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A team of researchers has observed an ultra-diffuse galaxy, FCC 224, uncovering an unusual system of globular clusters. The galaxy, located in the Fornax cluster approximately 65 million light-years away, has been found to host luminous and overmassive globular clusters. The study, conducted using the Hubble Space Telescope (HST) and supported by spectroscopic data from the Keck Cosmic Web Imager (KCWI), has provided insights into the formation and evolution of this galaxy and its star clusters. The findings indicate a single-burst star formation history, with the globular clusters displaying unique characteristics in terms of mass, size, and brightness distribution.

Overmassive Globular Cluster System Identified

According to the study published on the arXiv pre-print server, FCC 224 is a quiescent ultra-diffuse galaxy estimated to be around 10 billion years old. It has a major axis effective radius of roughly 6,160 light-years and a stellar mass of approximately 200 million solar masses. Observations have revealed that the galaxy hosts 12 exceptionally bright globular clusters, with some showing absolute magnitudes around -9.0 mag. The total mass of these clusters is estimated to be 3.8 million solar masses, accounting for nearly 2 percent of the galaxy’s stellar mass, which is significantly higher than expected for a galaxy of this size.

Distinctive Features of the Globular Clusters

As reported by phys.org, the study found that the globular clusters in FCC 224 closely resemble the galaxy’s diffuse starlight, exhibiting a narrow color range and lacking a significant color gradient. This suggests that the galaxy underwent a single, intense star formation period. Researchers also noted that these clusters have relatively small sizes, with half-light radii ranging between 7.8 and 15.6 light-years. The globular cluster population appears to be radially mass-segregated, with brighter clusters concentrated toward the galaxy’s center.

Implications and Future Research

Findings from the study indicate that FCC 224 possesses an unusual globular cluster system with characteristics that challenge conventional expectations. The research team has suggested that further theoretical studies will be needed to explain the origins of these distinctive properties and the role they play in the galaxy’s evolution.

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New Study Finds Active Lunar Tectonics, Challenges Moon’s Dormancy



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Solar System’s Journey Through Orion Complex May Have Altered Earth’s Climate

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Solar System’s Journey Through Orion Complex May Have Altered Earth’s Climate

The movement of the solar system through the Orion star-forming complex around 14 million years ago may have influenced Earth’s climate, according to scientists. This dense region of space, part of the Radcliffe Wave galactic structure, could have compressed the heliosphere—the protective shield surrounding the solar system—while increasing interstellar dust reaching Earth. Researchers suggest that this influx of cosmic dust might have left traces in geological records, potentially linking galactic activity to past climate changes.

Solar System’s Passage Through the Radcliffe Wave

According to the study published in Astronomy & Astrophysics, an international research team led by the University of Vienna used data from the European Space Agency’s Gaia mission and spectroscopic observations to determine that the solar system moved through the Radcliffe Wave in the Orion constellation between 18.2 and 11.5 million years ago. The most probable period was estimated between 14.8 and 12.4 million years ago. João Alves, Professor of Astrophysics at the University of Vienna and co-author of the study, stated to Phys.org, that this research builds on prior findings regarding the Radcliffe Wave. This structure, made up of interconnected star-forming regions, includes the Orion complex, which the sun is believed to have passed through.

Potential Impact on Earth’s Climate

The study suggests that the increased presence of interstellar dust may have influenced Earth’s atmosphere. Efrem Maconi, lead author and doctoral student at the University of Vienna, said that this dust might have contained traces of radioactive elements from supernovae, which could be detected in geological records using advanced technology in the future.

The solar system’s passage aligns with the Middle Miocene Climate Transition, a period marked by a shift from a warmer, variable climate to a cooler one, leading to the development of Antarctic ice sheets. Scientists highlight that while interstellar dust could have played a role, the dominant factor in this climate change was a long-term decrease in atmospheric carbon dioxide levels.

Not Comparable to Human-Induced Climate Change

Maconi noted that while interstellar dust could have contributed to past climate shifts, the amount required for significant change would need to be much greater than current data suggests. The Middle Miocene Climate Transition unfolded over hundreds of thousands of years, unlike modern climate change, which is occurring rapidly due to human activities

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Ancient DNA Sheds Light on the Diverse Genetic Origins of the European Huns

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Ancient DNA Sheds Light on the Diverse Genetic Origins of the European Huns

The origins of the Huns, a nomadic group that played a crucial role in the decline of the Roman Empire, have long remained uncertain. Recent DNA analysis of ancient skeletal remains has provided fresh insights into their ancestry, revealing a diverse genetic makeup rather than a singular point of origin. According to reports, researchers examined remains from individuals buried between the fourth and sixth centuries and found genetic links spanning Central Asia and Eastern Europe. These findings indicate that the Huns were not a homogenous group but a population shaped by centuries of migration and cultural interactions.

Genetic Analysis Reveals Diverse Ancestry

According to the study published in PNAS, a team led by Guido Gnecchi-Ruscone, an archaeogeneticist at the Max Planck Institute for Evolutionary Anthropology, analysed the genomes of 370 individuals. The research aimed to trace connections between European Huns and earlier nomadic groups, including the Xiongnu, whose empire thrived in Mongolia between 200 B.C. and A.D. 100. While certain Hun individuals exhibited direct genetic links to the Xiongnu elite, most carried varying degrees of Northeast Asian ancestry, underscoring a complex history of intermingling.

Connections Across the Eurasian Steppe

Using a technique called identity by descent (IBD) segment sharing, the researchers identified genetic ties across multiple regions over several centuries. Their findings suggested that trans-Eurasian relationships were maintained across generations. While high-status Xiongnu burials in Mongolia showed direct descendants among the European Huns, the study concluded that no large-scale migration of Xiongnu populations into Europe took place.

Insights from an Elite Hun Burial

A burial site in Pusztataskony, Hungary, yielded the remains of a Hun woman with an elongated skull, buried alongside gold earrings. Gnecchi-Ruscone told Live Science that this individual carried genetic markers linking her to the Xiongnu elite, suggesting that skull modification, a notable cultural practice, may have been passed down through generations. The study reinforces the view that the European Huns were a culturally and genetically diverse group shaped by centuries of movement and integration rather than a single migratory event.

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NASA’s IM-2 Mission Brings Ice Mining, Mobile Robots, and More on Moon



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NASA’s IM-2 Mission Brings Ice Mining, Mobile Robots, and More on Moon

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NASA’s IM-2 Mission Brings Ice Mining, Mobile Robots, and More on Moon

NASA is preparing to send advanced technologies to the Moon through Intuitive Machines’ second lunar delivery under the Commercial Lunar Payload Services (CLPS) initiative. The mission, part of the Artemis programme, aims to establish a sustainable human presence on the Moon. A range of scientific instruments and communication systems will be tested on the lunar surface. The launch window for Intuitive Machines’ second CLPS mission, IM-2, is scheduled to open on 26 February from Launch Complex 39A at NASA’s Kennedy Space Center. The Nova-C class lander will carry key technology payloads, including a drill, mass spectrometer, a cellular network, and a drone for terrain exploration.

Lunar South Pole Exploration

As reported, the landing site for IM-2 has been selected based on data from NASA’s Lunar Reconnaissance Orbiter. Located in the South Pole region, the site offers a relatively flat terrain, meeting the criteria for a safe landing. The area is of particular interest due to its potential for in-situ resource utilisation, which could support future lunar missions.

Demonstration of New Technologies

According to NASA’s Space Technology Mission Directorate, the Polar Resources Ice Mining Experiment-1 (PRIME-1) will be tested as part of the mission. PRIME-1 includes a drill and a mass spectrometer designed to search for water ice and other resources beneath the lunar surface. Data gathered from this experiment will assist in future space exploration efforts by providing insight into potential resource extraction for fuel and oxygen production.

Mobile Robotics on the Moon

Two technology demonstrations will be deployed near the lander under NASA’s Tipping Point initiative. Intuitive Machines has developed a small drone, named Grace, which will conduct high-resolution surveys of the lunar terrain. The drone is designed to navigate steep inclines, craters, and other challenging obstacles, helping scientists study permanently shadowed regions that cannot be accessed by traditional rovers.

Lunar Surface Communication System

A communication system developed by Nokia Bell Labs will be tested to establish a lunar cellular network. The system will enable communication between the lander, a Lunar Outpost rover, and the Grace drone. It will be the first demonstration of cellular-based connectivity on the Moon, with potential applications for future crewed missions and robotic exploration.

Collaboration for Lunar Exploration

NASA is working alongside several U.S. companies to deliver scientific and technological advancements to the lunar surface. The Space Technology Mission Directorate has integrated multiple research and development efforts to support future Moon missions. The combination of CLPS and Tipping Point initiatives aims to advance exploration capabilities, benefiting NASA and the broader space industry.

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