Thursday, May 22, 2025

 

New study reveals how competition between algae is transforming the gulf of Maine




Bigelow Laboratory for Ocean Sciences
Shane Farrell, UMaine 

image: 

Lead author, Shane Farrell, examines algae samples in the lab. Farrell spent several multiple months on a research visit with co-author Daniel Petras’s former lab at the University of Tübingen to learn the methods for non-targeted metabolomics analysis (Credit: Bigelow Laboratory for Ocean Sciences).

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Credit: Bigelow Laboratory for Ocean Sciences




As the ocean warms across its temperate regions, kelp forests are collapsing and turf algae species are taking over. This shift from dense canopies of tall kelp to low-lying mats of turf algae is driving biodiversity loss and altering the flow of energy and nutrients through reef ecosystems.

It’s also fundamentally altering the chemical ecology of coastal ecosystems.

New research in Scienceled by researchers at Bigelow Laboratory for Ocean Sciences, has shown for the first time how turf algae release chemicals that can kill young kelp. That creates a feedback loop where more turf algae means more harmful chemicals, which further inhibits recovery and reinforces kelp forest collapse. This chemically-mediated interaction, which scientists call allelopathy — or what the authors more bluntly call chemical warfare — reveals an indirect way that climate change is reshaping ocean ecosystems, complicating kelp forest recovery along Maine’s rapidly warming coast.

The study also includes researchers from University of Maine, University of California Riverside, University of Tübingen, Perry Institute for Marine Science, and Harvard University, working together to combine extensive field surveys, advanced chemical analysis, and novel lab experiments. 

That’s why this study is so powerful,” said Bigelow Laboratory Senior Research Scientist Doug Rasher, the study’s senior author. “It moves logically from describing a pattern in nature — the lack of recovery of kelp forests — to revealing that the chemical landscape of kelp forests and turf reefs are fundamentally different, to pinpointing that turf algae and the chemicals they exude prevent kelp recruitment.”

The impacts of kelp forest collapse and replacement by turf algae have been well documented in temperate ecosystems around the world.

“This shift from kelp to turf is analogous to a terrestrial forest transitioning into a grassland,” said the study’s lead author, Shane Farrell, a UMaine doctoral candidate based in Rasher’s research group. “With the loss of kelp forests, we see decreases in biodiversity, productivity, and the ecosystem services they provide to humans.”

Previous work has shown that once turf algae are established, they can inhibit kelp recovery by taking up space on the reef or harboring small grazers that eat baby kelp.

In tropical ecosystems, such as rainforests and coral reefs, scientists have previously shown that changes in the chemical environment also play a role in locking ecosystems into a degraded state and preventing recovery of foundational species. But no studies had considered whether that kind of chemical change could be at play in temperate kelp forests.

To answer this question, the researchers completed three years of field surveys across the Gulf of Maine, documenting a pattern of new kelp struggling to survive in the southern reaches of Maine’s coast where forests have collapsed. During those surveys, the team collected water and seaweed samples for chemical analysis.

Rather than focusing on known substances, they teamed up with Daniel Petras’s research group at the University of California, Riverside, employing non-targeted metabolomics analysis to understand the diverse chemistry in the samples. This approach involves analyzing all the small molecules within a system, which enabled the researchers to broadly identify the unique chemical features — in the water, in the seaweeds, and on the reef itself — at both kelp- and turf algae-dominated sites.

To characterize the suite of waterborne chemicals present, these methods rely on separating the molecules and breaking them into fragments, which are then matched against reference libraries, much like identifying a person from a fingerprint.

But, as Farrell pointed out, less than 2% of the chemical features the researchers found in this environment had been previously described. To fill in those gaps, the team turned to novel computational tools, which use chemical fragmentation patterns to predict compound identities, molecular formulas, and even chemical structures. These predictions allowed the researchers to classify unknown compounds into broad chemical families, highlighting just how distinct the chemical environment of a kelp forest is from a turf-dominated reef.

“It is awesome to see how our non-targeted metabolomics tools can shed new light on the fascinating chemical complexity caused by shifting environments, such as invasive algae,” Petras said. “This becomes especially powerful when we combine our chemical data with functional information, such as kelp survival.”

In a series of laboratory experiments, the researchers then tested the effects of both all the waterborne chemicals around the turf-dominated reefs, and the specific chemicals released by the five most abundant species of turf algae, on gametophytes, an early life stage of kelp. The experiments showed that gametophyte survival declined dramatically — up to 500% in some cases — when exposed to chemicals released by turf algae, confirming that the new chemical environment is directly responsible for kelp mortality.

“Our study is the first to reveal that chemical warfare can underpin the rebound potential of cold-water kelp forests. And surprisingly, some of the same types of molecules we identified on turf reefs are involved in the recovery dynamics of tropical coral reefs too,” Rasher said. “It shows we have a lot to learn about chemical warfare on temperate reefs, the organisms and molecules involved, and how this process varies globally.”

Previous work by Rasher’s research group confirmed that ocean warming is the primary driver of kelp forest decline in the Gulf of Maine. But these new findings, showing how turf algae can lock an ecosystem into a degraded state, will make it more challenging to promote kelp forest recovery.

“Once turf algae are established, just curbing global carbon emissions and reversing ocean warming is not going to bring Maine’s kelp forests back,” Farrell said. “Because of these feedback mechanisms, we need local interventions to remove the turf algae before kelp will actually recover.”

This study was supported by the NSF Established Program to Stimulate Competitive Research (Grant #OIA-1849227), the Louise H. & David S. Ingalls Foundation, the PADI Foundation, the Essex Avenue Foundation, and the German Research Foundation.





UMaine PhD candidates Shane Farrell and Dara Yiu dive off of Allen Island, Maine. Researchers involved in the study spent several months completing reef surveys to document kelp forest loss along the Maine coast and collect samples for chemical analysis (Credit: Rene Francolini).


Credit

Rene Francolini






Twenty milliliter vials reflect the internal chemistry of different types of brown, green, and red seaweed tissue after being freeze dried and ground up into powder for analysis (Credit: Shane Farrell).




Dive images show the habitat differences between a kelp-dominated reef (top) compared to a turf-dominated reef (lower). Researchers involved in the study have documented how kelp forests along large swaths of the Maine coast have collapsed and turf algae has proliferated in their absence (Credit: Shane Farrell).


Credit

Shane Farrell


 

An artificial protein that moves like something found in nature




University of California - San Francisco





The ability to engineer shapeshifting proteins opens new avenues for medicine, agriculture, and beyond.   

Proteins catalyze life by changing shape when they interact with other molecules. The result is a muscle twitching, the perception of light, or a bit of energy extracted from food.  

But this crucial ability has eluded the growing field of AI-augmented protein engineering.  

Now, researchers at UCSF have shown it is possible to make new proteins that move and change shape like those in nature. This ability will help scientists engineer proteins in powerful new ways to treat disease, clean up pollution, and increase crop yields. 

“This study is the first step on a path that will lead far beyond biomedicine, into agriculture and the environment,” said Tanja Kortemme, PhD, professor of bioengineering and senior author of the study, which appears May 22 in Science

The research was supported by the National Institutes of Health.  

Scientists have been engineering rigid proteins – proteins that can’t move or change shape – since the 1980s. These proteins were first used in commercial products like cleaning solutions. More recently, they’ve been employed to produce blockbuster medicines like artificial insulin, GLP-1 weight-loss drugs, and antibody treatments for cancer and inflammation.  

While important, these immovable molecules can’t match the potential of proteins that can swivel, twist, and morph in complicated ways and then return to their original shape, said Kortemme, who is also an investigator in the Chan-Zuckerberg BioHub San Francisco.  

She said the most important proteins to emulate for medical uses are those that regulate processes like metabolism, cell division, and other basic life functions. These powerful proteins are the targets of nearly 1 in 3 FDA-approved drugs. They facilitate communication within or between cells by changing from one shape into another, and then back again, like an on-off switch.  

An overwhelming problem 

Designing such stable yet dynamic forms requires computational power and artificial intelligence that didn’t exist until a few years ago. 

The challenge was huge, so Kortemme and graduate student Amy Guo began with something small: giving a simple natural protein the ability to move in a new way. Guo then made part of the protein swing so it could bind to calcium, a common way that proteins change shape.  

“We wanted to devise a design method that could be applied in lots of situations, so we focused on creating a movable part that does what many natural proteins do,” she said. “The hope is that this movement could also be added to static artificial proteins to expand what they can do, too.” 

Guo’s next step was to generate a virtual library of thousands of possible shapes that the protein could take. She picked two stable shapes for the protein: one that could bind calcium and another that couldn’t.  

Then, she zoomed in on specific areas of the virtual protein to look at how the atoms in it were interacting. The work, which began before the pandemic, accelerated once the artificial intelligence program AlphaFold2 became available. Guo used it to make the movable part twist and capture the calcium, and then untwist to set it free.  

The moment of truth came when the researchers tested their model in a computer simulation. They teamed up with Mark Kelly, PhD, a pharmaceutical chemist at UCSF who uses nuclear magnetic resonance to visualize the atoms in a protein. 

“I was amazed that the simulations showed it working exactly like we’d expected it to,” Guo said. “That really gives me confidence that this was for real, that we really did it.” 

In the medical realm, movable engineered proteins could be used in biosensors that change shape in response to signals of disease, triggering an alert. Or they could be used as medicinal proteins that are tailored to work with a person’s unique body chemistry.  

Shapeshifting proteins also could be designed to break down plastics or help plants resist climate-related stresses like drought or pests. They could even be used to make metal that can repair itself when it cracks.  

“The possibilities are truly endless,” Guo said. 

 
Authors: Additional authors include Deniz Akpinaroglu, Christina Stephens, Michael Grabe and Mark Kelly from UCSF, and Colin Smith from Wesleyan University.  

Funding: This work is supported by grants from the National Institutes of Health (R35 GM145236 and S10 OD023455). For all funding information, please see the study.  

 

About UCSF: The University of California, San Francisco (UCSF) is exclusively focused on the health sciences and is dedicated to promoting health worldwide through advanced biomedical research, graduate-level education in the life sciences and health professions, and excellence in patient care. UCSF Health, which serves as UCSF's primary academic medical center, includes top-ranked specialty hospitals and other clinical programs, and has affiliations throughout the Bay Area. UCSF School of Medicine also has a regional campus in Fresno. Learn more at ucsf.edu, or see our Fact Sheet.

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Turf algae chemically inhibit kelp forest recovery in warming coastal waters



Summary author: Walter Beckwith



American Association for the Advancement of Science (AAAS)






As kelp forests decline in the warming coastal waters of the Gulf of Maine, turf algae – dense mats of red algae replacing kelp in many regions – may chemically interfere with kelp recovery, a new study reports. This complicates efforts to restore these crucial marine ecosystems. Kelp forests are ecologically and economically vital marine ecosystems that support diverse life forms and functions. However, despite their widely recognized importance, kelp forests worldwide are threatened with collapse due to climate change and/or overfishing. In many regions where kelp forests have disappeared, they have been replaced by dense, low-lying mats of chemically rich, filamentous red seaweeds, also known as turf algae. This shift has been linked to declines in biodiversity and major disruptions in coastal ecosystem dynamics. Some research suggests that turf algae may actively hinder the recovery of kelp through allopathy – a common biological phenomenon by which one organism produces biochemicals that influence the growth, survival, development, and reproduction of other surrounding organisms. Understanding whether turf algae chemically inhibit kelp recovery is essential to managing and restoring these rapidly changing marine environments.

 

Shane Farrell and colleagues investigated whether allopathic turf algae suppress the recovery of kelp forests in the warming waters of the Gulf of Maine. Farrell et al. discovered that while kelp forests have persisted in the cooler waters of northeastern Maine, those in the warmer southwest have collapsed and failed to recover, with turf algae now dominating these reefs. By comparing the chemical composition of water and seaweed samples from kelp- and turf-dominated reefs, the authors identified distinct chemical signatures produced by turf algae. Laboratory experiments show that these turf-derived compounds inhibit the early growth stages of kelp. The findings suggest that turf algae alter the chemical ecology of the environment in ways that actively prevent kelp from re-establishing. “Future resilience strategies for marine ecosystems should integrate chemical ecology into climate change models,” write Colette Feehan and Karen Filbee-Dexter in a related Perspective. “By illuminating these hidden processes, we can better develop a fuller picture of how climate change is reshaping ocean ecosystems – and how we might better protect them.”

 SPACE/COSMOS

Unravelling the origin of mysterious radiation


Could black holes help explain high-energy cosmic radiation?



Norwegian University of Science and Technology

Super massive black holes 

image: 

Supermassive black holes at the centers of galaxies emit radiation and ultra-fast winds into space.
Here is an artistic interpretation.

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Credit: Illustration: NASA, JPL-Caltech





The universe is full of different types of radiation and particles that can be observed here on Earth. This includes photons across the entire range of the electromagnetic spectrum, from the lowest radio frequencies all the way to the highest-energy gamma rays. It also includes other particles such as neutrinos and cosmic rays, which race through the universe at close to the speed of light.

Curiously, "cosmic rays" are not actually rays – this name has historical reasons – but small particles, mostly atomic nuclei, which are accelerated to enormous energies somewhere in the universe. Although their sources are not yet fully understood, they are most likely associated with some of the most extreme environments in the universe, such as black holes, supernovae, or rotating neutron stars (a type of dead star).

But occasionally cosmic rays have much higher energy than usual. We've known about this since 1962, but we still have no idea why.

We also don’t know where this ultra-high-energy cosmic radiation comes from.

Now, research from the Norwegian University of Science and Technology (NTNU) may have found the answer to this big unanswered question in physics.

Supermassive black holes may be the cause

Foteini Oikonomou, an associate professor at NTNU's Department of Physics, is working on the case. In a recent article, she and her colleagues present a completely new and plausible explanation for this ultra-high-energy radiation.

We suspect that this high-energy radiation is created by winds from supermassive black holes.

The lead author is PhD research fellow Domenik Ehlert from the same department. The team also includes postdoctoral fellow Enrico Peretti from the Université Paris Cité.  Their work focuses on astroparticle physics, which studies the relationship between the smallest particles in the universe and the universe’s largest phenomena.

“We suspect that this high-energy radiation is created by winds from supermassive black holes,” said Oikonomou.

But what on earth does that mean?

Active black holes create winds

The Milky Way is the neighborhood in the universe where you and I live. Our Sun and solar system are part of this galaxy, along with at least 100 billion other stars.

“There is a black hole called Sagittarius-A* located right in the centre of the Milky Way. This black hole is currently in a quiet phase where it isn’t consuming any stars, as there is not enough matter in the vicinity,” Peretti said.

This contrasts with growing, supermassive, active black holes that consume up to several times the mass of our own Sun each year.

“A tiny portion of the material can be pushed away by the force of the black hole before it is pulled in.  As a result, around half of these supermassive black holes create winds that move through the universe at up to half the speed of light,” Peretti said.

We have known about these gigantic winds for approximately ten years. The winds from these black holes can affect galaxies. By blowing away gases, they can prevent new stars from forming, for example. This is dramatic enough in itself, but Oikonomou and her colleagues looked at something else, much smaller, that these winds could be the cause of.“

It is possible that these powerful winds accelerate the particles that create the ultra-high-energy radiation,” said Ehlert.

To understand this, we also need to explain a little bit about atoms.

Atoms and enormous amounts of energy

Atoms consist of a nucleus, which is made up of protons and neutrons. These particles are made up of quarks, but we don’t need to go into that right now.

One or more electrons can be found around this nucleus in the so-called cloud.

“The ultra-high-energy radiation consists of protons or atomic nuclei with energy up to 1020 electron volts,” explained Oikonomou.

A particle like this, which is smaller than an atom, contains about as much energy as a tennis ball when Serena Williams serves it at 200 kilometres per hour.

If that number doesn’t mean anything to you, you should know that in this context, it is an absolutely enormous amount of energy.

“A particle like this, which is smaller than an atom, contains about as much energy as a tennis ball when Serena Williams serves it at 200 kilometres per hour,” said Oikonomou.

It corresponds to approximately a billion times more energy than the particles created by researchers in the Large Hadron Collider in Switzerland and France.

Fortunately, these cosmic rays are destroyed by the Earth’s atmosphere. When they reach ground level, they are as harmless as all the other cosmic radiation that reaches us at the Earth's surface.

“But for astronauts, cosmic radiation is a very serious problem,” Oikonomou said.

Airline crews don’t need to worry about this because they don’t fly high enough.

“The main concern for astronauts is cosmic low-energy radiation produced by our own Sun, because it is much more common. The rays we study are infrequent enough that it is extremely unlikely they would pass through an astronaut,” she said.

Other suspects

Previously, researchers have looked into whether these high-energy particles come from gamma-ray bursts, from galaxies that are creating new stars at an extremely high rate, or from plasma outflows from supermassive black holes.

However, Oikonomou and her colleagues have another hypothesis.

“All the other hypotheses are very good guesses – they are all sources that contain a lot of energy. But no one has provided evidence that any of them are the source. That is why we decided to investigate the winds from the supermassive black holes,” said Ehlert.

Guilty? Maybe

So what do we actually know? Is it the winds that create the high-energy particles in the cosmic radiation?

When researchers ask questions like this, they often feel a sense of excitement and think “YES, that might just be the case!”

“Our answer is more of a cautious ‘maybe’, said Oikonomou.

That doesn’t sound particularly dramatic. However, when researchers ask questions like this, they often feel a sense of excitement and think “YES, that might just be the case!”, but that doesn't mean it is the case in this instance.

“We find that the conditions related to these winds align particularly well with particle acceleration. But we are still unable to prove that it is specifically these winds that accelerate the particles behind the high-energy cosmic radiation,” Oikonomou said.

However, the model the researchers are using can explain one specific aspect of these particles that we still don’t understand. Within a certain energy range, the particles have a chemical composition that other models cannot explain in any meaningful way.

“We can also test the model using neutrino experiments,” said Oikonomou.

That, however, is something for a completely different article.

“In the years to come, we hope to collaborate with neutrino astronomers to test our hypothesis,” Oikonomou said. Perhaps they will then find more evidence, one way or the other.

Reference: Domenik Ehlert, Foteini Oikonomou, Enrico Peretti, Ultra-high-energy cosmic rays from ultra-fast outflows of active galactic nuclei, Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 3, May 2025, Pages 2435–2462, https://doi.org/10.1093/mnras/staf457

 

Domenik Ehlert and Foteini Oikonomou in front of one of the 1,600 surface detectors that are part of the Pierre Auger Ultra-high Energy Cosmic Ray Observatory in Malargüe, Argentina.

Credit

NTNU