Latest News Archive

Please select Category, Year, and then Month to display items
Previous Archive
07 December 2023 | Story Leonie Bolleurs | Photo Charl Devenish
Dr Michelle Goliath
Dr Michelle Goliath received her PhD, providing significantly useful insights into artisanal mining. She says it is the prospect of contributing to positive change and advancing understanding in the field that has been the most exciting and fulfilling aspect of completing this research.

Dr Michelle Goliath completed her PhD in the Department of Urban and Regional Planning at the University of the Free State (UFS) and received her qualification during the December graduations. 

The PhD, which she began in 2018 under supervision of Prof Malene Campbell, is titled Urban Pacification Strategies and Solutions: Towards a Contested Space Theory of Artisanal Mining.

The focus of her thesis was on finding strategies to address informal mining in urban areas. “It considers the formalisation of informal miners, adapted land use management, risk management solutions, and action research to solve complex problems. In addition, it also looks at the social, economic, and environmental dimensions of the challenge and proposes a unique practical methodology on how to solve similar complex problems and challenges that urban planners and policy makers face daily,” explains Dr Goliath. 

A foundation for informed decision making

She is of the opinion that her research provides a foundation for informed decision making by town planners who seek to proactively address and mitigate challenges around artisanal mining.

Dr Goliath’s thesis introduces innovative strategies for managing land use specifically designed for the challenges of artisanal mining. She believes that recognising the importance of flexible and innovative land-use policies demonstrates a deep understanding of the spatial aspects involved in effectively accommodating and regulating artisanal mining activities. As reported by Dr Goliath, this customised approach ensures that the rules fit the unique characteristics of artisanal mining, promoting sustainable urban development.

Moreover, by integrating action research methodologies into the thesis, a dynamic and collaborative element is introduced into the decision-making process. She says that engaging in practical, on-the-ground research in collaboration with practitioners – in this instance a community of women artisanal miners in Kimberley – advocates for evidence-based decision making in urban planning. “This approach not only enriches the theoretical foundation of the thesis, but also ensures that the proposed solutions are rooted in the practical realities of the South African context,” she states.

Furthermore, the thesis offers both theoretical insights and practical policy recommendations, ensuring that its research findings extend beyond academia. These insights are directly applicable to the challenges confronted by town planners in South Africa and policy planners in other SADEC countries who are still navigating the policy process for similar challenges. “The incorporation of global trends in artisanal mining allows for a comparative approach, enhancing the relevance and transferability of the recommendations both locally and internationally,” remarks Dr Goliath.

The impact of empowerment

She says it is fulfilling to witness the transformative impact of empowerment. “Engaging with and supporting women in the artisanal mining sector has not only enhanced their economic opportunities but has also contributed to broader social and community development. It is the empowerment of these women, their resilience, and the tangible positive shifts in their lives that stand out as the most rewarding and impactful outcomes of my work in Kimberley.”

Besides the opportunity to help this group of women, she was also excited about the chance to contribute new knowledge and insights to the field. “The process of delving into unexplored aspects of artisanal mining in Kimberley, conducting thorough investigations, and analysing longitudinal data has been intellectually stimulating,” she states.

“The prospect of offering novel perspectives, innovative solutions, and evidence-based recommendations through my research is particularly thrilling. Witnessing the potential for this work to make a meaningful impact on policies, practices, and the lives of individuals involved in artisanal mining adds a sense of purpose and excitement to the research journey,” concludes Dr Goliath.

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.

We use cookies to make interactions with our websites and services easy and meaningful. To better understand how they are used, read more about the UFS cookie policy. By continuing to use this site you are giving us your consent to do this.

Accept