
Galactic halos, consisting of a spherical envelope of dark matter along with sparsely scattered stars, globular clusters, and gas, typically surround most spiral galaxies. Current research is investigating the possibility that some halos may exist solely of dark matter. Discovering halos without stellar matter carries profound implications for our understanding of the universe’s structure, galaxy formation processes, and the conditions required for star formation. More importantly, such a discovery would provide a unique laboratory to study dark matter in isolation, free from interference of normal matter. However, new findings suggest that starless halos may be even rarer than previously thought. This scarcity makes detecting such halos particularly challenging, as they are unlikely to be associated with observable galaxies.
Ethan Nadler, of the University of California San Diego, has demonstrated that molecular hydrogen requires significantly less mass for star formation compared to atomic hydrogen. His research shows that molecular hydrogen can cool sufficiently for gravity to initiate star formation at lower mass thresholds. Specifically, while past studies indicated that dark matter halos need between 100 million to 1 billion solar masses of atomic hydrogen to begin star formation, Nadler has revealed that molecular hydrogen can achieve the same result with as little as 10 million solar masses—a reduction by a factor of 10 to 100. While dark matter halos can theoretically form with masses as low as 10⁻⁶ solar masses, depending on the nature of dark matter, those capable of influencing galaxy formation typically require at least 10⁶ solar masses to enable star formation, further highlighting the challenge of finding starless halos. Detecting these small, starless halos would require identifying subtle perturbations in gravitational fields, a difficult task that may yield little if such halos are as rare as current models suggest.
Source: …Galaxy Formation Threshold, Nadler, AAS, April 2025. Graphic: Dark Matter Halo Simulation by Cosmo0. Public Domain.








