The P3 kimberlite and P4 lamproite, Wajrakarur kimberlite field, India: mineralogy, and major and minor element compositions of olivines as records of their phenocrystic vs xenocrystic origin

  • Azhar M. Shaikh
  • Satya P. Kumar
  • Suresh C. Patel
  • Satyajeet S. Thakur
  • Subramanian Ravi
  • Duryadhan Behera
Original Paper
  • 76 Downloads

Abstract

Distinctly different groundmass mineralogy characterise the hypabyssal facies, Mesoproterozoic diamondiferous P3 and P4 intrusions from the Wajrakarur Kimberlite Field, southern India. P3 is an archetypal kimberlite with macrocrysts of olivine and phlogopite set in a groundmass dominated by phlogopite and monticellite with subordinate amounts of serpentine, spinel, perovskite, apatite, calcite and rare baddeleyite. P4 contains mega- and macrocrysts of olivine set in a groundmass dominated by clinopyroxene and phlogopite with subordinate amounts of serpentine, spinel, perovskite, apatite, and occasional gittinsite, and is mineralogically interpreted as an olivine lamproite. Three distinct populations of olivine, phlogopite and clinopyroxene are recognized based on their microtextural and compositional characteristics. The first population includes glimmerite and phlogopite–clinopyroxene nodules, and Mg-rich olivine macrocrysts (Fo 90–93) which are interpreted to be derived from disaggregated mantle xenoliths. The second population comprises macrocrysts of phlogopite and Fe-rich olivine (Fo 81–89) from P3, megacrysts and macrocrysts of Fe-rich olivine (Fo 85–87) from P4 and a rare olivine–clinopyroxene nodule from P4 which are suggested to have a genetic link with the precursor melt of the respective intrusions. The third population represents clearly magmatic minerals such as euhedral phenocrysts of Fe-rich olivine (Fo 85–90) crystallised at mantle depths, and olivine overgrowth rims formed contemporaneously with groundmass minerals at crustal levels. Close spatial association and contemporaneous emplacement of P3 kimberlite and P4 lamproite is explained by a unifying petrogenetic model which involves the interaction of a silica-poor carbonatite melt with differently metasomatised wall rocks in the lithospheric mantle. It is proposed that the metasomatised wall rock for lamproite contained abundant MARID-type and phlogopite-rich metasomatic veins, while that for kimberlite was relatively refractory in nature.

Keywords

Kimberlite Lamproite Olivine Wajrakarur India Xenocrysts 

Notes

Acknowledgements

We are grateful to Geoffrey Howarth and Lynton Jaques for their detailed and valuable comments. Andrea Giuliani is thanked for editorial handling. The Department of Science and Technology, Government of India, provided the financial support (grant no. IR/S4/ESF-16/2009) for establishing the EPMA National Facility, Indian Institute of Technology Bombay, under the Intensification of Research in High Priority Areas (IRPHA) scheme.

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Copyright information

© Springer-Verlag GmbH Austria, part of Springer Nature 2018

Authors and Affiliations

  • Azhar M. Shaikh
    • 1
  • Satya P. Kumar
    • 1
  • Suresh C. Patel
    • 1
  • Satyajeet S. Thakur
    • 2
  • Subramanian Ravi
    • 3
  • Duryadhan Behera
    • 4
  1. 1.EPMA Lab, Department of Earth SciencesIndian Institute of Technology BombayMumbaiIndia
  2. 2.Wadia Institute of Himalayan GeologyDehra DunIndia
  3. 3.Geological Survey of IndiaHyderabadIndia
  4. 4.Department of Earth SciencesSambalpur UniversityBurlaIndia

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