On September 18, 2025, NASA’s CHANDRA X-Ray Observatory released a report that the James Webb Space Telescope (JWST) has made landmark discoveries regarding supermassive black holes in the early universe, revealing new classes of cosmic objects and deepening the mystery of how these massive structures formed so soon after the Big Bang. JWST identified extremely distant and massive black holes, such as one nicknamed “The Cliff,” lurking in compact, very red, and unexpectedly bright galaxies now known as “Little Red Dots.” Some of these were found only 500 – 700 million years after the Big Bang, suggesting black holes with masses up to hundreds of millions of solar masses already existed in the cosmic dawn.
 
The spectrum of “The Cliff” and similar objects has led scientists to propose the existence of “black hole stars” or rapidly accreting supermassive black holes shrouded by thick cocoons of gas. These objects could illuminate the origins of today’s massive galaxies and explain ultra-fast black hole growth in the early universe. JWST observations indicate that some young galaxies host black holes disproportionately massive compared to their host galaxy’s size, breaking previously believed cosmic scaling laws.
 
One theory is the “direct collapse” model, where primordial gas clouds bypass normal star formation and collapse straight into black holes. Evidence from JWST images, such as QSO1 and UHZ1, supports this as a potential pathway for forming early supermassive black holes. Little Red Dots, intensely red and compact, become prime candidates for galaxies powered by supermassive black holes because their brightness comes from the accretion processes rather than massive star clusters.
 
These findings challenge traditional models that require stars to form and then merge to build up massive black holes over billions of years. The presence of high-mass black holes in the first billion years of the universe implies a need to revise galaxy formation and evolution theories. Follow-up studies and peer-reviewed research based on JWST data continue to refine our understanding and fuel hypotheses about the rapid growth of these cosmic giants.
 
JWST’s results mark a major leap in our knowledge of supermassive black holes, suggesting the universe’s first behemoths appeared shockingly early and under unexpected conditions.
 
References
 
​Karantha, S. (2025, September 25). The James Webb telescope may have discovered a brand new class of cosmic object: the black hole star. LiveScience.
 
Lea, R. (2024, February 28). James Webb Space Telescope finds 'extremely red' supermassive black hole growing in the early universe. SPACE.Com.
Wood, C. (2025, September 12). A Single, Naked Black Hole Rewrites the History of the Universe. Quanta Magazine.
 
(2025, September 18). NASA's Chandra Finds Black Hole With Tremendous Growth. Chandra X-Ray Observatory. https://chandra.si.edu/press/25_releases/press_091825.html
 
(2025, September 12). Are Black Hole Stars Real? Max-Planck-Gesellschaft. https://www.mpg.de/25316826/black-hole-stars

​As of September 2025, the James Webb Space Telescope has discovered and directly imaged several new "alien worlds" while also investigating the atmosphere of the potentially habitable exoplanet TRAPPIST-1e. This information reflects multiple, distinct astronomical milestones for the telescope. 
 
TRAPPIST-1e, located approximately 40 light-years away from Earth, was initially discovered by a team of astronomers headed by Michaël Gillon  using the TRAPPIST (Transiting Planets and Planetesimals Small Telescope) telescope at the La Silla Observatory in the Atacama Desert, Chile, to search for orbiting planets. The team made their observations from September - December 2015 and published its findings in the May 2016 issue of the journal Nature. Initial analyses from the James Webb Space Telescope (JWST) suggest that the Earth-sized exoplanet TRAPPIST-1e might have a nitrogen and methane atmosphere, though a bare-rock planet without an atmosphere cannot be ruled out. Scientists used the JWST's Near-Infrared Spectrograph (NIRSpec) to observe TRAPPIST-1e as it transited, or passed in front of, its star, the red dwarf TRAPPIST-1. The light from the star passing through the planet's atmosphere revealed the planet's atmospheric composition. 
 
Early data suggests two primary possibilities for TRAPPIST-1e: a bare-rock planet with no atmosphere, or one with a secondary atmosphere rich in nitrogen and potentially trace amounts of methane. The intense radiation from the active red dwarf star likely stripped away any primordial hydrogen-helium atmosphere the planet may have once had. The data strongly suggests the planet does not have a thick, hydrogen-heavy atmosphere like Jupiter, or a dense carbon dioxide-rich atmosphere like Venus. The planet's host star is highly active, producing flares and star spots that can interfere with atmospheric measurements. Researchers filtered out this stellar contamination by comparing observations of TRAPPIST-1e with those of TRAPPIST-1b, a neighbouring planet known to be a bare rock.
 
Scientists plan to observe an additional 15 transits of the planet to gather more conclusive data and determine if it truly has an atmosphere. 
 
References
Gough, E. (2025, September 14). The Exoplanet TRAPPIST-1e Takes Its Turn in the JWST’s Spotlight. Phys.Org.
 
NASA Webb Mission Team. (2025, September 8). NASA Webb Looks at Earth-Sized Habitable-Zone Exoplanets TRAPPIST-1e. NASA.
 
(2025, September 16). TRAPPIST-1e. In Wikipedia,          https://en.wikipedia.org/wiki/TRAPPIST-1e