The western Sao Francisco pericraton interpreted from crustal magnetic and gravity sources

Simple item page
dc.contributor.authorOliveira dos Reis, Luciane Katiuscia
dc.contributor.authorVidotti, Roberta Mary
dc.contributor.authorCordeiro, Pedro
dc.contributor.authorde Oliveira, Claudinei Gouveia
dc.date.accessioned2025-01-23T19:48:02Z
dc.date.available2025-01-23T19:48:02Z
dc.date.issued2020
dc.description.abstractThe Neoproterozoic Brasiliano Orogeny shaped the former Sao Francisco paleocontinent into a preserved cratonic nucleus surrounded by a pericratonic region. In central Brazil, this pericraton crops out as the Goias Massif, the basement of the northern Brasilia Belt. The well-known difficulty of tracing suture zones on surface led to a longstanding dispute on whether the Rio Maranhao Thrust, a structure separating the Internal Zone and the External Zone of the Brasilia Belt, marked the Brasiliano suture. This interpretation was largely based on regional gravimetric data showing a steep discontinuity at depth, between these zones. However, the Rio Maranhao Thrust separates two pericratonic domains of the Goias Massif (Campinorte Domain and Cavalcante-Arraias Domain), which otherwise share similar Paleoproterozoic ages and geology. To properly address the main structural boundaries within the northern Brasilia Belt, this work was focused on comparing shallow and deep gravity and magnetic data processed as enhanced anomalies and through matched filter analysis. Our results show that the large mafic-ultramafic complexes within the Internal Zone of the Brasilia Belt are masking a smooth gravimetric transition into the External Zone. Additionally, the alleged suture zone is coincident with the Mesoproterozoic rift-related Juscelandia and Palmeiropolis volcano-sedimentary sequences, which have been largely ignored in their role as creating magnetic and gravity suture-like signatures. Along with previous structural and geochronological data, our results argue against the Rio Maranhao Thrust as a suture zone and, instead, support the alternative interpretation of the thrust as an intracontinental feature within a portion of the Sao Francisco pericraton. This pericratonic region, unliked the preserved cratonic core, was widely affected by Mesoproterozoic rifting and Neoproterozoic thick-skinned thrusting. The Rio Parana Thrust, on the other hand, is unnoticeable below 8 km depth in gravity and magnetic data, suggesting thin-skinned tectonics also associated with the Brasiliano Orogeny. Finally, the relative crustal homogeneity from the Sao Francisco craton into the Goias Massif evidenced by our gravity data and confirmed by first- and second-order magnetic lineaments confirms the nature of a pericraton with dominantly NE (N20-40E) trending lineaments. These lineaments were progressively overprinted by Brasiliano NNE (N45-70E) structures from the western margin of the External Zone into the Internal Zone.
dc.fuente.origenWOS
dc.identifier.doi10.1016/j.jsames.2020.102716
dc.identifier.eissn1873-0647
dc.identifier.issn0895-9811
dc.identifier.urihttps://doi.org/10.1016/j.jsames.2020.102716
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/100422
dc.identifier.wosidWOS:000572378000003
dc.language.isoen
dc.revistaJournal of south american earth sciences
dc.rightsacceso restringido
dc.subjectBrasilia belt
dc.subjectGoias Massif
dc.subjectRio maranhao thrust
dc.subjectMatched filtering
dc.subjectBrasiliano Orogeny
dc.subject.ods13 Climate Action
dc.subject.odspa13 Acción por el clima
dc.titleThe western Sao Francisco pericraton interpreted from crustal magnetic and gravity sources
dc.typeartículo
dc.volumen103
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
Files
Collections
Artículos de revistas