2020
DOI: 10.1029/2020tc006184
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From Crustal Thickening to Orogen‐Parallel Escape: The 120‐Myr‐Long HT‐LP Evolution Recorded by Titanite in the Paleozoic Famatinian Backarc, NW Argentina

Abstract: Exposed sections of accretionary orogens allow reconstruction of their tectonic evolution. Most commonly, orogens are characterized by two-dimensional shortening perpendicular to the orogenic front. We describe the midcrustal section of the backarc of the early Paleozoic Famatinian accretionary orogen, exposed in the Sierra de Quilmes. Here crustal deformation evolved from a typical two-dimensional shortening with tectonic transport toward the west, to a noncoaxial constrictional strain with a southward tecton… Show more

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Cited by 11 publications
(23 citation statements)
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References 124 publications
(208 reference statements)
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“…This was confirmed by Farias et al. (2020) who investigated titanite from footwall samples and concluded that this retro‐arc region “remained above 700°C for 120 Myr between 500 and 380 Ma” some 60 Myr longer than the hanging wall. In this paper, we expand on these finding by investigating the complementary temporal and thermal record of zircon, monazite and titanite of several samples from the footwall.…”
Section: Introductionsupporting
confidence: 56%
See 1 more Smart Citation
“…This was confirmed by Farias et al. (2020) who investigated titanite from footwall samples and concluded that this retro‐arc region “remained above 700°C for 120 Myr between 500 and 380 Ma” some 60 Myr longer than the hanging wall. In this paper, we expand on these finding by investigating the complementary temporal and thermal record of zircon, monazite and titanite of several samples from the footwall.…”
Section: Introductionsupporting
confidence: 56%
“…The most extensive dating work of rocks of the Agua del Sapo complex was the U‐Pb dating of titanites by Farias et al. (2020). They found widely variable ranges of dates.…”
Section: Geological Backgroundmentioning
confidence: 99%
“…Accordingly, it can be concluded that the main melting process took place at least between 430 and 410 Ma. Such age spreads of the melting process are common in hot orogens worldwide, including the Lachlan orogenic belt in Australia (Collins, 2002a, 2002b; Foster & Gray, 2000; White & Chappell, 1988) and the Famatinian Orogen in Argentina (Farias et al., 2020; Wolfram et al., 2019). By contrast, the timing of D1 B phase cannot be precisely determined by the current geochronological data.…”
Section: Discussionmentioning
confidence: 99%
“…Transport directions can, of course, change both spatially and temporally, and may reflect complex flow patterns (particularly under ductile conditions in the mid-lower crust) and strain path partitioning at a wide range of scales [7][8][9][10][11][12][13]. Additionally, orogen-scale arcuate lineation patterns are commonly interpreted as indicating transpressional deformation associated with variable components of orogen-perpendicular shortening and orogen parallel shearing (e.g., Burg et al, [14]; Xypolias et al, [15]).…”
Section: Introductionmentioning
confidence: 99%