Globular Clusters: Stars from Poorly Mixed Dough ✛

Original: "Globular cluster abundance patterns inherited from giant molecular clouds"
arXiv:2607.05509v1 · 2026-07-06 · CC BY 4.0 · 2 min
Chemical variations in globular clusters come from uneven gas mixing before the stars were born.

Imagine you’re making cookies: one part of the dough has more sugar, another more flour. After baking, the cookies will taste different because the initial mixing was poor. According to a new study, globular clusters formed in a similar way — giant spheres of hundreds of thousands of old stars. Once upon a time, these stars were born from a single giant gas cloud, but the cloud was not uniform. Some parts had more oxygen, others more nitrogen. So the stars inside the cluster have different chemical ‘flavors’, even though they are the same age and came from the same ‘dough’.

We learned about the chemical composition thanks to spectroscopy — the analysis of starlight. Back in the early 20th century, Cecilia Payne-Gaposchkin used it to establish that stars are giant spheres of hydrogen. The Hubble telescope later confirmed that chemical variations do exist inside globular clusters. All this analysis relies on a fundamental law: the speed of light is constant, and light from different elements carries its own unique color signature.

A new computer model recreated the history of a gas cloud in the early Universe, just after the Big Bang. Back in the early last century, Edwin Hubble saw globular clusters as key to understanding the scale of the cosmos. In those distant times, galaxies were small and often flared up with short bursts of star formation. After such a burst, explosions ejected gas rich in oxygen (like the flour in our example). Then, when the galaxy temporarily ‘quieted down’, dying stars added a lot of nitrogen to the surroundings (like sugar). Later, the oxygen-rich gas cooled, fell back, and collided with the nitrogen cloud. The mixing was imperfect — regions with different ratios of ‘flour’ and ‘sugar’ emerged. When stars ignited in these regions, they inherited the pre-existing chemical differences. No stars polluted anything afterwards.

Globular clusters don’t fly apart because they are held together by invisible mass — dark matter, discovered in the motion of galaxies by Vera Rubin. Perhaps in the future, sensitive gravitational wave detectors will catch mergers of black holes inside these clusters and reveal much about their interiors.

Globular clusters have almost no elements heavier than helium — because they formed from primordial gas, before the ‘building blocks’ of planets and life had a chance to accumulate.

[\text{N/Fe}] \approx -0.5\,[\text{O/Fe}] + \text{const}
The observed anti-correlation between nitrogen and oxygen in globular clusters indicates that these elements came from different sources. The slope of about –0.5 reflects the balance between enrichment from supernovae (oxygen) and asymptotic giant branch stars (nitrogen).
M_{\text{загрязн}} \approx 10 \times M_{\text{скопл}}
The mass deficit problem: to pollute the second generation of stars, the first generation would need to be tens of times more massive, which doesn't match observations. The new scenario bypasses this contradiction by assuming simultaneous formation from already enriched gas.
Scientists
Adam RiessBrian SchmidtEdwin HubbleGeorges LemaîtreMaarten SchmidtSaul Perlmutter
Concepts
globular cluster open cluster star formation in clusters stellar chemical abundances chemical galactic archaeology star formation gas molecular cloud stellar population galactic bulge starburst interstellar gas population iii stars dense clump galaxy distribution clump galaxy growth mechanisms large-scale structure of the universe constellation first stars early universe metal enrichment