GSA 2020 Connects Online

Paper No. 142-3
Presentation Time: 2:00 PM

OLIVINE MELILITITES, MANTLE XENOLITHS, AND XENOCRYSTS OF THE TAKARINDIONA DISTRICT: PETROGENESIS, MAGMATIC EVOLUTION, AND THE SUB-CONTINENTAL LITHOSPHERIC MANTLE OF EAST-CENTRAL MADAGASCAR


TUCKER, Robert1, ROCCO, I.2, MELLUSO, Leone3, MORRA, V.2 and D’ANTONIO, M.2, (1)Bureau des Recherches Géologiques et Minières, 9252 Wood Glade Drive, Great Falls, VA 22066, (2)Dipartimento di Scienze della Terra, Università degli Studi di Napoli Federico II, via Cinthia 21, ed. L1, Napoli, 80126, Italy, (3)Bureau des Recherches Géologiques et Minières, 9252 Wood Glade Drive, Great Falls, VA 22066; Dipartimento di Scienze della Terra, Università degli Studi di Napoli Federico II, via Cinthia 21, ed. L1, Napoli, 80126, Italy

The olivine melilitites from the southern part of the 6.8 Ma-old Takarindiona volcanic field (Eastern Madagascar) are olivine ± chromite -phyric lava flows, having zoned titanaugite, perovskite, melilite, nepheline, monticellite, Ba-mica and Fe-Ti oxides as microphenocrysts or groundmass phases. The volcanic rocks are very primitive ultrabasic rocks, rich in incompatible trace elements (e.g., Ba=1049 ± 153 ppm, Sr=1050 ± 167 ppm, Nb=98±13 ppm; La/Ybn= 41±5; La/Nb=0.88±0.05), with a restricted range of 87Sr/86Sr (0.70391-0.70410) and 143Nd/144Nd (0.51272-0.51282). The rocks follow a differentiation trend controlled by approximately 20% removal/addition of phenocryst olivine ± chromite. The ol-melilititic magmas are the product of small degrees of partial melting (1-3%) of a peridotitic source, enriched in highly incompatible trace elements by CO2-, F-, and H2O-rich melts, located within the garnet stability field (3-3.5 GPa and ~100km depth) of sub-continental lithospheric mantle, where carbonates (dolomite) were stable phases. Mantle xenoliths within the volcanic rocks are mostly spinel harzburgites having mineral modes and chemical compositions suggesting variable degrees of “basalt” melt extraction. Based on textural and chemical evidence, and quantitative thermobarometric estimates, the xenoliths were incorporated at a pressure of ~1.1 GPa (~ 35-40 km depth), far shallower than the source of the melilititic magmas, and along a predictably cool geotherm beneath Archean continental lithosphere. Berman's TWQ program (1991, Can. Mineral. 29, 833-855 and its version for Windows) has been applied to calculate log (a Quartz) vs. T-X in the SiO2-MgO-CaO-Na2O system for 3kb pressure. At 900oC the mel-ol assemblage is stable for log (a Quartz) between -1 and -1.5 (a Quartz - 0.1 to 0.03), and at 1000oC, the balance between diopside and akermanite - forsterite, fixes a Quartz at 0.06, a value compared to those, significantly higher, for the nepheline-albite balances (-0.47) and forsterite-enstatite (-0.57). Highly resorbed orthopyroxene xenocrysts, resembling those crystallizing in lower crustal granulites, indicate that the melilitites may have also entrained lower crustal or underplated subalkaline rocks.