4.5 Article

Was there SAMBA in Columbia? Paleomagnetic evidence from 1790 Ma Avanavero mafic sills (northern Amazonian Craton)

Journal

PRECAMBRIAN RESEARCH
Volume 244, Issue -, Pages 139-155

Publisher

ELSEVIER
DOI: 10.1016/j.precamres.2013.11.002

Keywords

Paleomagnetism; Avanavero sills; Amazonian Craton; Columbia Supercontinent

Funding

  1. FAPESP [07/59531-4, 11/50887-6, 07/53177-4, 12/50327-3]
  2. CNPq [302174/2011-7, 306217/2010-4, 301775/2012-5]
  3. Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP) [11/50887-6] Funding Source: FAPESP

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The Amazonian Craton represents an important piece in the Paleoproterozoic paleogeography of the Earth. This study presents paleomagnetic data obtained on well-dated (U-Pb) 1790 Ma mafic sills from the Avanavero magmatism in northern Amazonian Craton (Guiana Shield). AF and thermal treatments revealed southeastern, low downward/upward inclination, remanent magnetization directions that are carried by moderate to high-H-c and high-T-B Ti-poor titanomagnetite. The site mean directions cluster around the mean D-m = 138.2 degrees, I-m = -3.4 degrees (N= 13, proportional to(95) = 13.0 degrees), which yields a robust paleomagnetic pole (AV pole) at 27.9 degrees E, 48.4 degrees S (A95 = 9.6 degrees) with a Q-value of 5. The characteristic component disclosed for the Avanavero sill matches that obtained for sediments collected along the baked contact and are distinct from those away from the sill. The Avanavero directions are also significantly different from those obtained for younger units, with ages spanning from 1420 to 520 Ma, suggesting the sills carry a primary remanence. The Avanavero pole helps in constraining the paleogeography of the central pieces of Columbia. It is compatible with the Baltica and Amazonian Cratons SAMBA link in the Columbia Supercontinent at about 1780 Ma, but other configurations are also possible. When compared to other Paleo- to Mesoproterozoic paleomagnetic poles from the southern Amazonian Craton (Central Brazil Shield), our new paleomagnetic pole suggests intracratonic motions within the southern area of the Craton, probably after 1420 Ma ago. We tentatively suggest that these movements are related to the collision of the Paragua Block with the proto-Amazonian Craton at about 1350-1320 Ma ago. (c) 2013 Elsevier B.V. All rights reserved.

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