The galaxy, known as A1689B11, existed just 2.6 billion years after the Big Bang, when the universe was only one fifth of its present age.
Researchers including those from Australian National University (ANU) and Swinburne University of Technology used a powerful technique that combines gravitational lensing with the Near-infrared Integral Field Spectrograph (NIFS) on the Gemini North telescope in Hawai'i to verify the vintage and spiral nature of the galaxy.
Gravitational lenses are nature's largest telescopes, created by massive clusters composed of thousands of galaxies and dark matter.
"This technique allows us to study ancient galaxies in high resolution with unprecedented detail," said Tiantian Yuan from ANU.
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"We are able to look 11 billion years back in time and directly witness the formation of the first, primitive spiral arms of a galaxy," said Yuan, who led the research team.
"Studying ancient spirals like A1689B11 is a key to unlocking the mystery of how and when the Hubble sequence emerges," said Renyue Cen from Princeton University in the US.
"This galaxy is forming stars 20 times faster than galaxies today as fast as other young galaxies of similar masses in the early universe," he said.
"However, unlike other galaxies of the same epoch, A1689B11 has a very cool and thin disc, rotating calmly with surprisingly little turbulence. This type of spiral galaxy has never been seen before at this early epoch of the universe," said Cen.
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