Scientists have achieved their initial goal of converting light into a supersolid material that unites solid-stage characteristics with those of superfluids. The discovery establishes paths toward studying uncommon quantum nature states of matter while carrying great implications for technological growth.

The matter form known as a supersolid behaves as both a solid and shows the properties of a superfluid. Despite keeping its rigid arrangement, the material demonstrates smooth flow while remaining non-frictional. Theoretical research on supersolids as a matter state has continued for decades since scientists first considered them in the 1970s. Through precise conditions, scientists believe materials can develop combined solid and superfluid properties to produce an absolute natural anomaly.

The discovery shows how particular materials become supple when exposed to exceptionally cold temperatures because they transition into a viscosity-free state. The dual properties of rigidness combined with fluidity create an extraordinary phase called supersolid in matter. Traditional materials possess two distinct states because solids maintain their shape, yet liquids possess free movement. Supersolids demonstrate behaviour beyond normal fluid-solid definitions because they exhibit features of both states.

Scientists confirm exotic “Plastic Ice VII,” a rotating water ice phase under extreme conditions.

Now, scientists at UCL and the University of Cambridge have discovered a new type of ice that resembles liquid water more closely than any other known ice, which may rewrite our understanding of water and its many anomalies. The newly discovered ice is amorphous: Its molecules are disorganized. They need to be properly ordered as ordinary, crystalline ice.

In a jar frozen to-200 degrees Celsius, scientists employed a technique known as ball milling, aggressively shaking common ice and steel balls. Ball milling is used in several industries to grind or blend materials, but it has yet to be applied to ice.

In the study, liquid nitrogen was used to cool a grinding jar to-200 degrees Centigrade, and the density of the ball-milled ice was determined from its buoyancy in liquid nitrogen. Scientists used several other techniques, including X-ray diffraction and Raman spectroscopy, to analyze the structure and properties of ice. They also used small-angle diffraction to explore its long-range structure.

Technique for precise measurement of electrostatic properties of materials.

Tunneling spectroscopy confirms exotic superconducting state in iron-based superconductor.

A kind of metamaterial that has been beyond the reach of existing technologies so far.

Variability in the brightness of Sagittarius A* (Sgr A•, the black hole at the center of the Milky Way, could emerge through synchrotron radiation emitted by electrons accelerated by the supermassive black hole’s accretion disk [1]. That is the finding of a team of astronomers led by Farhad Yusef-Zadeh at Northwestern University, Illinois. The researchers hope that their results could lead to deeper insights into the distinctive flaring patterns in the material that surrounds many black holes.

Weighing in at just over 4 million solar masses, Sgr A* is a supermassive black hole, which is fueled by the material it draws in from interstellar space. Since it is both relatively close by and vastly more massive than any other body in the Galaxy, Sgr A* provides astronomers with an ideal opportunity to study how fueling material is irradiated, captured, accreted, and ejected by a black hole. In particular, astronomers have identified short outbursts, or flares, in the near-infrared (NIR) emission from infalling material. In many cases, radiation at this frequency is a key tracer of flow dynamics within a black hole’s inner accretion disk and can hint at the mechanisms driving those flows.

Yusef-Zadeh’s team observed these flares several times between 2023 and 2024 using the NIR instrument aboard the JWST observatory. This instrument allowed the team to observe Sgr A* at two different NIR frequencies, which enabled the researchers to study both the time variability of the flares and their energy distribution.

A new study by Rice University researchers Sho Shibata and Andre Izidoro presents a compelling new model for the formation of super-Earths and mini-Neptunes—planets that are 1 to 4 times the size of Earth and among the most common in our galaxy. Using advanced simulations, the researchers propose that these planets emerge from distinct rings of planetesimals, providing fresh insight into planetary evolution beyond our solar system. The findings were recently published in The Astrophysical Journal Letters.

For decades, scientists have debated how super-Earths and mini-Neptunes form. Traditional models have suggested that planetesimals—the tiny building blocks of planets—formed across wide regions of a young star’s disk. But Shibata and Izidoro suggest a different theory: These materials likely come together in narrow rings at specific locations in the disk, making planet formation more organized than previously believed.

“This paper is particularly significant as it models the formation of super-Earths and mini-Neptunes, which are believed to be the most common types of planets in the galaxy,” said Shibata, a postdoctoral fellow of Earth, environmental and planetary sciences. “One of our key findings is that the formation pathways of the solar system and exoplanetary systems may share fundamental similarities.”

However, their reliance on extremely low temperatures has limited their practical applications. Now, scientists may be one step closer to breaking that barrier.

In groundbreaking research led by Professor Kostya Trachenko of the Queen Mary University of London, the maximum temperature at which superconductors can operate has been linked to fundamental constants of nature, such as the electron mass, electron charge, and the Planck constant.

These constants, essential for atomic stability and star formation, set the upper limit for superconducting temperatures between hundreds and a thousand Kelvin. Encouragingly, this range includes room temperature.

In a new call for proposals, DARPA envisions living materials that could self-assemble into antennas, nets to capture debris, or even space station parts.