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07 June 2022 | Story Prof Felicity Burt, Prof Dominique Goedhals and Dr Charles Kotzé
Prof Felicity Burt, Dr Charles Kotze and Prof Dominique Goedhals
From the left; Prof Felicity Burt, Dr Charles Kotzé and Prof Dominique Goedhals.

Opinion article by Prof Felicity Burt , Prof Dominique Goedhals , Division of Virology at the University of the Free State (UFS), and Dr Charles Kotzé, National Health Laboratory Service (NHLS), Universitas Academic Hospital.
The recent COVID-19 pandemic has certainly highlighted the importance of vigilance and awareness of emerging diseases with public health implications. The monkeypox virus has recently made headlines, after the detection of more than 200 cases in geographically distinct regions. On 13 May, the World Health Organisation (WHO) was notified of human cases of the monkeypox disease occurring in the United Kingdom, outside of the known endemic region.

Exported cases have been detected previously and usually occur sporadically. In contrast, within the past two weeks, human cases have been confirmed in at least 21 countries, including various European countries, the United Kingdom, Israel, the Canary Islands, Canada and the United States, and Australia. The initial case appears to have been a traveller from Nigeria. Sequence data may help to determine if there have been multiple exportations from West Africa. 

What is monkeypox and what do we know

What is monkeypox and what do we know about the aetiologic agent? Monkeypox is the name given to a disease caused by the monkeypox virus, a zoonotic pathogen endemic in Central and West Africa and responsible for cases of the disease in the endemic region, with occasional exported cases in travellers. The virus was initially identified in 1958 in monkeys housed at a research laboratory in Denmark, and the name monkeypox was derived from the appearance of lesions and the occurrence in monkeys. The first human case was identified 52 years ago in the Democratic Republic of the Congo. Since then, human monkeypox cases have been reported in several other Central and West African countries: Cameroon, the Central African Republic, Ivory Coast, the Democratic Republic of the Congo, Gabon, Liberia, Nigeria, Republic of the Congo, and Sierra Leone. The first monkeypox outbreak outside of Africa was in the United States of America in 2003 and was linked to contact with infected prairie dogs imported as exotic pets. Since then, there have been various small, contained outbreaks outside of Africa that have mostly been linked to the importation of the virus from African countries. 

The virus is related to the smallpox virus, which was eradicated in the 1970s by vaccination. Although belonging to the same family of viruses as the smallpox virus, the disease caused by monkeypox is less severe, with fewer fatalities.   Unlike smallpox, which carries a case fatality rate of 30%, the case fatality rate in monkeypox is low (estimated at 3-6% in more recent outbreaks).  There are two clades of the monkeypox virus: the West African clade and the Congo Basin (Central African) clade. In this outbreak, all of the cases have been linked to the West African clade of the monkeypox virus.

Transmission occurs from animal to human, and from human to human, through close contact with lesions, body fluids, and contaminated materials. The virus enters the body through the respiratory tract, mucous membranes, or broken skin.  The disease begins with non-specific symptoms such as fever, headache, muscle pains, and swollen lymph nodes. This is followed by the typical skin rash, which progresses through stages known as macules, then papules, vesicles, pustules, and lastly crusts or scabs. Lesions can also occur on mucous membranes such as the mouth, eye, and genital area.  The infectious period lasts through all stages of the rash, until all the scabs have fallen off. There are a number of other infectious and non-infectious conditions that need to be differentiated; therefore, individuals presenting with these symptoms will need to consult their doctor to determine whether a diagnosis of monkeypox needs to be considered. In the current outbreak, a number of the cases in the United Kingdom and Europe have been detected in men who have sex with men, during visits to sexual health clinics. This pattern of spread has not previously been described and it remains to be determined whether the spread has occurred through close person-to-person contact or through sexual transmission.  

Vaccination against smallpox virus offers 85% protection against monkeypox

To date, no cases have been detected in South Africa, but the recent global spread of the severe acute respiratory syndrome coronavirus 2 (SARS_CoV-2) highlights the ability of pathogens to spread. The National Institute for Communicable Diseases (NICD) in Johannesburg offers a specialised diagnostic service for the monkeypox virus, using molecular assays and electron microscopy. 

Vaccination against the smallpox virus is believed to offer 85% protection against monkeypox, hence older persons should have some protection; however, vaccination against smallpox was phased out globally following the eradication of smallpox during the 1970s. A more recently developed vaccine against monkeypox is available but has very limited availability.  No specific antivirals are available with proven efficacy in clinical trials.

While the monkeypox virus can be spread via the respiratory route, this occurs in the form of large droplets, rather than aerosol transmission, which is seen with SARS-CoV-2 (causing COVID-19). Aerosols are smaller particles that can remain suspended in the air for prolonged periods, facilitating the transmission of SARS-CoV-2. Monkeypox is therefore less contagious than COVID-19, as close contact is required for longer periods.  For this reason, many experts around the world predict that this outbreak will not spread like SARS-CoV-2. The importation of monkeypox to South Africa is a definite possibility, because South Africa is a significant economic and travel hub for Africa. Previous outbreaks of monkeypox in non-endemic areas have been interrupted by contact tracing and isolation, which was very effective in controlling further spread.  Heightened vigilance is therefore needed for the early detection of such cases.

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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