Cretaceous intracontinental rifting at the southern Chatham Rise margin and initialisation of seafloor spreading between Zealandia and Antarctica
Introduction
The breakup of supercontinents such as Gondwana is often associated with a change from lithospheric convergence (i.e., subduction activity and orogeny) to lithospheric divergence (i.e., crustal thinning prior to seafloor spreading). The mechanisms controlling the polarity of tectonic forces play a key role in the Wilson cycle (Dewey and Burke, 1974), but are poorly understood. Options include triggering by mantle dynamics leading to rising plumes and result in active and ‘hot’ rifting or, alternatively, by tectonic forces through far-field processes with significantly less or without any magmatic activity, which lead to passive and ‘cold’ rifting.
The Cretaceous collision of the Hikurangi Plateau with Zealandia (Fig. 1A) is interpreted to have initiated the end of subduction activity and compression at the East Gondwana margin (e.g., Davy, 2014; Davy et al., 2008). At approximately the same time intracontinental rifting was initiated, which led to the separation of Zealandia and Antarctica (e.g., Mortimer et al., 2016; Tulloch et al., 2009b). While the Late Cretaceous to Cenozoic seafloor spreading history between Zealandia and Antarctica is relatively well studied (e.g., Eagles et al., 2004a; Wobbe et al., 2012; Wright et al., 2016), the early rifting history between both conjugate margins, in particular those of Chatham Rise and Amundsen Sea/eastern Marie Byrd Land sector (Fig. 1B), remains poorly understood. The temporal overlap of the Hikurangi Plateau collision, subduction cessation and onset of rifting raises the following questions: Did the former Hikurangi Plateau subduction influence or initiate the early rifting? Or were collision and crustal extension two independent causal processes in the highly complex continental area of the Chatham Rise?
Knowledge about the nature and crustal structure is essential for any sound reconstruction of the margin evolution and the role of subduction cessation and breakup at the former East Gondwana subduction zone. Is the southern Chatham Rise margin a volcanic-rifted type margin with seaward dipping reflectors indicating excessive emplacement of magma triggered by an upwelling plume (Storey et al., 1999; Weaver et al., 1994)? Or was the breakup at the southern Chatham Rise margin non-volcanically driven by tectonic forces like transtensional movements along the West Wishbone Ridge (Fig. 2A; Barrett et al., 2018; Davy, 2014)? Contrasting paleotectonic scenarios are possible depending on whether oceanic, stretched continental crust and/or exhumed mantle is assumed to underlie the SE Chatham Terrace (Figs. 1A and 2A), an area of seafloor south of the Chatham Rise, where water depth is shallower than the abyssal oceanic crust and hosts abundant seamounts and guyots. For a fundamental understanding of the driving forces of the breakup it is also essential to know details on the exact timing for the first formation of oceanic crust and the amount of volcanism related to the breakup.
In this study we attempt to answer these questions for the particular situation of the Chatham Rise east of the Chatham Islands and SE Chatham Terrace. We acquired three 330–485 km long seismic wide-angle reflection and refraction profiles during the RV Sonne cruise SO246 in 2016 (Gohl and Werner, 2016). Additionally, multi-channel seismic (MCS) reflection and potential field (gravity, magnetic) data were collected along these profiles. Here, we present the results of P-wave velocity and density forward modelling together with an interpretation of the MCS reflection data. Subsequently, we define crustal thicknesses and specify the nature of the southern Chatham Rise margin. Our study explores potential processes governing the cessation of subduction along the East Gondwana active margin and the earliest East Gondwana breakup along the southern Chatham Rise margin, i.e., the transformation of a formerly active subduction margin to a passive rifted margin. Our findings also have implications for the geological and tectonic evolution of other, once nearby, continental areas like the Bounty Trough and rift basins east of the South Island as well as the conjugate Marie Byrd Land margin of West Antarctica.
Section snippets
Tectonic and geological background
The North and South Islands of New Zealand represent a small fraction of the Zealandia Continent, which are elevated above the sea level (Fig. 1A; Mortimer et al., 2017). The larger submerged part of Zealandia is formed by thinned continental crust and includes Challenger Plateau, Lord Howe Rise and Norfolk Ridge (Fig. 1A; among New Caledonia further in the north) as parts of North Zealandia and Campbell Plateau, Bounty Platform and the Chatham Rise as parts of South Zealandia (Fig. 1A; e.g.,
Seismic wide-angle reflection/refraction data
Seismic wide-angle reflection/refraction data were collected along three deep-crustal profiles across the southern Chatham Rise margin (Fig. 2A and C) using ocean-bottom seismometers (OBSs), each equipped with a three-component seismometer and a hydrophone, and ocean-bottom hydrophone (OBH) systems with hydrophones only. Along profiles AWI-20160100 and AWI-20160200, 40 and 35 OBS/OBH instruments were deployed at ~11 km spacing. 21 OBS/OBH instruments were deployed with ~15 km spacing along
Model uncertainties
Generally, we find that the estimated layer boundary depth and velocity uncertainties in our three P-wave velocity models increase with depth (Table 1, Table 2, Table 3) and decreasing ray coverage. Velocity uncertainties are less than ±0.2 km/s for the sedimentary layers, ±0.1 to ±0.15 km/s for the upper crustal layers and reach up to ±0.4 km/s in a few zones of the lower crustal layers where refracted phases are sparse. Since several large-offset mantle refractions have been observed, mantle
Crustal structure of the southern Chatham Rise margin
Both the P-wave velocity-depth profiles and the density models from gravity data reveal a detailed structure of the various regions of the Chatham Rise, the SE Chatham Terrace, and adjacent ocean crust. We extracted 1D velocity-depth profiles in 5–10 km steps along all regions covered by the three P-wave velocity models and compared them to published data to compare and classify crustal types (Fig. 14). The three profiles indicate distinct variations of crustal thicknesses and occurrence of the
The collision of the Hikurangi Plateau with the East Gondwana margin
Along two of our seismic refraction profiles, we observe a Hikurangi Plateau that is underthrusted beneath the thicker Chatham Rise (Fig. 15B and C) east of the Chatham Islands (Fig. 15B and C). Collision and underthrusting of the Hikurangi Plateau with the East Gondwana margin in the area of the South Island is inferred to took place at 110 Ma (Fig. 17A; Davy, 2014), pre-dating the collision along the Chatham Rise west of the Chatham Islands (Fig. 17B) in the area of the two profiles. The
Conclusions
In this study, we present three newly acquired seismic reflection, seismic refraction/wide-angle reflection and potential field data from the southern Chatham Rise margin, including SE Chatham Terrace, and adjacent oceanic crust. P-wave velocity modelling reveals the crustal structure of these areas and provides new insights into the changeover from a convergent tectonic regime with subduction and collision of the Hikurangi Plateau with the East Gondwana subduction zone to a divergent regime
Declaration of competing interest
The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.
Acknowledgements
We thank Captain Oliver Meyer and his crew for their support and assistance during the RV Sonne cruise SO246. We are grateful to the two anonymous reviewers for their constructive comments and suggestions. This project was funded through grant no. 03G0246A of the German Federal Ministry of Education and Research (BMBF) and by AWI internal funding through the AWI Research Program PACES-II and its work package 3.2 “Earth systems on geological timescales: From greenhouse to icehouse world”. The
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