A handheld nuclear magnetic resonance (NMR) scanner that can diagnose diseases and identify pathogens has been built by scientists in the US.
The revolutionary scanner is many times smaller than conventional NMR spectroscopy machines, which require huge magnets to create the powerful magnetic fields necessary to make them work.
Nuclear magnetic resonance spectroscopy works by lining up nuclei in a sample using a powerful magnetic field and then zapping them with radio waves that cause them to wobble, or precess.
This precession induces currents in a nearby coil which can be used to determine the chemical structure of the molecules that contain the nuclei. The same process is used in magnetic resonance imaging machines to make non-invasive images of human bodies. The new device does not produce images, however.
Advertisement
Weaker fields
In conventional NMR spectroscopy machines, powerful fields are necessary to line up individual nuclei.
However, at Harvard Medical School in Cambridge, Massachusetts, US, and colleagues have found that magnetic nanoparticles generate a much larger signal than single nuclei, and can thus be detected using the weaker fields from small permanent magnets.
The trick that Weissleder and colleagues have perfected is to coat these nanoparticles with molecules that bind to specific biomolecules, or bacteria and viruses.
This binding process causes the nanoparticles to clump together, producing a measurable change in the signal they produce. In this way, the team says it can identify a large variety of biological targets.
The team has squeezed the electronics that detect and interpret the signals onto a chip (pdf format).
Small and sensitive
What’s more, the researchers have also designed a microfluidics network that shuttles the samples around and concentrates them in volumes of just five millionths of a litre (5 microlitres) – some 60 times less than conventional systems.
“The smaller the system, the better the sensitivity in terms of absolute amount of sample that can be detected,” says Hakho Lee, lead author on the research.
The prototype device has eight tiny coils, each of which can monitor nanoparticles sensitive to different biomolecules. Future devices could employ many more such coils.
The result is a prototype machine that is 800 times more sensitive than standard NMR scanners used in many laboratories, says Weissleder.
The team put the prototype through its paces, showing that it is sensitive enough to detect just 10 bacteria in a given sample. By loading each of the eight microcoils with different nanoparticles, the system could distinguish between simulated blood samples representing healthy individuals, those with cancer, and those with diabetes, by looking for eight different biomarker molecules.
Multiple applications
“The biggest advantage is that we don’t need sample preparation or purification steps,” Lee says. The nanoparticles are simply added to whatever samples are present. “This method could provide an easy and fast way to diagnose almost any kind of disease, such as bacterial infection or cancers in point-of-care settings – right next to the patient or in developing countries.”
The device could also be used to test for water purity or even applied to gaseous samples, to search for airborne pathogens or pollutants.
Other researchers are impressed with the work. “If you came to my lab you would see that our spectrometers occupy whole rooms, and we are always struggling with sensitivity in NMR experiments,” says , an NMR spectroscopist at the University of Edinburgh.
“They have been able to improve the sensitivity such that they can detect just a few bacteria. It’s quite remarkable that they can detect down to that limit,” he says.
Weissleder has filed a patent for the design and started a company called to market the devices.
Journal reference:
![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)


