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Although lifespan has long been the focus of ageing research, the need to enhance healthspan — the fraction of life spent in good health — is a more pressing societal need. Caloric restriction improves healthspan across eukaryotes but is unrealistic as a societal intervention. Here, we describe the rewiring of a highly conserved nutrient sensing system to prevent senescence onset and declining fitness in budding yeast even when aged on an unrestricted high glucose diet. We show that AMPK activation can prevent the onset of senescence by activating two pathways that remove excess acetyl coenzyme A from the cytoplasm into the mitochondria — the glyoxylate cycle and the carnitine shuttle. However, AMPK represses fatty acid synthesis from acetyl coenzyme A, which is critical for normal cellular function and growth. AMPK activation therefore has positive and negative effects during ageing. Combining AMPK activation with a point mutation in fatty acid synthesis enzyme Acc1 that prevents inhibition by AMPK (the A2A mutant) allows cells to maintain fitness late in life without reducing the mortality associated with advanced age. Our research shows that ageing in yeast is not intrinsically associated with loss of fitness, and that metabolic re-engineering allows high fitness to be preserved to the end of life.

The authors have declared no competing interest.

Adeno-associated virus (AAV) is a prominent method for delivering genes in vivo. Therapeutic delivery to target cells is achieved through full capsids containing the gene cargo. However, the presence of empty capsids in the AAV drug product can reduce therapeutic effectiveness, necessitating their detection at various stages of the AAV production process. Traditional methods for assessing the AAV empty/full (E/F) ratio are often slow, labor-intensive, and require significant optimization.

Consider a novel, rapid, and high-throughput approach for determining the AAV E/F ratio using Octet® Biolayer Interferometry (BLI) alongside Octet® AAVX Biosensors. This cutting-edge technique evaluates intact viral capsids and is perfect for screening both crude and purified samples, offering a quicker and more efficient workflow with results available in as little as 30 minutes.

Discover the advantages of this innovative method and enhance your AAV workflow by downloading the technical note.

Imagine walking into your kitchen and instantly knowing if the fish you bought yesterday is still fresh—or entering an industrial site with sensors that immediately alert you to hazardous gas leaks. This isn’t science fiction—it’s the promise behind our newly developed nanomechanical sensor array, a powerful tool we’ve created to detect and analyze complex gases in real-time.

In our recent study published in Microsystems & Nanoengineering, we introduce a miniaturized array of silicon and polymer-based capable of detecting various gases quickly and accurately.

This array utilizes a simple yet ingenious principle: when gas molecules enter the sensor, they diffuse into specific polymers, causing them to swell slightly. This swelling generates detected by tiny piezoresistive sensors embedded in silicon. It’s like watching a sponge expand as it absorbs water—but at a microscopic scale, with the expansion measured electrically to detect and identify gases.

Astronomers have identified an exoplanet named Enaiposha, also known as GJ 1214 b, located 47 light-years from Earth. Initially classified as a mini-Neptune, further observations suggest it may belong to a different planetary category.

We now know it isn’t just neutron stars that emit such pulses. A white dwarf and a red dwarf star have been discovered closely orbiting each other emitting radio pulses every two hours. Their findings means we know it isn’t just neutron stars that emit such pulses, but these are spaced unusually far apart.

An international team of astronomers led by Dr Iris de Ruiter, now at the University of Sydney, has shown that a white dwarf and a red dwarf star orbiting each other every two hours are emitting radio pulses.

Thanks to follow-up observations using optical and x-ray telescopes, the researchers were able to determine the origin of these pulses with certainty. The findings explain the source of such radio emissions found across the Milky Way galaxy for the first time.

Keratinocytes produce collagen fibers, while deeper fibroblasts later modify the collagen fibers initially formed by keratinocytes. Challenging the long-standing belief that fibroblasts produce skin collagen, researchers at Okayama University have investigated collagen formation in the ‘glass-skinned’ amphibian axolotl and other vertebrates. They discovered that keratinocytes, the surface cells of the skin, are responsible for producing collagen, which is then transferred deeper to form the dermis. Later, fibroblasts migrate into this collagen layer, modifying and reinforcing its structure.

The skin consists of two primary layers. The epidermis, the outermost layer, is predominantly made up of keratinocytes, while the deeper dermis contains blood vessels, nerves, and structural proteins such as collagen, which give the skin its strength and texture. Traditionally, fibroblasts — specialized supporting cells within the dermis — have been believed to play a key role in producing collagen.

In humans, collagen is formed before and after birth. It has been believed that fibroblasts play an exclusive role in collagen production in the skin, and no keratinocytes contribute to collagen production. The statement “Collagen production in the human skin is achieved by fibroblasts” has been an unspoken agreement in the skin research field.

In a striking development, researchers have created a quantum algorithm that allows quantum computers to better understand and preserve the very phenomenon they rely on – quantum entanglement. By introducing the variational entanglement witness (VEW), the team has boosted detection accuracy while