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Famatinian Orogeny

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Journal Article
Published: 28 November 2019
Journal of the Geological Society (2020) 177 (2): 233–257.
..., coupled with geochronological methods and P – T estimates, reveal polyphase contractional deformation and metamorphism during the Famatinian Orogeny over a long period of time. Peaks of metamorphic monazite and zircon ages are recorded at c. 500 Ma, between 484 and 465 Ma and at c. 440 Ma. Between 484...
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Journal Article
Published: 01 April 1999
Exploration and Mining Geology (1999) 8 (1-2): 1–20.
...-synmetamorphic emplacement at 478+ or -6 Ma during the Famatinian (Ordovician) orogeny. Minor to locally significant recrystallization and deformation of mafic-ultramafic rocks and redistribution of sulfides and PGE occurred during and following the Famatinian orogeny. The Las Aguilas intrusion is one of several...
Journal Article
Published: 13 January 2015
Journal of the Geological Society (2015) 172 (2): 186–200.
... with an additional peak at 1.3–0.9 Ga and they can be correlated with ‘Grenvillian’ age, and the Brasiliano, Pampean, and Famatinian orogenies. The zircon data reveal main transport from the nearby Ordovician Famatinian arc and related rocks. The Silurian sandstone units are more comparable with Cambrian units...
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Journal Article
Published: 15 March 2023
Geological Magazine (2023) 160 (5): 972–992.
... of the Famatinian orogeny, between 445 and 410 Ma, which is well exposed at Sierra de Ramaditas and neighbouring ranges in western Argentina. The Ramaditas Complex is formed by metasedimentary and meta-ultrabasic rocks and amphibolites. This complex forms the upper nappe of a thrust stack resulting from westward...
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Journal Article
Published: 18 July 2019
Geological Magazine (2020) 157 (2): 321–339.
... that underwent folding, thrusting and metamorphism during the Ordovician Famatinian orogeny. Mafic rocks and granitoids of the easternmost Sierra de Pie de Palo provide information about the magmatic activity at the proto-Andean margin of Gondwana during late Cambrian – Early Ordovician time. Magmatic activity...
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Journal Article
Journal: GSA Bulletin
Published: 01 January 1997
GSA Bulletin (1997) 109 (1): 16–42.
.... 455 Ma that followed Middle Ordovician collision with the proto-Andean margin of Gondwana as part of the complex Indonesian-style Taconic-Famatinian orogeny, which involved several island arc-continent collisions between the two major continental entities. Laurentia then continued its clockwise...
Series: GSA Special Papers
Published: 01 January 1990
DOI: 10.1130/SPE241-p77
... (e.g., Achala and Velasco batholiths) and widespread smaller plutons that were emplaced during the later stages of the early Paleozoic (Famatinian) orogeny. Common features of the larger bodies include the presence of muscovite, aluminum silicates, and a dominant porphyritic phase characterized...
Journal Article
Journal: GSA Bulletin
Published: 01 March 2017
GSA Bulletin (2017) 129 (3-4): 415–428.
... Cordillera of Peru, and the Amotapes Massif. Detrital sediments of the forearc are marked by a major gap in Early Cretaceous–Jurassic ages and the minor presence of Ordovician (Famatinian orogeny) and Carboniferous–Permian (340–285 Ma) ages. The age spectrum is not compatible with sediment input from...
Journal Article
Published: 14 October 2021
Geological Magazine (2022) 159 (3): 309–321.
... events during the Grenvillian orogeny, at c . 1235, 1155 and 1035 Ma, and a younger metamorphism at c . 440–420 Ma resulting from reactivation during the Famatinian orogeny. The sedimentary protoliths were deposited between 1.86 and 1.33–1.26 Ga (the age of the Andean-type Grenvillian magmatism recorded...
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Journal Article
Journal: GSA Bulletin
Published: 01 September 2006
GSA Bulletin (2006) 118 (9-10): 1270–1279.
... until at least the mid-Ordovician Famatinian orogeny. Our data show that the Puncoviscana Formation and associated metasedimentary rocks everywhere contain a similar, centimeter-scale spacing of original sedimentary layers and/or compositional bands. The earliest recorded fabric...
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Journal Article
Journal: Geology
Published: 01 August 1998
Geology (1998) 26 (8): 707–710.
... Ma highly peraluminous granites in the Eastern Sierras Pampeanas. After brief quiescence, a second major episode, the Famatinian orogeny, started with subduction ca. 490 Ma, forming a wide continental arc and ensialic backarc basin. This heralded the approach of Laurentia to Gondwana, during which...
Image
Generalized sketch map of the Sierras Pampeanas and southern Puna showing the main lithologies and distribution of the Pampean and Famatinian orogenic belts. The area of study is indicated by the box. *In part reworked by the Famatinian orogeny. ** Internal zone of the orogen.
Published: 01 July 2016
Figure 1. Generalized sketch map of the Sierras Pampeanas and southern Puna showing the main lithologies and distribution of the Pampean and Famatinian orogenic belts. The area of study is indicated by the box. *In part reworked by the Famatinian orogeny. ** Internal zone of the orogen.
Journal Article
Journal: Geosphere
Published: 12 October 2021
Geosphere (2021) 17 (6): 1786–1806.
... of the regional Famatinian orogeny (ca. 490–455 Ma). In addition, the Maz Complex records an earlier granulite facies event at ca. 1.2 Ga. The Taco and Ramaditas Complexes, in contrast, experienced medium- and low-pressure upper amphibolite to granulite facies metamorphism, respectively, between ca. 470–460 Ma...
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Image
Geodynamic model proposed in this work, from Rodinia accretion through the Pampean and Famatinian orogenies to the transcurrent displacement of Cuyania and its final arrival outboard of the Famatina orogen. Our interpretation of the opening and closing of the Puncoviscana Basin with the Western Sierras Pampeanas (WSP)/Arequipa-Antofalla (AA) rift from the western margin of Río de la Plata Craton/Amazonia follows that of Aceñolaza and Toselli (2009) and Ramos (2008). ESP = Eastern Sierras Pampeanas.
Published: 01 January 2022
Figure 10.  Geodynamic model proposed in this work, from Rodinia accretion through the Pampean and Famatinian orogenies to the transcurrent displacement of Cuyania and its final arrival outboard of the Famatina orogen. Our interpretation of the opening and closing of the Puncoviscana Basin
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 (a) Location of the studied zone within the Sierras Pampeanas de Córdoba. HP, El Hongo pluton; CP, Calmayo pluton; SAP, San Agustín pluton; CtL, Ctalamuchita lineament, LCL, Los Condores lineament. (b) Simplified geological map of the central sector of the Sierra Chica showing the El Hongo (HP) and Calmayo (CP) plutons and the trajectories of the regional foliation produced during the Famatinian orogeny.
Published: 01 September 2006
the El Hongo (HP) and Calmayo (CP) plutons and the trajectories of the regional foliation produced during the Famatinian orogeny.
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Geodynamic model of (1) origin of the Sierra de Maz–Arequipa–Rio Apa (MARA) Terrane from eastern Laurentia and its collision with the Kalahari Craton, generating the Pampean orogen, followed by the displacement of the Kalahari Craton and the Río de la Plata Craton (RPC) along the Córdoba fault, as proposed by Rapela et al. (2016), and (2) the subsequent rifting of Cuyania from the Ouachita embayment of Laurentia and its approach to Gondwana, generating the Famatinian orogeny, as proposed by Thomas and Astini (1996) and many others. ESP = Eastern Sierras Pampeanas.
Published: 01 January 2022
the Córdoba fault, as proposed by Rapela et al. ( 2016 ), and (2) the subsequent rifting of Cuyania from the Ouachita embayment of Laurentia and its approach to Gondwana, generating the Famatinian orogeny, as proposed by Thomas and Astini ( 1996 ) and many others. ESP = Eastern Sierras Pampeanas.
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Evolution of Famatinian Cambrian units within the Ocloyic Orogeny. Modified from Astini et al. (1995, 2007) and Astini & Dávila (2004).
Published: 01 March 2009
Fig. 8. Evolution of Famatinian Cambrian units within the Ocloyic Orogeny. Modified from Astini et al . (1995, 2007 ) and Astini & Dávila (2004 ).
Image
Ophiolite pulses and the distribution of major orogenic belts with ophiolite occurrences during the Phanerozoic. A. Ophiolite pulses and the geographic distribution of Phanerozoic ophiolites through time. B. Distribution of representative examples of major ophiolite types through time. C. Approximate time intervals for the lifespan of major supercontinents and their breakup, significant orogenic events, and supermagmatic events represented by the emplacement of giant dike swarms and large igneous provinces (LIPs). The main pulses of ophiolite generation coincide with plate movements leading to the closure of ocean basins and continental collisions, large magmatic events (with the production of large igneous provinces and giant dike swarms), and the breakup of supercontinents. Major orogenic events are (from youngest to oldest): Ar-Eu—Arabia-Eurasia collision, In-Eu—India-Eurasia collision, Al-Ur—Altaid-Uralian orogenies of Central Asia, Ap-Hy—Appalachian-Hercynian orogenies, Cld—Caledonian orogeny, Fmt—Famatinian orogeny, P-Af-Br—Pan-African–Brasiliano orogenies. Ng—Neogene; Pg—Paleogene. For a list of different ophiolite types, see Table 1.
Published: 01 March 2011
-Eurasia collision, Al-Ur—Altaid-Uralian orogenies of Central Asia, Ap-Hy—Appalachian-Hercynian orogenies, Cld—Caledonian orogeny, Fmt—Famatinian orogeny, P-Af-Br—Pan-African–Brasiliano orogenies. Ng—Neogene; Pg—Paleogene. For a list of different ophiolite types, see Table 1 .
Image
Composite plots of detrital zircon U-Pb age distributions for all detrital zircon U-Pb results from modern river sand samples in Ecuador. Plots show 0–300 Ma distribution (upper) and 0–2150 Ma distribution (lower), with each distribution defined by an age probability density function (thick black line), kernel density estimate (thin red line), and age histogram (open rectangles). Color bars highlight distinctive age populations in the composite plots, and match the pie diagram (lower right) showing color-coded age proportions for diagnostic age categories recognized in Ecuador (after Gutiérrez et al., 2019). Pl-Q—Pliocene–Quaternary; FMT—Famatinian orogeny; NPR—Neoproterozoic; SA—Sunsás; RSI—Rondonia–San Ignacio; RNJ—Rio Negro–Jurena; VT—Ventuari-Tapajós.
Published: 08 November 2019
Gutiérrez et al., 2019 ). Pl-Q—Pliocene–Quaternary; FMT—Famatinian orogeny; NPR—Neoproterozoic; SA—Sunsás; RSI—Rondonia–San Ignacio; RNJ—Rio Negro–Jurena; VT—Ventuari-Tapajós.
Series: AAPG Memoir
Published: 01 January 2018
DOI: 10.1306/13622115M1172855
EISBN: 9781629812809
... ), with some minor evidence of magmatic activity related to the rift phase ( Baldo et al., 2006 ; Ramos, 2009 ). The active margin was developed in the Puncoviscana belt and their associated calc-alkaline batholith, south of 22°S latitude ( Ramos, 2008 ). The Famatinian Orogeny The Famatinian orogenic...
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