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<front>
<journal-meta>
<journal-id journal-id-type="publisher">SED</journal-id>
<journal-title-group>
<journal-title>Solid Earth Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">SED</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Solid Earth Discuss.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1869-9537</issn>
<publisher><publisher-name></publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/sed-4-1379-2012</article-id>
<title-group>
<article-title>Mafic granulite xenoliths in the Chilka Lake suite, Eastern Ghats Belt, India: evidence of deep-subduction of residual oceanic crust</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bhattacharya</surname>
<given-names>S.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Chaudhary</surname>
<given-names>A. K.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Saw</surname>
<given-names>A. K.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Das</surname>
<given-names>P.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Chatterjee</surname>
<given-names>D.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Indian Statistical Institute, Kolkata 700108, India</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Indian Institute of Technology, Roorkee 247667, India</addr-line>
</aff>
<pub-date pub-type="epub">
<day>05</day>
<month>11</month>
<year>2012</year>
</pub-date>
<volume>4</volume>
<issue>2</issue>
<fpage>1379</fpage>
<lpage>1410</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2012 S. Bhattacharya et al.</copyright-statement>
<copyright-year>2012</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
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<abstract>
<p>Granulite xenoliths preserve key geochemical and isotopic signatures of
their mantle source regions. Mafic granulite and pyroxinite xenoliths within
massif-type charnockitic rocks from the Eastern Ghats Belt have recently
been reported by us. The mafic granulite xenoliths from the Chilka Lake
granulite suite with abundant prograde biotite are geochemically akin to
Oceanic Island Basalt (OIB). They can be distinguished from the
hornblende-mafic granulite xenoliths with signatures of Arc-derived basalt
occurring in the other suites of the Eastern Ghats Belt. These two groups of
xenoliths in the Paleoproterozoic Eastern Ghats Province have quite distinct
Nd-model ages- 1.9 Ga and 2.5 Ga respectively, which may be interpreted as
their crustal residence ages. Strong positive Nb anomalies, indicating
subducted oceanic crust in the source, LREE enrichment and strongly
fractionated REE pattern are key geochemical signatures attesting to their
origin as OIB-type magma. Also low Yb and Sc contents and high (La / Yb)&lt;sub&gt;N&lt;/sub&gt;
ratios can be attributed to melting in the presence of residual garnet and
hence at great depths (&gt; 80 km). The variable enrichment in
radiogenic &lt;sup&gt;87&lt;/sup&gt;Sr, between 0.70052 and 0.71092 at 1.9 Ga and less
radiogenic &lt;sup&gt;143&lt;/sup&gt;Nd between ε-1.54 and 7.46 are similar to those of the
OIBs compared to MORBs. As OIBs commonly contain some recycled oceanic crust
in their sources, we suggest that the residue of the oceanic crust from a
previous melting event (~ 2.5 Ga) that produced the
Arc-derived basalts (protoliths of hornblende-mafic granulite xenoliths)
could have subducted to great depths and mechanically mixed with the mantle
peridotite. A subsequent re-melting event of this mixed source might have
occurred at ca. 1.9 Ga as testified by the crustal residence ages of the
biotite-mafic granulite xenoliths of the Chilka Lake granulite suite.</p>
</abstract>
<counts><page-count count="32"/></counts>
</article-meta>
</front>
<body/>
<back>
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