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26 April 2019 | Story Opinion article by Dr Chitja Twala | Photo Sonia Small
Dr Chitja Twala
Dr Chitja Twala is the Vice-Dean of the Faculty of the Humanities at the University of the Free State.

This opinion piece is to reflect on the sacrifices and roles played by the Twelve Disciples in the Liberation Struggle in honour of #Freedom Day.

To the majority of South Africans, the struggle for liberation centres around high-profiled political leaders such as Nelson Mandela, Walter Sisulu, Govan Mbeki, Robert Sobukwe, Steve Biko, and others. Less known is the experience of a generation of young men who left South Africa clandestinely to build the ANC and spread its liberation message in places abroad. These young men became known as the Twelve Disciples of Mandela. Like many other youngsters who became political activists elsewhere in the country, this group received its political conscientisation at school at the then Bantu High School (later known as Sehunelo High School).

This group of youngsters came from the Mangaung township in Bloemfontein, although it is not clear why they were referred to as the Twelve Disciples of Mandela. When they left Bloemfontein, they were destined to join MK in exile. The formation of MK was announced on 16 December 1961. At the same time, MK began a sabotage campaign against strategic installations throughout South Africa. In a leaflet issued on 16 December 1961, the MK high command made its political allegiance quite clear by stating: “Umkhonto we Sizwe will carry on the struggle for freedom and democracy by methods which are necessary to complement the actions of the established national liberation organisations. Umkhonto we Sizwe fully supports the national liberation movement and calls on members, jointly and individually, to place themselves under the overall political guidance of the movement”. During the initial stages of its formation, MK avoided openly mentioning the ANC for tactical reasons. MK sought to protect the leadership of the ANC from reprisals by the South African government, in particular those who had nothing to do with the decision to take the route of armed struggle.

It is clear from interviews conducted with the surviving members of this group that nobody knew exactly why they were called the Twelve Disciples, except that there was a plan conceived by Mandela, called the M-Plan, calling for the total restructuring of the ANC to enable it to operate underground should it get banned. However, although several authors such as Edward Feit, Karis and Carter, Nelson Mandela, and Bruno Mtolo and a number of court records provide information on the M-Plan, details are sketchy.

The group of young men from Bloemfontein were Billy ‘Marakas’ Mokhonoana (left the country earlier than the others and allegedly died in London); Selebano ‘Tlhaps’ Matlhape (left for Tanganyika and later studied in Yugoslavia and East Germany); Theodore ‘Max’ Motobi (left for Tanganyika and underwent military training in Cuba); Moses ‘Dups’ Modupe (left for Tanganyika and later studied Economics in Yugoslavia); Benjamin ‘Lee’ Leinaeng (left for Tanganyika and later studied journalism in East Germany); Joseph Shuping ‘Coaps’ Coapoge (left for Tanganyika and later attended Lincoln and Temple Universities in the US); Elias Pule Matjoa (worked in the Ministry of Communications in Tanzania and underwent military training in Cuba. He later studied dentistry there); Percy Mokonopi (received military training in Cuba and later served on the Helsinki World Peace Council); Mochubela ‘Wesi’ Seekoie (left for Tanganyika and underwent military training in Cuba. He later studied Chemistry in the USSR); Matthew Olehile ‘Beans’ Mokgele (left for Tanganyika and became a professional boxer in exile. Following an injury, he went to East Africa and joined the MK); Bethuel Setai (left for Tanganyika and later obtained a PhD in Economics from Colombia University. He taught at the University of California Santa Cruz, and Lincoln University in the USA) ; and Peter Swartz (was an active member of the ANC from the coloured community in Bloemfontein. He met with the group in Dar es Salaam, following his arrest on his way to Tanzania. He attended Kivukoni College and later went to the UK where he attended the London School of Economics. He went missing in London in 1965, never to be seen again).

In honour of many of these unsung heroes, the history of the Twelve Disciples needs to be told to reflect what one could refer to as a ‘bottom up’ kind of history. Without doubt, this kind of history will add value to the country’s historiography about the liberation struggle and demystify the one-sided narrative that the (Orange) Free State played little if no role at all in the struggle for liberation.



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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