Astronomers Observe Cosmic Tug-of-Struggle as Gravity Reshapes Magnetic Fields in Star Clusters | Center for Astrophysics

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Cambridge, MA (October 8, 2025)— In the biggest and most detailed survey of its sort, astronomers utilizing the Atacama Large Millimeter/submillimeter Array (ALMA) have captured the clearest image but of how large stars are born. By zooming in to scales just a few instances bigger than our photo voltaic system, the crew was capable of see for the primary time the continued tug-of-war between magnetic fields and gravity that helps stars take form deep inside big molecular clouds. The new observations have been revealed right now in The Astrophysical Journal.

Star formation happens when gravity squeezes chilly fuel till it collapses in on itself. But this epic collapse is not pushed by gravity alone, and for many years, astronomers have debated which pressure— magnetic fields or gravity— dominates the star formation course of.

Led by Qizhou Zhang, senior astrophysicist on the Center for Astrophysics | Harvard & Smithsonian (CfA), these new observations have supplied front-row seats to the tug-of-war match as seen throughout 17 energetic star-forming areas, and revealed that as fuel turns into denser, gravity positive aspects the higher hand. While magnetic fields and turbulence each begin out strongly resisting the pull of gravity, magnetic fields are step by step pulled into alignment with infalling fuel when gravity takes over because the main pressure shaping the collapsing cloud.

“With ALMA’s extraordinary sensitivity and resolution, we can now probe these cosmic birthplaces in unprecedented detail,” stated Zhang. “We see that gravity actually reorients the magnetic field as clouds collapse, offering new clues about how massive stars,and the clusters they inhabit, emerge from the interstellar medium.”

The observations additionally revealed a shocking sample: magnetic subject orientations in molecular clouds do not happen randomly. Instead, they largely happen in two methods, typically lining up with the course of gravity, and typically perpendicular to it. The sample is proof of a posh and evolving relationship between these two cosmic forces.

Understanding how stars kind is key to nearly each subject of astronomy, shaping all the things from the origins of the Sun to the evolution of galaxies. The analysis gives new readability on the interactions between gravity and magnetic fields in large star formation, and offers scientists highly effective new instruments to check and refine theories concerning the life cycles of stars, planets, and molecular clouds.

Resource

Zhang, Qizhou et al. (4 Oct 2025). Impact of gravity on altering magnetic subject orientations in a pattern of large protostellar clusters noticed with ALMA. The Astrophysical Journal. pre-print: https://iopscience.iop.org/article/10.3847/1538-4357/adfdcb

About the Center for Astrophysics | Harvard & Smithsonian

The Center for Astrophysics | Harvard & Smithsonian is a collaboration between Harvard and the Smithsonian designed to ask—and in the end reply—humanity’s biggest unresolved questions concerning the nature of the universe. The Center for Astrophysics is headquartered in Cambridge, MA, with analysis services throughout the U.S. and world wide.

About NRAO

The National Radio Astronomy Observatory (NRAO) is a facility of the U.S. National Science Foundation, operated beneath cooperative settlement by Associated Universities, Inc.

About ALMA

The Atacama Large Millimeter/submillimeter Array (ALMA), a global astronomy facility, is a partnership of the European Southern Observatory (ESO), the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the National Science and Technology Council (NSTC) in Taiwan and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI).

ALMA development and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) gives the unified management and administration of the development, commissioning and operation of ALMA.

Media Contact:

Amy C. Oliver, FRAS
Public Affairs Officer
Center for Astrophysics | Harvard & Smithsonian
[email protected]
520-686-8712


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