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28 August 2025 | Story André Damons | Photo André Damons
Dr Bonita van der Westhuizen
Dr Bonita van der Westhuizen, Senior lecturer and Pathologist in the UFS Department of Medical Microbiology, identified the first case of S. oblongispora mucormycosis in sub-Saharan Africa and among HIV-positive patients.

Medical staff at the University of the Free State (UFS) and the National Health Laboratory Service (NHLS) at the Universitas Academic Hospital have identified the first case of S. oblongispora mucormycosis in sub-Saharan Africa and among HIV-positive patients.

This discovery was made when a 32-year-old male patient was admitted to the Universitas Academic Hospital with right-sided facial swelling. The patient was HIV-positive, with a CD4 count of 50 cells/µl, and on antiretroviral therapy (ART), together with trimethoprim–sulfamethoxazole (TMX) prophylaxis. Additionally, he had hypertension for which he was also receiving treatment. The patient’s facial swelling rapidly progressed, with extension of redness and swelling observed daily.

Four days after admission, he underwent computerised tomography (CT) scan, and tissue biopsies were collected. The patient died three days later.

 

A significant discovery

Dr Bonita van der Westhuizen, Senior lecturer and Pathologist in the UFS Department of Medical Microbiology, who identified this rare fungus said this discovery is significant because it highlights the presence of this fungal pathogen in a region where it may have been previously unrecognised or underreported. It now raises awareness about the diversity of fungal infections affecting immunocompromised populations and underscores the need for improved diagnostics, surveillance, and treatment strategies in the region.

Dr Van der Westhuizen says though it is unclear where the deceased might have picked up this infection, moulds are ubiquitous in the environment. Patients usually get infected by inhalation of spores or traumatic implantation.

Together with colleagues Drs Liska Budding and Christie Esterhuysen, both from the UFS Department of Anatomical Pathology and the NHLS, and Prof Samantha Potgieter, Infectious disease expert in the UFS Department of Internal Medicine, Dr Van der Westhuizen published the case earlier this month (August) in the Journal Case Reports in Pathology.

 

Progresses rapidly

“Mucormycosis, which is caused by fungi in the order Mucorales, progresses rapidly due to a combination of factors related to the fungus, the host, and external influences. Mucorales fungi are known for their fast growth and ability to invade blood vessels. This allows the infection to spread quickly through the body, potentially reaching vital organs,” she says.

These fungi, Dr Van der Westhuizen explains, can resist being killed by immune cells, allowing them to establish infection. Some Mucorales fungi can produce toxins that disrupt blood vessels, further aiding the spread of the infection. Additionally, certain host conditions weaken the body's defences, allowing the infection to spread quickly.

“External factors that may play a role are traumatic injuries, endothelial damage and rarely hospital acquired infections. In essence, the aggressive nature of Mucorales fungi combined with weakened host defences and external factors creates a perfect storm for rapid disease progression in susceptible individuals.

“The Mucorales as a group normally infects patients with underlying risk factors including factors including diabetes mellitus, malignancies, transplant recipients, and current or past COVID-19 infection, however, this organism in particular, usually infects immunocompetent patients after traumatic inoculation,” says Dr Van der Westhuizen.

It is important to note, she continues, that all available data comes from research done in tropical regions. There is no data on this organism in sub-Saharan Africa which means it is still unknown what role this pathogen plays in our local patient population. The diagnostic complexities and rapid disease progression may contribute to the paucity of data in developing countries.

This infection can be treated with available antifungal agents, as well as surgical debridement of infected tissue. The challenge, however, is the rapid disease onset and progression to death. There is only a tiny window to help the patient. That is why clinical suspicion is so important, as immediate aggressive surgical debridement with antifungal agents is the only way to improve patient outcome. Unfortunately, this infection still has a high mortality rate, despite therapy.

 

Fungal diagnostics is complex

An invasive fungal infection (IFI) was not suspected in this patient, and he received neither antifungal therapy nor surgical interventions. His cause of death, likely the IFI, was only identified after he passed away and because of a combination of different testing platforms was used to identify this infection. Says Dr Van der Westhuizen: “This is unfortunately the case with mould infections as most readily available diagnostic methods lack sensitivity and these pathogens take long to grow in the laboratory. Fungal diagnostics is a specialised field that requires expertise. However, if clinicians are aware of these infections and they have an increased index of suspicion, appropriate therapy can be initiated even before the results are available.

“If clinicians suspect this type of infection early and they involve the infectious diseases physicians, microbiology and histopathology for support and advice, they will be guided to collect the most appropriate samples to ensure that an accurate diagnosis is made.”

There is a possibility that these infections had been missed before and even still today. Fungal diagnostics is a very complex field for various reasons. There is no highly sensitive stand-alone test to make a rapid diagnosis available. As newer methods are being developed and molecular diagnostics are advancing, fungal diagnostics are improving. A combination of testing platforms is still required to improve the sensitivity of diagnosing these infections.

Her hope for this research, says Dr Van der Westhuizen, who will now also embark further research into local fungal species for her PhD, their epidemiology, diagnostics, and their impact on vulnerable populations, ultimately contributing to better clinical care and health outcomes, is to advance understanding and awareness of Invasive mould infections specifically S. oblongispora, in sub-Saharan Africa and among HIV patients. She aims to improve early diagnosis, treatment strategies, and clinical outcomes, as well as to highlight the importance of monitoring fungal infections in immunocompromised populations. Additionally, her goal includes encouraging further research and collaboration in this area to better address fungal infections in the region.

News Archive

UFS physicists publish in prestigious Nature journal
2017-10-16

Description: Boyden Observatory gravitational wave event Tags: Boyden Observatory, gravitational wave event, Dr Brian van Soelen, Hélène Szegedi, multi-wavelength astronomy 
Hélène Szegedi and Dr Brian van Soelen are scientists in the
Department of Physics at the University of the Free State.

Photo: Charl Devenish

In August 2017, the Boyden Observatory in Bloemfontein played a major role in obtaining optical observations of one of the biggest discoveries ever made in astrophysics: the detection of an electromagnetic counterpart to a gravitational wave event.
 
An article reporting on this discovery will appear in the prestigious science journal, Nature, in October 2017. Co-authors of the article, Dr Brian van Soelen and Hélène Szegedi, are from the Department of Physics at the University of the Free State (UFS). Both Dr Van Soelen and Szegedi are researching multi-wavelength astronomy.
 
Discovery is the beginning of a new epoch in astronomy
 
Dr van Soelen said: “These observations and this discovery are the beginning of a new epoch in astronomy. We are now able to not only undertake multi-wavelength observations over the whole electromagnetic spectrum (radio up to gamma-rays) but have now been able to observe the same source in both electromagnetic and gravitational waves.”
 
Until recently it was only possible to observe the universe using light obtained from astronomical sources. This all changed in February 2016 when LIGO (Laser Interferometer Gravitational-Wave Observatory) stated that for the first time they had detected gravitational waves on 14 September 2015 from the merger of two black holes. Since then, LIGO has announced the detection of two more such mergers. A fourth was just reported (27 September 2017), which was the first detected by both LIGO and Virgo. However, despite the huge amount of energy released in these processes, none of this is detectable as radiation in any part of the electromagnetic spectrum. Since the first LIGO detection astronomers have been searching for possible electromagnetic counterparts to gravitational wave detections. 
 
Large international collaboration of astronomers rushed to observe source
 
On 17 August 2017 LIGO and Virgo detected the first ever gravitational waves resulting from the merger of two neutron stars. Neutron star mergers produce massive explosions called kilonovae which will produce a specific electromagnetic signature. After the detection of the gravitational wave, telescopes around the world started searching for the optical counterpart, and it was discovered to be located in an elliptical galaxy, NGC4993, 130 million light years away. A large international collaboration of astronomers, including Dr Van Soelen and Szegedi, rushed to observe this source.
 
At the Boyden Observatory, Dr Van Soelen and Szegedi used the Boyden 1.5-m optical telescope to observe the source in the early evening, from 18 to 21 August. The observations obtained at Boyden Observatory, combined with observations from telescopes in Chile and Hawaii, confirmed that this was the first-ever detection of an electromagnetic counterpart to a gravitational wave event. Combined with the detection of gamma-rays with the Fermi-LAT telescope, this also confirms that neutron star mergers are responsible for short gamma-ray bursts.  
 
The results from these optical observations are reported in A kilonova as the electromagnetic counterpart to a gravitational-wave source published in Nature in October 2017.
 
“Our paper is one of a few that will be submitted by different groups that will report on this discovery, including a large LIGO-Virgo paper summarising all observations. The main results from our paper were obtained through the New Technology Telescope, the GROND system, and the Pan-STARRS system. The Boyden observations helped to obtain extra observations during the first 72 hours which showed that the light of the source decreased much quicker than was expected for supernova, classifying this source as a kilonova,” Dr Van Soelen said.

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