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31 August 2021 | Story Leonie Bolleurs | Photo Supplied
UFS scientists involved in revolutionary protein structure prediction
Left: Dr Ana Ebrecht, a former postdoctoral student of the UFS, was part of the team that validated the data for the Science paper. Right: Prof Dirk Opperman was involved in a revolutionary finding in biology, which predicts the structure of a protein. His work in collaboration with other scientists has been published in Science.

Prof Dirk Opperman, Associate Professor in the Department of Microbiology and Biochemistry at the University of the Free State (UFS), in collaboration with Dr Ana Ebrecht (a former postdoc in the same department) and Prof Albie van Dijk from the Department of Biochemistry at the North-West University (NWU), was part of an international collaboration of researchers who participated in solving an intricate problem in science – accurate protein structure prediction.

The team of researchers recently contributed to an influential paper describing new methods in protein structure prediction using machine learning. The paper was published in the prestigious scientific journal, Science.

“These new prediction methods can be a game changer,” believes Prof Opperman.

“As some proteins simply do not crystalise, this could be the closest we get to a three-dimensional view of the protein. Accurate enough prediction of proteins, each with its own unique three-dimensional shape, can also be used in molecular replacement (MR) instead of laborious techniques such as incorporating heavy metals into the protein structure or replacing sulphur atoms with selenium,” he says.

Having insight into the three-dimensional structure of a protein has the potential to enable more advanced drug discovery, and subsequently, managing diseases.

Exploring several avenues …

According to Prof Opperman, protein structure prediction has been available for many years in the form of traditional homological modelling; however, there was a big possibility of erroneous prediction, especially if no closely related protein structures are known.

Besides limited complementary techniques such as nuclear magnetic resonance (NMR) and electron microscopy (Cryo-EM), he explains that the only way around this is to experimentally determine the structure of the protein through crystallisation and X-ray diffraction. “But it is a quite laborious and long technique,” he says.

Prof Opperman adds that with X-ray diffraction, one also has to deal with what is known in X-ray crystallography as the ‘phase problem’ – solving the protein structure even after you have crystallised the protein and obtained good X-ray diffraction data, as some information is lost.

He states that the phase problem can be overcome if another similar-looking protein has already been determined.

This indeed proved to be a major stumbling block in the determination of bovine glycine N-acyltransferase (GLYAT), a protein crystallised in Prof Opperman’s research group by Dr Ebrecht, currently a postdoc in Prof Van Dijk’s group at the NWU, as no close structural homologous proteins were available.

“The collaboration with Prof Opperman’s research group has allowed us to continue with this research that has been on hold for almost 16 years,” says Prof Van Dijk, who believes the UFS has the resources and facilities for structural research that not many universities in Africa can account for.

The research was conducted under the Synchrotron Techniques for African Research and Technology (START) initiative, funded by the Global Challenges Research Fund (GCRF). After a year and multiple data collections at a specialised facility, Diamond Light Source (synchrotron) in the United Kingdom, the team was still unable to solve the structure.

Dr Carmien Tolmie, a colleague from the UFS Department of Microbiology and Biochemistry, also organised a Collaborative Computational Project Number 4 (CCP4) workshop, attended by several well-known experts in the field. Still, the experts who usually participate in helping students and researchers in structural biology to solve the most complex cases, were stumped by this problem.

Working with artificial intelligence

“We ultimately decided to turn to a technique called sulphur single-wavelength anomalous dispersion (S-SAD), only available at specialised beam-lines at synchrotrons, to solve the phase problem, says Prof Opperman.

Meanwhile, Prof Randy Read from the University of Cambridge, who lectured at the workshop hosted by Dr Tolmie, was aware of the difficulties in solving the GLYAT structure. He also knew of the Baker Lab at the University of Washington, which is working on a new way to predict protein structures; they developed RoseTTAaFold to predict the folding of proteins by only using the amino acid sequence as starting point.

RoseTTAaFold, inspired by AlphaFold 2, the programme of DeepMind (a company that develops general-purpose artificial intelligence (AGI) technology), uses deep learning artificial intelligence (AI) to generate the ‘most-likely’ model. “This turned out to be a win-win situation, as they could accurately enough predict the protein structure for the UFS, and the UFS in turn could validate their predictions,” explains Prof Opperman.

A few days after the predictions from the Baker Lab, the S-SAD experiments at Diamond Light Source confirmed the solution to the problem when they came up with the same answer.

Stunning results in a short time

“Although Baker’s group based their development on the DeepMind programme, the way the software works is not completely the same,” says Dr Ebrecht. “In fact, AlphaFold 2 has a slightly better prediction accuracy. Both, however, came with stunningly good results in an incredibly short time (a few minutes to a few hours),” she says.

Both codes are now freely available, which will accelerate improvements in the field even more. Any researcher can now use that code to develop new software. In addition, RoseTTAFold is offered on a platform accessible to any researcher, even if they lack knowledge in coding and AI.

News Archive

Discovery in Scorpius constellation may signify clean energy for Earth
2017-01-23

 Description: Discovery in Scorpius constellation may signify clean energy for Earth Tags: Discovery in Scorpius constellation may signify clean energy for Earth

Earlier this year, a group of international astronomers
announced the discovery of an exotic binary star system,
AR Scorpii. The system is in the Scorpius constellation.
Photos: Supplied

See article on Nature’s website 

In future, stargazers and astronomers will look at the Scorpius constellation near the Milky Way with new eyes. Earlier this year, a group of international astronomers announced the discovery of an exotic binary star system, AR Scorpii. The system is in the Scorpius constellation.

Prof Pieter Meintjes, researcher in the Department of Physics at the University of the Free State (UFS), worked with four colleagues on what he describes as a “wonderful discovery”. This sensational discovery, which could lead to the production of cleaner energy on Earth, will be published in the research journal, Nature, early in 2017.

Model developed to interpret new set of measurements
The exotic binary star which was discovered consists of a red dwarf and a white dwarf revolving around each other every 3,5 hours. The binary system showed very prominent pulsations of 117 and 118 seconds respectively. The pulsations can be explained by a bundle radiation produced by the white dwarf star.

“These new observations have shown that the radiation is strongly polarised, a sign that we are dealing with synchrotron radiation here. Synchrotron radiation is produced by electrons accelerated to extremely high energy levels in the magnetic field of the white dwarf star,” says Prof Meintjes.

He developed a theoretical model to interpret a new set of measurements that was taken by the 1,9 m telescope and the 10 m SALT telescope at the South African Astronomical Observatory (SAA0).

Totally unique phenomenon could contribute to energy production on Earth
“I further indicated that the interaction between the magnetic fields of the white dwarf star and the red dwarf star induces secondary processes that specifically describe the behaviour of the radiation in the radio band and infrared band accurately. AR Sco is the first white-red dwarf binary system of which all the pulsated radiation could be explained by the synchrotron process, which is totally unique,” says Prof Meintjes.

According to Prof Meintjes, the value of the model lies in the fact that the processes which produce the radiation in AR Sco, can also be applied to produce energy on Earth.

 

Plasma reactors are based on roughly the same processes which apply in AR Sco, and with refining, it could be utilised to generate electricity in future. This will be much cleaner than nuclear energy.

 

The model developed by Prof Meintjes explains all the radiation in the system – from radio waves to X-rays – in terms of electrons accelerated to extremely high energy levels by electric fields in the system, which then produce synchrotron radiation over a very wide band of the electromagnetic spectrum.

Prof Meintjes is currently working on a follow-up article examining the evolution of the AR Sco, in other words, the origin of such a unique system and the final state towards which it is evolving. “My vision for the immediate future is therefore to develop a model for the evolution of the source concerned,” he says.

 

 

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