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29 February 2024 | Story VALENTINO NDABA | Photo Stephen Collett
Prof Bradley
Prof Bradley Smith tackles the ambiguities surrounding trust misuse during divorce proceedings.

In his inaugural lecture on 21 February 2024 at the University of the Free State (UFS), Prof Bradley Smith explored the complexities of trust misuse in the context of property disputes during divorce proceedings. Prof Smith is an Extraordinary Professor at the UFS Faculty of Law. Drawing on two decades of judicial evolution in the Supreme Court of Appeal (SCA), Prof Smith highlighted the inconsistencies in the SCA’s treatment of this issue that impedes attempts to curb “divorce planning” by way of a trust and proposed solutions to address them.

One of the core issues he identified is the abuse of trusts, where assets are placed within a family trust to diminish a spouse’s personal estate value while treating the trust property as personal property for personal gain. This is often done in an attempt to evade the financial consequences of divorce. Prof Smith explained that this practice undermines the essence of trust law and that the inconsistent approaches by our courts exacerbate the challenges in dividing property during divorce proceedings in a manner that respects the spouses’ matrimonial property regime.

Navigating challenges: reflections on research and its importance

Prof Smith’s proposal revolves around the development of a consolidated test for piercing the veneer of an abused trust, aiming to enhance legal certainty. He emphasised the necessity of a unified approach. “Utilising this test will ensure uniformity because of its applicability to all marriages out of community of property, irrespective of whether the accrual system is involved,” he said.

His meticulous examination of conflicting judgments was praised by Dr Brand Claassen, head of the Department of Private Law, who described it as “the work of a master craftsman”. Retired Judge of Appeal, Eric Leach, also highlighted its critical importance in clarifying complex legal issues for the public good.

“It is of critical importance and in the public interest for judicial decisions, particularly those of higher courts such as the Supreme Court of Appeal and Constitutional Court, to be subjected to careful and considered analysis and, if needs be, criticism. Prof Smith’s inaugural lecture on combating trust form abuse in the context of matrimonial property claims at divorce, in which he carefully considered and analysed the conflict between several Supreme Court of Appeal judgments, was a valuable and important study on the issue,” said Judge Leach. He added that he hoped Prof Smith’s research would be considered by the SCA in future.

Future directions: advancing discourse and sound legal theory

Looking ahead, Prof Smith envisions further research into the applicability of the consolidated test to marriages in community of property, aiming to address remaining uncertainties that lie at the intersection of matrimonial property and trust law. He emphasised the importance of countering the prevailing “catch-me-if-you-can” attitude in divorce matters, advocating for proactive measures to uphold fairness and justice in matrimonial property disputes.

In conclusion, Prof Smith’s inaugural lecture provided valuable insights into combating trust form abuse within the context of matrimonial property claims at divorce. His proposed solutions and ongoing research efforts signify a commitment to advancing discourse on trust law theory and practice, with the ultimate aim of a sound judicial approach that serves the needs of South African society.

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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