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18 March 2024 | Story VALENTINO NDABA | Photo SUPPLIED
RIGHT TO VOTE 2024
Expert speakers dissecting South Africa's political landscape at the University of the Free State’s recent panel discussion on the 2024 elections.

The University of the Free State's (UFS) Centre for Gender and Africa Studies (CGAS), in collaboration with the South African Institute of Race Relations (IRR), recently organised an Africa Dialogue Series panel discussion titled ‘Elections 2024: South Africa’s Changing Political Landscape’. The event, held on 6 March 2024, brought together distinguished speakers and experts to dissect the evolving dynamics of South Africa's political landscape as the nation gears up for the 2024 elections.

The panel featured prominent figures including former Tony Leon, Makone Maja, Michael Atkins, and Terence Corrigan, who provided valuable insights into various aspects of the upcoming elections. Prof Heidi Hudson, Professor at the CGAS, expertly moderated the session, ensuring a robust exchange of ideas and perspectives.

Importance of informed dialogue

Prof Hussein Solomon, Senior Professor at CGAS and planner of the dialogue session, reflected on the success of the event in achieving its objectives. He emphasised the importance of informed dialogue in navigating the complex issues surrounding the 2024 elections. "The idea is to inform people of the issues at stake, but also to focus on key issue areas from an academic perspective," Prof Solomon said.

He expressed concerns about voter registration and the need for heightened awareness among youth, underscoring the significance of addressing societal challenges to ensure peaceful elections.

Unprecedented uncertainty in election outcome

Leon, former leader of the Democratic Alliance and a seasoned political analyst, opened the discussion by highlighting the unprecedented uncertainty surrounding the outcome of the 2024 elections. Contrary to previous elections where the victory of the African National Congress (ANC) was almost a given, Leon pointed out that the current political landscape presents a different scenario.

"In all the previous elections we were able to predict an ANC win. This time round it is not that simple," he said. "The ANC will not clear 50 and that’s going to be a big game-changer."

Leon underscored the fragmentation within the ANC itself, noting the emergence of multiple versions of the party with no clear ideological distinctions. He also raised concerns about voter turnout and the implications of a potential government controlled by parties representing a mere fraction of the voting population.

Declining youth political participation

Maja, Campaign Manager at the IRR, shed light on the decline in political participation by youth in South Africa. Drawing from statistical data, she emphasised the need to address the disillusionment among young voters, particularly regarding corruption and unemployment.

"I've been particularly curious about youth for their behaviour," she said. "A lot of the youth... did not align with political parties in South Africa, much more likely in the youth than in the older age categories."

Maja highlighted socioeconomic factors that are contributing to youth disengagement from the political process, and stressed the importance of political engagement in shaping democratic outcomes.

Upholding electoral integrity

Atkins, a seasoned political analyst and independent observer in South African elections, focused on the imperative of upholding electoral integrity. He criticised the flaws in the Electoral Amendment Bill and highlighted concerns about the accuracy of election results.

"We have seen a complete disrespect or even disdain for meaningful electoral reform through these last three years," he said. "Spurious claims of rigging must be objectively and speedily met and countered."

He called for increased transparency and accountability within the electoral process to ensure the legitimacy of election outcomes.

Political dynamics and future scenarios

Corrigan, a Project Manager at the IRR, delved into the changing political dynamics of South Africa and contemplated potential future scenarios. He questioned the sustainability of the dominant party paradigm and examined the possibility of coalition politics in the aftermath of the elections. Corrigan highlighted the emergence of new political players and the implications of coalition politics for stability and governance in South Africa.

The Africa Dialogue Series panel discussion provided a platform for robust debate and critical analysis of South Africa's political landscape, offering valuable insights into the challenges and opportunities that lie ahead in the 2024 elections and beyond.

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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