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Scientists Discover Two New Supernova Remnants in a Surprising Location

Two mysterious light sources detected on the outskirts of the Large Magellanic Cloud have been identified as previously unknown supernova remnants. The discovery was made using the European Space Agency’s X-ray observatory, XMM-Newton after observations revealed unexpected X-ray emissions. Supernova remnants are formed when massive stars explode, creating shock waves that ionise and compress surrounding interstellar matter. The detection of these remnants in an area where supernovae are rarely found has raised new questions about the distribution of ionised gas in this dwarf galaxy.

Identification of J0624-6948 and J0614-7251

According to a study published in Astronomy & Astrophysics, the two supernova remnants, J0624-6948 and J0614-7251, were observed as distinct circular structures in visible-light imaging. The newly released images from ESA show these remnants in the lower-left portion of the Large Magellanic Cloud, with J0624-6948 appearing in orange and J0614-7251 in blue. As reported by space.com, previously identified supernova remnants in the galaxy were marked with yellow crosses. The study explains that for a supernova to leave behind a remnant, the explosion must occur in a region containing ionised gas, typically found in dense star-forming areas rather than in the outskirts of a galaxy. The brightness and size of the newly detected remnants align with other confirmed cases in the Large Magellanic Cloud.

Impact on Understanding of Galactic Structures

In an official statement ESA scientists noted that these findings suggest a higher concentration of ionised gas in the Large Magellanic Cloud than previously estimated. The research proposes that interactions between the Milky Way, the Small Magellanic Cloud, and the Large Magellanic Cloud could be influencing the movement and compression of interstellar material. It is suggested that gravitational forces between these galaxies may be altering gas distribution, leading to unexpected regions of star formation and supernova activity.

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May 2024 Solar Storm Triggers Unusual Radiation Belts, Raising Space Safety Concerns

A significant solar storm that occurred in May 2024 led to the formation of two temporary radiation belts around Earth, as confirmed by satellite data. The discovery was made when a dormant satellite resumed operations after months of inactivity. The storm, which was among the most intense geomagnetic disturbances since 1989, resulted in widespread auroral displays and introduced high-energy particles into the Earth’s magnetosphere. While such temporary belts have been documented before, scientists have found that one of the newly formed belts exhibited unique properties, with a composition different from previous observations. One of the belts has already dissipated, but the other remains intact, posing potential challenges for future space missions.

Temporary Radiation Belts Detected Following Intense Solar Activity

According to research published in the Journal of Geophysical Research: Space Physics, the Colorado Inner Radiation Belt Experiment (CIRBE) satellite identified the new radiation belts upon reactivation in June 2024. The spacecraft had gone silent due to a technical issue in April, missing the peak of the storm. Upon its return, data analysis revealed the existence of two additional belts situated between the pre-existing Van Allen radiation belts.

It was determined that while the first belt contained high-energy electrons, consistent with previous storm-induced radiation belts, the second belt displayed an unusual concentration of high-energy protons. This presence of protons was linked to the extreme nature of the solar storm, which had released significant bursts of charged particles into Earth’s magnetic field.

Extended Lifespan of the Newly Formed Belts

Temporary radiation belts generated by solar storms are known to persist for weeks before dispersing. However, as per the findings, the electron-dominated belt remained for three months, while the proton-rich belt is still present. David Sibeck, a heliophysicist at NASA’s Goddard Space Flight Center, stated in an interview with Space.com that these particles could stay trapped for an extended period, creating a lasting impact on Earth’s inner radiation environment.

The proton belt’s resilience is attributed to its location in a more stable region of Earth’s magnetic field, where external disturbances have less impact. In contrast, a subsequent solar storm in June 2024 caused a reduction in the electron belt, with further weakening observed in August. Despite this, the proton belt has remained largely unaffected.

Implications for Space Missions and Satellite Operations

The existence of these new radiation belts has raised concerns regarding the safety of satellites and crewed space missions. Charged particles at high energy levels can pose risks to electronic components and human health in space. Spacecraft passing through these regions, particularly those traveling to geostationary orbit or beyond, may require additional shielding to mitigate radiation exposure.

As reported, the presence of these belts could necessitate adjustments in launch plans for future missions. With prolonged radiation hazards, space agencies may need to factor in the evolving space weather conditions before deploying satellites or sending astronauts beyond Earth’s orbit.

Despite the CIRBE satellite’s crucial discovery, the same solar activity that led to the identification of the new radiation belts also caused the spacecraft’s eventual demise. The increased energy injected into the atmosphere resulted in greater drag, which led to CIRBE’s descent and disintegration in October 2024.

The impact of solar storms on Earth’s magnetosphere continues to be closely monitored, with scientists studying how these phenomena affect both planetary and technological systems.

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NASA, General Atomics Test Nuclear Fuel for Faster Mars Missions

Efforts to develop nuclear thermal propulsion (NTP) for future space missions have taken a significant step forward. General Atomics Electromagnetic Systems (GA-EMS), in collaboration with NASA, has conducted tests on nuclear reactor fuel designed for space travel. The trials, held at NASA’s Marshall Space Flight Center in Alabama, assessed the fuel’s ability to withstand extreme conditions that would be encountered during deep space missions. The successful results could accelerate plans for faster, more efficient space travel, reducing transit times for crewed missions to Mars.

Successful Testing at NASA’s Marshall Space Flight Center

As reported by space.com, according to the tests conducted at NASA’s facility, the reactor fuel was subjected to six thermal cycles using hot hydrogen, rapidly heating it to 2326.6 degree Celsius. The objective was to evaluate the fuel’s resilience under extreme temperature fluctuations and exposure to hot hydrogen gas, conditions necessary for nuclear thermal propulsion. GA-EMS President Scott Forney stated in a company release that the fuel demonstrated the ability to endure these conditions, reinforcing confidence in its potential for safe and reliable space propulsion.

First-of-Its-Kind Testing of Nuclear Fuel

GA-EMS Vice President of Nuclear Technologies and Materials, Christina Back, highlighted the uniqueness of these tests in the company release. The company was reported to be the first to utilise the compact fuel element environmental test (CFEET) facility at NASA’s Marshall Space Flight Center for such trials. Fuel performance was tested at temperatures reaching 2,727 degree Celsius, with findings indicating a significant efficiency boost over conventional propulsion systems.

Potential Impact on Space Exploration

As per sources, NASA has prioritised the development of nuclear propulsion due to its potential to significantly reduce travel time to Mars. Shorter missions could lower the risks associated with long-duration spaceflight, including radiation exposure and the need for extensive life-support resources. In 2023, NASA and the Defense Advanced Research Projects Agency (DARPA) announced joint efforts to develop an NTP system, with a planned demonstration by 2027. The latest advancements in nuclear propulsion technology could play a crucial role in achieving that goal, bringing human missions to Mars closer to reality.

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Atmos Space Cargo’s Phoenix Capsule Set for First Orbital Test on SpaceX Mission

A cargo-return technology developed by Germany-based Atmos Space Cargo is set to undergo its first in-space test with an upcoming SpaceX mission. The company’s Phoenix capsule will be launched aboard the Bandwagon 3 rideshare mission, scheduled for no earlier than April. The capsule has been designed to facilitate the safe return of high-value materials from orbit, particularly benefiting the biomedical sector. The test mission aims to gather crucial data on the capsule’s subsystems, onboard payloads, and reentry performance.

Mission Objectives and Scientific Payloads

According to reports, the Phoenix capsule will carry four payloads, including a radiation detector from the German Aerospace Center (DLR) and a bioreactor from UK-based Frontier Space. The mission’s primary goals include testing Phoenix’s performance in orbit, evaluating data from customer experiments, and deploying its proprietary inflatable atmospheric decelerator (IAD) for reentry stabilisation. This technology, acting as both a heat shield and parachute, is intended to enable a controlled descent back to Earth.

Challenges in Returning Space Cargo

Industry experts highlight that while the cost and complexity of launching experiments into space have been reduced, bringing them back to Earth remains a challenge due to high costs, long turnaround times, and technical difficulties. Atmos Space Cargo has positioned Phoenix as a cost-effective and reliable solution for returning biomedical samples, microgravity-manufactured materials, and other sensitive payloads.

Future Prospects and Industry Impact

Despite expectations that Phoenix will not survive its debut mission, the collected data will contribute to future improvements. Larger iterations of the capsule are planned to carry heavier payloads, including potential returns of rocket stages. Advisory board member and former NASA Deputy Administrator Lori Garver has stated that advancements in reusable and affordable cargo return technology are critical for the future of orbital space operations. The initiative aligns with broader efforts to enhance accessibility to in-space manufacturing and research.

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Earthquake Swarm Near Santorini Triggers Emergency Response from Greek Authorities

Greek authorities have responded to an intensifying earthquake swarm near Santorini by closing schools and deploying emergency teams. The tremors, which began last week, have been growing in frequency and magnitude, raising concerns over potential stronger quakes in the region. While experts have ruled out immediate volcanic activity, the situation remains unpredictable due to the swarm’s unusual characteristics. The most powerful tremor recorded so far was a magnitude 5 earthquake, striking approximately 34 kilometres northeast of Santorini. The event occurred at 2:27 p.m. local time, as per the University of Athens’ earthquake monitoring system.

Seismic Activity Driven by Faults, Not Volcanic Unrest

According to reports, the ongoing tremors are attributed to fault movement rather than volcanic activity. Santorini, positioned on the Aegean Sea’s tectonic boundary, sits on the exposed section of a submerged volcano known as the Santorini caldera. David Pyle, Professor of Earth Sciences at the University of Oxford, told Live Science that the quakes are likely caused by fault lines shifting rather than magma activity. He described the swarm as unusual, highlighting the challenge of predicting future developments due to its underwater location.

Historical Earthquake Swarms and Regional Tectonics

The Aegean region experiences significant seismic activity due to the African plate moving beneath the Eurasian plate. Similar earthquake swarms have been recorded in the past, including a 2011-2012 event linked to magma movement beneath Santorini. However, the current swarm appears more extensive and is concentrated outside the Santorini caldera. Most tremors have been recorded between the underwater Kolumbo volcano and Anydros Island.

Kolumbo, last erupting in 1650, previously triggered a tsunami that affected nearby islands. While researchers remain uncertain about a direct link between current tectonic activity and potential volcanic unrest, ongoing monitoring continues to assess the evolving situation.

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Microplastics Found in Human Brain Tissue, Study Shows Rising Levels

Tiny plastic particles have been found in human brain tissue, raising concerns over their impact on health. Scientists have detected a significant increase in microplastics and nanoplastics (MNPs) in the brain over the past decades. The particles, commonly present in air, water, and food, have now been identified within human tissue, challenging previous assumptions about the brain’s protective barriers. Researchers are working to understand the long-term consequences of this plastic infiltration.

Rising Plastic Levels in Brain Tissue

According to the study published in Nature Medicine, 91 brain samples collected from individuals who died between 1997 and 2024 were analysed. Reports indicate a 50 percent increase in MNP concentrations from 2016 to 2024, with median levels rising from 3,345 micrograms per gram to 4,917 micrograms per gram. Andrew West, a neuroscientist at Duke University, told Science News that the sheer quantity of plastic detected was unexpected, stating that he didn’t believe it until he saw all the data.

Unexpected Particle Shapes and Sources

Findings suggest that the plastic particles are not uniform. Many were thin, sharp fragments rather than the engineered beads often studied in labs. Richard Thompson, a microplastic pollution expert at the University of Plymouth, told Science News that these plastics originate from everyday products such as grocery bags and bottles. Polystyrene, frequently used in medical and food industries, was found in lower amounts compared to polyethylene.

Higher MNP levels were found in the brains of 12 individuals diagnosed with dementia, but researchers have not confirmed a direct causal link. Some scientists speculate that neurological changes associated with dementia may increase plastic accumulation. Phoebe Stapleton, a toxicologist at Rutgers University, told Nature Medicine that further research is required to understand the biological impact, stating, that the next steps will be to understand what they are doing in the brain and how the body responds to them.

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Blue Origin’s New Shepard NS-29 Conducts First Lunar Gravity Simulation

A significant milestone in suborbital spaceflight was achieved by Blue Origin with the launch of its uncrewed NS-29 mission. The New Shepard rocket lifted off from the company’s West Texas facility on February 4 at 11 a.m. EST, following a week-long delay caused by adverse weather conditions and a technical issue in the rocket’s avionics system. The booster and capsule both returned to Earth successfully, though one of the capsule’s three parachutes did not fully deploy. Blue Origin stated during the live broadcast that the capsule was engineered to land safely with fewer than three parachutes.

Lunar Gravity Simulated for Research Payloads

According to reports, the NS-29 mission introduced a lunar gravity simulation for the first time using the New Shepard vehicle. The capsule achieved this by rotating approximately 11 times per minute for a duration of two minutes, a manoeuvre facilitated by its reaction-control thrusters. The mission carried 30 research payloads, with 29 focused on lunar-related technologies. Blue Origin outlined six key research areas, including in-situ resource utilisation, dust mitigation, advanced habitation systems, sensors and instrumentation, small spacecraft technologies, and entry, descent, and landing systems.

NASA-Supported Research Aboard the Flight

More than half of the payloads were backed by NASA’s Flight Opportunities Program. The U.S. space agency is engaged in efforts to establish a long-term human presence on and around the Moon through the Artemis programme. A NASA experiment named the Electrostatic Dust Lofting project examined how lunar dust becomes electrically charged and lifted under ultraviolet light exposure. Another NASA-supported study, the Lunar-g Combustion Investigation, explored fire behaviour under the Moon’s gravity conditions to enhance safety measures for future lunar habitats.

Future Applications of Gravity Simulation

In an X(formerly Twitter) post, Blue Origin Chief Executive Officer Dave Limp stated that this capability provides NASA and other lunar technology developers with a cost-effective method to conduct research. He added that New Shepard’s gravity simulation could be adapted for Mars and other celestial bodies, expanding its potential for future space exploration research.

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7,000-Year-Old Arrow Poison Found in South Africa, Shows Ancient Hunting Skills

A 7,000-year-old femur bone belonging to an antelope, discovered in a South African cave, has revealed the earliest confirmed use of a multi-component arrow poison. Three modified bone arrowheads were found embedded within the marrow cavity, and a recent scientific analysis has identified a mixture of plant-based toxins. This discovery provides new insight into the pharmacological knowledge and hunting practices of early humans, highlighting the complexity of their technological advancements and understanding of toxic substances.

Scientific Analysis of the Poisonous Compound

According to the reports published in The Conversation, Justin Bradfield, Associate professor at University of Johannesburg along with other researchers examined the femur using micro-CT imaging. The sediment-like substance inside the marrow cavity was found to be foreign matter rather than natural deposits. Chemical analysis confirmed the presence of digitoxin and strophanthidin, toxic cardiac glycosides that disrupt heart function. Ricinoleic acid, a derivative of ricin, was also detected, suggesting the use of multiple plant sources to create a potent poison.

Implications for Ancient Trade and Knowledge Systems

As per the research, the plants containing these toxic compounds are not naturally found near Kruger Cave, where the femur was originally discovered. No remains of these plants have been identified in previous archaeobotanical studies of the region. This suggests that early humans either travelled long distances to acquire these materials or engaged in an organised trade network for toxic plant ingredients. Such findings highlight the extensive knowledge early societies had regarding medicinal and toxic plants and their application in hunting strategies.

Historical Context of Poison Use in Hunting

Previous evidence of poison use dates back approximately 60,000 years, coinciding with the development of projectile hunting technology in Africa. While chemical verification of such early poison use remains unconfirmed, the newly analysed femur provides the first concrete proof of a deliberately mixed poison for arrows. The application of plant-based toxins to hunting weapons marks a significant evolutionary step in the efficiency of ancient hunting techniques, demonstrating a sophisticated level of planning and knowledge transfer among early human groups.

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Compact Neutrino Detector Successfully Identifies Antineutrinos at Nuclear Reactor

A compact neutrino detector has successfully identified antineutrinos at a nuclear power plant, marking a significant advancement in particle physics. Unlike conventional detectors that require massive infrastructure, this device weighs less than three kilograms. Despite its size, it effectively detected antineutrinos emitted from a nuclear reactor in Leibstadt, Switzerland. The experiment, which lasted 119 days, involved a detector composed of germanium crystals. Around 400 antineutrinos were recorded, aligning with theoretical predictions. Scientists believe this achievement could lead to improved testing of physics theories and potential applications in nuclear monitoring.

Study Findings and Expert Insights

According to a study submitted to arXiv on January 9, the experiment relied on a specific interaction where neutrinos and antineutrinos scatter off atomic nuclear. This phenomenon, which was first observed in 2017, enables smaller detectors to function effectively. Kate Scholberg, a neutrino physicist at Duke University, told Science News that the accomplishment is significant, as researchers have attempted similar feats for decades. She highlighted the simplicity of the interaction, comparing it to a gentle push rather than a complex nuclear reaction.

Christian Buck, a physicist at the Max Planck Institute for Nuclear Physics and co-author of the study, told Science News that this development opens a new avenue in neutrino physics. He noted that the interaction’s clean nature could help identify undiscovered particles or unexpected magnetic properties in neutrinos.

Potential Applications and Challenges

Physicists suggest that such detectors could play a role in monitoring nuclear reactors. The ability to detect antineutrinos could provide insights into reactor activity, including plutonium production, which has implications for nuclear security. However, challenges remain. Jonathan Link, a neutrino physicist at Virginia Tech, told Science News that while the technique is promising, it is still a difficult approach. The detector, despite its small size, requires shielding to eliminate background noise, limiting its portability.

This experiment also helps clarify past findings. In 2022, a similar claim of reactor antineutrinos scattering off nuclei was made, but inconsistencies with established theories led to controversy. Buck stated that the new study rules out the validity of those earlier results. With ongoing research, the field continues to evolve, potentially leading to further discoveries in particle physics.

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NASA Finalises Crew for Axiom Space’s Fourth Private Astronaut Mission in 2025

NASA and its international collaborators have finalised the crew for Axiom Space’s fourth private astronaut mission, set to launch aboard a SpaceX Dragon spacecraft no earlier than spring 2025. The mission, departing from NASA’s Kennedy Space Center in Florida, will see four astronauts spending up to 14 days aboard the International Space Station (ISS). The crew includes former NASA astronaut and Axiom Space’s director of human spaceflight Peggy Whitson as commander, ISRO astronaut Shubhanshu Shukla as pilot, and mission specialists Sławosz Uznański-Wiśniewski from the European Space Agency (ESA) and Tibor Kapu from Hungary.

Private Astronaut Missions Expand Space Access

According to NASA’s International Space Station Program Manager Dana Weigel, private astronaut missions are contributing to advancements in low Earth orbit operations. Weigel said that these missions are helping pave the way for commercial space activities while increasing accessibility to microgravity research. This mission will mark the first time an ISRO astronaut will board the ISS as part of a joint effort between NASA and the Indian space agency. It will also be the first ISS stay for astronauts from Poland and Hungary.

Axiom Space’s Growing Role in Private Spaceflight

As reported, Axiom Space has been steadily expanding its private spaceflight program since its inaugural mission in April 2022. Each mission has varied in duration, with the most recent, Axiom Mission 3, remaining docked at the ISS for 18 days in January 2024. Whitson, who also commanded Axiom Mission 2 in May 2023, highlighted the significance of international partnerships in commercial spaceflight, stating that each mission brings new opportunities for participating nations.

Future of Low Earth Orbit Operations

NASA’s long-term objective involves fostering a sustainable commercial space economy, allowing the agency to focus resources on deep space exploration. The ISS continues to serve as a key testing ground for space research and technology, supporting both government-led and private-sector initiatives.