LONDON (IT BOLTWISE) – New observations from the Very Large Telescope in Chile show that conditions at the center of the Milky Way are more stable than previously thought. An international research team has found that some dusty objects draw stable orbits around the supermassive black hole Sagittarius A*. This discovery contradicts previous assumptions that these objects could be swallowed by the black hole.
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In the center of the Milky Way, where the supermassive black hole Sagittarius A* resides, conditions are apparently more stable than previously assumed. New observations with the European Southern Observatory’s (ESO) Very Large Telescope (VLT) in Chile have shown that some dusty objects are forming stable orbits around the black hole. This discovery contradicts previous assumptions that these objects could be on the verge of being swallowed by the black hole.
Under the direction of private lecturer Dr. Florian Peißker from the University of Cologne, an international research team used the new observation instrument ERIS (Enhanced Resolution Imager and Spectrograph) to analyze the movements of these objects. In particular, the object G2, which was long thought to be a pure dust cloud, now shows a stable orbit, suggesting that there is a star inside the dust cloud. This finding challenges previous ideas about the destructive nature of the center of our galaxy.
Another remarkable object is the binary star system D9, which remains stable despite the enormous tidal forces of the black hole. It is the first known binary star system to be observed so close to a supermassive black hole. The theoretical possibility that the stars involved could merge into a single, more massive star has not yet been confirmed by the ERIS data. Objects X3 and X7 also show stable orbits, suggesting that the region is less fragile than previously thought.
These results open new perspectives for studying the interactions between black holes and stars. Dr. Peißker emphasizes that Sagittarius A* is less destructive than was long thought and that the center of our galaxy represents an ideal laboratory for researching these phenomena. The study, published in the journal Astronomy & Astrophysics, shows that the processes at the center of the Milky Way are more complex than previously thought. Future observations with ERIS and the upcoming Extremely Large Telescope will help further track the evolution of these objects and understand how stars can survive even in the extreme regions of the universe.
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