Tiny enceladus exercises giant electromagnetic influence at Saturn
Peer-Reviewed Publication
Updates every hour. Last Updated: 20-Apr-2026 08:15 ET (20-Apr-2026 12:15 GMT/UTC)
Enceladus, a tiny moon of Saturn, trails a wake of electromagnetic ripples that extends over half a million kilometres. A major study by an international team of researchers using data from the NASA/ESA/ASI Cassini spacecraft has revealed a lattice-like structure of crisscrossing reflected waves that flow downstream behind the moon in Saturn's equatorial plane, but also reach up to very high northern and southern latitudes. The analysis of data from four instruments aboard Cassini, collected over the mission's 13-year duration, demonstrates the crucial role that Enceladus plays in circulating energy and momentum around Saturn’s space environment.
The University of Trento has demonstrated the existence of an empty lava tube even in the depths of Venus, a planet whose surface and geology have been largely shaped by volcanic processes. The cave was identified through radar data analysis as part of a project funded by the Italian Space Agency. "Our knowledge of Venus is still limited, and until now we have never had the opportunity to directly observe processes occurring beneath the surface of Earth’s twin planet. The identification of a volcanic cavity is therefore of particular importance, as it allows us to validate theories that for many years have only hypothesized their existence," explains Lorenzo Bruzzone, the coordinator of the research, full professor of the University of Trento. "This discovery contributes to a deeper understanding of the processes that have shaped Venus’s evolution and opens new perspectives for the study of the planet," he adds.
The largest gas giants in our galaxy blur the line between planets and brown dwarfs. How do these very large gas giants form? A team of researchers, led by the UC San Diego, used spectral data from the James Webb Space Telescope to probe the HR 8799 star system, leading to a surprising answer to this longstanding astronomical question.
The right amount of oxygen being present when the Earth’s core was formed meant that there were sufficient phosphorus and nitrogen available in the mantle and crust. This means the Earth was the beneficiary of a stroke of chemical good fortune in the universe. It is located in a zone with optimal chemical conditions for the development of life. When searching for life elsewhere in the universe, scientists should therefore look for solar systems that resemble our own. Focusing on water is not sufficient.
For years, The University of Texas at Arlington has been a leader in space physics education and research. Now, it’s expanding that impact with the launch of the Center for Space Physics and Data Science.
A recent study, led by the Center for Astrobiology (CAB), CSIC-INTA and using modelling techniques developed at the University of Oxford, has uncovered an unprecedented richness of small organic molecules in the deeply obscured nucleus of a nearby galaxy, thanks to observations made with the James Webb Space Telescope (JWST). The work, published in Nature Astronomy, provides new insights into how complex organic molecules and carbon are processed in some of the most extreme environments in the Universe.
Around the world, the total toxicity and ecological harm from agricultural pesticides are rising, despite recent United Nations commitments to halve pesticide use and risks by 2030. The findings establish a global, toxicity-weighted baseline for pesticide use and identify a subset of pesticides, crops, and countries driving the most biodiversity impacts. The widespread use of agricultural pesticides is a growing threat to global biodiversity. To address this concern, the 15th United Nations Biodiversity Conference set the goal of halving pesticide use and risk by 2030 and recently adopted a new global indicator – total applied toxicity (TAT) – that captures not just how much pesticide is used, but how harmful different chemicals are to living organisms. However, pesticide toxicity varies widely across non-target species; earlier global studies have focused on limited types of pesticides or species or have relied only on usage amounts. They have typically overlooked major differences in toxicity. As a result, the true range of pesticide threats to biodiversity, and the progress made toward UN commitments, remain obscure.
Using the TAT approach, Jakob Wolfram and colleagues developed a globally consistent way to measure the ecological harm of pesticides. Instead of relying on standards from a single country, Wolfram et al. used average regulatory safety thresholds per species group and pesticide derived from seven major regulatory authorities worldwide to ensure that the results reflect global conditions. By weighting total pesticide use with these toxicity benchmarks, the authors created a single comprehensive indicator that captures risks of 625 pesticides for a wide range of species. The findings show that the overall ecological toxicity of pesticides is rising worldwide, with increasing trends observed across many countries, crops, and groups of species. Overall, TAT is dominated by only a small number of highly toxic chemicals, with fruits and vegetables, corn, soybean, cereals, and rice accounting for 76-83% of global pesticide toxicity. Moreover, China, Brazil, the United States, and India together contribute 53-68% to the global TAT. According to Wolfram et al., the findings demonstrate that most countries are not on track to meet UN pesticide reduction targets without substantial changes.