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31 August 2020 | Story Dr Chitja Twala
R Chitja Twala
Dr Chitja Twala is the Vice Dean in the Faculty of The Humanities.

In the 1940s, the then (Orange) Free State produced a crop of female leaders whose role in the liberation struggle is unknown – or rather, for whatever reason – ‘neglected’. Among these leaders was one Moipone Martha Motlhakwana. Testimony to the above was an article published by the Mail and Guardian on 25 August 2016 under the heading 60 Iconic Women – The people behind the 1956 Women’s March to Pretoria. In this article, only four lines are dedicated to her, contrary to what has been written about other leaders, such as Lilian Ngoyi, Lizzy Abrahams, Lucy Mvubelo, and many others. This is an indication of the possible ‘neglect’ in highlighting the role played by other women in places such as the Free State. In this article, I argue that Motlhakwana’s role in the liberation struggle was by no means minimal, compared to the leaders mentioned above. 

When one evaluates her role and contribution to the struggle, it is important to always keep in mind the context of the time and the scope of possibilities that were available to the liberation movements. This article briefly examines her role at a crucial time when Motlhakwana’s beloved movement, the African National Congress (ANC), is experiencing its most difficult and trying times since coming to power in 1994.

The Defiance Campaign

Motlhakwana was born into the Makabane family in Leqwala in the Thaba Nchu district on 23 December 1906. She was a devoted Christian. Being a Christian did not prevent her from participating fully in politics. Long before the 1956 anti-pass march, Motlhakwana was instrumental in organising the 1952 Defiance Campaign in Bloemfontein. Meetings for organising this campaign were held in an open space where the Paradise Hall in Bochabela Location in Bloemfontein is situated today. She led a women’s support group demanding the release of those arrested and jailed in the Ramkraal Prison in Bloemfontein. It became known to the Special Branch that her house was, at the time, used as the ANCWL’s ‘headquarters’ in town; therefore, the house was monitored and kept under police surveillance.

Motlhakwana also participated in the 1956 anti-mass march to Pretoria. In the Bloemfontein area, she mobilised people in the burning of passes. Her fearless organising strategies earned her a nickname in the community as Motabola Pasa or Mochesa Pasa (the one instrumental in tearing of the dompas or the one burning the passes). She was among the people who were arrested and detained during the Treason Trial. After being acquitted, she was placed under house arrest. Together with her friend in the struggle, Pretty Molatole, they were involved in establishing the ANCWL in Bloemfontein. Most of the league’s meetings were held at Motlhakwana’s place. She used to travel around the province to establish ANCWL branches in places such as Bethlehem, Ficksburg, and Thaba Nchu, to name a few. It was during this period in the mid-1950s that she worked closely with the leaders of the ANC in Bloemfontein, such as Jacob B Mafora, Caleb Motshabi, and Leslie Monnenyane.

In her honour

In honour of her contribution to the liberation struggle in South Africa and not only in the Free State, a tombstone was unveiled at the Phahameng Cemetery, adjacent to the Heroes’ Acre, on Thursday 5 January 2012; this unveiling coincided with the centenary celebrations of the ANC as the oldest liberation movement in Africa. Addressing the masses during the unveiling of the tombstone, the Chairperson of the ANCWL in the Free State and the current Premier, Sisi Ntombela, stated: “Most people have the concept that the anti-pass march started in Johannesburg in 1956, but that is not the case because the first march was started in the province by women such as Motlhakwana and Mei Likotsi and others who were leaders at the time, and mobilised the women for the march. As we unveiled the Motlhakwana tombstone, we also discovered that her grandchildren have kept the passes of those women whom she organised at that time. She made sure that women were developed, not only in politics but also in trade unionism. The Free State is the centre where everything started; this year [2012] is the ANC Centenary, but next year we will be holding the ANCWL Centenary for the Free State women.”

Owing to illness, Motlhakwana passed away on Thursday 27 July 1989. She was buried in the Phahameng ‘Magengenene’ Cemetery in Bloemfontein, not far from the Heroes’ Acre.

There are many women of Motlhakwana’s political stature in the Free State, whose histories should be documented in the form of biographies.

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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