By spying on star clusters in a nearby galaxy, the Hubble Space Telescope has shown that star clusters aren't always as old as they appear.
The long-running observatory turned its attention to collections of stars in the Large Magellanic Cloud (LMC), a satellite dwarf galaxy of the Milky Way located about 160,000 light-years from Earth. (A light-year is the distance light travels in a year, or roughly 6 trillion miles or 10 trillion kilometers).
In the LMC, astronomers observed the behavior of bright, blue stars known as "blue stragglers." These stars receive a bunch of extra fuel from other stars in their environment, which makes them bigger and brightens them up. This usually happens when a star steals gas from a neighbor or two stars crash into each other.
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Video: Watch Blue Straggler Stars Move Over Time in Animation (opens in new tab)
These stragglers revealed something interesting about how star clusters evolve, the researchers said. Because they are so bright, they are easy to track even if they are buried deep within the group of stars. They thus make a handy reference for star movement in a star cluster, which can consist of up to 1 million stars.
The mutual gravitational pull between stars in a cluster tends to change the cluster's structure over time, a process that astronomers call "dynamical evolution." Specifically, heavy stars sink toward the middle of the cluster and low-mass stars flee to the outskirts, Hubble officials said in a statement.
The "stragglers" showed, for the first time, that star clusters can be different physical shapes even if they formed during the same period. That's because the varying pull between stars "causes a progressive contraction of the cluster core over different time scales," Hubble officials said, "and means that star clusters with the same chronological age can vary greatly in appearance and shape because of their different 'dynamical ages.'"
The research was led by Francesco Ferraro, an astrophysicist at the University of Bologna in Italy. The work was published Sept. 9 in the journal Nature Astronomy (opens in new tab).
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