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10 January 2022 | Story Rulanzen Martin | Photo Supplied
Dr Mpumelelo Ncube is a dynamic an academic with a clear vision of growth for the Department of Social work and its students.

A drive to be an advocate for social justice is what drove Dr Mpumelelo Ncube, the new head of the Department of Social Work, to pursue a degree and career in Social Work. “I needed to be an advocate for social justice and empowerment of the vulnerable individuals and communities,” said Dr Ncube, who took over from Prof Sandra Ferreira earlier this year. 

Dr Ncube’s academic and professional repertoire is exceptional and his deep-rooted passion for social work is definitely a bonus for the UFS Department of Social Work. He has a PhD in Social Work from the University of Johannesburg, a master’s degree in Social Development, and a Bachelor’s degree in Social Work from the University of Witwatersrand. 

Driven by the need to succeed in whatever task he sets for himself, Dr Ncube says that he strives to make the lives of those in his path better – “The positive change should, however, begin with me so that others could easily believe in my efforts.” 

Opportunity to raise a new generation

He joined academia in 2013 after working as a psychosocial services manager in the NGO sector. “My move to the UFS was in line with my career progression and the need to contribute meaningfully at a strategic level of social work education and practice,” Dr Ncube says.  

The opportunity to work in academia has in fact provided him with an excellent opportunity. “I have the opportunity to raise a new generation of social work professionals that would be passionate, ethical and professional in their practice. In that way, my impact as an educator can be felt in all corners where my students are,” Dr Ncube says. 

An academic of note 

As a senior lecturer, he also notes the tidal changes currently sweeping through academia. He says, “In the age of the fourth industrial revolution, the Social Work academic programme should be able to identify and embrace various developments that would provide the flexibility to attract postgraduate students in different places without the need for relocation. This relates to the delivery of the programme. However, apart from adapting to these changes, the Social Work programme should also foster a cultural innovation with students and enable them to embrace the technological advancements in their social work practice.”

“I have the opportunity to raise a new generation of social work professionals that would be passionate, ethical and professional in their practice.” – Dr Mpumelelo Ncube. 


Apart from being an advocate for social justice and a lecturer he also sees his position as HOD as a being a catalyst to enable others within the department to publishing more research. “Research is a key performance area for any academic, hence the mantra, ‘publish or perish’,” he says. However, he also cautions that trick of publishing research lies in “self-discipline, self-motivation and finding a research niche”.  

Social work is his passion

Social work is Dr Ncube’s passion but he also says that it is a profession, which is “seriously underutilised especially in under developing nations”. The socio-economic conditions in these countries largely drive the underutilisation. “These are nations largely plagued by poverty, unemployment, political illiteracy challenges with policy development and implementation, and moral degeneration among many challenges,” he says. In addition, it is therefore, as Dr Ncube mentions, that “the relevance of the social work profession shall be ever-present”.

  

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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