Early galaxy looked like lumpy ‘cosmic grapes'
'Early galaxies form through dark matter and gas assembly, evolving into dynamically hot, chaotic structures driven by mergers and feedback,' the international research team explained in their Nature Astronomy study published on August 7. 'By contrast, remarkably smooth, rotating disks are observed in massive galaxies only 1.4 billion years after the Big Bang, implying rapid dynamical evolution.'
Understanding how this cosmic evolution unfolded requires the ability to study young galaxies—something previously made difficult by limitations in observational tools' sensitivity and spatial resolution. Even with the Hubble Space Telescope's groundbreaking abilities, the 'Cosmic Grapes' galaxy only appeared as a smooth, singular disk-like formation. Using more recent and advanced projects like JWST and ALMA, astronomers were able to refocus on the mystery target with some help from a cosmic neighbor.
According to a study announcement from the National Radio Astronomy Observatory, the Cosmic Grapes structure 'happened to be perfectly magnified by a foreground galaxy cluster through gravitational lensing.' The opportunity allowed researchers to devote over 100 hours of quality telescope time to the individual system, making it one of the early universe's most extensively analyzed galaxies.
Instead of the individual disk seen in Hubble's images, the exponentially greater resolution from JWST and ALMA showcased a wholly different situation—a rotating galaxy stuffed with giant, lumpy stellar formations resembling the vineyard fruit. The reveal is also the first time that astronomers successfully linked an early galaxy's smaller internal structures to their larger, collective rotation. The data was so detailed that they even managed to achieve a spatial resolution of 10 parsecs, or about 30 light-years.
What's particularly striking is that Cosmic Grapes isn't an oddball or extreme example given what astronomers understand of galactic evolution. Instead, it exists on the standard, main sequence of galaxies when it comes to attributes like star formations, mass, chemical composition, and size. This suggests many of the era's galaxies that have been previously documented as smooth may more resemble the clumpy, dynamic structure seen through JWST and ALMA.
'Because existing simulations fail to reproduce such a large number of clumps in rotating galaxies at early times, this discovery raises key questions about how galaxies form and evolve,' the National Radio Astronomy Observatory's announcement explained. 'It suggests that our understanding of feedback processes and structure formation in young galaxies may need significant revision.'
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