Hubble and Webb team up to investigate one of the Whirlpool Galaxy's spiral arms. (Image credit: ESA/Webb, NASA & CSA, A. Pedrini, A. Adamo (Stockholm University) and the FEAST JWST team) Share this article 0 Join the conversation Add us as a preferred source on Google Newsletter Subscribe to our newsletter Quick factsWhat it is: A spiral arm of the Whirlpool Galaxy (M51)
Where it is: 31 million light-years away in the constellation Canes Venatici
When it was shared: May 6, 2026
Stars form when vast clouds of dust and hydrogen gas collapse, creating a dense core that heats up until it transforms into a nuclear fusion reactor. What happens in the moments after a star emerges from its birth cloud, however, is a mystery.
This image of one of the spiral arms in the Whirlpool Galaxy (Messier 51) gets astronomers closer to solving that mystery — and in doing so, could answer a key question about the early universe.
Made by combining data from the James Webb Space Telescope (JWST) and the Hubble Space Telescope, the image shows that larger groups of stars leave their birth clouds much quicker than smaller ones. It is just one of a series from a paper published May 6 in the journal in Nature Astronomy, which reveals the processes that shape different galaxies.
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As more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet light, and powerful explosions called supernovas begin to push the surrounding gas away. This process, called stellar feedback, keeps much of a galaxy's gas from turning into new stars.
In this photo, red-orange threads of gas and dust stretch into lines, while blue bubbles light up some areas from the inside. Gaps in the gas show bright white groups of stars. (JWST's ability to see infrared light uncovered new stars that would be hidden behind dust with normal telescopes.)
Two zoomed-out and zoomed-in views of the Whirlpool Galaxy, as seen by the JWST and Hubble
(Image credit: ESA/Webb, NASA & CSA, A. Pedrini, A. Adamo (Stockholm University) and the FEAST JWST team)When combined with the other images from the study, this showed a clear pattern: the largest groups of stars cleared their birth gas clouds in about 5 million years, while smaller groups took between 7 and 8 million years to fully emerge. That has major implications for how galaxies evolve — and how the universe became hot again about 500 million to 1 billion years after the Big Bang.
After the universe cooled, electrons and protons combined to form neutral atoms. Later, an unknown energy source separated them again during a period called reionization. Could this have been caused by the intense ultraviolet radiation released into galaxies by massive star clusters?
Sign up for the Live Science daily newsletter nowContact me with news and offers from other Future brandsReceive email from us on behalf of our trusted partners or sponsors"It had to be the formation of massive star clusters that helped drive the reionization of the universe," study co-author Daniela Calzetti of the University of Massachusetts Amherst, said in a statement. "The fact that the most massive clusters can emerge from their natal clouds in just 5 million years means that they had enough time for producing the photons that reionized the universe."
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Jamie CarterLive Science contributorJamie Carter is a Cardiff, U.K.-based freelance science journalist and a regular contributor to Live Science. He is the author of A Stargazing Program For Beginners and co-author of The Eclipse Effect, and leads international stargazing and eclipse-chasing tours. His work appears regularly in Space.com, Forbes, New Scientist, BBC Sky at Night, Sky & Telescope, and other major science and astronomy publications. He is also the editor of WhenIsTheNextEclipse.com.
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