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28 May 2024 | Story Lunga Luthuli and Precious Shamase | Photo Supplied
Student Elections Debates 2024
Themba Hlasho, Executive Director: Student Affairs and Prof Prince Ngobeni, Qwaqwa Campus Principal were part of the debate series.

With South Africans going to the polls on 29 May 2024 for the seventh general elections since 1994, the University of the Free State (UFS) successfully hosted its first Institutional Elections Debate Series across its three campuses. The debates, organised by the Institutional Student Governance Office (ISGO), aimed to stimulate political engagement and intellectual discourse among students.

The debates took place on the three campuses and at different levels.  The debates were very successful; students were enthusiastic and well prepared to field critical questions to panellists.  The level of intellectual engagement was high and the facilitator, Ace Moloi – with his fine facilitation skills – helped to take the debates to higher levels.

Motlogelwa Moema, Head of the Student Governance Office, emphasised the alignment of the debates with the UFS’ commitment to societal progress and intellectual enquiry. "As an institution of higher learning, the UFS is committed to producing graduates who can function at various levels of society, contributing meaningfully to societal and intellectual enquiry. Platforms such as the debate series are important in stimulating political as well as electoral involvement while producing students who are leaders," Moema stated.

Student engagement in the electoral process was a key focus of the debates, with discussions highlighting the importance of translating campus political activity into national civic duty. Moema noted, "By bringing representatives from various political parties to all three campuses of the university, we ensured that students not only understood the importance of their votes, but also that they were able to align their values with those of the parties campaigning for their votes."

Informed voters: The debate allowed students to hear directly from the candidates about their platforms and stances on important issues. This can help students make informed decisions when they cast their votes.

Increased engagement: By hosting the debate, the Student Governance Office is encouraging student participation in the national elections. This led to a more vibrant and engaged student body.

Key themes of the debates included student funding, health care, governance, accountability, and economic policy. "The most topical theme across all three campuses was student funding. Additionally, students demonstrated great interest in the National Health Insurance, governance, and economic policies," Moema said, illustrating the depth and breadth of the discussions.

Reflecting on the role of universities in fostering political awareness, Moema acknowledged a generational disengagement from political activism. However, he stressed the importance of universities in cultivating a culture of debate and free thinking. "The recent debate series marked the beginning of the ISGO’s commitment to reviving dialogue across the university," he added.

Moema also highlighted the importance of universities in promoting critical enquiry and fact-checking, particularly during election periods. "Universities have a crucial role in creating platforms for fact-checking, critical enquiry, and clarification," he remarked.

Looking ahead, Moema hopes that the debate series will have a lasting impact on students’ democratic participation. "In the short term, the most ideal impact of the debate series should be a great turnout on election day. In the medium term, we hope to see the same energy during CSRC elections on all three campuses," he said.

The debate series was deemed a success, with significant improvements in turnout and the quality of engagement. "Our students showed a great level of tolerance for divergent views and respect for one another. The audience asked pertinent questions, showing remarkable understanding of societal dynamics, governance, social justice, and leadership values," Moema concluded.

The debates were moderated by Ace Moloi, a former student leader and award-winning journalist, whose experience and understanding of the university’s values greatly contributed to the event’s success.

The UFS is committed to developing well-rounded graduates who can think critically and contribute meaningfully to society. Looking ahead, the UFS hopes to see a high voter turnout on 29 May and continued student involvement in future elections. The debates' focus on critical thinking and informed participation aligns with Vision 130's objective of developing well-rounded graduates who can contribute meaningfully to society.

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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