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Ripples in spacetime, known as gravitational waves, are being used to determine the ancestry of black holes. These waves, first theorised by Albert Einstein, are offering insights into how black holes form and evolve. Scientists have uncovered that the spin of a black hole can indicate whether it originated from repeated mergers in densely packed star clusters. This finding has the potential to transform our understanding of black hole formation and growth.

According to a study published in Physical Review Letters, a team of researchers led by Fabio Antonini from Cardiff University’s School of Physics and Astronomy examined 69 gravitational wave events. The findings suggest that when a black hole reaches a certain mass, its spin undergoes a shift. This change aligns with models that propose black holes grow through sequential mergers in star clusters.

As reported by Live Science, Isobel Romero-Shaw, a researcher at the University of Cambridge, stated that the study provides a data-driven method to identify a black hole’s origin. The spin of high-mass black holes was found to be a strong indicator of their formation in regions where smaller black holes frequently collide and merge.

Gravitational Waves as Cosmic Identifiers

Gravitational waves are generated when massive objects, such as black holes, accelerate through space. The Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo Observatory have detected multiple signals from black hole mergers since 2015, confirming Einstein’s predictions. The study highlights that gravitational waves can be read like a cosmic birth certificate, revealing the formation history of black holes.

Thomas Callister, a researcher at the University of Chicago, mentioned that the results will aid in refining computer simulations of black hole formation. With upcoming observatories such as the Einstein Telescope and the Laser Interferometer Space Antenna (LISA), further discoveries are anticipated in the field of black hole research.

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

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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.

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Reef Sharks in French Polynesia Suffer Health Consequences From Feeding

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Reef Sharks in French Polynesia Suffer Health Consequences From Feeding

Blacktip reef sharks in French Polynesia are experiencing adverse effects on their health due to frequent exposure to low-quality food scraps from tourists. Reports indicate that these sharks, commonly found in the waters around Mo’orea, are being fed everything from frozen squid to human leftovers. This feeding practice has led to significant changes in their metabolism, movement, and reproductive patterns. Concerns have been raised regarding the long-term consequences on the species, classified as “vulnerable” by the International Union for Conservation of Nature.

Shark Feeding Practices Impact Metabolism

According to a study published in Animal Conservation, research conducted by marine behavioural ecologist Johann Mourier at the University of Montpellier and his team examined the metabolic and reproductive changes in these sharks. Over a three-year period, blood samples from 117 blacktip reef sharks across 17 sites—five of which were known for frequent tourist-driven feeding—were analysed. The results indicated that sharks at feeding sites displayed lower red blood cell levels, a marker of overall health. Blood glucose levels in females were also found to be lower, suggesting that the scraps provided lacked adequate nutritional value compared to their natural diet.

Reproductive Changes Observed in Feeding Site Sharks

Data from the study also highlighted notable shifts in reproductive hormone levels. Males at feeding sites exhibited increased testosterone levels, potentially due to heightened competition over food. Female sharks at non-feeding sites were consistently pregnant and exhibited triple the estrogen levels compared to those at feeding locations, where not all females carried pups. Scientists suggest that an unpredictable and nutritionally insufficient diet may be impacting reproductive success, ultimately affecting population sustainability.

Calls for Better Regulation of Shark Feeding

In an interview with Science News, Natascha Wosnick, a biologist at the Cape Eleuthera Institute, stated that unregulated shark feeding can alter natural behaviour and compromise welfare. Concerns extend beyond Mo’orea, as other species, such as nurse sharks in the Bahamas, may face similar risks due to increased energy expenditure linked to human-provided food. Experts suggest implementing regulations on the types of food offered to sharks, particularly during breeding seasons, to mitigate the negative impact on their health and reproduction.

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JWST Detects Unexpectedly Massive Black Holes in the Early Universe

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JWST Detects Unexpectedly Massive Black Holes in the Early Universe

Distant supermassive black holes, far larger than expected, have been detected in the early universe. Observations using the James Webb Space Telescope (JWST) indicate that these black holes hold a mass nearly 10 percent of their host galaxy’s stellar mass, a stark contrast to the 0.01 percent ratio observed in modern galaxies. This anomaly has raised new questions regarding the rapid formation and growth of black holes in the early stages of cosmic history.

Research Findings on Black Hole Growth

According to the study published in the paper repository arXiv, a team led by Jorryt Matthee, a scientist at the Institute of Science and Technology Austria (ISTA), analysed data from JWST. The findings suggest that some early galaxies, identified as “little red dot” galaxies, contain supermassive black holes with masses nearly 1,000 times higher than previously estimated norms. These galaxies, observed from a time when the universe was around 1.5 billion years old, exhibit an unusual balance between stellar mass and black hole mass, challenging existing growth models.

Implications for Early Universe Cosmology

As per reports, these small galaxies exhibit a red hue due to the presence of an accretion disk surrounding the black holes. The intense gravitational pull allows for rapid matter consumption, potentially accelerating black hole expansion beyond current theoretical expectations. The study indicates that the density of surrounding gas in the early universe may have facilitated this extraordinary growth. Matthee stated to Space.com that these findings provide a promising avenue for further understanding black hole evolution.

Further Observations Needed

Researchers emphasise the need for additional studies to confirm whether measurement errors or selection bias contributed to these unexpected results. Ongoing observations with JWST aim to refine the understanding of early black hole formation, shedding light on whether these supermassive black holes were nurtured by dense galactic environments or formed through alternative mechanisms, such as direct gas collapse. The findings suggest that black holes and star formation are more interconnected than previously thought, prompting a reassessment of cosmic evolution models.

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