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06 May 2025 | Story Tshepo Tsotetsi | Photo Supplied
Critical Dialogue
Guest speaker, Prof Gordon Zide, delivers his keynote address at the EDSA Critical Dialogue Series 2025.

The Office of the Executive Director: Student Affairs at the University of the Free State (UFS) hosted its annual Critical Dialogue Series on 29 April 2025 at the Centenary Complex on the Bloemfontein Campus. The dialogue brought together students, staff, and university leadership for an engaging conversation around ethical and servant leadership in higher education.

 

A conversation rooted in purpose

In his opening address, Temba Hlasho, Executive Director for Student Affairs said the dialogue was designed to provoke honest reflection and engagement on issues that affect student experience and institutional culture.

“We believe that there has to be some sort of transparency in terms of having to talk about topical issues that are very critical, that also touch on the very nerve of student experience,” Hlasho said.

He encouraged student leaders to see the platform not as ceremonial, but as a call to action. “You are in a country today where ethics have almost decayed. You, as the future of this country, will rely solely on the young people to change the narrative.”

 

Leadership anchored in service

UFS Vice-Chancellor and Principal Prof Hester C. Klopper delivered a powerful message on the importance of ethical and servant leadership in guiding the university’s direction. “Leadership – and specifically ethical and servant leadership – forms the cornerstone of what we stand for at the University of the Free State.”

She spoke about accountability, fairness, and leading with integrity. “It means treating every student fairly regardless of background or belief, and holding yourself accountable for your actions and decisions.”

Prof Klopper also highlighted the vital role student leaders play in shaping a culture of trust and excellence. “Leadership is not a title or a position, but a daily choice to serve with integrity, empathy, and purpose.”

 

Ubuntu, transformation, and power dynamics

The event’s keynote speaker was Prof Gordon Zide, an accomplished scholar, academic, intellectual, Africanist, author, transformation specialist, motivational speaker, and a former Vice-Chancellor and Principal of the Vaal University of Technology. Prof Zide is also a former Registrar at the University of South Africa. Drawing from a lifetime of experience in the sector, he interrogated the moral responsibilities of leadership within the South African higher education landscape.

“Leadership is a function of being a servant and being in charge of others,” he said. “It also requires the capacity to give strategic direction for the effective, efficient, and valued functioning of organisations.”

He emphasised that ethical leadership should be grounded in values such as vision, passion, patience, integrity, honesty, decisiveness, character, and charisma. Reflecting on the African philosophy of ubuntu, Prof Zide remarked: “When talking about servant leadership, it’s important to recognise other people and say to yourself: ‘I am what I am because of other people.’”

He encouraged students, particularly the current generation, to take charge and assume ethical leadership roles in their spaces. Referencing prominent anti-apartheid figure Robert Sobukwe, he urged, “Even when we are no longer here, they will always remember that we were there.”

Prof Zide also noted the practical benefits of ethical leadership in institutions, saying that it improves brand image, boosts morale among staff and students, and strengthens the recruitment process. He concluded by challenging the Department of Higher Education and Training (DHET), saying its tendency to micromanage universities undermines the autonomy and leadership authority of institutional management.

 

A call to lead with intention

Reflecting on the impact of the event, Acting President of the Institutional Student Representative Council (ISRC) Mpho Maloka said, “These kinds of conversations are needed because they help us go back to the ‘why’ – why we became student leaders in the first place, and how we can serve students in ways that actually make a difference.”

She added, “People have turned student leadership into something so political that others don’t even want to get involved. Dialogues like this bring it back to what really matters – serving students and growing as ethical leaders.”

As Prof Klopper concluded: “The lessons in ethical and servant leadership that you learn and practise here prepare you not just for impactful careers, but for responsible citizenship in a world desperately in need of ethical leadership.”

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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