A colossal quasar, initially misidentified as a star, is unveiled as the most luminous and rapidly expanding black hole observed, consuming daily material equivalent to a sun.
The object, known as J0529-4351, weighs between 17 billion and 19 billion solar masses and exists 12 billion light-years away, originating from a cosmic era when the universe was merely 1.5 billion years old. These black holes, formed through the collapse of massive stars, expand by voraciously consuming various celestial entities, including gas, dust, stars, planets, and other black holes.
Massive Black Hole Mistaken for a Star Is One of the Brightest, Fastest-Growing Quasars Ever Seen
Hungriest Black Hole Discovery Unveils Galactic Secrets
The hungriest black hole, situated at the heart of the quasar galaxy J0529-4351, engulfs an astounding amount of material, equivalent to a Sun's worth of gas and dust each day. This insatiable appetite propels the black hole's mass to an already colossal 17 billion Suns, making it the most voracious black hole discovered so far.
Light emitted from material heating up in voracious space-time ruptures creates active galactic nuclei (AGN), including quasars-supermassive black holes with luminous light blasts.
Initially misidentified in the 2022 Gaia spacecraft survey due to its star-like brightness, J0529-4351 is a quasar. In a paper, titled "The accretion of a solar mass per day by a 17-billion solar mass black hole" published in the journal Nature, researchers discovered J0529-4351 as a concealed quasar in ESA's Gaia survey and confirmed its identity using the Very Large Telescope (VLT) in the Atacama Desert.
Christian Wolf and a team of astronomers from the Australian National University lead the discovery, highlighting the black hole's unprecedented growth, pushing the limits of its accretion capacity.
The unique features of this cosmic entity offer scientists a rare opportunity to study the evolution of supermassive black holes. These colossal entities, millions to billions of times the Sun's mass, usually reside at the centers of galaxies, exerting gravitational dominance. Despite their prevalence, the origin of supermassive black holes, forming challenges established theories, particularly in the early universe.
The standard method of direct collapse and growth through collisions with stellar-mass black holes seems inefficient for supermassive ones. Astronomers study actively growing black holes, like those in quasars such as J0529-4351, offering insights into the feeding habits and mechanisms behind the massive accumulation of supermassive black holes.
Cosmic Mystery Spurs Telescope Tech Breakthroughs
The recent discovery of quasar J0529-4351, despite its exceptional brightness, has left astronomers perplexed. This cosmic entity, present in images from the ESO Schmidt Southern Sky Survey since 1980, went unrecognized as a quasar for years, showcasing the challenges of identification.
Identifying quasars involves sifting through vast observational data, complicated by machine-learning models that may overlook extraordinary objects like J0529-4351.
Initially mistaken for nearby stars, the quasar was eventually identified using the ANU 2.3-meter telescope at Siding Spring Observatory. Confirmation as the most luminous quasar required the advanced capabilities of the X-shooter spectrograph on ESO's VLT in the Chilean Atacama Desert.
This breakthrough discovery not only exposes the limitations of current machine-learning models but also opens avenues for further exploration with advanced instruments like the GRAVITY+ upgrade on ESO's VLT Interferometer and the upcoming Extremely Large Telescope (ELT) in the Chilean Atacama Desert.
These developments promise precise measurements of black hole masses, even at significant distances from Earth. Unraveling the mysteries of distant supermassive black holes contributes valuable insights into the early Universe and enhances understanding of galaxy formation and evolution.
RELATED ARTICLE: Powerful Black Hole Wind Observed in Distant Galaxy, Offering Insights Into Evolutionary Forces Shaping Galaxies
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