Geochemistry and petrogenesis of the Proterozoic dykes in Tamil nadu, southern India: another example of the Archaean lithospheric mantle source

Citation
T. Radhakrishna et M. Joseph, Geochemistry and petrogenesis of the Proterozoic dykes in Tamil nadu, southern India: another example of the Archaean lithospheric mantle source, GEOL RUNDSC, 87(3), 1998, pp. 268-282
Citations number
51
Categorie Soggetti
Earth Sciences
Journal title
GEOLOGISCHE RUNDSCHAU
ISSN journal
00167835 → ACNP
Volume
87
Issue
3
Year of publication
1998
Pages
268 - 282
Database
ISI
SICI code
0016-7835(199812)87:3<268:GAPOTP>2.0.ZU;2-X
Abstract
Approximately 1650-Ma-old NW/SE and NE/SW-trending dolerite dykes in the Ti ruvannamalai (TNM) area and approximately 1800-Ma-old NW/SE-trending doleri te dykes in the Dharmapuri (DP) area constitute major Proterozoic dyke swar ms in the high-grade granulite region of Tamil nadu, southern India. The NW - and NE-trending TNM dykes are compositionally very similar and can be reg arded as having been formed during a single magmatic episode. The DP dykes may relate to an earlier similar magmatic episode. The dolerites are Fe-ric h tholeiites and most of the elemental variations can be explained in terms of fractional crystallisation. Clinopyroxene and olivine are the inferred ferromagnesian fractionation phases followed by plagioclase during the late fractionation stages. All the studied dykes have, similar to many continen tal flood basalts (CFB), large-ion lithophile element (LILE) and light rare -earth element (LREE) enrichment and Nb and Ta depletion. The incompatible element abundance patterns are comparable to the patterns of many other Pro terozoic dykes in India and Antarctica, to the late Archaean (similar to 2. 72 Ga) Dominion volcanics in South Africa and to the early Proterozoic (sim ilar to 2.0 Ga) Scourie dykes of Scotland. The geochemical characteristics of the TNM and DP dykes cannot be explained by crustal contamination alone. Instead, they are consistent with derivation from an enriched lithospheric mantle source which appears to have been developed much earlier than thp d yke intrusions during a major crustal al building event in the Archaean. Th e dyke magmas may have been formed by dehydration melting induced by decomp ression and lithospheric attenuation or plume impingement at the base of th e lithosphere. These magmas, compared with CFB, appear to be the minor part ial melts from plume heads of smaller diameter and of shallow origin (650 k m). Therefore, the Proterozoic thermal events could induce crustal attenuat ion and dyke intrusions in contrast to the extensive CFB volcanism and cont inental rifting generally associated with the Phanerozoic plumes of larger head diameter (>1000 km) and of deeper origin (at crust mantle boundary).