Thursday, 31 December 2020

Microbial communities from deeply burried oceanic crust.

The upper oceanic crust is mainly composed of basaltic lava. It has been continuously created on Earth for about 3.8 billion years. Basaltic lava is erupted and solidified at mid-ocean ridges where high-temperature basalt-seawater reactions provide substantial energy for sustaining chemosynthetic life. On ridge flanks, circulation of crustal fluid is hydrothermally driven within the basaltic lava overburdened with sediments. The portion of basaltic lava beneath sediment cover is referred to as basaltic basement. Previous studies at 3.5- and 8-million-year-old ridge-flank systems demonstrated that these young crustal aquifers, respectively, harbor anaerobic thermophiles and aerobic mesophiles that contribute to hydrogen, carbon, and sulphur cycling. After rock fractures are filled with secondary minerals, intensities of fluid circulation and basalt-seawater reactions sharply decline with increasing crustal age; with most crustal oxidation occurring in the first 10 million years after crust formation.

More than 90% of Earth’s ocean lithosphere is older than 10 million years and long past its early stage of relatively high crustal oxidation rate. Despite its vast areal extent, the nature and extent of life in this old crust is previously unknown, in part because of the technological and analytical challenges of exploring the igneous rock habitat through scientific drilling. Alteration textures suggestive of biological activity have been observed in oceanic crust as old as 3500 million years. However, the role of microbial activities in creating these textures and the age of the crust at the time of texture formation remain unknown.

In a paper published in the journal Communications Biology on 2 April 2020, Yohey Suzuki, Seiya Yamashita, Mariko Kouduka, and Yutaro Ao of the Department of Earth and Planetary Science at the University of Tokyo, Hiroki Mukai, also of the Department of Earth and Planetary Science at the University of Tokyo, and of the Mantle Drilling Promotion Office at the Japan Agency for Marine-Earth Science and Technology, Satoshi Mitsunobu of the Department of Environmental Conservation at Ehime University, Hiroyuki Kagi of the Geochemical Research Center at the University of Tokyo, Steven D’Hondt of the Graduate School of Oceanography at the University of Rhode Island, Fumio Inagaki of the Kochi Institute for Core Sample Research and Mantle Drilling Promotion Office at the Japan Agency for Marine-Earth Science and Technology, and Yuki Morono, Tatsuhiko Hoshino, Naotaka Tomioka, and Motoo Ito, also of the Kochi Institute for Core Sample Research at the Japan Agency for Marine-Earth Science and Technology, investigate the occurrence of microbial communities in subseafloor basaltic lava older than 10 million years, recovered by Integrated Ocean Drilling Program Expedition 329 in the South Pacific Gyre. The presence of microbial cells in the iron-rich smectite on old subseafloor basaltic rock was revealed by nanoscale solid characterizations. Analysis of their lipid profiles and DNA sequences reveals the dominance of heterotrophic Bacteria, suggesting the presence of organic matter resources in the subseafloor basalt.

Within the South Pacific Gyre, extremely low sedimentation rates lead to burial of sediments nearly depleted in organic matter. In this ultraoligotrophic environment, dissolved oxygen penetrates from the  ocean floor to the basaltic basement and sustains aerobic microbes throughout the sediment column. During Expedition 329, using the drilling vessel JOIDES Resolution, core samples were obtained from basaltic basement at Sites U1365, U1367, and U1368 with crustal ages of 104 million years, 33.5 million years, and 13.5 million years.

Biogeochemical characteristics of surface seawater and sediment overlying region of the drilled basaltic basement. (a) Map of annual chlorophyll-a concentration in surface seawater. Sedimentary profiles of cell abundance (b), dissolved oxygen (c), and total organic carbon (d). Profiles span the sediment column  from seafloor to basement. The vertical line in (b) marks the minimum quantification limit. Suzuki et al. (2020).

Mineral characterisations were conducted for core samples with fractures/veins to clarify the presence of clay minerals typically produced by low-temperature rock–water interactions (weathering). X-ray diffraction analysis revealed the presence of iron-rich smectite in 33.5-million-year-old and 104-million-year-old core samples but not in 13.5-million-year-old core samples. Thin sections were prepared from the 33.5-million-year-old and 104-million-year-old core samples with sample codes: U1367F-6R1, U1365E-8R4, and U1365E-12R2 at depths of 51, 109.6, and 121.8m below the seafloor and observed by scanning and transmission electron microscopies coupled to energy-dispersive X-ray spectroscopic  analysis. Iron-rich smectite was found at the rims of fractures and veins mainly filled with celadonite and iron oxyhydroxides in U1365E-8R4 and U1365E-12R2, respectively, whereas veins are filled with Iron-rich smectite in U1367F-6R1. Two types of compositionally distinct iron-rich smectite veins were observed in U1367F-6R1: one is similar to those found in U1365E-8R4 and U1365E-12R2 with high magnesium and potasium contents; the other is characterised by high iron content, as typically observed in iron-rich smectite from deep-sea hydrothermal mounds.

Chemical compositions of two types of Fe-rich smectite found in U1367F-6R1 and cell distributions revealed by staining of thin sections with SYBR-Green I. (a) Trigonal diagram of aluminium-iron-magnesium content in sheet layer of nontronite and energy-dispersive X-ray spectroscopic spectra of nontronite formed by basalt weathering in green and hydrothermal alteration in orange. Fluorescence microscopy images of SYBR Green I-stained microbial cells with nontronite formed by basalt weathering (b) and hydrothermal alteration (c). Suzuki et al. (2020).

Fluorescence microscopy observations of the thin sections reveal that SYBR Green I-stained cell-like fluorescence signals are extensive along the rims of the rock fractures/veins associated with irom-rich smectite in U1365E-8R4 and U1365E-12R2. Although iron-rich smectite with high magnesium and potassium contents in U1367F-6R1 is correlated with fluorescence signals, fluorescence signals were not detected from veins filled with iron-rich smectite with high iron content in U1367F-6R1.

Basalt interface with microbial colonization. Light and fluorescence microscopy images of SYBR Green I-stained microbial cells in a fracture filled with celadonite in of U1365E-8R4 (a) and in a vein filled with iron oxyhydroxides in U1365E-12R2 (b). Suzuki et al. (2020).

To confirm that these greenish signals originate from microbial cells rather than from autofluorescent materials, roughly 10 × 10-μm² sections with a thickness of about 3 μm were fabricated by focused ion beam, and element-mapping images were obtained using nanoscale secondary ion mass spectrometry. Focused ion beam nanoscale secondary ion mass spectrometry analysis of U1365E-8R4 revealed overlapping signals of cyano radicals, phosphorus ions, and sulphur ions on the dense spots stained with SYBR Green I, indicating that those greenish signals are derived from microbial cells. The microbial cells are localized in the proximity of microscale voids and enrobed within iron-rich smectite.

Single-cell characterizations of fracture-hosted microbial populations. Scanning electron microscopic image of a mineral-filled fracture in U1365E-8R4 (a). Confocal laser microscopy image of SYBR Green I-stained microbial cells (b). Scanning electron microscope image of a focused ion beam-derived thin section of U1365-8R4 with a square region (roughly 10 × 10 μm²) analyzed by the JAMSTEC nanoscale secondary ion mass spectrometry (c). Nanoscale secondary ion mass spectrometry images of cyano radicals (¹²C¹⁴N⁻) (d), phosphourus ions (³¹P⁻) (e), sulphur ions (³²S⁻) (f), silicon ions (²⁸Si⁻) (g), and iron oxide ions (⁵⁶Fe¹⁶O⁻) (h) with intensity colour contours. Overlays are shown from the gallium ion image of the focused ion beam section in black and white and the nanoscale secondary ion mass spectrometry images of cyano radicals (¹²C¹⁴N⁻) in blue, phosphourus ions (³¹P⁻) in green, and sulphur ions (³²S⁻) in red (i). Dashed rectangles and an arrow show regions presented in the following figures. Suzuki et al. (2020).

The same result was obtained by focused ion beam nanoscale secondary ion mass spectrometry of U1365E-12R2. Element mapping using scanning transmission electron microscopy equipped with energy dispersive spectroscopy showed that the microbial cells are spatially associated with laths of iron-rich smectite. Given this association and the large compositional difference between iron-rich smectite and the bentonite clay used for drilling mud, the microbial cells were not introduced from the drilling mud. These results indicate that the detected signatures along the mineral-filled fractures/veins are derived from indigenous microbial communities in the deep crustal biosphere beneath the oceanic and sedimentary biospheres.

Single-cell characterisations of fracture-hosted microbial populations. Scanning electron microscopy image of the mineral-filled fractures in U1365E-12R2 (a). Confocal laser microscopy image of SYBR Green I-stained microbial cells (b). Gallium ion image of a focused ion beam thin section of U1365-12R2 (3-μm thick and a square region of roughly 10 × 10 μm²) analysed using JAMSTEC nanoscale secondary ion mass spectrometry (c), (d) and images of cyano radicals (¹²C¹⁴N⁻) (e), sulphur ions (³²S⁻) (f), silicon ions (²⁸Si⁻) (g), and iron oxide ions (⁵⁶Fe¹⁶O⁻) (h) with intensity colour contours. scanning transmission electron microscopy X-ray elemental mapping images of iron (i), magnesium (j), and potassium (k). Pink arrows and dashed rectangles denote spots or regions described in subsequent figures. Suzuki et al. (2020).

Core samples were evaluated for contamination using fluorescence microspheres (0.5 μm in diameter) that mimic microbial cells introduced from drilling fluid. Microscopic counting of microspheres in subsamples before and after cleaning steps such as washing with 3% sodium chloride solution and flaming the exterior showed that untreated exteriors of core samples contained detectable microspheres, but most post-treatment sample interiors contained no detectable microspheres. These results clarify that the contamination evaluation was properly conducted to show the level of drilling contamination for DNA analysis. 16S ribosomal RNA gene sequences were obtained from the V4 to V6 regions by tagsequencing from four core samples with no detected microspheres (U1365E-8R4, and -12R2 and U1367F-4R1 and U1368F-4R2), one microsphere-detected sample (U1368F-7R3), drilling fluid used at Site U1365, and a DNA extraction blank. To identify potentially contaminant operational taxonomic units from drilling and subsequent laboratory manipulations, the highly contaminated core from U1368F-7R3, the drilling fluid from U1365E, and the negative control were compared to the microsphere-undetected samples.

Chemical comparison of bentonite clay used for drilling fluid and nontronite spatially associated with microbial cells. Scanning electron microscopy-energy-dispersive X-ray spectroscopic spectra obtained from bentonite clay (a) and from nontronite (b). Suzuki et al. (2020).

Because α- and β-proteobacterial operational taxonomic units were identical among the contaminated sources such as the drilling fluid and the DNA extraction blank, the operational taxonomic units detected from the contaminated sources were removed from the microsphere-undetected core samples. In addition, operational taxonomic units obtained from the highly contaminated core (U1368F-7R3) were excluded for detailed analyses of indigenous microbial communities. According to phylogenetic affiliation based on 16S rRNA gene sequences, three types of microbial communities were identified.

Schematic diagram of procedures undertaken for contamination evaluation and decontamination of drilling fluid. Microsphere counting was performed for each step by epifluorescence microscopy. Suzuki et al. (2020).

Type SPG-I (relatively young crustal community: 13.5 million years old). At Site U1368, γ- and ε-proteobacterial sequences were proportionally abundant and included strains related to the genera Arcobacter, Thioreductor, Sulfurimonas, and Sulfurovum known as deep-sea sulphur- and/or hydrogen-oxidising chemolithoautotrophs and the genus Alteromonas globally distributed in deep-sea aquatic habitats with aerobic heterotrophy.

Effects of decontamination processes by washing and flaming. Microscopic counts of fluorescence microspheres in basaltic core samples after each round of decontamination. Rock pieces are represented in cm⁻³, and microsphere density in the surface wash solutions was calculated from the core volume subjected to salt washing. Suzuki et al. (2020).

Type SPG-II (aged crustal communities: 33.5–104 million years old). At Sites U1365 and U1367, β-proteobacterial sequences were predominant and closely related to aerobic organotrophs, such as Roseateles depolymerans isolated from pumice-bearing lake sediment. 

Phylogenetic distributions of the highly contaminated sample U1368F-7R3, the drilling-fluid sample from U1365E, and the negative control used for laboratory manipulations based on 16S rRNA gene sequences. Colours and legends represent differences in taxonomic classification ranging from genus to phylum. Each proteobacterial class or phylum is shown in parentheses. Suzuki et al. (2020).

Type SPG-III was only observed in U1365E-12R2 (a depth of 122 meters below sea floor), in which γ-proteobacterial sequences affiliated within the family Methylococaceae were predominantly detected. In general, these crustal microbial communities were comprised of Methylococaceae members typically found in methane-rich fluids emitted from the deep ocean floor, including cold seeps and hydrothermal vents.

Community composition in cold basaltic basement based on 16S ribosomal RNA gene sequences. Taxonomic profiles of basaltic rock cores from the South Pacific Gyre are shown as pie charts with major taxonomic groups ranging from genus to phylum. Community composition of a crustal fluid sample at North Pond (Site U1382; 8 million years old) is shown as a pie chart for comparison. Suzuki et al. (2020).

Microbial communities have previously been observed in rock core and fluid samples from North Pond (North Atlantic International Oceanic Drilling Program Site; 8 million years old), where oxygenated cold fluid actively circulates in sediment-covered basaltic basement. For microbiological investigations, a Circulation Obviation Retrofit Kit was installed to collect fluid samples from the basaltic basement at North Pond. However, it is possible that microbial communities in fluid samples are distinct from those attached to adjacent rock surfaces. Microbial communities in the North Pond fluid samples are mainly comprised of members of Campylobacterales and Alteromonadales. In contrast, rock core samples were not dominantly colonised by Campylobacterales members but Alteromonadales members. Dominant microbial populations obtained in our rock sample from Site U1368 (13.5 million years old) were similar to those obtained from the North Pond fluid samples. Thus, the nature of the basement fluid may be very similar in relatively young (8 million years old and 13.5 million years old) basaltic basement in both the Atlantic and Pacific Oceans. These results also indicate that the crustal biosphere can be technically evaluated from rock cores, as well as from circulating fluid.

Basement at 13.5 million years old and 33.5 million years old is mainly composed of pillow lava covered with 12- to 17-m thick sediment. The deepest sediment at both sites contains similar concentrations of dissolved oxygen and dissolved nitrate. Although the crustal structure and the dissolved oxidant chemistry are fairly similar at both sites, microbial community composition differs notably between the 13.5- and 33.5-million year old basements. The clay minerals that form in fractures/veins by low-temperature rock-water interactions provide information that may explain the difference between these communities; the presence and absence of iron-rich smectite in fractures/veins at Sites U1367 and U1368 indicate that iron-rich smectite formation was inhibited by vigorous seawater circulation at U1368.

Schematic illustrations of fluid flow regimes and key microbial populations. In basaltic basement, substrates are distinctively supplied from seawater and basalt rocks in 8–13.5 million year old (a) and 33.5–104 million year old (b). Blue and red arrows indicate abundant substrate supplies from seawater and basalt rocks, respectively. Suzuki et al. (2020).

Although the basaltic basement at Site U1365 comprises lava flows where fluid flow is generally between sheeted layers rather than along chilled margins of pillow lava, its microbial community composition is similar to that found at Site U1367, which is consistent with the presence of iron-rich smectite at Sites U1365 and U1367. Seafloor heat flow at U1367 and U1365 is consistent with conduction as the dominant mode of heat transport, while heat flow at U1368 falls below the expected conduction-only level, consistent with apparent heat transport by fluid circulation within the rocky crust. This difference is consistent with the basement ages of the respective sites, as fluid circulation and advective heat transport are generally much more vigorous in relatively young, warm crust (such as the 13.5-million year old crust at U1368) than in much older and consequently cooler crust (such as the 33.5-million year old and 104-million year old crust at, respectively, U1367 and U1365). We suggest that the basement habitability is controlled by heat and fluid flows, which generally decrease over time, versus the primary structure of the crust (e.g. pillow basalt or flow basalt). In addition, the formation of iron-rich smectite in the basaltic basement appears to be correlated with the kinds of microorganisms in aged oceanic crust.

Observations of microbial cells in focused ion beam sections (10 μm × 10 μm × 3 μm) suggest a cell density range of 3 300 000 000 cells/cm³. In the focused ion beam sections, 15 and 2 cyanide-bearing spots derived from microbial cells are visualized in U1365E-8R4 and U1365E-12R2, which gives approximate cell numbers of 50 000 000 000 and 7 000 000 000 cells/cm³. This cell density is narrowly limited to the iron-rich smectite at the interface between basalt and alteration minerals. Within that interface, cell density is exceedingly high in comparison with cell density in the deepest sediment overlying the basaltic basements at Sites U1365 and U1367 (roughly 100 cells/cm³), and in comparison with low-temperature fluids collected from 8-million year old basalt basement at North Pond (roughly 10 000 cells/cm³). The range of cell density estimated for the iron-rich smectite of the basalt-water interface is nearly the same or higher as in organic-rich near-seafloor sediment deposited on continental margins.

To verify the cell density estimates in the two focused ion beam sections, μ-Raman spectroscopy was used to obtain a diagnostic spectrum from the microbe-smectite assemblage. The spectrum is composed of broad peaks at 1200–1600 cm⁻¹ attributed to amorphous organic matter and a slope increasing with Raman shift attributed to smectite. The fingerprint spectrum was obtained throughout the interface regions filled with iron-rich smectite with high magnesium and potassium contents in U1367F-6R1, U1365E-8R4, and U1365E-12R2, but not from that filled with iron-rich smectite with the high iron content in U1367F-6R1. The lack of the fingerprint spectrum from iron-rich smectite with high iron content may be due to its formation at a deep-sea hydrothermal mound near the mid-ocean ridge.

μ-Raman spectra of the assemblage composed of microbes and Ferich smectite in U1365E-8R4. Optical microscopic image of the focused ion beam section with a laser spot where a μ-Raman spectrum was obtained (a). Circles indicate points analysed by μ-Raman spectroscopy in the gallium ion image overlain with nanoscale secondary ion mass spectrometry images (b). μ-Raman spectra from yellow circles associated with microbial cells (c) and from white circles without microbial cells (d). Suzuki et al. (2020).

Smectite is a fine-grained clay mineral, with a large surface area to adsorb organic matter. As dominant microbial communities detected from 33- and 104-million year old basaltic basements are heterotrophic, it is conceivable that organic matter bound to iron-rich smectite may help to sustain the high cell density at the basalt interface. Clay fractions were separated from the core samples and their organic carbon content was quantified. The clay fractions mainly composed of iron-rich smectite contained up to 22-fold higher organic carbon than the bulk core samples, supporting the inference that mineral-bound organic matter fuels heterotrophic activities of microorganisms at the basalt interface. Fourier transform infrared-ray spectra were obtained from the clay fractions to clarify the presence of lipids, based on the aliphatic CH₃/CH₂ absorbance ratios (R₃/₂). Given that the R₃/₂ values are domain-specific: Eukarya 0.3–0.5, Bacteria 0.6–0.7 and Archaea 0.8–1.0, the R₃/₂ ranges of the clay fractions from U1365E-8R4, U1365-12R2, and U1367F-6R1 were approximately in the Bacterial range, which agrees with the dominance of Bacteria indicated by 16S rRNA gene sequences from the corresponding core samples U1365E-8R4 and U1365-12R2 and from the other core sample collected from the same site(U1367F-4R1).

Raman spectra of microbe-nontronite assemblages in fractures/veins of basaltic basement. Broad peaks at 1200–1600 cm⁻¹ attributed to amorphous organic matter and a slope increasing with Raman shift attributed to smectite were obtained at the basalt interface in U1365E-8R4 (a), U1365E-12R2 (b), and U1367F-6R1 (c). Weak broad peaks at 1200–1600 cm⁻¹ attributed to amorphous organic matter at magnesium-poor nontronite in U1367F-6R1 (d). Yellow dots show points where strong peaks were obtained at 1200–1600 cm⁻¹. White dots show points where weak peaks were obtained at 1200–1600 cm⁻¹. Suzuki et al. (2020).

16S rRNA gene sequences related to aerobic and anaerobic methanotrophs were prominent among the 16S rRNA gene sequences detected from the mineral-filled fractures in 104-million year old basaltic basement. Almost half of the 16S rRNA gene sequences analyzed from U1365E-12R2 were closely related to Methyloprofundus sedimenti, an aerobic methanotrophic Bacterium isolated from a deep-sea sediment sample associated with a Whale fall. Additionally, anaerobic methane-oxidising Archaea subtype 1 (ANME-1) was detected from U1365E-8R4. As methane concentrations are below the detection limit (below 1.3 μM) in all sediment samples at Site U1365, methane bound to iron-rich smectite might be a source of energy for their persistence in situ.

The results of this study greatly extend understanding of bioenergetics and habitability in Earth’s upper oceanic crust. Previous studies of bioenergetics in subseafloor basalt have generally focused on chemoautotrophic mineral oxidation, which mostly occurs in crust younger than about 10 million years. Our results indicate that cells encased in iron-rich smectite densely coat rock surfaces of much older (33.5 million years and 104 million years) basalt and are largely sustained by aerobic heterotrophy and methanotrophy. Organic matter that may sustain these communities in the upper crustal aquifer includes (i) dissolved organic matter in the seawater that flows through the fractures and veins, and (ii) organic matter abiotically synthesized during rock weathering (e.g. Lost City where amino-acid production associated with formation of iron, magnesium-rich smectite in gabbroic basement at the Lost City hydrothermal field).

These results also have important implications for understanding the abundance and global distribution of microbial cells in the upper oceanic crust. Mineral (iron and sulphur) oxidation rates are highest in crust younger than about 10 million years. The number of cells that might be supported by aerobic iron oxidation in the upper marine crust has been estimated as 2 400 000 000 000 000 000 000 000 000 cells, potentially equivalent to 10% of total cell abundance in marine sediment. Because the abundant microbes reliant on aerobic heterotrophy and methanotrophy reside in much older crust (33.5 million years and 104 million years), inclusion of these heterotrophic and methanotrophic cells may substantialy increase estimate of total cell abundance in the upper oceanic crust.

The results of this study also have implications for the possibility of life on Mars and other planetary bodies. Basaltic crust is ubiquitous on other planets, such as Mars, as well on Earth. The Martian basaltic crust formed 4 billion years ago, to be followed by formation of iron, magnesium-rich smectite via hydrothermal alteration and weathering at the surface and in the subsurface until about 3 billion years ago. On modern Mars, the surface is cold and dry under high vacuum conditions, and methane is emitted from the subsurface into the atmosphere. Recently, the presence of subsurface liquid water has been indicated, which spurred international interest in the search for extraterrestrial life. Given the subsurface presence of methane and liquid water on Mars, the communities fueled by organic matter and methane in subseafloor basalt on Earth provide a clear model for extant life and/or biosignatures from past life in the subsurface of Mars and other planets.

See also...

Follow Sciency Thoughts on Facebook.

Follow Sciency Thoughts on Twitter.

Asteroid (418849) 2008 WM64 passes the Earth.

Asteroid (418849) 2008 WM64 passed by the Earth at a distance of about 18 550 000 km (48.3 times the average distance between the Earth and the Moon, or 12.4% of the distance between the Earth and the Sun), slightly after midnight GMT on Friday 25 December 2020. There was no danger of the asteroid hitting us, though were it to do so it would have presented a considerable threat. (418849) 2008 WM64 has an estimated equivalent diameter of 140-450 m (i.e. it is estimated that a spherical object with the same volume would be 140-450 m in diameter), and an object of this size would be predicted to be capable of passing through the Earth's atmosphere relatively intact, impacting the ground directly with an explosion that would be 300-176 000 times as powerful as the Hiroshima bomb. Such an impact would result in an impact crater 2-7 km in diameter and devastation on a global scale, as well as climatic effects that would last decades or even centuries.

The orbit and current position of (418849) 2008 WM64. JPL Small Body Database.

(418849) 2008 WM64 was discovered on 24 November 2008 by the University of Arizona's Mt. Lemmon Survey at the Steward Observatory on Mount Lemmon in the Catalina Mountains north of Tucson. The designation 2008 WM64 implies it was the 3112th asteroid (asteroid M64; in numbering asteroids the letters A-Z excluding I, are assigned numbers from 1 to 25, with a number added to the end each time the alphabet is ended, so that A = 1, A1 = 26, A2 = 51, etc., which means that M64 = (25 x 64) + 12 = 3112) discovered in the second half of November 2008 (period 2008 W; the year being split into 24 half-months represented by the letters A-Y, with I being excluded),  while the longer designation 418849 indicates that it was the 418 849th asteroid discovered overall (asteroids are not given this longer designation immediately, to ensure that numbered objects are genuine asteroids that have not been previously described). 

(418849) 2008 WM64 is calculated to have a 368 day (1.01 year) orbital period and an elliptical orbit tilted at an angle of 33.5° to the plain of the Solar System that takes it from 0.90 AU from the Sun (i.e. 90% of the average distance at which the Earth orbits the Sun) to 1.11 AU from the Sun (i.e. 111% of the average distance at which the Earth orbits the Sun). It is therefore classed as an Apollo Group Asteroid (an asteroid that is on average further from the Sun than the Earth, but which does get closer). This means that close encounters between the asteroid and Earth are extremely common, with the last having occurred in July this year and the next predicted in July next year. As an asteroid probably larger than 150 m in diameter that occasionally comes within 0.05 AU of the Earth, (418849) 2008 WM64 is also classified as a Potentially Hazardous Asteroid.

See also...

Follow Sciency Thoughts on Facebook.

Follow Sciency Thoughts on Twitter.

Bushizheia yangi: A new species of Euarthropod from the Early Cambrian Chengjiang Lagerstätte.

Over 250 species have been recorded from the Cambrian Series 2, Stage 3 Chengjiang biota of Yunnan Province, China, with Arthropods representing circa 33% of these species. These include taxa with soft anatomy preservation that are instrumental to elucidating early Euarthropod evolution. Among these, Arthropods with a grasping appendage, the so-called great or frontal appendages, are iconic animals of the Chengjiang biota. 

In a paper published in the journal Palaeontologica Electonica, Robert O’Flynn and Denis Audo of the Yunnan Key Laboratory for Palaeobiology and International Joint Laboratory for Palaeobiology and Palaeoenvironment at Yunnan University, Mark Williams of the School of Geography, Geology and the Environment at the University of Leicester and the International Joint Laboratory for Palaeobiology and Palaeoenvironment at Yunnan University, Dayou Zhai, also of the Yunnan Key Laboratory for Palaeobiology and International Joint Laboratory for Palaeobiology and Palaeoenvironment at Yunnan University, and Hong Chen, again of the Yunnan Key Laboratory for Palaeobiology at Yunnan University, and Yu Liu, once again of the Yunnan Key Laboratory for Palaeobiology and International Joint Laboratory for Palaeobiology and Palaeoenvironment at Yunnan University, describe a new species of Euarthrapod from the Chengjiang Biota.

The new species is known only from a single specimen with a well-preserved dorsal exoskeleton that is divided into head, thorax, and pygidium, but is most notable for its long frontal appendages that resemble those of Radiodonts and the Euarthropod Kiisortoqia soperi. O'Flynn et al. discuss what happened to the ‘great appendage’ with reference to two possibilities for the evolution of the primary antennae or ‘great appendage’: (1) that limb-like ‘great appendages’ evolved to form chelicerae, i.e. innervated from the deutocerebrum; or (2) that the labrum represents the transformed frontal ‘great appendage’, i.e. innervated from the protocerebrum.

Bushizheia yangi (YKLP 11421). (A) Photograph of dorsal view; (B) composite line drawing of dorsal view. Both scale bars are 10 mm. Abbreviations: app?ex, exopod of a post-frontal head limb appendage; cw, compression wrinkle; en, endopod; gr, groove; hl, frontal head limbs; hs, head shield; ps; pygidial segment; pyg, pygidium; tg1-8, tergites 1 through 8; ts, tailspine. O'Flynn et al. (2020).

The new species is described from a single specimen recovered from the Yu’anshan Member pf the Chiungchussu Formation at Jiucun Town in Chengjiang County. The Yu’anshan Member is informally divided stratigraphically into four lithologically and palaeontologically distinctive parts. The specimen was recovered from the third stratigraphic interval of the Yu’anshan Member from laminated mudstones
of the early Cambrian (Series 2, Stage 3). It is deposited in the Yunnan Key Laboratory for Palaeobiology at Yunnan University, Kunming, as specimen number YKLP 11421.

The specimen was prepared mechanically with a mounted steel needle under a binocular microscope, where only a small amount of matrix was required to be removed by a gentle scraping action. 

Fluorescence microscopy and photography (a Leica DFC7000 T linked to a Leica M205 FA fluorescence stereo microscope) were used to increase the contrast between the specimen (not autofluorescent) and the matrix (weakly autofluorescent). For photographs in natural colour, O'Flynn et al. captured several images with a Digital SLR Camera (a Canon EOS 5DS R and a Nikon D700) fitted with a 100 mm and a 105 mm macro lens, respectively, with extension rings for magnification factors above 1:1. The photographs were mostly captured in cross-polarised light to limit reflection of light and increase contrast. O'Flynn et al. also captured photographs with cropped light (light coming from a low vertical angle, highlighting structures at the surface) from various angles (default: from the top left) to reveal the micro relief of the fossil. The specimen was also investigated with Computed Tomography using a ZEISS Xradia 520 Versa, but no additional structures were revealed using this method.

Measurements were made on digital photographs using the image processing software ImageJ. Morphological characters measured include: (1) the total length, measured from the anterior margin of the head shield to the posterior termination of the tailspine; (2) the head, measured from the anterior margin to the posterior margin of the head shield; (3) tergites one through eight, measured from the anterior margin to the posterior margin of the tergite; (4) the frontal head limb, measured from the distal termination to the proximal margin of the podomeres; and (5) the pygidium, measured from the posterior margin of the posterior-most tergite to the posterior termination.

The new species is named Bushizheia yangi, where 'Bushizheia' derives from Bǔshízhě, the Mandarin for predator: an allusion to Kiisortoqia, from the Kalaallisut (Greenlandic) word kiisortoq, meaning predator, and 'yangi' honours Zhixin Yang, who recovered and prepared the fossil.

The genus Bushizheia is is ascribed to the total group Euarthropoda, as defined by the presence of fully Arthrodised bodies and limbs, because it has sclerotised trunk tergites, sclerotisation of post-antennal appendages, and does not have any isolated tergites in the cephalic segments.

It features a long, frontal grasping appendage that is morphologically like that of Radiodonts, but in combination with a completely Arthrodised body organisation; this distinguishes Bushizheia from all other Euarthropods, except Kiisortoqia.

Bushizheia and Kiisortoqia appear allied to each other by the possession of frontal ‘great appendage’-like head limbs. However, Bushizheia is sufficiently distinct to warrant erection of a monospecific genus. It differs from Kiisortoqia by: (1) Bushizheia  has a large pygidium with paired short falcate spines and a terminal tailspine; Kiisortoqia has a small tail shield with neither spines nor a tailspine and twice the number of thoracic tergites; (2) trilobation of thoracic tergites effaced; (3) dorsal spine is present on each podomere of the frontal head limb. 

Bushizheia yangi (YKLP 11421). (A), (C) Tungsten photography lighting of left frontal head limb and dorsal view of head shield, respectively; (B), (D) fluorescent photography lighting of the same. All scale bars are 2 mm. Abbreviations: cw, compression wrinkles; ds, dorsal spines; hl, frontal head limb. O'Flynn et al. (2020).

Bushizheia yangi is a Euarthropod with a semi-circular head shield lacking dorsal compound eyes, eight thoracic tergites, and a large, semi-circular pygidium. Frontal head limbs circa 33% of body length, strong, composed of at least 12 podomeres, each with paired spines laterally.

Bushizheia yangi is circa 54 mm long. The habitus is sub-elliptical in dorsal aspect, with a length (anterior margin of the head shield to the posterior termination of the tailspine) of circa 250% of the width (maximum width in the anterior half of the body at the third and fourth tergites). The length of the head shield is circa 20% of the total length. The trunk tapers from the fourth tergite backwards to a large pygidium (the tail shield of the exoskeleton covering the fused posterior segments of the body). The pygidium’s margin is spinose.

Bushizheia yangi (YKLP 11421). (A) Detail of pygidium; (B) detail of exopod setae. Scale bar 3A is 10 mm. Scale bar is 1 mm. Abbreviations: en, endopod; exs, exopod setae; pyg, pygidium; ts, tailspine. O'Flynn et al. (2020).

The head shield is a simple, semi-circular shield, with smoothly rounded posterolateral margins, and the length is circa 70% of its width.

The trunk consists of eight tergites. The anteriormost three tergites are virtually of equal length; the length is circa 20% of the width. Tergites 3-4 are widest; the width and length of tergites subsequently decrease posteriorly in width and length. Axially, the posterior border of each tergite overhangs the following tergite by circa 17% of its length, but by less abaxially. The first, second, and third tergites are reflexed anteriorly, whereas tergites posterior to that are transverse or reflexed posteriorly. The tergopleurae of the first and second tergites terminate bluntly posterolaterally. The tergopleurae of tergites 3-8 are extended into posterolateral projections.

Reconstruction of (A) Bushizheia yangi juxtaposed with (B) Kiisortoqia soperi in dorsal view. Both scale bars are 10 mm. O'Flynn et al. (2020).

The pygidium is a semi-circular shield and its length is circa 70% of its width; the margins bear eight paired short falcate spines, which curve very slightly posteriorly. The pleural regions of the pygidium’s anterior-most segment are effaced, but a transverse furrow is visible axially. The tailspine is sub-triangular and incompletely articulated; it is as wide as long, circa 8% of the total length, and circa 30% of the total length of the pygidium.

The frontal head limbs reach a length of circa 33% of the total length of the body: 12 podomeres extend beyond the head shield, each with lateral endites that bear two inward facing setae, and terminal setae that are outward facing. Podomeres 2-7 are of equal length but decrease in width distally.

All visible post-frontal head limb appendages consist of either an endopod or an exopod. The one (incompletely) preserved endopod comprises four narrow podomeres. The two preserved exopods are paddle-shaped flaps, fringed with setae. Martin Stein in his description of Kiisortoqia soperi, identified four cephalic appendiferous segments (a head incorporating the antennular plus three post-antennular limb-bearing segments), considered to be part of the ground pattern of Euarthropoda. The distal exopod of the anteriormost post-frontal head limb appendage of Bushizheia yangi appears beneath the head shield, and may, based on its position, be the fourth cephalic appendage. The limb immediately posterior of this, adjacent to the first trunk tergite, appears to be the first trunk appendage.

Bushizheia yangi is dorsoventrally compressed and lies parallel to lamination; its well-articulated nature (i.e., tergites preserved attached, exopods preserved in situ). This state of preservation, especially the presence of articulated frontal head limbs, suggests limited post-mortem transportation: in, e.g. in extant Crustaceans, antennae can easily disarticulate. Compression wrinkles in the head shield that parallel its margin, suggest localised, weak sclerotisation. It is, therefore, presumed that the head shield was a simple, convex shield, sclerotised but without substantial biomineralisation.

As a result of the state of preservation, not all podomeres of the frontal appendages are accessible for a straightforward description. The exact number of podomeres cannot be established; some are obscured by sediment. Lateral endites can be confirmed for at least podomeres 2-7, 9, 11, 12, and medial endites bearing two firm setae at their tips can be confirmed for at least 4, 5, 7, 11, and 12. Rotation of podomere 2 evinces widely spaced double rows of endites.

Limbs with exopod setae are visible to the right of the two anterior-most thoracic tergites; the exopod of the posterior-most cephalic limb protrudes from beneath the head shield directly adjacent to the border of the head shield and first tergite, and is significantly rotated posteriorly, as is, albeit to a lesser extent the exopod of the first trunk limb. Only a single posteriorly situated endopod is, due to a degradation or complete absence of the overlying tergite, visible. No additional limbs were revealed by palaeontological techniques. The exact number of podomeres in the frontal appendages cannot be ascertained due to poor preservation of the distal-most ones. The proximal portions of the exopods are unavailable for description, so it cannot be established as to whether they were bipartite and divided into proximal and distal portions as in Leanchoilia illecebrosa.

Bushizheia yangi and Kiisortoqia soperi possess a long, grasping frontal appendage very similar to that of the Radiodonts. However, neither of these two species closely resemble Radiodonts. Could the presence of raptorial appendages in Bushizheia yangi and Kiisortoqia soperi be symplesiomorphic, shared by Bushizheia yangi and Kiisortoqia soperi, but also with Radiodonts linked earlier in the clade, to which Martin Stein alluded? Or are they an interesting case of convergence in organisms that are not closely related (not monophyletic), which independently evolved similar traits as a result of having to adapt to similar life habits?

It is beyond the scope of O'Flynn et al.'s study to attempt to solve the Arthropod head problem. Indeed, the preservation of Bushizheia yangi does not allow assessment of the neurological connection of the raptorial appendage. Hence, O'Flynn et al. only compare them to other appendages based on their morphology. Therefore, O'Flynn et al. explore the significance of the raptorial appendage of Bushizheia yangi and Kiisortoqia soperi in the context of some current interpretations of the homology of cephalic Arthropodan appendages; more precisely, the interpretation of the nature of the ‘great appendage’ of Radiodonts.

Many palaeontologists consider that the Radiodonts, and other ‘great appendage’ Arthropods belong to the lineage leading to Chelicerates, and the ‘great appendage’ is homologous to the chelicera. Following this line of reasoning, the presence of the ‘great appendage’ in Bushizheia yangi and Kiisortoqia soperi would, in this case, most likely be homologous to the ‘great appendage’ of radiodonts. The presence of this ‘great appendage’ would tie Bushizheia yangi and Kiisortoqia soperi, and ‘great appendage’ and ‘short-great appendage’ Arthropods together. More precisely, within this group, Bushizheia yangi and Kiisortoqia soperi and Radiodonts would be one of the sister groups of Chelicerates and ‘short-great appendage’ Arthropods. The problem being to reconcile the apparently primitive scarcity of sclerites displayed by Radiodonts with them being included in Euarthropoda, especially when considering that Bushizheia yangi and Kiisortoqia soperi are fully sclerotised. One solution to this problem would be to consider that Radiodonts subsequently lost part of their tergites, perhaps due to their nektobenthic life habits. The sclerotisation of Bushizheia yangi and Kiisortoqia soperi in this scenario would then represent a primitive trait.

Another, currently more widely held view, is that Radiodonts are not Euarthropods, but belong to a series of sister groups to Euarthropods (so called ‘Stem-Group’), which documents the progressive transition from weakly sclerotised, segmented Animals resembling Lobopodians to fully sclerotised Animals, the Euarthropods. However, the results of two important phylogenies supporting this theory were criticised in a 2011 study by Joachim Haug, Dieter Waloszek, Andreas Maas, Yu Liu, and Carolin Haug, due to apparent discrepancies in the coding of some characters and taxa. The debate on the nature of Radiodonts is not closed yet: several phylogenetic analyses published in the last decade support a ‘stem-group’ affinity for Radiodonts. In this scheme, Bushizheia yangi and Kiisortoqia soperi clearly belong to Euarthropods, and in this scenario the appendage similarity is either a convergence with the ‘great appendage’ of Radiodonts, or, the ‘great appendage’ was retained in early Euarthropods, and lost, or modified beyond recognition in most lineages of Euarthropods.

The convergence hypothesis agrees with the interpretation of Graham Budd, who considered the ‘great appendage’ to represent a pre-antennular appendage that was transformed into the labrum in the group including Euarthropods. If the hypothesis that the ‘great appendage’ was lost or reduced into the labrum is accepted, then the presence of ‘great appendage’-like frontal head limbs require convergence. Such convergence can be easily explained if Bushizheia yangi and Kiisortoqia soperi used their frontal head limbs in a fashion like predatory Radiodonts.

Contrary to this last hypothesis, the composition and morphology of the raptorial appendage of Bushizheia yangi bears a striking resemblance to the plesiomorphic state of the raptorial appendage within Radiodonts (i.e. the predatory, microphagous species). Other, probably distantly related species also have a seemingly similar raptorial appendage, e.g. the Bradoriid Kunmingella douvillei. This could give credence to the hypothesis that the great appendage was not reduced in a group including Euarthropods, but rather was lost or reduced in a group within Euarthropods.

In the case of Bushizheia yangi, since O'Flynn et al. do not have access to the ventral surface of the Animal, they cannot describe the position of the raptorial appendage. This prevents observation of the connection of this appendage to the head, and its exact nature. O'Flynn et al. can only hope that better preserved specimens may help to understand this animal better, and perhaps lead to a better understanding of the Arthropod head.

Despite its overall similarity to Kiisortoqia soperi and the morphological similarity of its appendages with those of the Radiodonts, the posterior of the animal is quite different. Disparity between Bushizheia yangi and Kiisortoqia soperi in this regard may well indicate that these are not closely related organisms. On a similar line of thought, similitude between Bushizheia yangi and Trilobitomorphs due to the presence of a pygidium could have been acquired by convergent evolution, an allusion to the conspicuous resemblance of the appendages of Aglaspidid-like Arthropods with those of the Nektaspid Naraoia spinosa. Alternatively, a plesiomorphic pygidium was retained in various Arthropod groups; such a scenario conflicts with several studies in which the presence of the pygidium is synapomorphic for a clade composed by Xandarellida, Nektaspida, Conciliterga, and Trilobita.

Artiopoda (e.g. Xandarellida, Nektaspida, Conciliterga and Trilobita) are arthropods with filiform antennulae. Bushizheia yangi is ipso facto outside Artiopoda, ergo the presence of the pygidium is not synapomorphic for a clade composed by the aforementioned groups. If the interpretation of a plesiomorphic pygidium is correct, this would indicate that this structure was retained in some Arthropod groups (e.g. Bushizheia yangi and Trilobitomorpha) but lost in many others.

A variety of Arthropods from the Chengjiang biota were most likely predators. The frontal head limbs of Bushizheia yangi are sturdy, predatory appendages, reminiscent of the ‘great appendage’ of Radiodonts. The presence of limbs posterior of these frontal head limbs that bear paddle-shaped exopods suitable for swimming could be indicative of a nektobenthic habit. No eyes could be found in the specimen. If the eyes in Bushizheia yangi were situated under the anterior border of the head shield, as in e.g. Leanchoilia illecebrosa, it is possible that they, together with the other ventral features of that area, were not preserved. The alternative hypothesis is that Bushizheia yangi was blind. Although visual perception in animals plays an important role in prey detection, other senses are used by animals in pinpointing their prey; the absence of eyes does not preclude Bushizheia yangi from being a predator. In the case where visual perception is lacking, Bushizheia yangi may have been an ambush predator, lying in wait, and catching unsuspecting prey with its anteroventral raptorial appendage.

Bushizheia yangi possesses a fully arthrodised body and limbs and consequently rests comfortably within the Euarthropoda. The present data neither confirms nor refutes any of the current interpretations of the homology of cephalic arthropodan appendages and although the phylogenetic position of Bushizheia yangi is difficult to resolve because few ventral structures are visible, the many Euarthropod plesiomorphies possessed by the taxon may indicate a basal position of the species, and it demonstrates the importance of fossils in characterising ground patterns.

The dorsoventrally flattened exoskeleton and paddle-shaped exopods that are suitable for swimming suggest a nektobenthic mode of life and Bushizheia yangi likely used its ‘great appendage’-like frontal head limbs for predation.

See also...

Online courses in Palaeontology. 

Follow Sciency Thoughts on Facebook.

Follow Sciency Thoughts on Twitter.

Wednesday, 30 December 2020

Residents evacuated after landslide hits village in Viken County, Norway.

Ten people have been injured, one of them seriously, and another eleven are missing after a landslide hit the village of Gjerdrum in Viken County, southern Norway, at about 4.00 am local time on Wednesday 30 December 2020. Several houses are reported to have been buried under mud and debris in the village, with others sliding into the hole created by the landslip, and about 900 people have been evacuated amid concerns about further landslips.

A landslide in the village of Gjerdrum in Viken County, southern Norway, on 30 December 2020. 30 December 2020. BBC.

The landslide is thought to have been of a type known as a 'quick clay' landslip, in which an entire bedding plain of clay loses its cohesion at once, and flows like a liquid, a type of landslide largely peculiar to areas of heavy Pleistocene glaciation, such as the northern coasts of Scandinavia, Russia, Alaska and Canada. Quick clay deposits were laid down in areas where the land was pushed down beneath sealevel by the weight of glaciers, and has subsequently been uplifted after the glaciers retreated. These clays typically contain far higher salt contents than other marine clays, which can be washed out by rainfall. Significantly, they generally contain significant levels of positively charged sodium cations, which entered the clay as the sea above froze, and help to bond the negatively charged clay particles together. However, sodium particles are particularly soluble in water, and easily washed out, with the effect that once a certain level of sodium has been lost, the entire bedding plane loses its cohesion.

See also...

Follow Sciency Thoughts on Facebook.

Follow Sciency Thoughts on Twitter.