The James Webb Space Telescope has just captured the first direct measurement of a black hole
By Space Daily Editorial
- The official ESA Webb announcement on 27 May 2026 and two papers report the first
- direct mass measurement of a supermassive black hole in the first billion years after the Big
- Bang. The object sits at the heart of a small red galaxy called Abell2744-QSO1, seen as it was
- roughly 700 million years after the Big Bang. The mass comes out at 50 million times the mass
- of the Sun. The galaxy around it is so faint that the central object accounts for around two-thirds
- of the total mass of the system and is more massive than all the stars in the galaxy combined.
- If the measurements hold, the implications run against the standard idea of how supermassive
- black holes form, which has the galaxy assembling first and the central black hole growing in
- step with it.
- QSO1 belongs to a class of objects called Little Red Dots, first identified by the James
- Webb Space Telescope (JWST) shortly after its commissioning in 2022. These are very compact,
- very red sources, common in the first billion years of cosmic history and almost entirely absent
- in the local universe. Previous mass estimates for black holes in the first billion years had relied
- on indirect methods, mostly calibrated against scaling relations observed in the local universe.
- These methods give an answer but carry the assumption that the physics of black hole accretion
- in the distant past was broadly similar to what is observed nearby. According to Space.com’s
- report on the work, D’Eugenio explained the team’s concern with that approach plainly: “We
- didn’t know if those assumptions really apply to the distant universe”.
- The galaxy itself contains relatively few stars. According to Universe Today’s coverage of
- the papers, the stellar mass is constrained to be below roughly 20 million solar masses, and
- some analyses push the upper limit considerably lower. The black hole is therefore more
- massive than all the stars in its galaxy combined, by at least a factor of two and possibly far
- more. The authors note in the paper published in Nature that QSO1 sits about a factor of ten
- above even the most extreme cases of black-hole-heavy galaxies previously identified by the
- JWST. The standard picture of supermassive black hole formation has the black hole growing
- alongside its host galaxy, in a feedback relationship that takes billions of years. QSO1 cannot
- have formed this way. The galaxy is too small to have fed the black hole through ordinary
- accretion, and the time elapsed since the Big Bang at the moment of observation is too short
- for slow co-evolution to have produced this result.
- The team’s preferred interpretation, presented as such rather than as a conclusion, is
- that the black hole formed first and the galaxy is now assembling around it. Ignas Juodžbalis,
- one of the authors of the Nature paper, said that “This is very exciting because it is evidence
- for primordial black holes or direct collapse black holes, which have been theorized but not
- confirmed”. What the papers establish, in a narrower and more defensible sense, is that the
- standard local scaling between black hole mass and host galaxy mass does not apply in the
- first billion years. Whether QSO1 is unusual among Little Red Dots, or whether the population
- as a whole follows the same pattern, is the next question the Cambridge–Florence team is
- pursuing.
(Available at: https://spacedaily.com/d-the-james-webb-space-telescope-has-just-captured-the-first-directmeasurement-of-a-black-hole-50-million-times-the-mass-of-the-sun-sitting-in-an-ancient-galaxy-where-itoutweighs-every-star-around-i/ – text specially adapted for this test).