كيف استخدم جيمس ويب عدسة الجاذبية لوزن عملاق نائم بعيد بـ 10 مليارات سنة ضوئية

Stellar dynamics: weighing the invisible

With the lensed, magnified view, the team turned to JWST's NIRSpec Integral Field Spectrograph. This instrument captured a spectrum for every pixel in the image, allowing the scientists to map the velocities of stars at different distances from the galaxy's center. The technique is known as stellar dynamics—the same method used to weigh the Milky Way's central black hole, a feat that won the Nobel Prize in Physics in 2020 .

Stars closer to a supermassive black hole orbit faster. By modeling how the stellar velocities changed with radius using simple Keplerian motion, the team could identify the black hole's "sphere of influence"—the region where its gravity dominates the stars' motion. This allowed for a direct mass measurement. Before this study, the farthest direct stellar-dynamics measurement was for a black hole only about 700 million light-years away. MRG-M0138 shatters that record by more than a factor of ten .

What they found: a galaxy-quenching giant

The measurement confirmed a black hole of roughly 6 billion solar masses . Its host galaxy, MRG-M0138, is a massive, red elliptical galaxy that has long since stopped forming new stars. The central black hole is dormant, meaning it is not currently pulling in and heating up large amounts of gas .

The findings suggest a violent history. MRG-M0138 was likely once a brilliant quasar, powered by gas spiraling into the growing black hole. The immense energy output from this active phase could have heated or even ejected the very gas that star formation requires, effectively shutting down the galaxy's stellar factories. The dead, quiet state of the galaxy and the dormant state of the black hole today are, therefore, likely related; the black hole grew so large and powerful that it quenched its own host .

Challenging models of co-evolution

This discovery strikes at the heart of how we think galaxies and black holes grow together. In the local universe, a tight correlation exists between the mass of a central black hole and the properties of its host galaxy's central bulge, suggesting they co-evolve in lockstep. This measurement provides direct evidence that this relationship was not always in place, and that black holes can form and grow to enormous sizes before their host galaxies finish assembling their stars.

The data indicates that some of the densest regions in the early universe were sites of extremely rapid black hole growth, outpacing the surrounding galaxy . The MRG-M0138 measurement challenges simple co-evolutionary models where the growth of the black hole and the galaxy are always tightly coupled. Future surveys with JWST, Euclid, the Nancy Grace Roman Space Telescope, and next-generation ground-based observatories like the Giant Magellan Telescope aim to apply this lensing-plus-stellar-dynamics technique to many more galaxies, constructing a statistical picture of black hole and galaxy co-evolution across cosmic time .