Astronomers have identified a potential new class of stellar objects called 'black hole stars' or 'quasi-stars.'
The discovery originated from an investigation into 'little red dots' appearing in deep-space images.
Researchers used the James Webb Space Telescope to analyze these dense, mysterious red objects.
One specific object, MoM-BH*-1, is located in the constellation Cetus.
This object is approximately 100 billion times brighter than a typical star.
Unlike standard stars, these objects are powered by supermassive black holes rather than nuclear fusion.
The black hole's accretion disk is estimated to be as large as our solar system.
Lead researcher Rohan Naidu suggests these findings may confirm the existence of theoretical objects from the early universe.
The discovery may solve a lingering mystery regarding the nature of dense red dots captured in infrared data.
The study detailing these findings was published in the journal Nature.
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Reporting from different sources agrees that astronomers using the James Webb Space Telescope have identified a potential new class of objects known as quasi-stars, which are powered by black hole accretion rather than nuclear fusion.
The identification remains a probable discovery rather than a confirmed fact, and further peer review or observation of additional 'little red dots' could refine the classification of these objects.
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Neutral reporting focuses on the factual details of the study published in the journal Nature regarding 'black hole stars.' Reports describe the specific characteristics of these objects, such as their extreme brightness and the scale of their accretion disks compared to the solar system. The coverage maintains a steady tone, attributing the findings to the research team led by Rohan Naidu. It positions the discovery as a possible explanation for previously unidentified signals in deep-space photography.
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Researchers using the James Webb Space Telescope report they have likely identified a new class of stellar objects known as 'black hole stars' or 'quasi-stars.' This discovery follows an investigation into 'little red dots' (LRDs) that appeared in deep-space images but did not match known star or galaxy profiles. Lead researcher Rohan Naidu states that these objects, particularly one named MoM-BH*-1, are powered by supermassive black holes rather than nuclear fusion, with accretion disks as large as our solar system.
A study published in Nature reports the possible discovery of 'black hole stars,' potentially solving a mystery involving dense red dots captured by the James Webb Space Telescope. Astronomers, led by Rohan Naidu, analyzed a specific object in the constellation Cetus that is 100 billion times brighter than a typical star. The report notes these 'quasi-stars' are powered by massive black hole accretion disks rather than nuclear fusion. This finding may confirm the existence of a theoretical stellar object from the early universe.