In a new Science study, researchers report that bark microbes process methane, hydrogen, and carbon monoxide, showing that bark is an important component of global trace gas dynamics.
Learn more in a new Science Perspective.
Microbes living in bark can process the greenhouse gases methane, hydrogen, and carbon monoxide.
Vincent Gauci Authors Info & Affiliations
Science
Vol 391, Issue 6781
Challenging long-held assumptions, Aarhus University researchers have demonstrated that the protein building blocks essential for life as we know it can form readily in space. This discovery, appearing in Nature Astronomy, significantly raises the statistical probability of finding extraterrestrial life.
In a modern laboratory at Aarhus University and at an international European facility in Hungary (HUN-REN Atomki), researchers Sergio Ioppolo and Alfred Thomas Hopkinson conduct pioneering experiments. Within a small chamber, the two scientists have mimicked the environment found in giant dust clouds thousands of light-years away. This is no easy feat.
The temperature in these regions is a freezing −260° C. There is almost no pressure, meaning the researchers must constantly pump out gas particles to maintain an ultra-high vacuum. They are simulating these conditions to observe how the remaining particles react to radiation, exactly as they would in a real interstellar environment.
Astronomers have discovered a vast, dense cluster of massive galaxies just 1 billion years after the Big Bang, each forming stars at an intense rate from collapsing clouds of dust. Reported in Astronomy & Astrophysics by an international team, led by Guilaine Lagache at Aix-Marseille University, the structure appears to challenge existing models of how rapidly stars could have formed in the early universe.
In many newly forming galaxies, immense clouds of gas and dust collapse under their own gravity, igniting rapid bursts of star formation. This process can be studied by observing extremely distant galaxies, whose light is only now reaching Earth after traveling for more than 12 billion years.
However, these observations present a challenge for astronomers. Since dust within the distant galaxy is a strong absorber of the light produced by newly forming stars, these regions are often impossible to observe directly at visible wavelengths.
The interstellar object, 3I/ATLAS, was first discovered in July 2025, and made its closest approach to the sun (perihelion) in late October. New observations of 3I/ATLAS were taken in December from the SPHEREx observatory—a near-infrared space observatory used for spectrophotometry. The analysis of these observations was recently discussed by a team of scientists in a paper on arXiv, and reveals some dramatic differences from the data taken before 3I/ATLAS reached perihelion.
SPHEREx first analyzed spectrographic data from 3I/ATLAS in August, shortly after its discovery. At the time, the interstellar object was moving inward, getting closer to the sun, but still between Jupiter and Mars.
At this time, spectrographic analysis showed “barely detectable” H2O-gas, according to the study authors, along with a CO2 coma. The CO2 gas production was estimated in a prior study to be about 9.4 × 1026 molecules/sec, with upper limits for H2O and CO being much lower. Carbon-based organic compounds (collectively referred to as C-H), like methanol (CH3OH), formaldehyde (H2CO), methane (CH4), and ethane (C2H6) were not detectable at the time.
Quantum mechanics is rich with paradoxes and contradictions. It describes a microscopic world in which particles exist in a superposition of states—being in multiple places and configurations all at once, defined mathematically by what physicists call a “wavefunction.” But this runs counter to our everyday experience of objects that are either here or there, never both at the same time.
Typically, physicists manage this conflict by arguing that, when a quantum system comes into contact with a measuring device or an experimental observer, the system’s wavefunction “collapses” into a single, definite state. Now, with support from the Foundational Questions Institute, FQxI, an international team of physicists has shown that a family of unconventional solutions to this measurement problem—called “quantum collapse models”—has far-reaching implications for the nature of time and for clock precision.
They published their results suggesting a new way to distinguish these rival models from standard quantum theory, in Physical Review Research, in November 2025.
A hundred years ago, quantum mechanics was a radical theory that baffled even the brightest minds. Today, it’s the backbone of technologies that shape our lives, from lasers and microchips to quantum computers and secure communications.
In a sweeping new perspective published in Science, Dr. Marlan Scully, a university distinguished professor at Texas A&M University, traces the journey of quantum mechanics from its quirky beginnings to its role in solving some of science’s toughest challenges.
“Quantum mechanics started as a way to explain the behavior of tiny particles,” said Scully, who is also affiliated with Princeton University. “Now it’s driving innovations that were unimaginable just a generation ago.”
Light is a universal stimulus that influences all living things. Cycles of light and dark help set the biological clocks for organisms ranging from single-celled bacteria to human beings. Some bacteria use photosynthesis to convert sunlight into energy just like plants, but other bacteria sense light for less well-known functions.
In 2019, Sampriti Mukherjee, Ph.D., and her team at the University of Chicago discovered that far-red light, part of the light spectrum near the infrared range, prevents the formation of biofilms by the human pathogen Pseudomonas aeruginosa.
Biofilms form when communities of bacteria cluster together and attach to surfaces like medical devices or tissues. Pseudomonas aeruginosa is an antibiotic-resistant bacterium, normally found in the soil and water, that is known to cause difficult to treat infections in hospitalized patients, especially those with weakened immune systems, lung diseases, or large wounds like burns. Figuring out how to prevent this pathogen from forming biofilms could help treat these dangerous infections.
Researchers out of Spain and Italy report a globally pooled Internet Gaming Disorder prevalence of 6.1% among adults ages 18–35. Internet Gaming Disorder is considered a condition for further study in DSM-5-TR, with official classification in ICD-11.
Gaming problems often get viewed as an adolescent concern, while evidence indicates growing vulnerability in young adults. Late adolescents and young adults tend to show higher levels of depression, anxiety, and stress, along with lower self-esteem, compared to healthy regular gamers.
DSM-5-TR includes nine criteria for Internet Gaming Disorder, including preoccupation with gaming, withdrawal symptoms, tolerance, unsuccessful attempts to control gaming habits, loss of interest in previous hobbies, continued excessive gaming despite problems, deception about the extent of gaming, gaming used to escape negative mood, and jeopardizing relationships or opportunities. Diagnosis requires at least five of those nine criteria within 12 months.
A UCLA-led, multi-institution research team has discovered a metallic material with the highest thermal conductivity measured among metals, challenging long-standing assumptions about the limits of heat transport in metallic materials.
Published in Science, the study was led by Yongjie Hu, a professor of mechanical and aerospace engineering at the UCLA Samueli School of Engineering. The team reported that metallic theta-phase tantalum nitride conducts heat nearly three times more efficiently than copper or silver, the best conventional heat-conducting metals.