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18 March 2025 Photo Supplied
Dr Solomon Chibaya
Dr Solomon Chibaya is a lecturer in the Department of Education Management, Policy, and Comparative Education at the University of the Free State (UFS).

Opinion article by Dr Solomon Chibaya, Faculty of Education, University of the Free State.


One of the most humbling intellectual reckonings occurs when reality defies even the most well-reasoned predictions, compelling one to acknowledge misjudgement. Some may call it swallowing the humble pie, but in the realm of law and governance, it serves as a reminder of the unpredictable nature of socio-political dynamics. When the Basic Education Laws Amendment (BELA) Bill was signed into law, I anticipated a legal battleground - a flood of court challenges from those vehemently opposed to its provisions. I was wrong. I also foresaw fractures within the Government of National Unity (GNU), expecting tensions to manifest in visible discord. Wrong again. The fierce contestation promised by opponents of the Bill and the Act has, thus far, amounted to little more than rhetorical smoke without the anticipated fire. The impassioned declarations of legal warfare that once filled public discourse have not translated into the courtroom the battles as I had envisaged. This turn of events is not only fascinating but also challenges broader assumptions about resistance and contestation in contemporary policymaking.

Why have legal challenges not materialised?

To understand the absence of legal challenges against the BELA Act, one must retrace its origins - its conception, development, and the rigorous debates that shaped it. The BELA Bill was first drafted in 2013, following the African National Congress’s (ANC) 2012 elective conference, which mandated amendments to the South African Schools Act (SASA), 84 of 1996. At its core, the Bill was anchored in the transformative principles of the Constitution of South Africa, serving as a legislative instrument to advance equity, inclusivity, and equality in the education system. Given its constitutional foundation, one must ask: who could successfully litigate against a law built on such unassailable pillars of justice and democratic values? The very essence of the Act is woven into the broader framework of South Africa’s post-apartheid transformation, making any legal opposition not just a challenge to policy but a confrontation with the constitutional ideals that underpin the nation’s democracy.

Constitutional imperative for inclusivity

Any legal challenge against the BELA Act, particularly concerning language and admission policies, would ultimately be rendered unconstitutional. The Act is not merely a legislative adjustment; it is a transformative mechanism that promotes linguistic diversity, broadens access to education, and fosters inclusivity in school admissions and employment. These reforms align with the constitutional vision of democratic participation and equitable opportunity, ensuring that mother-tongue instruction evolves alongside a more integrated and representative education system. Who, then, could successfully contest a model that upholds these fundamental democratic values?

At the heart of the Act’s implementation lies a collaborative governance framework, where School Governing Bodies (SGBs) comprising parents, educators, and non-educator staff, work in tandem with the Department of Basic Education at both provincial and national levels to shape policies that best serve their schools. Rather than diminishing the role of SGBs, the Act strengthens their mandate within a broader, constitutionally guided educational ecosystem. Any resistance to this cooperative approach would not only be a defiance of participatory governance but also an attempt to obstruct the very principles upon which South Africa’s democratic and inclusive education system is built.

A masterstroke in legal foresight

A closer examination of the BELA Act reveals a legislative framework meticulously designed to pre-empt legal battles by embedding arbitration and mediation as the primary mechanisms for resolving disputes. In the event of conflicts between SGBs or their representatives, such as FEDSAS, and the Department of Basic Education, the Act prescribes alternative dispute resolution mechanisms, effectively curtailing costly and protracted litigation. Beyond its procedural elegance, the Act reflects a jurisprudential evolution, drawing heavily from precedents set by past court rulings and sealing the loopholes that once rendered the South African Schools Act (SASA) vulnerable to legal contestation. By doing so, the BELA Act assumes the character of case law, informed by judicial scrutiny and legislative refinement.

With such a robust legal foundation, the anticipated flood of litigation against the Act has failed to materialise. Could I have miscalculated again? Highly improbable. In a climate of economic volatility and geopolitical realignment, financial prudence is non-negotiable, and litigation remains an expensive and time-consuming endeavour. Even the most relentless legal advocates must recognise the futility of challenging a law so deeply embedded in the constitutional ethos of the Republic of South Africa (1996). The once-fiery calls for litigation have seemingly dissipated into a quiet acknowledgement of legal inevitability. 

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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