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30 October 2020 | Story Leonie Bolleurs | Photo Supplied
ARU Researchers on mountain slope
A team of international researchers discovered in March 2020 a new grass species, Festuca drakensbergensis, during extensive fieldwork in the 40 000 km2 Maloti-Drakensberg area.

In their search to learn more about the impact of humans and climate change on grasses in the Drakensberg Mountain Centre (DMC), one of the most studied mountain systems in the region, a group of scientists found a new grass species, which they named Festuca drakensbergensis (common name unknown; herein could be designated the ‘Drakensberg Alpine Fescue’).

The team who is working on the project includes Dr Vincent R. Clark, Head of the Afromontane Research Unit at the University of the Free State (UFS), Prof Steven P. Sylvester from the Nanjing Forestry University in Nanjing, Jiangsu, China, and Dr Robert J. Soreng, working in the Department of Botany at the Smithsonian Institution in Washington DC.

 

The discovery

The species, that was discovered in March 2020, was found during extensive fieldwork and herbarium research across the 40 000 km2 Maloti-Drakensberg area. The DMC has a very high endemic plant diversity, says Dr Clark.

He goes on to say that the DMC has a Montane Sub-Centre (below 2800 m) and an alpine sub-centre (above 2800 m). “It is the only mountain system in Africa south of Mt Kilimanjaro with an alpine component,” he adds.

ProfSylvester says the species was easily recognisable during their fieldwork, being found fairly common throughout the Afro-alpine landscape. Although at that point they only knew it to be a distinct taxon, they realised that the species was new to science when they tried to identify it and compared it with other closely related Festuca taxa.

Besides this discovery, the team also reinstated two varieties of Festuca caprina and rediscovered the overlooked F. exaristata, all of them endemic to the DMC. Prof Sylvester believes that this discovery highlights the importance of these high-elevation ecosystems as harbours of unique biodiversity that require focused conservation efforts.

Although grasses are a dominant species that control the ecosystem function in the Afro-alpine grasslands, they are the least known of all plant species found in these ecosystems. Up until now there has been a lack of focused research on Afro-alpine grasses.

 “We provide a taxonomic reappraisal of the Festuca caprina complex that will aid future ecological and biogeographical research in the DMC and allow us to better understand the complexities of these ecosystems and how to conserve and manage them,” says Prof Sylvester.

 

This discovery highlights the importance of these high-elevation ecosystems as harbours of unique biodiversity that require focused conservation efforts. - Prof Steven Sylvester

 

 

Adding value

According to Dr Clark, the species contributes to the grazing and rangeland value of the Maloti-Drakensberg. “It also has functional value in terms of maintaining ecosystem integrity and associated water production landscape value in the area,” he says.

“The species seems fairly robust to pressures from grazing and burning, being found in both heavily grazed areas and semi-pristine areas, and may prove a useful species as part of a seed mix of native grasses for reseeding degraded Afro-alpine slopes and ski slopes,” mentions Prof Sylvester regarding the benefits of this indigenous species to the region.

The species is very common in Lesotho in Bokong Nature Reserve, Sehlabathebe National Park, and Sani Pass, and at Tiffendell and AfriSki ski resorts. Dr Soreng believes the species is likely to have a wider distribution range across the Maloti-Drakensberg, than what was documented before research was cut short due to the COVID-19 pandemic.

 

Next steps

According to Prof Sylvester, this taxonomic research feeds into a large-scale ecological study looking at the response of Afro-alpine ecosystems to different grazing and burning regimes that is being run in collaboration with Dr Clark at the ARU and Dr Soreng of the Smithsonian Institute, Washington DC.

“While our research has uncovered interesting novelties and provided a greater understanding of the taxonomy of grasses from high elevation Maloti-Drakensberg, there is still much to be done with regards taxonomic research of cool-season grasses in southern Africa,” says Prof Sylvester.

Dr Clark supports this notion and states that there is a major need for a better holistic understanding of the alpine zone in the Maloti-Drakensberg, given immediate pressures from over-grazing, land-use transformation, invasive species, and climate change.

“This is because the Maloti-Drakensberg is the most important water tower in southern Africa, providing water for some 30 million people in three countries. As the Maloti-Drakensberg is dominated by natural grasslands, understanding grass diversity and ecological behaviour is a primary need in the face of immediate human impacts and global change,” he says.

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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