Busca avançada
Ano de início
Entree
(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

Is the Neoproterozoic oxygen burst a supercontinent legacy?

Texto completo
Autor(es):
Macouin, Melina [1] ; Roques, Damien [1] ; Rousse, Sonia [1] ; Ganne, Jerome [1] ; Denele, Yoann [1] ; Trindade, Ricardo I. F. [2]
Número total de Autores: 6
Afiliação do(s) autor(es):
[1] Univ Toulouse, CNRS, Geosci Environm Toulouse, UMR 5563, UR234, Toulouse - France
[2] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, Dept Geofis, Sao Paulo - Brazil
Número total de Afiliações: 2
Tipo de documento: Artigo Científico
Fonte: Frontiers in Earth Science; v. 3, 2015.
Citações Web of Science: 4
Resumo

The Neoproterozoic (1000-542 mol.yr ago) witnessed the dawn of Earth as we know it with modern -style plate tectonics, high levels of 02 in atmosphere and oceans and a thriving fauna. Yet, the processes leading to the fully oxygenation of the external envelopes, its exact timing and its link with the inner workings of the planet remain poorly understood. In some ways, it is a ``chicken and egg{''} question: did the Neoproterozoic Oxygenation Event (NOE) cause life blooming, low-latitudes glaciations, and perturbations in geochemical cycles or is it a consequence of these phenomena? Here, we suggest that the NOE may have been triggered by multi-million years oxic volcanic emissions along a protracted period at the end of the Neoproterozoic when continents were assembled in the Rodinia supercontinent. We report a very oxidized magma source at the upper mantle beneath a ring of subducting margins around Rodinia, and detail here the evidence at the margin of the Arabian shield. We investigate the 780 Ma Biotite and Pink granites and associated rocks of the Socotra Island with rock magnetic and petrographic methods. Magnetic susceptibility and isothermal remanent magnetization acquisitions show that, in these granites, both magnetite and hematite are present. Hematite subdivides magnetite grains into small grains. Magnetite and hematite are found to be primary, and formed at the early magmatic evolution of the granite at very high oxygen fugacity. Massive degassing of these oxidized magmas would reduce the sink for oxygen, and consequently contribute to its rise in the atmosphere with a net 02 flux of at least 2.25 x 107 Tmol. Our conceptual model provides a deep Earth link to the NOE and implies the oxygenation burst has occurred earlier than previously envisaged, paving the way for later changes in the outer envelopes of the planet epitomized on the extreme Neoproterozoic glaciations and the appearance of the first animals. (AU)

Processo FAPESP: 13/08862-1 - A intensidade do campo magnético terrestre durante o Neoproterozóico
Beneficiário:Ricardo Ivan Ferreira da Trindade
Modalidade de apoio: Auxílio à Pesquisa - Pesquisador Visitante - Internacional