img/revistas/cg/n96/n96a06t1e.jpg" width="395" height="304"></p>     
<p>&nbsp; </p>     <p><b><a href="#topt1a">TABLE 1f</a></b></p>     <p>Garnet and respective biotite inclusions composition of granulite 222-2 used    for the application of the SPEAR &amp; PARRISH (1996) method. Also present is    the dimension of each biotite inclusion and garnet&#8217;s core composition.    The latter was used together with each biotite Fe/Mg value to obtain each apparent    closure temperature using the FERRY &amp; SPEAR (1978) geothermometer.</p>     <p><img src="/img/revistas/cg/n96/n96a06t1f.jpg" width="388" height="268"></p>     
<p>&nbsp;</p>      <p><b>5. PETROLOGICALCOOLING RATES </b></p>     <p>As previously referred, diffusion induced by compositional variation in the    garnet-biotite interface is a function of Kd<sub>(</sub><sub>Mg/Fe)Garnet-Biotite</sub>    in response to thermal changes, such as cooling during retrograde path. Fe/(Fe+Mg)    results in garnet and biotite inclusions can thus be transformed in its respective    closure temperature (Tc) and converted in terms of thermochronological evolution    by obtaining cooling rates. </p>     <p>This work uses two significantly different methodologies that relies on Fe-Mg    exchange between garnet and biotite inclusions: a) the method proposed by SPEAR    &amp; PARRISH (1996), based on Fe-Mg exchange modelling between a garnet megablast    and its corresponding biotite inclusions; b) the method proposed by GANGULLY    <i style='mso-bidi-font-style:normal'>et al</i>. (1998) that uses garnet compositional    profiles near the garnet/biotite inclusion interface in order to infer metamorphic    cooling rates. These methods are relatively recent but have been applied successfully    in other orogenic belts (e.g.: SPEAR &amp; PARRISH, 1996; MUNHÁ <i style='mso-bidi-font-style:normal'>et al</i>., 2005; STORM &amp; SPEAR, 2005).</p>     <p><b>5.1. The S</b><b>PEAR </b><b>&amp; P</b><b>ARRISH </b><b>(1996) method </b></p>     ]]></body>
<body><![CDATA[<p>This method is based on Fe-Mg exchange modelling between a garnet megablast    and its corresponding biotite inclusions. Fe/(Fe+Mg) variations will be a function    of biotite inclusions size if diffusion is exclusive between garnet and the    several biotites included. This will produce larger compositional variations    in smaller biotite inclusions. Therefore, Fe/(Fe+Mg) in each inclusion can be    transformed in its respective apparent closure temperature using the garnet&#8217;s    core composition and the FERRY &amp; SPEAR (1978) thermometer (Tab. 1a-f). Cooling    rates are obtained using the diffusion coefficients of CHAKRABORTY &amp; GANGULLY    (1992), as shown in Fig. 7 and 8. </p>     <p>&nbsp;</p>     <p><img src="/img/revistas/cg/n96/n96a06f7.jpg" width="663" height="591"></p>      
<p>Fig. 7 &#8211; Examples of analysed biotite inclusions Fe/Mg results correlated    with respective inclusions size for migmatites (Fig. 7c; 7e) and granulites    (Fig. 7a; 7b; 7d; 7f). It is possible to observe that some present very high    dispersion of results whereas some show a good correlation between Fe/Mg and    biotite dimension.</p>     <p>&nbsp;</p>      <p><a name="f8"></a></p>     <p><img src="/img/revistas/cg/n96/n96a06f8.jpg" width="611" height="632"></p>     
<p><a href="#topf8">Fig. 8</a> &#8211; Examples of petrological cooling rates    for the studied migmatites (Fig. 8c; 8e) and granulites (Fig. 8a; 8b; 8d; 8f).    Samples are displayed in the same order as in Fig. 7. Some samples show a great    dispersion of results, making it impossible to accurately depict any trend for    cooling rates (Fig. 8a-c), whereas others show a very narrow closure temperature    variation (Fig. 8d-f), suggesting homogenized Fe/Mg values. Apparent closure    temperatures vs. biotite dimensions are plotted with the CHAKRABORTY &amp; GANGULLY    (1992) diffusion coefficients. Cooling rates are presented in ºC/Ma. </p>     <p>&nbsp;</p>      <p>Fig. 7 shows that some Fe/Mg results are indeed correlated with biotite inclusions    size, providing trends for some migmatites and granulites, whereas others provide    significant dispersion and no correlation. However, samples that provide correlation    trends between Fe/Mg results and biotite inclusions size are not significantly    different in Fe/Mg contents, having Fe/Mg variation &lt; 0.2, in most cases    (<a name="topt1a"></a><a href="#t1a">Table 1a-f</a>). This is problematic, since    small amplitudes in Fe/Mg of biotite inclusions provide a very narrow variation    for apparent closure temperatures, as can be seen in <a href="#t1a">Table 1</a>    and Fig. 8. </p>     ]]></body>
<body><![CDATA[<p>The several petrological cooling rates plots, summarized in Fig. 8, allow us    to state that samples that show high Fe/Mg dispersion, also show significant    closure temperature dispersion (Fig. 8 a-c) with cooling rates spanning from    0.1 to 200°C/Ma, whereas samples that show very narrow Fe/Mg variation provide    flat closure temperature patterns (Fig. 8 d-f) with cooling rates spanning from    1 to 200ºC/Ma.</p>     <p>&nbsp;</p>     <p><b>5.2. The GANGULLY <i>et al</i>. (1998) method </b></p>     <p>Another attempt to obtain petrologic cooling rates with compositional Fe-Mg diffusion between garnet and biotite was performed by using the GANGULLY <i>et al</i>. (1998) method. It consists in modelling the variation of garnet&#8217;s composition in the interface with a biotite inclusion, from the biotite/garnet interface to an area of the garnet that is far enough from the compositional effect caused by the biotite inclusion, i.e. the <i>plateau </i>composition of garnet. This method is significantly opposed to the previous one because it does not use the compositional variation of biotite inclusions, but the compositional variation of garnet around the biotite inclusion. For this second method we used the software &#8220;GARBIDIF&#8221; developed by MUNHÁ (personal communication) and the garnet Fe-Mg diffusion parameters of GANGULLY <i>et al</i>. (1998).</p>      <p>AGBI compositional profile was obtained for granulite 153c and migmatite 73A    (Tab. 2 a-b; Fig. 9-10) around the respective biotite inclusions. However, the    granulite garnet shows no Fe/(Fe/Mg) zoning in the interface with the biotite    inclusion, even with a minimum distance of analyse to the garnet &#8211; biotite    interface being 5 mm (Fig. 9). Migmatite 73A GBI profile shows 220 mm size Fe/(Fe/Mg)    zoning in the interface with the biotite inclusion (Fig. 10). This will be discussed    in the following section.</p>     <p>&nbsp;</p>      <p><a name="f9"></a></p>      <p><img src="/img/revistas/cg/n96/n96a06f9.jpg" width="480" height="304"></p>      
<p><a href="#topf9">Fig. 9</a> &#8211;GBI compositional profile of garnet with    no zoning pattern from near the biotite inclusion (at the left) to garnet core    (at the right) in granulite 153c. Minimum analysed distance to interface is    5 µm. Xalm is plotted in the main axis (at the left), whereas Xspss, Xpy and    Xgr are plotted in the secondary axis (at the right).</p>     <p>&nbsp;</p>      ]]></body>
<body><![CDATA[<p><a name="f10"></a></p>     <p><img src="/img/revistas/cg/n96/n96a06f10.jpg" width="514" height="322"></p>     
<p><a href="#topf10">Fig. 10</a> &#8211; Zoned GBI compositional profile of the    studied garnet in migmatite 73A, as explained in the text.</p>      <p>&nbsp;</p>     <p><b>6. DISCUSSION</b></p>     <p>The results obtained with the SPEAR &amp; PARRISH (1996) method are very difficult    to interpret both for granulites and migmatites, because biotite dimension (logarithmic)    vs. garnet &#8211; biotite apparent closure temperatures show very high dispersion    of results. It is, therefore, impossible to discriminate a cooling rates trend    (<a name="topf8"></a><a href="#f8">Fig. 8</a>). Other samples (<a href="#f8">Fig.    8</a> d-f) show a very low range of apparent closure temperatures for biotites    that are very different in terms of size. This suggests that garnet and its    biotite inclusions must have been reequilibrated (re-homogenized) at high temperatures    and then cooled very fast, inhibiting significant change in the Fe/Mg of biotite    inclusions, and consequently, in the apparent temperatures. In both cases, important    assumptions for the application of this method were not maintained: cationic    exchange with mass balance preservation between garnet and biotite inclusions    (i.e. close system behaviour) and/or sufficiently discriminating Fe/Mg variation    in biotite inclusions correlated with respective size. Therefore, although this    methodology provided some insights regarding the general trends for cooling    patterns, it did not constrain accurately the cooling rates of the studied rocks.</p>     <p>&nbsp;</p>     <p><b>TABLE 2a</b></p>     <p>GBI profile of granulite 153c used in the application of the GANGULLY et al.    (1998) method. Also present is the distance of the analysed garnet to the garnet-biotite    inclusion interface. Fe/(Fe/Mg) variation is reduced, spanning from 0.825 to    0.808, suggesting that no Fe/(Fe/Mg) diffusion occurred in the garnet &#8211;    biotite interface.</p>     <p><img src="/img/revistas/cg/n96/n96a06t2a.jpg" width="332" height="587"></p>     
]]></body>
<body><![CDATA[<p>&nbsp;</p>     <p><b>TABLE 2b</b></p>     <p>GBI profile of migmatite 73A used in the application of the GANGULLY et al.    (1998) method. Also present is the distance of the analysed garnet to the garnet-biotite    inclusion interface. Fe/(Fe/Mg) variation is significant, spanning from 0.676    to 0.623, suggesting that Fe/(Fe/Mg) diffusion in the garnet &#8211; biotite    interface occurred.</p>     <p><img src="/img/revistas/cg/n96/n96a06t2b.jpg" width="310" height="589"></p>     
<p>&nbsp;</p>     <p>The obtained compositional profiles using the GANGULLY <i>et al</i>. (1998)    method also provided unsatisfactory results, since granulite 153c shows no type    of Fe/(Fe/Mg) garnet zoning in the interface with the biotite inclusion (<a name="topf9"></a><a href="#f9">Fig.    9</a>). This implies that garnet was equilibrated with a significant amount    of biotite at high temperatures, followed by very fast cooling that did not    allow the formation of any type of zoning pattern (minimum distance of the analyses    to the garnet &#8211; biotite interface is 5 mm). This hampers any type of inference    regarding petrological cooling rates. However, it is possible to conclude (qualitatively)    that it must have been high temperature maintenance for a substantial amount    of time (that allowed for the garnet to be homogenized), followed by a period    of very fast cooling rates, as evidenced in samples 36Cb-1, 341a and 222-2 (<a href="#f8">Fig.    8</a> d-f). This is in overall agreement with geochronological cooling rates    provided by BENTO DOS SANTOS <i>et al</i>. (2008) (see below). </p>     <p>Migmatite 73A garnet compositional profile (<a name="topf10"></a><a href="#f10">Fig.    10</a>) in the interface with the biotite inclusion is significantly opposed    to the previous one, because it presents a pronounced zoning pattern from Fe/(Fe+Mg)    higher values close to the biotite to more Mg-rich values far from the interface    with the biotite inclusion. </p>     <p>The profile is divided in three parts (as evidenced in <a href="#f10">Fig.    10</a>): zone 1 (far from the biotite inclusion) shows plateau values (Fe/(Fe+Mg)    = 0.623 &#8211; 0.629; average Fe/(Fe+Mg) = 0.6261), equivalent with the garnet&#8217;s    core composition far from the inclusions (compare with Fig. 11 that shows the    RCR profile for the referred garnet; average core Fe/(Fe+Mg) = 0.628). This    area of the profile is absent of Fe-Mg cation exchange between the garnet and    the inclusion, i.e. there is preservation of garnet&#8217;s initial composition;    zone 2 shows an apparent arithmetic increase of Fe/(Fe + Mg) values according    with proximity to the biotite inclusion; and, finally, zone 3 shows an exponential    Fe/(Fe + Mg) increase with proximity to the biotite inclusion. </p>     <p>&nbsp;</p>      <p><img src="/img/revistas/cg/n96/n96a06f11.jpg" width="522" height="325"></p>      
]]></body>
<body><![CDATA[<p>Fig. 11 &#8211; RCR compositional profile of the studied garnet in migmatite 73A. X<sub>alm</sub> and X<sub>py</sub> are plotted in the main axis (at the left), whereas X<sub>spss</sub> and X<sub>gr</sub> are plotted in the secondary axis (at the right). This garnet does not show a typical RCR zoning pattern, because the left rim shows plateau values, probably due to retrograde consumption of garnet.</p>      <p>&nbsp;</p>      <p>Modelling for this compositional profile is based on the assumption that Fe-Mg cationic exchange between garnet and corresponding biotite inclusion is exclusive and that mass balance preservation between both minerals occurred. Therefore, the effective dimensions of each mineral were used (garnet radius (R<sub>Garnet</sub><sub>) </sub>is 1 mm and the average biotite dimension (R<sub>Biotite</sub>) is 0.1 mm) at different cooling rates. The other diffusive parameters used were D<sub>Fe/Mg</sub><sup>Biotite</sup><sup> </sup>= 100D<sub>Fe/Mg</sub><sup>Garnet</sup>; Initial Temperature (T<sub>i</sub>) = 800°C and Initial Pressure (Pi) = 8 kbar (BENTO DOS SANTOS, 2008; MUNHÁ <i>et al</i>., 2008); Fe/(Fe+Mg)<sub>i</sub><sup>Garnet</sup><sup> </sup>= 0.6261).</p>      <p>After performing several modelling with different cooling rates from 5 to 200°C/Ma (Fig. 12), it became evident that it was impossible to adequately adjust any cooling rate pattern to the obtained compositional profile, especially in zone 2. The mentioned modelling, besides not adjusting adequately to the profile, apparently would imply the possibility of having cooling rates so disparate as 5 and 200°C/Ma (Fig. 12).</p>      <p>&nbsp;</p>      <p><img src="/img/revistas/cg/n96/n96a06f12.jpg" width="494" height="306"></p>      
<p>Fig. 12 &#8211; Zoned compositional profile of garnet from migmatite 73A (as    in <a href="#f10">Fig. 10</a>) plotted with the different modelling results    at different cooling rates, based on the assumption that garnet &#8211; biotite    inclusion cationic diffusion is exclusive. As can be seen, the GBI profile is    only adequate in zone 3, near the biotite inclusion, implying the possibility    of having cooling rates as different as 5 and 200ºC/Ma.</p>      <p>&nbsp;</p>     <p>The fact that none of the obtained modelling is adjustable to the GBI profile    and because zone 2 presents arithmetic increase, suggests the existence of non-exclusivity    of diffusive processes between garnet and biotite inclusion. Hardly, such a    small inclusion of biotite (0.1 mm radius) could cause such a significant increase    in Fe/(Fe+Mg) in a part of the garnet so far away from the interface (220 mm),    even with very low cooling rates. Therefore, it is suggested that garnet may    have not maintained equilibrium exclusively with the referred biotite inclusion    during an early period of its cooling. This must have been caused by retrograde    reaction processes (SPEAR &amp; FLORENCE, 1992; KOHN &amp; SPEAR, 2000) with    a large amount of biotite, such as matrix biotite. Modelling performed with    similar amounts of garnet and biotite (R<sub>Garnet</sub> = 1mm; R<sub>Biotite</sub>    = 1mm; D<sub>Fe/Mg</sub><sup>Biotite</sup> = 100D<sub>Fe/Mg</sub><sup>Garnet</sup>;    T<sub>i</sub> = 800°C; Pi = 8 kbar; Fe/(Fe+Mg)<sub>I</sub><sup>Garnet</sup>    = 0.6261) at different cooling rates (Fig. 13) show very reasonable adjustment    to zones 1 and 2, suggesting initial very high cooling rates (50 to 200°C/Ma),    but a pronounced difference to the compositional profile in zone 3.</p>     <p>&nbsp;</p>      ]]></body>
<body><![CDATA[<p><img src="/img/revistas/cg/n96/n96a06f13.jpg" width="499" height="307"></p>      
<p>Fig. 13 &#8211; Zoned compositional profile of garnet from migmatite 73A (as    in <a href="#f10">Fig. 10</a>) plotted with the different modelling results    at different cooling rates, based on the assumption that garnet was in equilibrium    with reasonable amounts of matrix biotite. As can be seen, the GBI profile is    only adequate to zones 1 and 2 (far from the biotite inclusion) implying very    high cooling rates from 50 to 200ºC/Ma.</p>      <p>&nbsp;</p>     <p>Thus, migmatite 73A must have had a very complex cooling pattern during which    remained in equilibrium with a biotite reservoir such as available matrix biotite    (in an early period when biotite was very abundant or when garnet had smaller    dimensions than presently) at high cooling rates. This was probably followed    by a period when garnet must have been in exclusive equilibrium with its biotite    inclusion at lower temperatures. However, the aforementioned cooling pattern,    inferred by combining the two modelling with different garnet/biotite volume    proportions, cannot simply be put together to infer a coherent cooling pattern,    because the kinetics of garnet-biotite diffusion of each step is nonreproducible.    This was confirmed when several modelling were performed by combining a first    non-diffusive (open-system behaviour) followed by a purely diffusive (closed-system    behaviour) Fe-Mg exchange between garnet and biotite. No modelling provided    reasonable results compatible with the obtained garnet compositional profile    near the biotite inclusion.</p>      <p>It can be concluded, after the use of two significantly different methodologies to obtain petrological cooling rates, that there was not exclusivity of mass balanced diffusive processes between the studied garnets and respective biotite inclusions. The system was opened to reaction processes with the rock&#8217;s matrix, which increases the difficulty of using these methodologies. Therefore, the existence of non-diffusive processes in garnet, as well as the possibility of plastic deformation of garnet at high temperatures (STOREY &amp; PRIOR, 2005), such as those estimated for peak metamorphic conditions in central RFB (T = 800 &#8211; 900°C; BENTO DOS SANTOS, 2008; MUNHÁ <i>et al</i>., 2008), makes it very hard to apply this methodologies, since deformation at high temperatures reduces the effective dimension of garnet and allows the interaction between garnet&#8217;s core and matrix biotite. Probably, this is also the cause for the high dispersion of results in some samples used for the SPEAR &amp; PARRISH (1996) method.</p>      <p>BENTO DOS SANTOS <i style='mso-bidi-font-style:normal'>et al</i>. (2008) provided thermochronological constraints for the SFSAP sector based on integration of multiple isotopic systems and concluded that migmatites were cooled at relatively stable 3 &#8211; 5°C/Ma, whereas granulites were maintained at lower crustal levels and very slowly cooled (&lt; 2°C/Ma) during long-term sub-horizontal transpressive shearing (FONSECA <i>et al</i>., 2008). This period of slow-cooling endured until orogenic collapse occurred, leading to abrupt fast cooling of granulites (8 to 30°C/Ma) in the last stages of Brasiliano Orogeny. The present petrological cooling rates are very difficult to interpret and to quantify, but provide qualitative results in agreement with BENTO DOS SANTOS <i style='mso-bidi-font-style:normal'>et al</i>. (2008) conclusions, such as the idea of having high temperature maintenance that reequilibrated the garnets, followed by very fast cooling that did not allow significant Fe/Mg diffusion between garnet and biotite inclusions.</p>      <p>Intense deformation caused by the long-term sub-horizontal transpressive shearing (FONSECA <i>et al</i>., 2008) can be seen in sheared migmatites and granulites (as described in the Petrography section of this work), as well as in the fact that some are abundantly blastomylonitized. This is the probable cause for the open-system behaviour found in some samples. It may have altered biotite diffusion mechanisms and reequilibrated garnet with minerals or fluids outside the garnet &#8211; biotite inclusion system, adding complexities and increasing the uncertainties regarding the use of these methodologies.</p>      <p>&nbsp;</p>      <p><b>7. CONCLUSIONS </b></p>      <p>The several obtained petrological cooling rates with two significantly different    methodologies are very dubious and provide mainly qualitative results due to    the complex evolution of the belt that allowed open-system behaviour. This altered    biotite diffusion mechanisms or reequilibrated garnet with minerals or fluids    outside the garnet &#8211; biotite inclusion system. Nevertheless, the presented    results, although very difficult to interpret and to quantify, provide qualitative    results that are in broad agreement with previously obtained geochronological    cooling rates. Thermochronology based on integration of multiple isotopic systems    are thus more accurate for inferring cooling rates in rocks that endured complex    cooling patterns, significant deformation and Fe-Mg open-system behaviour. </p>     ]]></body>
<body><![CDATA[<p>&nbsp;</p>      <p><b>ACKNOWLEDGEMENTS </b></p>      <p>FAPESP, POCA-PETROLOG (CEGUL, UI: 263; POCTI/FEDER), GEODYN (POCTI &#8211; ISFL &#8211; 5 &#8211; 32) and a PhD scholarship from FCT (SFRH/BD/17014/2004) co-financed by FEDER provided support for field and analytical work. Teresa Palácios and Octávio Chaveiro are gratefully acknowledged for long-term logistic and moral support. The authors are also grateful for the comments and suggestions of two anonymous reviewers that greatly added to the improvement of this work.</p>      <p>&nbsp;</p>      <p><b>REFERENCES</b> </p>      <!-- ref --><p>BASCOU, J., RAPOSO, M., VAUCHEZ, A., EGYDIO-SILVA, M. (2002) &#8211; Titanohematite lattice preferred orientation and magnetic anisotropy in high temperature mylonites. <i>Earth</i><i> and Planetary Science Letters</i>, <b>198</b>, 77-92. &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;[&#160;<a href="javascript:void(0);" onclick="javascript: window.open('/scielo.php?script=sci_nlinks&ref=157257&pid=S1647-581X200900010000600001&lng=','','width=640,height=500,resizable=yes,scrollbars=1,menubar=yes,');">Links</a>&#160;]<!-- end-ref --><p>BENTO DOS SANTOS, T. (2008) &#8211; Petrologia e termocronologia de granulitos no sector central da Faixa Ribeira (Regi&#8249;o de São Fidelis, Rio de Janeiro, Brasil). <i>Unpublished</i><i> Ph.D. thesis</i>, University of Lisbon, Lisbon, 388. </p>      <p>BENTO DOS SANTOS, T., MUNHÁ, J., TASSINARI, C., FONSECA, P., DIAS NETO, C. (2007) &#8211; Thermochronological evidence for long--term elevated geothermal gradients in Ribeira Belt, SE Brazil. <i>Geochimica</i><i> et Cosmochimica Acta</i>, <b>71</b>, 15, 1, A79. </p>      <p>BENTO DOS SANTOS, T., FONSECA, P., MUNHÁ, J., TASSINARI, C., DIAS NETO, C. (2008) &#8211; Structural and thermochronological constrains on the tectonic evolution of Ribeira Belt, SE Brazil. <i>Geophysical Research Abstracts</i>, <b>10</b>, A-00261. </p>      <p>CAMPOS NETO, M., FIGUEIREDO, M. (1995) &#8211; The Rio Doce orogeny, Southeastern Brazil. <i>Journal of South American Earth Sciences</i>, <b>8</b>, 2, 143-162. </p>      ]]></body>
<body><![CDATA[<p>CHAKRABORTY, S., GANGULLY, J. (1992) &#8211; Cation diffusion in aluminosilicate garnets &#8211; experimental determination in spessar-tine-almandine diffusion couples, evaluation of effective binary diffusion coefficients, and applications. <i>Contributions</i><i> to Mineralogy and Petrology</i>, <b>111</b>, 74-86. </p>      <p>CORDANI, U. (1971) &#8211; Síntese da geocronologia Pré-Cambriana da região costeira atlântica meridional da América do Sul. <i>25</i><i>th </i><i>Congresso Brasileiro de Geologia (Extended Abstract)</i>, São Paulo, 179-180. </p>      <p>CORDANI, U., DELHAL, J., LEDENT, D. (1973) &#8211; Orogenéses superposées dans le Précambrien du Brésil sud-oriental (États de Rio de Janeiro et de Minas Gerais). <i>Revista</i><i> Brasileira de Geociências</i>, <b>3</b>, 1-22. </p>      <p>DODSON, M. (1973) &#8211; Closure temperature in cooling geochronological and petrological systems. <i>Contributions to Mineralogy and Petrology</i>, <b>40</b>, 3, 259-274. </p>      <p>EHLERS, K., POWELL, R., STUWE, K. (1994) &#8211; The determination of cooling rate histories from garnet-biotite equilibrium. <i>American Mineralogist</i>, <b>79</b>, 737-744. </p>      <p>FERRY, J., SPEAR, F. (1978) &#8211; Experimental calibration of the partioning of Fe and Mg between biotite and garnet. <i>Contributions to Mineralogy and Petrology</i>, <b>66</b>, 113-117. </p>      <p>FONSECA, P., BENTO DOS SANTOS, T., MUNHÁ, J., TASSINARI, C., DIAS NETO, C. (2008) &#8211; Thermochronological and structural analysis of the geodynamic evolution of Ribeira Belt, SE Brazil. <i>Geochimica</i><i> et Cosmochimica Acta</i>, <b>72</b>, 12, 1, A276. </p>      <p>GANGULLY, J., CHENG, W., CHAKRABORTY, S. (1998) &#8211; Cation diffusion in aluminosilicate garnets: experimental determination in pyrope-almandine diffusion couples. <i>Contributions to Mineralogy and Petrology</i>, <b>131</b>, 171-180. </p>      <p>HEILBRON M., MACHADO, N. (2003) &#8211; Timing of Terrane Accretion in the Neoproterozoic-Eopaleozoic Ribeira Orogen SE Brazil. <i>Precambrian</i><i> Research</i>, <b>125</b>, 87-112. </p>      <p>HEILBRON, M., VALERIANO, C., TUPINAMBÁ, M., ALMEIDA, J., VALADARES, C., SILVA, L., NVA, D., DIOS, F. (1993) &#8211; Compartimentação tectónica e evolução geológica do segmento central da Faixa Ribeira, a Sul do Cráton do São Francisco. <i>II Simpósio do CSF (Extended Abstract)</i>, Salvador, 263-265. </p>      ]]></body>
<body><![CDATA[<p>KOHN, M., SPEAR, F. (2000) &#8211; Retrograde Net Transfer Reaction (ReNTR) Insurance for P-T estimates. <i>Geology</i>, <b>28</b>, 1127-1130. </p>      <p>LASAGA, A., RICHARDSON, S., HOLLAND, H. (1977) &#8211; The mathematics of cation diffusion and exchange between silicate minerals during retrograde metamorphism. In: Saxena, S. K., Battacharji, S. (Eds.) <i>Energetics</i><i> of Geological Processes</i>, 354-387. </p>      <p>MACHADO, N., VALLADARES, C., HEILBRON, M., VALERIANO, C. (1996) &#8211; U-Pb geochronology of the central Ribeira belt Brazil and implications for the evolution of the Brazilian Orogeny. <i>Precambrian Research</i>, <b>79</b>, 347-361. </p>      <p>MUNHÁ, J., BENTO DOS SANTOS, T., TASSINARI, C., FONSECA, P. (2008) &#8211; Pseudosection and thermobarometry constraints on the P-T-t evolution of Ribeira Belt, SE Brazil. <i>Geochimica</i><i> et Cosmochimica Acta</i>, <b>72</b>, 12, 1, A664. </p>      <p>MUNHÁ, J., CORDANI, U. G., TASSINARI, C., PALÁCIOS, T. (2005) &#8211; Petrologia e Termocronologia de gnaisses migmatíticos da Faixa de Dobramentos Araçuaí, Espírito Santo, Brasil. <i>Revista</i><i> Brasileira de Geociências</i>, <b>35</b>, 1, 123-134. </p>      <p>PEDROSA SOARES, A., NOCE, C., WIEDMANN, C., PINTO, C. (2001) &#8211; The Araçuai-West Congo Orogen in Brazil: an overview of a confined orogen formed during Gondwanaland assembly. <i>Precambrian Research</i>, <b>110</b>, 307-323. </p>      <p>PEDROSA-SOARES, A., WIEDEMANN-LEONARDOS, C. (2000) &#8211; Evolution of the Araçuai Belt and its connection to the Ribeira Belt, Eastern Brazil. In: Cordani, U., Milani, E., Thomaz-Filho, A. and Campos, D.A (Eds.), <i>Tectonic Evolution of South America</i>. Rio de Janeiro, 265-285. </p>      <p>POWELL, R., HOLLAND, T. (1999) &#8211; Relating formulations of the thermodynamics of mineral solid solutions: Activity modelling pyroxenes, amphiboles and micas. <i>American Mineralogist</i>, <b>84</b>, 1-14. </p>      <p>SCHMITT, R., TROUW, R., MEDEIROS, S., DANTAS, E. (2008) &#8211; Age and geotectonic setting of Late Neoproterozoic juvenile mafic gneisses and associated paragneisses from the Ribeira Belt (SE Brazil) based on geochemistry and Sm &#8211; Nd data &#8211; Implications on Gondwana assembly. <i>Gondwana</i><i> Research</i>, <b>13</b>, 4, 502-515. </p>      <p>SCHMITT, R., TROUW, R., SCHMUS, W., PIMENTEL, M. (2004) &#8211; Late amalgamation in the central part of West Gondwana: new geochronological data and the characterization of a Cambrian collision orogeny in the Ribeira Belt (SE Brazil). <i>Precambrian Research</i>, <b>133</b>, 29-61. </p>      ]]></body>
<body><![CDATA[<p>SPEAR, F., FLORENCE, F. (1992) &#8211; Thermobarometry in granulites: Pitfalls and new approach. <i>Precambrian Research</i>, <b>55</b>, 209-241. </p>      <p>SPEAR, F., PARRISH, R. (1996) &#8211; Petrology and cooling rates of the Valhalla Complex, British   Columbia, Canada. <i>Journal of Petrology</i>, <b>37</b>, 733-765. </p>      <p>STOREY, C., PRIOR, D. (2005) &#8211; Plastic deformation and recrystallization of garnet: a mechanism to facilitate diffusion creep. <i>Journal of Petrology</i>, <b>46</b>, 12, 2593-2613. </p>      <p>STORM, L., SPEAR, F. (2005) &#8211; Pressure, temperature and cooling rates of granulite facies migmatitic pelites from the southern Adirondack Highlands,  New York. <i>Journal of Metamorphic Geology</i>, <b>23</b>, 107-130. </p>      <p>TROUW, R., HEILBRON, M., RIBEIRO, A., PACIULLO, F., VALERIANO, C., ALMEIDA, J., TUPINAMBÁ, M., ANDREIS, R. (2000) &#8211; The central segment of the Ribeira Belt. In: Cordani, U.G., Milani, E.J., Thomaz-Filho, A. and Campos, D.A (eds.), <i>Tectonic Evolution of South America</i>. Rio de Janeiro, 297-310. </p>      <p>TUPINAMBÁ, M. (1999) &#8211; Evolução tectônica e magmática da Faixa Ribeira na região serrana do Estado do Rio de Janeiro. <i>Unpublished Ph.D. thesis</i>, University of São Paulo, São Paulo, 236. </p>      <p>VALLADARES, C., MACHADO, N., HEILBRON, M., DUARTE, B., GAUTHIER, </p>      <p>G. (2008) &#8211; Sedimentary provenance in the central Ribeira belt based on laser-ablation ICPMS 207Pb/206Pb zircon ages. <i>Gondwana</i><i> Research</i>, <b>13</b>, 4, 516-526. </p>      <p>VAUCHEZ, A., TOMMASI, A., EGYDIO-SILVA, M. (1994) &#8211; Self-indenta-tion of a heterogeneous continental lithosphere. Geology, <b>22</b>, 967-970. </p>      <p>WIMMENAUER, W., BRYNHI, I. (2007) &#8211; 6. Migmatites and related rocks.    A proposal on behalf of the IUGS Subcommission on the Systematics of Metamorphic    Rocks. Web Version of 01.02.07, 1-5 (<a href="http://www.bgs.ac.uk/scmr/docs/papers/paper_6.pdf" target="_blank">http://www.bgs.ac.uk/scmr/docs/papers/paper_6.pdf</a>).  </p>     ]]></body>
<body><![CDATA[<p>&nbsp; </p>      <p><i>Artigo recebido em Julho de 2009</i></p>      <p><i>Aceite</i><i> em Outubro de 2009</i></p>       ]]></body><back>
<ref-list>
<ref id="B1">
<nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[BASCOU]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[RAPOSO]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[VAUCHEZ]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[EGYDIO-SILVA]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<article-title xml:lang="en"><![CDATA[Titanohematite lattice preferred orientation and magnetic anisotropy in high temperature mylonites]]></article-title>
<source><![CDATA[Earth and Planetary Science Letters]]></source>
<year>2002</year>
<volume>198</volume>
<page-range>77-92</page-range></nlm-citation>
</ref>
</ref-list>
</back>
</article>
