Sodic-Silicic Magmatism in Tadpatri Formation- A Study in Quartz Keratophyre and Albitite

2021 ◽  
Vol 97 (3) ◽  
pp. 227-237
Author(s):  
Kasturi Chakraborty ◽  
Prabir Kumar Mukhopadhyay ◽  
Sandip Nandy
Keyword(s):  
Lithos ◽  
2006 ◽  
Vol 86 (1-2) ◽  
pp. 137-166 ◽  
Author(s):  
L.S. Lauri ◽  
O.T. Rämö ◽  
H. Huhma ◽  
I. Mänttäri ◽  
J. Räsänen

Geology ◽  
1989 ◽  
Vol 17 (4) ◽  
pp. 324 ◽  
Author(s):  
Suzanne Mahlburg Kay ◽  
Victor A. Ramos ◽  
Constantino Mpodozis ◽  
Patricia Sruoga

Elements ◽  
2016 ◽  
Vol 12 (2) ◽  
pp. 91-96 ◽  
Author(s):  
Craig C. Lundstrom ◽  
Allen F. Glazner
Keyword(s):  

2020 ◽  
Author(s):  
Gerhard Wörner ◽  
Elena Belousova ◽  
Simon Turner ◽  
Jelte Kemann ◽  
Axel K Schmitt ◽  
...  

<p>Silicic magmatism in the Central Andes forms rhyolitic to dacitic volcanic deposits that range from large-volume ignimbrites (>1000 km3) to small local dome eruptions. The mass proportion between mantle-derived magmatic contributions to crustal melting was previously estimated to range from 20 to 70 % based on Sr-O isotope data obtained on separated feldspar and quartz contained as crystal cargo. New O-Hf isotope data from in-situ ion-probe and laser ablation measurements of U-Pb-dated zircons further constrain type, proportion, and processes of crustal input into silicic magmas. Variations in time and space of these geochemical parameters are documented here using representative samples that cover the entire Central Andes over 20 Ma and 800 km distance. Systematic covariations in isotope tracers relate to increasing crustal thickening through time during Andean orogenesis. Collectively, Sr-Nd-Pb-Hf-O isotopic signatures vary in space and time and temporally reflect increasing crustal input during ignimbrite flare-ups as the crust becomes thermally matures. Spatial variations derive from different crustal domains in the Central Andes and reflect the different age and composition of crustal components.</p><p>Remarkably, inherited zircon representing basement involved in crustal assimilation is exceedingly rare over the entire province. This most probably reflects high temperatures that exceed zircon saturation temperatures of crustal melts in ignimbrite-forming magmas. This observation distinguishes silicic ignimbrite-forming magmatism from typical granitoid-forming magmatism in orogenic settings where abundant older zircons inherited from the crust are commonly found.</p>


Geology ◽  
2020 ◽  
Vol 48 (12) ◽  
pp. 1174-1178 ◽  
Author(s):  
Brenda C. Rocha ◽  
Joshua H.F.L. Davies ◽  
Valdecir A. Janasi ◽  
Urs Schaltegger ◽  
Antônio J.R. Nardy ◽  
...  

Abstract The Valanginian Stage is marked by a period of global positive δ13C carbon cycle perturbation and biotic crises, which are collectively referred to as the Valanginian event (VE). Many attempts have been made to link the Paraná-Etendeka large igneous province volcanism with the VE. However, currently there is no conclusive proof to support this hypothesis, since the timing and duration of the volcanic activity are not known with sufficient precision. In this study, we significantly revise the time scales of magmatism and environmental impact of the Paraná magmatic province (PMP) in Brazil with new high-precision zircon U-Pb ages from the low-Ti Palmas and high-Ti Chapecó sequences. Our data demonstrate that significant volumes of low-Ti silicic rocks from the PMP erupted rapidly at ca. 133.6 Ma within 0.12 ± 0.11 k.y. The age of the high-Ti Chapecó sequence from central PMP is constrained at ca. 132.9 Ma and thus extends the duration of magmatic activity by ∼700 k.y. Our new ages are systematically younger than previous ages and postdate the major positive carbon isotope excursion, indicating that PMP silicic magmatism did not trigger the VE but could have contributed to extending its duration. Within the framework of the stratigraphic column of the PMP, the earliest low-Ti basalts could have been responsible for the VE if they are at least 0.5 m.y. older than the low-Ti silicic rocks dated herein.


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