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Atomic-level engineering enables new alloys that won’t break in extreme cold

Navigating the extreme cold of deep space or handling super-chilled liquid fuels here on Earth requires materials that won’t break. Most metals become brittle and fracture at such low temperatures. However, new research is pioneering an approach to build metal structures atom by atom to create tough and durable alloys that can withstand such harsh environments.

Traditional strengthening approaches are often not good enough for these applications. For example, a common heat treatment technique called precipitation hardening strengthens metals by creating tiny hard particles within their structure. But in , the materials can lose their ductility (the ability to bend, stretch or be pulled into a new shape without breaking) and fracture suddenly.

A study published in the journal Nature describes a new way to design so they stay strong and tough even at super low temperatures. The big idea is to create an alloy with two different types of perfectly arranged atomic structures inside it. These structures are called subnanoscale short-range ordering (SRO), which are tiny islands of organized atoms and nanoscale long-range ordering (NLRO), which are slightly larger.

Astrophysicists Zero In on Source of Strange Gamma-Ray Signals

Millisecond pulsar binaries may produce the excess 511 keV photons seen in the galaxy. These systems could expose hidden pulsars and even exoplanets. Many astrophysicists devote their work to tracing the origins of photons, since certain types are closely linked to specific cosmic processes. Iden

Mysterious “Soot Planets” May Be Hiding in Plain Sight Among the Stars

Some planets may be soot-rich rather than water-based. Atmosphere studies will be key to understanding their true nature. Astronomers generally consider water worlds to be among the most common types of planets in our galaxy, largely because of their low densities and the abundance of water ice b

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Isotopic analysis determines that water once flowed on asteroid Ryugu

A team of researchers, including those at the University of Tokyo, discovered that liquid water once flowed on the asteroid that spawned near-Earth asteroid Ryugu more than a billion years after it first formed. The finding, based on tiny rock fragments returned by the Hayabusa2 spacecraft of the Japan Aerospace Exploration Agency (JAXA), overturns long-held assumptions that water activity on asteroids only occurred in the earliest moments of solar system history. This could impact current models, including those describing the formation of Earth.

We have a relatively good understanding of how the solar system formed, but of course there are many gaps. One such gap in our knowledge is how Earth came to possess so much water. It’s long been known that so-called carbonaceous asteroids like Ryugu formed from ice and dust in the outer solar system supplied water to Earth.

Ryugu was famously visited by the Hayabusa2 spacecraft in 2018, the first visit of its kind, where not only were in-situ data collected, but small samples of material were brought back to Earth too. And it’s thanks to this endeavor that researchers can help fill in some missing details in the picture of our creation.

Unusual CO₂-rich disk detected around young star challenges planet formation models

A study led by Jenny Frediani at Stockholm University has revealed a planet-forming disk with a strikingly unusual chemical composition: an unexpectedly high abundance of carbon dioxide (CO2) in regions where Earth-like planets may one day form.

The discovery, made using the James Webb Space Telescope (JWST), challenges long-standing assumptions about the chemistry of planetary birthplaces. The study is published in Astronomy & Astrophysics.

“Unlike most nearby planet-forming disks, where dominates the inner regions, this disk is surprisingly rich in ,” says Jenny Frediani, Ph.D. student at the Department of Astronomy, Stockholm University.

Envisioning a Neutrino Laser

A Bose-Einstein condensate of radioactive atoms could turn into a source of intense, coherent, and directional neutrino beams, according to a theoretical proposal.

Neutrinos are the most abundant massive particles in the Universe, yet they are the ones about which we know the least. What makes these elusive particles hard to study is their feeble interaction with matter—trillions of neutrinos pass through our bodies every second without leaving a trace. However, neutrinos may hold deep secrets about the Universe—understanding their properties could hint at new particles and forces beyond the standard model of particle physics or shed light on why matter came to dominate over antimatter. Despite these tantalizing prospects, some of the most basic questions about neutrinos remain unanswered. To address such questions experimentally, Benjamin Jones of the University of Texas at Arlington and Joseph Formaggio of MIT suggest that a Bose-Einstein condensate (BEC) of radioactive atoms could offer a platform for building a “neutrino laser” [1].

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