Showing posts with label Starfish. Show all posts
Showing posts with label Starfish. Show all posts

Thursday, 24 November 2022

Acanthaster benziei: A new species of Crown-of-thorns Starfish from the Red Sea.

Crown-of-thorns Starfish, Acanthaster spp., are highly distinctive Starfish found across the tropical Indo-Pacific region from the east coast of Africa to the west coast of Mexico, which get their popular name from the covering of long, venomous spines found in most species. They are typically corallivorous, feeding on Coral Polyps by extruding their stomachs and digesting them externally. Notably, Crown-of-thorns Starfish can undergo sudden rapid population increases, known as outbreaks, which can lead to large areas of Coral Reefs being denuded of their living Polyps, something of great concern to conservationists at a time when Coral Reefs are facing a range of other threats, which has led to them being one of the most extensively studied groups of Marine Invertebrates.

Crown-of-thorns Starfish were first described by the German naturalist Georg Eberhard Rumphius in 1705, and given their own generic name, Acanthaster, by the French palaeontologist François Louis Paul Gervais  in 1841. For a long while, only two species were described within the genus, Acanthaster planci, the typical, long-spined, venomous, corallovorous form, and Acanthaster brevispinus, a shorter-spined, non-venomous form, which does not feed on Corals. However, genetic studies carried out within the past three decades have shown that Acanthaster planci is in fact a species cluster, made up of a number of physically very similar species (cryptospecies), which are nevertheless genetically distinct, which often appear to have diverged from one-another a long time ago. 

Based upon this, it was suggested that the original species should be split into four different species, each inhabiting a different geographical area; the Pacific, the Southern Indian Ocean, the Northern Indian Ocean and the Red Sea, which each of these species probably needing further division into several subspecies. Subsequent studies have indeed confirmed that the Pacific, North Indian Ocean, and South Indian Ocean populations are in fact separate species, although genetic material from the Red Sea population has not, until now, been available.

In a paper published in the journal Zootaxa on 17 November 2022, Gert Wörheide of the Department of Earth and Environmental Sciences Palaeontology and Geobiology, and the GeoBio-Center at Ludwig-Maximilians-Universität München, and the Bavarian State Collection of Palaeontology and Geology, Emilie Kaltenbacher and Zara-Louise Cowan, also of the Department of Earth and Environmental Sciences Palaeontology and Geobiology at Ludwig-Maximilians-Universität München, and Gerhard Haszprunar, also of the GeoBio-Center at Ludwig-Maximilians-Universität München, and of the Bavarian Zoological State Collections, describe the Red Sea population of Crown-of-thorns Starfish as a new population.

The new species is named Acanthaster benziei in honour of marine biologist John Benzie, for his extensive work on Crown-of-thorns Starfish. The description is based upon four specimens collected from species within the territorial waters of Saudi Arabia by  Sara Campana and OliverVoigt in 2017.

Typical colouration of Acanthaster benziei. (A) GW4081 (Paratype, hiding during the day under a crevice), Al-Lith, Saudi Arabia, (B)–(D) Thuwal Reefs, Saudi Arabia. Approximate diameter of specimens is 25–30 cm. Oliver Voigt & Gert Wörheide in Wörheide (2022).

Acanthaster benziei is a large Starfish with a convex disk and 11-14 arms (the range for the genus being 10-25), of uneven lengths, and tapering to a point. Each arm has two rows of ambulacral tube feet, which have flattened tips and lack suckers. The central disk of the species is 28-65 mm across, with an aboral (upper surface) covered in papulae (pimples) arranged in an apparently random manner. Both surfaces are covered in calcareous ossicles (plates) and spines. These Starfish are grey-green to grey-purple in colour, although the aboral spines are orange or red. The papulae on the aboral surface of the central disk can form darker patterns, giving this surface a 'bulls-eye' appearance.

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Tuesday, 16 June 2020

Astrolirus patricki: A new species of Sponge-associated Starfish, from the seamounts of the northwest Pacific.

Seamounts are deep-sea biomes in the global ocean which harbor diverse habitats and benthic communities. Sponges are one of the dominant benthic groups in seamount ecosystems, playing important ecological roles by providing habitat and settlement substrate for other seamount invertebrates, such as Molluscs, Hydrozoans and Echinoderms. Suspension-feeding Brittle Stars and Crinoids with long and flexible arms are often observed perching on or wrapped around Sponges. 

In a paper published in the journal PeerJ on 27 May 2020, Ruiyan Zhang of the School of Oceanography at Shanghai Jiao Tong University and the Key Laboratory of Marine Ecosystem Dynamics at the Second Institute of Oceanography of the Ministry of Natural Resources, Yadong Zhou, also of the Key Laboratory of Marine Ecosystem Dynamics at the Second Institute of Oceanography of the Ministry of Natural Resources, Ning Xiao of the Laboratory of Marine Organism Taxonomy and Phylogeny of the Institute of Oceanology and the Center for Ocean Mega-Science of the Chinese Academy of Sciences, and Chunsheng Wang, also of the School of Oceanography at Shanghai Jiao Tong University, the Key Laboratory of Marine Ecosystem Dynamics and the State Key Laboratory of Satellite Ocean Environment Dynamics at the Second Institute of Oceanography of the Ministry of Natural Resources, describe a new Starfish species, which was found attaching to deep-sea Sponges, based upon five specimens from northwestern Pacific seamounts.

Species of the family Brisingidae possess 7 20 spiny arms that are up to about 40 times the length of the disk radius. As exclusive deep-sea inhabitants, their long arms and spines potentially equip them to be excellent suspension feeders, stretching out and gathering food particles in the water column in the resource-diluted deep ocean. The Brisingidae is composed of 62 extant species designated into 10 genera. The genus Astrolirus currently contains only one species, Astrolirus panamensis, and is differentiated from the other genera based on the presence of intercostal plates on arms and a pair of marginal plates between the first adambulacral plates. Astrolirus panamensis was discovered in the eastern Pacific Ocean at 1820- 2418 m depth, with 1 eight-armed specimen and 27 nine-armed specimens of varying size (disc diameter 6- 26 mm) reported. Thereafter, Astrolirus has seldomly been reported or investigated. 

The new species is named Astrolirus patricki, in honour of the character `Patrick Star' in the famous cartoon `SpongeBob Squarepants', who always spends time with his best friend `SpongeBob', a benthic Sponge. Since all specimens of the new species were observed in situ living on Sponges, it was name by Patrick to reflect this curious relationship.

In situ photographs of Astrolirus patricki. Zhang et al. (2020).

All five specimens of the new species are seven-armed and were captured from Hexactinellid Sponges. Occasionally 2- 3 individuals were spotted on the same Sponge along with numbers of Ophiuroids and Crinoids. The new species differs greatly from Astrolirus panamensis in morphological characters and living habitat.

During the COMRA (China Ocean Mineral Resources R & D Association) cruises DY31, DY37, DY41, DY56 and a seamount cruise in the northwestern Pacific Ocean seamounts from 2013 to 2019, five specimens of the new species were collected by mechanical arms or siphon-pumps equipped on Human operated vehicles and remote operated vehicles. Specimens were photographed in situ and on board by digital cameras. Tube feet tissues were extracted from each specimen and frozen in -80°C refrigerator or liquid nitrogen for later molecular experiments, while other parts of specimens were preserved in 100% ethanol for morphological examinations. Morphological identification was conducted under a stereoscopic microscope. 

Astrolirus patricki has seven robust arms. The tntercostal integument is densely covered by irregular, abutting plates. There is no conection between proximal arm plates. The first pair of adambulacral plates is separated by a pair of marginal plates. A large interradial plate above the first marginal plates, is visible from the abactinal side, covered by scattered spinelets. The mouth spines and proximal adambulacral spines are robust, and densely distributed. There are 3-4 uboral spines and 1-2 subambulacral spines, the proximal ones of which are truncate and capitate. There is one lateral spine to each adambulacral plate, starting from about the 8th. There is a pair of gonads to each arm.

Astrolirus patricki, abactinal view. (A) Paratype RSIOAS028. (B) Paratype RSIOAS003. (C), (D), (H), holotype RSIOAS044, (C) Abactinal surface of disk and proximal part of arms, with red arrow pointing at the madreporite body, white arrow at the interradial plate and yellow arrows at the marginal plates. The red frame indicates the proximal region of arm connecting the disk and genital region, where pedicellariae do no form regular costae. (D) Abactinal surface of arm genital area with mosaic plating, red arrows show the costae bands. (E) Paratype RSIOAS003, abactinal surface of arm genital area, red arrows show the costae bands. (F) Paratype RSIOAS052, zoom in view of the abactinal disk, showing the multiple sharp spinelets on disk plates. (G) Paratype RSIOAS052, a piece of dissected skin from abactinal disk, shot from the inner side of the skin, showing the small round disk plates. (H) Abactinal surface at the middle of arm, black arrows indicate the pedicellariae bands. Zhang et ai. (2020).

See also...

https://sciencythoughts.blogspot.com/2019/08/asterodiscides-fourmanoiri-starfish.htmlhttps://sciencythoughts.blogspot.com/2019/01/acanthaster-solaris-using-environmental.html
https://sciencythoughts.blogspot.com/2019/01/sertulaster-keslingi-and-delicaster.htmlhttps://sciencythoughts.blogspot.com/2018/03/thousands-of-starfish-wash-up-on.html
https://sciencythoughts.blogspot.com/2016/02/estimating-role-of-temperature-in-sea.htmlhttps://sciencythoughts.blogspot.com/2013/12/a-mass-death-of-starfish-in-late.html
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Friday, 3 January 2020

Understanding enrolment behaviour in Chitons.

The ability of armoured animals to roll into a defensive ball is known from many disparate groups. This ability, called conglobation or enrolment, is known from Mammals such as Pangolins, Manidae, and Hedgehogs, Tenrecinae, and Echidna, Tachyglossidae, Arthropods including some Isopods, Trilobites, Pill Millipedes and larvae of other groups, and, among Molluscs, the multi-shelled Chitons. These animals have the flexibility to curve their entire body and touch the anterior to the posterior end, such that the hard dorsal elements cover the whole outer surface and the softer, ventral parts are protected inside the ball. Species with this ability span a broad variety of ecological niches and both terrestrial and aquatic environments; while the ability to display protective armour in every direction is doubtless beneficial to defence, the ability to become more spherical may have additional and more relevant implications in terms of functional morphology. Chitons are unusual among ball-forming invertebrate animals in that they entirely lack mechanisms that lock the body in the enrolled position. By contrast, many Trilobites, Oniscoid Isopods and Millipedes have intricate locking (or coaptive) devices that are modifications of the exoskeleton. Many of these ball-forming taxa with coaptive devices protect legs, antennae and reproductive structures, and at least some develop spines that protrude outward when the animal is in the enrolled position. Spines provide an additional defence against gape-limited predators, and in aquatic contexts may affect hydrodynamic dispersal. Conglobation with coaptive devices is common among living terrestrial arthropods, but is essentially unknown in living adults in the sea, perhaps implying that passive defence in the form of coaptive rolling up into a ball is no longer as effective as it once was during the Paleozoic heyday of the Trilobites.

In a paper published in the journal Biology Letters on 2 October 2019, Julia Sigwart of the Marine Laboratory at Queen’s University Belfast, Geerat Vermeij of the Department of Earth and Planetary Science at the University of California, Davis, and Peter Hoyer, also of the Marine Laboratory at Queen’s University Belfast, present the results of a study in which they  applied an experimental approach to test the response of dislodged Chitons with and without exposure to the threat of potential predation.

A Chiton attached to the substratum by its soft foot is well defended by its dorsal scleritome and will respond to disturbance by holding fast to the surface. The Chiton scleritome and its overlapping plates have been analysed as an armour that optimizes a trade-off between defence and mobility. When rolled into a ball, the valves and girdle together provide a complete armour, although much of the ‘ball’ is muscular tissue covered only by a thin cuticle. The potential predators in modern shallow marine settings, including Fish, Seastars, Birds and Crabs, are likely to consume an unattached Chiton whole. Anecdotal speculation has suggested the primary advantage of curling into a ball could instead be mobility, to allow Chitons to roll to a better position. This implies that enrolment is not a passive defence against attack, but perhaps a strategy to improve circumstances. If the tendency of armoured marine animals to roll into a ball is a passive defensive behaviour, then Chitons could be expected to spend relatively more time curled up in the presence of a predator, but if it is not then Chitons should spend less time enroled when a predator is nearby.

A Chiton, Mopalia swanni, in (a) in normal position, and (b) rolled into a ball, anterior is at top in both images. This species was not used in this experiment but shown for illustrative purposes. Sigwart et al. (2019).

Live Chitons were collected from the intertidal at Pinnacle Gulch in Bodega Bay, California and held in aquaria on flowthrough seawater at the University of California, Davis' Bodega Marine Laboratory. Chitons used in these experiments included three species: Mopalia hindsii (17 seventeen specimens), Mopalia muscosa (4 specimens), and Lepidozona mertensii (3 specimens). These species co-occur in the rocky intertidal in Northern California and are broadly distributed on the Pacific coast of North America. The Purple Sea Star, Pisaster ochraceus was selected to produce the predator cue as it is a co-occurring predator known to consume Chitons.

In each trial, a single randomly selected Chiton was placed up-side-down in the centre of the experimental aquarium. Seawater was siphoned continuously from one of two sources, selected by a coin flip: the 40 litre holding aquarium with captive Chitons (control condition), or a separate 20 litre aquarium holding a single Purple Sea Star (predator treatment). These two source aquaria were fed continuously with flow-through seawater. 

Chitons left up-side-down on a flat surface were never able to right themselves, except by manoeuvring close enough to the wall to contact and attach to the vertical surface. This occurred four
times in 24 trials, three of which were in the presence of the predator cue; the control animal that made contact with the side did so only after 109 minutes of a 120-minute trial, while animals in the predator treatment that manoeuvred themselves to the side did so relatively much faster, after 43–87 minutes.

Left in a prone orientation, Chitons adopted the enrolment position around 30% of the time overall; however, there was a strong association between the predator cue and time spent arching. The odds of an individual spending time in a ball are 2.85 times higher without a predator cue. In the presence of a predator cue, the odds of an individual Chiton spending time arching are 2.93 times higher. 

The sample sizes for Lepidozona mertensii (3 specimens) and Mopalia muscosa (4 specimens) were too small to allow robust comparison among species, although the trends were apparently broadly consistent in all three species used. Lepidozona mertensii spent more time overall curled into a ball, compared to the total group, and spent considerably more time rolled in the control condition  than in the presence of a predator cue.

In the presence of the chemical cue of a distant predator, the urgent pressure to reattach to the substratum prompted more exposed positions in Chitons, but that would (and in a few cases did) enable the animal to reattach to the substratum and regain normal posture. Chitons are not able to right themselves on an isolated, flat surface such as the bottom of an experimental aquarium. But extended flat surfaces and still water are unusual in the context of rocky marine benthos. The articulating armour of Chitons is flexible and the inability of chitons to right themselves is generally limited to environments with flat surfaces and no current. In normal circumstances, on a rugose surface in a dynamic environment with moving water, a rolled-up chiton can expect to be transported to a new position very rapidly, and an arching Chiton might also be buffeted more rapidly toward a potential safe haven. Although Chitons are often considered ‘primitive’, there is mounting evidence for neurological complexity and this behaviour suggests a certain level of strategic response.

The behaviour associated with conglobation has been studied most closely in Arthropods, especially the terrestrial Pill Bug, Armadillidium sp., which can roll into a completely sealed ball. In experimental exposure, Isopods were marginally more likely to be attacked when extended rather than when rolled into a ball, and the animals do use conglobation as an active response to attack by potential predators. Likewise, a dislodged Chiton, if physically prodded, would also roll up rather than arch and leave the foot exposed. Conglobation in Isopods has secondary advantages in that it may help prevent desiccation as well as predation, which would only be relevant for Chitons in the rare event of dislodgement when exposed to air at a low tide. There are certainly protective benefits to curling into a ball, but the ball configuration in Chitons and other animals is entirely incompatible with normal feeding and locomotion.

Some arthropods lack coaptive devices that lock the ball configuration, including a few terrestrial Caterpillars and Spiders. These animals roll into a wheel-like configuration and use powerful appendages to propel themselves away from danger. This situation, and the observation that the ability to roll into a ball is associated with rolling away from a disadvantageous situation rather than with direct or even indirect contact with a predator, is mirrored in Sigwart et al.'s observations of chitons. Whether energy-intensive as in these terrestrial Arthropods, or more passive, as in Chitons, rolling away evidently does not require coaptive devices and is more a temporary measure.

In Chitons, the action of enrolment is controlled by the diagonal dorsoventral muscles that connect the eight shell valves to the ventral foot. All Chitons are able to use anterior–posterior flexing, including species with reduced or internal shells (such as Cryptochiton stelleri). This muscular arrangement and additional longitudinal muscles also cause the typical curled posture in Aplacophoran Molluscs, which are anatomically and phylogenetically related to Chitons. This is in contrast to the coaptive interlocking exoskeletal elements involved in the conglobation postures of Arthropods. Although the shell-less condition in Aplacophorans is derived, curling does not require an exoskeleton and does not require physical coaptive devices.

The ability of animals to transform into a defended sphere is a solid defence with multiple benefits; however, the results here suggest that anti-predatory defence is not the principal merit for Chitons. Chitons demonstrate behavioural decision-making when faced with the threat of a potential predator, to enable it to right itself and regain a safe foothold. By contrast, some other species with coaptive mechanisms resist attack by a predator through special morphological features that strengthen the exoskeleton and make it difficult to manipulate for a gape-limited or skeleton-breaking predator. The rolled-up configuration in Chitons and other animals without coaptive devices is superficially convergent, but the similarity in these different forms of rolling up may hide fundamentally different approaches to defence.

See also...

https://sciencythoughts.blogspot.com/2020/01/shellfish-use-at-oakhurst-period-at.htmlhttps://sciencythoughts.blogspot.com/2019/12/unloved-paraphyletic-or-misplaced.html
https://sciencythoughts.blogspot.com/2019/10/eromangateuthis-soniae-large-fossil.htmlhttps://sciencythoughts.blogspot.com/2019/10/modiolus-cimbricus-new-species-of.html
https://sciencythoughts.blogspot.com/2019/08/washington-woman-hospitalised-by.htmlhttps://sciencythoughts.blogspot.com/2019/07/royal-canadian-mounted-police.html
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Tuesday, 15 October 2019

Modiolus cimbricus: A new species of Mussel from the Kattegat-Skagerrak Straight.

Mussels, Mytilidae, are a large, and highly successful group of Bivalve Molluscs found from the coastal shorelines to the deep ocean. They are particularly prominent cooler waters, where they form vast banks in shallow waters, making them a major shaper of the environment. Mussels are noteworthy for the production of a byssus, a thread by which they attach themselves to the substrate. 

In a paper published in the European Journal of Taxonomy on 24 September 2019, Kurt Ockelmann of the Marine Biological Laboratory at the University of Copenhagen, and Tomas Cedhagen of the Section of Aquatic Biology at Aarhus University, describe a new species of Mussel from the Kattegat-Skagerrak Staraight, the body of water that separates Denmark from Scandinavia and the North Sea from the Baltic.

The new species is placed in the genus Modiolus, and given the specific name cimbricus, in reference to the ancient Cimbrican people of northern Jutland. The species is described from a population previously known, but assigned to Modiolus adriaticus, a warm-water species no longer thought to be found this far north. The species has colourful asymmetric shells which can reach about 25 mm in length, although this size is seldom reached, with the Mussels becoming sexually mature after a year, when they are 4-6 mm in length.

Modiolus cimbricus, shell length 13.3 mm. The upper part of the fi gure shows the external shell side and the lower part shows the inner side of the valves. Scale bars are 5 mm. Ockelmann & Cedhagen (2019).

Modiolus cimbricus typically lives enwrapped in a ball of its own byssus threads, studded with particles of sand and other material. This is probably a defence against Starfish, voracious marine predators which are specialist Mussel-eaters, pulling their shells open by modifying their tube feet to form suction disks, then inserting their stomachs through the gaps to digest the Mussels. Attaching material to the outside of the shell is known to make such attacks harder, so the extensive covering of Modiolus cimbricus should be a good defence.

Modiolus cimbricus. A 17.5 mm long specimen in its ball of sand grains. This specimen has been cultured for fi ve years. Scale bar is 5 mm. Ockelmann & Cedhagen (2019).

Modiolus cimbricus is one of a high number of endemic species (species found nowhere else) known from the Baltic, Kattegat and Skagerrak regions. All endemic species and populations in the Baltic Sea must have evolved after the Weichselian Glaciation, between 115 000 and 11 700 years ago, when the Baltic was covered by an ice sheet. Speciation in the region can be very fast, for example the Brown Alga Fucus radicans evolved during the last four hundred years. Most marine species are unable to survive in the brackish water of the Baltic, enabling populations that find a way to survive to rapidly radiate into new niches.

Ockelmann and Cedhagen consider it highly likely that Modiolus cimbricus has evolved since the Weichselian Glaciation from a founder population of Modiolus adriaticus. The latter species forms part of a Mediterranean-centred population that reaches as far north as the English Channel and Irish Sea, where warm waters from the Gulf Stream circulate, but cut off from the Kattegat by the colder, Arctic-influenced waters of the North Sea. However, occasionally the autumn sees warm water packages from the Bay of Biscay move up the English Channel and into the southern North Sea, and one of these could conceivably have carried the ancestors of Modiolus cimbricus to the Kattegat.

See also...


https://sciencythoughts.blogspot.com/2019/01/molluscs-from-early-cambrian-shackleton.htmlhttps://sciencythoughts.blogspot.com/2018/12/novaculina-myanmarensis-new-species-of.html
https://sciencythoughts.blogspot.com/2018/09/british-and-french-fishing-fleets-clash.htmlhttps://sciencythoughts.blogspot.com/2018/05/meganodontia-haunuiensis-elliptiolucina.html
https://sciencythoughts.blogspot.com/2017/08/a-hydrocarbon-seep-from-late-triassic.htmlhttps://sciencythoughts.blogspot.com/2017/05/kuphus-polythalamia-can-giant-free.html
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Sunday, 4 August 2019

Asterodiscides fourmanoiri: A Starfish known only from southern Madagascar reported off the coast of Pakistan.

Starfish (Asteroidea) are benthic marine Echinoderms found across the globe. They have a simple bodyplan, with a central disk that has the mouth on the underside, surrounded by (usually) five arms, each with a double row of tube feet underneath. The upper surface of the Starfish is covered by an articulated armoured exoskeleton made up of thousands of small calcite plates. The animal moves by means of a water vascular system, which enables it to inflate and deflate the tube feet as required. There are currently around 1900 described species of living Starfish, grouped into 370 genera. The genus Amphiaster contains eighteen species of deepwater Starfish found in the Indian and western Pacific oceans, including Asterodiscides fourmanoiri, which is known only from waters off the Sainte Luce Reserve in southeast Madagascar.

In a paper published in  the Summer 2019 edition of Iranian Journal of Fisheries Sciences, Mohammad Reza Mirzaei, Arezoo Vahabnezhad and Fereidoon Owfi of the Iranian Fisheries Science Research Institute, record the presence of Asterodiscides fourmanoiri on the southern coast of Pakistan.

Mirzaei et al. report discovering Asterodiscides fourmanoiri living at a depth of between 83 and 85 m on a sand and rock seafloor trawl near Gwadar Bay in the northern Oman Sea, based upon a single specimen recovered from a sample trawl by the Research Vessel Ferdows in October 2016. This represents a significant extension of the known range of the species, making it likely that it is found elsewhere in the waters of the Indian Ocean.

Specimen of Asterodiscides fourmanoiri recovered from the coast of Pakistan in 2016. Mizaeri et al. (2019).

See also...

https://sciencythoughts.blogspot.com/2019/01/acanthaster-solaris-using-environmental.htmlhttps://sciencythoughts.blogspot.com/2019/01/sertulaster-keslingi-and-delicaster.html
https://sciencythoughts.blogspot.com/2018/03/thousands-of-starfish-wash-up-on.htmlhttps://sciencythoughts.blogspot.com/2016/02/estimating-role-of-temperature-in-sea.html
https://sciencythoughts.blogspot.com/2013/12/a-mass-death-of-starfish-in-late.htmlhttps://sciencythoughts.blogspot.com/2012/11/coral-decline-on-great-barrier-reef.html
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Tuesday, 15 January 2019

Acanthaster solaris: Using Environmental DNA to track the Crown-of-Thorns Starfish.

The Great Barrier Reef on Australia’s east coast is the world’s largest marine protected area, a World Heritage Site and a biodiversity hotspot of global importance. Despite this, the reef is estimated to have lost more than 50% of its Corals during the past three decades. Much of this is due to global warming, and the accompanying acidification of the seawater, but other factors are important. One of these has been repeated outbreaks of the Crown-of-Thorns Starfish, Acanthaster solaris, a Coral-consuming Echinoderm credited with having caused 42% of Coral loss on the Great Barrier Reef prior to the bleaching events of 2016-17. The Crown-of-Thorns Starfish has entered a boom-and-bust population cycle since the 1960s, with outbreaks producing huge numbers of Starfish that consume all the available food (i.e. Coral) then die out due to starvation. The precise cause of these booms is unclear, but probably linked to the life-cycle of the Starfish, which produce planktonic larvae, with the most likely explanation being greater numbers of larvae surviving because of increased food availability due to nutrients from agricultural runoff, or increased larval survival due to a reduced number of predators caused by overfishing. This makes Starfish booms of great interest to conservationists trying to protect the Great Barrier Reef, who need to detect new outbreaks as quickly as possible in order to take remedial action.
 
 An adult Crown-of-Thorns Starfish predating Coral. Hall et al. (2017).
 
In a paper published in the journal Coral Reefs on 12 September 2018, Sven Uthicke of the Australian Institute of Marine Science, Miles Lamare of the Department of Marine Science at the University of Otago, and Jason Doyle, also of the Australian Institute of Marine Science, describe the results of a trial of a method which used environmental DNA to track populations of the Crown-of-Thorns Starfish.

Environmental DNA (or eDNA) is DNA shed into the environment by an organism via shed skin cells, and excretion of mucus, urine or faeces. The detection of eDNA has become a standard methodology for detecting invasive of endangered species in freshwater environments, but the much larger volume of the oceans, which means that the eDNA will be significantly more diluted by the water, makes detecting eDNA in marine environments considerably harder, and the technique has yet to be successfully applied in this setting.

In order to establish the amount of eDNA produced by Crown-of-Thorns Starfish a single individual was placed in a 10 000 litre seawater tank at the Australian Institute of Marine Science’s National Sea Simulator. This tank had continuous through-flow of water at a rate that would replace all the water twice a day, and the Starfish was kept in it and monitored for one week. This was then repeated with two Starfish, then three, up to a maximum of sixteen, in order to calibrate the methods used for eDNA detection.

Seawater was then collected on four field trips between June 2016 and August 2017, covering reefs in the Cooktown, Innisfail and Ingham to Townsville regions, and tested for levels of Crown-of-Thorns Starfish eDNA. The areas covered included two reefs where there had previously been Starfish outbreaks, two where the Starfish had never been observed, five reefs with active outbreaks, and two reefs without outbreaks, but which were 50-65 km from a reef where and outbreak was ongoing.

No Crown-of-Thorns Starfish eDNA was detected at any site where the Starfish were not present, but it was found in the samples from all the reefs where the Starfish were observed. Furthermore, the levels of eDNA found in the samples closely reflected the known densities of Starfish on these reefs, indicating that the test is both a viable method for detecting the Starfish and a reliable way to estimate their population density.

Density estimates of Acanthaster solaris (left) and eDNA concentration on 11 reefs of the Great Barrier Reef, Australia. Uthicke et al. (2018). 

See also...

http://sciencythoughts.blogspot.com/2019/01/heliopora-hiberniana-second-species-of.htmlhttp://sciencythoughts.blogspot.com/2019/01/hana-hanagasa-and-hana-hanataba-two-new.html
http://sciencythoughts.blogspot.com/2019/01/sertulaster-keslingi-and-delicaster.htmlhttp://sciencythoughts.blogspot.com/2019/01/mesophotic-coral-reefs-from-middle.html
http://sciencythoughts.blogspot.com/2018/04/adelogorgia-osculabunda-adelogorgia.htmlhttp://sciencythoughts.blogspot.com/2018/03/thousands-of-starfish-wash-up-on.html
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Thursday, 10 January 2019

Sertulaster keslingi and Delicaster hotchkissi: Two new species of Starfish from the Ordovician and Carboniferous of eastern North America.

Starfish, Asteroidea, are important members of benthic invertebrate communities, often playing a major role in shaping marine ecosystems. They have a long fossil record, having first appeared in the Ordovician, but this record is extremely sparse due to the nature of their exoskeletons, which are made up of large numbers of tiny elements, which become disarticulated very easily upon the death of the animal, and when fossils are exposed at the surface. This makes it very hard to understand the evolutionary history of Starfish as a group, due to the limited number of preserved skeletons.

In a paper published in the Journal of Paleontology on 7 November  2018, Daniel Blake of the Department of Geology at the University of Illinois, and Joseph Koniecki of Ann Arbor in Michigan describe two new species of Starfish from the Ordovician and Carboniferous of eastern North America.

The first new species is named Sertulaster keslingi, where ‘Sertulaster’ means ‘garlanded star’ in reference to the primary circlet of skeletal plates, which resembles a garland, and ‘keslingi’ honours palaeontologist Robert Kesling for his work on ancient Starfish and other Echinoderms. The species is described from four partially complete specimens, one from the Verulam Formation at the LaFarge Belleville Quarry, near Belleville in Ontario, and three from the upper Bobcaygeon Formation of the Kirkfield Quarry at Kirkfield, Ontario; both formations are Late Ordovician in age. These specimens have an arm-tip radius of up to 15 mm, and a body radius of up to 5 mm.

(1)–(6) Sertulaster keslingi, family Palaeasteridae; specimens wetted to delineate ossicular shapes and arrangements. Surfaces are finely pustulate but enlarged spine bases are lacking. (1)–(3) Holotype UMMP 74694: (1) complete specimen, central disk ossicles lost or collapsed into disk interior; arrow at superomarginal (SM) series; (2) inclined view, inset primary circlet interradial (upper arrow) abuts two radials, primary circlet does not include supplemental ossicles; the interradial bears two ventrally directed flanges and is separated by two upright disk superomarginals from axillary (lower arrow), which lies between two arm marginal series; no intermarginal series is developed; (3) dorsal aspect, radial (arrow) at head of carinal series. (4) Paratype UMMP 74695, arrow at SM series; (5) paratype UMMP 74696, left arrow at SM series, right arrow at axillary, is beneath enlarged disk SM pair; (6) paratype UMMP 74697, arrow at SM series. (7) Eriaster ibexensis, is most similar to Sertulaster among known palaeasterid genera; overall view of holotype; primary circlet ossicle (left arrow) is subcircular and pustulate; enlarged carinal series ossicles extend to the arm tip and overlie marginal and intermarginal series (right arrow. Scales bars are 5 mm. Blake & Konieki (2018). 

The second species described is placed in the genus Delicaster, and given the specific name hotchkissi, in honour of palaeontologist Frederick Hotchkiss for his work on Starfish and other Echinoderms, including obtaining the specimen from which Delicaster hotchkissi is described. The species is described from a single specimen from the shale above the Willow Point Limestone Member of the Pennsylvanian (Carboniferous) Canyon Series at Bridgeport Clay Pit in Wise County, Texas. This specimen has a maximum arm radius of about 30 mm and an inner body radius of 12 mm, though this is likely to have been increased by flattening during burial.

Delicaster hotchkissi, holotype and only known specimen, YPM IP 238703. The two columns of figures illustrate the opposite surfaces of the single-known specimen, rotated 180° about the “vertical” axis. Disk ossicles are in disarray although arm intervals are largely intact. (1) The two more complete arms showing primarily marginal and ambulacral ossicular form in dorsal aspect, axillaries at arrows; (2) axillary at left arrow, madreporite immediately beyond axillary at right arrow; (3) disk region, ossicles largely disrupted; axillaries marked by two upper arrows, madreporite near upper left arrow; primary circlet ossicles and adradial face of ambulacral at two lower right arrows; (4) arm to left exposes the ventral surface; arm to right is exposed in dorsal view, folded across the ventral disk surface; adambulacral series at upper right arrow belongs to an arm obscured by the folded arm; lower arrows locate adambulacral ossicles; (5),upper left arm; adambulacral double series along midline is partially obscured and disrupted; adambulacral spines at arrow; (6) proximal interval of folded arm, partially displaced axillaries at arrows to left; small pustules along dorsal edge of marginals (middle arrow); adambulacral series in ventral view, ossicular outlines rectangular with transverse series of spine bases (right arrow). Scale bars are 10 mm. Blake & Konieki (2018).

See also...

https://sciencythoughts.blogspot.com/2018/03/thousands-of-starfish-wash-up-on.htmlhttps://sciencythoughts.blogspot.com/2016/02/estimating-role-of-temperature-in-sea.html
http://sciencythoughts.blogspot.com/2014/12/a-new-species-of-brittle-star-from.htmlhttp://sciencythoughts.blogspot.com/2014/06/a-new-species-of-brittle-star-from.html
https://sciencythoughts.blogspot.com/2013/12/a-mass-death-of-starfish-in-late.htmlhttps://sciencythoughts.blogspot.com/2012/11/coral-decline-on-great-barrier-reef.html
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