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06 November 2024 | Story Anthony Mthembu | Photo BORN2SHOOT
inaugural Albie Sachs Prestige Lecture 2024
From the left (back row): Dean of the Faculty of Law, Prof Serges Kamga; Judge of the Supreme Court of Appeal, Justice Nolwazi Mabindla-Boqwana; Deputy Vice-Chancellor: Research and Internationalisation at the University of the Free State (UFS), Prof Vasu Reddy; Project Director of the Albie Collection and Chair of the Albie Sachs Trust (ASCAROL), Vanessa September; and acting Deputy Vice-Chancellor: Academic at the University of the Free State (UFS), Prof Philippe Burger. From the left (front row): Acting Vice-Chancellor of the University of the Free State (UFS), Prof Anthea Rhoda; Emeritus Constitutional Court Justice Albie Sachs; and Chief Justice of South Africa, Mandisa Maya.

The Faculty of Law at the University of the Free State (UFS) hosted the inaugural Albie Sachs Prestige Lecture on the UFS Bloemfontein Campus on 30 October 2024. The lecture – delivered by Emeritus Constitutional Court Justice Albie Sachs – was titled, ‘Who actually wrote the Constitution, and why they gave eleven unelected judges the power to strike down laws and actions of the democratically chosen parliament and president’?

In attendance at the lecture were Chief Justice of South Africa, Mandisa Maya; acting Vice-Chancellor of the UFS, Prof Anthea Rhoda; Judge of the Supreme Court of Appeal, Justice Nolwazi Mabindla-Boqwana; Senior State Advocate, Antoinette Ferreira; Project Director of the Albie Collection and Chair of the Albie Sachs Trust for Constitutionalism and the Rule of Law (ASCAROL), Vanessa September; as well as the Dean of the Faculty of Law, Prof Serges Kamga, among other high-profile guests.

In his opening address, Prof Kamga indicated that the lecture aimed to provide some responses to the core questions about the constitution and constitutionalism in South Africa. As such, Prof Rhoda echoed this sentiment, highlighting that, “when it comes to the events that preceded, surrounded, and followed the drafting and adoption of our country’s constitution, there are few commentators better placed than Judge Albie Sachs”.

The making of the constitution

As part of his lecture, Justice Sachs gave a detailed account of the making of the South African constitution. According to Justice Sachs, a total of 490 members of parliament came together to draft the constitution, which included members of the National Assembly and the Senate. These members had been mandated by 20 million South Africans who wanted a better future. As such, he described that moment as a “huge accomplishment on the part of the liberation movement”.

However, he highlighted that fulfilling this mandate was not an easy task, as it required an enormous amount of thought and mobilisation of legal technology to enable those in power at the time to surrender control of the army, police, and to some extent the economy and law-making, among other aspects. These negotiations resulted in a two-state process of constitution-making, which included the drafting of an interim constitution and the establishment of a parliament that would draft the final constitution.

Justice Sachs indicated that once the constitutional assembly sent the constitutional text to the constitutional court to ensure its compliance with agreed principles, it was found non-compliant in eleven respects, for which they had to find solutions in order for the constitution to be adopted.

As he concluded his address, Justice Sachs underscored his pride in having been involved in what he describes as a wonderfully rich story.

Forging a partnership

Subsequent to the address by Justice Sachs, the Faculty of Law and ASCAROL signed a Memorandum of Understanding (MoU), formalising the Albie Sachs Prestige Lecture as an annual event and allowing further collaboration. In fact, Prof Kamga highlighted that if Justice Sachs was not available to deliver a lecture, the trust would appoint someone in his place. To further solidify this partnership, the faculty was gifted with some of Justice Sachs’ works, including books and other materials, for its library.

Prof Rhoda expressed gratitude for this collaborative effort, saying, “We are grateful to have found such a partner in Justice Albie Sachs and the Albie Sachs Trust. May this relationship continue to blossom and bear fruit – to the benefit of our young leaders of tomorrow.”

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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