New study may reshape how scientists measure the universe

University of Missouri astronomers have found evidence that one of the assumptions underpinning modern galaxy research may not apply universally: stars do not always form in the same proportions from one stellar nursery to another. The finding challenges the long-standing idea that galaxies, regardless of their size, age or surroundings, can be measured using a single mathematical description of how many massive and low-mass stars are born. If confirmed across larger samples, the result could alter estimates of galaxy mass, age and evolution—and may offer a new explanation for why some distant galaxies observed by the James Webb Space Telescope appear unexpectedly massive.

The assumption at the center of the study is known as the stellar initial mass function, or IMF. It describes the distribution of stellar masses produced during a generation of star formation. In a typical stellar population, high-mass stars are rare, while low-mass stars are far more numerous. Because massive stars are much brighter than their smaller counterparts, astronomers can often detect them in distant galaxies even when the faintest stars remain invisible. They then use the IMF to infer how many unseen low-mass stars must exist and calculate the total mass of the galaxy.

For more than half a century, researchers have commonly treated the IMF as universal. In this framework, a star-forming region in the Milky Way and a galaxy billions of light-years away are assumed to produce broadly similar proportions of massive and low-mass stars. That assumption makes it possible to convert the light from a galaxy into estimates of its stellar content. However, it also means that an incorrect IMF can systematically distort the measurements used to reconstruct the history of the cosmos.

The new research, led by scientists in the University of Missouri’s College of Arts and Science, indicates that the stellar mix can vary significantly between different environments. Rather than behaving as identical factories, star-forming regions may produce different proportions of stars depending on the physical conditions present when they collapse. Temperature, gas density, turbulence, chemical composition and the pressure within a molecular cloud could all influence how matter fragments into stars of different masses.

To investigate the possibility, the researchers turned to data from the European Space Agency’s Gaia mission. Gaia has created an extraordinarily detailed map of the Milky Way, measuring the positions, motions and other properties of nearly two billion stars. The Mizzou team focused on open and stellar clusters—groups of stars that formed from the same cloud at approximately the same time. Because cluster members share a common origin, they provide a natural laboratory for comparing stellar populations formed under related conditions.

If the IMF were truly universal, clusters should display essentially the same distribution of stellar masses after accounting for their ages and other effects. The researchers instead found meaningful differences from cluster to cluster. Some populations contained relative numbers of high- and low-mass stars that did not match the proportions predicted by a single universal IMF. The pattern was sufficiently consistent, the team reported, to suggest that the variation reflects differences in star-forming environments rather than random statistical noise or a simple observational error.

That result does not mean the IMF should be abandoned. Instead, the researchers propose that astronomers treat it as an environment-dependent tool. A galaxy dominated by dense, chemically enriched star-forming regions might require a different IMF from one where stars formed in more diffuse or metal-poor clouds. Applying the appropriate version could improve calculations of stellar mass, star-formation rates and the rate at which galaxies build up their visible matter over time.

The implications extend to some of the most surprising observations made by the James Webb Space Telescope. JWST has detected galaxies from the early universe that appear brighter and more massive than many theoretical models predicted. One possible explanation is that these galaxies grew more rapidly than expected, forcing scientists to reconsider aspects of cosmology and galaxy formation. Another possibility is that their stars formed with an unusual mass distribution. If early galaxies produced more massive, luminous stars than assumed, their light could make them appear to contain more stellar mass when interpreted through a standard IMF.

“Other galaxies weren’t breaking the laws of physics—we were measuring them with the wrong yardstick,” said Charles Steinhardt, an astronomy professor at the University of Missouri and co-author of the study. Undergraduate researcher Carter Meyerhoff, also a co-author, described the pattern as “surprisingly clean,” suggesting that astronomers may eventually be able to select an IMF based on the conditions in which a galaxy’s stars formed. The researchers emphasize that additional observations and independent analyses will be needed to establish how broadly the relationship applies beyond the Milky Way.

The study, titled “Direct evidence for stellar initial mass function variation in the Milky Way,” was published in The Astrophysical Journal Letters. Alexander Luening of the University of Rochester also contributed. By linking the birth environment of stars to the way astronomers interpret their combined light, the work points toward a more flexible model of the universe—one in which galaxies may not simply contain different numbers of stars, but may manufacture those stars according to different cosmic recipes.

Web References: University of Missouri College of Arts and Science: https://coas.missouri.edu/ ; Study DOI: https://doi.org/10.3847/2041-8213/ae7444

References: The Astrophysical Journal Letters, DOI: 10.3847/2041-8213/ae7444

Keywords

Stellar initial mass function, star formation, Milky Way, star clusters, Gaia mission, James Webb Space Telescope, galaxy evolution, stellar populations, astrophysics, astronomy