First-authors Gavin Rice (left) and Thorsten Wagner (right).
First-authors Gavin Rice (left) and Thorsten Wagner (right).

Germany creates AI software for dependable imaging of proteins in cells

Max Planck researchers from Dortmund programmed a tool that accurately recognizes and picks proteins in electron cryo-tomography, substituting troublesome hand selection

Electron cryo-tomography (cryo-ET) is emerging as a powerful technique to provide detailed 3D images of cellular environments and enclosed biomolecules. However, one of the challenges of the methodology is the identification of protein molecules in the images for further processing. A research team around Stefan Raunser, Director at the MPI of Molecular Physiology in Dortmund, led by Thorsten Wagner, developed software to pick proteins in crowded cellular volumes. The new open-source tool, called TomoTwin, is based on deep metric learning and allows scientists to locate several proteins with high accuracy and throughput without manually creating or retraining the network each time. TomoTwin processing map for a tomogram flattened to 2D. Particles of different macromolecules are arranged in the map according to their structure allowing users to identify and locate different macromolecules inside cells.

The more, the better

“TomoTwin paves the way for automated identification and localization of proteins directly in their cellular environment, expanding the potential of cryo-ET,” says Gavin Rice, co-first author of the publication. Cryo-ET has the potential to decipher how biomolecules work within a cell and, by that, to unveil the basis of life and the origin of diseases.

In a cryo-ET experiment, scientists use a transmission electron microscope to obtain 3D images, called tomograms, of the cellular volume containing complex biomolecules. To gain a more detailed image of each different protein, they average as many copies of them as possible – similar to photographers capturing the same photo at varying exposures to later combine them in a perfectly exposed image. Crucially, one has to correctly identify and locate the different proteins in the picture before averaging them. “Scientists can attain hundreds of tomograms per day, but we lacked tools to fully identify the molecules within them,” says Rice.

Hand-picking

So far, researchers used algorithms based on templates of already known molecular structures to search for matches in the tomograms, but these tend to be error-prone. Identifying molecules by hand is another option that ensures high-quality picking but takes days to weeks per dataset.

Another possibility would be to use a form of supervised machine learning. These tools can be very accurate but currently lack usability, as they require manually labeling thousands of examples to train the software for each new protein, an almost impossible task for small biological molecules in a crowded cellular environment.

TomoTwin

The newly developed software TomoTwin overcomes many of these obstacles: It learns to pick the molecules that are similar in shape within a tomogram and maps them to a geometric space – the system is rewarded for placing similar proteins near each other and penalized otherwise. In the new map (image 1), researchers can isolate and accurately identify the different proteins and use this to locate them inside the cell. “One advantage of TomoTwin is that we provide a pre-trained picking model,” says Rice. By removing the training step, the software can even run on local computers – where processing a tomogram usually requires 60-90 minutes, and runtime on the MPI supercomputer Raven is reduced to 15 minutes per tomogram.

TomoTwin allows researchers to pick dozens of tomograms in the time it takes to manually pick a single one, therefore increasing the throughput of data and the averaging rate to obtain a better image. The software can currently locate globular proteins or protein complexes larger than 150 kilodaltons in cells; in the future, the Raunser group aims to include membrane proteins, filamentous proteins, and proteins of smaller sizes.

Schematic of the inflaton field fragmented into oscillons, with superimposed gravitational waves. (Credit: Kavli IPMU, Volodymyr Takhistov)
Schematic of the inflaton field fragmented into oscillons, with superimposed gravitational waves. (Credit: Kavli IPMU, Volodymyr Takhistov)

Japanese researchers discover, explore the earliest Universe dynamics with gravitational waves

Researchers have discovered a new generic production mechanism of gravitational waves generated by a phenomenon known as oscillons, which can originate in many cosmological theories from the fragmentation into solitonic “lumps” of the inflaton field that drove the early Universe’s rapid expansion. The results have set the stage for revealing exciting novel insights about the Universe's earliest moments.

The inflationary period, which occurred just after the Big Bang, is believed to have caused the Universe to expand exponentially. In many cosmological theories, the rapid expansion period is followed by the formation of oscillons. Oscillons are a type of localized non-linear massive structure that can form from fields, such as the inflaton field, which are oscillating at high frequencies. These structures can persist for long periods, and as the researchers found, their eventual decay can generate a significant amount of gravitational waves, which are ripples in space-time.

In their study, Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU) Project Researcher Kaloian D. Lozanov, and Kavli IPMU Visiting Associate Scientist, International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles (QUP) Senior Scientist, and High Energy Accelerator Research Organization (KEK) Theory Center Assistant Professor Volodymyr Takhistov, have simulated the evolution of the inflaton field during the early Universe and found that oscillons were indeed present. They then found that oscillon decay was able to generate gravitational waves that would be detectable by upcoming gravitational wave observatories.

The findings provide a novel test of the early Universe dynamics independent of the conventionally studied cosmic microwave background radiation. The discovery of these gravitational waves would establish a new window into the Universe's earliest moments and could help shed light on some of the pressing fundamental questions in cosmology.

With the ongoing development of gravitational wave detectors and supercomputing resources, we can expect to gain even more insights into the Universe's early moments in the coming years. Overall, the new study demonstrates the power of combining theoretical models with advanced computational techniques and observations to uncover new insights into the Universe's evolution.

Artist's impression of how astronomical forces affect the Earth's motion, climate, and ice sheets. (Credit: NAOJ)
Artist's impression of how astronomical forces affect the Earth's motion, climate, and ice sheets. (Credit: NAOJ)

Japanese climatologists, astronomers use a supercomputer to enhance their models of the ice ages

A research team, composed of climatologists and an astronomer, has used an improved supercomputer model to reproduce the cycle of ice ages (glacial periods) 1.6 to 1.2 million years ago. The results show that the glacial process was driven primarily by astronomical forces in quite a different way than it works in the modern age. These results will help us better understand ice sheets' past, present, and future and the Earth’s climate.

Earth’s orbit around the Sun and its spin axis orientation change slowly over time, due to the pull of gravity from the Sun, the Moon, and other planets. These astronomical forces affect the environment on Earth due to changes in the distribution of sunlight and the contrast between the seasons. In particular, ice sheets are sensitive to these external forces resulting in a cycle between glacial and interglacial periods.

The present-day glacial-interglacial cycle has a period of about 100,000 years. However, the glacial cycle in the early Pleistocene (about 800,000 years ago) switched more rapidly, with a process of about 40,000 years. It has been believed that astronomical external forces are responsible for this change, but the details of the mechanism have not been understood. In recent years, it has become possible to investigate in more detail the role of astronomical forces through the refinement of geological data and the development of theoretical research.

A team led by Yasuto Watanabe at the University of Tokyo focused on the early Pleistocene Epoch from 1.6 to 1.2 million years ago using an improved climate supercomputer model. Astronomical forces based on modern state-of-the-art theory are considered in these simulations. The extensive numerical simulations in this study reproduce well the glacial cycle of 40,000 years of the early Pleistocene as indicated by the geological record data.

From the analysis of these simulation results, the team has identified three facts about the mechanisms by which astronomical forces caused changes in climate in those times. (1) The glacial cycle is determined by slight differences in the amplitude of variation of the spin axis orientation and the orbit of the Earth. (2) The timing of deglaciation is determined mainly by the position of the summer solstice on its orbit, which is at perihelion, not only by the effect of periodical change of the tilt of the Earth’s axis. (3) The timing of the change in the spin axis orientation and the position of the summer solstice on its orbit determines the duration of the interglacial period.

 “As geological evidence from older times comes to light, it is becoming clear that the Earth had a different climatic regime than it does today. We must have a different understanding of the role of astronomical forcing in the distant past,” says Takashi Ito from the National Astronomical Observatory of Japan, a member of this research team who led the discussion on astronomical external forces. “The numerical simulations performed in this study not only reproduce the Pleistocene glacial-interglacial cycle well but also successfully explain the complex effects of how astronomical forcing drove the cycle at that time. We can regard this work as a starting point for the study of glacial cycles beyond the present-day Earth.”

A 3D model of the Commander complex, a bundle of proteins that act as postal workers in cells.
A 3D model of the Commander complex, a bundle of proteins that act as postal workers in cells.

Australian researchers use AI to better understand dementia, infectious diseases including COVID-19

Professor Brett Collins from the University of Queensland (UQ) Institute for Molecular Bioscience and Professor Pete Cullen from the University of Bristol led a team that modeled the 16-subunit Commander complex, a bundle of proteins that act as ‘postal workers’ in cells.

“Just as the postal system has processes to transport and sort cargo, cells in our bodies have molecular machines that transport and sort proteins,” Professor Collins said.  A 3D model of the Commander complex, a bundle of proteins that act as postal workers in cells.

“Cargo transport is all about getting the right parcels to the right destination at the right time and in cells, the Commander complex controls this system to ensure the right amount of protein is delivered to the right place.”

This protein transport system is implicated in many diseases including heart disease, Alzheimer’s disease, and infections.

“Knowing the 3D shape of these proteins helps us understand how they function, why mutations cause disease, and how to design drugs to target them in the future,” Professor Collins said.

“Viruses such as SARS-CoV-2 – which causes COVID-19 – and human papillomavirus (HPV) which can lead to cancer need the Commander complex to infect cells and it has been linked to the transport of the amyloid protein in Alzheimer’s disease.

“Mutations in the Commander complex disrupt the transport of lipids into cells, causing high cholesterol and heart defects in people with the rare Ritscher-Schinzel syndrome which is characterized by intellectual disability and development delay.

“Knowing the structure of the Commander complex means we can better understand how this happens and advance our understanding of how it is involved in disease.” 

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The international team used state-of-the-art electron microscopy and machine learning methods to decipher the structure of the entire Commander protein complex.

Professor Cullen said mapping the complete structure of the Commander complex would not have been possible even 2 years ago without these new technologies.

The team also included Dr. Michael Healy from IMB, Dr. Kerrie McNally from the University of Cambridge, and Rebeka Butkovic and Molly Chilton from the University of Bristol.

This research was funded by organizations including the National Health and Medical Research Council (Australia), Medical Research Council (UK), and the Wellcome Trust.

The research is published in Cell.

Assembly of the 3D model of the Commander Complex

The Commander Complex is a 16-subunit bundle of proteins that act as ‘postal workers’ in cells, transporting and sorting proteins. This protein transport system is implicated in many diseases including heart disease, Alzheimer’s disease, and infections.

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