Wednesday, February 15, 2023

Climate change could cause mass exodus of tropical plankton

Peer-Reviewed Publication

UNIVERSITY OF TEXAS AT AUSTIN

Live foraminifera under light microscope 

IMAGE: A MICROSCOPE IMAGE OF A SHELLED PLANKTON. ACCORDING TO RESEARCH FROM THE UNIVERSITY OF TEXAS AT AUSTIN, PLANKTON POPULATIONS LIKE THIS FLOURISHED IN THE TROPICS DURING PAST GLOBAL COOLING AND MAY VANISH AS THE CLIMATE WARMS. view more 

CREDIT: TRACY AZE

The tropical oceans are home to the most diverse plankton populations on Earth, where they form the base of marine food chains. Modern plankton biodiversity in the tropics is a surprisingly recent development and the result of 8 million years of global cooling, according to a study led by researchers at The University of Texas at Austin. 

The finding raises concerns that rapid ocean warming could force the plankton to move away from the tropics, which would negatively affect ocean ecosystems, including those of important fish such as tuna and billfish, and coastal communities that depend on them. The research was published in the journal Nature.

Using microfossils to track the history of a group of zooplankton called Foraminifera, the researchers found that the last time Earth was this warm – just before global cooling began 8 million years ago – tropical plankton populations lived in waters more than 2,000 miles from where they are today. The natural cooling of the past 8 million years that allowed the plankton to flourish in the tropics has been reversed by climate change during the past century.

“Earth’s current biosphere evolved for ice ages,” said lead author Adam Woodhouse, a postdoctoral fellow at the University of Texas Institute for Geophysics. “By suddenly switching to an Earth of 8 million years ago, we’re not just killing off a few species, we’re changing the entire chemistry of the atmosphere and oceans, and nothing is ready for that.”

To conduct the study, researchers analyzed a database of 500,000 microfossils — the largest of its kind — gathered during 55 years of scientific ocean drilling. Each fossilized shell tells where and when the plankton lived, how deep its habitat was, and the conditions of the ocean around it. 

The scientists grouped the information and analyzed it alongside a geologic record of past climate change. They found that as global cooling began 8 million years ago, plankton species were pushed toward the equator. By the modern age, the most diverse plankton populations had moved to the tropics, while the poles of today became too harsh for all but a handful of specialized species.

With global temperatures and atmospheric carbon dioxide now approaching what they were 8 million years ago, the findings suggest that plankton species could evacuate the equator and head poleward, researchers said. Other studies of modern plankton have already documented signs of this happening. Researchers fear that the loss of diversity in plankton populations could trigger a cascade of extinctions like those seen in rainforests after logging and fires.

“The important thing now is to determine how the effect of climate change on those species will cascade across food webs,” said Harvard University network scientist Anshuman Swain, who co-led the research. 

When analyzing the data, the researchers used a technique better known for investigating social structures like Twitter to reveal connections between plankton evolution, habitats and climate change over deep time. First developed to explore social interactions and friendships in sociology, network analysis is increasingly being used in ecology and environmental science and could help inform action to mitigate the worst effects of climate change, Swain said.

The time for action, however, could be running out, said Tracy Aze, an associate professor of marine micropaleontology at the University of Leeds who helped develop the plankton database but was not involved in the current study. According to Aze, today’s unprecedented warming means that the world is now operating on unpredictable time scales.

“The fact that we've already begun seeing an appreciable difference in the diversity of many marine groups like fish and the plankton means we might be closer to certain temperature tipping points than we thought,” she said.

The plankton database, Triton, was developed and published at the University of Leeds and the University of Oxford in 2021. The current research was funded by the University of Maryland and University of Texas Institute for Geophysics, a research unit of the Jackson School of Geosciences.  


The scientific drilling ship Joides Resolution near the Greek island of Santorini in 2023. Aboard was mission scientist Adam Woodhouse, a postdoctoral fellow at the University of Texas Institute for Geophysics. His studies of microfossils gathered on previous missions have revealed how the climate affects global plankton populations.

CREDIT

Thomas Ronge

Large-scale fossil study reveals origins of modern-day biodiversity gradient 15 million years ago

Peer-Reviewed Publication

UNIVERSITY OF OXFORD

Painting of Planktonic foraminifera 

IMAGE: DEPICTIONS OF PRESENT-DAY PLANKTONIC FORAMINIFERA FLOATING IN THE DEEP SEA. IMAGE CREDIT: RICHARD BIZLEY, BIZLEYART. view more 

CREDIT: DEPICTIONS OF PRESENT-DAY PLANKTONIC FORAMINIFERA FLOATING IN THE DEEP SEA. IMAGE CREDIT: RICHARD BIZLEY, BIZLEYART.

  • Today, species richness peaks in equatorial regions but until now there has been no clear explanation for this.
  • By analysing fossil records, researchers found that a key driver of the modern biodiversity gradient was a global cooling event that occurred 15 million years ago.
  • This produced a steeper temperature gradient between low and high latitudes, and within the water column, causing tropical regions to support a greater number of ecological niches for species to inhabit.

Researchers have used nearly half a million fossils to solve a 200-year-old scientific mystery: why the number of different species is greatest near the equator and decreases steadily towards polar regions. The results – published today in the journal Nature – give valuable insight into how biodiversity is generated over long timescales, and how climate change can affect global species richness.

It has long been known that in both marine and terrestrial systems species (including animals, plants, and single-celled organisms) show a ‘latitudinal diversity gradient’, with biodiversity peaking at the equator. But until now, limited fossil data has prevented researchers from thoroughly investigating how this diversity gradient first arose.

In this new study, researchers at the Universities of Oxford, Leeds and Bristol, used a group of unicellular marine plankton called planktonic foraminifera. The team analysed 434,113 entries in a global fossil database, covering the last 40 million years. They then investigated the relationship between the number of species over time and space, and potential drivers of the latitudinal diversity gradient, such as sea surface temperatures and ocean salinity levels.

Key findings:

  • The modern-day latitudinal diversity gradient first started to emerge around 34 million years ago, as the Earth began to transition from a warmer to cooler climate.
  • This gradient initially remained shallow, until around 15–10 million years ago, when it steepened significantly. This coincides with a significant increase in global cooling.
  • Peak richness for planktonic foraminifera occurred at higher latitudes from 40–20 million years ago. By around 18 million years ago, however, peak richness shifted to between 10° to 20° latitude, consistent with the diversity pattern observed today.
  • There was a strong positive relationship between species richness and sea surface temperatures – both when modelled over time at specific locations, or at different locations at a specific time.
  • There was also a positive relationship between species richness and the strength of the thermocline: the temperature gradient that exists between the warmer mixed water at the ocean's surface and the cooler deep water below.

According to the researchers, these results indicate that the modern-day distribution of species richness for planktonic foraminifera could be explained by the steepening of the latitudinal temperature gradient from the equator to the poles over the last 15 million years. This may have opened up more ecological niches in tropical regions within the water column, compared with higher latitudes, promoting greater rates of speciation.

To test this hypothesis, the researchers examined the extent to which modern species of planktonic foraminifera live at different depths within the vertical water column. They found that in low latitudes closer to the equator, species today are more evenly distributed vertically within the water column, compared with high latitudes.

This suggests that a key driver of the modern-day diversity gradient was a significant increase in the difference in sea surface temperatures between low- and high-latitude regions, and within the water column, from 15 million years onwards. The warmer waters at the tropics were able to support a broader range of different temperature habitats and ecological niches within the vertical water column, encouraging higher numbers of species to evolve.

This is supported by the fact that the tropics today are richer than the tropics of warmer time periods in the past (such as the Eocene and Miocene) when there was little or no vertical temperature gradient in the oceans.

In addition, cooling sea temperatures at high latitudes likely caused many regional populations of species to become extinct, contributing to the modern diversity gradient.

Planktonic foraminifera originate from the Early to Middle Jurassic period (around 170 million years ago). They are found in oceans all over the world – from polar regions to the equator – and occupy a range of ecological niches in the upper two kilometers of the oceans. Because they produce hard outer shells, they can be preserved in large numbers. The global abundance of planktonic foraminifera and their exceptional fossil record from the last 66 million years made them an ideal group for this study.

Dr Erin Saupe (Department of Earth Sciences, University of Oxford), lead author for the study, said: ‘By resolving how spatial patterns of biodiversity have varied through deep time, we provide valuable information crucial for understanding how biodiversity is generated and maintained over geological timescales, beyond the scope of modern-day ecological studies.’

Associate Professor Tracy Aze (School of Earth and Environment, University of Leeds), a co-author for the study, added: ‘Although they are small enough to fit on the head of a pin, planktonic foraminifera have one of the most complete species-level fossil records known to science. Our research builds on 60 years of deep-sea sample collection and the diligent counting and recording of hundreds of thousands of specimens by research scientists. It’s fantastic to be able to produce such important results about the drivers of species distributions through time and to do justice this wonderful fossil archive.’

Study co-author Dr Alex Farnsworth, Senior Research Associate at the Department of Geographical Sciences, University of Bristol, said: ‘Understanding why species in ancient history were more diverse and plentiful nearer the equator and less so nearer the poles can give important insights how marine species, such as plankton, might respond in future. These tiny single-celled organisms are a vital link in the marine food chain, so studying their reactions to changing climates may help us better predict how they will likely be affected as temperatures continue to warm with the increasing onset of climate change. This has potentially large implications for marine food webs, such as fish and aquatic mammals like seals and whales, and could be used to inform future measures to protect sea life and preserve biodiversity.’

A scanning electron microscope image of the shell of the planktonic foraminifera species Globigerinella adamsi. This specimen was collected from sea floor sediments in the Southwest Indian Ocean aboard the GLOW Cruise.

A light microscope image of a planktonic foraminifera (bottom right) surrounded by thin strands of its cytoplasm that extend into the surrounding environment. This living specimen had recently been collected from the water in the Southwest Indian Ocean aboard the GLOW Cruise. 


Image credit: Tracy Aze, University of Leeds.

Notes to editors:

The paper ‘Origination of the modern-style diversity gradient 15 million years ago’ will be published in Nature.

After the embargo lifts, the paper will be available at: https://www.nature.com/articles/s41586-023-05712-6

For interview requests and to view a pre-embargo copy of the paper, contact Dr Caroline Wood: caroline.wood@admin.ox.ac.uk

A range of images are available of planktonic foraminifera. To request these, contact Dr Caroline Wood: caroline.wood@admin.ox.ac.uk

About the University of Oxford

Oxford University has been placed number 1 in the Times Higher Education World University Rankings for the seventh year running, and ​number 2 in the QS World Rankings 2022. At the heart of this success are the twin-pillars of our ground-breaking research and innovation and our distinctive educational offer.

Oxford is world-famous for research and teaching excellence and home to some of the most talented people from across the globe. Our work helps the lives of millions, solving real-world problems through a huge network of partnerships and collaborations. The breadth and interdisciplinary nature of our research alongside our personalised approach to teaching sparks imaginative and inventive insights and solutions.

Through its research commercialisation arm, Oxford University Innovation, Oxford is the highest university patent filer in the UK and is ranked first in the UK for university spinouts, having created more than 200 new companies since 1988. Over a third of these companies have been created in the past three years. The university is a catalyst for prosperity in Oxfordshire and the United Kingdom, contributing £15.7 billion to the UK economy in 2018/19, and supports more than 28,000 full time jobs.

University of Leeds  

The University of Leeds is one of the largest higher education institutions in the UK, with more than 39,000 students from about 140 different countries. We are renowned globally for the quality of our teaching and research. 

We are a values-driven university, and we harness our expertise in research and education to help shape a better future for humanity, working through collaboration to tackle inequalities, achieve societal impact and drive change.   

The University is a member of the Russell Group of research-intensive universities, and is a major partner in the Alan Turing, Rosalind Franklin and Royce Institutes www.leeds.ac.uk   

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About the University of Bristol 

The University is ranked within the top 10 universities in the UK and 61st in the world (QS World University Rankings 2023); it is also ranked among the top five institutions in the UK for its research, according to analysis of the Research Excellence Framework (REF) 2021; and is the 3rd most targeted university by top UK employers. 

The University was founded in 1876 and was granted its Royal Charter in 1909.  It was the first university in England to admit women on the same basis as men.   

The University is a major force in the economic, social and cultural life of Bristol and the region, but is also a significant player on the world stage. It has over 20,000 undergraduates and over 7,000 postgraduate students from more than 150 countries, and its research links span the globe.  

Astrophysicists discover the perfect explosion in space

Peer-Reviewed Publication

UNIVERSITY OF COPENHAGEN - FACULTY OF SCIENCE

Darach Watson and Albert Sneppen 

IMAGE: DARACH WATSON AND ALBERT SNEPPEN view more 

CREDIT: DARACH WATSON

When neutron stars collide they produce aexplosion that, contrary to what was believed until recently, is shaped like a perfect sphere. Although how this is possible is still a mystery, the discovery may provide a new key to fundamental physics and to measuring the age of the Universe. The discovery was made by astrophysicists from the University of Copenhagen and has just been published in the journal Nature.

Kilonovae - the giant explosions that occur when two neutron stars orbit each other and finally collide - are responsible for creating both great and small things in the universe, from black holes to the atoms in the gold ring on your finger and the iodine in our bodies. They give rise to the most extreme physical conditions in the Universe, and it is under these extreme conditions that the Universe creates the heaviest elements of the periodic table, such as gold, platinum and uranium.

But there is still a great deal we do not know about this violent phenomenon. When a kilonova was detected at 140 million light-years away in 2017, it was the first time scientists could gather detailed data. Scientists around the world are still interpreting the data from this colossal explosion, including Albert Sneppen and Darach Watson from the University of Copenhagen, who made a surprising discovery.

"You have two super-compact stars that orbit each other 100 times a second before collapsing. Our intuition, and all previous models, say that the explosion cloud created by the collision must have a flattened and rather asymmetrical shape," says Albert Sneppen, PhD student at the Niels Bohr Institute and first author of the study published in the journal Nature.

This is why he and his research colleagues are surprised to find that this is not the case at all for the kilonova from 2017. It is completely symmetrical and has a shape close to a perfect sphere.

"No one expected the explosion to look like this. It makes no sense that it is spherical, like a ball. But our calculations clearly show that it is. This probably means that the theories and simulations of kilonovae that we have been considering over the past 25 years lack important physics," says Darach Watson, associate professor at the Niels Bohr Institute and second author on the study.

The spherical shape is a mystery

But how the kilonova can be spherical is a real mystery. According to the researchers, there must be unexpected physics at play:

"The most likely way to make the explosion spherical is if a huge amount of energy blows out from the center of the explosion and smooths out a shape that would otherwise be asymmetrical. So the spherical shape tells us that there is probably a lot of energy in the core of the collision, which was unforeseen," says Albert Sneppen.

When the neutron stars collide, they are united, briefly as a single hypermassive neutron star, which then collapses to a black hole. The researchers speculate whether it is in this collapse that a large part of the secret is hidden:

"Perhaps a kind of 'magnetic bomb' is created at the moment when the energy from the hypermassive neutron star's enormous magnetic field is released when the star collapses into a black hole. The release of magnetic energy could cause the matter in the explosion to be distributed more spherically. In that case, the birth of the black hole may be very energetic," says Darach Watson.

However, this theory does not explain another aspect of the researchers' discovery. According to the previous models, while all elements produced are heavier than iron, the extremely heavy elements, such as gold or uranium, should be created in different places in the kilonova than the lighter elements such as strontium or krypton, and they should be expelled in different directions. The researchers, on the other hand, detect only the lighter elements, and they are distributed evenly in space.

They therefore believe that the enigmatic elementary particles, neutrinos, about which much is still unknown, also play a key role in the phenomenon.

"An alternative idea is that in the milliseconds that the hypermassive neutron star lives, it emits very powerfully, possibly including a huge number of neutrinos. Neutrinos can cause neutrons to convert into protons and electrons, and thus create more lighter elements overall. This idea also has shortcomings, but we believe that neutrinos play an even more important role than we thought," says Albert Sneppen.


A New Cosmic Ruler

The shape of the explosion is also interesting for an entirely different reason:

"Among astrophysicists there is a great deal of discussion about how fast the Universe is expanding. The speed tells us, among other things, how old the Universe is. And the two methods that exist to measure it disagree by about a billion years. Here we may have a third method that can complement and be tested against the other measurements," says Albert Sneppen.

The so-called "cosmic distance ladder" is the method used today to measure how fast the Universe is growing. This is done simply by calculating the distance between different objects in the universe, which act as rungs on the ladder.

"If they are bright and mostly spherical, and if we know how far away they are, we can use kilonovae as a new way to measure the distance independently – a new kind of cosmic ruler," says Darach Watson and continues:

"Knowing what the shape is, is crucial here, because if you have an object that is not spherical, it emits differently, depending on your sight angle. A spherical explosion provide much greater precision in the measurement.”

He emphasizes that this requires data from more kilonovae. They expect that the LIGO observatories will detect many more kilonovae in the coming years.

Artistic illustration of kilonova

CREDIT

Robin Dienel/Carnegie Institution for Science)

FACT BOX: ABOUT KILONOVAE

  • Neutron stars are extremely compact stars that consist mainly of neutrons. They are typically only about 20 kilometers across, but can weigh one and a half to two times as much as the Sun. A teaspoon of neutron star matter would weigh about as much as Mount Everest.
     
  • When two neutron stars collide, the phenomenon of a kilonova occurs. This is the name of the gigantic explosion that the merger creates. It is a radioactive fireball that expands at enormous speed and consists mostly of heavy elements formed in the merger and its aftermath — both the lighter and the very heavy elements — which are ejected into space.
     
  • The phenomenon was predicted in 1974 and first clearly observed and identified in 2013. In 2017, detailed data from a kilonova was obtained for the first time, when the detectors LIGO (in the USA) and Virgo (in Europe) sensationally succeeded in measuring gravitational waves from the kilonova AT2017gfo, which was in a galaxy 140 million light years away.

 

FACT BOX: ABOUT THE STUDY

  • The analyses have been carried out on data from the kilonova AT2017gfo from 2017. Those data are the ultraviolet, optical, and infrared light from the X-shooter spectrograph on the Very Large Telescope at the European Southern Observatory, combined with previous analyses of gravitational waves, radio waves and data from the Hubble Space Telescope.
     
  • The scientific article about the study has been published in the journal Nature.
     
  • The study is an important early result of the HEAVYMETAL collaboration, which was recently awarded an ERC Synergy grant.
     
  • The following researchers contributed to the work: Albert Sneppen and Darach Watson from the Cosmic Dawn Center / Niels Bohr Institute, University of Copenhagen; Andreas Bauswein and Oliver Just, GSI Helmholtzzentrum für Schwerionenforschung, Germany; Rubina Kotak from the University of Turku, Finland; Ehud Nakar and Dovi Poznanski from Tel Aviv University, Israel; and Stuart Sim from Queen's University Belfast, UK.

Engineered magic: Wooden seed carriers mimic the behavior of self-burying seeds

Geometric design and engineering of biodegradable materials could improve versatility, efficiency of aerial seeding

Peer-Reviewed Publication

CARNEGIE MELLON UNIVERSITY

Drilling Time Lapse 

IMAGE: THIS TIME-LAPSE SHOWS AN E-SEED CARRIER DRILLING INTO THE GROUND AFTER EXPOSURE TO MOISTURE. view more 

CREDIT: CARNEGIE MELLON UNIVERSITY

How seeds implant themselves in soil can seem magical. Take some varieties of Erodium, whose five-petalled flowers of purple, pink or white look like geraniums.

The seed of these plants is carried inside a thin, tightly wound stalk. During rain or high humidity, the corkscrew-like stalk unwinds and twists the seed into the soil, where it can take root and is safe from hungry birds and harsh environmental conditions. 

Inspired by Erodium's magic, Lining Yao, the Cooper-Siegel Assistant Professor of Human-Computer Interaction at Carnegie Mellon University, worked with a team of collaborators to engineer a biodegradable seed carrier referred to as E-seed. Their seed carrier, fashioned from wood veneer, could enable aerial seeding of difficult-to-access areas, and could be used for a variety of seeds or fertilizers and adapted to many different environments. It's an idea that Yao, the daughter of part-time farmers, has pondered since she was a Ph.D. student at MIT in the mid-2010s.

"Seed burial has been heavily studied for decades in terms of mechanics, physics and materials science, but until now, no one has created an engineering equivalent," said Yao, director of the Morphing Matter Lab in the School of Computer Science's Human-Computer Interaction Institute. "The seed carrier research has been particularly rewarding because of its potential social impact. We get excited about things that could have a beneficial effect on nature."

The team's research appeared in the February issue of Nature.

Danli Luo, a former research assistant at the Morphing Matter Lab and the lead author of the Nature paper, said design and construction of the seed carrier were inspired by the self-burying mechanism that Erodium evolved as it adapted to arid climates.

Erodium's stalk forms a tightly wound, seed-carrying body with a long, curved tail at the top. When it begins to unwind, the twisting tail engages with the ground, causing the seed carrier to push itself upright. Further unwinding creates torque to drill down into the ground, burying the seed.

But Erodium's one-tailed carrier only works well on soils with crevices. To employ their E-seed carriers in a broader range of environments, the research team developed a three-tailed version that is more efficient at pushing itself upright. 

"Geometry can enhance the functionality of the materials beyond what nature offers us. It also makes the design versatile to be applied to other materials," said Shu Yang, a materials scientist and co-author from the University of Pennsylvania.

The researchers considered a number of possible materials for their carriers, including hydrogels, paper and other forms of processed cellulose. They ultimately chose veneers of white oak — a species of tree abundant in Schenley Park adjacent to the CMU campus in Pittsburgh — and widely used in furniture. Like Erodium, veneers respond to moisture.

"Seeds have a magic response to rain," Yao said. 

Growing up in Inner Mongolia, Yao learned early from her parents the importance of timing the seeding process with the prospect of rain. Her appreciation for that timing grew during this project, as the researchers did plenty of field testing of the carriers, rather than just lab tests. That meant they had to keep their eyes on the weather, rushing the carriers to a test field when rain was in the offing.

The team developed a five-step process including both chemical washing and mechanical molding to manufacture the seed carriers. Although the carriers are currently fabricated in the lab, the researchers anticipate adapting the process to an industrial scale.

"Making E-seed through digital design and fabrication methods is crucial for our long-term goals," said Guanyun Wang, a former postdoctoral researcher in the Morphing Matter Lab who continued on the project after assuming a faculty position at Zhejiang University. 

In addition to seeds, the researchers demonstrated they could use the carriers to deliver nematodes (worms used as natural pesticides), fertilizers and fungi. Work is also underway to adapt them for planting seedlings. 

"Gaining insight into the mechanics of wood and seed drilling dynamics leads to improved design and optimization," said Teng Zhang, associate professor of mechanical and aerospace engineering at Syracuse University, who performed modeling and simulations to explain the working mechanism of the wood actuators and the benefits of E-seed's three-tailed design. 

These applications were possible thanks to a user study conducted by Aditi Maheshwari and Andreea Danielescu from ​Accenture Labs, who interviewed subject matter experts in reforestation, agriculture and soil health management to inform the applicability of E-seed in the real world.

"Understanding real-world applications of bioengineered technologies like E-seed is crucial for advancing ecological design," said Maheshwari, research and development principal at Accenture Labs, who works on sustainable materials and environments.

Danielescu, director of the Future Technologies R&D group at Accenture Labs, said E-seed can improve ecological resilience. 

"Technologies like E-seed can help us address real-world problems — helping us avoid landslides, reducing the impact of invasive species and improving reforestation of hard-to-reach places," Danielescu said. 

The carriers also could be used to implant sensors for environmental monitoring. They might also assist in energy harvesting by implanting devices that create current based on temperature fluctuations.

"The interest in the research from agriculture, forestry and other disciplines has been encouraging," Yao said. But perhaps one of the most important endorsements came from a source close to her: her father, the part-time farmer.

"When I mentioned the idea to him, he got it immediately."


E-seeds are dropped from a drone during a field test of the engineered seed carriers.

E-seeds on the ground near Hangzhou, China, after being dropped from a drone.

A vegetable plant growing next to its E-seed carrier. This seed was planted in a garden on Carnegie Mellon University’s campus in Pittsburgh, Pennsylvania.

CREDIT

Carnegie Mellon University