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James Webb Telescope has successfully observed the farthest known active supermassive black hole to date.

In this groundbreaking endeavor, researchers have now uncovered the most distant active supermassive black hole ever observed.

With its unprecedented capabilities, the James Webb Space Telescope has revolutionized the field of astronomy, enabling scientists to explore celestial phenomena that were previously beyond their reach. One such remarkable discovery, as part of the Cosmic Evolution Early Release Science (CEERS) Survey, involves the observation of ancient galaxies that defy theoretical expectations.

 

Leveraging the near- and mid-infrared imagery captured by the James Webb Telescope, scientists successfully identified a supermassive black hole residing within a galaxy named CEERS 1019. Astonishingly, they determined that this black hole formed a mere 570 million years after the Big Bang and possesses a mass approximately 9 million times that of our Sun. Furthermore, the telescope’s data unveiled a fascinating revelation—the black hole exhibits voracious gas consumption and promotes the birth of new stars through its energetic processes.

According to Jeyhan Kartaltepe, a member of the CEERS team from the Rochester Institute of Technology in New York, the heightened activity observed in the black hole of CEERS 1019 may be attributed, at least in part, to a merger between galaxies.

This galactic collision potentially contributes to the acceleration of gas feeding the black hole, consequently fostering an environment conducive to enhanced star formation. In the image provided below, CEERS 1019 manifests as three distinct luminous clumps, further exemplifying the intriguing nature of this cosmic phenomenon.

 

In contrast to previously identified active supermassive black holes, the black hole found within CEERS 1019 boasts a comparatively modest mass of 9 million solar masses.
Typically, these astronomical entities exhibit masses exceeding 1 billion times that of our Sun, rendering them significantly brighter and more detectable. In terms of scale, the CEERS 1019 black hole bears a closer resemblance to the black hole residing at the core of our own galaxy, with a mass estimated at approximately 4.6 million times that of the Sun.
Confirmation of the existence of smaller black holes in the early universe has been a long-standing expectation among scientists, a fact acknowledged by NASA. However, the recent operational status of the James Webb Space Telescope has finally provided the means to substantiate this hypothesis.
In a remarkable turn of events, the CEERS Survey team, utilizing data from the telescope, has discovered two additional ancient yet relatively small black holes. The first, known as CEERS 746, emerged approximately 1 billion years after the Big Bang, while the second, designated as CEERS 2782, has been in existence since roughly 1.1 billion years after this monumental cosmic event.
These findings contribute to our understanding of the cosmic landscape and shed light on the prevalence of smaller black holes during the early stages of the universe.
When observed through alternative instruments, these black holes exhibit the appearance of typical galaxies engaged in the process of star formation.
astronomers are actively examining additional black holes discovered using the data acquired by the James Webb Telescope. As a result, it is possible that the record held by CEERS 1019 for being the most distant active supermassive black hole might be surpassed in the near future. The ongoing exploration of these distant cosmic entities promises exciting prospects for uncovering even more intriguing discoveries.