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Recent tracking efforts have uncovered how the common noctule bat, a species capable of covering over 1,000 kilometres in a few days, adapts its migration patterns. Using tiny transmitters and environmental data, researchers have detailed the flexibility these bats display during seasonal migrations. The study highlights their reliance on tailwinds to traverse large distances across Europe, revealing a more dynamic migration strategy than previously understood.

Innovative Technology Tracks Migration Routes

According to a study published in the Science journal, researchers from the Max Planck Institute of Animal Behavior employed a 1-gram sensor attached to bats using temporary surgical glue. These devices recorded data such as acceleration and temperature, transmitting daily summaries.

Despite initial plans to use the International Space Station for data transmission being halted, an interconnected network of ground-based sensors provided the necessary tracking capabilities. Data from 71 of 125 tagged bats showed varied migration routes, with speeds ranging between 13 and 43 meters per second and flights extending up to 383 kilometres in a single night.

Environmental Cues Influence Timing

The study integrated weather data, including wind speed, direction, and temperature, to determine how environmental conditions influenced migration timing. It was found that the bats adjusted their departures, aligning with warming conditions to “surf” air currents ahead of weather fronts. This adaptive strategy allows them to conserve energy while maximizing travel efficiency.

Potential Conservation Applications

The findings may aid in the development of conservation strategies, particularly in mitigating bat fatalities caused by wind turbines. Edward Hurme, a behavioural ecologist at the Max Planck Institute, told Science.org that the potential to predict migration patterns and adjust turbine operations to minimise risks. Charlotte Roemer, a conservation biologist not involved in the study, noted to the publication that the technology promises to revolutionise migration research and answer longstanding questions about bat behaviour.

Reports have also linked similar behaviour to other bat species, such as Nathusius’ pipistrelle, demonstrating that warm air currents play a significant role in enhancing migration speed and efficiency.

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Scientists Discover Heaviest Proton-Emitting Nucleus After Nearly 30 Years

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Scientists Discover Heaviest Proton-Emitting Nucleus After Nearly 30 Years

Nuclear physicists have detected the radioactive disintegration of a rare isotope of astatine for the first time. This shows that the heaviest element found in nature may be modified a lot, maybe even destroyed, in a way that scientists didn’t predict. That oddball radioactive decay with 85 protons and 103 neutrons is almost (but not quite) a nuclear species that we would call stable. The finding was made by researchers at the University of Jyväskylä in Finland, and it’s a major development for nuclear physics. It describes something that just shouldn’t be and then shows us what the forces are that make for heavy atomic structures.

Rare Proton Decay in 188At Sheds Light on Extreme Nuclear Shapes and Stability Limits

As per a report published in Nature Communications on May 29, 2025, the isotope was produced using a fusion-evaporation reaction that entailed the irradiation of a natural silver target with strontium-84 ions. The exotic nucleus, 188 At, has a pronouncedly prolate form (of a ”watermelon” type) generated by the neutron and proton normal and attractive interaction in the inner shells of heavy nuclei experienced as a projectile in our case study.

Henna Kokkonen, the doctoral researcher who made the discovery, has mentioned that the proton emitted allows an unstable nucleus to progress towards stability by getting rid of a proton. The 190 At isotope was found by Kokkonen with the investigation of rare decay in the heavy nucleus, the rare interaction in the binding energy of the proton, and presumably a tendency change in the heavy atom region.

The team of the theory and experiment workshop pointed out the importance of exploring new decay modes and testing predictive models at the extremes of the periodic table. They also talked about how technology has improved in making and studying isotopes with short lifetimes.

Isotope discoveries of this scale remain rare in modern nuclear physics. Kokkonen expressed pride in contributing to a global effort that deepens our understanding of atomic structure. Each such finding helps refine our knowledge of nuclear forces, elemental formation, and the fundamental limits of matter. The breakthrough underscores how even after a century of nuclear science, the field continues to yield surprises from the smallest building blocks of the universe.

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Hubble Unveils Galactic ‘Cotton Candy’ in the Large Magellanic Cloud

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Hubble Unveils Galactic ‘Cotton Candy’ in the Large Magellanic Cloud

Hubble’s latest view reveals a jewel-like cloudscape of gas and dust in the Large Magellanic Cloud (LMC), a dwarf galaxy about 160,000 light-years from Earth. This Milky Way companion is our galaxy’s largest satellite, and its active stellar nurseries glow in intricate pastel filaments. The wispy tendrils in the image have been likened to brightly colored “cotton candy” because of their pink, blue and green hues. Astronomers use scenes like this to probe star formation and dust. By tracing where dust hides newborn stars, Hubble’s sharp view reveals the structure of stellar nurseries in this nearby galaxy.

Galactic Cotton Candy: Nebula and Stars

According to NASA’s official site, this rich nebula was imaged with Hubble’s Wide Field Camera 3 (WFC3) using five different filters, including ultraviolet and infrared bands. Each filter isolates a range of wavelengths, so the composite image highlights different components of the cloud. Bright regions mark hot young stars lighting up gas, while darker filaments are cooler dust clouds blocking light.

In effect, the image maps the interplay of stars and gas: astronomers see how massive stars sculpt the nebula, triggering new generations of star birth in the gas and dust. The vivid patterns of emission and absorption trace the LMC’s galactic structure, helping researchers study how its interstellar medium fuels star formation.

Beyond the Visible: Filters and False Color

Hubble’s technicians assigned colors to the filtered data to make the invisible visible. Visible-light filters use their natural hues, while ultraviolet light is shown as blue/violet and infrared as red. In this five-filter image, for example, ultraviolet-dominated spots and infrared-bright regions are translated into shades of blue, purple and red. This color scheme “closely represents reality while adding new information” from parts of the spectrum our eyes cannot see. In practice, it means the image remains scientifically faithful but emphasizes features that humans would otherwise miss.

The final result is both a tool and a portrait: astronomers gain insight into the composition and temperature of the gas and dust (for example, hydrogen-rich regions glowing pink), while the public enjoys a stunning, otherworldly view of a neighboring galaxy.

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James Webb Telescope Maps Fiery Atmosphere of Turbulent Exoplanet WASP-121b

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James Webb Telescope Maps Fiery Atmosphere of Turbulent Exoplanet WASP-121b

Astronomers have found a way to see through the turbulent atmosphere of a distant planet that experienced heat and gale-force winds — conditions that are thought to be similar to those on an early version of Earth that was also cold and blanketed by clouds. They accomplished it with the help of the NASA James Webb Space Telescope (JWST). WASP-121b orbits 900 light-years from Earth and circles its star once every 30 hours. That is why it has been shaped like a football and cooked to such a high degree; one side may become hotter than 3,000°C, which is hot enough to melt iron. This hellish world’s atmosphere has been analysed in unprecedented detail, revealing complex chemical signatures that hint at its violent origins and ongoing transformation.

JWST Detects Rare Molecules in WASP-121b’s Atmosphere, Revealing Planet’s Fiery Migration and Extreme Conditions

As per a recent report published by NASA, with JWST’s Near Infrared Spectrograph (NIRSpec) instrument, scientists have been able to detect several molecules in the atmosphere of WASP-121b. A research study used a technique on a planetary atmosphere and found that silicon monoxide is the most important chemical. The research says that it developed early in the history of its star system, in a colder part of space, like Jupiter and Uranus in our solar system. This inward spiral, which was probably caused by gravity, cut off frozen material but let carbon-rich gas build up, which is what caused the present imbalance in the atmosphere.

The researchers used a three-dimensional model to depict how the temperature varies from the sunlit side to the night side of WASP-121b. They detected silicon monoxide, indicating that minerals were sponged up from the earliest asteroid impacts. It was hot, yes, but they detected methane on the nightside, a sign of vigorous up-and-down mixing that was pushing back toward the planet from cooler altitudes in the atmosphere. That flies in the face of everything we know about the atmospheres of other planets.

Observations of ultra-hot gas giants teach us about how atmospheres evolve, and JWST could share new insights. Then again, this could change the way we model and comprehend the formation of the planets around stars that aren’t so friendly.

It’s not what one would call a gentle planet, WASP-121b, a slapdash world. The observations made by JWST will be deeper, and scientists are eager to learn the variety of types of exoplanets out there in our galaxy.

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