New paleomagnetic data on dykes to assess the accretions to West African Craton to Columbia and Rodinia

• Main Authors: Aifa, Tahar, Merabet, Nacer-Eddine
• Other Authors: Géosciences Rennes (GR), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centre National de la Recherche Scientifique (CNRS), Centre de Recherche en Astronomie Astrophysique et Géophysique (CRAAG)
• Format: Conference Object
• Language: English
• Published: HAL CCSD 2017
• Subjects: West African craton; Rodinia; Dykes; Columbia; Rock magnetism; Paleomagnetism; Apparent Polar wander path; [SDU.STU.GP]Sciences of the Universe [physics]/Earth Sciences/Geophysics [physics.geo-ph]; [SDU.STU.TE]Sciences of the Universe [physics]/Earth Sciences/Tectonics; Fennoscandia
• Online Access: https://insu.hal.science/insu-01661630

International audience A new Apparent Polar Wander Path has been calculated for the West African Craton (WAC) using paleomagnetic data obtained on the Yetti-Eglab intrusions and stromatolite-bearing formations. As no contact test was available, the magnetic stability of carriers was demonstrated thanks to rock magnetic measurements. One, two or three magnetization components on 159 oriented specimens (14 sites) have been isolated using principal component analysis or great circles technique, mainly on doleritic dykes. High and low unblocking temperature components were isolated in six dykes but also in four sites of the well dated Hank stromatolite-bearing formation (875-890 Ma). For the two kinds of rocks, the main components show stable remanent magnetization mainly carried by magnetite (or titanomagnetite) as described using thermomagnetic or Isothermal Remanent magnetization curves, where no significant mineralogical transformation occurred at high temperatures.Five groups of paleopoles have been calculated: they witness the existence of a large circum-terrestrial loop with a drift from the high latitudes of the lower hemisphere to the high southern latitudes of the upper hemisphere followed by a re-entry in the high latitudes of the lower hemisphere. This is in agreement with the previous loop computed by Sabaté and Lomax (1975) between 2.1 Ga and 1.7 Ga. The Yetti and Eglab blocks amalgamated around 1.9 Ga and participated to the formation of Columbia Supercontinent. The paleopole computed for the stromatolite-bearing formation corresponds with the location of Rodinia Supercontinent at its early stages of amalgamation.The geodynamic evolution of the WAC respect with that of Columbia and Rodinia Supercontinents suggests that the Eglab and Yetti were clearly separated by a large oceanic crust before 1.9 Ga. A volcanic arc developed during the subduction of this ocean followed by crustal thickening which generated an intrusive suite (Aftout granites) when it was at the northern low latitudes. Fennoscandia ...