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14 September 2021 | Story Dr Jan du Plessis and Dr Mampoi Jonas

Opinion article by Dr Jan du Plessis, Head of the Paediatric Oncology Unit, and Dr Mampoi Jonas, senior lecturer in the Paediatric Oncology, University of the Free State 


For many years childhood cancer has remained a taboo subject in our communities, mainly because too little was or is known about it. Many have known or come across an adult with cancer but for a child to be diagnosed with cancer is totally unheard of. No parent wants to hear the news that their ‘heartbeat in human form’ has fallen ill. One moment they are OK, the next, waves of emotions flood the parents. Mixed in all this are feelings of guilt, anxiety, uncertainty, constant wondering if they could have done anything differently. Most importantly the question, often unuttered remains “Is my child dying/ how much time do I have”.

Most young cancer patients live in developing countries

Childhood cancer is rare and involves only 1% of all cancers. It is reported that globally approximately 70% of all childhood cancer cases occur in low- and middle-income countries. If diagnosed early, approximately 70-80% of childhood cancers are curable in developed countries. Unfortunately, most children with cancer live in developing countries with limited resources and the cure rate does not reflect the same success. The low survival rates can be attributed to poor diagnosis coupled with too few specially trained doctors and nurses and the misbelief that child cancer is too difficult to cure. However, even in resource-poor environments at least 50% of childhood cancers can be cured.

Numerically, childhood cancer is not a significant cause of death in sub-Saharan African countries, which leaves childhood cancer less of a priority. In Africa, the most common paediatric health problems are malnutrition, infectious diseases such as HIV and tuberculosis. Whereas in Western countries, after accidents, cancer is the second leading cause of death in children and is a burden to the health system.

A study done by Stones et al in 2014 published the survival rates for children with cancer in South Africa at two different Units (Universitas and Tygerberg Hospitals) to be around 52%. The conclusion was that the children present late and with advanced-stage disease, which obviously affects their outcome. They also concluded that strategies to improve awareness of childhood cancer should be improved. Identifying early warning signs of childhood cancer is critical for parents and healthcare workers to ensure early diagnosis and improved cure rates. We often refer to these as red flag signs that should raise suspicion of the possibility of cancer as a diagnosis for the presenting patient.

Almost 85% of childhood cancers will present with the red flag signs, which could suggest the possibility of a childhood cancer, namely:
1. Pallor and purpura (bruising)
2. Bone and joint pain
3. Lymphadenopathy
4. Unexplained masses on any body part
5. Unexplained neurological signs
6. Changes in the orbit or eye
7. Persistent unexplained fever and weight loss

The most common cancer in children is leukaemia (blood cancer). Brain tumours are the most common non-haematological cancers, followed by nephroblastomas (kidney cancers) and neuroblastomas (sympathetic chain cells, the adrenal glands the most common site of origin).

We honour the children currently battling cancer and their families 

Once there is clinical suspicion of cancer, the child should be investigated or referred for the relevant investigations to be conducted to get to the right diagnosis. Treatment for childhood cancer includes chemotherapy, surgery or radiotherapy. These may be given separately or in combination depending on the diagnosis. Many models of care exist, but regardless of the outcome, children and families who receive compassionate, holistic care of symptomatology and address their non-physical needs are able to face their illness with dignity and energy.  

Childhood Cancer should not remain a taboo subject in South Africa and should be a topic of conversation more often so that people can be educated regarding the early warning signs and become more aware of its occurrence amongst children. Get the word out that a cure is possible. This month, which is known as Childhood Cancer Awareness Month, and throughout the year, we honour the children currently battling cancer, the families who love them, the clinicians and other caregivers treating them, the survivors of childhood cancer and the children who lost their lives to childhood cancer. 

Authors

Dr Jan Du Plessis for web 
Dr Jan du Plessis is the Head of the Paediatric  Oncology Unit in the Faculty of Health Sciences at
the University of the Free State (UFS).  


DrJonas for web
Dr Mampoi Jonas is a senior lecturer in the Paediatric Oncology, University of the Free State (UFS).

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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