2023-05-18 01:44:40
Delving into the vast abysses of the universe, we find endless cosmic wonders that arouse our curiosity and wonder. Among these enigmatic wonders are hidden the mysterious “heavenly monsters”, fascinating stellar phenomena that defy the relentless passage of time and reveal a captivating glimpse into the oldest memories of our cosmic past.
What are celestial monsters?
In the depths of the universe there are mysterious groupings of stars called ‘sky monsters’, also known as globular clusters. These enigmatic clusters are dense spheres stretching up to 100 light-years across, containing millions of stars that shine brightly in the sky.
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This was the discovery of the celestial monsters
Recently, a group of astronomers has made an amazing discovery that changes our understanding of early star formation. Using advanced chemical analysis techniques, they have detected a chemical trail of massive stars in globular protoclusters, which were born just 440 million years after the Big Bang. This finding presents unique chemical anomalies not found in any other stellar population and challenges our preconceptions about early star formation.
This milestone in astronomical research would not have been possible without the hard work of the team of scientists from the Universities of Geneva and Barcelona, together with the Paris Institute of Astrophysics (CNRS and the Sorbonne University). This discovery undoubtedly brings us closer than ever to discovering the deepest secrets of the universe and its origins.
What are the characteristics of celestial monsters?
He James Webb Space Telescope has revealed amazing clues about the existence of these unique stars. Globular clusters, with a mass between 5,000 and 10,000 times that of the Sun, harbor a core temperature five times hotter.
These clusters are 10 to 13 billion years old, but the superstars that make them up have died out prematurely, with a maximum lifetime of just two million years.
Scientists have found that these clusters have exceptionally high nitrogen ratios and significant stellar density. This can only be explained by the combustion of hydrogen at extremely high temperatures, which are only achieved in the core of supermassive stars.
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