Newborn stars born in the biggest stellar clusters tear themselves out of their birth clouds much faster than those that grow up in small clusters, according to a new study.
Using NASA‘s Hubble Space Telescope and James Webb Space Telescope, researchers studied nearly 9,000 examples from four different galaxies: Messier 51, Messier 83, NGC 4449, and NGC 628.
Because no one can watch a single cluster evolve over millions of years in space, scientists instead observed many clusters at different intervals and treated them like snapshots in a sequence. Some stars were still completely buried in dust. Some had partly emerged. Others were fully exposed.
What researchers found was a consistent pattern: The star clusters moved through the same sequence but how quickly depended on their mass. For the largest clusters, clearing the cloud of gas and dust may only take about 5 million years. The smaller ones may not break free for 7 to 8 million years.
The research puts real numbers on something that has remained ambiguous up until now. Simulations of star formation already factor in so-called “stellar feedback” — the radiation, stellar winds, and supernovas that young stars produce — but the models disagree on how fast those events and processes blow away gas. These new measurements, published in Nature Astronomy, give scientists a concrete timeline based on a large sample, said Angela Adamo, a lead author on the study from Stockholm University and the Oskar Klein Centre in Sweden.
The patterns showed up everywhere the team looked, even though each galaxy doesn’t look or behave the same way. That consistency suggests the timing isn’t just a product of a local quirk in one environment, but a basic feature of how star clusters evolve.
Mashable Light Speed
The clusters all started off similarly: with baby stars releasing their energy in secret. At the earliest stage, they’re hidden deep within a thick cloud of gas and dust that blocks their visible light. Only infrared light can pass through that haze.
Inset images zoom in on newborn star clusters in Messier 51, one of the four galaxies included in the new James Webb Space Telescope and Hubble study.
Credit: ESA / NASA / CSA / A. Pedrini / A. Adamo
As the concealed stars grow, they change their environment, heating the surrounding gas and blasting out radiation and fast stellar winds. Over time, that energy pushes the gas and dust away, revealing what’s inside.
By counting how many clusters appear in each stage, the researchers estimated how long each phase lasts. The idea is simple: If lots of clusters show up in a stage, it tends to last longer; if only a few do, it’s over more quickly.
Once the cloud is gone, there’s nothing holding the stars back. Their ultraviolet radiation can travel farther through their home galaxy, colliding with nearby gas and influencing where new stars can or cannot form next.
When that stellar feedback is unleashed, it creates a lot of waste, sterilizing regions of galaxies. Most of the gas never gets used for star formation.
That extends to planets, too. Young stars form with disks of gas and dust around them, and those disks birth planets. If a cluster blows away its surrounding material quickly, those disks get exposed earlier, vulnerable to harsh radiation that can interrupt the process of world building.
The research has implications for scientists working on a variety of cosmic mysteries, said Alex Pedrini, lead author of the study, who is also based at Stockholm University and the Oskar Klein Centre in Sweden.
“We can look into the cradles of star clusters and connect planet formation to the cycle of star formation and stellar feedback,” he said in a statement.
