Showing posts with label Southern Ocean. Show all posts
Showing posts with label Southern Ocean. Show all posts

Sunday, 3 August 2025

Musellifer leasiae: A new species of Gastrotrich from Antarctica.

The waters of the Southern Ocean, which surrounds Antarctica, are considered to be a hotspot for marine biodiversity, yet only their macrofauna has been extensively studied. The meiobenthos (bottom dwelling organisms larger than single-celled microbes, but still difficult or impossible to see with the naked eye) of this region has been particularly poorly studied, and almost all of the studies which have occurred have been of Nematodes or Crustaceans. To date, twenty species of Tardigrades have been described from the waters around Antarctica, two Gnathostomulids, one of which was only identified to family level, and five Kinorynchs (although a study which should be published later this year is expected to add to this) have been described from this region, but not a single Scalidophoran, Loriciferan, or meiobenthic Priapulid.

Gastrotrichs are a phylum of minute animals, generally less than a millimetre in length, found in interstitial spaces in sediments. Their small size meant that they went unnoticed until the event of microscopy, with the group not being discovered until the 1860s. Despite this unfamiliarity they seem to be ubiquitous in marine sediments, and are also often found in non-marine settings. To date, only a single Gastrotrich, Thaumastoderma antarctica, has been identified from Antarctic waters, although there have been several reports of unidentified Gastrotrichs.

In a paper published in the journal Zootaxa on 17 June 2025, Martin Sørensen of the Natural History Museum of Denmark at the University of Copenhagen, Thiago Araújo of the University of Massachusetts Lowell, Lara Macheriotou and Ulrike Braeckman of the Marine Biology Research Group at Ghent University, Craig Smith of the Department of Oceanography at the University of Hawai’i at Mānoa, and Jeroen Ingels of the Coastal and Marine Laboratory at Florida State University, and the National Institute for Water and Atmospheric Research in Wellington, New Zealand, describe a second species of Gastrotrich from Antarctic waters.

The new species is described from specimens collected in December 2015 and April 2016 from sediment cores collected from depths of between 532 and 701 m in Andvord Bay the west coast of Graham Land, and the Gerlache Strait, which separates the Palmer Archipelago from the Antarctic Peninsula. It is placed within the genus Musellifer, and given the specific name leasiae, in honour of marine biologist  Francesca Leasi in recognition of her numerous contributions to Gastrotrich taxonomy and morphology.

Map showing the sampling stations. (A) Overview of Antarctica, with the Antarctic Peninsula framed. (B) Antarctic Peninsula with sampling area framed. (C) Sampling area with stations. Red star indicates the type locality; yellow dots indicate additional stations with Musellifer leasiae. Sørensen et al. (2025).

Specimens of Musellifer leasiae are between 322 and 415 μm in length, and have a body with a pointed head, a weakly defined neck, a parallel-sided body, and a pair of tapering furcal branches ('tails'). This body is covered by approximately 26 columns of scales, with an average of 45 scales per column. The columns can be divided into eight dorsal columns, two sets of five ventral columns, and eight ventral columns. The ventral surface also has two rows of locomotory cilia.

Line art illustration of Musellifer leasiae, (A) Dorsal view. (B) Ventral view. (C) Close-ups of head scales, anterior-, and posterior trunk scales, and terminal furca scales. Sørensen et al. (2025).

Five species of Musellifer have been described previously; Musellifer delamarei and Musellifer profundus from the Mediterranean, Musellifer tridentatus from the Caribbean, Musellifer reichardti from the Atlantic coast of Florida, and Musellifer sanlitoralis from the San Juan Archipelago in Washington State. Only a single specimen has previously been described from the Southern Hemisphere, a possible specimen of Musellifer profundus, making Musellifer leasiae the first known species in the genus with a Southern Hemisphere, as well as the first species from the Antarctic.

Light micrographs showing overviews and details of holotype NHMD-1801023 (A)-(H) and paratype NHMD-1801024 (I) of Musellifer leasiae. (A) Ventral overview. (B) Body, anterior, U0-32, dorsal view. (C) Body, anterior, U0-32, ventral view. (D) Body, median, U26-55, dorsal view. (E) Body, median, U28-60, dorsal view. (F) Body, posterior, U54-84, dorsal view. (G) Body, posterior, U54-86, ventral view. (H) Caudal furca branches, U67-100, ventral view. (I) Body, posterior, U54-82, focused on adhesive glandular tissue. Abbreviations: agt, adhesive glandular tissue; lcf, locomotory ciliary field; vcb, ventral ciliary bands. Sørensen et al. (2025).

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Thursday, 8 February 2024

The hottest January on Record.

January 2024 was the hottest January on record, according to the European Union's Copernicus Climate Change Service, with average global surface air temperatures reaching 13.14°. This exceeds the previous hottest January ever recorded, 2020, by 0.12°C, and the average for the period 1991-2000 by 0.70°C, as well as the (calculated) average for the period 1850-1900 by 1.66°C. This is the eight consecutive calender month to have been the hottest example of that particular calender month on record, starting from June 2023 (July 2023 was also the hottest month ever recorded).

Surface air temperature anomaly for January 2023 relative to the January average for the period 1991-2020. Copernicus Climate Change Service.

The average global sea surface temperature between 60°S and 60°N reached 20.97°C, making it the hottest January ever recorded in terms of sea surface temperatures, exceeding the previous record, set in January 2016, by 0.26°C. The month was also the second highest month overall in terms of sea surface temperature, with the hottest ever month, August 2023, being only 0.01°C hotter at 20.98°C. The average sea surface temperature for February so far exceeds this record, but the average for the month may be brought down if there are cooler days later on.

Daily sea surface temperature (°C) averaged over the extra-polar global ocean (60°S–60°N) for 2015 (blue), 2016 (yellow), 2023 (red), and 2024 (black line). All other years between 1979 and 2022 are shown with grey lines. Copernicus Climate Change Service.

Surprisingly, sea ice levels in the Arctic have been the highest since 2009, with above average concentrations of ice in the Greenland Sea (a persistent feature since October) and Sea of Okhotsk, although levels were below average in the Labrador Sea. Antarctic sea ice levels were the sixth lowest ever recorded, although they were significantly higher than in January 2023.

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Tuesday, 5 December 2023

Austropallene halanychi: A new species of Pycnogonid 'Sea Spider' from the Ross Sea, Antarctica.

Pycnogonid 'Sea Spiders' are a distinctive group of marine Arthropods, thought to be either members of the Chelicerata (the group which also includes Arachnids, Horseshoe Crabs, and the extinct Eurypterid Sea Scorpions), or a basal Arthropod group, forming the sister group to all other living Arthropods. Pycnogonids have four (or sometimes five) pairs of long legs emerging from a very small body, The head has a distinct proboscis which allows them to suck nutrients from soft-bodied Animals, as well as ocular tubercle with eyes, and up to four pairs of appendages, from front to back the chelifores, the palps, the ovigers (used for cleaning themselves and caring for eggs and young), and the first pair of walking legs. About 1300 species of extant Pycnogonids are known, most of which are very small (to the extent that the leg muscles in some species comprise a single cell), although some deep water and Antarctic species get quite large, with the largest having a leg span of over 70 cm.

In a paper published in the journal ZooKeys on 28 November 2023, Jessica Zehnpfennig and Andrew Mahon of the Department of Biology at Central Michigan University, describe a new species of Pycnogonid from the Ross Sea, Antarctica.

The new species is placed in the genus Austropallene, and given the specific name halanychi, in honour of Kenneth Halanych, a marine biologist whose commitment and dedication to the benthic marine systems in the Southern Ocean has provided a wealth of information related to biodiversity in the Antarctic system. It is described from a single male specimen, collected by benthic trawl from the RVIB Nathaniel B. Palmer on 31 January 2023.

Austropallene halanychi, male holotype. (A) Dorsal view. (B) Dorsal-frontal view; note shape, relative size, and black tips of chela fingers, cephalic spurs, and eye tubercle and eyes; note sharp conical outgrowths at base of fixed and movable fingers of chelifores (red arrow). Zehnpfennig & Mahin (2023).

The single known specimen of Austropallene halanychi was collected from a depth of 570 m on the Ross Shelf seafloor. It is 10.5 mm in length with walking legs up to 28.78 mm long. Its body is slender with a fully segmented trunk, a distinct neck, The abdomen is short, and the proboscis is directed downwards and tapers to a point. Four eyespots are present. 

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Monday, 27 November 2023

Iceberg A23a has begun to move.

An iceberg known as A23a, considered to currently be the largest in the world, with a surface area of about 4000 km² and a thickness of about 400 m, has begun to move, after remaining grounded within the Weddell Sea for several decades. The iceberg was one of a cluster that broke away from the Filchner Ice Shelf in November 1986, prompting the emergency evacuation of a Russian science station which was located on the breakaway part of the ice, but subsequently became grounded in the shallow waters of the Weddell Sea. The iceberg subsequently moved a short way in 2020, but again became grounded. It has now begun moving again, and appears likely to move out of the Weddell Sea and into the Antarctic Circumpolar Current, which will carry it west towards South Georgia and South Africa.

The current location of Iceberg A23a. Copernicus-Sentinal 3/BBC.

The increased rate of movement and break up of many ice sheets, which leads to the formation of icebergs, is thought to be directly connected to rising global temperatures. However, the movement of icebergs once they have formed is less well understood and it is unclear to what extent these events are climate driven. Icebergs from the Antarctic Peninsula and Ronne Ice Shelf typically become trapped in the Weddell Sea for many years, before migrating into the Antarctic Circumpolar Current. Icebergs in this, slightly warmer, current will tend to melt over time, but can drift a long way first, sometimes becoming stranded off South Georgia or even drifting into the shipping lanes around South Africa.

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Saturday, 26 August 2023

All Emperor Penguin colonies on the Bellingshausen Sea believed to have failed in 2022.

Emperor Penguins, Aptenodytes forsteri, are the largest species of Penguin, and have become iconic symbols of Antarctic wildlife, being the only Vertebrates that overwinter on the Antarctic continent. The species is dependent on the presence of anchored sea ice (sea ice attached to land rather than drifting) during the breeding season, with breeding and moulting taking place on the ice, while foraging for food is largely accomplished in waters around the ice shelf. Emperor Penguins typically arrive at their breeding grounds in March and April and lay eggs in May and June, with chicks hatching in July and August and fledging in December and January. This means that stable, land-fast ice needs to remain in place between April and January for breeding to succeed.

This means the Emperor Penguins are directly threatened by climate change, with loss of sea ice, or changes in its distribution, known to have caused failure at individual breeding sites in the past. Attempts at predicting the future of the species have painted a bleak picture, with current climate predictions suggesting that 90% of Emperor Penguin colonies will no longer be viable by the end of the twenty first century due to global warming and the accompanying loss of sea ice. This is the first anthropogenic threat the species has faced; Emperor Penguins have never been hunted, never suffered direct habitat loss due to Human expansion, and their fishing grounds have not been overfished by Human competitors, making them the only known Vertebrate species for which climate change is the sole threat to their long-term survival. 

A group of Emperor Penguins, Aptenodytes forsteri, on the Antarctic Ice Shelf. Ty Hurly/ICUN Red List of Threatened Species.

There are five known Emperor Penguin colonies on the Bellingshausen Sea, at (from east to west) Rothschild Island, Verdi Inlet, Smyley Island, Bryant Peninsula and Pfrogner Point. All of these colonies have been discovered within the past 14 years, using medium resolution satellite imagery, and subsequently had their populations assessed using very high-resolution imagery. Only the Rothschild Island colony has ever been visited, although the Smyley Island colony has been sighted from the air. The sites are assumed to be breeding colonies because they are occupied between October and December, when large aggregations of non-breeding Emperor Penguins have never been recorded. The largest of the Bellingshausen Sea colonies is on Smyley Island, where an average of 3500 pairs have been recorded, while the smallest is on Rothschild Island, with only 630 pairs recorded.

In a paper published in the journal Communications Earth and Environment on 24 August 2023, Peter Fretwell of the British Antarctic Survey, Aude Boutet, an independent researcher from Paris, and Norman Ratcliffe, also from the British Antarctic Survey, discuss the impact that loss of sea ice across much of the Bellingshausen Sea in November and December 2022 had upon Emperor Penguin breeding colonies of the area.

Antarctic sea ice extent in 2022–2023. The red line shows sea ice extent (more that 15% concentration) for 2022–2023, blue line shows 2021–2022 and the orange line is the 1981–2010 mean. The yellow ribbon is the satellite record (1979–2022). The grey shading refers to breeding stages of Emperor Penguin chicks. Critically sea ice must be stable for Emperor Penguins until the end of the fledging stage for all chicks to survive. Between October and January 2022–2023 sea ice around the continent has been at or below to the lowest ever recorded in the 45 year satellite record. Only briefly in mid-November did the concentration fleetingly rise to the second lowest extent. This low period intersected with the end of créching and fledging period in the emperors breeding cycle. Data courtesy of National Snow and Ice Data Center, Boulder, Colorado. Fretwell et al. (2023).

Four of the five Penguin colonies were affected by early sea-ice loss in November 2022; at this time much of the Southern Ocean around Antarctica was affected by sea-ice loss, but the Bellingshausen Sea suffered the most significant loss. Three of these colonies had been visible in satellite images in late October and early November, but were abandoned by the start of December, when the chicks should have begun fledging. The Pfrogner Point colony, which is the most westerly on the Bellingshausen Sea, and which was outside the area of the sea-ice anomaly, was also abandoned at some point between 29 October and 9 November 2022, probably due to earlier loss of sea ice.

Antarctic sea ice anomaly for November 2022. Blue areas in the map show positive sea ice anomaly, red shows negative. Although most of the continent has witnessed negative sea ice extent, the Bellingshausen Sea area has been particularly badly affected with up to 100% loss of ice in the region. Fretwell et al. (2023).

Exact timings of chick hatching and fledging on the Bellingshausen Sea have never been made, so assumptions about when these events occur have been based upon observations on Cape Washington and Pointe Géologie in the east Antarctic, where fledging begins in early- to mid-December, and finishes in late December or early January. This makes it likely that the Bellingshausen Sea colonies suffered total failure in 2022, due to losing their sea-ice before these dates. It is possible that some chicks were able to survive on grounded icebergs, but this is unlikely to have been a significant proportion of the whole, and the three colonies which disappeared before the onset of December were simply abandoned by the adult Penguins.

Emperor penguin colonies in the central and eastern Bellingshausen Sea. The locations of the five emperor penguin colonies in this region superimposed over the regional sea ice concentration anomaly for November 2022 shown in red. Fretwell et al. (2023).

Although satellite data is only available for the entire of the Bellingshausen Sea from 2018 onwards, only one of the colonies is known to have previously suffered a complete loss of sea-ice (Bryant Peninsula in 2010), and statistical models which predicted the colony failures in 2022 from satellite data suggest that it is unlikely that other such losses have gone undetected. 

The timing of satellite imagery showing sea ice break up and colony disappearance at the five colonies, in comparison with the timing of the breeding stage of the species. The dark blue circles denote Sentinel2 images where the colony can be seen. Light blue hexagons denote where ice was still present but there was no sign of the colony (no brown pixels) and orange squares denote images where sea ice had broken up or dispersed. Note that four of the five colonies were abandoned by the start of the fledging season. Fretwell et al. (2023).

The Verdi Inlet colony was first detected in 2018, and has been found in satellite imagery each year since. in 2018-2021 sea-ice around the inlet did not break up until January, with an estimated 3000 pairs of Penguins using the site in November 2021. The colony was observed in September 2022, but was much smaller than in previous years. The last of the land-bound sea-ice around Verdi Inlet broke up between 31 October and 4 November 2022, with all ice having vanished by early December. No signs of Penguin activity were detected after the initial break-up of the ice, suggesting the colony was abandoned at this point.

The Smyley Island colony was first detected in Landsat imagery in 2009, and the colony has been monitored in Very High-Resolution satellite imagery by the British Antarctic Survey since that time. The colony was home to between 1000 and 6500 pairs of breeding Penguins each year, with a ten-year average of 3000 pairs. Bound sea-ice was observed around the island until at least early December, until 2022, when the ice broke up in mid-November. Prior to this, the colony had split into two groups about 4 km apart (suggesting the Penguins were aware there was a problem, and had reacted to it), Some Penguins were detected on a grounded iceberg in December, although it is unclear if any chicks survived.

The Bryant Coast colony was first detected in Landsat data in 2014, and subsequently found in images dating back as far as 2000. The colony was absent in 2010, and reached a maximum size of 2000 breeding pairs in 2014. Multi-year bound-ice was present at the colony site from 2010 until 2021, providing the Penguins with a stable year-round platform. In 2022 the colony was detected in mid-November, but again seemed smaller than usual. By 25 November, the sea-ice could be seen retreating close to the colony, and by 29 November the bound sea-ice around the colony had gone, although floating pack-ice was still present, with some brown staining (indicative of the presence of Penguins) observed on this ice. However, by 2 December all signs of Penguin activity had vanished, and the colony is presumed to have failed. 

The Pfrogner Point colony was first detected in satellite imagery in 2019, and has been found in satellite images from 2018-2022, with a single estimate putting the population at 1200 pairs of Penguins. The colony is situated on an ice shelf (part of a glacier flowing out over the sea) rather than directly on the sea-ice, and appears to have shifted between the main shelf and a tongue of ice associated with an outflowing creek. The colony was detected on 9, 22, and 29 October 2022, although it appeared smaller than usual, but was not seen in an image taken on 8 November, nor any subsequent image. by 12 December all sea ice in the area had vanished, and no Penguins could be observed. This colony appears to have been abandoned before the ice began to break up, although why this was the case is unclear. Very high resolution satellite images suggest that the ice cliff at the edge of the shelf was about 4.5 m high, with a snow ramp between the shelf and the sea ice below at the foot of the ice creek. Satellite images from October suggest that the sea ice beneath this ramp may have broken close to the ice cliff, which would have made it impossible for the adult Penguins to return from the sea to their chicks, forcing them to abandon the colony.

The Rothschild Island colony is the furthest north of the Bellingshausen Sea colonies, being found on sea ice between Alexander Island and Rothschild Island within the Wilkinson Sound embayment. It is a small colony, home to about 700 pairs of breeding Penguins. The colony was directly observed by helicopters deployed from the luxury cruise ship Commandant Charcot on 20 November 2022, which counted 228 adult Penguins, and 820 chicks. Satellite images revealed that there was still ice beneath the colony on 5 and 17 December, although several large patches of open water had appeared within the ice shelf, with the ice around the colony starting to break up on 20 December, making likely that at least some of the chicks fledged successfully. Rothschild Island was close to the heart of the 2022 sea-ice anomaly, and yet the sea-ice appears to have remained sufficiently intact for the Penguins chicks to fledge. It is possible that the sheltered position within the shallow Wilkinson Sound and the many icebergs in the surrounding sea helped to stabilize the sea for longer than at other locations.

Sentinel2 imagery from the five colonies in 2022 showing the progressive sea ice extent though the créching and fledging season. Each of the five columns shows multiple images from a single colony, with the earlier images at the top and the later images below. Images where the brown pixels of guano staining, indicative of emperor penguin colonies can be seen are highlighted with yellow circles. Fretwell et al. (2023).

Scientists have been monitoring Emperor Penguins by satellite since 2009, and other instances of breeding colonies being lost to rapid ice break-up. Some colony sites, such as the Leda Bay colony in Marie Byrd Land appear to be particularly prone to this, and fail regularly. However, the 2022 event is the first recorded instance of a widespread sea-ice failure affecting multiple colonies before the chicks fledge. Moreover, only one of the Bellingshausen Sea breeding colonies had previously undergone such a failure, suggesting that the 2022 sea-ice collapse event was genuinely significant.

Emperor Penguin colonies have been known to relocate in response to repeated sea ice failure. A colony of Penguins which formerly bred at Halley Bay in the Weddell Sea, but the ice here began to fail regularly from 2016 onwards, prompting the Penguins to relocate their breeding site to a more stable location on Dawson Lambton Glacier, 85 km to the south. However, more widespread failures of the ices shelf due to global warming would make such relocations impossible, although some respite might be offered by refugia such as the Rothschild Island location.

It is difficult to predict exactly how climate change will affect the future of the ice shelf, but all current models suggest that a long-term decline in the ice cover is to be expected. Satellite records of the extent of the ice shelf go back 45 years, with four of the lowest sea-ice coverages recorded since 2016, and the lowest two coverages being in the 2021-22 and 2022-23 seasons. It is possible that this loss is part of an episodic cycle rather than a genuine long-term trend, and answering this question is now a priority for scientists studying the Antarctic climate and sea-ice. The extreme sea-ice loss seen in 2021-22 and 2022-23 is likely to have been influenced by the three years of La Niña conditions in the southern Pacific, which tends to lead to warmer conditions and lower sea ice in the waters off western Antarctica, and that the switch to El Niño conditions in the Pacific in 2023 will lead to a return of cooler conditions and more stable sea ice, but the failures seen in 2022 still represent a warning about the future of Emperor Penguin  in a warming global climate.

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Saturday, 26 December 2020

Understanding the climate of southeast Australia during the Eemian Interglacial.

The Eemian or peak of the Last Interglacial (Marine Isotope Stage 5e, roughly 129 000–116 000 years Before Present) is the most recent geologic period when global temperatures were similar to present, but in response to orbital forcing rather than greenhouse gas loading of the atmosphere. While this makes the Eemian an imperfect analogue for near-future climate due to anthropogenic global warming, the latitudinal temperature distribution was similar to the present. Eemian global mean temperature was 0-2°C warmer than present, mean global sea surface temperatures were indistinguishable from current sea surface temperatures, though sea level was around 6–9 m higher from meltwater inflows from the Greenland and Antarctic ice sheets. Therefore, understanding the climate of the Eemian may provide valuable insight to future climate and its variability.

While often thought of as a period of relative climate stability, climate variability during the Eemian was likely greater than in the Holocene. This has been attributed to meltwater outflows disturbing the Atlantic meridional overturning circulation and a general global cooling trend toward glacial inception. The resulting changes in sea surface salinity and temperature are believed to have driven regional changes in atmospheric circulation leading to periods of widespread aridity across Europe, and onset of abrupt cold periods as sea surface temperatures cooled by several degrees Celsius.

Our understanding of Southern Hemisphere Eemian climate is limited as proxy records are rare. The climate of Australia is globally relevant, as it responds to key global teleconnection forcing, including El Niño Southern Oscillation, Pacific Decadal Oscillation, and the Indian Ocean Dipole. It is also relevant as the severity of recent droughts and bushfires have been linked to increasing temperatures caused by anthropogenic greenhouse gas emissions, thereby stimulating interest in understanding past warm climate conditions such as during Marine Isotope Stage 5e.

Numerical modelling studies suggest reduced seasonal contrast in Marine Isotope Stage 5e temperatures across Australia with warmer winter temperatures, most notably in the north and northwest of the continent by +3°C to +5°C. Austral summer (December–February) temperatures are believed to have been cooler by −1°C to −2°C with modelling studies suggesting that the Australian monsoon was weaker and drier than present with January-April precipitation anomalies of more than − 3 mm per day. A weaker Marine Isotope Stage 5e monsoon aligns with evidence of a variable Lake Eyre hydrology with temporally isolated small inflow events These were likely caused by irregular southward penetration of the Intertropical Convergence Zone and decaying tropical cyclone(s) over the headwaters of the Lake Eyre Basin; conditions similar to those of today that deliver inflows to Lake Eyre.

Winter temperatures in southern Australia during Marine Isotope Stage 5e are believed to have been warmer than present, reflecting warmer sea surface temperatures in the Southern Ocean. This would have reduced the meridional temperature gradient between the sub-tropics and mid/high latitudes with less frequent precipitation bearing cold fronts and extratropical depressions at a time concurrent with strengthening of interannual variability of sea surface temperatures in the eastern tropical Pacific associated with El Niño Southern Oscillation. Slightly cooler Marine Isotope Stage 5e sea surface temperatures to the northwest of Australia relative to present may have contributed further to reduced rainfall over southeast Australia similar to the impact of present day positive Indian Ocean Dipole events. Combined with changes to Atlantic meridional overturning circulation and associated sea surface temperatures, which have been shown under present day conditions to teleconnect to the Pacific Ocean, the climate of Marine Isotope Stage 5e in Australia is likely to have been variable, but in general drier than present. In particular, in southeast Australia where under the current climate positive Indian Ocean Dipole and El Niño Southern Oscillation result in reduced rainfall. However, a dearth of high temporal resolution paleoclimate records from Marine Isotope Stage 5e have until present not been available to test this thesis and the possible links to climate state forcings such as teleconnections and solar variability.

In a paper published in the journal Scientific Reports on 22 October 2020, Hamish McGowan of the Atmospheric Observations Research Group at the University of Queensland, Micheline Campbell and John Nikolaus Callow of the School of Agriculture and Environment at the University of Western Australia, Andrew Lowry, also of the Atmospheric Observations Research Group at the University of Queensland, and Henri Wong of the Australian Nuclear Science and Technology Organisation, present a near annual resolution reconstruction of climate developed from a speleothem that spans the Eemian (Marine Isotope Stage 5e) from 117 500 to 123 500 years before present, the most recent period in the Earth’s history when temperatures were similar to those of today.

In Australia, speleothems offer the greatest potential to develop high temporal resolution terrestrial palaeoenvironmental records. Stalagmite GC001 was removed from a small chamber approximately 60 m into the Grotto Cave, Yarrangobilly Caves, New South Wales, Australia in 2012. The caves are located at the northern end of the Snowy Mountains, at an elevation where the water balance changes from an energy (demand) to supply (precipitation) limited system. The caves were formed through karstification of the Yarrangobilly Limestone, a massive Silurian limestone formation with an extent of about 1.4 km by 14 km and a maximum depth of roughly 450 m. Past work has concluded that reduced rainfall invokes prior calcite precipitation at Yarrangobilly and hence up (down) trend in magnesium/calcium ratios implies increased (decreased) drip water contact time under drier (wetter) conditions.

 
Location map of the Yarrangobilly Caves (a) and aerial oblique perspective of the entrance to the Grotto Cave (b) 300 mm long cross-section of stalagmite GC001 from which samples were extracted for uranium series dating and geochemical analysis (c). The small core perpendicular to the growth axis is the result of in-situ sampling of GC001 for age determination prior to removal from the Grotto Cave (c). McGowan et al. (2020).

The present day climate of the Yarrangobilly area is influenced by the northern extension of the mid-latitude westerly winds. It experiences cool to cold montane temperatures through winter, while in summer warm to hot and dry conditions dominate under the influence of the subtropical ridge. Major Southern Hemisphere ocean–atmosphere teleconnections including the El Niño Southern Oscillation, Southern Annular Mode, Pacific Decadal Oscillation, and Indian Ocean Dipole all affect the regional climate state. Rain bearing weather systems that affect Yarrangobilly Caves may originate from the tropics and the southern mid-latitudes. Mean annual precipitation is approximately 1147 mm, with a mean annual temperature of 12°C. The most effective precipitation occurs during the cool, wet winter and while snow may fall, the site is below the seasonal snowline and no snowpack remains through winter. Temperature logging from where GC001 was collected in the Grotto Cave found mean internal cave temperature was 8.8°C during the study (August 2014 to February 2015).

The magnesium time series for GC001 shows clear cycles of higher/lower concentrations with a marked increase occurring around 120 800 years before present. This period of elevated magnesium concentrations prevailed until around 118 500 years before present. It then remained mostly stable until a sharp decrease at approximately 117 850 years before present. This period of higher magnesium concentrations (drier) in GC001 aligns with a period of increased depletion of the proportion of oxygen¹⁸ in a speleothem from northern Borneo indicating wetter conditions there, indicative of a more northerly position of the Intertropical Convergence Zone. It also correlates with periods of increased dust deposition recorded at Dome C, Antarctica. Australia is a known source of interglacial dust to the Antarctic. Accordingly, McGowan et al. infer drier conditions in southeast Australia as indicated by higher magnesium concentrations from 120 800 to 118 500 years before present in GC001 sustained regional mega-drought(s) across this period with associated wind erosion contributing to increased dust flux at Dome C, Antarctica such as between 119 050 to 120 300 years before presnt. Slightly higher dust flux values from 117 500 to 117 800 years before presnt, may have also originated from southeast Australia but do not correlate with elevated magnesium concentrations in GC001, or any notable signal in the proportion of oxygen¹⁸ record from northern Borneo.

 
Time series of magnesium, strontium and barium concentrations from GC001 (a)–(c); proportion of oxygen¹⁸ from a speleothem collected at Whiterock Cave, northern Borneo (d); dust concentrations from Dome C, Antarctic (e), and temperature departure from the average of the past 1000 years Dome C, Antarctic (f). Pink shading indicates periods of intermediate magnesium concentrations and dust flux (a), (e); yellow shading highest magnesium concentrations and dust flux (a), (e) and blue shading (d) corresponding period of depleted proportion of oxygen¹⁸ indicating wetter conditions in Western Pacific. Vertical dashed blue lines constrain the period interpreted as a mega-drought(s). McGown et al. (2020).

The strontium time series displays some periods of higher/lower concentrations that are concurrent with variability in the magnesium record, such as around 121 000 years before present. However, unlike the magnesium record, the strontium time series exhibits an overall trend of decreasing concentrations with the period between approximately 120 800 years to 118 500 years before present, remaining relatively constant at approximately 25 parts per million, before decreasing more quickly. This is similar to the barium concentrations time series which is strongly correlated with strontium reflecting a reduced growth rate (less drip water) under the drier conditions known to have minimal impact on magnesium concentrations. Barium concentrations do display a more consistent decreasing trend that flattens between 120 800 and 119 100 years before present, before decreasing further after 118 500 years before present.The decreasing trends in the strontium and barium concentrations correlate with the Marine Isotope Stage 5e temperature anomaly reconstruction for Dome C, Antarctic and Marine Isotope Stage 5e sea surface temperatures reconstructions from northwest of Australia and east of New Zealand. Accordingly, the magnesium, strontium and barium concentrations in GC001 collectively record the onset of a prolonged drier period from around 120 750 years before present to 118 500 years before present that was associated with increased atmospheric dust and a cooling in atmospheric and ocean temperatures from Marine Isotope Stage 5e maximums.

Normalised Lomb-Scargle periodograms for magnesium, strontium and barium were calculated to test for the influence of teleconnection and/or solar cycle forcing on the Marine Isotope Stage 5e climate of southeast Australia. The periodograms show common peaks in spectral density around 200 years which align with the de Vries solar cycle (about 205 years). Spectral peaks are also found from 1147 years (magnesium) to 1268 years (strontium) and are within the range of the roughly 1000 year Eddy solar cycle. The strontium and barium records have peaks at about 66.8 and 88.6 years, which match with the Pacific Decadal Oscillation and Gleissberg solar cycle respectively and display coherent spectral peaks at 301.3 years, 454.8 years, 602.7 years and at 3443.8 years. The 301.3 years and 454.8 years cycles are close to the 300 year and 470 year cycles found in sediments from Jeju Island, South Korea. These have been attributed to solar forcing along with the 3443.8 year cycle, which is aligned with the 3300 year Holocene cycles in the proportion of oxygen¹⁸ record from Greenland Ice Sheet Project 2 core. The magnesium record displays a strong 709 year cycle that may be a harmonic of the 1400 year cycle found in glacial and interglacial periods in magnesium/calcium derived sea surface temperatures records from the South China Sea. Accordingly, the geochemistry of GC001 displays cyclic variability indicative of climate variability forced by both teleconnections and solar cycles recorded globally in geologic archives.

 
Periodograms of magnesium, strontium and barium with 0.9 (red dashed line) and 1.0 probability thresholds shown. Selected dominant periods (annotated) are rounded to the nearest decade. McGowan et al. (2020).

Wavelet transforms for magnesium, strontium and barium show regions of significant periodicity (95% confidence level). All three elements display significant 4 to 8 year cycles that McGowan et al. interpret as El Niño Southern Oscillation and around 20 to 30 years, and 50 to 65 years, which are indicative of the Pacific Decadal Oscillation. While caution is required in attributing shorter-duration cycles given laser ablation sampling resolution, the magnesium record shows clear gaps in El Niño Southern Oscillation (4–8 year) cycles from approximately 121 500 years before present to around 120 500 years before present. These coincide with a change in magnesium concentrations from about 140 to about 200 parts per million indicating a transition to drier conditions, while the period from 118 500 to 117 500 years before present overlaps with the return to magnesium concentrations, about 140 parts per million suggesting increased moisture availability. Pacific Decadal Oscillation like cycles are most common from around 119 800 years before present to 118 500 years before present.

 
Wavelet plots of magnesium (a), strontium (b), and barium (c). The thick black lines represent 95% confidence levels. The lightly shaded region toward the bottom is the Cone of Influence and values in the light region should be considered with caution. McGowan et al. (2020).

In the strontium wavelet transform diagram, the El Niño Southern Oscillation signals are most frequent from the start of the record to about 122 100 years before present and are concurrent with the occurrence of the multi-decadal Pacific Decadal Oscillation like cycle. This longer decadal cyclicity is also evident from 121 500 years before present to 118 500 years before present with evidence of a separate 20 to 30 year cycle and longer 55 to 75 year cycle. The barium wavelet plot shows also a dominant short duration El Niño Southern Oscillation signal in the early part of the record that progressively becomes less frequent. The Pacific Decadal Oscillation period cycle is not strong and only occurs above the 95% confidence level occasionally from 123 500 years before present to around 122 200 years before present and again from around 121 000 years before present to 119 500 years before present.

Understanding the causes and frequency of climate variability is essential to inform prediction of future climate. Proxy of climate variability dating from Marine Isotope Stage 5e, the most recent warm period with temperatures similar to the present, offer potential to develop this understanding. The magnesium Marine Isotope Stage 5e record from stalagmite GC001 shows multi-centennial periods of increased Mg concentration indicating drier climatic conditions in southeast Australia, notably from 118 500 to 120 750 years before present. This period coincides with increased dust flux recorded in Antarctic ice. The strontium and barium concentrations show evidence also of this climate variability with trends of decreasing concentrations correlated with cooling air temperatures and sea surface temperatures. Collectively, the magnesium, strontium and barium records from GC001 with supporting regional paleoclimate records suggest that southeast Australia during Marine Isotope Stage 5e experienced multi-centennial periods of reduced precipitation, temperature variability and increased atmospheric dust. These conditions such as from 118 900 to 120 400 years before present are indicative of mega-droughts. Superimposed on these multi-centennial periods of drier climatic conditions are higher frequency interannual to interdecadal teleconnections and solar forced cycles of further variability.

A drier climate during Marine Isotope Stage 5e such as from 118 900 to 120 400 years before present would align with results from numerical modelling which found a generally weaker summer monsoon and warmer winter conditions. A weaker monsoon aided by cooler sea surface temperatures northwest of Australia at this time would lessen moisture transport into southeast Australia via meridional conveyors such as northwest cloud bands, while warmer temperatures during winter would have increased evaporation, intensifying dry conditions that spanned centuries as evident in our record. Numerical modelling of future climate at +1.5°C indicates that the Australian monsoon may weaken, resulting in an increase in the frequency of dry days. Accordingly, the convergence of our paleoclimate record from stalagmite GC001 and published numerical modelling strongly suggest that the climate of southeast Australia will likely become drier throughout the twenty-first century with increased risk of multi-centennial duration dry periods widely referred to as mega-droughts.

The magnesium, strontium and barium records from stalagmite GC001 all display cycles with periodicity of well documented solar and teleconnection forcings of climate. Dominant solar cycles including the Gleissberg solar cycle (88 years), de Vries solar cycle (about 205 years) and possible Eddy solar cycle (about 1000 years) are evident in the geochemistry of GC001. Increases (and decreases) in total solar irradiance through such cycles result in direct heating (and cooling) of the troposphere and Earth’s surface. Indirectly, changes in total solar irradiance influence galactic cosmic ray flux affecting cloud microphysics and cloud cover. Variation in total solar irradiance also causes change in ultraviolet radiation flux, which for a 0.1% increase in total solar irradiance, increases by 4 to 8%. Concurrently this will increase ozone production in the mid and upper stratosphere through the photolysis of oxygen. Corresponding increases in ultraviolet absorption by stratospheric ozone leads to heating and change in the thermal stratification of the atmosphere.

Numerical modelling has shown that enhanced ultraviolet heating of the atmosphere corresponding to total solar irradiance maxima results in a stratospheric zonal wind anomaly that is most pronounced in the Southern Hemisphere during mid to late winter. Dynamical links between the stratosphere and troposphere caused by such ultraviolet forcing lead to change in atmospheric circulation, including jet-stream behaviour, and therefore tropospheric synoptic circulation and ocean dynamics. McGowan et al. therefore postulate that periods of increased total solar irradiance contribute to drier conditions (increased magnesium in GC001) over southeast Australia in response to increased zonal (westerly) flow and a corresponding more southern track of mid-latitude winter storm systems. This occurs in response to a stronger thermal wind component between the tropics/subtropics and the mid to high latitudes causing a response in atmospheric circulation similar to a more positive Southern Annular Mode. The associated decline in precipitation is recorded clearly in stalagmite GC001 by elevated magnesium concentrations and stable to slight decreases in strontium and barium concentrations due to reduced speleothem growth, i.e. reduced drip rate during Marine Isotope Stage 5e.

GC001 records 4 to 8 years El Niño Southern Oscillation-like cycles along with multi-decadal cyclicity indicating Pacific Decadal Oscillation type influences, two teleconnections which have been shown to have the greatest impact on the modern climate and in particular rainfall in southeast Australia. It is therefore reasonable to suggest that these Pacific Ocean teleconnections have been robust and long-lived drivers of interannual and multi-decadal hydroclimate variability in southeast Australia with warm/cool El Niño Southern Oscillation and Pacific Decadal Oscillation phases causing dry/wet periods.

Evidence of El Niño Southern Oscillation cycles in GC001 become no longer statistically significant from around 118 200 yrs before present. This is about 500 years before rapid decline in magnesium concentrations, which suggests reduction in drip water residence times and onset of a wetter climate. This change in magnesium and to a lesser amount in strontium and barium correspond to a rapid increase in sea level of around 5 to 6 m at 118 100 years before present caused by ice sheet melt. McGowan et al. suggest that this dramatic rise in sea level possibly disrupted El Niño Southern Oscillation and Pacific Decadal Oscillation teleconnections and their impact on the climate of southeast Australia at this time.

Collectively, the Marine Isotope Stage 5e climate record developed from GC001 indicates that southeast Australia will likely continue to experience interannual to interdecadal wet–dry cycles driven by teleconnections and solar variability at least until current global warming exceeds Eemian temperatures, possibly within the next decade. However, McGowan et al.'s record also shows that in a warm interglacial climate such as today or near future, there is risk of multi-centennial periods of less effective precipitation (mega-droughts), initiated by natural variability. Should such prolonged periods of drier conditions occur again, then they may be reinforced by anthropogenic global warming, thereby increasing their severity. As a result, McGowan et al. stress the need for further research into the Eemian climate of Australia and the Southern Hemisphere to resolve the causes of prolonged dry periods during Marine Isotope Stage 5e and to determine their spatial impacts. This will allow new insights to our future climate and the risks it may bring such as drought and associated bushfires.

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