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30 January 2025 | Story Jacky Tshokwe | Photo Supplied
Samantha Durrant
Samantha Durrant, the first violinist and Artistic Leader of the Odeion String Quartet, appointed since May 2024.

In the world of music, certain instruments resonate not just with sound, but with profound emotion and history. For Samantha Durrant, her journey with the violin began at the tender age of seven, inspired by the heartfelt story of Music of the Heart. This film, coupled with her exposure to the harmonious symphonies of the KwaZulu-Natal Philharmonic Orchestra, planted seeds that grew into a lifelong devotion to the violin and classical music.

Now, as part of the Odeion String Quartet – the only quartet in residence at a South African university – Durrant stands at the forefront of a mission that transcends performance. She sees her role not only as a performer, but as a steward of South Africa’s string-playing legacy. Her vision is bold yet grounded: to make the Odeion String Quartet the centrepiece of string training and performance in the country.

Reflecting on her journey, Durrant emphasises the critical role of mentorship, exposure, and perseverance. "There wasn’t one pivotal moment in my career," she shares. "It was the culmination of experiences with colleagues, mentors, and friends, all encouraging me to push my boundaries."

The Odeion String Quartet is bridging South African talent with global excellence, performing works by masters such as Haydn and Beethoven while celebrating contemporary compositions, including those from South Africa's rich tapestry of composers. For Durrant, the opportunity to collaborate with living composers is an unparalleled gift, offering insights into their inspirations and musical intentions.

Education and community are at the heart of the quartet's mission. Through school concerts, youth orchestra engagements, and performances at prestigious events such as the Vice-Chancellor’s Concert and the Rector’s Farewell, the quartet inspires audiences of all ages. "Youth orchestras represent unity," Durrant notes. "They bring people together, showcasing our shared humanity."

To those stepping into the challenging world of music, Durrant offers sage advice: "Be patient with yourself. Understand that this field is not easy, but the journey of self-discovery it offers is unparalleled."

With a packed performance calendar and ambitious goals for the quartet’s future, Durrant remains hopeful about music's place in society. "Music has the power to heal, inspire, and unite," she says. "In these challenging times, it is balm for the soul – an essential part of our humanity."

As the Odeion String Quartet continues its journey, its melodies remind us of the transformative power of music, resonating with hope and possibility across generations.

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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