The end-Permian Mass Extinction (EPME, 252 Ma) represents an interval of significant disruption and global change driven by the emplacement of the Siberian Traps Large Igneous Province (LIP; eg. Reichow et al. 2009; Burgess et al. 2017; Fielding et al., 2020; Vajda et al. 2020; Frank et al., 2021; McLoughlin et al. 2021) marked by an estimated extinction of 97% of marine organisms and on land 49% of tetrapod families on land(Krull et al., 2004; Korte and Kozur, 2010; Song et al., 2013; Saitoh and Isozaki, 2021; Wu et al., 2021). Following the EPME was a period of recovery that is thought to have lasted around 5 million years, marked by more arid conditions globally and with notable recovery by the Middle Triassic (cf. Korte and Kozur, 2010; Dal Corso et al., 2020; Saitoh and Isozaki, 2021). While the EPME is considered one of the most significant extinction events on Earth, before the onset of the event and following the prolonged recovery, the Earth experienced other major carbon cycle perturbations associated with substantial environmental and climatic change, including, but not limited to, Olsen’s Extinction (~273 Ma late Cisuralian to early Guadalupian; Brocklehurst et al., 2017; Zhang et al., 2020), the Guadalupian Carbon Isotope Excursion (G-CIE) ending in the Capitanian Extinction Event (~262 Ma; Wang et al., 2004; Isozaki et al., 2007a; Lai et al., 2008; Bond et al., 2010a, 2015; Saitoh et al., 2013; Detian et al., 2013; Nishikane et al., 2014; Wei et al., 2018; Saitoh and Isozaki, 2021; Li et al., 2022; 2023), the Carnian Pluvial Episode (CPE, ~232–234 Ma; Dal Corso et al., 2012, 2015, 2021; Mueller et al., 2016; Sun et al., 2016, 2020; Miller et al., 2017; Li et al., 2020, 2022; Fu et al., 2020; Tomimatsu et al., 2021; Peng et al., 2022; Cho et al., 2022) and the mid-Norian Event (MNE, ~215 Ma; Onoue et al., 2016; Jin et al., 2022) leading up to the end-Triassic Mass Extinction (eg. Hallam, 2002, Davies et al. 2017, Wignall and Atkinson, 2020). Records of these events are relatively common from the Northern Hemisphere (e.g., Krull and Retallack, 2000; Wit et al., 2002; Ward et al., 2005; Coney et al., 2007; Hornung et al., 2007; Retallack et al., 2007; Tabor et al., 2007; Retallack and Jahren, 2008; Thomas et al., 2010; Birgenheier et al., 2010; Shen et al., 2013; Mancuso et al., 2020; Lucas, 2017; Peng et al., 2022) but there is a lack of high-resolution records of these events from high-latitude Southern Hemisphere localities. Here we present new evidence of these events from a drill core recovered in Eastern Tasmania, known as Bicheno-5, including high-resolution carbon isotope chemostratigraphy, elemental and sedimentological data (pXRF and hylogging), as well as a palynological assessment. These data are combined with previously published geochronology, allowing the identification of three major carbon cycle and environmental perturbations; the Late Permian G-CIE, the CPE, and the MNE. Importantly these records highlight the impact of carbon cycle perturbations in the paleo-Antarctic circle, as, during the Middle Permian, Tasmania was at a paleo-latitudes of 78°S, moving Northward to 69°S by the Late Triassic (Fig. 1).
The Guadalupian (Middle Permian, ~262 Mya) mass extinction event is associated with a significant negative CIE of >-5 ‰ disrupting the otherwise positive carbon isotope trend in Mid-Permian sediments (cf. Wang et al., 2004; Isozaki et al., 2007a, 2007b; Lai et al., 2008; Wignall et al., 2009; Bond et al., 2010a; Detian et al., 2013; Shen et al., 2013; Zhang et al., 2020; Li et al., 2023). This event is typically interpreted to be associated with an overall climatic cooling, a drop in biological productivity both on land and in the oceans, and the demise of many photosynthetic marine taxa (Wang et al., 2004; Isozaki et al., 2007a, 2007b; Detian et al., 2013; Nishikane et al., 2014), formation of ocean stratification and anoxia (Saitoh et al., 2013; Zhang et al., 2015), sea-level change (Wang et al., 2004; Lai et al., 2008; Wei et al., 2018), and methane release (Retallack and Jahren, 2008; Bond et al., 2010b). The Guadalupian CIE (G-CIE) coincides with the emplacement of the Emeishan LIP in Southwest China between ~257–260 Ma (eg. Shellnutt et al., 2008, 2012; Wignall et al., 2009; Bond et al., 2010a, Huang et al. 2022). However, the link between the emplacement of the Emeishan LIP, the G-CIE, extinction, and evidence of the global extent of the event is still heavily debated, owing to the lack of chronologically well-constrained high-resolution carbon isotope records.
The CPE, (ca. ~232–234 Ma, Bernardi et al. 2018) is a defining point in the Late Triassic, marked by a significant climate shift to more wet and humid conditions globally. It is associated with carbon cycle perturbations of up to -6 ‰ (cf. Dal Corso et al., 2012, 2015, 2018; Sun et al., 2016; Miller et al., 2017; Fu et al., 2020; Li et al., 2020, 2022; Tomimatsu et al., 2021), changes in land biota including a notable global shift from a conifer-dominated forest community to a fern-dominated community suggestive of increased humidity (Peng et al., 2022), and the extinction of some Triassic crinoid taxa (Simms and Ruffell, 2018). The CPE is also considered a critical event leading to the rise and diversification of dinosaurs (Benton et al., 2018; Bernardi et al., 2018). The rapid switch between arid to more humid conditions, caused significant plant extinctions and subsequent ecological shifts, enabling explosive diversification, and radiation, especially of herbivorous dinosaurs (Singh et al., 2021; Zhang et al. 2023). It is linked to the emplacement of the Wrangellian Terrian LIP in the North Pacific (cf. Dal Corso et al., 2012; Jin et al. 2023 ); however, more detailed studies are needed to understand the global nature and impact of the CPE. To date carbon isotope records of the CPE are limited to China (eg. Sun et al., 2016; Fu et al., 2020; Li et al., 2020, 2022, Jin et al. 2023 ), Japan (Tomimatsu et al., 2021), the UK (Miller et al., 2017, Baranyi et al., 2019), the Barents Sea (Mueller et al., 2016), the NW Tethys (Italy and Hungary; Dal Corso et al., 2012, 2015, 2018;), the Indian Himalayas (Hornung et al., 2007), and Argentina (Mancuso et al., 2020). The evidence of the CPE from Argentina derives from a relatively low-resolution carbonate carbon-isotope record and does not show the typical CPE stepped excursion; however, it does provide a relatively precise U-Pb age of 234.47 ± 0.44 Ma in the Carnian-aged lower Los Rastros Formation above which evidence for the CPE is recorded. This section also provides evidence of the hydrological cycle intensification based on clay mineralogy and paleontological evidence of the rapid diversification of dinosaurs during the Carnian (Mancuso et al., 2020).
The MNN carbon cycle perturbation typically has a magnitude of -2–3 ‰ (Onoue et al., 2016) and evidence of a drop in atmospheric CO2 during a period typically marked by relatively high atmospheric CO2 values, as estimated from pedogenic carbonate data (Kent and Clemmensen, 2021). The climate was mainly dry, with a gradual increase in humidity beginning in the late Norian (Berra, 2012; Haas et al., 2012, 2017). An extraterrestrial bolide impact at ~215.5 Ma identified from the 90-km-diameter Manicouagan crater in Canada is postulated as the main driver of this event (eg. Walkden et al., 2002; Onoue et al., 2016; Clutson et al., 2018; Sato et al., 2020). It is associated with intense aridity in the tropical desert belts; unstable climate(Kent and Clemmensen, 2021); a shutdown of primary productivity in the oceans, following the impact, as demonstrated by the decline in biogenic silica and burial fluxes of radiolarian silica, and the proliferation of siliceous sponges (Sato et al., 2020). The shift to more humid climatic belts, which starts in the Norian, is often associated with the dispersal of dinosaurs further north (Kent and Clemmensen, 2021) and ultimately ended the prolonged arid climate that dominated the Triassic.
These three events are characterized by significant ecological and environmental change. In order to understand how these events affected global processes such as weathering rates, the carbon cycle, and climate, we need to examine records spanning the North, mid-latitudes, and paleo-South. Here we present a new high-resolution record from the Bicheno-5 core, Llandaff coalfield, Eastern Tasmania, Australia (Fig 1) representing a unique view into the southern polar circle during this critical interval of Earth’s History.