Wolf-Rayet 104’s Orbit Tilt Reduces Gamma-Ray Burst Threat, Study Finds
A new study has shed light on the orbital alignment of the well-known Wolf-Rayet 104 (WR 104) system, long considered a potential threat due to its speculated gamma-ray burst (GRB) risk. Observations conducted using multiple instruments at the W. M. Keck Observatory in Hawaiʻi have confirmed that the star system‘s orbit is tilted 30 to 40 degrees away from Earth. This discovery significantly reduces concerns that a supernova from WR 104 could direct a GRB toward the planet.
Study Confirms Orbital Tilt
According to research published in the Monthly Notices of the Royal Astronomical Society, WR 104 comprises two massive stars locked in an eight-month orbital cycle. The system features a Wolf-Rayet star emitting a strong carbon-rich wind and an OB star producing a hydrogen-dominated stellar wind. Their collision generates a distinctive dust spiral that glows in infrared light.
The structure was first observed in 1999 at the Keck Observatory, and early models suggested that the pinwheel-like dust formation was face-on from Earth’s perspective. This led to speculation that the rotational axis of the stars—and potentially a GRB—could be aimed directly at Earth. However, new spectroscopic data contradicts this assumption.
Unexpected Findings Challenge Previous Models
Reportedly, Grant Hill, Instrument Scientist and astronomer, stated, that their view of the pinwheel dust spiral from Earth absolutely looked face-on and it seemed like a pretty safe assumption that the two stars are orbiting the same way. However, his analysis revealed a surprising discrepancy, with the stellar orbit misaligned from the dust structure.
This unexpected finding raises new questions about how the dust plume forms and whether additional factors influence its shape. While the discovery brings relief regarding potential GRB risks, it also suggests there is still much to understand about WR 104’s unique characteristics
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Marine mammals rely on oxygen to survive, yet some species stay underwater for long periods without breathing. Scientists at the University of St Andrews wanted to understand how gray seals manage their time underwater without relying on carbon dioxide buildup as a signal. Six adult gray seals were placed in a controlled environment to observe their diving patterns. The seals were only allowed to surface at a designated chamber, where researchers adjusted oxygen and carbon dioxide levels to test their responses.
Research Confirms Oxygen as the Primary Trigger
According to the study published in Science, different air compositions were tested to measure their effect on dive times. The air in the breathing chamber was adjusted across four conditions: normal air, increased oxygen, reduced oxygen, and heightened carbon dioxide levels. When oxygen levels were increased, seals stayed underwater for longer. When oxygen was reduced, they surfaced sooner. Carbon dioxide changes did not alter their behavior, suggesting that oxygen, not carbon dioxide, determines when they come up for air.
Unique Adaptation in Marine Mammals
Researchers says that grey seals have an internal system to track oxygen levels. This allows them to surface before reaching dangerous limits. This ability prevents drowning and may be common among other marine species. Since deep-diving mammals must manage oxygen carefully, similar mechanisms could be present in whales, dolphins and other seals.
Experts Weigh in on the Discovery
Lucy Hawkes from the University of Exeter and Jessica Kendall-Bar from the University of California, San Diego, discussed the study’s impact. They noted that understanding this adaptation sheds light on how marine mammals survive in extreme underwater conditions. Further research could explore how this system works in different species and environments.
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A team of scientists in Japan has developed a new type of “universal memory” technology that could significantly reduce energy consumption while increasing processing speeds in future computing devices. The breakthrough, which centres on an improved form of Magnetoresistive Random Access Memory (MRAM), addresses a critical challenge in current memory technologies by combining the speed of RAM with the ability to retain information without constant power supply.
Overcoming Previous MRAM Limitations
According to the study published in the journal Advanced Science on December 25, 2024, the newly developed MRAM technology overcomes the high energy requirements that have traditionally limited MRAM implementation. While conventional MRAM devices consume minimal power in standby mode, they require substantial electric current to switch magnetisation directions that represent binary values, making them impractical for widespread use.
Innovative Component Design
The research team created what has been described as a “multiferroic heterostructure” that consists of ferromagnetic and piezoelectric materials separated by an ultrathin layer of vanadium. This configuration allows magnetisation to be controlled by an electric field rather than current, significantly reducing power consumption.
Vanadium Layer Provides Stability
Previous MRAM prototypes struggled with structural fluctuations in the ferromagnetic layer. This made it difficult to maintain stable magnetisation directions. The addition of the vanadium layer acts as a buffer between the materials. This in turn helps in enabling the device to maintain its shape and form while preserving the magnetic state even after the electric charge is removed.
Future Impact and Considerations
As per the researchers, their prototype demonstrated the ability to switch magnetisation direction using minimal electric current. However, the study did not address potential degradation in switching efficiency over time. This is a common issue in electrical devices.
This technology could potentially enable more powerful commercial computing with longer device lifespans, as it requires significantly less power than previous solutions and offers greater resilience than current RAM technologies without requiring moving parts.
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