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Petrogenesis of the Dunite Peak ophiolite, south-central Yukon and the
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distinction of upper plate and lower plate settings: a new hypothesis for
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the late Paleozoic – early Mesozoic tectonic evolution of the Northern
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Cordillera
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A.J. Parsons1*, A. Zagorevski2, J.J. Ryan1, W.C. McClelland3, C.R. van Staal1, M.J. Coleman4, M.L.
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Golding1.
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* andrew.parsons@earth.ox.ac.uk
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1
Dept. Earth Sciences, University of Oxford, South Parks Road, Oxford, OX1 3AN, United Kingdom.
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2
Geological Survey of Canada, 1500-605 Robson Street, Vancouver, BC, V6B5J, Canada.
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Geological Survey of Canada, 601 Booth St., Ottawa, ON, K1A 0E8, Canada.
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4
Dept. Earth and Environmental Sciences, 115 Trowbridge Hall, University of Iowa, Iowa City, IA, 52242,
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USA.
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Canada.
Dept. Earth and Environmental Sciences, University of Ottawa, 120 University, Ottawa, ON. K1N 6N5,
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ABSTRACT
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Upper plate and lower plate settings within subduction zones have distinct geological signatures. Identifying
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and discriminating between these settings is crucial to the study of accretionary orogens. We apply this
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distinction to the Northern Cordillera in Yukon, British Columbia and Alaska, and focus on the
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identification of upper plate and lower plate domains during the late Paleozoic to early Mesozoic evolution
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of the allochthonous Yukon-Tanana terrane, the west Laurentian margin and the intervening Slide Mountain
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Ocean. We present new data from the Dunite Peak ophiolite in south-central Yukon, previously interpreted
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as ocean plate stratigraphy that was obducted from the subducting Slide Mountain Ocean (i.e. lower plate).
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Whole-rock geochemical and Sm-Nd isotopic analyses, and U-Pb zircon geochronology indicate that the
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Dunite Peak ophiolite formed in an intra-oceanic suprasubduction zone setting (i.e. upper plate) with
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magmatism at 265 ± 4 Ma. We propose that the Dunite Peak ophiolite correlates with other mid-Permian
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suprasubduction zone ophiolites of the Slide Mountain terrane, collectively defining the previously
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unrecognized mid-Permian Dunite Peak intra-oceanic arc. This intra-oceanic arc was active from ~280 to
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260 Ma, located within the Slide Mountain Ocean, between the Yukon-Tanana terrane and west Laurentia.
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Existence of this arc is incompatible with previous models which proposed that accretion of the Yukon-
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Tanana terrane to Laurentia was facilitated by Permian subduction of Slide Mountain Ocean beneath the
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Yukon-Tanana terrane. Our results, combined with existing datasets suggest that during the mid- to late
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Permian, Yukon-Tanana terrane subducted eastward beneath the Dunite Peak intra-oceanic arc. Subsequent
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collision and accretion of the Yukon-Tanana – Dunite Peak composite terrane with Laurentia must have
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occurred after the Middle Triassic.
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1. INTRODUCTION
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The understanding of subduction, accretion and collision processes in active and ancient settings has been
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vastly improved by modern geochemical and geochronological constraints. Specifically, subduction zone
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upper-plate settings and subduction zone lower-plate settings in accretionary orogens may be discriminated
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using key geochemical indicators, especially with respect to the origin and timing of formation of ophiolites
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(e.g. Wilson, 1989; Wakabayashi & Dilek, 2000; Pearce, 2008, 2014; Dilek & Furnes, 2014; McGoldrick et
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al., 2017). In this study, we investigate the petrogenesis of Permian ophiolites associated with the Slide
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Mountain terrane (SMT) of the Northern Cordillera accretionary orogen in Alaska, Yukon and British
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Columbia (Figure 1), with particular focus on distinction between subduction zone upper-plate and
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subduction zone lower-plate processes. This includes new field, geochemical and geochronological analyses
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of the Dunite Peak ophiolite (de Keijzer et al., 2000; Parsons et al. 2017a, b) in south-central Yukon, which
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has been assigned previously to the SMT (e.g. Colpron et al., 2016). Previous studies consider the SMT to
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be the accreted remnants of the Slide Mountain Ocean, which they interpreted as a back-arc oceanic basin
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between the western Laurentian margin and the allochthonous Yukon-Tanana terrane (YTT, a continental
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island arc), during the Late Devonian to Permian (see review of Nelson et al., 2013).
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In this study, we first present the concept of upper-plate and lower-plate distinctions in subduction zone
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settings and their relevance for studies of accretionary orogens. This is followed by an introduction to
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current tectonic models for the Northern Cordillera and the locally defined mid- to late Permian ‘Klondike
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orogeny’ (260-252.2 Ma) as proposed by previous works (e.g. Mortensen, 1992a; Beranek & Mortensen,
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2011; Nelson et al., 2006; 2013; Colpron et al., 2006a; 2007). We present new data from the Dunite Peak
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ophiolite (Figure 1e), integrate it with existing data from the SMT, and argue that most mid-Permian
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ophiolites assigned to the SMT are supra-subduction zone (SSZ) ophiolites, derived from the upper plate of
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a previously unrecognized intra-oceanic arc. We define this arc as the Dunite Peak intra-oceanic arc.
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Our findings are incompatible with current tectonic models for Northern Cordillera and require an
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alternative explanation. We integrate our findings with existing datasets to present a new hypothesis for the
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late Paleozoic to early Mesozoic evolution of the Northern Cordillera. This study not only bears significance
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for our understanding of the Northern Cordillera, but also demonstrates the importance of identifying and
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distinguishing between upper-plate and lower-plate components in any accretionary orogen, and how
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misidentification of such components can result in markedly different tectonic interpretations.
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1.1. Upper plate – lower plate distinction in accretionary orogens
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Distinguishing subduction zone upper-plate processes/components from subduction zone lower-plate
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processes/components is a complicated and yet essential part of any study of accretionary orogens (e.g.
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Wakabayashi & Dilek, 2000; Zagorevski & van Staal, 2011; McGoldrick et al., 2017). Here, we define
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accretion as the sequential addition of material from a subducting lower plate to an overriding upper plate or
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vice versa, via underplating obduction or transform faulting. We define the term collision as entry of a lower
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plate oceanic plateau, arc or continental lithosphere into a subduction zone. During the life of an active
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subduction zone, it is possible to classify the structural components that interact with it into one of three
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groups: (1) Upper-plate material of the active subduction zone. These include the arc, fore-arc and back-arc,
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plus the arc substrate comprising continental lithosphere, oceanic lithosphere or fragments of the two. Where
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oceanic lithosphere is present in the upper plate, SSZ ophiolites may also form in this setting (e.g. Dilek &
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Furnes, 2014). (2) Subducted lower-plate material. This group accounts for almost all lower-plate oceanic
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lithosphere that enters a subduction zone and is rarely preserved in the geological record as most of this
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material subducts into the mantle (e.g. Dewey, 2003; Wakabayashi, 2017). At the point of cessation of
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subduction, this lower-plate material may be preserved, juxtaposed to the upper plate via a suture. In such
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cases, cessation of subduction typically corresponds to a collision, facilitated by the arrival of a lower-plate
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arc, continent, or ocean plateau into the subduction zone (e.g. Cloos, 1993; Mann & Taira, 2004; Afonso &
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Zlotnik, 2011; Brown et al., 2011). (3) Accreted lower-plate material. Material derived from the lower plate
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that is accreted to the upper plate during subduction-accretion (e.g. the Franciscan complex, California;
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Wakabayashi, 2017). For ancient subduction zones this is usually the only remaining record of the lower
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plate and is commonly used to reconstruct the paleo-ocean plate stratigraphy of the lower plate (e.g. Isozaki
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et al., 1990; Kusky et al., 2013; Wakabayashi, 2017).
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Distinguishing between upper-plate and accreted lower-plate material may be challenging in any subduction
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zone setting, but is particularly difficult when studying polyphase accretionary orogens such as the Central
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Asian orogenic belt (e.g. Lin et al., 2018), the Appalachians (e.g. van Staal et al., 2009; Zagorevski & van
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Staal, 2011) or the Northern Cordillera (e.g. Nelson et al., 2013). Such orogens preserve episodic collisions,
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formation of composite terranes, and subduction polarity reversals, which result in upper- and lower-plate
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material of older subduction zones (including SSZ ophiolites) residing in either the lower or upper plates of
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a younger subduction zone (e.g. Lush’s Bight ophiolite, Newfoundland, Zagorevski & van Staal, 2011). In
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such settings, the study of ophiolites and accretionary complexes can provide an invaluable record of
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subduction-accretion and paleo-subduction polarity during multiple collisional and suturing events (e.g.
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Dilek & Furnes, 2014; Zagorevski & van Staal, 2011; Wakabayashi, 2017). However, misidentification of
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upper-plate, accreted lower-plate and subducted lower-plate material in an accretionary orogen can lead to
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unlikely or implausible tectonic models, as is discussed below (section 2).
2. THE NORTHERN CORDILLERA AND THE KLONDIKE OROGENY (PREVIOUS
WORK)
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The North American Cordillera accretionary orogen (Figure 1) has served as a type example for accretionary
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orogenesis since the establishment of the terrane concept (Coney et al., 1980). It has a complex tectonic
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evolution that involved multiple extensional, collisional and magmatic events since the Proterozoic,
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followed by as much as 1000-2000 km lateral displacement of accreted allochthonous and parautochthonous
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units during the Cenozoic (see review of Nelson et al., 2013). This study focuses on the Paleozoic-Mesozoic
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accretionary history of YTT, SMT and the Laurentian margin, which occurred prior to Mesozoic to Eocene
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dextral translation of terranes along the Cordilleran margin (e.g. Gabrielse et al., 2006).
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It is generally accepted that YTT is an allochthonous continental island arc terrane (Figure 1) built on a
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substrate of peri-cratonic (Laurentian) continental crust (e.g. Colpron et al., 2006a; Piercey & Colpron,
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2009; Nelson et al., 2013). The SMT (Figure 1) comprises Mississippian to early Permian supracrustal
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igneous and sedimentary oceanic rocks and mid-Permian mafic-ultramafic ophiolites that are interpreted as
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vestiges of accreted ocean floor stratigraphy of the Slide Mountain Ocean (see summaries by Nelson et al.,
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2006, 2013). Most models propose that YTT rifted from the west margin of the Laurentia during the Late
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Devonian – Early Mississippian via back-arc rifting of the Yukon-Tanana arc to form the Slide Mountain
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Ocean (e.g. Mortensen, 1992a; Nelson et al., 2006; 2013; Colpron et al., 2006a, 2007). These models then
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propose a subduction polarity reversal across YTT from east-dipping subduction of the Panthalassa Ocean to
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west-dipping subduction of the Slide Mountain Ocean, which led to re-accretion of YTT to Laurentia and
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suturing of Slide Mountain Ocean in the late Permian (e.g. Beranek & Mortensen, 2011).
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Beranek and Mortensen (2011) referred to late Permian (260-252.5 Ma) collision between YTT and
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Laurentia as the ‘Klondike orogeny,’ although similar versions of this model had been proposed prior to
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their work by others (e.g. Mortensen, 1992a; Dusel-Bacon et al., 1995; 2002; Nelson et al., 2006; Berman et
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al., 2007; Colpron et al., 2007; Johnston et al., 2007). Most studies concerning the Paleozoic to early
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Mesozoic evolution of YTT, SMT and Laurentia conducted since Beranek and Mortensen (2011) have been
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interpreted within, and supportive of this framework for the Klondike orogeny (e.g. Nelson et al., 2013;
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Petrie et al., 2015; 2016; Colpron et al., 2015; 2016; Golding et al., 2016a; Staples et al., 2016; Gilotti et al.,
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2017). Such hypotheses typically cite the following as supporting evidence:
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(1) Similarities in lithostratigraphy and detrital zircon populations of pre-Late Devonian metasedimentary
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basement of YTT and metasedimentary rocks of Laurentia are interpreted as indication that YTT initially
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formed part of the Laurentian margin prior to rifting (e.g. Colpron et al., 2006a; Piercey & Colrpon, 2009).
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(2) Occurrences of Mississippian to Permian arc plutonic and volcanic rocks within YTT that are not
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recorded within Laurentia are interpreted as indications that YTT rifted from Laurentia during the Late
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Devonian and then evolved independently, remaining allochthonous to Laurentia at least until the end of the
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Permian (e.g. Mortensen, 1992a; Nelson et al., 2006; 2013). The presence of Mississippian and Permian to
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Triassic metamorphism in YTT but its absence from Laurentia are also used as evidence for separation until
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the Triassic (e.g. Berman et al., 2007; Staples et al., 2016).
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(3) Outcrops of SMT located along the present-day YTT-Laurentia boundary are interpreted as Slide
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Mountain ocean floor stratigraphy accreted to YTT and/or Laurentia, marking a suture that formed
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following Permian subduction and closure of the Slide Mountain Ocean (e.g. Mortensen, 1992a; Murphy et
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al., 2006).
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(4) Mid-Permian blueschist and eclogite assumed to be metamorphosed slivers of Slide Mountain oceanic
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crust (e.g. Creaser et al., 1997; 1999; Erdmer et al., 1998), and mid- to late Permian Sulphur Creek plutonic
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suite and volcanic Klondike schist (collectively referred to as the Klondike assemblage), within YTT (e.g.
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Mortensen, 1990; Colpron et al., 2006a) have been interpreted as a ‘paired metamorphic belt’ that recorded
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subduction of Slide Mountain Ocean beneath YTT (e.g. Mortensen, 1992a; Nelson et al., 2006; Beranek &
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Mortensen, 2011). Beranek and Mortensen (2011) split the Klondike cycle into an early subduction-related
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phase of arc magmatism, deformation and metamorphism between 260 and 254 Ma and a later phase of
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crustal-melt derived post-tectonic magmatism between 254 and 252 Ma. These studies bracket the closure of
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Slide Mountain Ocean and the Klondike orogeny between 260 and 252.5 Ma (Beranek & Mortensen, 2011;
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Nelson et al., 2013).
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(5) The Triassic Jones Lake Formation (Beranek et al., 2010) that overlies parts of Laurentia, SMT and YTT
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in Yukon and British Columbia has been interpreted as a syn-orogenic sedimentary cover succession
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initiated in the Early Triassic (e.g. Colpron et al., 2005; 2006; 2007; Beranek et al., 2010; Beranek &
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Mortensen, 2011; Golding et al., 2016a). Mississippian to Permian detrital zircon populations from these
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strata have been interpreted as indications of a YTT-derived sediment source, which formed an overlap
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succession marking the final stages of collision, accretion and related subsidence between YTT and
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Laurentia (Colpron et al., 2006; 2007; Beranek & Mortensen, 2011).
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2.1. Unresolved issues, conflicting datasets and alternative models
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Other datasets and models for the tectonic evolution of YTT, SMT and Laurentia disagree, or are hard to
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reconcile with models of the Klondike orogeny. These are summarized below and are considered in light of
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our own findings, following presentation of our geochemical and geochronological analyses from the Dunite
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Peak ophiolite. These include:
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(1) Mid-Permian eclogites previously interpreted as metamorphosed slices of SMT oceanic crust have since
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been identified as mafic intrusions within YTT (Petrie et al., 2016). Furthermore, it has been demonstrated
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that the YTT metasedimentary rocks which host these intrusions also record mid-Permian eclogite facies
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metamorphism (Gilotti et al., 2017). As such, deformation, metamorphism and magmatism previously
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attributed to the Klondike orogeny (e.g. Mortensen, 1990; 1992a; Berman et al., 2007; Beranek &
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Mortensen 2011; Staples et al. 2016; Petrie et al., 2016; Gilotti et al., 2017) are exclusively recorded in
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YTT, which forms the upper plate in these models. There is no evidence of contemporaneous lower-plate
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(i.e. Laurentia) deformation or metamorphism to support these models (Berman et al., 2007; Staples et al.,
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2016).
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(2) Existing models do not account for the presence of mid-Permian igneous rocks in SMT with
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geochemical signatures that require formation in an SSZ setting (e.g. Nelson et al., 1993; Plint & Gordon,
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1997; Dusel-Bacon & Cooper, 1999; Fallas et al., 1999; Colpron et al., 2005; 2006b; Dusel-Bacon et al.,
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2006). These data are incompatible with models which propose that Slide Mountain Ocean subducted
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beneath YTT during the mid-Permian (e.g. Mortensen, 1992a; Murphy et al., 2006; Nelson et al., 2006;
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2013; Johnston et al., 2007; Beranek & Mortensen 2011).
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(3) Detrital zircons and conodont fauna do not validate, and in some cases are inconsistent with a model of
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deposition of Triassic syn-orogenic clastic sediments in a regional-scale basin overlapping YTT, SMT and
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Laurentia following Permian collision (e.g. Colrpon et al., 2007; Beranek et al., 2010; Beranek &
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Mortensen, 2011). With the exception of three Mississippian zircons, detrital zircon populations of Early
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Triassic strata on the west Laurentian margin in Yukon (cf. Beranek et al., 2010) may be entirely explained
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by a Laurentian source (Archean, Proterozoic and pre-340 Ma Paleozoic zircons). Middle to Late Triassic
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strata deposited on Laurentia in Yukon and northern British Columbia contain pre-340 Ma zircons that may
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be explained by a Laurentian source or by a YTT source, plus Mississippian to Triassic zircons that require
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either a YTT source (i.e. a Laurentian zircon population plus abundant Mississippian to Permian zircons), or
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Stikinia/Quesnellia source (i.e. Mississippian, minor Permian and abundant Triassic zircons). In contrast,
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most Middle Triassic strata overlying SMT in Yukon and northern British Columbia (e.g. Nelson &
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Bradford, 1993; Murphy et al., 2002; Colpron et al., 2005) have unimodal/bimodal Permian-Triassic ±
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Devonian – Early Mississippian detrital zircon populations (Beranek & Mortensen, 2011). This is suggestive
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of sediment derived from a late Paleozoic – early Mesozoic arc such as Stikinia/Quesnellia, and is not
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consistent with sediment derived from YTT ± Laurentia, which would also contain Pennsylvanian,
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Devonian to Cambrian, Proterozoic and Archean zircons. In the Finlayson Lake district (Figure 1c), the Late
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Triassic Bug Island Limestone, which overlies SMT, yielded a detrital zircon population of Laurentian
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zircons plus five Mississippian zircons that may suggest a YTT source (Beranek, 2009). Conodont fauna
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from this limestone includes the “exotic” Tethyan species Norigondolella hallstattensis (Orchard, 2006) that
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has been reported from other allochthonous terranes (e.g. Wrangell terrane; Orchard, 1991), but is not
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recorded from anywhere along the autochthonous Laurentian margin (Orchard, 2006; Beranek, 2009).
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Additionally, the Bug Island Limestone overlies Middle Triassic clastic sedimentary rocks with
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unimodal/bimodal zircon populations that are not suggestive of a Laurentian or YTT source (Beranek, 2009;
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Beranek & Mortensen, 2011). It is therefore unlikely that these Middle to Late Triassic strata that overlie
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parts of SMT were deposited in the same basin system as coeval strata deposited on Laurentia (Orchard,
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2006).
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In central to southern British Columbia, Anisian (Middle Triassic) to Rhaetian (Late Triassic) strata
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overlying Laurentia are interpreted as foreland basin deposits derived from YTT and Laurentia following
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their collision in the Permian (Golding et al., 2016a). However, detrital zircon populations in these strata can
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be explained by a Laurentian source with the minor addition of sediment from YTT or Stikinia, to account
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for the presence of four zircon grains with Mississippian ages and three zircon grains with Permian ages,
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(Ferri, 2009; Ferri et al., 2010; Golding et al., 2016a). Additionally, Rhaetian clastic strata in central British
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Columbia analysed by Golding et al. (2016b), are dominated by Late Triassic euhedral zircon grains that
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suggest a volcanic source from Quesnellia. As such, these data indicate that Middle to Late Triassic
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sedimentary strata in southern and central British Columbia can be explained coherently with sources
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derived from Laurentia and Stikinia/Quesnellia, with no demand for a YTT sediment source (Golding et al.,
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2016a, b). As such, detrital zircon data from Triassic strata in Yukon, British Columbia and one sample in
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Alaska do not indicate that YTT collided and accreted to Laurentia during the Permian.
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(4) Paleomagnetic studies from across the Northern Cordillera suggest that between 90-70 Ma and 50 Ma,
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YTT, SMT and parautochthonous parts of Laurentian were fixed together as they moved northwards to their
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current position relative to stable North America (see reviews of Gabrielse et al., 2006 and Enkin, 2006).
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Prior to this, paleomagnetic data from Middle Pennsylvanian – early Permian red cherts from SMT in the
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Sylvester allochthon (Figure 1a) and at Sliding Mountain, in northern and central British Columbia, suggest
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that these parts of SMT were deposited ~20° south of their current locations with respect to stable North
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America (Richards et al., 1993). Secondary magnetization suggests that following deposition at equatorial
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latitudes, these chert units migrated northwards with respect to Laurentia until the Early to Middle Jurassic.
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Based on the occurrence of an Early Jurassic chemical remagnetization event (Cole et al., 1992) recorded
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locally within the Cache Creek terrane (Figure 1), and on the intersection of the small circle for the
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secondary magnetization pole in these chert units with the Middle to Late Jurassic portion of the apparent
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polar wander path for Laurentia (their Figure 8), Richards et al. (1993) favoured an Early to Middle Jurassic
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timing of obduction and accretion of these SMT units to Laurentia. This contradicts the Permian timing for
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closure of Slide Mountain Ocean favoured by most authors.
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(6) Of most striking contrast to the Klondike orogeny model of Beranek and Mortensen (2011) and others,
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are the Cordilleran Ribbon Continent models for the Northern American Cordillera (Johnston, 2008;
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Hildebrand, 2009). These models proposed that parts of the parautochthonous Laurentian margin, such as
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the Cassiar platform (CA – Figure 1) in Yukon and British Columbia are actually exotic with respect to
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Laurentia and collided with the intermontane terranes (YTT, Stikinia, Quesnellia) in the Late Triassic to
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form a composite continental ribbon. Accretion of the ribbon continent to Laurentia is proposed to occur in
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the Cretaceous (Johnston, 2008; Hildebrand, 2009). This model has received little support from the scientific
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community (e.g. Monger, 2014; Colpron et al., 2015; Sigloch & Mihalynuk, 2017; Matthews et al., 2017;
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2018), partly because the occurrence of a Cretaceous suture between ribbon continent and Laurentia, which
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should be located inboard of the Cassiar platform, remains cryptic (e.g. Johnston, 2008; Monger, 2014).
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3. STUDY AREA: THE DUNITE PEAK OPHIOLITE AND LOCAL GEOLOGY
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The Dunite Peak ophiolite (DPO, Figure 1e and 2) forms klippen of mid-Permian mafic-ultramafic rocks
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(267 ± 10 Ma, de Keijzer et al., 2000) previously assigned to SMT (Figure 2), overlying rocks previously
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assigned to YTT (Parsons et al., 2017a,b). The location of the DPO study area (Figure 2) with respect to the
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major terrane boundaries is indicated on Figure 1. The tectonic boundary between YTT and Laurentia
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(Cassiar terrane, Figure 1), is inferred to lie 5 km east of the study area shown in Figure 2 (Colpron et al.,
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2016a). This boundary is structurally equivalent to the Middle Triassic to Early Jurassic ductile and post-
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Jurassic brittle Tummel fault zone (Figure 1i, Colpron et al., 2005) and the post-Late Triassic Inconnu thrust
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(Murphy et al., 2006). To the west of the study area, the N-S striking d’Abbadie fault system (Figure 2) had
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an early normal sense of motion and subsequent post-96 Ma right-lateral strike-slip motion with ~4 km
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dextral displacement that truncated the DPO along its length (de Keijzer et al., 1999; Colpron et al., 2017).
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The dominant transposition foliation within the DPO and all underlying units is sub-parallel to
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compositional layering. Mineral stretching lineations and shear-sense indicators in these units broadly
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correspond to a NE-SW transport direction, most commonly with a top-SW shear sense. These fabrics are
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folded by an open synform that plunges gently WSW (Figure 2). The bedrock geology in the Dunite Peak
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region (Figure 2) may be split into three distinct units, listed from structurally lowest to highest: (1) A basal
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marble unit; (2) a marine metasedimentary succession; and (3) the Dunite Peak ophiolite. Within each of
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these, unit subdivisions are identified, as described below. Additional field observations from this area are
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described by Parsons et al., 2017a, b and de Keijzer et al. (1999, 2000).
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3.1. Basal marble unit
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The structurally lowest unit (Figure 2) comprises coarse grained massively bedded marble, weathered
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yellow-grey, ≥600 m thick, with rare garnet-kyanite bearing metapelitic and garnet-amphibole-epidote
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bearing meta-igneous layers. This basal marble unit is identified as part of the Snowcap assemblage of YTT
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based on the occurrence of Mississippian Simpson Range suite orthogneiss within this metasedimentary
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unit, both north and south of the study area (de Keijzer et al., 2000; Westberg et al., 2009, 2010; Colpron et
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al., 2016a). Based on its lithology, the basal marble unit probably forms the northern continuation of the
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Scurvy Creek succession, a locally defined subdivision of the Snowcap assemblage which crops out 10-30
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km south of our study area (Westberg et al., 2009; 2010; Colpron et al. 2016a).
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3.2. Marine metasedimentary succession
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The marine metasedimentary succession has a structural thickness of ~350-500 m (Figure 2) and is visually
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distinct from the underlying basal marble unit. From bottom to top, this succession divides into four mapped
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units (Figures 2 and 3a): (1) MMS1 – Micaceous and carbonaceous quartzite and carbonaceous shale (~100-
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150 m thick); (2)MMS2 – white quartzite overlain by interbedded quartzite, marble and subordinate
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carbonaceous calc-silicate layers (~100 m thick); (3) MMS3 – a unit of carbonaceous semipelite and shale,
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which locally contains an upper portion of thinly interbedded carbonaceous shale/semipelite and subordinate
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chert, quartzite (silt/sandstone) and metavolcanics (150-250 m thick); at one outcrop, pillow basalt was also
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observed within this unit; and (4) MMS4 – dark grey, micritic, mylonitized marble (200-250 m thick) with
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locally less deformed and fossiliferous zones containing deformed bryozoa and unidentified shelly fauna.
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Mylonitic foliation within the marine metasedimentary succession increases in deformation intensity up-
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section towards the base of the DPO crustal section. A metamorphic assemblage of biotite ± garnet ±
281
staurolite ± chlorite suggests that this unit is of a lower metamorphic grade than the basal marble unit. Based
282
on its lithology and structural relationship with the basal marble unit we speculate that the marine
283
metasedimentary succession may correlate with either the Nasina assemblage or Swift River Group of the
284
Finlayson assemblage (e.g. Colpron et al., 2006a; Nelson et al., 2006).
285
3.3. The Dunite Peak ophiolite (DPO)
286
The DPO has a variable structural thickness of ~450 m to >1650 m, and comprises a crustal section of mafic
287
to intermediate volcanic/volcaniclastic and plutonic rocks, structurally overlain by ultramafic rocks (Figures
288
2 and 3).
289
Crustal Section (DPc)
290
The DPO crustal section (DPc, Figure 2) is an internally deformed thrust stack of metamorphosed basaltic to
291
andesitic volcanics and volcaniclastics, gabbro and leucogabbro with a variable thickness of ~300-650 m
292
(Figures 2 and 3). The degree of metamorphism and deformation in these rocks is such that it is often not
13
293
possible to distinguish between volcanic, volcaniclastic and hypabyssal lithologies. Henceforth, we use the
294
term ‘greenstone’ to collectively refer to the metamorphosed products of these rock types. Generally, the
295
lithologies of this unit (Figure 4) transition from a lower portion of fine to medium grained (≤1 mm)
296
greenstone to an upper coarser grained portion of interlayered greenstone, gabbro and leucogabbro.
297
The base of the DPO crustal section is dominated by light green, very fine grained, homogeneous and
298
locally fissile greenstone with rare pelitic and silicic horizons and sheared pillows (Figure 4a-c). These rocks
299
probably represent volcanic and volcaniclastic successions erupted/deposited in a subaqueous environment
300
with intermittent chert and argillite deposition. Up-section, the DPO crustal section is dominated by gabbro
301
and coarser grained pyroxene- ± plagioclase-phyric greenstone that probably represent a mix of plutonic and
302
vent-proximal volcanic and hypabyssal successions (Figure 4d-e). In the upper portion of the crustal section,
303
pelitic and silicic horizons are not observed, and gabbro and leucogabbro commonly intrude greenstone
304
(Figure 4e-f). Variability in grain size and in relative proportions of leucocratic to melanocratic minerals
305
within the gabbro and leucogabbro define compositional layering sub-parallel to foliation with locally
306
undulating and discordant boundaries corresponding to original intrusive relationships. The top of the crustal
307
section consists of medium to coarse grained (~0.5-2 mm) cumulate to adcumulate gabbro, leucogabbro and
308
plagiogranite and subordinate fine grained greenstone layers (Figure 4f). Leucogabbro contains rare rafts of
309
greenstone.
310
The DPO crustal section is pervasively sheared with a mylonitic fabric at its lower and upper contacts.
311
Thrust imbrication of this unit incorporates thrust-bounded slivers of the marine metasedimentary succession
312
(MMS3, Figure 2). A peak metamorphic mineral assemblage of hornblende-actinolite + epidote-clinozoisite
313
+ albite-oligoclase is indicative of upper greenschist to lower amphibolite facies conditions. Peak
314
metamorphic conditions do not appear to vary between vertical structural positions or between
315
metavolcanic/volcaniclastic units and metaplutonic units. As such, the observed metamorphism of the DPO
316
probably corresponds to burial and heating during or after emplacement, rather than metasomatism during
317
ophiolite formation, which would display increasing metamorphic grade from supracrustal to plutonic
318
sections of an ophiolite.
319
Ultramafic Section (DPu)
14
320
The ultramafic section of the DPO is the structurally highest unit (DPu, Figures 2 and 3) and forms isolated
321
klippen emplaced onto the DPO crustal section (DPc) with variable thicknesses of ~150 m to >1000 m
322
(Figures 2-3). The lowermost ~5-50 m of these klippen (DPu1, Figure 2) are ubiquitously defined by
323
sheared, locally cataclastic blue-green and dark-blue-black ‘fish-scale’ serpentinite (Figure 3b). This
324
transitions up-section into orange-weathered, variably serpentinized harzburgite and dunite with subordinate
325
lherzolite (DPu2, Figure 2). Pyroxene-rich layers define compositional layering within these rocks, which
326
vary in orientation across the klippen. Planar intrusions of pyroxenite and gabbro cross-cut these ultramafic
327
rocks (DPu3, Figures 2 and 3b). Dunites contain aggregates of undeformed olivine and serpentine-
328
psuedomorphs of olivine with interlocking, adcumulate textures and no interstitial material between grains.
329
Harzburgites contain orthopyroxene phenocrysts with oikocrysts of olivine and clinopyroxene, plus chromite
330
with orthopyroxene overgrowths that may be indicative of exsolution cumulate residuum. The basal
331
serpentinite of the DPO ultramafic section (DPu1) displays S-C fabrics with C-planes parallel to mylonitic
332
foliation in underlying DPO crustal section. S-planes show no consistent transport direction. Above this,
333
thrust faulting and chaotic folding decrease in intensity up-section until they are absent from the orange-
334
weathered upper portion of planar-stratified ultramafic layers (DPu2).
335
4. U-Pb ZIRCON GEOCHRONOLOGY
336
Zircon U-Pb isotopic analysis was conducted for geochronology on sample 16RAY-AP074A1; a coarse
337
grained gabbro intruded into greenstone from the top of the DPO crustal section (Figure 2). This gabbro
338
does not cross-cut the deformation fabric in the greenstone. Analyses were conducted by secondary ion
339
microprobe spectrometry (SIMS) at the U.S. Geological Survey-Stanford University SHRIMP-RG (sensitive
340
high resolution ion microprobe-reverse geometry) facility. Analytical procedures are described in detail in
341
Supplementary Materials 01. The full U-Pb isotopic dataset is presented in Supplementary Materials 02.
342
Sample 16RAY-AP074A1 yielded euhedral to subhedral zircon with oscillatory zoning and some thin
343
cathodoluminescence (CL) dark, high-U rims that may reflect resorption (Figure 5a). Spot analyses (Figure
344
5a) conducted on 12 zircon grains produce a simple cluster of grain ages overlapping concordia and,
345
excluding the oldest analysis, define a weighted mean
206
Pb/238U age of 265 ± 4 Ma (MSWD = 0.9; Figure
15
346
5b). The oldest analysis (283 ± 4 Ma) was obtained from a euhedral, CL-bright, low-U (50 ppm) grain core
347
domain (spot 4.1, Figure 5a) and inclusion of this grain yields a mean age of 268 ± 6 Ma (MSWD = 2.7).
348
Whilst analytical scatter cannot be ruled out, textural evidence suggests that the core domain represents a
349
xenocryst that records an earlier magmatic history. Chondrite-normalized trace element signatures are
350
depleted in LREEs relative to HREEs and have little variation between each grain (Figure 5c). Together, the
351
trace element signatures, grain morphology and spread of individual grain ages suggest that the calculated
352
mean age reflects the timing of crystallization of the magmatic protolith. Ti-in-zircon thermometry (Ferry &
353
Watson, 2007) yields a mean zircon crystallization temperature of 761±21 °C (1σ error).
354
5. GEOCHEMISTRY
355
The degree of metamorphism and deformation recorded by the DPO makes it difficult to identify and
356
distinguish between specific igneous protoliths using field observations and optical microscopy alone. We
357
utilize whole-rock major and trace element and Sm-Nd isotopic analyses to provide additional constraints on
358
protoliths and igneous petrogeneses of different rock types in the DPO. Whole-rock geochemical analyses of
359
52 samples were conducted by Activation Laboratories Ltd. (Ancaster, ON). Sm-Nd isotopic analysis of 7
360
samples was conducted at Carleton University (Ottawa, ON). Analytical procedures for both analyses are
361
described in Supplementary Materials 01.
362
5.1. Immobile element fingerprinting
363
For interpretation of the whole-rock element analysis, only immobile rare earth elements (REEs) and high
364
field strength elements (HFSEs) are considered, in order to minimize the effects of element mobility during
365
metamorphism (e.g. Pearce, 1996; 2014). REE-HSFE profiles (Figure 6) and normalized element
366
concentrations and ratios (Table 1) are given relative to N-MORB (Sun & McDonough, 1989, plus V and Sc
367
from Klein, 2004) for Groups 1-4, defined below and relative to primitive mantle (Sun & McDonough,
368
1989, plus V and Sc from McDonough & Frey, 1989) for Group 5, defined below. Immobile element ratios
369
Nb/Y and Zr/Ti provide proxies for Na2O+K2O (total alkalinity) and SiO2, respectively (Cann, 1970; Pearce,
370
1996) (Figure 7a). Fractionation of immobile elements Y, La and Nb provides a means to classify crustal
371
samples in terms of magmatic setting, due to the variable sensitivity of these elements to degree of partial
16
372
melting/fractionation, composition of melt source and subduction zone interaction (Figure 7b) (Cabanis &
373
Lecolle 1989). Relative concentrations of Th, Nb, and Yb, provide a means to distinguish suprasubduction
374
zone (SSZ) settings from intra-plate and mid-ocean spreading ridge settings (Figure 7c) (Pearce, 2008,
375
2014). Th and Nb behave similarly in the mantle (Th/Nb ≈ 1), except during subduction where Nb is
376
retained in the subducting slab, whilst Th is released from the subducting slab into the mantle wedge. This
377
results in high positive Th/Nb ratios in mantle wedge-derived magmas (Pearce, 2008). The concentration of
378
Yb, relative to Th and Nb provides an indication of degree of fractionation, which may be used to
379
distinguish intra-oceanic arc from continental arc settings and mid-ocean ridge from intra-plate settings
380
(Pearce, 2008; 2014).
381
From the 52 samples analyzed, five geochemically distinguishable groups are defined. Groups 1 to 3 contain
382
mafic to intermediate samples from the DPO that are distinguished from each other on geochemical bases,
383
irrespective of lithology, following the identification of three distinct geochemical signatures. Group 4
384
contains a single sample of pillow basalt from the marine metasedimentary succession (MMS3). Group 5
385
contains ultramafic samples from the DPO. Locations of samples are given in Figure 2 with group-specific
386
symbology. Seven fine-grained greenstone samples from the DPO were selected for Sm-Nd isotopic analysis
387
prior to distinction of Groups 1 to 3. Of these seven samples, four derive from Group 1 and three derive
388
from Group 3. The results of Sm-Nd isotopic analyses are reported alongside the whole-rock analyses of
389
these groups.
390
Group 1 (DPO mafic to intermediate rocks)
391
Group 1 (n =18) displays LREE enriched spectra and large Th/Nb anomalies (Figure 6a), and may be
392
divided into two subgroups based on the relative concentrations of Ti, V and Sc (Figure 6a). Group 1a has
393
less enrichment ([La/Yb]N = 2.87, LaN = 1.08, [Th/Nb]N = 14.67) than Group 1b ([La/Yb]N = 4.68, LaN =
394
4.21, [Th/Nb]N = 27.95). Group 1a displays minor negative and a single strong positive Ti anomaly. V and
395
Sc are enriched relative to other HREEs and Ti. These samples display minor negative anomalies in Zr-Hf
396
(Figure 6a). In contrast, Group 1b displays strong negative Ti, V and Sc anomalies, but no Zr-Hf anomalies
397
(Figure 6a). Small positive Eu anomalies are common in both subgroups. Sm-Nd isotopic analysis of four
17
398
samples from Group 1 yielded ƐNd(t=265) values of +7.2, +7.4, +7.5 (Group 1a) and +7.4 (Group 1b) (Table
399
1).
400
Group 2 (DPO mafic to intermediate rocks)
401
Group 2 (n = 11, Figure 6b) displays moderately LREE-enriched to flat spectra ([La/Yb]N = 2.91). Element
402
concentrations are depleted relative to N-MORB by up to a factor of 10 (LaN = 0.85, YbN = 0.32). Group 2
403
samples have large Th/Nb ratios ([Th/Nb]N = 17.43), negative Ti anomalies and strong positive V and Sc
404
anomalies relative to HREEs and Ti (Table 1). Negative Zr-Hf anomalies and positive Eu anomalies are
405
sometimes displayed (Figure 6b).
406
Group 3 (DPO mafic to intermediate rocks)
407
Group 3 (n = 6, Figure 6b) displays flat spectra ([La/Yb]N = 1.41) with N-MORB-comparable
408
concentrations (LaN = 1.49, YbN = 1.07). All samples have positive Th/Nb ratios ([Th/Nb]N = 5.29) and
409
negligible to small positive V anomalies, negative Sc anomalies, but no significant Ti or Eu anomalies.
410
Three samples from Group 3 yielded ƐNd(t=265) values of +8.3, +8.1 and +9.0 (Table 1).
411
Group 4 (pillow basalt)
412
Group 4 (n = 1, Figure 6c) has an LREE-enriched spectrum ([La/Yb]N = 2.14) with N-MORB-comparable
413
concentrations of HREEs (LaN = 1.42, YbN = 0.66). Unlike Groups 1-3, Group 4 has no Nb anomaly
414
([Th/Nb]N = 1.55), nor does it have Ti, V, Sc or Eu anomalies (Table 1).
415
Group 5 (DPO ultramafic rocks)
416
Group 5 (n = 16, Figure 6d) comprises samples from the DPO ultramafic section (DPu). CIPW normative
417
major element concentrations of Group 5 samples mostly plot within the harzburgite (6 samples) and dunite
418
(6 samples) fields. A minority plot within lherzolite (3 samples) and pyroxenite (1 sample) fields (Figure
419
7d). Two reference compositions for depleted-MORB mantle (DMM – Salters & Stracke, 2004; Workman
420
& Hart 2005) are also included on the REE-HFSE diagram (Figure 6d). Group 5 is depleted in HREEs
421
relative to primitive mantle and DMM (YbN = 0.21). LREEs are enriched relative to HREEs and DMM (LaN
18
422
= 0.50, [La/Yb]N = 2.37). Several samples have positive Th anomalies equal to, or greater than primitive
423
values (ThN = 1.06), and most have Nb concentrations below the analytical detection limit. One sample had
424
detectable amounts of both Th and Nb, producing [Th/Nb]N = 14.26. Positive V and Sc and Zr anomalies are
425
common.
426
5.2. Interpretation of geochemistry results
427
Group 1 comprises greenstone and gabbro from the DPO crustal section (Figure 6a). Differences between
428
Groups 1a and 1b probably reflect crystal fractionation processes. Group 1a plots within subalkaline basaltic
429
to basaltic andesite island arc tholeiite (IAT) fields and probably represents plutonic/hypabyssal IATs
430
(Figure 7a-b). These samples have positive V, Eu, and Sc anomalies, plus one positive Ti anomaly, and
431
negative Zr-Hf anomalies. These are generally attributed to crystallization and retention of magnetite/rutile
432
(Ti enrichment) and clinopyroxene (Sc enrichment) and extraction of an intermediate-acid melt (Zr-Hf
433
depletion) (e.g. Pearce, 1996). Positive V anomalies are generally attributed to hydrous mantle melting (e.g.
434
Pearce, 2014). Positive Eu anomalies are most easily explained by the presence of cumulate plagioclase (e.g.
435
Rollinson, 1993). Positive Th/Nb ratios and negative Nb anomalies suggest a SSZ setting (Figure 7c).
436
Group 1b plots within basaltic-andesite to andesite IAT–calc-alkaline (CA) fields (Figure 7a-b) and
437
represents a more fractionated component of IAT to CA hypabyssal magmatism or volcanism. This is
438
suggested by negative Ti anomalies and the absence of Zr-Hf anomalies; Ti is depleted in moderately
439
evolved magmas due to early fractionation of Ti-bearing phases in basaltic magmas, whereas Zr and Hf
440
remain incompatible during fractionation of intermediate melts. Negative Sc anomalies can be attributed to
441
early clinopyroxene fractionation in basaltic magmas. Negative V anomalies may be attributed to increased
442
compatibility of V during crystal fractionation of intermediate melts (e.g. Pearce, 1996). Positive Th/Nb
443
ratios and negative Nb anomalies suggest a SSZ setting (Figure 7c). ƐNd values from Groups 1a and 1b
444
ranging between +7.2 and +7.5, indicate that these magmas did not interact with continental crust (e.g.
445
Rollinson, 1993).
446
Group 2 comprises layered gabbro, leucogabbro and subordinate greenstone from the DPO crustal section
447
(Figure 6b) with subalkaline basaltic to basaltic andesite compositions (Figure 7a). These data form an array
19
448
from the intersection between IAT-CA and CA fields to the intersection between IAT, N-MORB and back-
449
arc basin basalt (BABB) fields, mostly plotting in the IAT field (Figure 7b). Based on the same
450
interpretations as provided for Group 1a (see above), the depleted nature of Group 2 including Zr-Hf
451
negative anomalies and V-Sc positive anomalies suggests that these rocks represent crustal cumulates
452
derived from hydrous mantle melting. Variations in Ti and V most likely reflect variable proportions of
453
cumulate phase (Ti depleted) versus melt phase (Ti enriched) ± later addition of Ti-bearing fluids, as
454
suggested by the presence of titanite veins in some samples. Positive Th/Nb ratios and negative Nb
455
anomalies suggest a SSZ setting (Figure 7c).
456
Group 3 comprises gabbro intrusions from the DPO ultramafic section and greenstone from the DPO crustal
457
section (Figure 6b) with subalkaline basaltic N-MORB-comparable compositions (Figure 7a-b) plus Nb and
458
V anomalies suggesting subduction zone interaction (Figure 7c) and hydrous mantle melting (e.g. Pearce,
459
1996; 2014). Minor negative Sc anomalies probably reflect earlier crystallization of clinopyroxene (e.g.
460
Pearce, 1996). Group 3 is interpreted as primary BABB melts derived directly from depleted mantle, with
461
little or no subsequent crystal fraction or melt extraction. Positive Th/Nb ratios and negative Nb anomalies
462
suggest a SSZ setting (Figure 7c). ƐNd values from Group 3 ranging between +8.8 and +9.0, indicate that it
463
has not interacted with continental crust (ƐNd of depleted mantle = 9.0-9.6, Kimura et al., 2017).
464
Group 4 is a pillow basalt sample from the marine metasedimentary succession (Figure 6c), and has a
465
geochemical signature comparable to subalkaline E-MORB (Figure 7a-c). The stratigraphic association of
466
Group 4 with the marine metasedimentary succession and absence of E-MORB signatures from the DPO
467
(one Group 1a sample excepted) suggest that Group 4 does not derive from the same SSZ setting as Groups
468
1-3.
469
Group 5 comprises ultramafic rocks from the DPO (Figure 6d) that displays lithological, petrographic (see
470
Section 3.3) and geochemical characteristics typical of lower crustal or mantle cumulates, rather than mantle
471
tectonites. It is dominated by dunite and harzburgite with cumulate and adcumulate textures. Enrichment in
472
LREEs relative to HREEs and large V/Ti ratios suggest that Group 5 derived from partial melting of the
473
mantle under hydrous conditions. Positive Sc anomalies probably reflect the presence of cumulate
20
474
clinopyroxene. Positive Zr anomalies may correspond to enrichment from slab-derived fluids (e.g. Bizimis
475
et al., 1999) or recycling of lower crustal material during crustal foundering (e.g. Arndt & Goldstein, 1989).
476
Strong depletion in Nb (all but one Group 5 sample have Nb concentrations below the detection limit), and
477
enrichment in Th and the presence of BABB intrusions (Group 3) within these rocks suggests that the DPO
478
ultramafic section formed in the same SSZ setting as Groups 1-3.
479
6. PETROGENESIS OF THE DUNITE PEAK OPHIOLITE
480
Large Th/Nb ratios, large positive ƐNd values, enriched concentrations of LREEs and N-MORB-comparable
481
concentrations of HREEs indicate that the DPO is an SSZ ophiolite (Figure 7b-c) comprising a dismembered
482
crustal section and lower crustal/lithospheric mantle cumulates of an intra-oceanic arc system. U-Pb zircon
483
geochronometry from a Group 2 IAT gabbro (this study, Figures 2 and 5) and a leucocratic granitic dike (de
484
Keijzer et al., 2000, Figure 2) within the DPO crustal section yielded respective ages of 265 ± 4 Ma and 267
485
± 10 Ma. The ages and geochemical signatures of these rocks suggest that constructional volcanism was
486
occurring along an intra-oceanic arc that resided somewhere within the ocean separating YTT and Laurentia
487
during the mid-Permian (currently modelled as the Slide Mountain Ocean). The single zircon xenocryst age
488
(283 ± 4 Ma) from sample 16RAY-AP074A1 (this study), may derive from the Group 1 IAT greenstone into
489
which it intrudes (e.g. Figure 4e-f), corresponding to the earliest record of magmatism along this intra-
490
oceanic arc. Comparison of volcanic glass and whole rock REE-HFSE signatures of basalt, basaltic andesite
491
and andesite samples collected from four active intra-oceanic arc settings in the SW Pacific Ocean (Figure
492
8) with geochemical signatures from the Dunite Peak ophiolite supports our interpretation that the Dunite
493
Peak ophiolite derived from an intra-oceanic arc system (Figure 8b, e) in which arc (IAT/CA) and
494
subordinate back-arc (BABB) magmatic assemblages were generated co-spatially (Figure 8c, f).
495
6.1. Correlative SSZ ophiolites in the Northern Cordillera
496
The DPO is comparable to other mid-Permian ophiolites currently assigned to SMT that comprise sections
497
of oceanic crust and lithospheric mantle with mafic to intermediate SSZ geochemical signatures (e.g.
498
Mortensen, 1990; Nelson & Bradford, 1993; Dusel-Bacon et al., 2006; Petrie et al., 2015). These
499
comparable sections are as follows:
21
500
In Division II of the Sylvester allochthon, north British Columbia (Figure 1a), the Quartzrock Creek gabbro,
501
Cassiar block, Zus Mountain block and Blue Mountain block form ophiolitic sections of coarse grained
502
cumulate gabbro and leucogabbro, layered clinopyroxene and dunite and tectonized harzburgite (Gabrielse
503
et al., 1993; Nelson, 1993; Nelson & Bradford, 1993). U-Pb zircon geochronology from a layered
504
leucogabbro in the Zus Mountain block yielded an age of 268.6 +6.8/-3.4 Ma (Figure 1a) (Gabrielse et al.,
505
1993). Geochemical signatures from Division II basalts (Nelson, 1993) are mostly N-MORB; however a
506
minority of these samples have arc signatures (IAT or CA) requiring an SSZ setting.
507
In south-central Yukon, the St Cyr klippe and Tower Peak assemblage (Figure 1d) comprise harzburgite,
508
gabbro, leucogabbro and basaltic to andesitic metavolcanic rocks currently assigned to SMT (Fallas et al.,
509
1998; 1999; Petrie et al., 2015). Andesitic greenschists from the Tower Peak assemblage have IAT to CA
510
geochemical signatures (Fallas et al., 1999) indicative of a SSZ setting. In the Finlayson Lake district
511
(Figure 1c) most occurrences of SMT have N-MORB, E-MORB and OIB geochemical signatures. However,
512
localized occurrences of SMT greenstone, gabbro and leucogabbro have signatures ranging between
513
IAT/CA, BABB and N-MORB (Plint & Gordon, 1997; Murphy et al., 2006; Piercey et al., 2012) suggestive
514
of a SSZ setting. Locally, in the Finlayson Lake district (Figure 1c), gabbro and leucogabbro are commonly
515
observed intruding greenstone (Plint & Gordon, 1997), as is observed in the DPO. U-Pb zircon
516
geochronology of a leucogabbro, and of a plagiogranite within a serpentinized shear zone (Figure 1c-d),
517
respectively yielded crystallization ages of 273.4 ± 1.4 Ma (Murphy et al., 2006) and 274.3 ± 0.5 Ma
518
(Mortensen, 1992b).
519
In the Glenlyon region, central Yukon, the Tummel fault zone (Figure 1i) forms the boundary between YTT
520
and Laurentia, comprising fault slices of SMT serpentinized harzburgite mantle tectonite, gabbro,
521
greenstone and associated marine sedimentary rocks (Colpron et al., 2005, 2006b). Greenstones have
522
basaltic to andesitic compositions and geochemical signatures that mostly range between N-MORB and IAT
523
(Colpron et al., 2005, 2006b), suggesting an SSZ origin. To the northwest, the Ragged Lake klippe (Figure
524
1j) comprises serpentinite and gabbro, structurally overlying Laurentia with an IAT/CA geochemical
525
signature (Colpron et al., 2005, 2006b). U-Pb zircon geochronology from an IAT andesitic greenstone in the
22
526
Tummel fault zone and from the IAT/CA gabbro in the Ragged Lake klippe respectively yielded
527
crystallization ages of 267.8 ± 1.5 Ma and 260.3 ± 0.8 Ma (Figure 1, Colpron et al., 2005, 2006b).
528
In west-central Yukon and east-central Alaska, ophiolitic klippen of SMT and the Seventymile terrane
529
(Alaskan correlative of SMT) structurally overlie YTT, comprising pyroxene-phyric greenstone, cumulate
530
gabbro, harzburgite, dunite and subordinate clinopyroxenite (Figure 1o, Foster & Keith, 1974; Foster et al.,
531
1994; Mortensen, 1990; Dusel-Bacon et al., 2006). Notable ophiolite occurrences include Clinton Creek
532
(Mortensen, 1990; Dusel-Bacon et al., 2006), Mount Sorensen, Salcha River and American Creek (Foster et
533
al., 1994; Dusel-Bacon et al., 2006). Geochemical signatures of greenstones in the Eagle quadrangle
534
(Alaska) and Clinton Creek/Dawson area (Yukon) (Figure 1o) range between N-MORB, BABB and CA
535
(Dusel-Bacon et al., 2006), suggestive of a SSZ setting. Metaharzburgite in the Eagle quadrangle has a
536
similar Nb depletion and Th enrichment to our Group 5 DPO samples that is suggestive of a SSZ setting
537
(Dusel-Bacon et al., 2013). Most notably, the Wolf Mountain klippe is dominated by greenstone with
538
basaltic to andesitic and IAT to CA geochemical signatures (Dusel-Bacon & Cooper, 1999; Dusel-Bacon et
539
al., 2006) that closely resemble IAT/CA greenstone from the DPO.
540
7. THE DUNITE PEAK INTRA-OCEANIC ARC
541
As outlined above, mid-Permian SSZ ophiolites with mean crystallization ages of ~275-260 Ma (including
542
the DPO), are distributed along the structural boundary between YTT and Laurentia over a distance of
543
~1000 km between northern British Columbia, Yukon and eastern Alaska (Figure 1). Based on their similar
544
lithological, structural, geochemical and geochronological characteristics, we propose that collectively, they
545
represent tectonic slivers of a regionally extensive intra-oceanic extensional arc system that was active
546
within the Slide Mountain Ocean from 275 and 260 Ma. If our oldest zircon dated from IAT gabbro sample
547
16RAY-AP074A1 (283 ± 4 Ma) was inherited from the greenstone layer also of IAT composition (sample
548
16RAY-AP074A2, Table 1), into which it intrudes, then magmatism along this intra-oceanic arc occurred as
549
early as ~280 Ma. This is the first recognition of this arc system, which we define here as the Dunite Peak
550
intra-oceanic arc.
23
551
The DPO and correlative ophiolitic sections at the Tummel fault zone and Ragged Lake, St Cyr and Wolf
552
Mountain klippen (Figure 1) are dominated by basaltic to andesitic arc-magmatic rocks (IAT/CA), which we
553
interpret as constructional volcanic centers along the Dunite Peak intra-oceanic arc. Correlative ophiolitic
554
sections in the Sylvester allochthon (Figure 1a) and Finlayson Lake district (Figure 1c) have been
555
interpreted as remnants of a fossil transform fault system (Nelson & Bradford, 1993; Murphy et al., 2006;
556
Piercy et al., 2012) or ocean core complexes and syn-volcanic extensional faults (Ryan et al., 2015), and
557
yield geochemical signatures indicative of extensional magmatism in an SSZ setting (BABB, N-MORB ± E-
558
MORB). We interpret these sections as extensional magmatic zones along the Dunite Peak intra-oceanic arc.
559
The distribution of constructive volcanic centers (e.g. DPO, Wolf Mountain klippe) and extensional
560
magmatic zones (e.g. Zus Mountain block, Sylvester allochthon) suggests that the Dunite Peak intra-oceanic
561
arc may represent a disorganized extensional intra-oceanic arc (e.g. Weissel et al., 1981; Tamaki, 1985;
562
Wysoczanski et al., 2010). These systems are characterized by constructional volcanic centers surrounded
563
by localized zones of disorganized extensional faulting and associated magmatism. Extensional magmatism,
564
typically considered indicative of back-arc spreading (BABB) may occur along strike, adjacent to, and
565
contemporaneous with constructive arc-related magmatism (IAT/CA). Modern examples of disorganized
566
extensional intra-oceanic arcs include the Kermadec arc – Havre trough system (Wysoczanski et al., 2006;
567
2010; Smith et al., 2009), and the Lau basin (Keller et al., 2008; Sleeper & Martinez, 2014; Sleeper et al.,
568
2016) in the SW Pacific Ocean (Figure 8) and the Calabrian arc in the Mediterranean Sea (Florio et al.,
569
2011). In the geological record, comparable disorganized extensional intra-oceanic arc systems have been
570
inferred for the ancient settings of the Permian Nahlin ophiolite of the Cache Creek terrane in northern
571
British Columbia (McGoldrick et al., 2017) and the Middle Ordovician Annieopsquotch Accretionary Tract
572
of the Newfoundland Appalachians (Zagorevski et al., 2015). The development of the Dunite Peak intra-
573
oceanic arc as a disorganized extensional intra-oceanic arc provides a plausible explanation for the relatively
574
small volume of identifiable remnants of this arc and its elusiveness in the geological record.
24
575
8. INTEGRATION WITH EXISTING DATASETS: A NEW HYPOTHESIS FOR THE LATE
576
PALEOZOIC – EARLY MESOZOIC TECTONIC EVOLUTION OF THE NORTHERN
577
CORDILLERA
578
Slide Mountain Ocean could not have formed the lower plate of a westward-dipping subduction zone
579
beneath YTT (e.g. Mortensen, 1992a; Nelson et al., 2006; Beranek and Mortensen, 2011), at the same time
580
that it generated SSZ ophiolites with upper-plate intra-oceanic arc geochemical compositions (as required by
581
geochemical and geochronological constraints). This would require a more complicated double subduction
582
zone model that would still fail to adequately explain the variable duration and timing of YTT eclogitization,
583
SSZ ophiolite formation, Klondike cycle magmatic rocks and mid-Permian to Middle Triassic exhumation
584
of YTT. We propose an alternative model: structural juxtaposition of mid-Permian SSZ ophiolites and mid-
585
Permian YTT eclogites along the eastern margin of YTT (Figure 1) (e.g. Fallas et al., 1998; Petrie et al.,
586
2015, 2016; Gilotti et al., 2017) by eastward subduction and collision of YTT (lower plate) beneath the
587
Dunite Peak intra-oceanic arc (upper plate) (Figure 9). In the following sections, we present a new
588
hypothesis for the Klondike orogeny (Figure 9) in the context of our analyses of the Dunite Peak ophiolite,
589
combined with existing datasets from across the Northern Cordillera. This includes datasets that were
590
previously inconsistent or hard to reconcile with previous models (see Section 2.1). Our proposed model is
591
supported by an extensive geochronology dataset (total of 110 published ages), displayed in Figure 10 (see
592
Supplementary Materials 05 for details), to constrain the timing of specific events. Note that in our model,
593
use of the term ‘Klondike orogen’ refers to the accreted mass (i.e. composite terrane) of YTT and the Dunite
594
Peak intra-oceanic arc.
595
8.1. Mid- to late Permian arc-continent collision: the Klondike orogeny
596
~280-260 Ma: Dunite Peak intra-oceanic arc magmatism and subduction and collision of YTT
597
continental crust
598
Subduction related magmatism within the Dunite Peak intra-oceanic arc (Figure 1) is bracketed between
599
~280 and 260 Ma (Figures 9a & 10, this study; Mortensen, 1992b; Gabrielse et al., 1993; de Keijzer et al.,
600
2000; Colpron et al., 2005; 2006b; Murphy et al., 2006). Along the length of this intra-oceanic arc,
25
601
lithological and geochemical variations between ophiolites (see Sections 6.1 and 7) probably reflect
602
development of constructive volcanic centers and localized zones of upper-plate extension and associated
603
magmatism, representative of a disorganized extensional intra-oceanic arc such as the present day Kermadec
604
arc – Havre trough system (e.g. Wysoczanski et al., 2010). It is expected that most of the lower plate oceanic
605
lithosphere subducted into the mantle during that period, although some lower plate material may have
606
accreted to the Dunite Peak intra-oceanic arc (blue accretionary prism, Figure 9a). Early Permian and older
607
occurrences of SMT that contain chert, argillite and pillow basalt with mid-ocean ridge and/or within-plate
608
geochemical signatures such as parts of the Campbell Range basalts in the Finlayson Lake district (Figure
609
1c, Murphy et al., 2006; Piercy et al., 2012) may represent accreted remnants of this oceanic lower plate.
610
Subduction and collision of YTT continental crust beneath the Dunite Peak intra-oceanic arc began as early
611
as ~275 Ma (Figure 10, Gilotti et al., 2017) and continued, coeval with magmatism in the Dunite Peak intra-
612
oceanic arc to ~260 Ma (Figures 1e, h, i, g & 10, Creaser et al., 1997; Fallas et al., 1998; Godwin-Bell,
613
1998; Petrie et al., 2016; Gilotti et al., 2017). Many of the recorded eclogite occurrence from YTT are
614
described as eclogite pods hosted within amphibolite, greenschist or blueschist facies rocks (e.g. Erdmer et
615
al., 1998; Fallas et al., 1998; Petrie et al., 2015). Where blueschist is preserved, such as in the Faro, Ross
616
River and St Cyr regions (Figure 1d, g-h), muscovite cooling ages of ~263 to 235 Ma (Erdmer et al., 1998;
617
Fallas et al., 1998) suggest that these rocks may represent lower plate material from an accretionary complex
618
that formed above the subduction zone between YTT and the Dunite Peak intra-oceanic arc (e.g. blue shaded
619
accretionary complex, Figure 9a). However, most exposures of SMT and/or the Dunite Peak intra-oceanic
620
are structurally interleaved with slices of YTT and/or Laurentia (e.g. Mortensen, 1990; Fallas et al., 1998;
621
Murphy et al., 2006; Petrie et al., 2015) suggesting that the original accretionary complex and subduction
622
interface between YTT and the Dunite Peak intra-oceanic arc has been overprinted or structurally displaced
623
from its original configuration. The arrangement of ultramafic over mafic rocks in the DPO and the apparent
624
absence of a metamorphic discontinuity between the DPO and the underlying YTT also suggest that
625
emplacement structures relating to the original subduction zone and accretionary complex between YTT and
626
the Dunite Peak intra-oceanic arc have been structurally overprinted and/or displaced. This probably
26
627
occurred during subsequent regional metamorphism and deformation record in YTT during the latest
628
Triassic to Early Jurassic and Late Jurassic to Early Cretaceous (e.g. Staples et al., 2016).
629
Amphibolite facies metamorphism of YTT metasedimentary units (Snowcap assemblage) in Canada
630
recorded at ~260 Ma (Berman et al., 2007), 259.3 ± 3.4 Ma (Villeneuve et al., 2003) and 263.6 ± 3.4 Ma
631
(Staples, 2014) probably relates to crustal thickening during the final stages of subduction and collision of
632
YTT (Figures 1 & 10). Subduction and eclogitization of YTT and associated magmatism in the Dunite Peak
633
intra-oceanic arc ceased sometime between 265 and 260 Ma (Figure 10). Based on the ages listed here, we
634
define the earliest record of subduction and collision of YTT (~275 Ma) as the start of the Klondike orogeny
635
(Figure 10).
636
The coeval generation of SSZ ophiolites in the Dunite Peak intra-oceanic arc and eclogite facies
637
metamorphism of YTT suggests collision was diachronous. This may imply that the subducting margin of
638
YTT had an irregular shape with promontories and re-entrants and/or that collision of YTT with respect to
639
the intra-oceanic arc was oblique (e.g. Cawood & Suhr, 1992). Similarly, we have no constraint on the
640
length of the Dunite Peak intra-oceanic arc, and so it is possible that YTT collided only with a portion of the
641
arc and that adjacent to the subducting YTT, normal oceanic subduction and associated intra-oceanic arc
642
magmatism was maintained. Present-day collision and subduction of the Australian continent adjacent to
643
subduction of oceanic lithosphere beneath the Solomon – New Hebrides intra-oceanic arc is a modern
644
example of this process (e.g. Hall, 2002). Because of these potential and likely complexities and the lack of
645
further constraints, we make no attempt at estimating the width of oceanic crust subducted beneath the
646
Dunite Peak intra-oceanic arc.
647
265-252 Ma: Slab break-off, subduction polarity reversal, orogenic collapse and associated magmatism
648
The period between 265 and 260 Ma (Figure 10) marks; (1) the latest occurrence of eclogite facies
649
metamorphism of YTT, and magmatism in the Dunite Peak intra-oceanic arc (see above); (2) the earliest
650
record of exhumation and cooling of YTT blueschist and eclogite (Wanless, et al., 1978; Erdmer &
651
Armstrong, 1988; Erdmer et al., 1998; Fallas et al., 1998); (3) the emplacement of orogenic peridotite within
652
YTT (Canil et al., 2003; Johnston et al., 2007); and (4) the beginning of the Klondike magmatic cycle within
27
653
YTT (e.g. Colpron et al., 2006a; Beranek & Mortensen, 2011). We interpret the temporal overlap of these
654
events between 265 and 260 Ma (Figure 10) as a record of cessation of subduction of YTT continental
655
lithosphere accompanied or soon followed by orogenic collapse and associated magmatism (Figure 9b).
656
The Buffalo Pitts peridotite (Figure 1m) has been interpreted as megaboudin of orogenic mantle peridotite
657
emplaced into metasedimentary rocks of YTT during lithospheric extension of the terrane (Canil et al.,
658
2003; Johnston et al., 2007). U-Pb zircon crystallization ages of 261.5 ± 2.3 Ma from an associated
659
leucogabbro, and 262.3 ± 0.4 Ma from an emplacement-related migmatite derived from the YTT
660
metasedimentary rock which hosts the peridotite (Figure 10), mark the timing of peridotite emplacement
661
during extension and exhumation of YTT (Canil et al., 2003; Johnston et al., 2007). This occurred
662
contemporaneously with exhumation of blueschsits and eclogites within the east margin of YTT (Figure 10)
663
(e.g. Erdmer et al., 1998; Fallas et al., 1998).
664
The Klondike magmatic cycle is recorded by granitic plutons (Figure 1) and associated volcanics
665
(collectively referred to as the Klondike assemblage) within YTT between ~265 and 252 Ma (Figure 10) in
666
Yukon, northern British Columbia and eastern Alaska (e.g. Harms, 1985; Gabrielse et al., 1993; Nelson &
667
Friedman, 2004; Liverton et al., 2005; Murphy et al., 2006; Colpron et al., 2006a; Dusel-Bacon et al., 2006;
668
Nelson et al., 2006 and Beranek & Mortensen, 2011). Beranek and Mortensen (2011) argued for syn-
669
tectonic subduction-related magmatism, deformation and metamorphism between 260 and 254 Ma and post-
670
tectonic magmatism between 254 and 252 Ma. However, the reported occurrences of deformed and
671
undeformed Klondike magmatic assemblages collated in Figure 10 do not show a distinct phase of post-
672
tectonic magmatism. Instead, metamorphism and deformation of YTT metasedimentary units is recorded
673
between ~260 and ~252 Ma (Figures 1 & 10, Fallas, 1998; Villeneuve et al., 2003; Berman et al., 2007;
674
Staples, 2014), contemporaneous with Klondike cycle magmatism and exhumation of YTT (Figures 9c &
675
10, Wanless et al., 1978; Htoon, 1981; Erdmer & Armstrong, 1988; Hunt & Roddick, 1988; 1993; Oliver,
676
1996; Erdmer et al., 1998; Fallas et al., 1998; Breitsprecher & Mortensen 2004; Joyce et al., 2015). Within
677
our proposed tectonic framework, the Klondike magmatic cycle is interpreted as either, (1) exhumation-
678
driven and/or asthenospheric flow-driven crustal melting in response to orogenic collapse (i.e. extension)
28
679
after slab break-off (Figure 9b-c) (e.g. Dewey, 1988; Huw Davies & von Blackenburg, 1995; Atherton &
680
Ghani, 2002; Brown et al., 2011; Li et al., 2016), (2) arc-derived magmatism generated in response to
681
initiation of westward subduction beneath the Klondike orogen following slab break-off and subduction
682
polarity reversal (e.g. Stern, 2004); or; (3) a combination of both (1) and (2). All three interpretations fit with
683
geochemical and geochronological constraints from plutonic components of the Klondike magmatic cycle
684
(e.g. Ruks et al., 2006; Beranek & Mortensen, 2011). We also note that magmatism in response to eastward
685
subduction of Panthalassa Ocean beneath YTT cannot be ruled out.
686
We propose that the events described above occurred in response to buoyancy-driven slab break-off from
687
the subducted margin of YTT continental crust (e.g. Cloos, 1993; Afonso & Zlotnik, 2011) followed by
688
initiation of westward subduction and roll-back of the ocean basin that lay east of the Dunite Peak intra-
689
oceanic arc (e.g. Dewey, 1988; Huw Davies & von Blackenburg, 1995; Atherton & Ghani, 2002; Duretz et
690
al., 2010; Brown et al., 2011). Obduction of SSZ ophiolites of the Dunite Peak intra-oceanic arc on to YTT
691
probably occurred during or soon after these events, whilst they were young (<10 M.yr.) and hot (e.g.
692
Dewey, 2003). The period between 265 and 260 Ma marks the starting point for these events, triggered by
693
the cessation of subduction of YTT (Figure 10), but we note that the relative timing and duration of slab
694
break-off and subduction polarity reversal is poorly constrained and may have taken longer than five million
695
years (e.g. Brown et al., 2011). The latest occurrence of metamorphism of YTT coeval with exhumation and
696
Klondike magmatism marks the final stage of the Klondike orogeny. Thus, we bracket the duration of
697
Klondike orogeny between ~275 and ~252 Ma (Figure 10). This outlined sequence of events is comparable
698
to the evolution of other ancient arc-continent collisions, such as the Grampian, Taconic and Kamchatka arc-
699
continent orogens (e.g. Dewey, 2005; Boutelier & Chemenda, 2011; Brown et al., 2011 and references
700
therein). We also note that the duration of the Klondike orogeny (~20-25 M.yr) is comparable to the
701
duration of other arc-continent collisions (~20-50 M.yr.), as opposed to the longer duration of continent-
702
continent collisions (≥50 M.yr.), which would be expected for a collision between YTT and Laurentia (e.g.
703
Friedrich et al., 1999; Dewey, 2005; van Staal et al., 2007; Chew et al., 2010; Brown et al., 2011).
704
9. REMAINING PROBLEMS AND FUTURE WORK
29
705
9.1. Accretion of the Klondike orogen to Laurentia
706
Our study argues that YTT did not collide with Laurentia during the Permian. Previous studies proposed that
707
deposition of the Jones Lake Formation on YTT, Laurentia and SMT marked the final stages of collision,
708
accretion and related subsidence between YTT and Laurentia, following their collision in the Permian
709
(Colpron et al., 2006; 2007; Beranek & Mortensen, 2011). However, close inspection of variations in detrital
710
zircon populations and conodont fauna within the Jones Lake Formation (see Section 2.1 for a review of this
711
data) indicate that these data are at best, consistent with a post-Middle Triassic collision but do not validate,
712
and in some cases are inconsistent with a model of deposition in a regional Triassic basin overlapping YTT,
713
SMT and Laurentia following Permian collision (e.g. Colrpon et al., 2007; Beranek et al., 2010; Beranek &
714
Mortensen, 2011). We also note that the widespread Late Triassic to Middle Jurassic plutons and Permian
715
and Jurassic high-grade metamorphism recorded within YTT are absent from Laurentia in Yukon (e.g.
716
Berman et al., 2007; Staples et al., 2014; Colpron et al., 2016b).
717
The present day lithospheric structure of the Northern Cordillera suggests that YTT forms an overriding
718
thrust sheet emplaced on top of Laurentia (e.g. Gordey, 2002; Cook et al., 2004; Calvert et al., 2017). To
719
satisfy this constraint, we suggest that after the Klondike orogeny, oceanic lithosphere that lay between
720
Laurentia and the Dunite Peak intra-oceanic arc was subducted westward beneath the Klondike orogen
721
(Figure 9d). We propose that the Jones Lake Formation represents accreted remnant ocean plate stratigraphy
722
(magenta accretionary complex, Figure 9c-d) and/or forearc/passive margin basin sediments (e.g. Gordey,
723
2013) deposited in the basin between the Klondike orogen and Laurentia (e.g. Ingersole, 1988; Ingersole et
724
al., 2003), which closed sometime after the Middle Triassic (e.g. Hansen et al., 1991; Stevens et al., 1996;
725
Plint & Gordon, 1997; Hansen and Dusel-Bacon 1998; Gordey, 2002, 2013). This is consistent with the
726
occurrence of unimodal/bimodal Permian-Triassic ± Devonian – Early Mississippian detrital zircon
727
populations (Beranek & Mortensen, 2011) and “exotic” Tethyan conodont species (Orchard, 2006) in
728
Middle to Late Triassic strata that overlie parts of SMT Yukon and northern British Columbia. Additionally,
729
paleomagnetic analysis of red chert units of SMT (Richards et al., 1993), suggested that parts of SMT
730
remained allochthonous with respect to Laurentia until the Early Jurassic (see Section 2.1.). We propose that
30
731
these red chert units derived from the basin between the Dunite Peak intra-oceanic arc and the Laurentian
732
margin.
733
The exact timing of collision between Laurentia and the Klondike orogen is unclear. Early Jurassic
734
amphibolite facies metamorphism followed by Early to Middle Jurassic exhumation recorded within YTT in
735
Canada and eastern Alaska may record collision between Laurentia and the Klondike orogen and its
736
subsequent collapse (e.g. Dusel-Bacon et al., 2002; Berman et al., 2007; Joyce et al., 2015; Morneau, 2017;
737
Morneau et al., 2017). However, Jurassic metamorphism and exhumation within YTT have also been
738
interpreted as a record of collision and accretion between YTT and Stikinia-Quesnellia (e.g. Colpron et al.,
739
2015; Clark, 2017). Collision between YTT-Stikinia and the Insular terranes (Alexander-Wrangellia, Figure
740
1) is hypothesized during the Early to Middle Jurassic (Monger, 2014) or the Late Jurassic to Cretaceous
741
(Sigloch & Mihalynuk, 2017). The timing of collision and accretion and the polarity of subduction zones
742
responsible for accretion between the Intermontane terranes (YTT-Stikinia-Quesnellia), the Insular terranes
743
and Laurentia is still debated (e.g. Johnston, 2008; Hildebrand, 2009; Monger, 2014; Sigloch & Mihalynuk,
744
2017).
745
The distribution of Early Cretaceous plutonic suites emplaced within both YTT and Laurentia (e.g. Colpron
746
et al., 2016b) provides a latest constraint on this collision and accretion, suggesting that YTT had accreted to
747
Laurentia by ~120 Ma. Emplacement of Early Cretaceous plutons into YTT and Laurentia (e.g. Colpron et
748
al., 2016b) was contemporaneous with amphibolite facies metamorphism of the underlying Laurentian
749
margin (e.g. Gibson et al., 2008; Moynihan, 2013; Staples et al., 2016; Ryan et al., 2017). This has led some
750
authors to propose that the allochthonous terranes first accreted with each other before accreting to Laurentia
751
sometime during the Cretaceous (e.g. Johnston, 2008; Hildebrand, 2009).
752
Integration of our study with existing datasets indicates that that collision and accretion between the
753
Klondike orogen and Laurentia occurred after the Middle Triassic (e.g. Hansen et al., 1991; Richards et al.,
754
1993; Stevens et al., 1996; Plint & Gordon, 1997; Hansen and Dusel-Bacon 1998; Gordey, 2002, 2013), and
755
perhaps as late as post-Jurassic (e.g. Johnston, 2008; Hildebrand, 2009). However, the variability of timing
756
estimates and subduction zone polarity models hypothesized by previous studies (described above),
31
757
demonstrates that the timing, order and sequence of collisions between the allochthonous terranes and
758
Laurentia that occurred after the Klondike orogeny requires further investigation. The disruption and/or
759
displacement of original emplacement structures associated with the Permian subduction zone beneath the
760
Dunite Peak intra-oceanic arc occurred during one or more of the subsequent collisional events listed above.
761
9.2. Re-assessment of the Slide Mountain terrane
762
Within our model we make a clear argument that the DPO and other correlative SSZ ophiolites derive from
763
the upper plate of the Dunite Peak intra-oceanic arc. Less certain, is the identification of ocean plate
764
stratigraphy (OPS) derived from the lower plate that subducted beneath this intra-oceanic arc or from the
765
basin between the Dunite Peak intra-oceanic arc and Laurentia. We suggest that early Permian and older
766
occurrences of SMT may represent accreted remnants of OPS from the subducting oceanic plate that was
767
attached to the east continental margin of YTT. These comprise supracrustal sections of basinal sedimentary
768
rocks and associated mafic volcanics with mid-ocean ridge and/or within-plate geochemical signatures, such
769
as parts of the Campbell Range basalts in the Finlayson Lake district (Figure 1c, Murphy et al., 2006; Piercy
770
et al., 2012). As our model predicts that the basin between the Dunite Peak intra-oceanic arc and Laurentia
771
closed following the Klondike orogeny, OPS attached to the passive margin of Laurentia should be capped
772
by Triassic and younger sediments that are possibly represented by the Jones Lake Formation (see Section
773
9.1.).
774
Our model also predicts structural separation between remnants of mid-Permian SSZ ophiolites,
775
Mississippian to Permian OPS attached to YTT, and Mississippian to Triassic or younger OPS from the
776
basin between the Dunite Peak intra-oceanic arc and Laurentia. In our study area, the single outcrop of
777
pillow basalt from the marine metasedimentary succession with an E-MORB geochemical signature (Group
778
4) may be one such example of this lower-plate accreted OPS. Elsewhere, a possible example of structurally
779
distinct elements of SMT is presented in the Finlayson Lake district (Figure 1c) where SMT containing N-
780
MORB, and BABB geochemical signatures appears to be structurally separated from SMT containing N-
781
MORB, E-MORB and OIB (Murphy et al., 2006, their Figure 16).
32
782
As our study is the first to predict these structurally distinct elements of OPS within SMT, it is difficult to
783
identify these elements of SMT from previous work without reliable age and geochemical constraints.
784
Furthermore, it is likely that subsequent deformation during the Jurassic and Cretaceous (e.g. Staples et al.,
785
2016) overprinted or removed original emplacement-related structural relationships. Further work should be
786
conducted to robustly identify and distinguish between our three predicted elements of SMT. Based on their
787
distinct age, lithology and structural separation from other parts of SMT, we suggest that all upper-plate
788
assemblages associated with the Dunite Peak intra-oceanic arc be recognized as a distinct terrane (e.g.
789
Coney et al., 1981; Ryan et al., 2015).
790
9.3. Spatial and temporal extent of the Dunite Peak intra-oceanic arc
791
We encourage further work to investigate its spatial and temporal extent of the Dunite Peak intra-oceanic
792
arc. Our model requires that following the Klondike orogeny, westward subduction of the ocean basin
793
between the Klondike orogen and Laurentia occurred so that they could collide sometime after the Middle
794
Triassic (see Section 9.1.). A potential caveat of this hypothesis is the relatively low abundance of Triassic
795
arc-magmatic rocks within YTT (e.g., the Stikine suite, Colpron et al., 2016b). Although we can only
796
speculate, a potential solution is that the magmatic response to westward-subduction of the ocean basin
797
between the Klondike orogen and Laurentia may be recorded by the Triassic Quesnel intra-oceanic arc (see
798
review of Nelson et al., 2013). This would imply that the Quesnel intra-oceanic arc formed on or close to the
799
eastern margin of the Klondike orogen, as a successor arc to the Dunite Peak intra-oceanic arc. Other
800
potentially misidentified correlatives of the Dunite Peak intra-oceanic arc may include greenstone from the
801
Klinkit intra-oceanic arc, which is currently considered part of YTT (e.g. Colpron et al., 2006; Nelson et al.,
802
2013), and yet yielded a U-Pb igneous age of 281 ± 2 Ma and juvenile (ƐNd = +6.7 to +7.4) IAT geochemical
803
signatures (Roots et al., 2002; Simard et al., 2002). Similarly, recent study of the Permian Nahlin ophiolite,
804
currently assigned to the Cache Creek terrane, also calls for the presence of a previously unrecognized
805
Permian-Triassic intra-oceanic arc that is allochthonous to the intermontane terranes (McGoldrick et al.,
806
2017). Based on our recognition of the Dunite Peak intra-oceanic arc and its similarity with other intra-
807
oceanic arcs in the Northern Cordillera, plus our prediction of two structurally confined OPSs within SMT
33
808
that are distinct from each other and the Dunite Peak intra-oceanic arc, we suggest that the current
809
tectonostratigraphic framework of terranes and assemblages in the Northern Cordillera be re-evaluated.
810
10. CONCLUSIONS
811
This study demonstrates the importance of identifying and distinguishing between upper-plate and lower-
812
plate components when attempting to understand the tectonic evolution of an accretionary orogen. We have
813
applied this concept to our study of the Dunite Peak ophiolite in south-central Yukon and other previously
814
studied mid-Permian ophiolites in Alaska, Yukon and British Columbia. Our findings indicate that a new
815
explanation is required for the late Paleozoic to early Mesozoic tectonic interaction between of the Yukon-
816
Tanana terrane, Slide Mountain terrane and Laurentian margin of the Northern Cordillera.
817
The Dunite Peak ophiolite (DPO) forms klippen of mafic-ultramafic strata structurally emplaced over
818
metasedimentary rocks of Yukon-Tanana terrane (YTT). Field structural, geochemical and geochronological
819
analyses conducted on the DPO and underlying metasedimentary strata yield the following conclusions:
820
1) Whole-rock geochemical and Sm-Nd isotopic analyses of mafic-ultramafic assemblages from the
821
DPO identify 5 distinct geochemical groups. Groups 1-3 correspond to arc (Groups 1-2 = IAT to CA) and
822
back-arc (Group 3 = BABB) magmatic components of a SSZ ophiolite formed in the upper plate of an intra-
823
oceanic arc (ƐNd = +7.2 to +9.0). Group 5 corresponds to highly depleted mantle/lower crustal ultramafic
824
cumulates, formed in a SSZ setting. The geochemical signatures from these groups are comparable to those
825
derived from modern day intra-oceanic arcs, such as the Izu-Bonin, Mariana and Kermadec arcs and Lau
826
basin, in the SW Pacific Ocean. Group 4 corresponds to E-MORB pillow basalt with no record of interaction
827
with a subduction zone and may therefore by tectonically unrelated to the DPO.
828
829
2) U-Pb zircon geochronology of an IAT gabbro from the DPO yielded a mean igneous crystallization
age of 265 ± 4 Ma.
830
3) Geochemical and geochronological constraints correlate the DPO with other mid-Permian (275-260
831
Ma) ophiolites previously assigned to Slide Mountain terrane (SMT). These correlatives include Quartzrock
832
Creek gabbro, Cassiar block, Zus Mountain block and Blue Mountain block (northern British Columbia,
833
Sylvester allochthon), St Cyr klippe and Tower Peak assemblage and the Finlayson Lake greenstones and
34
834
gabbros (south-central Yukon), Tummel fault zone and Ragged Lake klippe (central Yukon), Clinton Creek
835
ophiolite (west Yukon) and the Wolf Mountain klippe (east Alaska) (Figure 1). Together, these ophiolites
836
represent the dismembered upper-plate remnants of a regionally extensive intra-oceanic arc active between
837
YTT and Laurentia during the mid-Permian (~280-260 Ma). We name this arc the Dunite Peak intra-
838
oceanic arc.
839
4) We propose that the Klondike orogeny records deformation, metamorphism and magmatism
840
associated with mid-Permian eastward subduction and collision of YTT beneath the Dunite Peak intra-
841
oceanic arc. Subduction of YTT and associated intra-oceanic arc magmatism terminated at ~265-260 Ma.
842
This was accompanied/followed by slab break-off, orogenic collapse and associated magmatism, and the
843
initiation of westward subduction (present coordinates) beneath the east margin of the Klondike orogen
844
(composite of YTT and the Dunite Peak intra-oceanic arc) between ~265 and ~252 Ma. During this time,
845
the Klondike magmatic cycle occurred in response to either: (1) exhumation-driven crustal melting; (2)
846
newly initiated westward subduction; or (3) a combination (1) and (2).
847
5) Accretion of the Klondike orogen with Laurentia occurred after the Permian, and probably after the
848
Middle Triassic. This is supported by reassessment of detrital zircon populations and conodont fauna with
849
Triassic sedimentary rocks on YTT, SMT and Laurentia, and the distribution of Triassic to Early Jurassic
850
metamorphism, magmatism and exhumation within YTT that is not record by Laurentia.
851
6) Mid-Permian SSZ ophiolites of the Dunite Peak intra-oceanic arc are distinct from older supracrustal
852
sections of SMT that formed in an intra-plate/mid-ocean spreading ridge setting. The definition of SMT
853
should be modified to formally recognize the distinction between mid-Permian SSZ ophiolites from older
854
SMT sections. Other parts of SMT may be subdivided into accreted ocean plate stratigraphy derived from
855
(1) the oceanic lower plate attached to YTT that subducted beneath the Dunite Peak intra-oceanic arc and (2)
856
the ocean basin which formed between the Dunite peak intra-oceanic arc and Laurentia. The latter should
857
contain younger strata (post-Permian) than the former. This younger lower plate material from the basin
858
between the Dunite Peak intra-oceanic arc and Laurentia may include the Triassic Jones Lake Formation.
859
The Dunite Peak intra-oceanic arc should be recognized as a distinct terrane and that the current
35
860
tectonostratigraphic framework of terranes and assemblages in the Northern Cordillera should be re-
861
evaluated.
862
Acknowledgements
863
This research was has received funding from the Geological Survey of Canada, GEM-II Cordillera project and the
864
European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme
865
(grant agreement 639003 “DEEP TIME”). We thank Brad Singer (science editor), John Waldron (ass. editor), John
866
Wakabayashi, Cynthia Dusel-Bacon and Steve Johnston for constructive reviews. JoAnne Nelson (BCGS) is thanked
867
for helpful discussion during initial write-up. Dejan Milidragovic (BCGS) is thanked for guidance during initial
868
interpretations of geochemical data. We thank Shuangquan Zhang (Carlton University) for the Sm-Nd isotopic
869
analyses presented in this study. We thank Capital Helicopters Inc. and the Yukon Geological Survey for logistical
870
support during fieldwork.
871
872
36
873
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Figure 1. Terrane map of the Northern Cordillera. Modified from Colpron et al. (2007). Study area (Dunite Peak
326
ophiolite, DPO) outlined by black box (Figure 2). Inset map (bottom right corner) shows location of Figure 1 with
327
respect to North America. Geochronology localities discussed in this article and synthesized into our new hypothesis
328
are labelled with letters (a) to (o). Age ranges are given for localities with multiple geochronology analyses and
329
correspond to the oldest age plus error and the youngest minus error. Klondike magmatic assemblage (Ass) and
330
correlative units drawn from Cui et al. (2015) and Colpron et al. (2016a). (a-o) Superscript numbers next to ages
331
correspond to geochronology data sources (discussed in text): (1) Gabrielse et al., 1993, (2) Erdmer et al., 1998, (3)
332
Murphy et al. 2006, (4) Mortensen, 1992b, (5) Fallas et al., 1998, (6) Petrie et al., 2015, (7) Petrie et al., 2016, (8)
333
Gilotti et al., 2017, (9) de Keijzer et al., 2000, (10) Creaser et al., 1997, (11) Erdmer & Armstrong, 1988, (12)
334
Godwin-Bell, 1998, (13) Philippot et al. 2001, (14) Colpron et al., 2005, (15) Oliver, 1996, (16) Joyce et al., 2015,
335
(17) Johnston et al., 2007, (18) Colpron et al., 2006b, (19) Breitsprecher & Mortensen 2004, (20) Staples, 2014, (21)
336
Berman et al., 2007, (22) Htoon, 1981.
337
Figure 2. Geological map of the Dunite Peak ophiolite (DPO) with locations of geochronology and geochemistry
338
samples and Figure 3 photo locations. Geochemistry symbols correspond to geochemical groups in Figures 6-7.
339
Figure 3. (a-b) Photographs of the eastern klippe of the Dunite Peak ophiolite (DPO) with unit boundaries overlain.
340
See Figure 2 and text for map unit descriptions. See Figure 2 for photo locations.
341
Figure 4. Field images of the Dunite Peak ophiolite (DPO) crustal section. (a) Greenstone volcaniclastic rocks (Group
342
1 geochemistry) with subordinate chert horizons, lower DPO crustal section. (b) Sheared pillow basalt and greenstone
343
(Group 1a geochemistry) with subordinate sedimentary layers, lower DPO crustal section. (c) Typical lithological
344
representation of volcanic/volcaniclastic greenstone. (d) Typical lithological representation of gabbro (Group 2
345
geochemistry, upper DPO crustal section). (e) Gabbro (Group 2 geochemistry) intruding fragmental volcaniclastic
346
greenstone, upper DPO crustal section. (f) Gabbro (Group 2 geochemistry) intruding greenstone (Group 1
347
geochemistry), upper DPO crustal section.
348
Figure 5. U-Pb geochronology, sample16RAY-AP074A1 (a) Representative cathodoluminescence (CL) images of
349
zircon grains analyzed and (b) Tera–Wasserburg and (c) chondrite-normalized rare earth element plots of sensitive
350
high-resolution ion microprobe reverse-geometry (SHRIMP-RG) U/Pb and trace element data from sample 16RAY-
351
AP074A1. U/Pb data plotted as 1σ error ellipses uncorrected for common Pb. Black ellipses are used in calculating
352
concordia ages. Weighted mean age uncertainty is reported at the 95% confidence level.
53
353
Figure 6. Rare earth element – high field strength element (REE-HFSE) spider diagrams. (a-c) Groups 1-4 normalized
354
against N-MORB (Sun & McDonough, 1989). N-MORB V and Sc concentrations based on Klein (2004). (d) Group 5
355
normalized against primitive mantle (Sun & McDonough, 1989). Primitive mantle V and Sc concentrations based on
356
McDonough and Frey (1989). Standard REE-HFSE profiles for depleted-MORB mantle (DMM) are displayed for
357
comparison (Salters & Stracke, 2004; Workman & Hart 2005).
1358
Figure 7. Geochemical-tectonomorphic discrimination diagrams. (a) Nb/Y (total alkalinity proxy) vs. Zr/Ti (SiO2
359
proxy), based on Pearce (1996). (b) Y-La-Nb ternary discrimination diagram based on Cabanis & Lecolle (1989). (c)
360
Suprasubduction/spreading ridge/within-plate magmatism discrimination diagram (Nb/Yb vs. Th/Yb) based on Pearce
1361
(2008, 2014). Black squares show typical values for the magma types indicated by adjacent labels. Vertical arrows
1362
represent subduction zone enrichment. (d) Geochemical classification of Group 5 ultramafic samples, based on CIPW
1363
normative major element concentrations.
364
Figure 8. Geochemical signatures of basalt, basaltic andesite and andesite samples collected from active intra-
1365
oceanic arcs in the SW Pacific Ocean compared with data collected from the Dunite Peak ophiolite. (a-f) Volcanic
1366
glass and whole rock rare earth element – high field strength element (REE-HFSE) concentrations from the Izu-Bonin
1367
arc (red shaded area – e.g. Tollstrup et al., 2010; Ishizuka et al., 2014), Mariana arc (orange shaded area – e.g.
1368
Pearce et al., 2005; Tamura et al., 2014), Kermadec arc (blue shaded area – e.g. Wysoczanski et al., 2006;
1369
Smith et al., 2009) and Lau Basin (green shaded area – e.g. Keller et al., 2008; Bézos et al., 2009), drawn from
1370
datasets of n samples. Data are split into arc samples (a-c) and back-arc/trough/ridge samples (d-e). Note that only
1371
data collected from back-arc/trough/ridge settings are available from the Lau Basin (green shaded area). Geochemical
1372
data from the Dunite Peak ophiolite are delineated with black to grey lined, unshaded areas (g-i) and overlain on SW
1373
Pacific data sets for comparison (a-f). Spider diagrams are normalized against N-MORB (Sun & McDonough, 1989).
1374
N-MORB V and Sc concentrations based on Klein (2004). Explanation and abbreviations for geochemical-
1375
tectonomorphic discrimination diagrams (b-c), (e-f), and (h-i) are same as in Figure 7b-c. Data complied and extracted
1376
from GEOROC database (Sarbas & Nohl, 2008). Full dataset and sources (total of 57 sources) are presented in
1377
Supplementary Materials 04.
1378
Figure 9. Cartoon summary of our new model for the Paleozoic–Mesozoic tectonic evolution of the Northern
1379
Cordillera, see text for discussion. Yukon-Tanana terrane crust – dark green; YTT eclogite – purple; Laurentian crust
1380
– blue: Laurentian margin accretionary complex – magenta; Dunite Peak intra-oceanic arc crust – light grey; Dunite
54
1381
Peak arc accretionary complex – dark blue; oceanic crust – dark grey; lithospheric mantle – light green; volcanic
1382
centres – orange triangles. Not drawn to scale.
1383
Figure 10. Synthesis of isotope geochronology data from Yukon-Tanana terrane (YTT) and the Dunite Peak intra-
1384
oceanic arc. Sample numbers (x-axis) correspond to published geochronology data entries in Supplementary Materials
1385
05. Time scale (y-axis) based on Geological Society of America timescale. Data points are divided into specific
1386
tectonic processes, labeled in top header, with a color bar to highlight period of activity (e.g. duration of Dunite Peak
1387
intra-oceanic arc magmatism indicated by orange bar). Tectonic interpretations of data summarized on right panel.
1388
Hatched zone at 265-260 Ma corresponds to cessation of subduction and collision of YTT with the Dunite Peak intra-
1389
oceanic arc and the initiation of slab break-off, subduction polarity reversal and associated magmatism. Hatched zone
1390
at post-220 Ma marks possible timing of collision and accretion between YTT and Laurentia. See text for discussion.
Figure 1
140°W
21
0
(l) 264 ± 3 Ma 20
255 ± 3 Ma 20
239 ± 3 Ma 20
AL
AS
KA
(n) 239 ± 7 Ma
KS
NORTHW EST
TERRITORIES
(k) 217 ± 1 Ma19
(j) 260 ± 1 Ma18
(h) 270-245 Ma 13
SM
WR
CG
NAb
(g) 255 ± 8 Ma12
AX
Cordilleran Terranes
Outboard
YT
(b) 207 ± 1 Ma2
Geochronology Localities
(a) Zus Mountain, Blue Dome
(Sylvester allocthon)*
(b) Klatsa
(c) Finlayson Lake*
(d) St Cyr / Quiet Lake*
(e) Dunite Peak*
(f) Last Peak
(g) Ross River
(h) Faro
(i) Tummel fault zone*
(j) Ragged Lake klippe*
(k) Little Kalzas Lake
(l) McQuesten
(m) Buffalo Pitts
(n) Stewart River
(o) Clinton Creek /
Eagle Quadrangle*
* Denotes mid-Permian supra-
NAc
(a) 269 ± 7 Ma1
CC
CG
CA
Ancestral N America
CA - Cassiar
NAb - NA basinal
NAp - NA platform
NAc - NA craton & cover
62°N
subduction zone ophiolite locality
Y U KO
N TE R
R ITOR
B RIT
Y
IS H C
O LU M B
IA
WR - Wrangellia
AX - Alexander
KS - Kluane,Windy,Coast
CC - Cache Creek
ST - Stikinia
QN - Quesnellia
YT - Yukon-Tanana
SM - Slide Mountain
Klondike Ass (YT)
(c) 273 ± 1 Ma3
CA
YT
200
CC
Insular
Intermontane
(c) 274 ± 0.5 Ma4
DPO
(Fig. 2)
(d) 275-261 Ma 5,6,7,8
(d) 265-223 Ma 5
YA - Yakutat
CG - Chugach
58°N
(g) 275-237 Ma2,11
(f) 269 ± 2 Ma 10
(f) 267 ± 7 Ma 2
KS
(e) 267 ± 10 Ma 9
WR
YA
(h) 263-257 Ma 2
(i) 215 ± 4 Ma 16
YT
ST
WR
NAp
(i) 243-208 Ma 15
(i) 268 ± 2 Ma14
(m) ~262 Ma 17
100
km
NAp
(n) ~260 Ma 21
62°N
124°W
(o) 245 ± 8 Ma 22
YT
NAb
132°W
NAp
CG
AX
YT
NAc
ST
Slide Mountain Terrane - U/Pb age
Buffalo Pitts peridotite - U/Pb age
Figure 1
Permian Yukon-Tanana terrane eclogite facies metamorphism - U/Pb & Sm/Nd age
Permian-Triassic Yukon-Tanana terrane amphibolite facies metamorphism - U/Pb age
KS& Ar/Ar age
Exhumation of Yukon-Tanana terrane eclogite/blueschist - K/Ar
QN
Exhumation of Yukon-Tanana terrane (other than eclogite/blueschist)- K/Ar & Ar/Ar age
(a) Letters corresponds to geochronology locality
1 Superscript numbers correspond to data source (see figure caption)
132°W
124°W
58°N
134.04° W
134° W
MMS3
133.96° W
1700
Locality
U-Pb zircon age
61.66° N
Field station
140
0
DPc
1800
00
Group 5 (Pyrxnt.)
2
0
1600
3
4
Kilometers
00
BM
15
00
00
1800
14
1500
1300
1700
0
14
1500
1
N
170
00
1700
1700
00
13
00
16
MMS4
00
Group 5 (Lherz.)
18
00
MMS3
Group 5 (Dun./Harz.)
Group 2 (IAT, plutonic)
0
0.5
16
13
Group 4 (E-MORB)
Group 1b (IAT-CA)
Group 3 (BABB)
130
00
MMS3
Group 1a (IAT/IAT-CA)
180
1500
0
14
DPu
61.64° N
Superscript number refers
to data source:
1 - This study
2 - De Keijzer et al. 2000
15
MMS3
133.88° W
Geochemical Samples (Figs. 6 & 7)
265 ± 4 Ma1
Figure photo,
with viewing
direction
133.92° W
1800
61.66° N
134.08° W
BM
265 ± 4 Ma1
MMS2
61.64° N
134.12° W
18
00
134.16° W
Figure
2
1700
BM
140
0
FAULT SYST
MMS3
00
1300
14
00
MMS2
DPc
MMS1
MMS3
DPc
MMS3
DPu1
0
18
00
1400
18
170
00
0
0
DPc
MMS3
1900
0
1000
DPu2
0
19
Fig. 3b
0
DPu2
19
00
1800
1900
0
180
MMS3
BM
2000
DPu2
MMS3
DPc
DUNITE
PEAK
DPu2
DPu
DPc
267 ± 10 Ma2
DPc
MMS2
MMS1
00
16
DPc
MMS2
0
MMS1
12
1300
00
BM
0
90
Marine metasedimentary succession
DPu1 - Serpentinite, sheared and imbricated
00
14
0
MMS2 - White quartzite, interbedded
quartzite & marble,
subordinate carbonaceous calc-silicate layers
MMS1
MMS1 - Micaceous/carbonaceous quartzite and
carbonaceous shale 1100
1200
MMS2
10
Axial trace, synform
0
DPc
1400
DPc - Volcanic/volcaniclastic greenstone, subordinate
shale, chert (lower portion), hypabyssal greenstone, gabbro,
leucogabbro, sheared and imbricated
134.08° W
134.04° W
Basal marble
BM - Marble, subordinate siliciclastics, pelite, mafic
CB
13
intrusions, garnet-epidote-amphibolite
facies
00
134° W
Normal fault, observed
Normal fault, constrained
Normal fault, inferred
133.96° W
Geographic Symbols
1400
1100
Dunite Peak
1500
0
Crustal Ultramafic section
section
DPu1
MMS3 - Carbonaceous shale/semipelite, subordinate
chert, greenstone
0
10
61.56° N
DPu2
DPu2 - Dunite, harzburgite,subordinate
lherzolite, variably serpentinized
MMS3
Strike-slip fault, observed
Strike-slip fault, constrained
00
Strike-slip13 fault, inferred
Contact, observed
Contact, inferred
Contact, constrained
0
134.12° W
DPu3 - Gabbro/pyroxenite dike/sill
MMS4 - Marble/limestone, fossiliferous, mylonitized
120
K
DPu3
1100
Dunite Peak ophiolite (DPO)
BM
Geologic Boundaires
MMS4
0
Cretaceous Granite - Biotite granite
(Last Peak Granite, 95.7 ± 0.6 Ma, Gallagher, 1999)
00
15
K
120
0
80
Geologic Map Units
61.58° N
900
61.58° N
0
MMS3
0
17
MMS3
130
110
0
00
Fig. 3a
MMS3
DPu
10
61.6° N
170
0
DPu2
0
18
61.6° N
18
00
1900
DPc
MMS3
Contour interval - 100 m
1500
Thrust fault, observed
Thrust fault, constrained
Thrust faiult, inferred
River or stream
133.92° W
133.88° W
Waterbody
61.56° N
D’ABBADIE
00
16
DPu2
DPc
DPu
1800
DPu2
1400
1500
DPu1
61.62° N
170
0
11
61.62° N
MMS3
12
MMS3
1500
EM
DPc
Figure
(a) 3
Looking NW
Dunite Peak
(2020 m)
DP
u1
DPu2
DPc
MMS3
MMS2
MMS1
(b)
DP
Dunite Peak
(2020 m)
Looking W
DPu3
u1
DPu2
DPc
DPu2
Figure 4
(a)
Sedimentary layer
Greenstone - volcaniclastic
(b)
Greenstone
Chert
Sheared pillows
Greenstone - volcaniclastic
Sheared pillows
Sheared pillows
Chert
Sheared pillows
Greenstone - volcaniclastic
Greenstone
5 cm
20 cm
(c)
(d)
astic
anicl
lc
al vo
Gree
nst
one -
ent
fragm
(e)
(f)
act
sive
t
con
u
Intr
Greenstone
Intrusive contact
Gabbro
5 cm
Gabbro
5 cm
Figure 5
a.
b.
0.064
265 ± 4 Ma
(MSWD= 0.9)
2.1
207
1.1
Pb/ 206 Pb
2.1
300
280
0.048
21
5.1
4.1
240
260
238
U/ 206 Pb
26
10.1
9.1
zircon/chondrite
c.
10
3
10
2
10
1
10
0
10
-1
-2
10
100 µm
La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu
100
Figure
6
100
(a) Group 1
Group 1:
Greenstone + gabbro,
Dunite Peak ophiolite
crustal section
10
Group 2: layered gabbro +
leucogabbro + subordinate
greenstone, Dunite Peak
ophiolite crustal section
Group 3: gabbro intrusions
from the ultramafic section
+ greenstone from the crustal
section, Dunite Peak ophiolite
Rock/N-MORB
Rock/N-MORB
10
(b) Groups 2 & 3
1
1
.1
.1
Group 1a (n = 9)
Group 1b (n = 9)
.01
Nb
Th
Ce
La
Sm
Nd
Hf
Zr
εNd = +7.2 to +7.5
Ti
Eu
Dy
Gd
Er
Y
Lu
Yb
Sc
εNd = +8.1 to +9.0
Group 2 (n = 11)
Group 3 (n = 6)
.01
V
Nb
Th
Ce
La
Sm
Nd
Hf
Zr
Ti
Eu
Dy
Gd
Er
Y
Lu
Yb
Sc
V
100
100
Group 4:
Pillow basalt, Marine
metasedimentary
succession (MMS3)
(c) Group 4
(d) Group 5
Dunite Peak ophiolite ultramafic rocks
Dunite/Harzburgite (n = 10)
Lherzolite (n = 3)
Pyroxenite (n = 1)
DMM standard composition
10
Rock/N-MORB
Rock/Primitive Mantle
10
1
1
.1
.1
Group 4 (n = 1)
.01
Nb
Th
Ce
La
Sm
Nd
Hf
Zr
Ti
Eu
Dy
Gd
Er
Y
Lu
Yb
Sc
V
.01
Nb
Th
Ce
La
Sm
Nd
Hf
Zr
Ti
Eu
Dy
Gd
Er
Y
Lu
Yb
Figure
(a) 7
(b)
Y/15
alk. rhyolite
1
IAT
rhyolite +
dacite
IAT-CA
tephriphonolite
trachyandesite + andes.
Zr/Ti
Group 1a (n = 9)
Group 1b (n = 9)
trach.
.1
N-MORB
phonolite
* BABB
*
Group 2 (n = 11)
E-MORB
Group 3 (n = 6)
basaltic
andesite
Calc-alkali
basalt
1
Nb/Y
10
100
Nb/8
Ol
(d)
(c)
Alkaline
Intercontinental
rifts
La/10
Dunite
SS
OIB
1
ite
hrl
We
Ha
rz b
urg
ite
Z
10
.1
Group 5
foidite
alk.
bas.
.01
Continental.
.01
Group 4 (n = 1)
Th/Yb
Lherzolite
E-MORB
PERIDOTITE
PYROXENITE
Ol-Websterite
N-MORB
SS
Z
.1
.01
.1
1
Nb/Yb
10
100
Opx Ortho-
pyroxenite
Websterite
Clino- Cpx
pyroxenite
Dunite/Harzburgite (n = 12)
Lherzolite (n = 3)
Pyroxenite (n = 1)
Izu-Bonin arc
Mariana arc
Kermadec arc
Lau basin
n (a-c) = 566
n (d-f) = 43
n (a-c) = 131
n (d-f) = 96
n (a-c) = 136
n (d-f) = 46
n (d-e) = 282
Y/15
10
(b)
Group 1 (IAT/CA)
(a)
(c)
IAT-CA
Th/Yb
1
*
SS
Z
.1
(d)
(e)
Z
SS
Th/Yb
*
E-MORB
SS
Z
.1
N-MORB
Calc-alkali
.01
10
La/10
Group 1 (IAT/CA)
(h)
Z
IAT-CA
Th/Yb
Rock/N-MORB
IAT
N-MORB
*
E-MORB
Th
Ce
La
Sm
Nd
Hf
Zr
Ti
Eu
Dy
Gd
Er
Y
Lu
Yb
Sc
V
Calc-alkali
.01
.1
1
Nb/Yb
10
100
La/10
Continental.
N-MORB
SS
Z
.1
Nb
* BABB
E-MORB
.1
.01
Nb/8
Y/15
OIB
1
1
Alkaline
Intercontinental
rifts
(i)
SS
Group 2 (IAT/CA cumulates)
Group 3 (BABB)
* BABB
E-MORB
.1
10
N-MORB
IAT
IAT-CA
(g)
Nb/8
Y/15
OIB
1
1
Alkaline
Intercontinental
rifts
(f)
Group 3 (BABB)
10
.01
100
Dunite Peak
ophiolite
Calc-alkali
La/10
Group 2 (IAT/CA cumulates)
Rock/N-MORB
Back-arc / Trough /
Ridge
N-MORB
.01
10
Group 1 (IAT/CA)
* BABB
E-MORB
E-MORB
.1
.01
100
N-MORB
OIB
1
Rock/N-MORB
Arc
10
IAT
SS
Z
Group 2 (IAT/CA cumulates)
Group 3 (BABB)
Continental.
100
Continental.
Figure 8
Alkaline
Intercontinental
rifts
Nb/8
(a) Mid
Figure
9 Permian (280-260 Ma)
Dunite Peak intra-oceanic arc
(light grey unit)
- Magmatism recorded by the Dunite
Peak intra-oceanic arc between ~275
Accretionary complex of
and 260 Ma and perhaps as early
lower plate material (blue)
as ~280 Ma
- Eclogite facies metamorphism of
Yukon-Tanana terrane recorded
Yukon-Tanana
between ~275 and 260 Ma
terrane
- Late Permian and older parts of Slide
Mountain terrane may represent accreted
lower plate material from the subducted
oceanic lithosphere (dark blue)
- Width of subducted ocean basin is unknown
- St Cyr blueschist may represent accretionary
complex of lower plate material (dark blue)
Extensional
zone
Volcanic
centers
Width of basin between Dunite Peak
intra-oceanic arc and Laurentian
margin is unknown
Laurentia
Generation of
surpasubduction
zone ophiolites
Eclogite facies metamorphism
of Yukon-Tanana continental
crust (purple)
Earliest record of eclogite facies metamorphism of Yukon-Tanana terrane marks start of the Klondike orogeny. Coeval Dunite Peak magmatism and eclogite facies
metamorphism of Yukon-Tanana terrane suggests Yukon-Tanana had an irregular shape with promontories and re-entrants and/or collided obliquely with the Dunite Peak
intra-oceanic arc. Co-spatial and coeval development of constructional volcanic centres (e.g. Dunite Peak, Wolf Mountain klippe) and zones of extensional volcanism
(e.g. Sylvester allochthon, Finlayson Lake district) is comparable to disorganized extensional intra-oceanic arcs such as the Kermedac arc - Havre trough system
(b) Mid/late Permian (265-260 Ma)
Orogenic collapse and associated magmatism
(Klondike magmatic cycle)
Suprasubduction zone ophiolites
obducted onto Yukon-Tanana
Width of basin between Dunite Peak
- Cessation of Dunite Peak magmatism
and subduction of Yukon-Tanana terrane
by 260 Ma
Yukon-Tanana
- Exhumation of Yukon-Tanana terrane
terrane
blueschists and eclogites initiated at 265 Ma
- Emplacement of Buffalo Pitts orogenic
peridotite within Yukon-Tanana
terrane at ~262 Ma
- Main phase of Klondike magmatic
cycle between 265 and 252 Ma
Extension of Yukon-Tanana terrane
accompanied by emplacement of the
Buffalo Pitts orogenic peridotite
intra-oceanic arc and Laurentian
margin is unknown
Laurentia
Slab
break-off
Initiation of westward subduction
of ocean between Klondike orogen
and North American cratonic margin.
Roll-back promotes extension.
Buoyancy-driven slab break-off from the east margin of Yukon-Tanana terrane was followed by extension, exhumation and
magmatism associated with orogenic collapse and initiation and roll-back of westward subduction beneath the Klondike orogen
(c) Late Permian (260-252 Ma)
Orogenic collapse and associated magmatism
(Klondike magmatic cycle)
- Continued exhumation of Yukon-Tanana terrane blueschists
and eclogites between 265 and 256 Ma
Yukon-Tanana
- Klondike magmatic cycle continued until 252 Ma
terrane
- Amphibolite facies metamorphism of Yukon-Tanana
terrane recorded between ~260 and 252 Ma
Exhumation of YTT eclogite & blueschist
Accretionary complex
of lower plate
material (magenta)
Laurentia
Latest occurrence of Klondike magmatism and metamorphism of Yukon-Tanana terrane coeval
with exhumation marks the final stages of the Klondike orogeny, which ended by ~252 Ma
(d) Post-Middle Triassic
Accretionary complex of lower plate material
may contain Triassic Jones Lake Fm. (magenta)
Yukon-Tanana
terrane
Laurentia
Westward subduction leads to collision
and accretion of Klondike orogen to Laurentia
- Collision and accretion of Klondike orogen to Laurentian margin facilitated by westward subduction of the ocean basin between the Klondike orogen and Laurentia
- Triassic clastic deposits of the Jones Lake Formation (magenta) may represent obducted lower plate sediments from the basin between the Klondike orogen and Laurentia
- Detrital zircons from the Jones Lake Formation suggest the Klondike orogen and Laurentian margin were in close proximity by the Late Triassic
- Late Triassic - Jurassic magmatism and Early Jurassic metamorphism recorded by Yukon-Tanana terrane are absent from Laurentia in Yukon
- Early Jurassic metamorphism and exhumation of Yukon-Tanana terrane records an Early Jurassic collisional event
- Early Cretaceous plutonic suites in Yukon-Tanana terrane and Laurentia indicate collision and accretion of Klondike orogen to Laurentian margin occurred by that time.
- Collision and accretion of Klondike orogen with Laurentian margin occurred after the Middle Triassic and by the Early Cretaceous
Eclogite facies
metamorphism
Sub-eclogite
facies metam.
Klondike magmatic cycle
YTT cooling/exhumation
Undeformed
by Permian
fabrics
Deformed by Permian fabrics
or no information given
YTT eclogite and blueschist facies crust
YTT crust
Buffalo
Pitts
orogenic
peridotite
209
210
LATE
NORIAN
TRIASSIC
228
Tectonic interpreation
See text for discussion
220-206 Ma
Metamorphism of YTT
Late Triassic Early Jurassic
RHAETIAN
Dunite Peak
intra-oceanic
arc
magmatism
Possible timing of
YTT-NAC Accretion
Figure 10
201
Exhumation of
YTT
220
CARNIAN
230
MIDDLE
LADINIAN
241
EARLY
247
250
240
ANISIAN
Exhumation
of YTT
eclogites
and blueschists
265-220 Ma
270-223 Ma
237
Exhumation of YTT
(other than
eclogites and
blueschists)
Buffalo Pitts
peridotite
emaplced
during
extension
of YTT
Orogenic
collapse
and
subduction
polarity
reversal
OLENEKIAN
250
INDUAN
252
269
WORDIAN
279
270
Dunite Peak
intra-oceanic
arc magmatism
Subduction
of YTT
continental
crust
KUNGURIAN
280
Cisuralian
272
PERMIAN
ROADIAN
265-260 Ma
265
275-260 Ma
Guadalupian
260
CAPITANIAN
~262 Ma
260
Klondike
magmatic
cycle
~280-260 Ma
WUCHIAPINGIAN
265-252 Ma
254
Klondike orogeny
(275-252 Ma)
Lopingian
CHANGHSINGIAN
Geochronology isotope
and mineral system
K-Ar Hornblende
U-Pb Zircon
ARTINSKIAN
290
290
SAKMARIAN
296
U-Pb Titanite
K-Ar Muscovite
U-Pb Monazite
K-Ar Biotite
Sm-Nd
Ar-Ar Hornblende
Rb-Sr
Ar-Ar Muscovite
Lu-Hf
Ar-Ar Biotite
Sample numbers correspond to geochronology sample
data entry presented in Supplementary Materials including
data source, sample description and analytical notes
ASSELIAN
299
10
20
30
40
50
60
SAMPLE NUMBER
70
80
90
100
110
Table 1
Sample
Group
Lithology
Map
Unit
LaN(1)
Mean
LaN(1)
YbN(1)
Mean
YbN(1)
[La/Yb]N(1)
Mean
[La/Yb]N(1)
[Th/Nb]N(1)
Mean
[Th/Nb]N(1)
[V/Ti]N(2,3)
Mean
[V/Ti]N(2,3)
Ɛ Nd(4)
17RAY-AP034A1
1a
Greenstone
DP1
0.81
1.08
0.33
0.37
2.44
2.87
11.65
14.67
2.21
2.38
17RAY-AP043B1
1a
Greenstone
DP1
0.64
0.20
3.27
1.99
15RAY-JR074A
1a
Greenstone
DP1
1.20
0.41
2.93
6.47
2.36
7.2
15RAY-JR076A
1a
Greenstone
DP1
0.88
0.32
2.71
9.71
2.65
16RAY-AP074A2
1a
Greenstone
DP1
1.28
0.47
2.73
14.56
2.06
7.4
16RAY-AP075A2
1a
Greenstone
DP1
0.92
0.38
2.42
2.36
2.86
7.5
16RAY-AP076B1
1a
Greenstone
DP1
2.05
0.50
4.06
21.03
2.30
16RAY-AP088A1
1a
Greenstone
DP1
0.94
0.32
2.91
36.89
2.73
16RAY-JR111A2
1a
Greenstone
DP1
0.98
0.41
2.38
2.26
17RAY-AP035A2
1b
Greenstone
DP1
4.32
4.21
0.99
0.90
4.38
4.68
17.93
27.95
0.54
0.93
17RAY-AP040A1
1b
Greenstone
DP1
4.12
0.90
4.60
15.78
0.61
16RAY-AP076A1
1b
Greenstone
DP1
4.00
0.73
5.50
19.00
1.15
16RAY-AP087B2
1b
Greenstone
DP1
4.64
0.98
4.72
7.66
0.84
7.4
16RAY-AP104A1
1b
Greenstone
DP1
4.04
0.83
4.87
15.05
1.03
16RAY-AP159A1
1b
Greenstone
DP1
5.20
1.04
5.00
20.10
0.65
16RAY-AP181A1
1b
Gabbro
DP1
4.20
1.07
3.94
114.56
0.98
16RAY-AP209A1
1b
Greenstone
DP1
2.50
0.60
4.20
20.63
1.43
16RAY-AP234A1
1b
Greenstone
DP1
4.84
0.98
4.94
20.87
1.11
17RAY-AP041A1
2
Greenstone
DP1
1.30
0.85
0.46
0.32
2.82
2.91
12.82
17.43
2.08
2.54
17RAY-AP043A1
2
Gabbro
DP1
0.67
0.27
2.53
8.74
2.83
17RAY-AP043C1
2
Gabbro
DP1
0.52
0.59
0.87
1.56
17RAY-AP044A1
2
Gabbro (cumulate)
DP1
2.50
0.30
8.27
5.11
2.82
16RAY-AP074A1
2
Gabbro
DP1
0.92
0.37
2.46
32.04
2.46
16RAY-AP078C1
2
Gabbro
DP1
0.89
0.15
5.79
33.66
4.22
16RAY-AP095A1
2
Gabbro
DP1
0.60
0.24
2.52
14.56
3.19
16RAY-AP120B1
2
Leucogabbro
DP1
0.22
0.20
1.12
1.85
16RAY-AP195A1
2
Gabbro
DP1
0.74
0.32
2.32
15.05
1.56
16RAY-AP202A1
2
Greenstone
DP1
0.64
0.47
1.37
17.48
2.08
16RAY-AP212B1
2
Gabbro
DP1
0.38
0.20
1.90
3.24
17RAY-AP041B1
3
Greenstone
DP1
0.85
1.49
0.62
1.07
1.37
1.41
16.50
5.29
1.58
1.20
17RAY-AP053A1
3
Gabbro (cumulate)
DP2c
1.92
1.35
1.42
2.62
1.06
16RAY-AP121B2
3
Greenstone
DP1
1.76
1.04
1.69
3.52
1.17
16RAY-AP130C3
3
Gabbro (cumulate)
DP2c
1.54
1.31
1.17
1.43
0.84
9.0
16RAY-AP179A1
3
Greenstone
DP1
0.99
0.65
1.53
4.85
1.51
8.3
16RAY-AP199A1
3
Gabbro (cumulate)
DP2c
1.88
1.46
1.29
2.84
1.03
8.8
16RAY-AP079A1
4
Pillow Basalt
MMS3
1.42
1.42
0.66
0.66
2.14
2.14
1.55
1.55
1.43
1.43
15RAY-JR075A
5
Harzburgite
DP2b
0.50
0.10
0.21
2.37
14.26
5.87
16RAY-AP088D1
5
Dunite
DP2b
0.64
0.18
3.51
2.04
16RAY-AP093A1
5
Dunite
DP2b
0.58
0.24
2.39
4.00
16RAY-AP094A1
5
Dunite
DP2b
0.04
8.59
16RAY-AP099A2
5
Harzburgite
DP2b
0.73
0.08
8.97
11.75
16RAY-AP101A1
5
Lherzolite
DP2b
0.35
0.43
0.82
2.80
16RAY-AP113A2
5
Harzburgite
DP2b
0.14
8.46
16RAY-AP123A2
5
Dunite
DP2b
0.10
0.06
1.67
7.40
16RAY-AP151A1
5
Harzburgite
DP2b
1.98
0.57
3.49
14.26
0.64
16RAY-AP172A2
5
Lherzolite
DP2b
0.15
0.20
0.72
2.42
16RAY-AP172A1
5
Lherzolite
DP2b
0.70
0.53
1.32
2.02
16RAY-AP174A2
5
Dunite
DP2b
0.07
0.06
1.20
4.26
16RAY-AP178B1
5
Pyroxenite
DP2b
0.13
0.10
1.29
26.82
16RAY-AP196D1
5
Dunite
DP2a
0.51
0.22
2.28
1.57
16RAY-AP205A1
5
Harzburgite
DP2a
0.42
0.37
1.16
2.47
16RAY-AP206A1
5
Harzburgite
DP2a
0.20
0.10
2.01
2.80
Footnotes
Full data set and QC presented in Supplementary Materials 02
-' indicates no data, due to concentratons outside of detection limits
1) Normalized against standard N-MORB composition (Sun & McDonough, 1989), except Group 5, which is normalized against standard primative mantle composition (Sun & McDonough, 1989)
2) Ti normalized against standard N-MORB composition (Sun & McDonough, 1989), except Group 5, which is normalized against primative mantle composition (McDonough & Frey, 1989)
3) V normalized against standard N-MORB composition (Klein, 2004), except Group 5, which is normalized against primative mantle composition (McDonough & Frey, 1989)
4) ƐNd calculation based on a model age of 265 Ma
Latitude
Longitude
61.63506654
61.59242971
61.59007387
61.59540921
61.63129486
61.59011971
61.5836507
61.63073
61.58143204
61.63232538
61.58670054
61.5836507
61.63234
61.62589037
61.59755302
61.60605985
61.62199554
61.58258804
61.58804837
61.59242971
61.59242971
61.59493771
61.63095953
61.59874752
61.62962702
61.59001219
61.59460302
61.58652204
61.61442871
61.58804837
61.61659902
61.59276702
61.60996203
61.60182918
61.59690452
61.62613451
61.60353936
61.63073
61.62613
61.62751169
61.62295119
61.6222022
61.61678803
61.60240819
61.62396118
61.59975069
61.59975069
61.59814669
61.61149835
61.59532635
61.59274121
61.59335037
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