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01 September 2020 | Story Nonsindiso Qwabe | Photo Supplied
Women
Carol Bouwer and Prof Puleng LenkaBula believe that the nation is constantly diverting to other issues that take the focus away from amplifying voices for the protection of women and children, hence no real change has taken place. Photo: Supplied

The intersectionality between politics, feminism, and social justice was unpacked extensively in the Student Affairs Women’s Month Webinar that took place on 25 August 2020. This was the second in a series initiated by the Qwaqwa Campus Student Affairs. Director of Student Affairs, Nicole Morris, said the webinars were initiated to encourage difficult conversations around womanhood in South Africa.

UFS Vice-Rector Institutional Change, Student Affairs, and Engaged Scholarship, Prof Puleng LenkaBula, and renowned businesswoman and media mogul, Carol Bouwer, were featured in the second instalment. Together they unpacked the dynamics of being a woman in modern-day South Africa in the face of the scourge of violence against women and children, as well as the transformation and greater representation of women in both positions and institutions of power.

 

Challenge the systems

Setting the tone, Prof LenkaBula said society as a collective needed to come together to challenge systems that oppress, mute, silence, and make it impossible for women to become dignified and contribute fully to the society we live in.

 “If we are to promote social justice, feminism, ethics, and gendered analysis, we have to ensure that we constantly challenge, rethink, and think again around issues that we feel are withholding women from being fully themselves.”

 Bouwer and Prof LenkaBula said the nation is constantly diverted to other issues that are shifting the focus from amplifying voices for the protection of women and children, hence no real change has taken place.

 “As someone who began working during the birth of our freedom in 1994, I think back to the elation that we felt at the creation of the constitution. There was so much jubilation about it, but we exported that excitement to the world and talked about what we had attained without practising it here.”

 “We continue to create systems and amazing documents as a nation, yet we do not implement the very things that will lead to a point where discussions such as these do not need to take place,” Bouwer said.

 Bouwer said the COVID-19 pandemic showed that South Africa had the necessary resources to prioritise gender-based violence, but those in power chose not to.

 “As we speak today, gender-based violence has become a national crisis. We talk about the intersectionality between politics, feminism, and social justice against the confluence of the opposite happening. With what happened when the COVID-19 pandemic was declared a national disaster, we’ve realised that we do have the wherewithal to mobilise for action in this nation, and it is the one thing we have not seen our leaders do,” she said.

 

Part-time feminism will not help

Prof LenkaBula said rethinking feminism was needed to move away from definitions of anti-manhood in order to promote feminist ideals that would benefit the nation as a whole.

 “As a feminist, I want to promote the idea that feminists are not promoting the defamation or marginalisation of men or stripping them of their dignity. We are saying that as men and women, no matter our gender or sexuality, we can work together to ensure that we all live with dignity, we all are equal, and we all express our talents, and are able to utilise opportunities that are available to us in fair ways.”

 Alluding to this, Bouwer said she hoped to see part-time feminism done away with in the rebuilding of society after the pandemic. “Coming out of this pandemic, may our feminism be transformed by everything that is currently happening. There is a huge injection of pathos happening right now and I hope that it is not a fad like everything else that has happened in South Africa, but that it becomes something that we really embody as we go back to whatever normal is going to look like,” she said.

 Qwaqwa Campus SRC Secretary General, Nelisiwe Masango, said the Division of Student Affairs planned the Women’s Month Webinars to discuss topics on issues that affect women directly.

 “These programmes are quite insightful and uplifting. They especially encourage young women to see that the revolution is there, it is real, and it is practical. It gives meaning to continue advocating for better and safe spaces for women. Many times, spaces of contestation are male dominated and therefore women have to be empowered to contest these spaces. These engagements must be ongoing or continuous so that we all understand the issues we are affected by and advocate for a better 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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