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A pair of stars, designated D9, has been identified orbiting Sagittarius A, the supermassive black hole at the core of the Milky Way, according to a study published in Nature Communications. This is the first time a binary star system has been detected in close proximity to such an immense gravitational force. The finding was made using data from the European Southern Observatory’s (ESO) Very Large Telescope (VLT). The binary system, described as a young stellar pair, was observed in the S cluster, a densely packed region of stars and other objects near Sagittarius A. D9’s existence offers critical insights into how stars and their systems can survive in environments characterised by extreme gravitational forces.

The lead researcher, Florian Peißker from the University of Cologne, stated in Nature Communications that this discovery challenges previous assumptions about the hostile nature of black hole surroundings, stating that black holes may not be as destructive as we thought.

Significance of the Binary System

Reportedly, binary star systems, which involve two stars orbiting each other, are commonly found across the universe. However, their presence near a supermassive black hole was previously thought unlikely due to the destabilising effects of the black hole’s intense gravity. D9, believed to be about 2.7 million years old, is expected to merge into a single star within the next one million years due to these forces.

According to Michal Zajaček, a researcher at Masaryk University, in a statement, gas and dust surrounding D9 suggest the binary system formed near the black hole, defying long-standing theories about star formation in such conditions.

Implications for Future Research

The discovery was made using a combination of data from ESO’s SINFONI and ERIS instruments, revealing recurring patterns in D9’s light spectrum. Researchers suggest this finding could enhance understanding of other enigmatic objects in the S cluster, including the so-called G objects. With advancements in instruments like ESO’s Extremely Large Telescope, further exploration of this unique environment is anticipated.

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Boeing Starliner Astronauts’ Return Delayed Until March 2025 Following SpaceX Delay

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Boeing Starliner Astronauts’ Return Delayed Until March 2025 Following SpaceX Delay

NASA astronauts Barry Wilmore and Sunita Williams, who embarked on Boeing’s Starliner spacecraft in June 2024, will now extend their stay on the International Space Station (ISS) until March 2025. The return, initially set for February, has been postponed due to a delay in SpaceX’s Crew-10 mission, NASA confirmed on December 17. The decision was attributed to ongoing work on a new Crew Dragon spacecraft, as per official statements.

Crew-10’s Revised Timeline

Crew-10, which will carry NASA astronauts Anne McClain and Nichole Ayers, along with JAXA’s Takuya Onishi and Roscosmos cosmonaut Kirill Peskov, is now scheduled for a late-March launch aboard a SpaceX Falcon 9 rocket. This adjustment pushes back Crew-9’s return, leaving Wilmore and Williams aboard the ISS for approximately nine months instead of the originally planned 10-day mission.

The delay arose as SpaceX completes its latest Crew Dragon capsule, which is expected to arrive at NASA’s Kennedy Space Center in January 2025 for final processing and testing. Steve Stich, Manager of NASA’s Commercial Crew Program, stated in the official release that fabricating and integrating a new spacecraft requires meticulous attention to detail.

Unexpected Mission Extension

Wilmore and Williams were integrated into the Crew-9 mission after their Starliner capsule, slated for an initial 10-day journey, encountered technical challenges. NASA’s Nick Hague and cosmonaut Aleksandr Gorbunov, who launched aboard the Crew Dragon Freedom in September 2024, were joined by Wilmore and Williams during their prolonged mission.

This is not unprecedented; astronauts have previously faced extended ISS missions. Notable examples include Scott Kelly’s year-long twin study in 2015-2016 and Frank Rubio’s 365-day stay following complications with a Soyuz spacecraft.

SpaceX’s expanding Crew Dragon fleet is expected to enhance mission flexibility, allowing NASA greater adaptability in managing ISS operations and addressing unforeseen delays.

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James Webb and Chandra Capture Images of Star Clusters in Distant Galaxies

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James Webb and Chandra Capture Images of Star Clusters in Distant Galaxies

A striking new image has been captured near the edge of the Small Magellanic Cloud, a galaxy located approximately 200,000 light-years from Earth. The image, highlighting the star cluster NGC 602, was produced using data from the James Webb Space Telescope (NASA/ESA/CSA) and NASA’s Chandra X-ray Observatory. Reports suggest the cluster resides in an environment reminiscent of the early universe, characterised by low concentrations of heavy elements. Dense dust clouds and ionised gas within the region point to active star formation, offering insights into stellar creation under conditions vastly different from those in the solar neighbourhood.

A Stellar Wreath Shaped by Dust and Light

Reportedly, the Webb Telescope’s data, which includes near-infrared and mid-infrared imaging, reveals a wreath-like structure encircling NGC 602. This ring of dense dust clouds is displayed in shades of green, blue, orange and yellow, while Chandra’s X-ray observations add vibrant red tones, signifying high-energy radiation from young, massive stars. It has been indicated in reports that these stars emit powerful winds, illuminating the surrounding material. Lower-mass stars contribute an extended glow, combining to create a festive cosmic image resembling a holiday wreath.

Christmas Tree Cluster Viewed with New Precision

According to sources, another cluster, NGC 2264, has been presented in a recently released composite image. This cluster, situated roughly 2,500 light-years away, features young stars estimated to be between one and five million years old. Chandra X-ray data in red, purple, blue, and white has been blended with optical observations from astrophotographer Michael Clow, captured in November 2024. The imagery reveals a cone-shaped structure reminiscent of a Christmas tree, dotted with starlight.

Both observatories are managed by NASA’s Marshall Space Flight Center, with Chandra operations overseen by the Smithsonian Astrophysical Observatory. These images continue to expand understanding of star formation across vastly different cosmic conditions.

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SWOT Satellite Reveals Key Insights on Ohio River Basin Lakes and Reservoirs

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SWOT Satellite Reveals Key Insights on Ohio River Basin Lakes and Reservoirs

Researchers have been provided with a detailed analysis of lakes and reservoirs in the Ohio River Basin through data collected by the Surface Water and Ocean Topography (SWOT) satellite. According to reports, the U.S.-European mission, a collaboration between NASA and CNES (Centre National d’Études Spatiales), has delivered critical insights into freshwater systems. Spanning an area comparable to France, the basin, which serves over 25 million residents, has been under close observation. The satellite has monitored global water heights across oceans, rivers, lakes, and reservoirs since early 2023, providing comprehensive coverage every 21 days. Its data, released earlier this year, includes water level measurements and spatial extent, offering an unparalleled understanding of water storage and movement.

Significance of High-Resolution Water Data

The information generated by SWOT is being used to calculate changes in water storage over time. As per a report by NASA, researchers can now evaluate river discharge with greater precision, enabling a clearer picture of how water moves through various stretches of rivers. Visual data for the Ohio River Basin, collected between July 2023 and November 2024, show water levels ranging from over 1,600 feet above sea level to under 330 feet, with variations marked in yellow and dark purple. These insights are expected to assist hydrologists in assessing local and watershed-wide water availability, the report further added.

Challenges in Freshwater Data Collection

Sources reveal that understanding water availability has traditionally been hindered by inconsistent data collection methods. While ground sensors and airborne surveys provide some coverage, their spatial and temporal limits necessitate additional data from satellites. However, these measurements often require integration with computer models, which have struggled to accurately represent regulated basins like the Ohio River Basin due to dam operations.

SWOT’s unified approach to measuring water levels and extent is reportedly providing a broader perspective. Colin Gleason, hydrologist and member of the SWOT science team, has stated to various publications that this data facilitates better collaboration among water managers. Researchers are still navigating the extensive data, but the potential to revolutionise water management practices has been highlighted.

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