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30 April 2025 | Story Leonie Bolleurs | Photo Supplied
Dr Palesa Mohajane
Dr Palesa Mohajane, scientist production at the Department of Water and Sanitation, received her PhD from the UFS for her research on the impact of pandemic-related burials on groundwater quality.

Dr Palesa Mohajane, a scientist production at the Department of Water and Sanitation in Hartbeespoort, was recently awarded her doctoral degree at the University of the Free State’s (UFS) autumn graduation ceremony. Her thesis, titled Modelling the effect of pandemic-induced burials on groundwater contamination: a hydrogeological and epidemiological assessment, looks at the impact of increased burial rates on groundwater quality.

 

Safeguarding groundwater resources

Dr Mohajane explains that witnessing the dramatic rise in burial rates during the COVID-19 pandemic – including instances of mass burials – and the resulting strain on cemeteries, raised concerns about the potential risk of groundwater contamination. This became a motivator for her research.

Her study bridges the gap between environmental science and epidemiology, developing tools to predict how disease outbreaks and related deaths can impact groundwater systems. “By focusing on this intersection, the study contributes knowledge that informs not only responsible cemetery management, but also the protection of groundwater resources important to public health,” she says.

Dr Mohajane highlights the environmental risks that come with an increase in burial activity during pandemics. “When death rates rise sharply, cemeteries experience a surge in burials, which accelerates decomposition within confined spaces. As bodies decompose, they release organic and inorganic pollutants, which can seep through geological layers and affect groundwater quality.”

She notes that if cemeteries are established without proper hydrogeological assessments, these substances can infiltrate the soil and contaminate water sources, posing a threat to both environmental and human health.

 

Using advanced tools to predict groundwater pollution

Dr Mohajane conducted her research during the post-pandemic period when the longer-term environmental effects of COVID-19-related burial practices began to surface. “Groundwater sampling and quality testing were conducted between September 2023 and January 2024. This period provided a suitable time frame to monitor contaminant release and assess the hydrochemical effects of the burial practices,” she explains.

Langberg Cemetery was selected as a case study due to its representative geological and human-made characteristics, making it a strong candidate for validating the research models. “This site allowed for real-world testing of the mathematical models and simulations, offering important insights into how contaminants move through soil and rock layers and impact groundwater,” says Dr Mohajane.

Her findings revealed that groundwater contamination is influenced by multiple interacting factors – including burial depth, body mass, and geological features. She explains that shallower burials allow pollutants to reach the water table more rapidly, while deeper burials may delay but not prevent eventual leaching. Larger body masses produce more decomposing material, increasing the number of pollutants released. Geological conditions such as fractures and varied rock formations also play a role in the spread of contaminants.

Dr Mohajane’s work has serious implications for both public health and water sustainability. The presence of elevated levels of total dissolved solids, electrical conductivity, specific ions, alkalinity, and mineralisation indicates potential health hazards. As groundwater is an important source of drinking water, she stresses the urgency of addressing these risks. “We need to use advanced tools to predict and prevent groundwater pollution before it occurs. With proper water management systems, we can reduce the environmental impact of pandemics,” she says.

She also emphasises the importance of continuous monitoring to detect pollutant levels that exceed safety limits. “Improving burial practices – including thorough geological assessments before establishing cemeteries and optimising burial depths – can help reduce contaminant migration. These measures are important to protect community water resources,” she adds.

 

Measures to protect groundwater and public health

Dr Mohajane’s research proposes a range of practical measures to safeguard groundwater and public health. Cemeteries should only be developed after detailed geological evaluations, and clear regulations must guide cemetery design to manage increased burial needs during pandemics. Regular water quality monitoring using modern detection tools is key, along with the inclusion of environmental assessments in public health planning.

“These policy measures, if adopted at both regional and national levels, can help to reduce the risk of groundwater pollution and support long-term public health,” she says.

Ultimately, this research supports South Africa’s efforts to protect its groundwater by encouraging collaboration between scientists and policy makers. It offers predictive tools, evidence-based guidelines for sustainable cemetery management, and highlights how scientific research can shape practical, effective policies. The goal is to ensure that groundwater remains a safe and secure resource during future public health and environmental crises.

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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