They Didn't Disappear—They Became Normal Galaxies: An Explanation from Nearly 100 Samples
The James Webb Space Telescope discovered a striking class of objects in the early universe: compact structures with reddish colors, present in considerable numbers, then almost entirely absent after the universe reached an age of roughly two billion years.
Astronomers call them little red dots. Their disappearance is itself a puzzle: where did these compact red objects go?
A team led by Associate Professor Zhang Huanian and Professor Wu Qingwen of the School of Physics at Huazhong University of Science and Technology, in collaboration with Peking University, the Institute of High Energy Physics of the Chinese Academy of Sciences, and other institutions, used a sample of nearly 100 spectroscopically confirmed little red dots to offer the first explanation based on large-scale environment and dark matter halo mass evolution. The study was published online in *Nature Astronomy* on October 8.
In the Very Early Universe, They Lived Alone
The first finding concerns where they lived.
In the very early universe, little red dots tended to live in isolation in low-density environments, while ordinary galaxies of the same epoch clustered in dense matter regions—a starkly different distribution.
As the universe evolved to roughly two billion years of age, the environments of little red dots gradually became indistinguishable from those of ordinary galaxies.
Wu Qingwen put it plainly: the little red dots did not disappear—they simply gradually became like ordinary galaxies.
A Twenty-Fold Growth in Dark Matter Halos
The second finding is harder evidence: a direct measurement of dark matter halo masses.
Little red dots underwent a period of rapid growth early in their existence. When the universe was about 800 million years old, their dark matter halo masses were around 10 billion solar masses. By 1.8 billion years, they had grown to 200 billion solar masses.
To put 200 billion solar masses in perspective: that is already the level of ordinary galaxies' dark matter halos.
Wu Qingwen's conclusion is direct: little red dots are not a permanent class of special objects, but a brief phase in galaxy evolution. They continuously evolve and grow, ultimately converging with ordinary galaxies and no longer appearing as compact red points.
Putting the Numbers Together
Growing from 10 billion to 200 billion solar masses is a twenty-fold increase. In that growth, the little red dots' dark matter halos caught up with those of ordinary galaxies. At the same time, their environments shifted from low-density regions to places where ordinary galaxies gather. Together, these two changes removed the reason for their compact, red appearance.
| Dimension | Very early (~800 Myr) | After evolution (~1.8–2 Gyr) | |---|---|---| | Dark matter halo mass | 10 billion solar masses | 200 billion solar masses | | Environment | Low-density, isolated | Similar to ordinary galaxy clustering regions | | Appearance | Compact, red | No longer compact red points | | Sample basis | ~100 spectroscopically confirmed objects | Same sample |
What Nearly 100 Spectroscopic Confirmations Mean
The figure of nearly 100 is the methodological foundation of the study.
Little red dots were initially selected from imaging; only spectroscopic confirmation can separate true targets from various contaminants. Purely imaging-based samples are of limited use in research on this class of objects.
Using nearly 100 spectroscopically confirmed samples for statistical analysis means that the conclusions on environment and halo mass are each backed by close to a hundred independent data points, rather than the intuitive extrapolation of a few cases.
The work offers a new perspective on the co-evolution of black holes and galaxies in the early universe, and suggests that early galaxy evolution may be more diverse and dynamic than previously thought.
Sources and Caveats
- All numbers are taken from a Xinhua report dated October 12; the original *Nature Astronomy* paper and tables were not obtained
- Measurement methods, error ranges, telescopes used, and sample selection criteria for halo masses were not disclosed
- The confirmation standards, spectral criteria, and origin of the ~100 spectroscopically confirmed samples were not given in the report
- The paper title, full author list, and DOI were not obtained; only Zhang Huanian and Wu Qingwen were named
- The comparison of 200 billion solar masses to ordinary galaxies' halos is described in the report as "approaching"; this article follows that wording rather than treating it as an equality