Showing posts with label Spherules. Show all posts
Showing posts with label Spherules. Show all posts

Wednesday, 2 March 2022

Determining the time of year when the Chicxulub Impactor fell.

The end-Cretaceous extinction event wiped out 76% of known species on Earth, but was strangely selective in the way it did so. The non-Avian Dinosaurs were wiped out, as were the Pterosaurs, most Marine Reptiles, Ammonites, Belemnites, and Rudists, amongst other groups. The extinction event is believed to have been caused by a bolide impacting the Gulf of Mexico near the Yucatan Peninsula, creating the Chicxulub Impact Crater. Evidence of the direct effects of this impact, including impact glass fallout, large-scale forest fires and tsunamis, have been found in areas of North America more than 3500 km from the impact site, and the subsequent events are thought to have included a global climatic breakdown which lasted for thousands of years.

The Tanis Event Deposits of North Dakota record a seiche event (tsunami-like wave within an enclosed environment such as a river valley or small lake) including a significant death assemblage of latest Cretaceous fauna, directly overlying the End Cretaceous Hell Creek Formation. This is thought to represent the very end of the Cretaceous, containing the fossils of organisms that died and to have been burried more-or-less instantly in a seiche event brought about by that impact. The reconstruction scenario is that within a few tens of minutes of the impact, a large volume of water and soil was forced upstream from the Tanis Estuary, pushing with it large volumes of marine, freshwater, and terrestrial organisms, whilst also accumulating impact spherules (spherical silica particles formed as melted droplets of rock recrystalise in mid air) which were falling from above. Within this deposit were large numbers of Acipenseriform Fish (Sturgeon and Paddlefish), which were buried alive in alignment with the flow of the seiche, and which had numerous impact spherules trapped within their gills.

In a paper published in the journal Nature on 23 February 2022, Melanie During of the Department of Earth Sciences at the Vrije Universiteit Amsterdam, and the Subdepartment of Evolution and Development at Uppsala University, Jan Smit, also of the Department of Earth Sciences at the Vrije Universiteit Amsterdam, Dennis Voeten, also of the Subdepartment of Evolution and Development at Uppsala University, and of the European Synchrotron Radiation Facility, Camille Berruyer and Paul Tafforeau, also of the European Synchrotron Radiation Facility, Sophie Sanchez, again of the Subdepartment of Evolution and Development at Uppsala University, and the European Synchrotron Radiation Facility, Koen Stein of the Directorate ‘Earth and History of Life’ at the Royal Belgian Institute of Natural Sciences, and of Earth System Science at the Vrije Universiteit Brussel, Suzan Verdegaal-Warmerdam, again of the Department of Earth Sciences at the Vrije Universiteit Amsterdam, and Jeroen van der Lubbe, once again of the Department of Earth Sciences at the Vrije Universiteit Amsterdam, and of the School of Earth and Environmental Sciences at Cardiff University, attempt to determine the season in which the Fish of the Tanis Event Deposits died by examining cyclical bone growth patterns in their skeletons to see at which point growth ceased.

 
Reconstruction of a Paddlefish with impact spherules in the gill rakers. (a) Three-dimensional rendering of Paddlefish FAU.DGS.ND.161.4559.T in left lateral view with the location of a higher-resolution scan (depicted in (b)) indicated (white outline). (b) Three-dimensional rendering of the subopercular and gills in a with trapped impact spherules (yellow). Scale bars are 2 cm. During et al. (2022).

Tree-ring evidence of the Maastrichtian (latest Cretaceous, 72.1 to 66 million years ago) climate of North Dakota suggests a temperate climate with four distinct seasons. The Tanis site is reconstructed as having had annual temperature fluctuations that varied from an average of roughly 19 °C in summer, down to a winter average of 4–6 °C. As well as the rings in trees, these climate variations are recorded in the bones of Acipenseriform Fish, potentially providning a clock which could have recorded the season in which the Chicxulub Impactor fell. To this ende During et al. analysed three Paddlefish dentaries and three Sturgeon pectoral fin spines from the Tanis deposits.

 
PPC- SRμCT data of FAU.DGS.ND.161.4559.T, a partial Paddlefish from the Tanis locality. (a) Orthogonal virtual thin sections (100 μm thick, average-value projections) obtained in front, top, and right view. (b) Impact spherules in virtual thin sections of (a), indicated with yellow circles. Scale bars (a) 1 mm. (c) Three-dimensional rendering (in left lateral view) with virtual cross sections of (d) (blue), (e) (green), and (f) (red) indicated. (d) Coronal virtual slice. (e) Sagittal virtual slice. (f) Axial virtual slice, brain-enveloping tissues indicated with red arrows. (g) Three-dimensional rendering in right lateral view with anatomical labels. (h) Three-dimensional rendering in left lateral view with anatomical labels. During et al. (2022).

During et al. traced lines of arrested growth (marks left in growing bone by slowed growth at one time of year, typically winter in a temperate climate) in dermal bones from six Acipenseriform Fish, by preparing slices of bone as microscope slides. They corroborated this by creating a three-dimensional map of the skulls using propagation phase-contrast synchrotron radiation micro-computed tomography at the European Synchrotron Radiation Facility, which enabled optimal projection of the bone deposition pattern across multiple cross-sectional planes, enabling them to determine the relationship between growth lines and seasonality across a wider area of bone. In addition, During et al. carried out an investigation into the isotopic composition of the growth lines in one Paddlefish specimen.

 
Osteohistological thin sections of five Acipenseriform Fish. (a)–(e) Thin sections in transmitted light of VUA.GG.2017.MDX-3 (a), VUA. GG.2017.X-2743M (b), VUA.GG.2017.X-2744M (c), VUA.GG.2017.X-2733A (d) and VUA.GG.2017.X-2733B (e), showing congruent pacing of bone apposition during the final years of life, terminating in spring. Red arrows indicate lines of arrested growth. Scale bars are 0.5 mm. During et al. (2022).

The tomographic reconstructions also demonstrate that impact spherules are found only in the gill rakers of the Fish, and are absent elsewhere within their bodies, strongly supporting the idea that they were taken in during the last minutes of their lives, and did not have time to penetrate the oral cavity or further down the digestive tract before they died. This also rules out the possibility that they were introduced to the Fish post-mortem, by penetrating decomposing bodies, indicating the Fish were buried rapidly after their death, which strongly supports the idea that the death of the Fish was close to simultaneous with the arrival of the seiche wave, and therefore that these Fish were alive and active in the very last moments of the Cretaceous.

 
Carbon isotope record alongside the incremental growth profiles. (a) Proportion of carbon¹³ expressed as ‰ on the Vienna Pee Dee Belemnite reference scale. The colour gradient highlights the theoretical range between maximum values during seasonal (summer) trophic increase of carbon¹³ (yellow) and minimum values during trophic decrease of carbon¹³ (winter) (blue). (b) Virtual thick section (average-value projection with 0.1 mm depth) showing growth zones during the favourable growth seasons and annuli and lines of arrested growth outside the favourable growth seasons. (c) Cell density map of a virtual thick section (minimum-value projection with 0.2 mm depth) showing fluctuating osteocyte lacunar densities and sizes, with higher densities and largest sizes recorded during the favourable growth seasons (orange) and lower densities and smaller sizes outside the favourable growth seasons (purple). (d) Microscopic thin section in transmitted light showing lines of arrested growth (red arrows) and a single growth mark indicated (bracket) spanning the distance between two subsequent lines of arrested growth and including a zone and an annulus, Scanning data visualized in (b) and (c) were obtained approximately 10 mm distal from the physically sectioned thin slice of (d), which itself was located directly proximal to the thick section sampled for (a). Scale bars are 1 mm. During et al. (2022).

During et al. used micro-X-ray fluorescence to search for signs of taphonomic alteration within the bones, finding that iron and manganese oxides were present both within the surrounding sediments and the sediments surrounding the bones, and the vascular canals within the bones, but had not penetrated into the bone tissue itself. Potassium and silicon were present in the sediment but not in the bones, while the bones themselves maintained a homogeneous distribution of phosphorus and calcium, which would be expected in unaltered bone. The fine detail of the fossils, including the preservation of non-ossified tissues that surrounded the brains of the Fish, also points towards there being almost no taphonomic alteration of the specimens.

 
Elemental distribution maps of Acipenseriform elements from the Tanis locality obtained with micro-X-ray fluorescence. (a) Calcium, phosphorus, and manganese distribution in Paddlefish dentary VUA.GG.2017.X-2724. (b) Calcium, phosphorus, and manganese distribution in Sturgeon pectoral fin spine VUA.GG.2017.MDX-3. (c) Calcium, phosphorus, and manganese distribution in Paddlefish dentaries VUA.GG.2017.X-2733A, VUA.GG.2017.X-2733B, and the surrounding sediment matrix. (d) Calcium, phosphorus, and manganese distribution in Sturgeon pectoral fin spine VUA.GG.2017.X-2743M. (e) Calcium, phosphorus, and manganese distribution in Sturgeon pectoral fin spine VUA.GG.2017.X-2744M. (f) Potassium, silicon, and iron distribution in Paddlefish dentary VUA.GG.2017.X-2724. (g) Potassium, silicon, and iron distribution in Sturgeon pectoral fin spine VUA.GG.2017.MDX-3. (h) Potassium, silicon, and iron distribution in Paddlefish dentaries VUA.GG.2017.X-2733A, VUA. GG.2017.X-2733B and the surrounding sediment matrix. (i) Potassium, silicon, and iron distribution in Sturgeon pectoral fin spine VUA.GG.2017.X-2743M. (j) Potassium, silicon, and iron distribution in Sturgeon pectoral fin spine VUA.GG.2017.X-2744M. During et al. (2022).

The dentaries of Paddlefish form by the ossification of tissue around the Meckel’s cartilage, while the pectoral spines of Sturgeon form by the ossification of embryonic mesoderm tissue within the skin. Neither of them form by the direct ossification of cartilage. Instead they grow incrementally, with new bone tissue being secreted by rows of osteoblasts on the growing surface. This generates an annual growth pattern, with each year represented by a thick zone of bone laid down under favourable conditions, followed by a narrower area of bone laid down under less favourable growth conditions, then a line of arrested growth, representing a period when no bone was laid down. During et al.'s examination of Acipenseriform Fish remains from the terminal Cretaceous Tanis Event Deposits showed that in all cases growth had stopped for the final time shortly after the bones had begun to grow again following a line of arrested growth.

 
Osteohistology of Acipenseriform Fish from the Tanis locality. (a) Thin section of Paddlefish dentary VUA.GG.2017.X-2724 under transmitted light. (b) Detail of VUA.GG.2017.X-2724 thin section (white box in (a)), scale bar 100 μm. (c_ Detail of VUA.GG.2017.X-2724 thin section (white box in (b)), scale bar 100 μm. (d) Thin section of Sturgeon pectoral fin spine VUA.GG.2017. MDX-3 under transmitted light. (e) Detail of VUA.GG.2017.MDX-3 thin section (white box in (d)), scale bar 100 μm. (f) Detail of VUA.GG.2017.MDX-3 thin section (white box in (e)), scale bar 100 μm. (g) Thin section of Paddlefish dentary VUA. GG.2017.X-2733A under transmitted light. (h) Detail of VUA.GG.2017.X-2733A thin section (white box in (g)) with red arrows indicating lines of arrested growth, scale bar 100 μm. (i) Detail of VUA.GG.2017.X-2724 thin section (white box in (h)), scale bar 100 μm. During et al. (2022).

The visible growth lines within the bones were corroborated using stable isotope ratios, which showed seasonal variations in the proportion of carbon¹³, which is linked to diet, and a constant proportion of oxygen¹⁸, which is related to environment, and therefore indicates that the Fish had been living within the river basin their entire lives, rather than migrating to the sea (as some modern do, and which is likely to have been done by some of their Mesozoic forebears). This confirms that the the variation in carbon isotope values and growth rates reflect seasonal variations within that river basin, and not migratory behaviour on behalf of the Fish. This can be seen in both Paddlefish and Sturgeon, despite the different lifestyles of the two types of Fish.

The Paddlefish of the Late Cretaceous Tanis River Basin were filter-feeders (as are Paddlefish today), which are thought to have fed on zooplankton such as Copepods. Such a feeding strategy would have led to seasonal variations in the availability of food, with the maximum availability falling in the summer. This would have led to a summer season when the Fish was both growing faster, and absorbing a higher proportion of carbon¹³. Examination of the distribution of carbon¹³ within fossil Paddlefish bones from the Tanis deposits reveals that at the time of their deaths the proportion of carbon¹³ in their diets was rising, but had not reached its annual peak, supporting the hypothesis that when the Fish died it was spring in the northern hemisphere.
 
Previous studies on palaeobotanical material from Wyoming has suggested that the Chicxulub Impactor fell in June, although those studies are now considered unreliable for a variety of reasons, leaving us with no standing theory on the time of year when the impact event happened. During et al.'s study appears to show a direct record of the season in which Fish that died directly as a result of the impact died, giving a strong line of support for a springtime extinction event.

If correct, the finding that the Chicxulub Impactor fell in the Northern Hemisphere's spring season may go some way to explaining the selective nature of the extinction it caused. Spring is the breeding season for many Animals, which can potentially make them more vulnerable to environmental perturbations. In the aftermath of the impact the ecosystems of the Southern Hemisphere are known to have recovered much more quickly than those of the north, which could potentially have been linked to an event which hit Northern Hemisphere organisms in their breeding season. The event also impacted larger organisms, with longer breeding cycles, more than it did smaller ones with shorter breeding cycles, which could again be linked to the disruption of a breeding season. An event which happened shortly before the onset of winter in the Southern Hemisphere would have been favourable for the survival of organisms which hibernate in burrows (such as many small Mammals), and which might already have been entering a dormant phase when the bolide impacted, something which could potentially also apply to some Amphibians, Birds, and even Crocodilians. 
 
If this is the case then it goes some way towards decoupling the short- and long-term effects of the Chicxulub Impact, with the initial events being particularly harsh on organisms with a spring breeding cycle in the Northern Hemisphere, and relatively benign to organisms with a winter dormant phase in the Southern Hemisphere, while the longer term climatic and ecosystem breakdowns would favour organisms flexible in their environmental and dietary needs, which would be better able to survive amid collapsing food webs, in either hemisphere.

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Tuesday, 2 January 2018

Micrometerites from Late Cretaceous Chalk depostits from southern England.

Micrometeorites are tiny (less than 2 mm) fragments of asteroidal (or occasionally cometary) material that survive the descent through the Earth's atmosphere, and which are collected by planetary scientists from sites where input from terrestrial sedimentary sources is minimal, such as Antarctic ice- and snow-fields and oceanic basins. Some micrometeorites survive the journey to the Earth relatively impact, but most are melted by the temperatures caused by friction with the Earths atmosphere (which is greater than that caused by simply falling due to the high relative speeds at which these bodies are travelling prior to encountering the Earth), often reaching temperatures in excess of 2000°C,  which causes them to melt, forming spherical droplets due to surface tension, which recrystallise to form circular bodies called spherules.

These spherules do not retain the same chemistry as their parent bodies; lighter elements, such as sodium, sulphur, phosphorus, chlorine, and manganese tend to evaporate completely, while heavier elements such as iron and nickel separate internally, forming discrete layers. As these liquid spherules descend further they are quench cooled through contact with the denser lower atmosphere, causing them dendritic crystals to form. About 95% of such spherules have a silicate dominated composition, while about 4% are iron dominated and about 1% have a mixed composition. Silicate dominated spherules can have different mineralogies, which is thought to relate to the temperature to which they were heated, rather than their original composition, with porphyritic spherules forming at the lowest temperatures, then barred olivine spherules, then cryptocrystalline spherules, and finally vitreous (glassy) spherules at the highest temperatures. Iron dominated spherules are divided into metal-bearing spherules, which contain an iron-nickel bead surrounded by a layer of wüstite (an iron-oxide mineral), and oxidised sperules, which are composed of a mixture of wüstite and magnetite (another iron-oxide mineral).

Spherules, unlike unaltered micrometeorites, are distinctive enough to be recognised in the rock record and recovered from ancient sediments, with examples having been recovered from a wide range of sedimentary rocks, from Archean limestones in Australia to Eocene marine sediments in Barbados, as well as ancient granites in China. However, such spherules do not simply enter the rock record and remain unchanged waiting to be discovered, they are altered by chemical processes going on within the rock, causing changes referred to as taphonomy. This taphonomy can take a number of forms, including alteration of minerals, hydration or dissolution of anhydrous minerals and metals, and encrustation with halite (salt), calcite (carbonate) or other materials.

In a paper published in the journal Earth and Planetary Science Letters on 1 September 2017, Martin Suttle and Mathew Genge of the Impacts and Astromaterials Research Centre at Imperial College London and the Department of Earth Science at the Natural History Museum, describe the discovery of spherule micrometeorites in Late Cretaceous chalk deposits obtained from a road cutting at Ranmore Common in Surrey, southern England.

Suttle and Genge were able to obtain 76 spherules from their rock sample, including 60 iron oxide spherules, 13 iron/silica spherules and 3 silica spherules, ranging in size from 10 to 165 μm. The majority of the iron oxide spherules were comprised of magnetite, with small amounts of aluminium, silicon and manganese, and trace amounts of other minerals but no nickel, while one was comprised of a mixture of wüstite and magnetite, with a significant proportion of nickel. The iron/silica spherules also lacked any nickel, but did contain small amounts of chromium and manganese. The silica spherules contained small amounts of iron, aluminium and manganese.

External and internal textures of Fe-oxide spherules, interpreted as fossilised cosmic spherules. Particle (D) (C16-0003) is the single unaltered nickel-bearing iron oxide spherule, composed of wüstite, while the remaining spherules are composed of maganese-bearing magnetite. Surface dendrites and residual chalk sediment, including fragmented coccolithophore tests can be seen coating external surfaces of spherules (A)–(C). In spherule (D) and (F) sub-circular cavities are present, representing the loss of an iron–nickel metal bead by corrosion during residence on the Cretaceous seafloor, these spherules can therefore, be identified as metal-bearing iron oxide spherules. In contrast, spherule (G) contains isolated irregular small cavities, representing vesicles formed by residual gas trapped during inward crystallisation and is therefore an oxidised iron spherule. Suttle & Genge (2017).

The iron oxide and iron silica spherules were either homogeneous throughout or showed dendritic crystal formation, with many of the spherules with dendritic crystals also having cavities within, probably indicative of dissolution of minerals. One of the silica spherules has an olivine mineralogy, with the other two being porphyritic.

External and internal textures of iron-silicide spherules, most probably composed of suessite. These spherules are interpreted as fossilised cosmic spherules. Replacement by silicides imperfectly pseudomorphs the original texture, leading to changes in volume, accounting for the presence of micron sized voids seen in (F) and protrusions (D), protecting from the particle’s surface. Despite preservation artifacts, original textures can be discerned, allowing their identification as cosmic spherules. Dendritic crystals are observable in all particles and attest to a rapid cooling history as molten droplets. Particle C16-0009 (A) and (B) preserves only a single phase (most likely wüstite) while particle C16-0010 (D)–(F) preserves both the original magnetite and wüstite as different silicide minerals. Cavities in (B) are a result of volatile gases released during atmospheric entry. Suttle & Genge (2017).

Four of the spherules, the three silica spherules and the nickel-bearing wüstite spherule, are essentially identical to modern spherules obtained from Antarctic snowfields, leaving little doubt as to their meteoric origin. The presence of dendritic crystals in many of the magnetite spherules suggests being heated to a temperature of over 1350°C. The cavities within many of the spherules are probably due to the dissolution of soluble crystals as the spherules lay upon the sea-floor.

Sectioned images of silicate cosmic spherules. Spherules (A) and (B) are ancient, unaltered chondritic silica-type spherules, classified as micro-porphyritic (A) and barred olivine (B) subtypes. For comparison particle (C) is a modern, barred olivine spherule recovered from Larkman Nunatak, Antarctica. Suttle & Genge (2017).

The presence of manganese in many of the spherules requires more explanation, as manganese is extremely rare in modern micrometeorites. Suttle and Genge suggest that this is probably not indicative of the original composition of the meteorites, but rather re-crystallisation of the spherules on the seafloor. They suggest that the spherules probably had a nickle-bearing wüstite composition, which was recrystallised to magnetite on the seafloor, in the process losing their nickel content, but gaining manganese (which is often abundant in marine sediments).

See also...

http://sciencythoughts.blogspot.co.uk/2017/12/determining-origin-of-scoriaceous.htmlhttp://sciencythoughts.blogspot.co.uk/2017/09/understanding-deposition-of-suevites-in.html
http://sciencythoughts.blogspot.co.uk/2017/02/looking-for-pieces-of-piecki-meteor.htmlhttp://sciencythoughts.blogspot.co.uk/2017/01/osterplana-065-unique-meteorite-from.html
http://sciencythoughts.blogspot.co.uk/2016/12/micrometeorites-from-urban-environments.htmlhttp://sciencythoughts.blogspot.co.uk/2015/03/a-second-naturally-occurring.html
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Monday, 16 March 2015

The formation of glassy spherules in volcanic ash clouds struck by lightning.


Glassy spherules are found in many geologic strata, and are commonly taken as evidence of meteorite strikes. They can be formed by the melting of mineral grains in the atmosphere at temperatures in excess of 3000 ˚C, and meteorites typically strike the Earth’s atmosphere at very high speeds due to their orbital momentum, resulting in friction with the atmosphere that can heat them to over 10 000 ˚C. However such spherules are also known to form under some circumstances in volcanic rocks, and as a result of lighting striking the ground.

In a paper published in the journal Geology on 27 February 2015, Kimberly Genareau of the Department of Geological Sciences at the University of Alabama, John Wardman and Thomas Wilson of the Department of Geological Sciences at the University of Canterbury, Stephen McNutt of the School of Geosciences at the University of South Florida and Pavel Izbekov of the Geophysical Institute at the University of Alaska Fairbanks, discuss the formation of glassy spherules due to lighting strikes on clouds of volcanic ash.

Genareau et al. were carrying out experiments into the effects of volcanic ash on electric power systems, and in particular ash-induced insulator flashover, where the conductive properties of the ash allow for discharge from high voltage insulators. They found that such discharges commonly resulted in the formation of glassy spherules similar to naturally occurring spherules.

Scanning electron microscope images of pseudo-ash samples collected from tracks of electrical discharge on insulators used in high-voltage flashover experiments. Larger particles (A) display fluidal morphologies indicative of partial melting, but are coated with smaller particles (B–D) with spherical morphologies similar to those found in natural ash-fall samples. Genareau et al. (2015).

Genareau et al. compared these spherules to spherules from ash falls associated with the 2009 eruption of Mount Redoubt, Alaska, and the 2010 eruption of Eyjafjallajökull, Iceland, two volcanic events where numerous lighting strikes on ash columns were documented (such strikes are common, ash columns can build up considerable charge variations leading tofrequent electrical discharges), finding spherules within these deposits similar to those created artificially. Since lightning can generate temperatures in excess of 30 000 ˚C, this is a plausible method for the formation of such spherules.

Secondary electron images of lightning-induced volcanic spherules observed in samples from the A.D. 2009 eruption of Mount Redoubt, Alaska, USA (A–B) and the A.D. 2010 eruption of Eyjafjallajökull, Iceland (C). Textures range from almost perfect spheres to spherules displaying surface cracks and holes to aggregates of numerous spherules fused together. Genareau et al. (2015).

A slightly larger range of spherule types was found in the natural samples, with slightly larger spherules present, aggregates of spherules and spherules with a distinctive cracked surface morphology. The cracked morphology is thought to be due to the vaporization of volatiles (probably water) within mineral grains as they are melted, the fused spherules could either have been adhered to one-another by the action of the lightning or drawn together subsequently by electrostatic attraction, whereas the overall size of the particles is probably directly related to the energy released in the lightning burst; the artificial samples produced larger grains showing signs of partial melting, suggesting that a more powerful discharge could have melted them completely (the experiment was intended to reproduce energy levels in power lines not lighting bursts).

See also…

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