Showing posts with label Mass Extinctions. Show all posts
Showing posts with label Mass Extinctions. Show all posts

Friday, 7 October 2022

Assessing the possibility that Marsupial Megafuana may have survived on New Guinea long after the arrival of Modern Humans.

During the Late Pleistocene Australia and New Guinea formed a single continuous landmass, known as Sahul. This landmass was home to a wide range of large Marsupials, Reptiles, and Birds, the vast majority of which appear to have become extinct in a relatively short period of time towards the end of the Pleistocene. Although not well dated, these extinctions have widely been linked to the arrival of Modern Humans on Sahul, something which also happened towards the end of the Pleistocene, and which has been linked to other extinction events in different parts of the world. 

However, some evidence appears to run contrary to this evidence, including fossil remains of Megafaunal Animals from Kangaroo Island, South Australia, and Willandra Lakes, New South Wales, which appear to considerably post-date the arrival of Humans in the area. This matter remains difficult to resolve, due to a paucity of Late Pleistocene Animal remains with accurate dating information, combined with a poor understanding of when Modern Humans colonised the different ecoregions of Sahul.

New Guinea today comprises about 10% of the remaining Sahul Landmass, and has a climate, geography, and ecology very different from most of Australia. The island is likely to be a key to understanding the Human settlement of Sahul, as it would have been reached first by any colonisers making their way from Eurasia across the islands of Indonesia, the only plausible model for the settlement of the region. Unfortunately, the Pleistocene fossil and archaeological record of New Guinea is even poorer than that of Australia (something common in tropical forested and upland environments, which cover most of the island).

There are currently five archaeological sites across Sahul which combine Human-made artefacts with Megafaunal remains. Four of these are in Australia: Clogg’s Cave in Victoria State, Cuddie Springs in New South Wales, Seton Rockshelter on Kangaroo Island, South Australia, and Warratyi Rockshelter, in the Flinders range of South Australia. The fifth is at Nombe Rockshelter in Chimbu Province, Papua New Guinea. 

Nombe Rockshelter is particularly interesting, both because it is the only site on New Guinea which appears to combine Late Pleistocene Megafaunal remains with evidence of Human activity (a second possible such site, at Kelangurr Cave in West Papua, has yet to be confirmed), and because of the great distance that separates it from the Australian sites, all of which are on the southern part of that landmass. 

The material at Nombe Rockshelter includes a variety of faunal remains, largely identified from cranial evidence (i.e. skull fragments and teeth), combined with archaeological remains (tools etc.) and charcoal fragments, from which dates ranging from 25 500 to 19 600 years before the present have been obtained, i.e. younger than the date generally given for the mass extinction event which impacted continental Australia and Tasmania, at about 40 000 years before the present.

However, our current understanding of the Nombe Rockshelter material suggests that it cannot be taken as unequivocal evidence of the co-existence of a Human population with indigenous Megafauna. This is because the site was disturbed during a Late Pleistocene occupation of the site; at some point a trench was dug at the back of the cave, and the much of the surface layer in the cave has been reworked by the action of both Humans and Pigs, making it possible that zoological material found in the same layers as tools and charcoal may have been excavated from an earlier layer by the makers of those items.

In a paper published in the journal Archaeology in Oceania on 16 September 2022, Gavin PrideauxIsaac Kerr, and Jacob van Zoelen of the College of Science and Engineering at Flinders UniversityRainer GrĂ¼n of the Research School of Earth Sciences at the Australian National University, Sander van der Kaars of the School of Earth, Atmosphere and Environment at Monash UniversityAnnette Oertle and Katerina Douka of the Department of Evolutionary Anthropology at the University of Vienna, Elle Grono, Aleese Barron, and Mary-Jane Mountain of the School of Archaeology and Anthropology at the Australian National University, Michael Westaway of the School of Social Science at the University of Queensland, and Tim Denham, also of the School of Archaeology and Anthropology at the Australian National University, review the faunal material from the Nombe Rockshelter, with an emphasis on the previously undescribed post-cranial material from the site, present uranium isotope dates obtained from these remains, examine other sources of dating information from the site, including pollen and protein, and discuss the implications of their findings for our understanding of the timing of Megafaunal extinctions on Sahul.

The Nombe Rockshelter was discovered in 1964 by Peter White of the Australian National Museum, on a limestone outcrop in the Porol Range, part of the Papua New Guinea Highlands, and was the subject of a series of investigations led by Mary-Jane Mountain between 1971 and 1980. 

Map of the Porol Range showing Nombe and other archaeological sites, with inset showing site location within Papua New Guinea. Prideaux et al. (2022). 

The stratigraphy of the Nombe Rockshelter is complex, with the site apparently having been the subject of repeated episodes of disturbance, but the deposits there can be grouped into four main strata. Radiocarbon dating has enabled broad time-frames to be applied to each of these strata, and suggests that three of the four deposits has suffered considerable internal mixing, but that there is little or no mixing between the layers.

The layer at Nombe Rockshelter that does show reliable internal stratigraphy, is termed Stratum B, which forms a clearly layered and well dated Holocene sequence, dated to between 10 400 and 6300 years before the present, which has produced numerous archaeological artefacts. 

However, the layer of of interest in Prideaux et al.'s study is Stratum D, which is rather more complicated to interpret. Stratum D can be divided into five sub-strata, with the uppermost of these being D1 and D5. Sub-stratum D1 being a red-brown clay, and D5 being similar, but with limestone flecks. These overlay sub-stratum D2, a gingerish red-brown clay, which in turn overlies D3, a dense red-brown clay, which in turn overlays D4, a dense brown clay. Substrata D2-D4 are all more than 25 500 years old, and comprised of reworked material which was originally laid down in the beds and banks of a drainage channel. D1 and D5, on the other hand, were laid down on top of these deposits after the channel had ceased activity.

Excavations at Nombe: main figure shows stratigraphic section from backwall (A1) to front (A7) of rockshelter, ith insets showing excavation plan (upper left) and photograph (upper right). Prideaux et al. (2022).

Previous analysis of the site has reported remains attributed to a Thylacine, Thylacinus sp., in both Pleistocene and and Holocene strata at Nombe, as well as four extinct species of large, herbivorous Marsupials, Dendrolagus noibano, Protemnodon tumbuna, Nombe nombe (originally identified as Protemnodon nombe), and a Pig-sized Diprotodontid from the Pleistocene layers (but principally substrata D1 and D5), as well as later, Holocene, deposits. 

Little archaeological material has been recovered from the Pleistocene layers at Nombe, but sufficient to establish the presence of Humans. These include a waisted blade and other materials found directly in context with Megafaunal remains, as well as other archaeological remains older than this. Noteworthy items include an axe blade with a ground edge, recovered from Substratum D1, and the waisted blade, which was found within a crack which had penetrated down into Substratum D3, but was filled with material from Substratum D1, with Megafaunal remains found directly above it, still within Substratum D1. Similar waisted blades are known from some of the oldest known Human settlements on New Guinea, at Bobongara and Ivane Valley, although their use appears to have continued for a long time, and there are much younger examples.

The bones buried in Pleistocene strata at Nombe Rockshelter show some loss of nitrogen (and therefore collagen) and carbon, but on the whole are well preserved, having been quickly incorporated into a clay-rich, anoxic matrix. These Pleistocene layers include faunal remains which have apparently derived from a number of different sources, with a higher proportion of smaller elements than is the case in later Holocene deposits at the site. This may be because bones in the Holocene layers remained at the surface for longer, exposing them to trampling and the deleterious effects of the tropical climate, although it may also indicate that small predators, such as Owls or Dasyurids, were bringing prey items to the site for consumption. Whatever the case, the site is also contains medium and large bones, possible brought to the site by Thylacines, as well as sparse archaeological material, which probably implies the site being visited by Humans only infrequently. The tools and the larger bones appear to date from about the same time as the stone tools, but none of them show direct evidence of Human activity (such as cut-marks)m and no robust stratigraphy has been developed for the site.

Previous studies of the Nombe site and the materials recovered from it have concentrated on attempting to date the material and determine whether New Guinea saw a long period of Human-Megafauna coexistence, with more recent studies turning to isotope dating methods to try to understand the stratigraphy of the site.

Prideaux et al. used uranium-thorium dating to obtain direct dates from Megafaunal remains at Nombe Rockshelter, as well as identifying the post-cranial remains used in the study. Uranium-thorium dating works because uranium decays to thorium at a known rate, so that the ratio  of the two elements in minerals that naturally incorporate uranium but not thorium can be used to establish a date for the minerals. Neither uranium nor thorium are typically found in organic tissues, but uranium can be absorbed into mineral skeletal elements, such as tooth and bone, after an animal is dead, creating the possibility for using uranium-thorium dating to at least establish a minimum age for such tissues; the uranium can potentially be absorbed at any point after death, not necessarily immediately post-mortem, so the method cannot be used to establish a maximum age. They used palynology (pollen analysis) as a way of assessing the environment in which the deposits were laid down, and to better refine the boundaries between strata C and D. 

The first piece of fossil evidence examined, NCA A3 11, is comprised of four fragments of thin cortical bone, with a thin spine which starts 15 mm from the articular facet. The bone lacks a distal articulation, indicative of being either the end of a limb or part of the pelvic or shoulder girdle, and its general morphology is consistent with that of a Mammalian scapula. The size of the bone, combined with its age and location, would indicate that it came from either a very large Monotreme or a medium-to-large Marsupial, and since Monotremes have a quite differently structured scapula to other Mammals, the bone can be assumed to be the scapula of a Marsupial.

Five groups of Marsupials which would have been present in the Late Pleistocene of New Guinea produce members large enough to have a scapula the size of the specimen; the Macropodidae (Kangaroos and Wallabies), Thylacinidae (Thylacines), Thylacoleonidae (Marsupial Lions), Diprotodontidae (an extict group of large Marsupial browsers) and Vombatidae (Wombats). Macropods have a distinctive scapular spine, which is deflected towards the cranium, whereas that of NCA A3 11 is deflected at 10° from the perpendicular. The scalpulas of Thylacoleonids are compressed craniocaudally, giving them a very straight cranial border with a small scapular notch, quite unlike the shape of NCA A3 11. The only Pleistocene Wombat large enough to have produced the specimen, Phascolonus gigas, has a scapula inwardly deflected with outward-bowed borders, rulling out the specimen coming from a Vombatid. The scapulas of Diprotodontids are significantly larger and more robust than NCA A3 11.

This leaves a Thylacine as the only plausible origin of the bone, with specimens assigned to the species Thylacinus cynocephalus (which became extinct on the island of Tasmania in the 20th century) previously described from the Late Pleistocene of Chimbu Province. Since specimen NCA A3 11 is morphologically a good match for Thylacinus cynocephalus, Prideaux et al. feel confident in assigning the specimen to that species.

Surface scans of a partial left scapula of Thylacinus cynocephalus (NCA A3 11). (a) Medial view; (b) lateral view; (c) distal view. Prideaux et al. (2022).

The second specimen examined, NCA X2.12 255, is identified as a Mammalian ascending ramus (the rear part of the upper jaw, and the part which connects to the skull), based upon the presence of distinct coronoid and condylar processes, the shallow temporo-masseteric concavity and the flattened nature of the specimen. 

Again, the size and shape of the specimen indicates that it is derived from a large Marsupial, although in this instance the specimen is clearly not a Macropodid, Diprotodontid or Vombatid, as these groups have a coronid process which narrows rapidly when seen in lateral view, while the coronid process of NCA X2.12 255 is broad in lateral view, something seen in only in the carnivorous Thylacoleonidae and Thylacinidae. The only Thylacoleonid likely to have been present in the area in the Late Pleistocene is Thylacoleo carnifex, which has a distinct hook upon its coronid process, something absent from NCA X2.12 255. The morphology is again consistent with the Thylacinid Thylacinus cynocephalus, a species already identified as being present at Nombe Rockshelter, and Prideaux et al. also assign this specimen to the species.

Surface scans of a partial right dentary of Thylacinus cynocephalus (NCA X2.12 255). (a) Lateral view; (b) medial view; (c) dorsal view. Prideaux et al. (2022).

A piece of bone from close to the area where the fourth molar would have been present in life was removed from NCA X2.12 255 was removed for uranium-thorium dating.

The next specimen examined, NCA Z6 13/14 316, an end portion of a long bone, identified by the presence of what are clearly recognisable as a deltoid tuberosity, pectoral crest, greater tubercle and lesser tubercles as the proximal extremity of a right humerus. The specimen has a fused epiphysis, indicating it came from an adult Animal. The proportions and size of this specimen are incompatible with it having come from anything other than a large Diprotodontid Marsupial. Furthermore, it is very similar to the right humerus of the holotype specimen of Hulitherium tomasettii, making it very unlikely that it came from any other species.

Surface scans of the proximal portion of the right humerus of Hulitherium tomasettii. (a)–(c) NCA Z6 13/14 316 (Nombe rockshelter), cranial, caudal and proximal views. (d)–(f) PNGMR 25063 (Pureni Swamp, holotype, reversed), cranial, caudal and proximal views. Gt, greater tubercle; Lt, lesser tubercle; Pec, pectoral crest; Ba, fossa form. brachialis; Del, deltoid tuberosity; Bg, bicipital groove; H, humeral head. Prideaux et al. (2022).

A sample of bone was taken from this specimen for uranium-thorium dating.

Specimen NCA X2.12 250 is another fragment of a long bone, on this occasion heavily abraded and showing signs of having been gnawed at by a rodent. One end of this specimen has what appear to be the remains of a large, inverted process, which makes it likely that it is a fragment of ulna. The specimen has what appears to be a large styloid process, something characteristic of Plio-Pleistocene Diprotodontids. The specimen is to badly preserved to be classified any more precisely, although Prideaux et al. note that its size is compatible with it being derived from Hulitherium tomasettii, the only confirmed Diprotodontid species at the site. 

Surface scans of a distal ulna fragment of Hulitherium sp. cf. Hulitherium tomasettii (NCA X2.12 250) in three views (a)–(c). Prideaux et al. (2022).

Specimen NCA A1:6 18 measures 122 mm x 51 mm, and is broken at either end, indicating that it is a fragment of a much larger bone. The fragment is roughly triangular in cross-section at one end, with slightly convex edges, but changes about half-way along its length into a thickened-planar shape. One face of the triangular section has an articular facet, while the planar section has an attachment for a large muscle or ligament. This general morphology is consistent with the middle portion of a right ilium, with the thickened planar section being the caudodorsal iliac spine and the scarred area the sacral surface. 

The size of this specimen implies a large Marsupial. An origin from a member of the Vombatidae can be ruled out, as the ilium of large Wombats is rounded with a dorsally twisted iliac spine. Similarly, the Palorchestidae (large Diprotodontids) can be excluded, as these Marsupials have a broad, triangular iliac spine and a distinctive projected rectus tubercule. The presence of an iliac spine rules out other Diprotodontid groups, as well as the Thylacoleonidae. 

The general morphology of the bone is consistent, however, with it having come from a Macropodid, although most large members of this group have a lateral projection on the iliac spine, which NCA A1:6 18 lacks. This absence is found in members of the genus Protemnodon, an extinct genus closely related to Grey Kangaroos, but thought to have resembled large, robust Wallabies.

Two members of the genus Protemnodon have previously been described from Nombe, Protemnodon tumbuna, and 'Protemnodon' nombe; although 'Protemnodonnombe has recently been shown not to be closely related to other species assigned to the genus, and renamed Nombe nombe. This being the case, Prideaux et al. assign specimen NCA A1:6 18 to Protemnodon tumbuna.

Surface scans of a proximal ilium fragment of Protemnodon tumbuna (NCA A1:6 18). (a) Lateral view; (b) medial view. Prideaux et al. (2022).

Specimen NCA M71 9 is another section of long bone, in this case curved and with three articular facets set into one side, roughly a fifth of the way along the shaft. This specimen is roughly 130 mm long and 32 mm thick, and is split into two fragments. The proportions and morphikigyof this bone are consistent with is being a Mammalian limb-bone, and its possession of a shaft which extends beyond the articular facets marks it out as the ulna of a Marsupial, with the position of those facets indicating it is a right ulna. The bone probably came from a juvenile, as the olecranon process lacks a fused proximalepiphysis.

The specimen lacks the outward deflected ventral margin of a Thylacine ulna, and the robust nature and large olecranon process of a Wombat, nor the robust nature and enlarged oronoid process, of the Diprotodontid Thylacoleo carnifex. The bone does, however, fit well with the expected proportions of a large Macropodid, and in particular with members of the genus Protemnodon. Two species of Protemnodon are known from the Late Pleistocene of New Guinea, Protemnodon otibandus and Protemnodon tumbuna. Prideaux et al. believe the specimen is most similar to Protemnodon tumbuna, a species already known from the Nombe assemblage, and that NCA M71 9 is therefore highly likely to be another example of that species.

Partial left ulna of Protemnodon tumbuna (NCA M71 9). (a) Cranial (dorsal) view; (b) lateral view; (c) medial view. Prideaux et al. (2022).

A second specimen, NCA X2.13 241, also appears to be a Macropodid right ulna. This is loosely similar to NCA M71 9, but smaller, and has a fused proximal epiphysis, indicating that it is from an adult. Since this adult specimen is smaller than the juvenile NCA M71 9, it is unlikely to be another specimen of Protemnodon tumbuna, nor does it bear any obvious similarity to any other Macropodid known from the Late Pleistocene of Papua New Guinea for which the ulna is known. The only other Macropodid from the Nombe assemblage is Nombe nombe, which was described from cranial material only, with no known post-cranial elements. It is quite possible that NCA X2.13 241 represents the ulna of this species, but until more complete specimens are found, there is no way to be certain of this.

Surface scans of a partial right ulna of Macropodinae gen. et sp. indet. (NCA X2.13 241). (a) Cranial (dorsal) view; (b) lateral view; (c) medial view. Prideaux et al. (2022).

A third specimen, NCA H71 9, appears to be another Macropodid ulna, this time the left. This specimen is broken into two segments. The specimen is very similar to specimens of Protemnodon, although not similar enough to specimens of Protemnodon tumbuna to be assigned to that species. It is also close enough to NCA X2.13 241 that is is likely to be an adult member of the same species, for which reason Prideaux et al. have decided not to make any taxonomic assessment of this specimen at this time.

Surface scans of a partial left ulna of Macropodinae gen. et sp. indet. (NCA H71 9). (a) Cranial (dorsal) view; (b) lateral view; (c) medial view. Prideaux et al. (2022).

The final specimen examined, NCA X2.13 249, is a collection of small bones, interpreted as a left capitatum magnum, a left trapezoid, a left  scaphoid,  a probable pisiform  fragment, and a  distal  phalanx. These appear to be from a moderately large Marsupial, and probably a ground-dwelling Macropodid.

Five manual elements referable to Macropodinae gen. et sp. indet. (NCA X2.13 249). Prideaux et al. (2022).

Uranium-thorium dating can only provide a minimum age for a specimen, as, uranium can seep into a specimen shortly after death, it can also enter the same specimen at later stages, effectively overwriting the original signal, and making the specimen appear younger than it actually is. Prideaux et al. took samples from five specimens from the Nombe assemblage for uranium-thorium dating, chosen for their preservation state, and taxonomic identifiability. 

These were part of a tooth from a mandible assigned to the Thylacine, Thylacinus cynocephalus, a section of bone taken from the humerus assigned to the Diprotodontid Marsupial, Hulitherium tomasetti, a piece of bone taken from the ilium assigned to the Macropodid, Protemnodon tumbuna, and three fragments of ulna, one from the specimen of Protemnodon tumbuna, and the two from unknown Macropodids.

Three separate dates were obtained from different sections of the Thylacine tooth, these being 126 700, 134 100, and 136 800 years before the present, i.e. all comfortably before the arrival of Humans on New Guinea.

The specimen from the Diprotodontid Marsupial, Hulitherium tomasetti, was dated to 54 600 years before the present, around the time Humans are thought likely to have arrived in the area.

The ilium assigned to the Macropodid, Protemnodon tumbuna, could not be assertained.

The three Macropodid ulnas, however, produced much younger dates, with the specimen assigned to Protemnodon tumbuna producing a date of 25 100 years before the present, and the two unidentified specimens producing dates of 22 300, and 27 200 years before the present, after the arrival of Humans in the area.

Collagen fingerprinting (a technique which seeks to identify specimens from their collagen content, the exact molecular structure of collagen being species specific) was carried out on 163 unidentified bone samples from Nombe. Of these, 26 were identified, three as Diprontodontids and 23 as Macropodids. Notably, the three Diprontodontids came from the same strata as Macropodid ulnas, indicating that these Animals were also present after the arrival of Humans.

A pollen analysis of the deposits suggests that these Animals lived in a forested environment dominated by Southern Beach, Nothofagus sp., trees, with abundant Mosses, Tree Ferns, Ferns, and other Pteridophytes, but very few Grasses. This type of environment is still found in New Guinea today, at altitudes of between 600 and 3100 metres above sealevel. The site seems to have been in an area of relatively undisturbed, which is consistent with the low level of archaeological material present, suggesting the area was only infrequently visited by Humans.

The oldest signs of Human activity at Nombe, including stone tools and charcoal, significantly predate the youngest specimens of at least two Megafaunal species, Protemnodon tumbuna and another, unknown, Macropodid, with another Megafaunal Marsupial, Hulitherium tomasettii, present at around the time Humans are thought to have appeared in the area. 

Waisted blade found in basal Stratum D1 orStratum D3 from crack in Unit M71. D Markovic in Prideaux et al. (2022).

Historically, the identification of Marsupial remains at archaeological sites has relied almost exclusively on cranial and dental material. The study of a wider range of material at sites such as Nombe clearly has the potential to identify a greater range of taxa, enabling a better understanding of the fauna associated with these sites. 

Of the species identified at Nombe from their postcranial remains, Thylacinus cynocephalus and Protemnodon tumbuna had previously been identified from cranial material, but Hulitherium tomasettii had only been recorded as a 'Pig-sized Diprotodontid'. The Macropodid Nombe nombe may also be represented by postcranial remains at the site, as it is the most likely source of the unidentified Macropodid ulnas, but this is impossible to confirm at this time. Collagen fingerprinting also appears to have considerable potential for the identification of fragmentary bones in archaeological material.

Uranium-thorium dates obtained from Megafaunal Macropodid remains at Nombe suggest that these Animals were still present here 30 000 years after the arrival of Humans on Sahul, although it is worth remembering that this method can produce dates substantially younger than the true age of a fossil. However, these bones are stratigraphically above the oldest tools, which does support the proposition that they are younger. Prideaux et al. suggest that a definite resolution of this matter would require a careful re-excavation of the site, with the deployment of multiple dating methods to all excavated material of biological material, as well as flowstones separating the layers, as well as detailed studies of all bones, artefacts, charcoal, pollen, and sediments. 

The Clogg's Cave site in eastern Victoria State, Australia, produced Megafaunal Macropodid remains which were, until recently, thought to be of a relatively young age, but which have now, by careful re-examination of the site, been shown to be about 45 000 years old. Prideaux et al. believe such an approach should also be applied to the Nombe Rockshelter, as well as to other places showing late Megafaunal survival, such as Seton Rockshelter on Kangaroo Island, and the sites of the Willandra Lakes region.

Records of early Human (and Hominin) settlement of the interior highlands of Papua New Guinea are rare, although a series of archaeological sites in the Ivane Valley suggest that areas between 1900 and 2000 m above sealevel were being visited by 45 000 years ago. There is evidence for the consumption of starch-rich tuberous Plants and the leaves and nuts of Pandanus Palms, as well as burning in the Kosipe Swamp. Other intra-montane valleys along the highland spine of New Guinea, although these are generally not well dated, and only two sites, in the Upper Wahgi Valley and Upper Baliem Valley, show signs of Human activity which can be confidently dated to more than 30 000 years ago.

The Nombe Rockshelter is in an area which appears to have been dominated by Montane (Nothofagus) Beech forests, showing little sign of large-scale disturbance, human or otherwise, before the Early Holocene, something which fits with the very low number of pre-Holocene tools found. A very low Human population density with a low frequency of visits to the area would explain the ability of Magafauna to survive in the area till around 25 000 years ago.

This raises the possibility that pockets such Megafauna may also have survived in other remote and rugged environments in Sahul, if such environments were not favoured by early Human settlers, and were visited only seldomly. Other research has shown that in the nearby Sunda Islands the local Megafauna also survived for an extended period after the arrival of Modern Humans. This has been explained by the presence of earlier Hominids on the islands, something which would have given the local fauna an opportunity to adapt to Human-like behaviour before the arrival of Modern Humans. No direct evidence of earlier Hominins has ever been found on Sahul, but inferences from genetic data have been used to suggest that New Guinea may have been settled by Denisovans, an archaic Human group, before the arrival of fully Modern Humans, and Prideaux et al. suggest that this might have given the wildlife there a degree of resilience to Human behaviour. 

Current evidence from the Nombe Rockshelter suggests that some elements of the Sahul Megafuana may have survived on New Guinea for tens of thousands of years after the arrival of Modern Humans, at least in areas where the environment was considered less than favourable by those Humans, and which were subsequently visited infrequently. However, the dating of this site is still less than perfect, and further, and more complete, investigations of the site are needed before the late dates for the Megafauna can be confirmed.

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Friday, 26 June 2020

Carbon Dioxide emissions from the Central Atlantic Magmatic Province, and their implication for the End-Triassic Extinction.

Volatile elements affect the behaviour of magmas during their rise through the crust, and control the timing and energy of volcanic eruptions. When rapidly released into the atmosphere, volcanic gases such as carbon monoxide, carbon dioxide, methane, sulphur dioxide, hydrogen sulphide, hydrochloric acid, and chloromethane, can have a devastating impact on the global climate and biota. The best example from the geologic record is the emplacement of large igneous provinces, which are synchronous with several major Phanerozoic mass extinctions, indicating large igneous provinces as potential triggers of global-scale climatic and environmental changes via the release of volatiles. Large igneous provinces, often volumetrically dominated by continental flood basalts, are exceptional intraplate magmatic events involving huge magma volumes (up to 10 million cubic kilometres), that are emplaced episodically, leading to a pulsed release of their volatile phases. This potentially results in rapid rise of atmospheric carbon dioxide and global climate warming.

In addition to perturbing the climate, volcanic carbon dioxide plays a key role in the storage, ascent and eruption of magma, and drives the stability and evolution of magma reservoirs, regulating flood basalt magmatism and associated degassing fluxes. The importance of exsolved volatile phases (e.g., carbon dioxide-rich fluids) is highlighted by recently developed models of magmatic plumbing systems. In these new models, magma reservoirs are dominated by a crystalline mush, forming a multi-phase (i.e., solid, liquid and gas) system in which crystals, melt, and exsolved volatiles can interact and ascend independently towards the surface. Due to the low solubility of carbon dioxide in silicate melts, exsolution of carbon dioxide-rich fluids from melts occurs deep in the crust (i.e., within magmatic plumbing system) or even in the upper mantle, whereas at shallow depths the fluids typically become more water-rich. Since the exsolution of carbon dioxide changes the physical properties (e.g., density, viscosity and buoyancy) of magmas, it may therefore play a crucial role in their ascent, and could explain the pulsed eruptive style observed for large igneous provinces. However, direct evidence of carbon dioxide abundance in the deep magmas of large igneous provinces is lacking.

In a study published in the journal Nature Communications on 7 April 2020, Manfredo Capriolo and Andrea Marzoli of the Department of Geosciences at the University of Padova, LĂ¡szlĂ³ Aradi of the Lithosphere Fluid Research Lab at Eötvös LorĂ¡nd University, Sara Callegaro, also of the Department of Geosciences at the University of Padova, and of the Centre for Earth Evolution and Dynamics at the University of Oslo, Jacopo Dal Corso, Robert Newton, Benjamin Mills, and Paul Wignall of the School of Earth and Environment at the University of Leeds, Omar Bartoli, again of the Department of Geosciences at the University of Padova, Don Baker of the Department of Earth and Planetary Sciences at McGill University, Nasrrddine Youbi of the Department of Geology at Cadi Ayyad University, the Instituto Dom Luiz at the University of Lisbon, and the Faculty of Geology and Geography at Tomsk State University, Laurent Remusat of the MusĂ©um National d’Histoire Naturelle, Richard Spiess, once again of the Department of Geosciences at the University of Padova, and Csaba SzabĂ³, also of the Lithosphere Fluid Research Lab at Eötvös LorĂ¡nd University, investigate the history of volatiles in the magmas of the Central Atlantic Magmatic Province, of Earth’s largest large igneous provinces, by analysing volatiles in melt inclusions, particularly carbon dioxide.

Capriolo et al. examine the implications of these findings for magma eruption history and subsequent impact on the global climate. The emplacement of the Central Atlantic Magmatic Province (with (peak activity at 201.6–201.1 million years ago) occurred during the early stages of the Pangaea supercontinent break-up, leading to the opening of the Central Atlantic Ocean, and is synchronous with the End-Triassic Extinction, one of the five most severe biotic crises during the Phanerozoic. At least 3 million cubic kilometres of Central Atlantic Magmatic Province basaltic magmas were erupted or intruded into the continental crust over an area of 100 million square kilometres in brief pulses, from a few centuries to a few millennia each, characterised by high eruption rates. Such short and powerful eruptions may have had a severe impact on global climate by limiting the time in which negative feedback processes, such as the weathering of calcium-magnesium silicates, can abate warming and acidification. Central Atlantic Magmatic Province magmatism coincided in time with three marked negative carbon isotope excursions bracketing the main extinction period, and with an inferred strong rise of atmospheric carbon dioxide. In general, the pulsed magmatic and degassing activities of large igneous provinces can cause a rapid rise of atmospheric carbondioxide and greenhouse conditions, which are reflected by rapid carbon¹³ negative excursions recorded in both organic matter and carbonates, testifying to a global perturbation of the exogenic (i.e., superficial) carbon cycle. A rapid input of carbon¹³-depleted volatile phases into the atmosphere–hydrosphere system is possibly triggered by the emission of volcanic carbon dioxide, enhanced by the emission of carbon dioxide and methane derived from the thermal metamorphism of intruded organic matter-rich sediments.

Capriolo et al. screened a suite of over 200 intrusive and effusive samples from Central Atlantic Magmatic Province basaltic lava flows and sills in North America (USA and Canada), Africa (Morocco) and Europe (Portugal), and combined several in situ analytical techniques to investigate the presence of carbon dioxide within melt inclusion bubbles and constrain their formation depth. Capriolo et al.'s multidisciplinary analytical approach reveals that gas exsolution bubbles trapped in melt inclusions are a previously unappreciated direct proxy of volatile species degassed during large igneous province magmatic activity. In the case of the Central Atlantic Magmatic Province, Capriolo et al.'s analysis confirms the abundance of carbon dioxide (up to 10 000 gigatonnes of volcanic carbon dioxide degassed during Central Atlantic Magmatic Province emplacement) and indicates that at least part of this carbon has a middle- to lower-crust or mantle origin, suggesting that Central Atlantic Magmatic Province eruptions were rapid and potentially catastrophic for both climate and biosphere.

Map of Central Atlantic Magmatic Province in central Pangea at about 200 million years ago. The black symbols indicate the provenance of the studied samples: triangle for Portugal, circle for Morocco, square for New Jersey, USA, and diamond for Nova Scotia, Canada. Capriolo et al. (2020).

About 10% of the over 200 investigated intrusive and effusive Central Atlantic Magmatic Province basaltic rocks show gas exsolution bubble-bearing melt inclusions, hosted mainly in clinopyroxene and occasionally in plagioclase, orthopyroxene and olivine. The studied Central Atlantic Magmatic Province basaltic rocks are mainly porphyritic and microcrystalline, and the principal mineral phases are labradoritic-bytownitic plagioclase, augitic (abundant) and pigeonitic (scarce) clinopyroxene, rare magnesium-rich orthopyroxene, and rare and mostly altered magnesium-rich olivine. As accessory mineral phases, magnetite is common, while ilmenite is rare. In effusive rock samples (from USA, Canada, Morocco and Portugal), glomerocrystic aggregates of augitic clinopyroxene and plagioclase are commonly present, and are interpreted as clots of partially crystallised mineral mush from the transcrustal magmatic plumbing system. In the only studied intrusive sample (from Palisades sill, USA), olivine is abundant and usually well preserved.

Representative analysed samples at transmitted light optical microscopy. (a) Porphyritic and microcrystalline texture with phenocrysts of clinopyroxene and plagioclase (Cpx and Pl; sample NEW31, New Jersey, USA). (b) Glomerocrystic aggregate of clinopyroxene (Cpx; sample NEW31, New Jersey, USA). (c) Large phenocryst of plagioclase (Pl; sample AN156A, Morocco). (d) Crystals of plagioclase, clinopyroxene and well-preserved olivine (Pl, Cpx and Ol; sample NEW136B, New Jersey, USA). Capriolo et al. (2020).

Melt inclusions are nearly ubiquitous in glomerocrystic aggregates of clinopyroxene and plagioclase. The bubble-bearing melt inclusions usually have irregular shapes, can be singleor multi-bubble melt inclusions, and contain up to 25 bubbles per inclusion, displaying a large range of glass/bubble ratios even within the same host crystal or crystal clot (i.e., there is no proportionality between the volume of glass and the volume/number of bubbles). In detail, the estimated volume fraction of bubbles within each melt inclusion ranges from less than 0.1 to more than 0.5 approximately. Moreover, melt inclusions present a great variability in size, approximately from 5 to 50 μm on the principal axis. Bubbles within them usually have spherical shape and generally range from 1 to 15 μm in diameter. Sometimes bubbles are aggregated in the melt inclusions, probably due to post-entrapment coalescence. Some melt inclusions are partially crystallised, containing μm-sized daughter minerals in addition to, or instead of, bubbles. These crystals, likely formed from the melt after the entrapment, are mainly opaque mineral phases, such as sulphides and oxides (e.g., magnetite). The melt inclusion glass has a more silicic (mainly andesitic) and more differentiated composition compared to the host basaltic rocks, and is clearly different from typical Central Atlantic Magmatic Province basalts or basaltic andesites. The melt inclusion glass is generally enriched in silicon dioxide and aluminium oxide, and depleted in iron oxide, magnesium oxide, and calcium oxide compared to the host rocks, and would correspond to a residual melt after fractionation of about 40%vaugitic clinopyroxene, 10% plagioclase and 5% magnetite from a typical Central Atlantic Magmatic Province basalt. Such differentiation can only partly be due to post-entrapment crystallisation of the few tiny crystals within the melt inclusions or of the host clinopyroxene, which displays constant augitic composition, shows only faint chemical zonation towards the glass, and is substantially out of equilibrium with it. The most evident compositional zoning of the host clinopyroxene consists of a decrease in calcium oxide content and a slight increase in both magnesium oxide and iron oxide content close to the contact with the melt inclusions. Hence, the local thin rim around the melt inclusions of slightly calcium-depleted and iron and/or magnesium-enriched clinopyroxene suggests the probable presence of augite–pigeonite exsolution lamellae close to the boundary of melt inclusions, which likely formed at subsolidus conditions from an intermediate composition clinopyroxene that crystallized from the entrapped melt (i.e. post-entrapment crystallisation). However, the chemical disequilibrium between the melt inclusion glass and the host clinopyroxene, and the lack of significant chemical zoning within the host clinopyroxene at the contact with melt inclusions are not consistent with substantial diffusive re-equilibration within the host clinopyroxene and suggest a rapid cooling after melt entrapment. This indicates that a previously differentiated bubble-bearing melt was entrained between interstices of growing crystals, and rapidly cooled down, forming melt inclusions.

Representative single- and multi-bubble melt inclusions at transmitted light optical microscopy. The black arrows indicate the bubble-bearing melt inclusions. (a) Multi-bubble melt inclusions characterised by a highly variable range in bubble size, hosted in augitic clinopyroxene (Cpx; sample NS12, Nova Scotia, Canada). (b) Coalescent bubbles within melt inclusion, hosted in augitic clinopyroxene (Cpx; sample AN18, Morocco). (c)-(f) Single- and multi-bubble melt inclusions hosted in augitic clinopyroxene (Cpx) at increasing depth in the same crystalline aggregate, displaying different ratios between the volume of glass and the volume/number of bubbles (sample NS9, Nova Scotia, Canada). Capriolo et al. (2020).

The bubbles within melt inclusions were investigated in all the samples by confocal Raman microspectroscopy looking for carbon species (carbon monoxide, carbon dioxide, methane and elemental carbon), as well as for other important volatile compounds in volcanic systems (sulphur dioxide, hydrogen sulphide and water). In almost all analysed bubbles, carbion dioxide (within 54 bubbles of 9 samples) or elemental carbon (within 41 bubbles of 2 samples) were detected in both single- and multibubble melt inclusions of rock samples collected from all over the Central Atlantic Magmatic Province. In detail, Raman spectra show that carbon dioxide in Central Atlantic Magmatic Province bubbles is characterized by low density (roughly 0.1 g/cm³), and elemental carbon in Central Atlantic Magmatic Province bubbles is characterized by low crystallinity (i.e. it is present as disordered graphite and amorphous carbon). Carbion dioxide concentrations from 0.5 to 1.0 percent by weight in whole melt inclusions (i.e. glass plus bubbles) were calculated from the density of gaseous carbon dioxide within the bubbles and from the estimated volume fraction of these bubbles within melt inclusions. Other volatiles such as carbon monoxide, methane, sulphur dioxide and hydrogen sulphide were not detected, while water was often found within the glass of melt inclusions, but never in the bubbles. The melt inclusion glass, investigated through nanoscale secondary ion mass spectrometry, contains about 0.5–0.6 percent by weight water and 30–90 parts per million carbon dioxide.

Chemical maps of glomerocrystic clinopyroxene aggregates. Backscattered electrons image (a) and corresponding scanning electron microscopy with energy-dispersive X-ray spectroscopy maps (b)–(f) of a thin section area including melt inclusions and the hosting glomerocrystic clinopyroxene aggregates. In the backscattered electrons image image the brighter portions of clinopyroxene have augitic (Aug) composition and the darker ones have pigeonitic(Pgt) composition. In the scanning electron microscopy with energy-dispersive X-ray spectroscopy maps the brighter regions correspond to higher concentrations of the analysed element. These maps were acquired on sample NEW31 (New Jersey, USA). The scale bar is shown in (a). (a) Backscattered electrons image, (b) aluminium map, (c) calcium map, (d) iron map, (e) magnesium map, and (f) titanium map. Capriolo et al. (2020).

The analysed bubble-bearing melt inclusions strongly suggest that the Central Atlantic Magmatic Province magmatic system was rich in carbon dioxide. Most of the analysed bubbles contains carbon dioxide or, less frequently, elemental carbon, and no detectable amounts of any other investigated volatile phase. In particular, confocal Raman microspectroscopy allowed Capriolo et al. to distinguish and characterize both carbon dioxide and elemental carbon. The Raman spectrum of carbon dioxide is characterised by two sharp bands, usually called Fermi diad or Fermi doublet, associated to two symmetrical weak bands, usually called hot bands. Instead, the first-order Raman spectrum of elemental carbon is characterised by two different bands, the composite D band, activated in disordered graphite by lattice defects and typical of non-crystalline structures. and the single G band, typical of graphite. This last band was employed by Capriolo et al. in a crossplot to characterise the different types of elemental carbon, distinguishing disordered graphite and amorphous carbon Interestingly, carbon dioxide and elemental carbon within gas exsolution bubbles are never present together in the same samples. The elemental carbon, which is likely present as a thin film coating the inner spherical surface of the bubbles, replaces carbon dioxide in some samples, probably due to a change in the oxidation state within melt inclusions, for instance related to a diffusive loss of oxygen from the bubbles to the melt, when the latter crystallized oxides during cooling. The large variability in volume and number of bubbles observed in coexisting MIs (ranging from 1 to 25 bubbles per melt inclusion, approximately occupying from less than 0.1 to over 0.5 of the melt inclusion volume, as optically estimated in thin and thick sections) reveals heterogeneous entrapment of melt inclusions. Therefore, the bubbles within melt inclusions are interpreted as gas exsolution bubbles, formed during exsolution of a carbon dioxide-rich fluid phase likely from the silicate melt prior to, or during, their entrapment. Gas exsolution within melt inclusions after melt entrapment was probably of minor importance, particularly for melt inclusions with large bubbles, because the trapping of a bubble-free melt would have produced homogeneous melt inclusions, displaying very similar glass/bubble ratios, which were not observed in this study. The volatile-saturated melt and the volatiles may have a cogenetic origin (i.e., the melt was entrapped along with volatiles immediately after, or during, gas exsolution), or may have different origins (i.e., the melt was entrapped along with volatiles exsolved from deeper magmas, or degassed and fluxed from intruded crustal rocks).

Bubble-bearing melt inclusions at transmitted light optical microscopy and confocal Raman microspectroscopy. Left column: transmitted light photomicrographs at optical microscope of the analysed areas, bordered by dotted lines. Right column: Raman hyperspectral maps of the corresponding areas. (a), (c), (e) Photomicrographs of elemental carbon-bearing single- and multi-bubble melt inclusions (a) and (c) sample NEW31, New Jersey, USA; (e) sample AN39, Morocco. (b), (d), (f) Raman hyperspectral maps of the same samples area. (g) Photomicrograph of an irregular-shaped carbon dioxide-bearing multi-bubble melt inclusion, sample NS12, Nova Scotia, Canada. (h) Raman hyperspectral map of the same sample area. The Raman signal of carbon dioxide is weak due to its low density. However, spot analyses confirmed the presence of carbon dioxide in all bubbles. Capriolo et al. (2020).

Clinopyroxene compositions and volatile element concentrations suggest that carbon dioxide entrapment occurred within the deep magmatic roots of Central Atlantic Magmatic Province. The pressure of crystallisation of host clinopyroxene crystal clots can be calculated from mineral compositions using methods developed for magmatic systems, The geothermobarometer based on the equilibrium between clinopyroxene and a magmatic liquid was applied using whole rock composition as proxy for the original magmatic liquid composition, because the melt inclusion glass is in chemical disequilibrium with the host clinopyroxene. The calculated crystallization pressure ranges from 0.1 to 0.7gigapascals (at temperatures from 1150 to 1230°C) and is consistent with previous estimates from clinopyroxene crystallisation pressures (from 0.2 to 0.8 gigapascals) in basalts from the entire Central Atlantic Magmatic Province. These results suggest that the crystallisation of clinopyroxene in the investigated Central Atlantic Magmatic Province samples occurred predominantly within the middle continental crust (on average 12 km for a pressure/depth gradient of about 0.03 gigapascals/km). The deep origin of melt inclusions is consistent with observed volatile concentrations in both their glass and bubbles. The presence of sulphides within some melt inclusions shows that the entrapped melt became sulphide-saturated with sulphur concentrations likely exceeding 1500 parts per million. Sulphur concentrations of the same order of magnitude were estimated for Central Atlantic Magmatic Province basalts. Moreover, about 0.5–0.6 percent by weight water was detected in the melt inclusion glass through nanoscale secondary ion mass spectrometry analysis, revealing hydrated conditions for these melts. Despite the presence of water and sulphur in the melt inclusion glass, these volatiles were not detected in the bubbles. Hence, considering a realistic maximum primary concentration of about 1 percent by weight water and ca. 0.1 percent by weight sulphur dioxide in tholeiitic within-plate basaltic melts, most water and sulphur dioxide are expected to exsolve at pressures lower than 0.1 gigapascals (i.e. less than 3 km depth). Even considering that hydrogen ions may move from the bubbles into the glass, and carbon dioxide from the glass into the bubbles after melt inclusion entrapment, the observed distribution of volatile species between glass and bubbles within melt inclusions suggests the dominant occurrence of gas exsolution and bubble formation at relatively high pressures from a carbon dioxide-rich melt.

The inferred depth of carbon dioxide exsolution and entrapment indicates that this volatile species has a deep origin (at least 12 km on average). It therefore reveals that the entire carbon dioxide budget involved in Central Atlantic Magmatic Province emplacement could not have originated exclusively from assimilation and degassing of shallow intruded sediments, because sediments in the circum-Atlantic basins only reach a thickness of 5 km in eastern North America and less than 1 km in Morocco and Portugal. On the contrary, at least part of the carbon dioxide most probably derived from assimilation of deep to middle-crustal metasedimentary rocks (e.g. metacarbonates or graphite-bearing amphibolites/granulites) or from the mantle source of the Central Atlantic Magmatic Province basalts, containing significant amounts of recycled sedimentary material.

Sketch of the transcrustal plumbing system of Central Atlantic Magmatic Province basaltic magmas from the mantle to the surface. The evolution of basaltic magmas occurs at variable depth by crystallisation of minerals, which then form aggregates in crystalline mushes and entrain bubble-bearing melt, forming melt inclusions. Different volatile species exsolve at variable depth. In particular, carbon dioxide-rich fluids (white bubbles) start exsolving at great depth, whilst water-rich fluids (blue bubbles) and S-rich fluids (yellow bubbles) start exsolving at shallow depth. The black dashed arrows indicate the potential sources for the carbon inCentral Atlantic Magmatic Province magma: the mantle, the deep crust and the Palaeozoic or Triassic sedimentary basins in which Central Atlantic Magmatic Province sills intruded. The carbon within the studied melt inclusions derives from the deep sources as demonstrated with clinopyroxene geobarometry data. Capriolo et al. (2020).

The calculated depth of entrapment (roughly 12 km) allows an estimation of the carbon dioxide concentration originally present in Central Atlantic Magmatic Province magmas. The carbon dioxide saturation in basaltic melts is achieved at about 1000 parts per million at 0.2 gigapascals, increasing by ca. 500 parts per million for each 0.1 gigapascals. Considering the calculated crystallisation depths, the minimum estimate for the carbon dioxide concentration of Central Atlantic Magmatic Province magma, before gas exsolution, is between about 500 and 4000 parts per million. Such values are consistent with the carbon dioxide concentrations in the melt inclusions, calculated from carbon dioxide density within the bubbles, which range from 0.5 to 1.0 percent by weight. Moreover, starting from the minimum calculated values of the carbon dioxide concentration within melt inclusions (i.e. 0.5–0.6 percent by weight) as representative of Central Atlantic Magmatic Province magma, assuming an average density of 2.90 g/cm³ for basaltic rocks and considering 5–6 million km³ for the total volume of Central Atlantic Magmatic Province (in order to take into account the deep plumbing system), the total amount of degassed volcanic carbon dioxide during Central Atlantic Magmatic Province mplacement would be up to 100 000 gigatonnes. Interestingly, the values estimated for the carbon dioxide concentration of Central Atlantic Magmatic Province magma (0.5–1.0 percent by weight) and for the total amount of degassed volcanic carbon dioxide during Central Atlantic Magmatic Province emplacement (up to 100 000 gigatonnes) are consistent with those assessed in several other large igneous provinces, using different approaches

The high-volume fractions of carbon dioxide and elemental carbon-bearing bubbles within Central Atlantic Magmatic Province melt inclusions, along with the inferred depths of formation, reveal the high abundance (0.5–1.0 percent by weight) of carbon dioxide in the Central Atlantic Magmatic Province transcrustal magmatic plumbing system. The carbon dioxide-bearing bubbles identified in Central Atlantic Magmatic Province melt inclusions can be interpreted as batches of ascending volatiles entrapped in crystalline mush shortly prior to its mobilization and prior to eruption. This evidence for carbon dioxide saturation in the basaltic magmas at depth can explain the pulsed eruptive style of Central Atlantic Magmatic Province, where carbon dioxide acts as propellant for magma ascent, causing rapid and violent eruptive pulses. For instance, carbon dioxide-rich Hawaiian basalts have been shown to rapidly rise from over 5 km depth and to cause high fountaining eruptions. 

The presence of large amounts of carbon dioxide-bearing bubbles, the pulsed eruption and the efficient degassing of carbon dioxide from the basaltic magmas, strengthens the role of Central Atlantic Magmatic Province in triggering end-Triassic extreme greenhouse conditions The rate of volatile release plays a fundamental role in determining the severity of the surface environmental response; more rapid release increases the maximum transient concentration of atmospheric carbon dioxide and the subsequent severity of any environmental cascade. Assuming 0.5–1.0 percent by weight carbon dioxide in Central Atlantic Magmatic Province basalts, as suggested by the average carbon dioxide density and most common glass/bubble ratio within melt inclusions, and considering its efficient rise to the atmosphere through the magmatic transcrustal roots, it is possible that just a single Central Atlantic Magmatic Province volcanic pulse may have severely affected the end-Triassic climate. In fact, a single short-lived Central Atlantic Magmatic Province magmatic pulse (roughly  100 000 km³ erupted over 0.5 thousand years may emit about the same total amount of projected anthropogenic carbon dioxide emissions over the 21st century, according to the Representative Concentration Pathway 4.5 (a Representative Concentration Pathway is a greenhouse gas concentration trajectory adopted by the Intergovernmental Panel on Climate Change; four pathways were used for climate modeling and research for the Intergovernmental Panel on Climate Change Fifth Assessment Report in 2014.). This scenario for rapid carbon dioxide emissions predicts a global temperature increase of about 2 °C and an oceanic pH decrease of about 0.15 units over 100 years, and suggests that the end-Triassic climatic and environmental changes, driven by carbon dioxide emissions, may have been similar to those predicted for the near future.

See also...

https://sciencythoughts.blogspot.com/2020/06/ptychites-embreei-new-species-of.htmlhttps://sciencythoughts.blogspot.com/2020/03/dynamosuchus-collisensis-new-species-of.html
https://sciencythoughts.blogspot.com/2019/10/pseudotherium-argentinus-possible.htmlhttps://sciencythoughts.blogspot.com/2019/08/clevosaurus-hadroprodon-new-species-of.html
https://sciencythoughts.blogspot.com/2019/07/first-discovery-of-horsetail.htmlhttps://sciencythoughts.blogspot.com/2019/05/pachypleurosaurs-from-triassic-of.html
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Friday, 19 June 2020

Methylmercury poisoning as a possible cause of the end-Devonian Mass Extinction.

The end-Devonian was a time of significant changes in the global climate and biosphere, including the biodiversity crisis known as the Hangenberg Event. This event occurred roughly. 13.5 million years after the Frasnian-Famennian Mass Extinction, and was linked with globally widespread deposition of the anoxic Hangenberg Black Shale. The Hangenberg Extinction (with 50% marine genera loss) significantly affected the pelagic realm, especially Ammonoids, Conodonts, many Vertebrates, and benthic reef biotas, such as Trilobites and Ostracods, and had an ecological impact similar to the end-Ordovician Mass Extinction. Moreover, a drastic reduction of Phytoplankton diversity is also observed at the Devonian/Carboniferous boundary. Deposition of the Hangenberg Black Shale was a short-term event that lasted between about 50 and 190 thousand years, while the extended crisis interval encompassed a time span of one to several hundred thousand years. The postulated factors responsible for this global event, such as high productivity and anoxia, a calcification crisis caused by ocean acidification, perturbation of the global carbon cycle, glacio-eustatic sea-level changes driven by orbital forcing, volcanic and hydrothermal activity, and evolution of Land Plants, are still vividly discussed. In fact, extensive volcanism has been implicated in all ‘Big Five’ mass extinctions and other biotic crises in the Phanerozoic, including the Hangenberg Crisis. As the main source of mercury in the geological past was volcanic and submarine hydrothermal activity, and mercury anomalies in the sedimentary record have recently been used as a proxy for volcanic activity in relation to global events and palaeoenvironmental perturbations, including for the Devonian/Carboniferous boundary from different palaeogeographical domains.

In a paper published in the journal Scientific Reports on 30 April 2020, MichaÅ‚ RakociÅ„ski, Leszek Marynowski, and Agnieszka Pisarzowska of the Faculty of Natural Sciences at the University of Silesia in Katowice, Jacek BeÅ‚dowski and Grzegorz Siedlewicz of the Institute of Oceanology of the Polish Academy of Sciences, MichaÅ‚ ZatoÅ„, also of the Faculty of Natural Sciences at the University of Silesia in Katowice, Maria Cristina Perri and Claudia Spalletta of the Department of Biological, Geological and Environmental Sciences at the University of Bologna, and Hans Peter Schönlaub of the Commission for Geosciences of the Austrian Academy of Sciences, report very large, anomalous mercury spikes in two marine Devonian/Carboniferous successions of the Carnic Alps, supporting volcanism as the driving mechanism (ultimate cause) of the Hangenberg Event. Furthermore, They also detected methylmercury, a strong neurotoxin that bioaccumulates in the food chain, in sedimentary rocks for the first time. Thus, RakociÅ„ski et al. claim that volcanic-driven methylmercury poisoning in otherwise anoxic seas could be an another proximate (direct) kill mechanism of the end-Devonian Hangenberg extinction.

Rakociński et al. examined two successions of deep-water, pelagic sedimentary rocks, encompassing the uppermost Devonian and Devonian/Carboniferous boundary intervals: Kronhofgraben (Austria) and Plan di Zermula A (Italy) in the Carnic Alps. The Kronhofgraben and Plan di Zermula A sections consist of organic-rich Hangenberg Black Shale and micritic limestone.

Late Devonian (360 million years ago) palaeogeographic map. showing the studied localities and the location of prominent areas of Late Devonian magmatism and associated volcanism, as well as (Al) giant mercury deposits reactivated by Variscan magmatic and tectonic activity in AlmadĂ©n (Spain). RakociÅ„ski et al. (2020).

The Kronhofgraben section in the central Carnic Alps of Austria is situated in a gorge of the AĂŸnitz Creek, about 7 km east of Plöckenpass and 1 km northwest of the Kronhof Törl pass at the Austrian–Italian border. The Devonian/Carboniferous boundary beds crop out in the eastern side of the Kronhofgraben gorge at an altitude of 1390 m. The Plan di Zermula A section in the southern Carnic Alps of Italy appears on the western slope of the Mount Zermula massif, along the road from Paularo to Stua di Ramaz. Grey limestones and black shales represent the studied interval in both sections. The Hangenberg Black Shale horizon is assigned to the upper part of the Bispathodus ultimus Conodont Biozone (equivallent to the Middle-Upper Siphonodella praesulcata zones) in Kronhofgraben (40 cm thick) and in Plan di Zermula A (15 cm thick) is underlain by Cephalopod limestones of the lower part of the Bispathodus ultimus Zone (equivallent to the Upper Apsotreta  expansa- Lower Siphonodella praesulcata zones). The first carbonate bed above the Hangenberg Black Shale belongs to the Siphonodella sulcata Zone (equivallent to the Protognathodus kockeli Zone).

The Devonian/Carboniferous boundary in both sections is situated directly above the Hangenberg Black Shale. The Devonian/Carboniferous boundary may be somewhat problematic and needs redefinition (caused by problems with discrimination of Siphonodella sulcata from its supposed ancestor Siphonodella praesulcata). The new criterion for definition of the base of the Carboniferous System proposed by the Working Group on the boundary is: identification of the base of the Protognathodus kockeli Zone, beginning of radiation and top of major regression (top of Hangenberg Black Shale) and end of mass extinction. In the limestone overlying the Hangenberg Black Shale, Conodonts of the species Protognathodus kockeli were found in both sections. Therefore, the position of the Devonian/Carboniferous boundary did not changed in comparison to previous studies.

The Devonian/Carboniferous boundary successions in the Plan de Zermula A and Kronhofgraben were deposited in deeper palaeoenvironment. In the late Devonian, Carnic Alps represented the northern tips of Gondwana and belonged to the Gondwana-derived Bosnian–Noric Terrane accreted to the intra-Alpine Mediterranean terrane during the Carboniferous. The investigated rocks outcropped in the Carnic Alps reflected strong thermal alteration.

The Hangenberg Black Shale intervals in the sections investigated display extremely high mercury values, with maxima of 20216 and 9758 parts per billion in Kronhofgraben and Plan di Zermula, respectively. The Hangenberg Black Shale from the Plan di Zermula A section contains mercury anomalies that are roughly 13–100 times higher than the 100 parts per billion background, whereas in the Kronhofgraben section the anomalies are roughly 12–84 times higher than the background values.

Interestingly, significant concentrations of methylmercury were found in the whole Kronhofgraben section, where methylmercury is in the range 13–348 picograms per gram, dry weight. Additionally, we found 55 picograms per gram, dry weight of methylmercury in the Novchomok section in Uzbekistan and 72.72 picograms per gram, dry weight of methylmercury sampled from the uppermost Devonian part of the Woodford Shale from the Arbuckle Anticline in Oklahoma, USA. Traces of methylmercury were also found in the Hangenberg Black Shale interval at Kowala Quarry, Poland (20.66 picograms per gram, dry weight of methylmercury).

In comparison to methylmercury levels found in modern sediments (reaching from 1000 to 700000 picograms per gram, dry weight in polluted basins), those detected in sedimentary rocks studied, are relatively low. However, the original amounts of methylmercury in the investigated sediments would have been higher but impoverished during diagenesis. The mercury enrichments are observed in organic-rich Hangenberg equivalent intervals such as Kronhofgraben (from 0.51 to 13.28% total organic carbon) and Plan di Zermula A (from 0.7 to 12.53% total organic carbon). The values of the mercury/total organic carbon ratio in the Hangenberg Black Shale at Kronhofgraben range from 815 to 8096.5 (parts per billion/%), while the background samples show a range from 387.5 to 985 (parts per billion/%). In Plan di Zermula A, the values of mercury/total organic carbon ratios in the Hangenberg Black Shale range from 779 to 3269 (parts per billion/%) and are higher than those from the background samples (ranging from 84.5 to 676.8 parts per billion/% mercury/total organic carbon).

Volcanic and hydrothermal activities are considered to be the main sources of elevated mercury in sedimentary. Besides mercury delivery to the atmosphere by volcanic activity, other processes can produce mercury spikes in the sedimentary record, including widespread wildfires, terrestrial input, magmatic emplacement or thermogenic processes related to bolide impact rocks. Additionally, some authors have suggested that mercury enrichments can be sulphide-hosted in euxinic (high sulphur/low oxygen) facies, and high mercury spikes not necessary would be connected with volcanic activity. However, in such a case, the Hg enrichments would be well-correlated with total sulphur, which is not observed in our sections. Although extensive wildfires on land were confirmed during the Hangenberg event, based on the co-occurrence of charcoal and high concentrations of polycyclic aromatic hydrocarbons in sedimentary rocks, these, however, could have also been induced by volcanism, as evidenced by the co-occurrence of charcoals and ash layers. No conclusive evidence for bolide impact at the Devonian/Carboniferous boundary has been detected thus far. In fact, at the Devonian/Carboniferous boundary, volcanic activity has frequently been documented, mainly on the basis of the presence of ash layers below, above and within the Hangenberg Black Shale (e.g. in the Holy Cross Mountains, Iberian Pyrite Belt, and Rhenish Massif), mercury spikes, as well as the presence of abnormal or strongly altered spores (tetrads), which could reflect the mutagenic effect of regional acidification caused by explosive volcanism. The most plausible sources of very large amounts of mercury during the end-Devonian interval are the massive Magdalen silicic large igneous province and the Siberian (Yakutsk–Viluy) and/or the Kola–Dnieper large igneous provinces; however, the interval also overlaps with formation of the Almaden mercury deposit (last mineralisation pulse episodes), which constitutes one of the largest geochemical anomalies on Earth and coincided with the first phase of the Variscan Orogeny (mountain-building episode associated with the formation of the supercontinent of Pangea), as considered for the Hangenberg Crisis. According to current knowledge, three large igneous provinces encompass the Late Devonian interval (380–360 million years ago): Yakutsk-Viluy (Siberia; continental type with an area of 0.8 million km²), Kola-Dnieper (Baltica; continental type with area of 3 million km²) and Magdalen (Laurussia, continental-silic type). Moreover, RakociÅ„ski et al. cannot exclude other additional mercury sources, for instance connected with explosive eruptions which could overlap with large igneous province activity. Mercury has a strong affinity to organic matter and to a minor extent can also be associated with sulphides and clay minerals; therefore, mercury is normalized to total organic carbon content. Importantly, the mercury spikes in RakociÅ„ski et al.'s sections are also evident when normalized to total organic carbon content, which can be interpreted as an effect of increased input of mercury to the basins independently of the potential influence of reducing depositional conditions. The mercury vs. aluminium oxide correlation in the investigated successions is very weak, indicating no correlation of mercury with the clay fraction. However, mercury exhibits a good correlation with molybdenum in the all sections. This could indicate that some mercury was associated with sulphides as a result of its intensified precipitation in a sulphide-rich (euxinic) water column. In the sections investigated, mercury vs. total sulphur correlation is very weak, which does not confirm sulphides as host of mercury. However, the mercury vs. total organic carbon correlation in the Devonian/Carboniferous boundary at Novchomok section is very low, which confirm that mercury enrichments are facies independent and thus are indicative of volcanic activity during this time. For the Kronhofgraben and Plan di Zermula A sections this correlation is good, suggesting possible different sources of this element. However, as already emphasised, there are a number of lines of evidence for volcanic and hydrothermal activities, as well as widespread wildfires, during this time allowing for a firm statement that increased mercury input to the basins was connected with diverse volcanic activities and related combustion of biomass on land. Moreover, the Hangenberg Event took place during an interglacial period; therefore, some mercury could have originated from permafrost melting but even if this process had taken place, mercury would have previously accumulated in the permafrost as a result of volcanic or pyrogenic processes. To summarise, based on all the available data, RakociÅ„ski et al. state that the main sources of mercury were volcanism and related hydrothermal activities. In fact, volcanic processes are main sources of mercury in atmosphere.

Schematic model of deposition, mercury sources and mercury methylation during the Hangenberg Event. Rakociński et al. (2020).

The organic form of mercury (methylmercury) is a strong neurotoxin that is bioconcentrated in aquatic food chains and is able to cross the blood–brain barrier; thus, this form of mercury is much more toxic to living organisms than inorganic mercury. In modern environments, methylmercury is generated predominantly by anaerobic microorganisms, such as sulphate-reducing Bacteria (e.g., Geobacter sulfurreducens). Despite widespread mercury pollution, annual emissions of mercury have recently been higher from natural sources than anthropogenic ones, constituting as much as 70% of all mercury emissions. However, the concentrations of mercury detected in all the end-Devonian sections are surprisingly high, similar to the present-day mercury concentrations found in highly polluted basins, e.g., some parts of the Baltic Sea. The mercury concentrations of up to 20 000 parts per billion in Kronhofgraben and 1000–10 000 parts per billion in the Plan di Zermula A, and mercury spikes determined in Germany, south Vietnam, the Czech Republic and south China sections suggest, that global mercury concentrations were highly elevated during the Hangenberg event. This finding implies that, during favorable sedimentary conditions, very high concentrations of methylmercury can be produced on the global scale. In the investigated samples RakociÅ„ski et al. measured relatively minor amounts of methylmercury in comparison with the methylmercury levels in modern sediments. In polluted basins, concentrations of methylmercury vary from 1000 to 700 000 picograms per gram, dry weight of methylmercury and are much higher relative to total methylmercury concentration from RakociÅ„ski et al.'s sections. However, the original amounts of methylmercury in the investigated sediments would have been higher, assuming large enrichment of total mercury in anomalous samples. It is very probable that methylmercury could have been demethylated during diagenesis as a result of the common diagenetic process of demethylation, which is influenced by temperature. Because of the strong thermal alteration of the investigated rocks, the occurrence of demethylation seems to be very likely.

Therefore, regardless of the mercury source, its high level in the end-Devonian water column, subsequent trapping in sediment and biomethylation to the more toxic methylmercury form by anaerobic Bacteria, would have had an additional devastating impact on aquatic life during the Hangenberg Event. This can be produced under conditions of extended anoxia/euxinia during this time and the occurrence of rich sulphate-reducing Bacteria communities which can change mercury to its methyl form. Additionally, blooms of Green Algal phototrophs (prasinophytes) during black shale events would have contributed, mostly indirectly, to methylmercury production. However, indisputable evidence for Bacterial mercury methylation is the occurrence of notable concentrations of methylmercury in the sediments investigated and the similarities in the distributions of mercury and methylmercury in the Kronhofgraben section.

Observation of modern marine environments has confirmed that methylmercury is highly toxic to animals at higher trophic levels (such as Fish, Birds and Mammals). In this light it seems to be evident that severe extinction of marine and nonmarine Fish and Tetrapods, as well as pelagic Conodont Animals, during the Hangenberg event may also have resulted from methylmercury poisoning that could have affected different aquatic habitats. Although the effect of methylmercury on benthic invertebrates is regarded as minimal, these organisms were significantly affected by concomitant, globally widespread anoxia. Such anoxia asphyxiation–methylmercury poisoning may have also been kill mechanisms in other mass extinctions, but this should be tested by searching for traces of methylmercury in other sedimentary rocks.

See also...

https://sciencythoughts.blogspot.com/2020/06/coldwater-lamellorthoceratid.htmlhttps://sciencythoughts.blogspot.com/2020/02/resolving-age-of-middle-devonian-basin.html
https://sciencythoughts.blogspot.com/2019/07/sphenothallus-sica-branching-conularid.htmlhttps://sciencythoughts.blogspot.com/2018/10/dipleura-dekayi-north-american.html
https://sciencythoughts.blogspot.com/2018/08/looking-for-eastern-margin-of-palaeo.htmlhttps://sciencythoughts.blogspot.com/2017/11/eddianna-gaspiana-new-species-of.html
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