Vampire bat: not so deadly (credit: Stephen Dalton/Minden/Getty)
A group of Peruvians thought to have survived untreated rabies infection have bucked the notion that the virus is universally lethal to humans.
A team led by of the US Centers for Disease Control and Prevention, in collaboration with the Peruvian Ministry of Health, travelled to two communities in a remote part of the Peruvian Amazon. Outbreaks of rabies infection caused by bites from vampire bats over the past couple of decades.
When the team sampled the blood of 63 people from these communities they found that seven of them had “rabies virus neutralising antibodies”. One of these people had had the rabies vaccine before but the other six had not, though they reported having been bitten by bats in the past.
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The antibodies are produced when the body is directly exposed to rabies or exposed to a vaccine for the virus. Gilbert and her colleagues concluded that the six unvaccinated people with the antibodies must have been exposed to rabies without dying from it, suggesting they have a natural immunity.
However, the researchers admit that they don’t know whether these people actually developed an infection or were exposed to a small dose of the virus which they were able to fight off. “Despite the fact that we find antibodies, these people are still considered at risk,” says Gilbert. The level of antibodies required to protect someone is unknown, she says.
If further studies confirm that there are populations of people with a greater natural immunity to rabies, they could pave the way for new treatments.
Past fighters
Even if these six patients did manage to fight off the infection themselves, it might not be the first time that natural resistance to rabies has appeared.
When a person suspects they might have been infected with rabies they are advised to seek immediate treatment in the form of a series of vaccines. If they do this within a few days, before exposure causes an active infection, they almost always survive. But they must receive the treatment before symptoms start to show.
A treatment known as the Milwaukee protocol – where unvaccinated people are sent into a drug-induced coma to buy time to fight off the infection – appears to have worked on at least six patients. But it has been tried on at least 35, so it is not clear whether the survivors owe their lives to the Milwaukee protocol or their own immune system’s ability to fight off what could have been a weak strain of the virus.
Journal reference: , DOI: 10.4269/ajtmh.2012.11-0689
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


