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01 September 2019 | Story Lacea Loader | Photo Stephen Collett
Chief Justice Mogoeng Mogoeng
From the left: Prof Prakash Naidoo, Vice-Rector: Operations at the UFS; Justice Mogoeng Mogoeng, Chief Justice of the Republic of South Africa; and Prof John Mubangizi, Dean: Faculty of Law at the UFS.

    Watch the full prestige lecture HERE.


“The government of the day should be based on the will of the people and must be led by people who deserve to lead us.” These were the words of Justice Mogoeng Mogoeng, the Chief Justice of the Republic of South Africa, during a prestige lecture delivered in the Faculty of Law on the Bloemfontein Campus of the University of the Free State (UFS) on 30 August 2019.

In addressing the topic of ‘Transformative Constitutionalism’, Chief Justice Mogoeng Mogoeng said this simply meant that the constitution was used as a tool to change or move a family, society, institution or the nation from an unacceptable to a more desirable position. He added that constitutionalism can be enhanced through ethical, courageous, and visionary leadership.

“There is a belief that judges should have nothing to do with matters of politics. I agree, but only to a certain extent. Judges are supposed to deal with political issues, as they interpret the constitution and the law. It is inescapable in a South African context. Some say that judges should only speak through their judgments. I've always said that our constitution is political in nature.”

“The preamble of our Constitution says this country belongs to all who live in it, but to what extent have we allowed our Constitution to achieve these objectives? A constitution does not implement itself. It takes people with a particular mindset and conviction. Transformation demands from the public to ensure that government is truly based on the will of the people,” he said.

According to the Chief Justice, South Africa needs strong and well-resourced institutions – including a strong judiciary. Institutions must be vigilant for any form of abuse of power and capture. Institutions cannot only be captured by external forces. They can be captured internally as well.

Another crucial element is education and the quality and condition of higher education at every level. “Our school system must allow the youth who are coming from high school to be able to adapt with ease when they get to university.”

“We need people who truly love their country to assume positions of power. Transformative constitutionalism is all about giving expression in a practical way. We should look at solutions for our country based on compromise that can bring us together as South Africans.”

He paid tribute to people such as former President Nelson Mandela, Mama Albertina Sisulu, and Adv Bram Fischer, who opted for the greater good of many, rather than personal satisfaction and gain. “South Africa belongs to all – not some – who live in it, united in our diversity. Are you prepared to serve the state? Do you love this nation? Go out there and pursue social justice. Don't buy things from thieves just because they are cheap. You are encouraging crime.”

“We can't continue this way and expect a different outcome. It is not too late; go out there and contribute towards building the South Africa that we can be proud of,” he concluded.

Hosted by Prof John Mubangizi, Dean of the UFS Faculty of Law, the prestige lecture was attended by approximately 800 guests, comprising senior members of the Supreme Court of Appeal, the Free State Division of the High Court, the university’s executive management, the Faculty of Law, staff members, students, and members of the public.

The Prestige Lecture Series was originally known as the Law Deans’ Prestige Lecture Series and was initiated by the late Prof Johan Henning, former Dean of the UFS Faculty of Law. The series started in 2011 as an initiative to encourage, develop, and expand academic discourse on topical jurisprudential issues and other related matters. Previous lectures were delivered by, among others, Prof Barry Rider from the University of Cambridge in the UK; Justice Richard Goldstone, formerly of the Constitutional Court of South Africa; former Deputy Chief Justice Dikgang Moseneke; and more recently, Judge President Dennis Davis.

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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