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Magmatic History and Crustal Genesis of : Constraints from U-Pb Ages and Hf of Detrital in Modern Rivers

Item Type text; Electronic Dissertation

Authors Pepper, Martin Bailey

Publisher The University of Arizona.

Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author.

Download date 23/09/2021 09:38:39

Link to Item http://hdl.handle.net/10150/347220

MAGMATIC HISTORY AND CRUSTAL GENESIS OF SOUTH AMERICA: CONSTRAINTS FROM U-Pb AGES AND Hf ISOTOPES OF DETRITAL ZIRCONS IN MODERN RIVERS

by

Martin Pepper

______Copyright © Martin Pepper 2014

A Dissertation Submitted to the Faculty of the

DEPARTMENT OF GEOSCIENCES

In Partial Fulfillment of the Requirements

For the Degree of

DOCTOR OF PHILOSOPHY

In the Graduate College

THE UNIVERSITY OF ARIZONA

2014

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THE UNIVERSITY OF ARIZONA GRADUATE COLLEGE

As members of the Dissertation Committee, we certify that we have read the dissertation prepared by Martin Pepper, titled Magmatic History and Crustal Genesis of South America: Constraints from U-Pb ages and Hf isotopes of detrital zircons in modern rivers and recommend that it be accepted as fulfilling the dissertation requirement for the Degree of Doctor of Philosophy.

______Date: (11/17/2014) Peter Reiners

______Date: (11/17/2014) Paul Kapp

______Date: (11/17/2014) George Zandt

Final approval and acceptance of this dissertation is contingent upon the candidate’s submission of the final copies of the dissertation to the Graduate College.

I hereby certify that I have read this dissertation prepared under my direction and recommend that it be accepted as fulfilling the dissertation requirement.

______Date: (11/17/2014) Dissertation Director: George Gehrels

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STATEMENT BY AUTHOR

This dissertation has been submitted in partial fulfillment of the requirements for an advanced degree at the University of Arizona and is deposited in the University Library to be made available to borrowers under rules of the Library.

Brief quotations from this dissertation are allowable without special permission, provided that an accurate acknowledgement of the source is made. Requests for permission for extended quotation from or reproduction of this manuscript in whole or in part may be granted by the copyright holder.

SIGNED: MARTIN PEPPER

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ACKNOWLEDGEMENTS

I would like to express my deepest gratitude to Professor George Gehrels for giving me this opportunity to execute such a unique research project and further my knowledge and experiences. The opportunities gained now and in the future are irreplaceable and I am eternally thankful for my new directions in life.

I would also like to thank my wife Lena Pepper for her support and understanding during this long academic stint with long hours and little time outside of my projects.

Thank you mother (Karen Pepper) and father (Carl Pepper) for always encouraging me to keep learning and allowing me to push my boundaries.

I am also very thankful for my colleagues and the other students in our department that were extremely helpful in this project, namely, Mauricio Ibanez-Mejia, Alex Pullen, Ned Brown, Mark Pecha, Jay Quade, Gayland Simpson, Dominique Giesler, Chelsea White, Clayton Loehn, Glynis Jehle and Victor Valencia.

Furthermore, I couldn’t have completed such an arduous journey throughout South America without the help of my field crew: Franco Urbani, David Mendi, Agustin Cardona, Camilo Bustamante, Giovani Jimenez and Herman Bayona.

Thank you!

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TABLE OF CONTENTS

LIST OF FIGURES………………………………………………………………………... 6 LIST OF TABLES………………………………………………………………………… 7 ABSTRACT……………………………………………………………………………….. 8 INTRODUCTION…………………………………………………………………………. 10 GEOLOGICAL FRAMEWORK OF SOUTH AMERICA………………………………... 13 Cratonal Nucleus…………………………………………………………... 13 Northern (NA)…………...…………………………………………. 14 Central Andes (CA)………………...……………………………………… 14 Southern Andes (SA)……………………..……………………………….. 14 PRESENT STUDY………………………………………………………………………… 16 Sampling Methodology……………………………………………………………. 16 Sample Descriptions……………………………………………………………….. 16 Northern Andes (NA)………………………………………………………. 16 Central Andes (CA)………………………………………………………… 17 Southern Andes (SA)……………………………………………………….. 17 U-Pb Analytical Methods………………………………………………….. 17 Hf Analytical Methods…………………………………………………….. 18 RESULTS………………………………………………………………………………….. 21 U-Pb Geochronology………………………………………………………………. 21 Northern Andes (NA)………………………………………………………. 21 Central Andes (CA)………………………………………………………… 21 Southern Andes (SA)……………………………………………………….. 21 East-West comparison of U-Pb ages………………………………………. 22 Hf Geochemistry…………………………………………………………... 22 Northern Andes (NA)………………………………………………………. 22 Central Andes (CA)………………………………………………………… 22 Southern Andes (SA)……………………………………………………….. 23 COMPARISON WITH EXISTING U-Pb AND Hf DATA FROM SOUTH AMERICA… 24 U-Pb………………………………………………………………………………... 24 HF………………………………………………………………………………….. 25 INTERPRETATION OF RESULTS………………………………………………………. 26 Magmatic History…………………………………………………………………. 26 Crustal Evolution………………………………………………………………….. 28 DISCUSSION……………………………………………………………………………… 33 Magmatic Processes……………………………………………………………….. 33 Crustal Generation and Reworking………………………………………………... 35 CONCLUSIONS…………………………………………………………………………... 37 ACKNOWLEDGEMENTS……………………………………………………………….. 40 APPENDIX A. FIGURE 1. GEOLOGIC MAP WITH OUTLINED CATCHMENTS…. 41 APPENDIX B. U-Pb REFERENCES USED IN ATTACHED DATA COMPILATION .. 44 APPENDIX C. Hf REFERENCES USED IN ATTACHED DATA COMPILATION…... 88 REFERENCES…………………………………………………………………………….. 106

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LIST OF FIGURES

FIGURE 1. MAP OF RESEARCH AREA……………………………………………….. 90 FIGURE 2. U-PB AND HF FOR NA ………………………………………….. 91 FIGURE 3. U-PB AND HF FOR CA REGION ………………………………………….. 92 FIGURE 4. U-PB AND HF FOR SA REGION ………………………………………….. 93 FIGURE 5. U-PB DISTRIBUTIONS OF ALL AREAS………………………………….. 94 FIGURE 6. 0-200MA DISTRIBUTIONS FOR ALL AREAS..………………………….. 95 FIGURE 7. MAP OF SAMPLE LOCATIONS OF COMPILED DATA.……………….. 96 FIGURE 8. SUMMARY OF U-PB AND HF FOR NA REGION ……………………….. 97 FIGURE 9. SUMMARY OF U-PB AND HF FOR CA REGION ……………………….. 98 FIGURE 10. SUMMARY OF U-PB AND HF FOR SA REGION ………………………. 99 FIGURE 11. SUMMARY OF U-PB AND HF FOR ALL ……………………. 100 FIGURE 12. 0-200MA U-PB, HF AND CONVERGENCE DATA OF ALL REGIONS..101-102 FIGURE 13. COMPARISON OF THIS PROJECT WITH GLOBAL DATA…………… 103 FIGURE 14. COMPARISON OF THIS PROJECT WITH HASCHKE ET AL., 2002… 104

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LIST OF TABLES

TABLE 1. SAMPLE INFORMATION…………………………………………………… 105

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ABSTRACT

South America provides an outstanding laboratory for studies of magmatism and crustal evolution because it contains older Archean-Paleoproterozoic that amalgamated during

Mesoproterozoic and assembly, as well as a long history of

Andean magmatism that records crustal growth and reworking in an accretionary orogen. We have attempted to reconstruct the growth and evolution of South America through U-Pb geochronology and Hf isotope analyses of detrital zircons from 59 samples of sand from modern rivers and shorelines. Results from 5,524 new U-Pb ages and 1,199 new Hf isotope determinations are reported. We have also integrated our data into a compilation of all previously published geochronologic and Hf isotopic information, yielding a record that includes

>42,000 ages and >1,600 Hf isotope analyses. These data yield five main conclusions: (1) South

America has an age distribution that is similar to most other , presumably reflecting the , with maxima at 2.2-1.8 Ga, 1.6-0.9 Ga, 700-400 Ma, and 360-200 Ma;

(2) <200 Ma magmatism along the western margin of South America has age maxima at 183 Ma

(191-175 Ma), 151 Ma (159-143 Ma), 126 Ma (131-121 Ma), 109 Ma (114-105 Ma), 87 Ma (95-

79 Ma), 62 Ma (71-53 Ma), 39 Ma (43-35 Ma), 19 Ma (23-15 Ma), and 6 Ma (10-2 Ma); (3) for the past 200 Ma, there appears to be a positive correlation between magmatism and the velocity of convergence between central South America and Pacific oceanic plates; (4) Hf isotopes record reworking of older crustal materials during most time periods, with incorporation of juvenile crustal materials at ~1.6-1.0 Ga, 500-400 Ma and ~200-100 Ma; and (5) the Hf isotopic signature of <200 Ma magmatism is apparently controlled by the generation of juvenile during extensional tectonism and reworking of juvenile versus evolved crustal materials during crustal thickening and arc migration.

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Keywords: Detrital zircon, U-Pb geochronology, Andes, South America, Hf isotopes, orogenic cycles, crustal evolution

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INTRODUCTION

The ‘Andean type’ is frequently referenced as a modern analog for the based orogeny of a current or an ancient oceanic plate beneath a continental plate (Hodges et al., 1982).

The problem with this statement is that we still do not completely understand what has been occurring along this Pacific margin in terms of magmatic flux and crustal evolution either in a regional context, east and west variations and/or along the entire ~7000 km length of the Andes.

Ideally, a single project would encompass the whole Andes in order to compare and contrast the different aspects of this orogen while minimizing bias and error from multiple researchers, sampling strategies and data gathering instruments. In order to execute a project of this scale a novel technique needs to be used that not only collects the most information but also reduces possible biases. Since rivers are the major conduit for transporting from mountains to basins and oceans, employing river sands not only increases the regions sampled (see catchment sizes in Appendix 1 Table 1 and Fig. 1), but also adds a random sampling aspect that allows for a more robust sampling approach. Rivers are actively eroding what they come in contact with, thus samples will not only contain information on the latest magmatic events but also the old recycled orogenic detritus.

Understanding the generation and reworking of continental has been a long- standing goal in science (Armstrong, 1968). South America provides an excellent laboratory for studying crustal evolution because it contains older cratons that record

Precambrian crustal genesis and assembly, and also early through modern magmatic assemblages that formed along a convergent/accretionary plate boundary along the western margin (Cordani et al., 2000; Acenolaza et al., 2002; Cawood, 2005; Franz et al., 2006; Cawood and Buchan, 2007; Ramos, 2009). This history has been reconstructed through a large number of

10 detailed studies of specific areas (e.g., Loewy et al., 2004; Herve et al., 2007; Augustsson and

Bahlburg, 2008; Chew et al., 2008; Miskovic et al., 2009; Bahlburg et al., 2009, 2011), as well as several syntheses that have focused on the assembly of South America (e.g., Goodwin, 1996) and the evolution of the Andean margin (e.g., Acenolaza et al., 2002; Haschke et al., 2002; Cawood,

2005; Cediel et al., 2003; Franz et al., 2006; Kay et al., 2005; Cawood and Buchan, 2007).

This study attempts to reconstruct the magmatic history and crustal evolution of South

America through U-Pb geochronologic and Hf isotopic analysis of detrital zircon grains from 59 samples of modern sediment (Fig. 1). Combined U-Pb geochronology and Hf isotope analysis in zircon is a powerful method for evaluating the evolution of large regions with the power of sedimentary averaging (Link et al., 2005), the durability of zircon even under most P-T conditions (Speer, 1982), the ability of U-Pb geochronology to record to intermediate- composition magmatism (e.g, Condie et al., 2011), and the petrogenetic information provided by

Hf isotopes (e.g, Augustsson et al., 2006; Bahlburg et al., 2009, 2011; Hawkesworth et al., 2010;

Dhuime et al., 2011).

It is important to note, however, that the age and Hf isotopic signature of detrital zircons provides only indirect information on magmatic history and crustal evolution. A full analysis would require consideration of (1) variations in zircon abundance related to rock composition

(e.g., SiO2 and/or Zr content) (Moecher and Samson, 2006; Dickinson 2008), (2) 3-dimensional analysis of the volumes of present in the Andes through time (e.g., Paterson and

Ducea, in press), and (3) the importance of crustal additions and removals arising from tectonic processes (e.g., , subduction ), delamination/relamination, and erosion.

Such analyses are beyond the scope of this paper, but will be facilitated by the new and compiled information presented herein.

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Our study complements the work of Rino et al. (2004, 2008), Condie et al. (2005, 2009),

Mapes et al. (2005), and Iizuka et al. (2010), who presented ages of detrital zircons from modern sand samples along the Amazon and Paraná Rivers. To complement the information from large rivers, we include samples from numerous smaller river systems (e.g., Milliman and Syvitski,

1992) that are present along the eastern and western flanks of the modern Andes.

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GEOLOGICAL FRAMEWORK OF SOUTH AMERICA

The South American consists, to first order, of several Archean-

Paleoproterozoic cratons that were effectively welded together during Mesoproterozoic through early Paleozoic orogenesis (Goodwin, 1996). This continental cratonic nucleus served as the backstop for accretionary processes that formed the Andean orogen along the Paleo-Pacific margin (Coney, 1992; Cawood, 2005; Cawood and Buchan, 2007). The following sections outline the geologic evolution of cratonal South America and the northern, central, and southern

Andes, with an emphasis on patterns of magmatism and crustal generation/reworking (Fig. 1).

Cratonal Nucleus

The nucleus of South America consists mainly of the Amazon, Sao Francisco, Parana, and Rio de la Plata cratons (Fig. 1). The Central Amazon (CAm) has Archean ages from

3.3–2.5 Ga. The Maroni-Itacaiunas province (MI) occurs east of the CAm with radiometric ages between 2.2–1.9 Ga. Westward, the Ventuari-Tapajos (VT) mobile belt (2.0–1.8 Ga) and the Rio

Negro Juruena mobile belt (RNJ; 1.8–1.6 Ga) formed during the accretion of intraoceanic arcs.

The Rodonian San Ignacio (RSI) province (1.6–1.3 Ga) consists of accreted arc and micro-continents that experienced high grade during Mesoproterozoic time

(Teixeira et al., 1989; Tassinari and Macambira 1999; Santos et al., 2000, 2008; Cordani and

Teixeira, 2007; Cordani et al., 2009). Along the western margin of the Amazon craton is the

Sunsas orogen, which yields ages between 1.2 and 0.9 Ga (Litherland and Power, 1989; Teixera et al., 2010; Ibanez-Mejia et al., 2011). Separating these cratons are the Brasiliano mobile belts, with dominant magmatism during Neoproterozoic-earliest Paleozoic (0.7–0.5 Ga) time

(Goodwin 1996; Rapela et al., 1998, 2007; Kröner and Cordani, 2003; Valeriano et al., 2008;

Cordani et al., 2009; and Cordani, 2009).

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Northern Andes (NA)

The northern Andes are divided into three separate mountain ranges that consist mainly of (Cordani et al., 2005; Ordóñez- Carmona et al., 2006; Ibanez-Mejia et al., 2011). The western Cordillera (w of Fig. 1) comprises oceanic magmatic and deep-marine sedimentary rocks (McCourt et al., 1984; Cortés et al., 2005; Kennan and Pindell,

2009; Borrero et al., 2012). The main along the central Cordillera (c of Fig. 1) is composed mainly of -Cretaceous igneous rocks intruded into and resting on both oceanic and continental crystalline basement (Aspden and McCourt, 1986; Aspden et al., 1987; Cediel et al., 2003). The eastern Cordillera (e of Fig. 1) consists of Mesoproterozoic-Archean inliers surrounded by 1.1–1.0 Ga rocks (Restrepo-Pace et al., 1997; Ruiz et al., 1999; Cordani et al.,

2005; Jiménez-Mejía et al., 2006; Ordóñez-Carmona et al., 2006; Chew et al., 2007a, 2007b,

2008; Cardona et al., 2009; Miskovic et al., 2009; Ibanez-Mejia et al., 2011).

Central Andes (CA)

The central Andes consist of arc-type and basinal assemblages that formed in a convergent-margin setting from early Paleozoic time to the recent. Some of these assemblages may belong to terranes that are exotic to South America (e.g., terrane; Astini et al.,

1999; Ramos, 2004; Thomas et al., 2004; Finney, 2007), whereas most formed during long-lived accretionary tectonism along the proto-Andean margin (Cawood, 2005). Some of these terranes contain older basement (Shackleton et al., 1979; Loewy et al., 2004; Chew et al.,

2007a). The eastern CA also includes uplifted Neoproterozoic basement (Allmendinger et al.,

1997; Jordan and Allmendinger 1986; Strecker et al., 1989; Escayola et al., 2007).

Southern Andes (SA)

The SA consist primarily of Paleozoic and Proterozoic rocks exposed in basement uplifts

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(Pankhurst et al., 2000; 2006; Augustsson et al., 2006), rimmed to the west by post- magmatic rocks of the Andean orogen (Kay et al., 2005; Herve et al., 2007). The southern portion of SA belongs to the microcontinent, which consists of widespread Paleozoic magmatic arcs and marine basins that formed in the broad accretionary orogen

(Coney, 1992; Stern and De Wit, 2003; Cawood and Buchan, 2007; Ramos, 2008; Barbeau et al.,

2009).

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PRESENT STUDY

Sampling Methodology

Samples were collected from active channels of modern rivers and from beaches along shorelines. Most of the rivers sampled do not have dams or major construction projects that could have influenced zircon distributions. Each sample consisted of a mixture of sediment from multiples sites (within a ~10 m2 area) with a wide range of grain sizes (silt to coarse sand).

Material coarser than 2 mm was removed during sample collection. This strategy was followed in an effort to maximize the number of age groups recognized and reduce biases from hydrodynamic sorting (Garzanti et al., 2009; Lawrence et al., 2011). Heavy minerals from each composite sample were initially concentrated with a pan, and then zircons were extracted using a Frantz isodynamic separator and heavy liquids (techniques described by Gehrels, 2000).

Sample Descriptions

Fifty-nine samples were collected from rivers draining the northern, central, and southern

Andes and from beach deposits along these rivers (Fig. 1; Table 1).

Northern Andes (NA)

Thirteen samples were collected from the northern Andes as follows. Sample NA01 was collected from the Caribbean coast. Seven samples were collected from the Magdalena River system in the Magdalena Valley (separating the eastern and central Cordilleras of Figure 1), with

NA02 from lowlands 140 km upstream, NA03-04 from the Magdalena delta, NA05 along the coast 70 km west of the Magdalena delta, and NA06-09 from the flanks of the eastern and western Cordillera (EC and CC) in the Magdalena highlands. Four samples were collected farther south, with NA10 from the Andean highlands, NA11 from a tributary of the Amazon

River system, and NA12- NA13 along the western flank of the western Cordillera (w of Fig. 1).

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Central Andes (CA)

Twenty-five samples were collected from both the western and eastern flanks of the

Central Andes, with a spacing of approximately 300-400 km. Along the eastern flank of the

Andes, CA01-04 were collected from tributaries of the Rio de la Plata river system, CA05-06 are from tributaries of the system, CA07-08 are from the Andean highlands, and

CA09-10 are from southern Amazon tributaries. Along the western flank of the Andes, samples

CA11-23 were collected along the from small perennial rivers. CA16 and CA23 are from beach sands to the west.

Southern Andes (SA)

Five SA samples (SA01-05) were collected from the western flank of the orogen from rivers with a spacing of ~300 km. Samples SA01 and SA02 are from perennial rivers within 10 km of the coast, whereas sample SA03 was collected from the coast and SA04 was collected farther upstream. SA06-SA22 are from the eastern flank of the Andes, with a spacing of ~200 km. These samples are from lowland portions of rivers, approximately 30-50 km from the

Atlantic coast.

U-Pb Analytical Methods

U-Pb geochronology of zircons was conducted by laser ablation multicollector inductively coupled plasma mass spectrometry (LA-MC-ICPMS) at the Arizona LaserChron

Center (www.laserchron.org) using analytical methods described by Gehrels et al. (2006, 2008) and Gehrels and Pecha (2014). Cathodoluminescence (CL) images, acquired with a Gatan

Chroma CL2 system (www.geosemarizona.org), were used to ensure that analyses were conducted on homogeneous (generally interior) portions of zircon grains.

The U-Pb analytical data are reported in Appendix A Tables 2-4. These tables present the

17 isotopic ratios, concentrations, calculated ages, and uncertainties for each analysis. Uncertainties are reported at 1-sigma, and include only internal uncertainty components (measurement of

206Pb*/238U, 206Pb*/207Pb*, 206Pb*/204Pb), and a factor to incorporate the over dispersion of primary standard analyses. Systematic (external) uncertainties are reported for each sample (at 2- sigma) in Appendix A Tables 2-4, and include contributions from the scatter of primary standard analyses, composition of common Pb, age of the primary standard, and U decay constants. Also reported for each analysis is the “Best Age,” which is based on 206Pb*/238U for <900 Ma grains and 206Pb*/207Pb* for >900 Ma grains.

Not included in these tables are analyses that are highly (>20%) discordant or highly

(>10%) reverse discordant, and analyses with >10% uncertainty. These filters are not applied to

<600 Ma 206Pb*/207Pb* ages and <100 Ma 206Pb*/238U ages. Also included in Appendix A

Tables 2-4 are Pb*/U concordia diagrams and relative age-probability diagrams (from Ludwig,

2008). The age-probability diagrams sum all ages (and associated uncertainties) from a sample into a single curve.

For interpretive purposes, U/Th ratios for each analysis are reported in Appendix A

Tables 2-4. Most (>90%) analyses have U/Th in the range of typical igneous values (e.g., 1-10;

Rubatto, 2002), suggesting that most ages record episodes of igneous activity. Values >10 are interpreted as possibly of metamorphic origin (e.g., Gehrels et al., 2009).

Hf Analytical Methods

Hf analyses were also conducted by LA-MC-ICPMS at the Arizona LaserChron Center, using methods described by Cecil et al. (2011) and Gehrels and Pecha (2014). Laser ablation analyses were conducted with a laser beam diameter of 40 microns, with ablation pits located either on top of the U-Pb analysis pits or adjacent to the U-Pb pit but in the same domain (using

18

CL images as guides). Each acquisition consisted of one 40-second integration on backgrounds

(on peaks with no laser firing) followed by 60 one-second integrations with the laser firing. The isotope ratios and uncertainties reported are based on all measurements, with only a 2-sigma filter to remove outliers. Critical isotope ratios used in data reduction are as follows: 179Hf/177Hf

= 0.73250 (Patchett and Tatsumoto, 1980); 173Yb/171Yb = 1.132338 (Vervoort et al., 2004);

176Yb/171Yb = 0.901691 (Vervoort et al., 2004; Amelin and Davis, 2005); 176Lu/175Lu = 0.02653

(Patchett, 1983); and the decay constant of 176Lu = 1.867e-11 (Scherer et al., 2001; Söderlund et al., 2004). Hf Depleted Mantle model ages are not calculated because of uncertainties in the

176Hf/177Hf and 176Lu/177Hf of source material(s) from which the zircons crystallized.

Analyses were calibrated using solution analyses of JMC475, solutions of JMC475 mixed with varying concentrations of 176Lu and 176Yb, and laser ablation analyses of standard zircons

Mud Tank, 91500, Temora2, R33, FC1, and Plesovice. Solutions of JMC475 yielded a weighted mean value of 0.282156± 0.000007 (2, n=17). Solutions mixed with 176Yb and 176Lu [with

176(Yb+Lu)/176Hf up to 1.6] yielded a similar weighted mean value of 0.282150± 0.000008 (2, n=16) with 173Yb/171Yb adjusted to 1.132423 (from value of 1.132338 suggested by Vervoort et al., 2004) to alleviate a correlation between measured 176Hf/177Hf and 176(Yb+Lu)/176Hf.

Zircon standards yielded 176Hf/177Hf values that were generally lower than previously reported values. With measured values increased by 0.8 epsilon units, the following results were obtained:

 Mud Tank: weighted mean value of 0.282518 ± 0.000007 (2, n) compared with

reported value of 0.282507 (Woodhead and Hergt, 2005). This yields an offset of +0.4

epsilon units.

 91500: weighted mean value of 0.282292 ± 0.000021 (2, n) compared with reported

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value of 0.282313 (Fisher et al., 2014). This yields an offset of -0.7 epsilon units.

 Temora2: weighted mean value of 0.282677 ± 0.000009 (2, n) compared with reported

value of 0.282686 (Fisher et al., 2014). This yields an offset of -0.3 epsilon units.

 Plesovice: weighted mean value of 0.282480 ± 0.000007 (2, n) compared with

reported value of 0.282484 (Slama et al., 2008). This yields an offset of -0.1 epsilon units.

 FC1: weighted mean value of 0.282170 ± 0.000009 (2, n) compared with reported

value of 0.282183 (Fisher et al., 2014). This yields an offset of -0.4 epsilon units.

 R33: weighted mean value of 0.282735 ± 0.000009 (2, n) compared with reported

value of 0.282764 (Fisher et al., 2014). This yields an offset of -1.0 epsilon units.

These offsets suggest that the accuracy (external reproducibility) of a set of analyses is ~2 epsilon units. The precision (internal reproducibility) of individual analyses is 2-3 epsilon units, as indicated by an average measurement uncertainty of 3.3 epsilon units (average standard deviation of all standard measurements, at 2), and an average standard deviation for measurements of each standard of 2.8 epsilon units (at 2).

Data from all unknowns have been adjusted using a correction factor of +0.8 epsilon units, and the revised 173Yb/171Yb value reported above.

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RESULTS

U-Pb Geochronology

A total of 5,524 new U-Pb analyses are reported in Appendix A Tables 2-4. Appendix A

Table 1 provides a description of the zircon grains present in each sample. Highlights of the results from samples from northern, central, and southern regions are described in following sections and shown on Figures 2-4. Figures 5 and 6 summarize the U-Pb age distributions from each region.

Northern Andes (NA)

Samples from the northern Andes contain detrital zircons that are quite variable in age

(Fig. 2). Most samples contain a few ages between ~2100-1700 Ma. The only age group that is present in most samples ranges from ~1600 to 950 Ma, with dominant ages near ~1000 Ma.

Several samples contain grains of ~700-400 Ma, and most samples contain abundant <400 Ma grains. The dominant ages for <200 Ma grains are shown on Figure 6.

Central Andes (CA)

For >200 Ma ages, the age patterns in the central Andes (Fig. 3) generally resemble data from regions to the north (Fig. 2), although proportions of the main age groups are somewhat different (Fig. 5). Namely, most samples are missing the ~1600 to 950 Ma and 400 to 200 Ma age groups. Similarly, for <200 Ma ages, some age groups (e.g., ~183 and ~126 Ma) are also missing from CA, and the proportions of other age groups are somewhat different (Fig. 6). The

600 to 400 Ma age group is much more prominent in the CA than the NA.

Southern Andes (SA)

The southern Andes yield age distributions that are quite different than the NA and CA, with predominance of 400-250 Ma and <25 Ma grains in most samples, and abundant 200-25 Ma

21 ages in only three samples (Figs. 4-6). SA samples contain very few ages between 900-700 Ma ands > 1200 Ma.

East-West comparison of U-Pb ages

As a complement to the above north-south comparison of ages, Figures 5 and 6 compare age distributions from rivers that are located along the eastern versus western flanks of the modern Andes. Omitted from this compilation are samples from the rivers in the northernmost

Andes (which drain northward) and in southern Patagonia (which have no sampled westerly counterpart). This comparison highlights the dominance of older basement sources in rivers of the eastern Andes, versus the prevalence of Phanerozoic igneous rocks in the western Andes.

This compilation also records a strong cyclicity to Andean magmatism, which is explored in detail below.

Hf Isotope Geochemistry

The results of our Hf isotope analyses are described in the following sections for samples from the northern, central, and southern Andes. A total of 1,199 new analyses are reported in

Appendix A Tables 5-7. These tables report all details of individual analyses, and show plots with results from each sample. Results are summarized on Figures 2-4.

Northern Andes

Hf isotope data from the northern Andes are quite variable, and record interesting patterns through time. As shown on Figure 2, epsilon Hf values progressively decrease (become more evolved) from ~1600 Ma through ~400 Ma, increase (become more juvenile) from ~300 to

~100 Ma, and then in most cases become more evolved again after ~100 Ma (Fig. 2).

Central Andes

Analyses from the central Andes reveal a generally similar pattern of changing epsilon Hf

22 values (Fig. 3). Additional patterns include the presence of more abundant >1600 Ma grains with variable epsilon Hf values, more juvenile values for 1.2-1.0 Ga grains, a distinctive pull-down of

650-500 Ma values, and considerably more negative epsilon Hf values for the youngest grains.

Southern Andes

The southern Andes (Fig. 4) yield few >1.2 Ga grains, mostly juvenile 1.2-1.0 Ga grains, abundant 600-300 Ma grains with intermediate epsilon Hf values, values that increase from moderately negative to positive from 300 to 100 Ma, and then mostly positive values for <100

Ma grains.

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COMPARISON WITH EXISTING U-Pb AND Hf DATA FROM SOUTH AMERICA

U-Pb

In an attempt to compare our U-Pb geochronologic data set with previously published information, we have compiled ages reported from igneous and detrital samples from all of western South America (Fig. 7). All available U-Pb ages are included in the compilation, whereas only young (<200 Ma) volcanic K-Ar and Ar-Ar ages are included because of the likelihood that pre-200 Ma ages record cooling rather than igneous activity. Ages of individual analyses are included where reported; mean ages are reported where results from individual analyses are not available. Appendix B Table 1 includes all compiled ages, with corresponding references listed in Appendix B below. A total of 26,851 detrital ages and 9,929 igneous ages are included in this compilation, in addition to our 5,524 new ages.

Comparisons between our detrital data, previously published detrital data from both sedimentary rocks and modern sediment, and igneous rocks are provided on Figure 5. This comparison shows that our data and previously reported detrital data are quite similar in the dominant ages recognized, and in the approximate proportions of different age groups. These two data sets are somewhat different from the age distribution defined by igneous samples, presumably because of biases in sample selection.

Included in this compilation are analyses of detrital zircon ages from several South

American rivers. Condie et al. (2005, 2009) report ages from rivers in Brazil and , whereas

Iiuzka et al. (2010) and Rino et al. (2004, 2008) report ages from the Amazon and Parana rivers.

Mapes et al. (2009) have also conducted analyses from Amazon river sediment, with analyses that are forthcoming. Campbell and Allen (2008) have included analyses from South American rivers in their database, but these ages have not been included in our compilation because sample

24 locations were not reported.

Hf

Hf data were also compiled from previous studies that reported essential information about the analyses (e.g., instrumentation, methodology, and data reduction). The acceptable data are tabulated in Appendix C Table 1, with associated references reported in Appendix C below. No acceptable analyses are available for the northern Andes, 351 were found from the central Andes, and 85 from the southern Andes. As shown on Figures 8-11, the published data are quite similar to our new results.

25

INTERPRETATION OF RESULTS

Our new and compiled data provide significant new insights into the magmatic history and crustal evolution of South America. Each of these aspects is described below.

Magmatic History

The U-Pb data presented herein, combined with existing geochronologic information and interpretations (e.g., Cediel et al., 2003; Franz et al., 2006; Pankhurst et al., 2006; Miskovic et al., 2009), provide important new information about the history of magmatism in South America.

This record is most relevant for igneous activity of felsic to intermediate composition, given that most of the information is derived from ages of zircon, and zircon is of low abundance in magmas. As noted above, the connection between age distribution and magmatic flux is also complicated by potential variations in Zr content (and hence zircon fertility) through space and time, the long and complex history of uplift and erosion in the Andes, and potential additions and removals from the system by tectonic and erosional processes.

Given the objective of reconstructing the magmatic history of South America, with emphasis on both ages and proportions of magmatism, it is important to recognize that all three sets of information (our data, published detrital data, and published igneous data) have biases.

For igneous ages, it is clear that the age distribution is controlled in large part by the geographic and temporal focus of the constituent studies. This is apparent in the igneous age distribution

(Figures 5 and 6) by the large proportion of young igneous ages, which reflects the large number of studies of Andean magmatism. In contrast, previously published detrital ages from are biased away from these young ages, given that detrital zircons in sandstones always predate deposition. The detrital ages reported herein are biased toward contributions from the modern

Andes, given that most rivers in South America have headwaters in the Andes, and that most of

26 our samples were collected from within or adjacent to the Andes. It is also important to note that detrital age distributions may over-represent older sources given the tendency for zircon grains to be recycled. For these reasons, the following discussions focus on general patterns of ages, with the assumption that short-term variations in the proportion of ages may reflect true variations in magmatic addition, whereas variations over longer time periods may be controlled mainly by geologic or sampling biases.

Figure 5 shows that there are notable similarities in all three records. Most impressive is the similarity in detrital data sets from this study and previous studies in terms of both presence/absence of ages and proportions of ages. Igneous ages are also similar for most areas and time periods, but, as noted above, emphasize young Andean magmatism.

One of the first-order patterns apparent in all data sets is the relatively low abundance of pre-1.2 Ga ages, in spite of the fact that much of South America is underlain by Archean and

Paleoproterozoic cratonal rocks (Fig. 1). This low abundance is due in part to biases in sampling

(as noted above), but also suggests that little Archean-Paleoproterozoic cratonal material is present in the modern Andes.

The oldest significant age group includes 1.2-1.0 Ga grains, at least for the central and northern Andes. These 1.2-1.0 Ga grains presumably record magmatism within the Sunsas belt

(Fig. 1), which is exposed along the eastern flank of the northern and central Andes. Grains of these ages may also have been distributed widely across South America during Mesoproterozoic tectonism, as has been documented for sediment derived from the Grenville orogen in North

America (e.g., Rainbird et al., 2012).

The next main phase of magmatism recorded in the three data sets begins at ~700 Ma and extends into early Paleozoic time. This magmatism occurred within the Brasiliano belt (0.7-0.5

27

Ga) during assembly of the South American craton, which coincides with the Pan-African orogeny and the assembly of (Windley, 1995; Brito Neves et al., 1999). This phase of continental assembly overlapped with the Late Neoproterozoic onset of magmatism along the western margin of South America in a broad and long-lived accretionary orogen (Coney, 1992;

Cawood, 2005; Cawood and Buchan, 2007). Igneous geochronology records magmatism along this convergent margin from ~610 Ma until ~470 Ma (Cawood and Buchan, 2007), which is also reflected in the record of detrital zircon ages (Fig. 5).

Our three geochronologic records all show a decrease in magmatism during mid-

Paleozoic time (~400 to 360 Ma), followed by significant magmatic addition between 360 and

200 Ma (Fig. 6). This pattern is quite similar to the magmatic history that Cawood and Buchan

(2007) reconstruct for the proto-Andes and other portions of the .

The data provide a rich record of variations in magmatism during the past ~200 Ma. As summarized on Figure 6 (which shows age distributions smoothed using a ±3 m.y. sliding window average), the record is somewhat different from east to west, from north to south, and in the three different data sets. Of significance is the occurrence of age maxima at 183 Ma (191-175

Ma), 151 Ma (159-143 Ma), 126 Ma (131-121 Ma), 109 Ma (114-105 Ma), 87 Ma (95-79 Ma),

62 Ma (71-53 Ma), 39 Ma (43-35 Ma), 19 Ma (23-15 Ma, and 6 Ma (10-2 Ma), with an average periodicity (from mid-points) of ~22 m.y. (vertical gray bars of Figure 6). This record is quite different from the apparent magmatic history from the south-central Andes presented by Haschke et al. (2002), as described below.

Crustal Evolution

The Hf data presented herein, combined with previously published Hf isotope analyses, provide new constraints on the crustal evolution of South America. All of the available data are

28 shown for NA, CA, and SA on Figures 8-10, and together for all areas on Figure 11.

Accompanying these Hf isotope plots are age-distribution diagrams for our new data as well as for all available (igneous and detrital) data.

Yellow arrows on these diagrams show interpreted trajectories of Hf evolution. Arrows with slopes that are parallel to average crustal evolution are interpreted to represent successive remelting of a relatively uniform suite of older crustal materials, with little addition of juvenile . Arrays that project toward more positive (or less negative) values than average crust are interpreted to record the additional input of juvenile magmas. Arrays that project toward more negative values than average crust may result from incorporation of a greater proportion of older crustal material (and hence less juvenile material), and/or involvement of increasingly negative crustal material.

Using this interpretive framework as a guide, the Hf data support the following history of crustal genesis and reworking for South America:

1. Grains that are >1.6 Ga in age are scarce (especially in NA) and epsilon Hf values are highly variable, but there is a general trend toward more negative epsilon Hf with time. This is interpreted to record Paleoproterozoic reworking of mostly Archean crustal materials, with little input of juvenile material. This history presumably pertains in large part to the cratonal rocks of

South America (Fig. 1).

2. Between ~1.6 Ga and ~1.0 Ga, epsilon Hf values in CA and possibly SA tend to become more positive, reflecting progressive incorporation of juvenile magmas. In contrast, epsilon Hf values in NA remain intermediate in value, reflecting lesser addition of juvenile crustal material. Given the proximity of the Sunsas belt with NA, the latter history may be relevant for the Mesoproterozoic crustal evolution of northern South America. The more juvenile

29

Mesoproterozoic zircons in CA and SA may have been shed from other regions, for example

North America, which yields positive epsilon Hf values for grains of this age (Gehrels and

Pecha, 2014). Distribution of these zircons may have occurred as part of a global sediment dispersal system during assembly of (e.g., Rainbird et al., 2011), or less likely, from early Paleozoic arrival of North American tectonic fragments with 1.2-1.0 Ga basement (e.g.,

Cuyania) along the Andean margin (e.g., Astini and Thomas, 1999; Thomas et al., 2004; Ramos

2004).

3. Between ~1.0 Ga and ~500 Ma, epsilon Hf values have trajectories that are generally similar to average crustal evolution (Figs. 8-11). This is interpreted to reflect mainly reworking of >1.0 Ga crustal materials, with little addition of juvenile magma. Franz et al. (2006) came to a similar conclusion on the basis of Sr-Nd isotope signatures of igneous and sedimentary rocks from the central Andes. In addition to this overall trend, there are apparent pull-downs (negative excursions) in epsilon Hf at about 650-550 and 500-450 Ma (Fig. 11). The older of these excursions likely reflects reworking of older crustal components in Brasiliano orogens, whereas the younger excursion may record involvement of older crustal components within early

Paleozoic arcs along the proto-Andean margin (blue line on Figure 1). It is interesting that other portions of the broad Terra Australis orogen are also characterized by significant reworking of older crustal materials during this time period (e.g., Cawood et al., 2009, 2012; Kemp et al.,

2009; Hawkesworth et al., 2010).

4. Early Paleozoic (500 to 400 Ma) magmatism contains epsilon Hf values that become more positive in the CA and SA. This ~100 m.y. progression towards an overall juvenile signature suggests an extensional tectonic regime with thinned and significant additions of mantle material related to the extensive early Paleozoic arc (e.g., Ducea et al., 2015).

30

5. Late Paleozoic (~360 to ~250 Ma) magmatism is treated separately from early

Paleozoic igneous activity based on a ~40 m.y. magmatic lull and a significant change in Hf isotope evolution. As shown on Figure 11, there is an overall trend toward more negative epsilon

Hf values during this time, reflecting increased involvement of older crustal materials in the late

Paleozoic magmatic arcs established along the Andean margin (Fig. 1). This trend is apparent in

NA (Fig. 8) and SA (Fig. 10), but is less obvious in the data from CA (Fig. 9). Involvement of continental material may have increased as the late Paleozoic arcs approached and were firmly accreted to the proto-Andean margin (e.g., Willner et al., 2008; Ramos, 2009; Bahlburg et al.,

2009).

6. Between ~250 and ~100 Ma, epsilon Hf values become more positive in all areas (Fig.

8-11), and mirror the presence of juvenile Sr-Nd-Pb isotopes in rocks of the central Andes (Franz et al., 2006) and epsilon Nd values in Patagonia (Herve et al., 2007). This trend is interpreted to result in large part from Triassic through extensional tectonism at the subduction plate boundary that is well documented all along the Andean margin (Fig. 12; Franz et al., 2006; Ramos, 2009; Maloney et al., 2013; Rossel et al., 2013). Such extension also manifests as widespread -related strata and normal faults of Triassic and Jurassic age (Ramos,

2009), formation of the Rocas Verdes back-arc basin in the southern Andes during Late Jurassic time (Dalziel et al., 1974), formation of the Salta rift system during Late Jurassic-Early

Cretaceous time (Salfity and Marquillas, 1994), and the opening of -floored basins during

Late Jurassic-Early Cretaceous time in the northern Andes (Maloney et al., 2013). The observed trend toward more positive epsilon Hf values may also have resulted from migration of the magmatic arc westward. As reported by Haschke et al. (2002) and Franz et al. (2006), the Late

Jurassic-Early Cretaceous magmatic arc was situated along the far western margin of the orogen,

31 which is underlain by Paleozoic arc terranes with little evolved continental material (Fig. 1).

7. Between ~100 and ~35 Ma, most zircons lie along trends toward more negative epsilon

Hf values that are steeper than average crustal evolution (Figs. 8-11). This is interpreted to reflect a progressive decrease in the proportion of juvenile magma generated within the arc systems, and/or reworking of progressively older crustal materials. The former may be related to a change in subduction dynamics caused by an increase in the age of the slab being subducted and/or an increase in the convergence rate between South America and outboard ocean basins

(Fig. 12; Maloney et al., 2013). It is also likely that the average age of reworked crustal materials increased with time as the magmatic arc migrated back toward cratonal South America

(e.g., Haschke et al., 2002; Franz et al., 2006). Although most zircons lie along this apparent trend, at least in NA and CA, it is important to note that many <100 Ma zircons (especially in

SA) yield highly positive epsilon Hf values. Such variable proportions of juvenile versus reworked materials are not surprising given the length and complexity of the Andean magmatic arc system.

8. Zircons that are younger than ~35 Ma yield a broad range of epsilon Hf values, ranging from below -10 to above +10 (Fig. 11), which is similar to the broad range of epsilon Nd values in Patagonia (Pankhurst et al., 1999; Herve et al., 2007). This range is interpreted to reflect the broad range of tectonic settings along the Andean magmatic arc, from areas of crustal thickening where magmas are forming due to crustal melting, to areas of extension where mantle-derived melts are present (e.g., Kay et al., 2005; Ramos, 2009; DeCelles et al., 2009, 2014).

32

DISCUSSION

Magmatic Processes

There is a relatively consistent pattern of magmatism and crustal evolution in all of the geochronologic and Hf isotopic data sets available for South America. In terms of ages of felsic to intermediate-composition (e.g., zircon-bearing) magmas, the history is apparently episodic, with long-term patterns that parallel the first order global record (Fig. 13; Voice et al., 2011;

Condie, 2014). Significant mismatches are the abundance of <200 Ma ages and the scarcity of

>1.4 Ga ages in our South American record, which is not surprising given that most of our samples were collected in proximity to the Andean orogen or from rivers with headwaters in the

Andes. This apparent episodicity, with a period of ~0.6 Ga, is widely ascribed to the supercontinent cycle (Hawkesworth et al., 2009, 2010; Belousova et al., 2010; Voice et al., 2011;

Condie et al., 2011; Condie, 2014), with periods of low zircon production and preservation related to break-up of (Fig. 13).

As shown on Figures 6 and 12, there is also a strong episodicity in the ages of magmatism during the past 200 Ma. Approximately similar times of high and low magmatism are apparent in all data sets, with age maxima at approximately 183, 151, 126, 109, 87, 62, 39,

19, and 6 Ma (vertical gray bars on Figures 6 and 12). There are significant variations in these records, however, with peak ages that are younger, older, or missing entirely along some transects. The origin of this apparent ~22 m.y. episodicity, and ultimately the control on magmatic addition, remains uncertain, but has been suggested to be from the subducting slab folding on itself at the 660 km discontinuity (Lee and King, 2011; Gibert et al., 2012). As shown on Figure 12, there does not appear to be a correlation between magmatism and the age of the down-going plate for any region (purple curves, from Maloney et al., 2013). Likewise, there is

33 no obvious correlation between magmatism and the absolute motion of South America (green curves, from Maloney et al., 2013). There is, however, an apparent correlation between magmatism and the relative convergence rates between South America and oceanic plates along the CA and SA (blue curves, from Maloney et al., 2013). An interpretation of this correlation is that periods of high magmatism occur at times of high plate convergence due to higher inputs of water and hydrous melts (Davies and Stevenson, 1991) and rapid ascent of magmas (Elliot et al.,

1997). Correlations are strongest along the CA most likely because it is has a relatively simple subduction history in comparison with the more complex plate boundaries to the north and south.

Equally important is the presence of outboard terranes and eastern cratons with evolved Hf signatures in CA that were most likely involved in melting during periods of compression and crustal thickening. Maloney et al., (2012) states that there might be some inaccuracies with their results for older plate motion estimates and for areas with large changes in subduction dynamics

(i.e. trench jumps, terrane accretions and complicated plate dynamics). Complicated plate dynamics have been noted in the NA and SA.

Haschke et al. (2002, 2006) reported a somewhat different episodicity for the central

Andes, with four phases of magmatism at 195-129 Ma, 123-82 Ma, 76-37 Ma, and 22-0 Ma, yielding an average periodicity of ~50 m.y. (blue fields on Figure 14). Magmatic gaps are reported to exist at 129-123 Ma, 82-76 Ma, and 37-22 Ma. Haschke et al. (2002) suggest that a correlation between magma addition and convergence rate may be due to a ~50 m.y. cycle of decreasing slab dip (periods of high magma addition) followed by slab break-off or roll-back

(periods of low magma addition). Ramos (2009) proposes an Andean orogenic/magmatic cycle that invokes changes in slab dip and delamination of lower crustal roots as a primary control on types and volumes of magmatism. DeCelles et al. (2009, 2014) provide an alternative

34 explanation of cyclicity that involves periods of compressional , heating, hydration, eclogitization, and delamination of the upper plate, with less reliance on processes directly associated with the subducting plate (e.g., slab angle, subduction velocity).

Crustal Generation and Reworking

As with magmatic processes, our data set provides new insight into processes of crustal generation/reworking that operate at two different time scales. On a broader time scale, our data provide an interesting contrast to the Hf isotopic results presented by Belousova et al. (2010) and

Condie et al. (2011), which emphasize data from cratonal regions of , , and South

America. Our data resemble the global patterns prior to ~800 Ma, but are somewhat different for younger time periods. The first significant difference is the abundance of juvenile values from

800-650 Ma in the global data set, which is not seen in South America. Next is the slight negative excursion from 650-500 Ma in our data set, which is much more pronounced in the global record due to Pan-African tectonism. A final difference is the abundance of juvenile values from 400 to 200 Ma in the global record (mainly due to juvenile terranes of Asia), which is not found in South America.

On a more recent time scale, our data record a dramatic change in crustal evolution during the past 200 Ma that is not seen in older orogenic events or in the global record (Figures

11-13). Magmatism in proto-Andean magmatic arcs initiated with relatively evolved Hf signatures that reflect incorporation largely of older continental crust. Beginning at ~180 Ma, epsilon Hf values become significantly more juvenile until ~100 Ma, and then become more negative until ~35 Ma. The pre-100 Ma trend toward more juvenile values may result largely from extension within the magmatic arc, as has been proposed for the Tasmanides (Kemp et al.,

2009; Hawkesworth et al. 2010). This excursion to more juvenile values may also have resulted

35 from the Late Jurassic-Early Cretaceous magmatic arc having been located far to the west, where there was little influence from continental assemblages.

As has been suggested in most previous syntheses (e.g., Haschke et al., 2002; Kay et al.,

2005; Ramos, 2009), the trend toward more evolved values during the past ~100 Ma most likely resulted from the onset of shortening and crustal thickening within the Andes, causing more crustal melting, and also migration of magmatism eastward into older crust. The abundance of epsilon Hf values between +5 and +15 for <35 Ma zircons (Fig. 11) demonstrates that some

Andean magmatism is dominated by juvenile contributions.

Of particular interest for this study are the La/Yb, Sr isotope, and Nd isotope patterns reported by Haschke et al. (2002), which were interpreted to record changes in Andean subduction dynamics on a ~50 m.y. time scale. As shown on Figure 14, the patterns appear to record increasing incorporation of crustal material toward the end of each ~50 m.y., cycle, as well as an overall trend toward more evolved values during the past 200 Ma. The data generated and compiled in this study from the same region (CA) show the general trend toward more evolved values, especially since ~100 Ma. The ~50 m.y. pull-downs apparent from the Nd, Sr, and La/Yb data are not shown, however, by our Hf-in-zircon data, and, as noted above, our age data also do not record the magmatic gaps that were interpreted by Haschke et al. (2002) to separate these magmatic cycles. A possible explanation of these discrepancies is that our record is biased toward felsic to intermediate composition magmatism, whereas the samples reported by

Haschke et al. (2002) also include mafic components.

36

CONCLUSIONS

This study of U-Pb geochronology and Hf isotope geochemistry yields five major contributions to understanding the magmatic history and crustal evolution of South America:

1. Our U-Pb ages (n=5,524), combined with previously published ages (n=36,764), record maxima at 1.6-0.9 Ga, 700-400 Ma, 360-200 Ma, and 190 Ma to the present day (Figure

13). Because this record has been assembled largely from studies of detrital zircons in rivers with headwaters in the modern Andes, the age distributions are biased toward felsic to intermediate composition magmatism, and toward younger events that are preserved in the Andean orogen.

2. Magmatism during the past 200 Ma has been variable north-to-south along the length of the Andes and east-west across the Andes, and studies of igneous rocks yield slightly different patterns than studies of detrital minerals (Fig. 6). Most records are consistent, however, with age maxima at 183 Ma (191-175 Ma), 151 Ma (159-143 Ma), 126 Ma (131-121 Ma), 109 Ma (114-

105 Ma), 87 Ma (95-79 Ma), 62 Ma (71-53 Ma), 39 Ma (43-35 Ma), 19 Ma (23-15 Ma, and 6

Ma (10-2 Ma) (vertical gray bars on Figure 6).

3. The full distribution of ages is an excellent match with the global record of magmatism

(Fig. 13), and correlates well with the supercontinent cycle (Hawkesworth et al., 2009, 2010;

Belousova et al., 2010; Voice et al., 2011; Condie et al., 2011; Cawood et al., 2012; Condie,

2014). The younger magmatic record has a periodicity of ~22 Ma (Fig. 12), and shows an apparent correlation with convergence rate between South America and Pacific oceanic plates

(Maloney et al., 2013).

4. Our Hf isotope determinations (n=1,199), combined with published Hf isotope data

(n=436), record eight phases in the crustal evolution of South America (Fig. 11):

 Prior to ~1.6 Ga, most grains record Paleoproterozoic reworking of mostly Archean crustal

37

materials.

 Between ~1.6 Ga and ~1.0 Ga, an increasing proportion of juvenile magma was mixed with

reworked Paleoproterozoic-Archean crust.

 Between ~1.0 Ga and ~500 Ma, most magmatic processes involved reworking of older

crustal materials, with little generation of new crust.

 Between ~500 and 400 Ma, increasing juvenile magmatism in CA resulted from extension

and crustal thinning throughout the extensive Famatinian-Puno arc (Ducea et al., 2015).

 Following a magmatic lull between ~400 and 360 Ma, there was an increase in the amount of

juvenile magmatism in proto-Andean arc terranes, followed by a trend toward greater

interaction with older crust until ~250 Ma. This increase in crustal reworking is presumably

related to accretion/consolidation of the arc terranes along the Andean margin.

 Following a magmatic lull between ~240 and ~180 Ma, and continuing until ~100 Ma,

magmatism increased and significant volumes of juvenile magma were generated. This phase

coincides with extensional tectonism (Ramos, 2009), a reduction in both convergence

velocity and westward motion of South America (Maloney et al., 2013), and migration of the

magmatic arc westward into more juvenile arc-type crust (Franz et al., 2006).

 Between ~100 Ma and ~35 Ma, abundant magmatism continued, but with decreasing

juvenile magma and increasing involvement of older continental crust. This phase

presumably relates to contractional tectonism and early formation of the modern Andes (Kay

et al., 2005; Franz et al., 2006; Ramos, 2009; DeCelles et al., 2014), an increase in both

convergence velocity and westward motion of South America (Maloney et al., 2013), and

migration of the magmatic arc eastward into more evolved crust (Hachke et al., 2002; Franz

et al., 2006).

38

 During the past ~35 Ma, high-flux magmatism continued with highly variable Hf isotope

signatures. No evolutionary trends are apparent, although there is a spatial variation with

more juvenile values in the northern and southern Andes and more evolved values in the

central Andes (Figures 11 and 12). These variations presumably reflect differing tectonic

settings (contractional versus extensional) along and across the orogen in response to changes

in both the subducting and over-riding plates.

5. The South American record of crustal evolution is somewhat different from the global record

(e.g., Belousova et al., 2010; Condie, 2014) in that South America lacks significant volumes of

800-650 Ma and 400-200 Ma juvenile crust and highly evolved 650-500 Ma crust. The main pattern of increasing juvenile crust before 100 Ma and decreasing juvenile crust after 100 Ma

(Fig. 11) is presumably a result of Jura-Cretaceous extension within the arc system (presumably due to lower convergence rates), as well as migration of the magmatic arc first outboard into more juvenile arc terranes and then inboard into crust with greater proportions of older continental crust.

39

ACKNOWLEDGEMENTS

We are grateful for support from the Geological Society of America (student grant 9157-06) and

Chevron-Texaco summer support grant. Analyses were conducted in the Arizona LaserChron

Center, which has been supported by NSF EAR-1338583. We also thank LaserChron staff

members Chen Li, Gayland Simpson, Chelsi White, Dominique Geisler, Mark Pecha, Clayton

Loehn, and Glynis Jehle for assistance with sample preparation and analysis. Ned Brown

provided valuable discussions of the work presented in this publication. We would also like to

thank the ExxonMobil COSA project that provided lots of discussions, and covered costs of a

Central Andean field trip. We are also very grateful for Agustin Cardona, Franco Urbani, David

Mendi, Camilo Bustamante, Giovani Jimenez and Herman Bayona who helped in field support

and the field collections for this project.

40

APPENDIX A FIGURE 1. GEOLOGIC MAP WITH OUTLINED CATCHMENTS

41

42

Appendix A Figure 1. Geologic map with legend of ages and rock types in lower right corner. Red polygons outline individual catchment areas for each sample that is described in Appendix A Table 1. White dots are sample locations with tie-line to sample names used in text. Samples are described further in Appendix A Table 1 with all the new data that has been generated for this project in attached Tables 2-7.

43

APPENDIX B

U-Pb REFERENCES USED IN ATTACHED DATA COMPILATION

Northern Andes detrital zircon ages

Ayala, R.C., Bayona, G., Cardona, A., Ojeda, C., Montenegro, O.C., Montes, C., Valencia, V.,

and Jaramillo, C., 2012, The synorogenic succession in the northwestern

Maracaibo block: Tracking intraplate uplifts and changes in sediment delivery systems:

Journal of South American Earth Sciences, v. 39, p. 93-111.

Bande, A., Horton, B.K., Ramírez, J.C., Mora, A., Parra, M., and Stockli, D.F., 2012, Clastic

deposition, provenance, and sequence of Andean thrusting in the frontal Eastern

Cordillera Llanos of Colombia: Geological Society of America Bulletin,

v. 124, p. 59-76.

Bayona, G., Cardona, A., Jaramillo, C., Mora, A., Montes, C., Valencia, V., Ayala, C.,

Montenegro, O., and Ibañez-Mejia, M., 2012, Early Paleogene magmatism in the

northern Andes: insights on the effects of oceanic –continent convergence: Earth

Planetary Science Letters, v. 331, p. 97-111.

Cardona, A., Chew, D., Valencia, V.A., Bayona, G., Miskovik, A., and Ibanez-Mejia, M.,

2010b, Grenvillian remnants in the Northern Andes: Rodinian Phanerozoic

paleogeographic perspectives: Journal of South American Earth Sciences, v. 29, p. 92-

104.

Cardona, A., Valencia, V.A., Bayona, G., Duque, J., Ducea, M., Gehrels, G., Jaramillo, C.,

Montes, C., Ojeda, G., and Ruiz, J., 2011, Early subduction related orogeny in the

northern Andes: Turonian to magmatic and provenance record in the Santa Marta

Massif Rancheria Basin, northern Colombia: Terra Nova, v. 23, p. 26-34.

44

Chew, D.M., Schaltegger, U., Kosaler, J., Whitehouse, M.J., Gutjahr, M., Spikings, R.A., and

Miskakovic, A., 2007, U-Pb geochronologic evidence for the evolution of the

Gondwanan margin of the north-central Andes: Geological Society of America Bulletin,

v. 119, p. 697-711.

Chew, D.M., Magna, T., Kirkl, C.L., Misakovic, A., Cardona, A., Spikings, R., and

Schaltegger, U., 2008, Detrital zircon fingerprint of the Proto-Andes: Evidence for a

Neoproterozoic active margin?: Precambrian Research, v. 167, p. 186-200.

Ibanez-Mejia, M., Valencia, V.A., Cardona, A., Gehrels, G.E., and Mora, A.R., 2011, The

Putumayo Orogen of Amazonia and its implications for Rodinia reconstructions: new U–

Pb geochronological insights into the Proterozoic tectonic evolution of northwestern

South America: Precambrian Research, v. 191, p. 58-77.

Martin-Gombojav, N., and Winkler, W., 2008, Recycling of Proterozoic crust in the Andean

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detrital zircons in the southern central Andes Neogene foreland (36°–37° S): Constraints

on Andean exhumation: Journal of South American Earth Sciences, v. 32, p. 555-566.

Tunik, M., Folguera, A., Naipauer, M., Pimentel, M., and Ramos, V.A., 2010, Early uplift and

orogenic deformation in the Neuquén Basin: constraints on the Andean uplift from U–Pb

and Hf isotopic data of detrital zircons: Tectonophysics, v. 489, p. 258-273.

Uriz, N.J., Cingolani, C.A., Chemale Jr., F., Macambira, M.B., and Armstrong, R., 2011,

Isotopic studies on detrital zircons of Silurian–Devonian siliciclastic sequences from

86

Argentinean North Patagonia and Sierra de la Ventana regions: comparative provenance:

International Journal of Earth Sciences, v. 100, p. 571-589.

Varela, A.N., Poiré, D.G., Martin, T., Gerdes, A., Goin, F.J., Gelfo, J.N., and Hoffmann, S.,

2012, U-Pb zircon constraints on the age of the Cretaceous Mata Amarilla Formation,

Southern Patagonia, Argentina: its relationship with the evolution of the Austral Basin:

Andean Geology, v. 39, p. 359-379.

Willner, A.P., Gerdes, A., and Massonne, H.J., 2008, History of crustal growth and recycling at

the Pacific convergent margin of South America at latitudes 29–36 S revealed by a U–Pb

and Lu–Hf isotope study of detrital zircon from late Paleozoic accretionary systems:

Chemical Geology, v. 253, p. 114-129.

87

APPENDIX C

Hf REFERENCES USED IN ATTACHED DATA COMPILATION

Augustsson, C., Muenker, C., Bahlburg, H., and Fanning, C.M., 2006, Provenance of late

Palaeozoic metasediments of the SW South American Gondwana margin: a combined U–

Pb and Hf-isotope study of single detrital zircons: Journal of the Geological Society, v.

163, p. 983-995.

Bahlburg, H., Vervoort, J.D., Du Frane, S.A., Bock, B., Augustsson, C., and Reimann, C., 2009,

Timing of crust formation and recycling in accretionary orogens: Insights learned from

the western margin of South America: Earth-Science Reviews, v. 97, p. 215-241.

Bahlburg, H., Vervoort, J.D., Andrew DuFrane, S., Carlotto, V., Reimann, C., and Cárdenas, J.,

2011, The U–Pb and Hf isotope evidence of detrital zircons of the Ordovician

Ollantaytambo Formation, southern Peru, and the Ordovician provenance and

paleogeography of southern Peru and northern Bolivia: Journal of South American Earth

Sciences, v. 32, p. 196-209.

Chernicoff, C.J., Zappettini, E.O., Santos, J.O., Beyer, E., and McNaughton, N.J., 2008, Foreland

basin deposits associated with Cuyania accretion in La Pampa Province,

Argentina: Gondwana Research, v. 13, p. 189-203.

Chernicoff, C.J., Zappettini, E.O., Santos, J.O., McNaughton, N.J., and Belousova, E., 2013,

Combined U-Pb SHRIMP and Hf isotope study of the Late Paleozoic Yaminué Complex,

Rio Negro Province, Argentina: Implications for the origin and evolution of the

Patagonia composite terrane: Geoscience Frontiers, v. 4, p. 37-56.

Chew, D.M., Schaltegger, U., Košler, J., Whitehouse, M.J., Gutjahr, M., Spikings, R.A., and

Miškovíc, A., 2007, U-Pb geochronologic evidence for the evolution of the Gondwanan

88

margin of the north-central Andes: Geological Society of America Bulletin, v. 119, p.

697-711.

Dahlquist, J.A., Pankhurst, R.J., Gaschnig, R.M., Rapela, C.W., Casquet, C., Alasino, P.H.,

Galindo, C., and Baldo, E.G., 2013, Hf and Nd isotopes in Early Ordovician to Early

Carboniferous granites as monitors of crustal growth in the Proto-Andean margin of

Gondwana: Gondwana Research, v. 23, p. 1617-1630.

Montecinos, P., Schärer, U., Vergara, M., and Aguirre, L., 2008, Lithospheric origin of

Oligocene–Miocene magmatism in Central Chile: U–Pb ages and Sr–Pb–Hf isotope

composition of minerals: Journal of Petrology, v. 49, p. 555-580.

Polliand, M., Schaltegger, U., Frank, M., and Fontboté, L., 2005, Formation of intra-arc

volcanosedimentary basins in the western flank of the central Peruvian Andes during Late

Cretaceous oblique subduction: field evidence and constraints from U–Pb ages and Hf

isotopes: International Journal of Earth Sciences, v. 94, p. 231-242.

Willner, A.P., Gerdes, A., and Massonne, H.J., 2008, History of crustal growth and recycling at

the Pacific convergent margin of South America at latitudes 29–36 S revealed by a U–Pb

and Lu–Hf isotope study of detrital zircon from late Paleozoic accretionary

systems: Chemical Geology, v. 253, p. 114-129.

89

Figure 1. Map showing first-order geologic features of South America (adapted from Goodwin,

1996; Ramos, 2008, 2009, 2010; Bahlburg et al., 2009). Samples are keyed to three regions as follows: Northern Andes (NA; 12oN-4oS), Central Andes (CA; 4oS-34oS) and Southern Andes

(SA; 34oS-54oS).

90

Figure 2. Diagram showing U-Pb and Hf isotopic results from NA samples. 1339 U-Pb ages and

308 Hf isotope analyses are reported. Reference lines for Hf isotope data are as follows: DM =

176 177 176 177 Depleted Mantle array, calculated using Hf/ Hf0 = 0.283225 and Lu/ Hf0 = 0.03830

(Vervoort and Blichert-Toft, 1999); CHUR = Chondritic Uniform Reservoir, calculated using

176Hf/177Hf = 0.282785 and 176Lu/177Hf = 0.0336 (Bouvier et al., 2008). Arrows showing

Average Crustal Evolution represent trajectories with present-day 176Lu/177Hf = 0.0115 (Vervoort and Patchett, 1996; Vervoort et al., 1999). The average measurement uncertainty for all NA analyses is 2.8 epsilon units (2σ). Age-distribution curves for 0-200 Ma and 200-2800 Ma have been normalized such that area under each curve is the same.

91

Figure 3. Diagram showing U-Pb and Hf isotopic results from CA samples. 2172 U-Pb ages and

447 Hf isotope analyses are reported. See Figure 2 for explanation. The average measurement uncertainty for all analyses is 2.6 epsilon units (2σ).

92

Figure 4. Diagram showing U-Pb and Hf isotopic results from SA samples. 2013 U-Pb ages and

444 Hf isotope analyses are reported See Figure 2 for explanation. The average measurement uncertainty for all analyses is 3.0 epsilon units (2σ).

93

Figure 5. Comparison of U-Pb age distributions from this study, from published analyses of detrital and igneous minerals (Appendix B Table 1 and Appendix B sources cited below). Ages of basement provinces are from Figure 1. The numbers of ages reported are as follows for this study, published detrital ages, and published igneous ages: NA = 1,339/8,871/1,492, CA =

2,172/12,264/5,723, SA = 2,013/5,716/2,714, All = 5,524/26,851/9,929.

94

Figure 6. Comparison of 0-200 Ma ages from various data sets. Vertical bands show interpreted maxima of ages. Note that curves are smoothed with a sliding window average (with a band width of 6 m.y.), and are normalized by height (not area).

95

Figure 7. Map showing location of samples included in compilation of published data. Each polygon is the area sampled for each publication.

96

Figure 8. Summary of all available U-Pb and Hf isotope data from NA. See Figure 2 for explanation. All Hf data are from this study (n=308). U-Pb data are from this study (n=1,340) and from previous studies (Appendix B Tables 1-2; detrital n=8,871, igneous n=1,492). Note that proportions of >250 Ma ages are enhanced by a factor of 5 relative to <250 Ma ages.

97

Figure 9. Summary of all available U-Pb and Hf isotope data from CA. See Figure 2 for explanation. Hf data are from this study (n=447) and from previous studies (Appendix C Table 1; n=351). U-Pb data are from this study (n=2172) and from the previous studies (Appendix B

Tables 1-2; detrital n=12,264, igneous n=5,723). Note that proportions of >250 Ma ages are enhanced by a factor of 5 relative to <250 Ma ages.

98

Figure 10. Summary of all available U-Pb and Hf isotope data from SA. See Figure 2 for explanation. Hf data are from this study (n=444) and from previous studies (Appendix C Table 1; n=85). U-Pb data are from this study (n=2,013) and from the previous studies (Appendix B

Tables 1-2; detrital n=5,716, igneous n=2,714).

99

Figure 11. Summary of all available U-Pb and Hf isotope data from South America. See Figure

2 for explanation. Hf data are from this study (n=1199) and from previous studies (Appendix C

Table 1; n=436). U-Pb data are from this study (n=5,524) and from the previous studies

(Appendix B Tables 1-2; detrital n=26,851, igneous n=9,929).

100

101

Figure 12. Diagram comparing the results of Maloney et al. (2013) with our data for all three regions (e.g. NA, CA and SA) for the past 200 Ma. Red diamonds in upper portion of plots show

Hf isotope data from this study. Filled orange curves in lower portion of plots show all available

U-Pb ages (smoothed with a 6 m.y. sliding window average). Vertical gray bands show interpreted age maxima (from Fig. 6). Central portion of upper plot shows information about plate convergence along the NA margin (average of sites 2-9 of Maloney et al., 2013), with gray line equal to zero age and velocity: purple line = age of the downgoing plate (maximum age of

78 m.y.); blue line = convergence velocity between South America and outboard oceanic plates

(maximum velocity of ~6.1 cm/yr); green line = absolute motion of South America (maximum westward velocity of ~3.1 cm/yr). Central portion of center plot shows information about convergence along the CA margin (average of sites 12-36 of Maloney et al., 2013), velocity: purple line maximum age of 66 m.y.; blue line maximum velocity of ~6.0 cm/yr; green line maximum westward velocity of ~2.4 cm/yr. Central portion of lower plot shows information about convergence along the SA margin (average of sites 39-54 of Maloney et al., 2013), purple line maximum age of 62 m.y.; blue line maximum velocity of ~7.2 cm/yr; green line maximum westward velocity of ~2.8 cm/yr.

102

Figure 13. Comparison of U-Pb and Hf isotope data from South America with global compilation of U-Pb ages and Hf isotope data. See Figure 2 for explanation. Hf data are from this study (n=1,199) and from the global compilation of Belousova et al. (2010) (n=12,375). The sliding window average of global Hf data is from Belousova et al. (2010). U-Pb data are from this study (n=5,524), all available data from South America (n=42,304), and the global compilation of Belousova et al. (2010) (n=23,178). Color bands are from Condie (2014), with green = supercontinent assembly and red = supercontinent breakup.

103

Figure 14. Diagram comparing the results of Haschke et al. (2002) with our CA data for the past

200 Ma. Blue fields in upper plot show age and Nd isotope fields of Hashke et al. (2002). Red diamonds in upper plot show CA age and Hf isotope data from this study. Age distribution diagrams show, in deepening shades of red, our results from CA (n=1,339), our results from all of South America (n=5,524), and all ages available from South America (n=42,304). Vertical gray bands show interpreted age maxima (from Fig. 6).

104

Table 1. Sample information Northern Andes (NA) CA - continued Sample # analyses # analyses name ID Sand type U-Pb/Hf ID Sample ID Sand type U-Pb/Hf NA01 RRANCO01 Delta 100/28 CA17 RLLUCH01 River 96/20 NA02 RMAGCO06 River 102/23 CA18 RCAMCH01 River 106/25 NA03 RMAGCO07 Delta 101/20 CA19 RLOACL01 River 79/17 NA04 RMAGCO08 Delta 97/20 CA20 RLOACL02 Beach 85/18 NA05 RSINCO01 River 106/23 CA21 RCONCH01 River 104/18 NA06 RCHICO01 River 101/20 CA22 RCHOCH01 River 106/9 NA07 RNEICO01 River 106/24 CA23 BVILCH01 River 112/19 NA08 RMAGCO01 River 92/20 Southern Andes (SA) NA09 RPAICO01 River 93/27 SA01 RMATCH01 River 93/20 NA10 RCHOTEC01 River 99/20 SA02 RMAUCH01 River 94/25 NA11 RBLAEC01 River 80/15 SA03 RBIOCH01 Delta 87/27 NA12 RTENEC01 River 69/21 SA04 RBIOCH02 River 99/17 NA13 RJUBEC01 River 103/25 SA05 RBUECH01 River 94/18 NA14 RSULPE01 River 88/23 SA06 RCOLAR01 River 86/20 Central Andes (CA) SA07 RCOLAR02 River 94/27 CA01 RPILAR02 River 74/17 SA08 RSAUAR01 River 93/21 CA02 RBERAR02 River 95/20 SA09 RNEUQAR01 River 101/20 CA03 RPILAR01 River 76/20 SA10 RLIMAR01 River 93/18 CA04 RBERAR01 River 81/13 SA11 RNEGAR01 River 100/19 CA05 RHUALPE01 River 96/20 SA12 RNEGAR02 River 104/21 CA06 RPUCPE01 River 97/20 SA13 ASALAR01 River 100/25 CA07 RHUANPE01 River 91/22 SA14 RCHUAR01 River 99/16 CA08 RLUNPE01 River 100/20 SA15 RCHUAR02 River 107/25 CA09 RMDDPE01 River 92/20 SA16 RCHIAR01 River 104/23 CA10 RAQUIPE01 River 100/23 SA17 RDESAR01 Arroyo 99/26 CA11 RTRUPE01 River 100/21 SA18 RDESAR02 Arroyo 95/17 CA12 RHUAPE01 River 107/21 SA19 RCHIAR02 River 93/22 CA13 RCLAPE01 Beach 101/21 SA20 RSCRAR01 River 59/16 CA14 RICAPE01 River 78/20 SA21 RGALAR01 River 97/20 CA15 ROCOPE01 River 97/22 SA22 RCHIAR03 River 22/1 CA16 BILOPE01 River 99/22

105

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