'Just like the Milky Way': Scientists discover REBELS-25 galaxy, raising new questions for cosmic evolution theories

Produced by: Tarun Mishra Designed by: Manoj Kumar

Distant Galaxy REBELS-25 Discovered

Astronomers have identified a distant galaxy, REBELS-25, using the Atacama Large Millimetre/submillimetre Array (ALMA). Despite being young, this galaxy shows an orderly structure similar to the Milky Way.

Unexpected Rotation-Dominated Structure

Unlike the clumpy, chaotic appearance expected from early galaxies, REBELS-25 is rotation-dominated, challenging current assumptions about early cosmic formation.

Challenges to Galaxy Formation Theories

Dave Clements, an astrophysicist at Imperial College London, noted the surprising disc-like structure of REBELS-25, questioning if it is an anomaly or if current galaxy formation theories need revision.

Seen 700 Million Years After the Big Bang

REBELS-25 is observed as it was when the universe was only 700 million years old. Its early formation contradicts the traditional belief that galaxies evolve over billions of years.

Comparison to the Milky Way

The study’s lead author, Lucie Rowland, highlighted that the similarities between REBELS-25 and the Milky Way question how quickly galaxies in the early universe could have formed.

ALMA’s Role in the Discovery

Andrew Blain, an astrophysicist at the University of Leicester, emphasized that ALMA was crucial in detecting the faint details of galaxies like REBELS-25, revealing finer structures than previous telescopes could capture.

Ongoing Research and Future Observations

The research, accepted for publication in the Monthly Notices of the Royal Astronomical Society, will continue with further observations to confirm the presence of spiral arms and other advanced features in REBELS-25.

Potential Impact on Cosmic Evolution Understanding

The discovery of REBELS-25 offers new insights into early galaxy formation, potentially reshaping how astronomers understand the evolution of galaxies in the universe's early stages.