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13 December 2024 Photo Supplied
Dr Solomon Chibaya
Dr Solomon Chibaya, lecturer in the Department of Education Management, Policy, and Comparative Education, University of the Free State.

Opinion article by Dr Solomon Chibaya, lecturer in the Department of Education Management, Policy, and Comparative Education, University of the Free State.


Friday 13 December 2024 marks a crucial moment in South African education law. All stakeholders are awaiting the decision regarding implementation of the contentious sections 4 and 5 of the Basic Education Amendment Bill. After President Cyril Ramaphosa signed the Bill into law, he delayed implementation of the sections on language and admission policies for three months. This was meant to allow for consultation on proposals for resolving the conflicts around the contested sections.

The main issue around the language and admission policies is that the Bela Act allows the provincial heads of departments to have the final say on these policies after the school governing bodies (SGBs) have developed them. Some SGBs see this as their powers being usurped, which contradicts the democratisation of school governance. However, cases in which the powers of SGBs have been abused in ways that led to exclusionary language and admission policies presents the need for oversight of these critical school policies.

Friday 13 December 2024 is the deadline for the resolution.

One cannot avoid thinking about the implications of the different possible outcomes of the decision beyond 13 December. The president could approve the Act without any changes, or clauses 4 and 5 could be returned to the National Assembly for reworking.

If approved

If the Act is to be approved with the two contentious clauses in their current form, there will be a barrage of court cases from opponents of the decision. Over the past few months preceding the signing of the Bela Bill and after it was signed on 13 September 2024, the DA, AfriForum and other lobby groups have promised to take the matter to court. In such a scenario, all parties must prepare themselves for long, vicious and contentious court battles that have enormous implications for the political context defined by the Government of National Unity (GNU).

What will add further fuel to the fire is that at the helm of the department in which the Act is being debated is a DA minister, Minister Siviwe Gwarube. Will she toe the line and follow the law as expected by her office? Or will she follow the direction of her political party, which has been clear about how much it abhors the Act, especially in relation to its current form? She could find herself in the firing line.

If approved in its current form, beyond 13 December 2024, the Act will appease proponents who have been clear about their support for it. Proponents of the Bela Act, such as the ANC (which has been campaigning for it to be embraced by all), SADTU (which on countless matches in support of the Act and have even threatened the president with litigation if they do not get their way), and other political parties like the EFF and the MK Party will be vilified. Considering this, the country’s polarisation is apparent and is a potential and real threat to the GNU/coalition.

If sent back

The DA, AfriForum, and other lobby groups, especially those who want clauses 4 and 5 overhauled, will celebrate, but only for a moment. At least they can battle against the Act’s current form in the National Assembly. Rather than the rigour and expenses surrounding litigation, the different sides must now use their different lawmakers to make a case for them.

The results from the last votes on the BELAB held on 16 May 2024 showed that 223 votes were in favour of and 78 votes against the bill. If these results are anything to go by, there is little change the National Assembly would make to the Act. It will boil down to votes, and the scale will be lopsided. We will be heading for litigation and threats.

At the centre of this is the child whose best interest we are supposed to looking out for. Beyond Friday 13 December 2024, our focus will move away from the child to the National Assembly, the courtrooms, the never-say-no law firms. All eyes will be on the political space. 

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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