Saturday, June 25, 2022

CTHULHU STUDIES

The octopus’ brain and the human brain share the same “jumping genes”


A new study has identified an important molecular analogy that could explain the remarkable intelligence of these invertebrates

Peer-Reviewed Publication

SCUOLA INTERNAZIONALE SUPERIORE DI STUDI AVANZATI

Octopus 

IMAGE: DRAWING OF AN OCTOPUS view more 

CREDIT: GLORIA ROS

The octopus is an exceptional organism with an extremely complex brain and cognitive abilities that are unique among invertebrates. So much so that in some ways it has more in common with vertebrates than with invertebrates. The neural and cognitive complexity of these animals could originate from a molecular analogy with the human brain, as discovered by a research paper recently published in BMC Biology and coordinated by Remo Sanges from SISSA of Trieste and by Graziano Fiorito from Stazione Zoologica Anton Dohrn of Naples. The research shows that the same 'jumping genes' are active both in the human brain and in the brain of two species, Octopus vulgaris, the common octopus, and Octopus bimaculoides, the Californian octopus. A discovery that could help us understand the secret of the intelligence of these fascinating organisms.

Sequencing the human genome revealed as early as 2001 that over 45% of it is composed by sequences called transposons, so-called 'jumping genes' that, through molecular copy-and-paste or cut-and-paste mechanisms, can 'move' from one point to another of an individual’s genome, shuffling or duplicating. In most cases, these mobile elements remain silent: they have no visible effects and have lost their ability to move. Some are inactive because they have, over generations, accumulated mutations; others are intact, but blocked by cellular defense mechanisms. From an evolutionary point of view even these fragments and broken copies of transposons can still be useful, as 'raw matter' that evolution can sculpt.

Among these mobile elements, the most relevant are those belonging to the so-called LINE (Long Interspersed Nuclear Elements) family, found in a hundred copies in the human genome and still potentially active. It has been traditionally though that LINEs’ activity was just a vestige of the past, a remnant of the evolutionary processes that involved these mobile elements, but in recent years new evidence emerged showing that their activity is finely regulated in the brain. There are many scientists who believe that LINE transposons are associated with cognitive abilities such as learning and memory: they are particularly active in the hippocampus, the most important structure of our brain for the neural control of learning processes.

The octopus’ genome, like ours, is rich in 'jumping genes', most of which are inactive. Focusing on the transposons still capable of copy-and-paste, the researchers identified an element of the LINE family in parts of the brain crucial for the cognitive abilities of these animals. The discovery, the result of the collaboration between Scuola Internazionale Superiore di Studi Avanzati, Stazione Zoologica Anton Dohrn and Istituto Italiano di Tecnologia, was made possible thanks to next generation sequencing techniques, which were used to analyze the molecular composition of the genes active in the nervous system of the octopus.

“The discovery of an element of the LINE family, active in the brain of the two octopuses species, is very significant because it adds support to the idea that these elements have a specific function that goes beyond copy-and-paste,” explains Remo Sanges, director of the Computational Genomics laboratory at SISSA, who started working at this project when he was a researcher at Stazione Zoologica Anton Dohrn of Naples. The study, published in BMC Biology, was carried out by an international team with more than twenty researchers from all over the world.

“I literally jumped on the chair when, under the microscope, I saw a very strong signal of activity of this element in the vertical lobe, the structure of the brain which in the octopus is the seat of learning and cognitive abilities, just like thehippocampus in humans,” tells Giovanna Ponte from Stazione Zoologica Anton Dohrn.

According to Giuseppe Petrosino from Stazione Zoologica Anton Dohrn and Stefano Gustincich from Istituto Italiano di Tecnologia “This similarity between man and octopus that shows the activity of a LINE element in the seat of cognitive abilities could be explained as a fascinating example of convergent evolution, a phenomenon for which, in two genetically distant species, the same molecular process develops independently, in response to similar needs.”

“The brain of the octopus is functionally analogous in many of its characteristics to that of mammals,” says Graziano Fiorito, director of the Department of Biology and Evolution of Marine Organisms of the Stazione Zoologica Anton Dohrn. “For this reason, also, the identified LINE element represents a very interesting candidate to study to improve our knowledge on the evolution of intelligence.”

This Ancient Vampire of The Deep Ocean Really Sucked

MICHELLE STARR
23 JUNE 2022

Artist's impression of Vampyronassa rhodanica. (A. Lethiers, CR2P-SU)

A fearsome 'vampire' predator that lurked in Earth's oceans more than 160 million years ago probably did actually suck its prey, at least in a sense.

A new analysis of exceptionally well-preserved fossils of a small cephalopod named Vampyronassa rhodanica, related to modern vampire squids (neither actually vampires, nor squids), reveals the presence of muscular suckers that the beastie likely used for snaring and manipulating prey.

In other words, it was an active predator, hunting the pelagic depths for tasty morsels.

This is in direct contrast to the animal's present relatives, Vampyroteuthis infernalis, whose suckers seem largely non-functional, and which collect drifting flakes of organic material using sticky cells on a pair of specialized, thread-like appendages.

"The contrast in trophic niches between the two taxa is consistent with the hypothesis that these forms diversified in continental shelf environments prior to the appearance of adaptations in the Oligocene leading to their modern deep-sea mode of life," writes a team of researchers led by paleontologist Alison Rowe of Sorbonne University in France.

Mushy animals like cephalopods are pretty scarce in the fossil record. Soft tissues don't fossilize as readily or well as bones, which makes fossils, especially good fossils, very rare.

Rare doesn't mean nonexistent, however, and Rowe and her colleagues were able to study three V. rhodanica fossils from a lagerstätte (sedimentary deposit) dating back to over 160 million years ago in La Voulte-sur-Rhône in France. This is a type of very fine sedimentary fossil bed that is exceptionally good at preserving fossils, including soft tissue.

Even soft tissue preserved in this way isn't always easy to parse. To understand the anatomy of V. rhodanica, Rowe and her team took the fossils to the European Synchrotron Radiation Facility in France to undergo non-invasive 3D imaging.

One of the exceptional fossils of V. rhodanica. (P. Loubry, CR2P)

"The fossils are on small slabs, which are very difficult to scan," Rowe explains.

"On top of that, soft tissues are preserved but we needed phase contrast imaging to visualize the faint density variation in the data. The coherence of ESRF beamline ID19 was therefore very important to perform propagation phase-contrast computed-tomography and track all the minute details, such as the suckers and small fleshy extensions, called cirri."

The scans revealed some interesting differences between V. rhodanica and V. infernalis, which is now the only living member of the Vampyromorph order.

Both are relatively small (the former just 10 centimeters or 4 inches in length), with oval bodies flanked by two small fins. Both also have small, fleshy projections called cirri emerging from their arms.

Yet there were no signs of the thread-like food snares on any of the V. rhodanica fossils – instead an extended pair of arms with a unique arrangement of suckers.

On the tips of these two specialized dorsal arms, it sports more robust, muscular cirri and suckers. V. infernalis has smaller cirri, and its suckers appear only on the ends of their arms farthest from their bodies. What's more, they appear to be passive; it doesn't use them for grasping prey.

"We believe that the morphology and placement of V. rhodanica suckers and cirri in the differentiated arm crown allowed V. rhodanica increased suction and sensory potential over the modern form, and helped them to manipulate and retain prey," Rowe says.

In other words, V. rhodanica has the equipment to be an active predator in the pelagic seas, with more sensitive sensory organs and the ability to grasp prey. V. infernalis is more peaceful and opportunistic.

Although related, the two species occupy different ecological niches... neither of which is actually anything to do with vampirism. Oh well.

By the Oligocene, about 30 million years ago, vampire squids were already in the depths, lurking about, waiting for organic debris to rain down into their hungry arms.

Sometime in the intervening millions of years, vampire squids made a significant lifestyle change. How and why this happened will need to be the subject of future research… if the fossils can be found.

The team's research has been published in Scientific Reports.


X-rays reveal the strange appendage this ancient vampire squid used to hunt

New technology makes it possible to glean a lot more information from rare fossils.


By Grant Currin
Jun 24, 2022


The modern vampire squid is a cryptic creature. It lives a slow life deep in the ocean — far from shore — where it makes a living by scavenging on whatever dead things happen to sink past it on their journey to the ocean floor. 

Was life always this way? That's a hard question to answer for animals like squid, octopuses, and cuttlefish because those creatures (a group of evolutionary cousins called "coleoids") are defined by what they don't have: a hard shell. That means they don't have body parts that lend themselves to becoming a fossil. Conditions have to be just right for a coleoid's soft body to make it into the fossil record.

That's why a new paper, published Thursday in the peer-reviewed journal Scientific Reports, is a big deal. Paleontologist Alison Rowe and her team used 3D imaging to analyze rare fossilized remains of an extinct relative of the vampire squid. Their findings suggest that Vampyronassa rhodanica may have been a bit more, well, vigorous. Their results point to a fearsome eight-armed hunter that likely captured prey with a pair of powerful suction cups.

Interesting Engineering sat down with Rowe to discuss the study, what they learned about Vampyronassa rhodanica, and what that new information reveals about the ancient oceans. 

This interview has been edited for length and clarity.

Interesting Engineering: How did you and your co-authors carry out this study?

Alison Rowe: In this study, we utilized powerful X-ray imaging techniques to scan fossil and modern specimens. This allowed us to observe previously unseen internal structures of the fossils, as well as view the external soft tissue anatomy with much better resolution.

From the comparative analysis between the fossil and extant form, we can show for the first time that there was a combination of anatomical characters in V. rhodanica that aren’t seen today. This research provides a small window on the diversity of character combinations that occurred in the Jurassic that are now lost.

IE: In the paper, you compare V. rhodanica to the modern-day vampire squid. For context, can you give us a crash course on the vampire squid and its relatives? 

Rowe: The vampire squid is actually not a squid. It is closer to octopuses than to squids.  Like the octopus, it has 8 arms, but also two filaments that are developmentally homologous to arms, which makes it somewhat comparable to squid or cuttlefish (Decabrachia) that have 10 arms. It has cirri on the arms like the incirrates [a suborder of the order Octopoda]. It has its own characteristics such as its type of sucker attachment, and its gladius, which is a kind of internal organic shell.

It is uniquely adapted to living in the deep sea, often in areas of low oxygenand is an opportunistic detritivore, feeding on organic material falling through the water column.

IE: What samples did you use for this study?

Rowe: We reanalyzed 3 fossil specimens of Vampyronassa rhodanica and 2 extant samples of V. infernalis [the modern-day vampire squid] from the collections at the American Museum of Natural History and the Yale Peabody Museum. We also compared these specimens with other fossils from the literature.

The V. rhodanica fossils were collected from a Lagerstätte in the Ardèche region of France called La Voulte-sur-Rhône. Most lagerstätte preserve fossils as impressions, but at La Voulte-sur-Rhône, specimens are often preserved in 3D. 

IE: In the paper, you describe a reanalysis of the fossils using modern techniques. When was the original analysis and what did those investigators find?

Rowe:  The initial description of V. rhodanica was by Fischer & Riou in their 2002 paper. At the time of publication, the authors had to rely on observations of the external form for their anatomical descriptions. They were able to describe many external features, and based on this they positioned this species as the oldest likely relative of the modern-day vampire squid (V. infernalis).

IE: What new tools did you use to analyze these fossils two decades later?

Rowe: We chose to reanalyze some of the Vampyronassa rhodanica specimens described in the 2002 paper using powerful X-ray-based imaging techniques at both the Muséum national d'Histoire naturelle in Paris and the European Synchrotron Radiation Facility Synchrotron (ESRF, ID 19 beamline, Grenoble, France). We used these same X-ray techniques at the American Museum of Natural History on the two modern vampire squid. 

Using these data, we were able to identify the boundaries of anatomical structures and reconstruct them in 3D.

IE: What did that analysis reveal?

Rowe:  The results were exciting. For example, the kind of resolution we were able to get on the suckers of V. rhodanica was completely unknown before the acquisition of this data. We were able to determine that the sucker attachment of V. rhodanica is the same type seen only in modern V. infernalis, though the overall shape is of the sucker itself and reflects those of octopuses.

IE: What do those findings suggest about V. rhodanica's life and behavior?

Rowe: Though we obviously can’t observe how V. rhodanica used their suckers. By comparing preserved anatomical features with that of coleoids today – suckers and cirri for example – and knowing how they function now, we can infer how the same features may have been used by the Jurassic V. rhodanica. Based on functional comparisons with modern coleoids, the combination of characteristics observed in the arm crown of V. rhodanica, as well as their streamlined, muscular mantle, suggest they were adapted to a pelagic, predatory lifestyle.

IE: Were you surprised? Were your findings consistent with the original analysis?

Rowe: The soft tissues of modern coleoids hold a lot of information about their lifestyle, though this is rarely preserved in fossils. Based on previous work we had a sense of the external characters that had been preserved, though the resolution with which we could see the detail of these tissues in the scans was fantastic.

IE: How do your findings change what experts know about V. rhodanica? Do they offer clues about its broader environment or ecology?

Rowe: The lifestyle of V. rhodanica is in contrast with that of the modern vampire squid. It is unclear when the adaptation to the deep-sea lifestyle occurred in the lineage, though recent work has described a fossil species of this family inhabiting this environment in the Oligocene, around 33.9 to 23 million years ago. The initial shift from shallower to deeper waters was possibly driven by competition in onshore environments. The mosaic of characters found in the coleoid taxa at La Voulte-sur-Rhône (V. rhodanica and other species), suggests that Mesozoic coleoids co-occurred in different ecological niches during the mid-Jurassic.


Seismic waves from earthquakes reveal changes in the Earth's outer core

Seismic waves from earthquakes reveal changes in the Earth’s outer core
The blue path illustrates a core-penetrating seismic wave moving through a region in the
 outer core, where the seismic speed has increased because a low-density flow has moved
 into the region. Credit: Ying Zhou

In May 1997, a large earthquake shook the Kermadec Islands region in the South Pacific Ocean. A little over 20 years later, in September 2018, a second big earthquake hit the same location, its waves of seismic energy emanating from the same region.

Though the earthquakes occurred two decades apart, because they occurred in the same region, they'd be expected to send seismic waves through the Earth's layers at the same speed, said Ying Zhou, a geoscientist with the Department of Geosciences in the Virginia Tech College of Science.

But in data recorded at four of more than 150 Global Seismographic Network stations that log seismic vibrations in real time, Zhou found an anomaly among the twin events: During the 2018 , a set of seismic waves known as SKS waves traveled about one second faster than their counterparts had in 1997.

According to Zhou, whose findings were recently published in Communications Earth & Environment, that one-second discrepancy in SKS wave travel time gives us an important and unprecedented glimpse of what's happening deeper in the Earth's interior, in its .

What's inside counts

The outer core is sandwiched between the mantle, the thick layer of rock underneath the Earth's crust, and the , the planet's deepest interior layer. It's composed mainly of  that undergoes convection, or , as the Earth cools. This resulting swirling of liquid metal produces electrical currents responsible for generating the Earth's magnetic field, which protects the planet and all life on it from harmful radiation and solar winds.

Without its magnetic field, the Earth could not sustain life, and without the moving flows of liquid metal in the outer core, the magnetic field wouldn't work. But scientific understanding of this dynamic is based on simulations, said Zhou, an associate professor. "We only know that in theory, if you have convection in the outer core, you'll be able to generate the magnetic field," she said.

Scientists also have only been able to speculate about the source of gradual changes in strength and direction of the magnetic field that have been observed, which likely involves changing flows in the outer core.

"If you look at the north geomagnetic pole, it's currently moving at a speed of about 50 kilometers [31 miles] per year," Zhou said. "It's moving away from Canada and toward Siberia. The  is not the same every day. It's changing. Since it's changing, we also speculate that convection in the outer core is changing with time, but there's no direct evidence. We've never seen it."

Seismic waves from earthquakes reveal changes in the Earth’s outer core
Blue lines are seismic rays in the outer core, where core-penetrating seismic waves moved
 through that region faster in 2018 than in 1997. Credit: Ying Zhou

Zhou set out to find that evidence. The changes happening in the outer core aren't dramatic, she said, but they're worth confirming and fundamentally understanding. In seismic waves and their changes in speed on a decade time scale, Zhou saw a means for "direct sampling" of the outer core. That's because the SKS waves she studied pass right through it.

"SKS" represents three phases of the wave: First it goes through the mantle as an S wave, or shear wave; then into the outer core as a compressional wave; then back out through the mantle as an S wave. How fast these waves travel depend in part on the density of the outer core that's in their path. If the density is lower in a region of the outer core as the wave penetrates it, the wave will travel faster, just as the anomalous SKS waves did in 2018.

"Something has changed along the path of that wave, so it can go faster now," Zhou said.

To Zhou, the difference in wave speed points to low-density regions forming in the outer core in the 20 years since the 1997 earthquake. That higher SKS wave speed during the 2018 earthquake can be attributed to the release of light elements such as hydrogen, carbon, and oxygen in the outer core during convection that takes place as the Earth cools, she said.

"The material that was there 20 years ago is no longer there," Zhou said. "This is new material, and it's lighter. These light elements will move upward and change the density in the region where they're located."

To Zhou, it's evidence that movement really is happening in the core, and it's changing over time, as scientists have theorized. "We're able to see it now," she said. "If we're able to see it from seismic waves, in the future, we could set up seismic stations and monitor that flow."

What's next

That's Zhou's next effort. Using a method of wave measurement known as interferometry, her team plans to analyze continuous seismic recordings from two seismic stations, one of which will serve as a "virtual" earthquake source, she said.

"We can use earthquakes, but the limitation of relying on earthquake data is that we can't really control the locations of the earthquakes," Zhou said. "But we can control the locations of seismic stations. We can put the stations anywhere we want them to be, with the wave path from one station to the other station going through the outer core. If we monitor that over time, then we can see how core-penetrating seismic waves between those two stations change. With that, we will be better able to see the movement of fluid in the outer core with time.Swarm satellites unveil magnetic waves that sweep the outermost part of Earth's outer core

More information: Ying Zhou, Transient variation in seismic wave speed points to fast fluid movement in the Earth's outer core, Communications Earth & Environment (2022). DOI: 10.1038/s43247-022-00432-7

Journal information: Nature Communications Earth & Environment 

Provided by Virginia Tech 

Hidden carbon layer may have sparked ancient bout of global warming

Rift between Greenland and Europe implicated in 56-million-year-old hothouse

23 JUN 2022
BY PAUL VOOSEN
The Vestmanna cliffs of the Faroe Islands were formed by rare, carbon-rich lavas during the rifting of Greenland 56 million years ago.
STEVE HUMPHREYS/ISTOCK

There is no perfect parallel in Earth’s past for present-day climate change—human-driven warming is simply happening too fast and furiously. The closest analog came 56 million years ago, when over the course of 3000 to 5000 years, greenhouse gases soared in the atmosphere, causing at least 5°C of warming and pushing tropical species to the poles.

The cause of the Paleocene-Eocene Thermal Maximum (PETM) has long been debated, with researchers invoking exotic mechanisms such as catastrophic releases of methane from the sea floor or even asteroid strikes. But over the past few years, evidence has mounted for a more prosaic culprit: carbon-spewing volcanoes that emerged underneath Greenland as it tore away from Europe. Now, researchers have found signs of an effect that would have supercharged the warming effect of the volcanoes, making them a stronger suspect. The underside of Greenland is thought to be encrusted with carbon-rich rocks, like barnacles on the keel of a ship. During the rifting, they might have liberated a gusher of carbon dioxide (CO2), says Thomas Gernon, a geologist at the University of Southampton and leader of the new study. “It’s a perfect storm of conditions.”

The PETM has long fascinated paleoclimatologists. “Since dinosaurs kicked the bucket, this is the biggest global warming event we have,” says Pincelli Hull, a paleoclimate scientist at Yale University. It can yield clues to how quickly Earth warms as greenhouse gas levels rise and how climate extremes alter ecosystems. But the comparison to today isn’t exact. Although the total release of carbon during the PETM exceeded the total of today’s known oil and gas reserves, it was slower than today’s surge of greenhouse gases and drove more gradual warming. Life had more time to adapt than it does today: Fossil records show trees migrated uphill and to higher latitudes, with animals following in their wake, even as tropical corals disappeared and ecosystems wholly changed.

Past explanations for the PETM centered on methane, a greenhouse gas even more powerful than CO2 although shorter lived. Samples of ancient plankton shells seemed to show the atmosphere during the brief hothouse was enriched in light carbon, the isotope favored by life. That suggested the carbon responsible for the warming surge originated in living things, as most methane does, rather than in the gases spewed by volcanoes, which rise from deep Earth.

At first, researchers thought a small amount of warming might have destabilized methane hydrates—seafloor deposits of methane trapped in cages of ice crystals—triggering a massive release of carbon. But the 2010 Deepwater Horizon oil spill in the Gulf of Mexico put a dent in that theory. Microbes simply chewed up the methane the broken well released into the ocean, suggesting seeps of seabed methane would rarely get all the way into the air. “Most modeling studies suggest you can’t release enough greenhouse gases just through hydrates,” says Sev Kender, a palaeoceanographer at the University of Exeter.

Mudrocks on the sea floor also contain carbon that originated in living things, and magma from submarine eruptions could have heated the rocks and liberated the carbon. But in 2017, researchers analyzed plankton fossils from an ocean core and found the carbon released during the PETM was heavier than previously thought. For some, that indicated the carbon wasn’t from living sources. “Given the current state of knowledge, it seems likely to be volcanism,” says Marcus Gutjahr, a geochemist at GEOMAR Helmholtz Centre for Ocean Research Kiel, who led the 2017 study.

Greenland was rifting away from Europe at the time of the PETM as a mantle plume traveled under the island, priming the 180-kilometer-thick crust above to be pulled apart. Like all volcanism, the process would have released CO2. Gernon calculated, however, that the eruptions during the rifting would have only provided one-fifth of the more than 10,000 gigatons of carbon needed to explain the PETM warming. But he knew that over the eons, CO2 and other gases can bubble out of tectonic plates as they dive into the mantle, percolating up into the underside of thick crusts like Greenland’s, and forming carbonate formations that can be stable for millions or even billions of years.

If the crust is ever pulled apart by rifting, however, the trapped carbon can spill upward and erupt as rare carbonatite lava, which contains far more CO2 than standard lava. Indeed, such a process appears to be underway in East Africa right now, where a rift has begun to tear the horn of Africa away from the rest of the continent, says James Muirhead, a structural geologist at the University of Auckland. “At the very edge of the craton we get these carbonatite lavas,” he says. “And adjacent to the craton we get high CO2 fluxes.”

Similarly, the hot spot that burned through Greenland starting 60 million years ago could have mobilized any carbonate under its crust, Gernon says. When the rifting began to open up what today is the northeastern Atlantic Ocean, “you’ll have a huge amount of carbon venting.”

Evidence of the carbon-rich melt is abundant on either side of the North Atlantic rift, the tectonic division that marks the old boundary between Greenland and Europe, Gernon and his co-authors report in a study published today in Nature Geoscience. In an ocean core collected in 1981, they found volcanic tuffs indicating a sharp increase in volcanism during the PETM. They also combed the literature for studies of other rocks matching the core, and found reports in East Greenland and the Faroe Islands of anomalous lavas rich in magnesium, titanium oxide, and rare earth elements—signatures of melting of carbonate rock from deep in the crust. The lavas date roughly to 56.1 million years ago, and the investigators calculate that the rifting would have produced enough of them to explain nearly all of the needed carbon emissions.

Kender says Gernon makes a compelling case, but adds the timing is key. The PETM happened in a geological instant, lasting only several thousand years. Meanwhile, the volcanism has not been precisely dated. “Whether it was at the onset, in the middle, or later, we can’t say yet,” Kender says. Gernon’s team says more precise geochemical dating from the ocean core, still unpublished, supports the idea that the lavas they’re studying could be from the onset of the PETM. “I’m quietly confident the story works,” Gernon says.
O'Regan stops in Edmonton to tout talks with unions over federal green transition plans

Lisa Johnson - Yesterday 

Natural Resources Minister Seamus O'Regan.

Federal Labour Minister Seamus O’Regan stopped in Edmonton Friday to tout his government’s work with unions in developing its plan to help transition energy workers to a green economy.

The Liberals have set aside a $2 billion Futures Fund to support fossil fuel-reliant provinces like Alberta, but the government is still in consultations on its Just Transition plan intended to support workers affected by the transition to a low-carbon economy.

O’Regan said it will be released “very soon” and he expects “significant” investments, with many coming from the corporate sector.

“That plan is going to be sweeping and doesn’t just involve what we refer to as Just Transition, which is about workers, but it’s also about energy transition — they are absolutely interlinked,” he said.

“The jobs that we’re creating in renewable energy need to be good jobs.”


Alberta Federation of Labour president Gil McGowan said at the news conferences labour leaders have been telling government leaders there is a need for major infrastructure investments.

“Don’t just give us promises of training alone. Give us a plan, give us projects, give us jobs — we’ll do the rest,” said McGowan.

“We need a plan for economic transformation and the money and the political will to back it up. That doesn’t mean shutting down our oil and gas sector, but it does mean helping them pivot, and decarbonize so that they can remain competitive and viable for as long as possible,” he said.

Associate Finance Minister and Edmonton Centre MP Randy Boissonnault said the “evolution of energy” will require investments of between $100 billion to $125 billion per year until 2050 for it to be done.

“If we think $2 billion is going to get us to where we need to get, then we’ve got to have a reset of expectations,” he said, pointing to the federal government’s investment in Alberta of $1 billion towards orphan well cleanup, as well as the $15 billion Canada Growth Fund.

lijohnson@postmedia.com

twitter.com/reportrix

BC

Lower Mainland concrete workers' strike ends after 5 weeks

New agreement includes 15 per cent wage increase over four years

Striking workers, shown June 9 at Ocean Concrete in Vancouver, shut down operations at 12 facilities in the Fraser Valley and Metro Vancouver. (Ben Nelms/CBC

A deal was reached Thursday between the unions representing concrete workers and Rempel Bros. Concrete, ending a five-week-long strike in the Lower Mainland and Fraser Valley. 

The strike, which shut down operations at 12 facilities operated by Rempel Bros. Concrete, Ocean Concrete and Allied Ready Mix on May 20, put concrete foundation projects weeks behind schedule.

The strike saw almost 300 employees off the job, and initially impacted more than 50 per cent of construction projects in Metro Vancouver and the Fraser Valley, according to a statement from the International Union of Operating Engineers (IUOE) Local 115. 

The workers are represented by both the Teamsters and the IUOE. They include concrete plant operators, concrete mixer truck drivers and others in their ranks.

Residential and industrial projects were affected, as well as public infrastructure projects such as the Pattullo Bridge replacement and the Broadway subway project. 

Workers were back on the job at 6 a.m. Friday, according to the union. (Ben Nelms/CBC)

The union said major concerns in the dispute included long working hours, missed breaks, and wages. They said drivers were being asked to work 14-hour days without sufficient breaks. 

The parties worked with a mediator, former chair of the Labour Relations Board Jacquie De Aguayo, to reach the agreement. 

Josh Towsley, assistant business manager with IUOE Local 115, said while workers previously had to ask for breaks, workers will now be able to inform their employer when they are taking their break. 

"This crew has been working really hard for a long time and I think they felt a bit burnt out and a bit under appreciated," said Towsley.

The agreement also includes wage increases of 15 per cent over the next four years, he said. 

The strike involved about 160 workers at the six Lower Mainland Rempel Bros. facilities. Since those employees also work at six other concrete sites operated by Ocean Concrete and Allied Ready Mix, 134 workers at those facilities respected picket lines and refused to work during the strike. 

"People are relieved that the supply of concrete is coming back online, there's no doubt ... our members are focused on getting back to work, getting the industry moving again," said Towsley. 

Workers were back working at 6 a.m. Friday, according to the union. 

Canadian Forces Base Edmonton celebrates Pride with first ever parade on a base

Anna Junker - Yesterday 
Edmonton Journal

Maj. John McDougall raises the Pride flag and then participates in a Pride walk at 3rd Canadian Division Support Base (3 CDSB) on Friday, June 24, 2022.

Members of Canadian Forces Base Edmonton and their families made history on Friday, marching in the first Pride parade to take place on a Canadian military base.

Acceptance and love were celebrated in an emotional ceremony, where the Pride flag was raised, followed by a parade of military members and their loved ones through the base, with military police vehicles, tanks and trucks decked out in Pride memorabilia.

Master Sailor Antoine Lavoie, co-chair of the Defense Team Pride Advisory Organization (DTPAO), said Friday was an important day, that showed the LGBTQ2S+ community is supported.

“Knowing that we can be here and there’s not this binary and we can be who we are and serve, that means the world,” said Lavoie.

Maj. John McDougall, champion for the DTPAO, said he has now been a part of “three firsts.” He marched in the first Pride parade in Toronto that allowed military members, and he raised the first Pride flag on the base in 2013.

“Today, I cannot define how I feel,” he said. “The support, the respect, the inclusion, everybody wanting to join this, we can put out policy, but we can’t make people be inclusive. And these people are here because they chose to be part of our family, part of our queer community.”

McDougall was arrested by the military police and RCMP in the early ’90s when it was still illegal to be gay in the military.

“I used to have to put on two uniforms. I’d put on my military uniform, and then I’d put on the ‘straight John’ uniform,” he said.

“Now I get to wear just one uniform, a uniform that says we’re inclusive, we’re welcoming, we want this to be a safe place for anybody that wants to be part of the Canadian Armed Forces. It’s a sigh of relief. My shoulders are lighter. It feels amazing.”

Col. Rob McBride, commander of the 3rd Canadian Division Support Group, said Friday was a historic day.

“I’ve been in the military now for 29 years, and I can say during that 29 years, we’ve come leaps and bounds ahead of where we were,” he said. “The inclusivity now, the strength that that inclusivity brings to the defence team is truly phenomenal.”

Lavoie added that it felt surreal he could march in a Pride parade on the base while in uniform.