Léo A. Hartmann, Mariana Werle, Cassiana R. L. Michelin, Cristiano Lana, Gláucia N. Queiroga, Marco P. Castro, Karine R. Arena. Proto-Adamastor ocean crust (920 Ma) described in Brasiliano Orogen from coetaneous zircon and tourmaline[J]. Geoscience Frontiers, 2019, 10(4): 1623-1633. DOI: 10.1016/j.gsf.2018.09.018
Citation: Léo A. Hartmann, Mariana Werle, Cassiana R. L. Michelin, Cristiano Lana, Gláucia N. Queiroga, Marco P. Castro, Karine R. Arena. Proto-Adamastor ocean crust (920 Ma) described in Brasiliano Orogen from coetaneous zircon and tourmaline[J]. Geoscience Frontiers, 2019, 10(4): 1623-1633. DOI: 10.1016/j.gsf.2018.09.018

Proto-Adamastor ocean crust (920 Ma) described in Brasiliano Orogen from coetaneous zircon and tourmaline

  • Proto-Adamastor ocean bathed Rodinia and successor continental fragments from 1.0-0.9 Ga up to 0.75 Ga, and evolved into world Adamastor Ocean at 0.75-0.60 Ga. Mesoproterozoic oceanic crust is poorly preserved on continents, only indirect evidence registered in Brasiliano Orogen. We report first evidence of ophiolite originated in proto-Adamastor. We use multi-technique U-Pb-Hf zircon and δ11B tourmaline isotopic and elemental compositions. The host tourmalinite is enclosed in metaserpentinite, both belonging to the Bossoroca ophiolite. Zircon is 920 Ma-old, εHf(920 Ma)=+12, HfTDM=1.0 Ga and has ‘oceanic’ composition (e.g., U/Yb < 0.1). Tourmaline is dravite with δ11B=+1.8‰ (Tur 1), 0‰ (Tur 2), -8.5‰ (Tur 3). These characteristics are a novel contribution to Rodinia and associated world ocean, because a fragment of proto-Adamastor oceanic crust and mantle evolved at the beginning of the Brasiliano Orogen.
  • loading

Catalog

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return