Local environment shapes galaxy growth in early universe
Peer-Reviewed Publication
Updates every hour. Last Updated: 28-May-2026 02:16 ET (28-May-2026 06:16 GMT/UTC)
Astronomers using the James Webb Space Telescope observed a large group of galaxies which had been discovered in the early Universe by the Subaru Telescope. The observations show that even as early as 1.2 billion years after the birth of the Universe, the local environment was already influencing galaxy growth. These results provide new insights into the development of galaxies throughout the history of the Universe.
Scientists from Israel and Germany have completed integration and testing of the first nanosatellite in the CloudCT network, an innovative space mission designed to improve climate predictions through three-dimensional imaging of clouds. The satellite is scheduled for launch from California in June 2026, with ten additional satellites planned for 2027 if the precursor mission succeeds.
Led by Prof. Ilan Koren of the Weizmann Institute of Science, Prof. Yoav Schechner of the Technion – Israel Institute of Technology, and Prof. Klaus Schilling of Zentrum für Telematik, the project introduces a novel cloud observation method inspired by computed tomography (CT) used in medicine. The system combines simultaneous multi-angle satellite imaging, polarization-sensitive cameras, and AI-based analysis to reconstruct the internal structure and microphysical properties of clouds in unprecedented detail.
Researchers say the mission addresses major uncertainties in climate and weather modeling by capturing small cloud formations that are difficult to observe with existing remote-sensing technologies. The miniature precursor satellite weighs about 4 kilograms and must autonomously orient itself toward target clouds with extremely high precision.
The project was supported by a European Research Council (ERC) Synergy Grant.
Biochar, a charcoal-like substance added to soil, is widely seen as a tool for improving crop yields and locking away carbon. When added to soil, it creates a unique micro-environment known as the charosphere, where complex chemical reactions take place. A new investigation from Northwest A&F University now shows that this zone can become a hotspot for reactive oxygen species (ROS)—highly unstable molecules that can influence critical soil processes. The findings demonstrate that how biochar is produced determines the type of ROS created, with significant consequences for its ability to mitigate greenhouse gases.
The research team, led by corresponding author Hanzhong Jia, conducted controlled incubation experiments to track chemical changes in the soil immediately surrounding biochar. They produced biochar at two different pyrolysis temperatures—a lower 300°C and a higher 500°C—to see how this affected its properties. Using fluorescence imaging and electron paramagnetic resonance spectroscopy, they identified and quantified the different ROS being generated in the charosphere over time and space, linking them back to the specific particles released by each type of biochar.
A large-scale study of human mobility and wildlife movement across the United States suggests that the day-to-day presence of humans – not just how they alter the landscape – is a major ecological force that shapes how animals move through and use their environments, researchers report. Human activity is accelerating global biodiversity loss by transforming climates and rapidly reshaping natural landscapes. Yet beyond these physical alterations of the environment, there is a growing recognition that the direct presence of humans themselves may greatly influence how animals behave, including how they perceive risk, move through their habitats, compete for resources, and interact with other species. Despite this, large-scale comparative research has rarely examined human presence as a distinct and dynamic pressure on wildlife, largely due to the fact that detailed data on where and when people move are difficult to obtain. Most existing studies have focused on local settings or broad proxies of human presence, such as pandemic-related lockdowns, and have concentrated largely on mammals. As a result, relatively little is known about how interacting forms of human activity and presence combine to affect wildlife.
To address this gap, Ruth Oliver and colleagues combined data on numbers of mobile devices and vehicles in each U.S. census block as a measure of human presence, along with detailed measures of human landscape modification, with animal tracking data from more than 4,500 birds and mammals representing 37 species. By centering their study on the years 2019 and 2020 and leveraging the unique, temporary decline of human movement in modified landscapes during the COVID-19 pandemic, Oliver et al. were able to disentangle the direct effects of human activity from the broader impacts of landscape change and evaluate how each factor influenced the amount of space animals used. According to the findings, direct human presence influenced the movement patterns or use of the environment of 65% of species examined. Many mammals reduced the amount of territory they used in response to greater human activity, particularly in less-developed habitats where animals may perceive humans as a threat. On the other hand, some species, like gray wolves, expanded their ranges, likely to better avoid people. Adaptable species such as white-tailed deer appeared more comfortable incorporating human-modified environments into their usable habitats. Birds likewise showed highly variable responses, with some species becoming more spatially constrained and others altering their habitat use depending on the surrounding degree of development. In a related Perspective, Lydia Beaudrot discusses the study and its findings in greater detail.
Using observations from the James Webb Space Telescope (JWST), researchers have identified cloudy “mornings” and clear “evenings” on a distant gas giant exoplanet. The findings suggest that the planet’s atmospheric aerosols are dominated by condensation-driven clouds that form, circulate, and evaporate as they move through extreme temperature contrasts across the planet. Aerosols play an important role in shaping the appearance, chemistry, and temperature of exoplanet atmospheres. However, there is limited information about the nature of these particles, including their atmospheric distribution or the physical processes that determine their properties. In hot Jupiters – a class of gas giant exoplanets that are physically similar to Jupiter – it has long been debated whether atmospheric aerosols are primarily mineral clouds formed through condensation or photochemical hazes generated by intense stellar radiation. Because they can obscure or distort spectral signals, they also complicate efforts to determine the chemical composition of distant worlds.
Here, Sagnick Mukherjee and colleagues used the Near Infrared Imager and Slitless Spectrograph (NIRISS) instrument on the JWST to observe the tidally locked, hot Jupiter exoplanet, WASP-94A b, and analyzed the light passing separately through the planet’s “morning” and “evening” atmospheric horizons. The findings revealed stark differences between the two hemispheres: the cooler morning side appeared heavily shrouded in high-mineral clouds that obscure gaseous signatures, while the hotter evening side is comparatively clear and shows strong water vapor absorption. According to Mukherjee et al., this pattern suggests that the planet’s aerosols are dominated by clouds formed through condensation rather than photochemical processes. Moreover, further analysis using a 3D general circulation model indicates a dynamic cloud cycle driven by extreme temperature contrasts of roughly 450 degrees Kelvin between the planet’s two hemispheres. Clouds appear to form on the cooler night side of the planet, circulate toward the morning side, and then evaporate as they move into the intensely heated day side. According to Mukherjee et al., the findings warn that treating an exoplanet’s atmosphere as uniform, which is a common simplifying assumption, can significantly distort or bias estimates of their chemistry and physical properties, and suggest that previous measurements of exoplanet atmospheres may need to be reconsidered to account for complex, asymmetric weather systems.
A new large-scale study led by a research team from the Yale Center for Biodiversity and Global Change has found that wildlife responds not only to how humans reshape their habitats, but also to the simple presence of humans — and sometimes in surprising ways.
Even small changes in how people move through environments can significantly affect animal behavior and could have implications for wildlife conservation efforts, the study finds.
“Our findings provide an important nuance in our understanding of wildlife in a rapidly changing world,” said Walter Jetz, a professor of ecology and evolutionary biology in Yale’s Faculty of Arts and Sciences and director of the Yale Center for Biodiversity and Global Change.
“Animals are affected by both direct human presence and by human-caused changes to the physical environment, such as agriculture and urbanization,” Jetz said. “This study is the first to directly assess at scale how both causes, separately and in combination
Suppose there are signs of extraterrestrial life and we have not yet been able to detect them. What does that mean? In the renowned journal Nature Astronomy, researchers discuss the consequences of these so-called false-negative results. “We are currently investing a great deal of money in missions that might need to be designed differently.”