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15 December 2021 | Story Nondsindiso Qwabe | Photo Supplied
Bachelor of Education third-year student, Moeketsi ‘Escalator’ Ngesemane.

By day he is a third-year Bachelor of Education student on the Qwaqwa Campus, but this young man is a Sesotho music maestro with a deep-rooted passion for traditional music and a diligent devotion to unearthing new talent and connecting more people to the cultural artistry that Sesotho music has to offer.

Moeketsi Ngesemane, better known as ‘Escalator’ in the world of music, is only 22 years old, but he has already released one solo album and featured in two more, leads a group of more than 80 traditional singers and dancers, and is responsible for a string of groups around Qwaqwa. He has made strides far beyond his age, and Ngesemane says he is only getting started. He was also instrumental in coordinating the Qwaqwa traditional groups that performed during this year’s Multilingual Mokete festival, where he also featured.

Born and bred in Qwaqwa, Ngesemane pins his love for traditional music as something that was cultivated in his childhood while singing traditional songs with his mother and brother. “My mother is a traditional healer, so Sesotho music was a big part of my upbringing. As I grew older, my brother and I would perform in town and people would give us money. I have not looked back since.”

He cemented himself as an artist and artist manager in his first year in 2009. The name ‘Escalator’ came about in an uncanny way, as he fondly recalls. “I had a friend who was afraid of escalators when he first saw it – but I wasn’t, so he named me ‘Escalator’. I hated the name until I personalised the meaning behind it. It is able to take people from one point to another and from one level to another, which is something I am passionate about doing through traditional music, so the name was fitting.”

He captivated the minds and hearts of both young and old people who want to be under his leadership, and he grooms young people as young as ten, who will also thrive and take traditional praise singing and dancing to greater heights. This, he says, helps him alleviate some responsibilities so that he can focus on his schoolwork.

Celebrating the Sesotho culture through music

Word about his music skill often spreads quickly. “Even when I am on teaching practicals at different schools, once learners find out what I do, they ask to join my group and I can’t say no. Their ages range from 7 to 21, and I know that my group will have more than 100 members before the year ends,” he said.

He often puts together music shows with his group around Qwaqwa. This, he says, he does to promote Sesotho music and art.

Ngesemane has been selected to represent the Basotho Kingdom at the Indoni Mr and Miss Cultural South Africa – an indigenous event focused on promoting South Africa’s diverse cultural heritage, taking place at the Durban ICC on 17 December. He describes this as a dream come true.

“It’s a great honour to be representing the Basotho culture. I have discovered that young people, especially, have neglected their cultural roots and often look down on traditional music and regalia. I’ve made it my personal aim to promote and uphold the Sesotho culture through praise singing and dancing.”

You can vote for Ngesemane by SMS’ing ‘Indoni Mr Sotho’ to 33616.

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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