The James Webb Space Telescope has given astronomers a stunning new window into the history of galaxies like our own Milky Way.
By analyzing 111 edge-on galaxies, researchers discovered that galaxies form in two main stages: an early, chaotic thick disk followed by a calmer, thin disk that forms inside it. This pattern was observed even in galaxies 10 billion light-years away. The findings suggest that our Milky Way’s layered structure isn’t unique but part of a broader galactic trend, offering new insight into how galaxies evolve, build stars, and possibly even shape life-sustaining elements like oxygen and carbon.
Disk Galaxies and Their Fossil Records
Many galaxies, including our own Milky Way, have a remarkable structure: a flat, spinning disk made of stars. These stellar disks typically come in two main parts. The thin disk is home to younger stars rich in heavy elements like oxygen and carbon, while the thick disk holds older, more primitive stars. These distinct components act like cosmic fossils, preserving clues about how galaxies grow, form stars, and create the elements essential for life.
Until recently, scientists could only see these two-layered disks in the Milky Way and a few nearby galaxies. Previous telescopes simply weren’t powerful enough to spot the thin edge of faraway galaxies when viewed from the side.
That all changed with the launch of the James Webb Space Telescope (JWST) in 2021 the most advanced and sensitive space telescope ever built.
A Galactic Survey Through Time
Now, an international team of astronomers has analyzed 111 edge-on galaxies captured by JWST. These side views allowed researchers to clearly see the vertical structure of distant galaxies and identify both thin and thick disks.
Takafumi Tsukui (formerly of the Australian National University and now based at Tohoku University), who led the research team, says that observing distant galaxies is akin to using a time machine, allowing us to see how galaxies have formed their disks over cosmic history.
“Thanks to the JWST’s sharp vision, we were able to identify thin and thick disks in galaxies beyond our local universe, some going as far back as 10 billion years ago.”
The study revealed a consistent trend: in the earlier universe, more galaxies appear to have had a single thick disk, while in later epochs, more galaxies showed a two-layered structure with an additional thin disk component. This suggests that galaxies first formed a thick disk, followed by the formation of a thin disk within it. In more massive galaxies, this thin disk appears to have formed earlier.
Website: International Research Awards on High Energy Physics and Computational Science.
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