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22 February 2018 Photo Sonia Small
Histories of whites beyond whiteness the focus of inaugural lecture
Prof Hendri Kroukamp, Acting Vice-Rector, Academic, Prof Neil Roos, Professor in the Centre for Africa Studies, and Prof Heidi Hudson, Acting Dean: Faculty of The Humanities.

Growing up in a small milling village on the Natal South Coast sugar belt from the mid-1960s to the early 1980s, Prof Neil Roos was exposed to poverty, privilege, liberalism, and racism. He carved out a promising academic career at the University of Natal, initially on white communists and the anomaly they represented in South African society - researching their histories in the Springbok Legion, a radical wartime kind of ‘trade union’ for soldiers.

During his doctoral work with the University of the North-West, he shifted his attention from the small number of whites who defied segregation and apartheid, to the large numbers who did not, and he began to engage with historical and comparative approaches to race. He was also interested in the sense of comradeship shown by white war veterans in the village where he lived, which included his own father, and used this interest to investigate the kinds of networks white veterans developed, as well as their role in movements like the war veterans’ Torch Commando and the Memorable Order of Tin Hats (MOTH). He used this history to show how white people were able simultaneously to ’oppose’ apartheid, yet accept its core premise of racial supremacy.

Possibility, dismay, and challenge

During his inaugural lecture on 14 February 2018 at the University of the Free State (UFS), Prof Roos addressed issues that delivered new insights under his fresh and rigorous research approach. “I intended to plot how histories of whites in South Africa have been written during several big historiographic moves, with sub-titles ‘possibility’, ‘dismay’ and ‘challenge’.” In the first section, ‘possibility’, he dealt with the vibrant 1980s-vintage South African social history, arguing that social histories of whites were at looked in a rather simplistic way. In ‘dismay’ he looked at the rise of cultural studies of whites in the new millennium which, he argued, tend to be self-absorbed, ahistorical and outside of any rigorous critique of society as a whole. In ‘challenge’ he proposed that contemporary political concerns, notably demands of the decolonisation movement, should inspire a new, activist, anti-racist history of race which draws on some of the strengths of the earlier social history movement as well as some of the techniques developed during the 1990s and the millennium to understand power, ideology and representation.

A new approach

Prof Roos proposes that histories of whites must more properly be histories of race. “This history must show the production of racial categories, reflect on the moral historiographies of being white, and the kinds of dehumanisation this demanded. It must also identify how and where whites transgressed, defied, opposed, or were simply docile. It must be emphatically anti-racist, and must absolutely avoid the possibility of apologia, of trying to gloss over or present with a human face histories of whites under colonialism, segregation and apartheid.” He also argued for an historical approach to present-day iterations of racial identity occurrences of racism, racial supremacy and racial violence.

“I intended to plot how histories of whites
in South Africa have been written during
several big historiographic moves.”

In arguing for the democratisation of studies about whites, Prof Roos argued that it is inconceivable that only whites write about histories of whites. He pointed out that black scholars bring fresh insights to the study of race, and of whites, and appealed for funding to be made available to black scholars pursuing these angles.  

Prof Roos, who is the author of Ordinary Springboks: White Servicemen and Social Justice in South Africa, 1939-1961, has held fellowships at the University of Chicago, the University of Technology Sydney, Harvard and Notre Dame. He is a professor in the International Studies Group and co-directs the Prestige Scholars’ Programme. He is the author of Whites in Apartheid Society, due for publication by Indiana University Press in 2018.

 

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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