New JWST low-mass galaxy observations could help settle scientific debate about early universe origins

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Image: The process of reionization in numerical simulations. Credit: J. Rosdahl, H. Atek and the SPHINX project team
Image: The process of reionization in numerical simulations. Credit: J. Rosdahl, H. Atek and the SPHINX project team

International researchers have made a major astronomical discovery, revealing that small galaxies are very likely at the origin of reionization – a crucial period in the early universe where neutral hydrogen transformed into ionized gas.

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From: Swinburne University of Technology

International researchers have made a major astronomical breakthrough, revealing that small galaxies are very likely at the origin of reionization – a crucial period in the early universe where neutral hydrogen transformed into ionized gas.

A paper published in Nature has used the James Webb Space Telescope (JWST) to obtain the first spectra of very low-mass galaxies less than a billion years after the Big Bang.

Their observations could help settle a long-running scientific debate about the drivers of reionization and could be essential to understanding the formation of the very first galaxies.

Swinburne University of Technology is the only Australian university as part of the international collaboration, led by Associate Professor Ivo Labbe.

Co-author, JWST Australian Data Centre Senior Scientist, and Swinburne Laureate Postdoctoral Research Associate in Galaxy Spectral Modelling Dr Themiya Nanayakkara says he is thrilled with the outcomes of this global research involving the Paris Astrophysics Institute (Sorbonne University/CNRS), and universities in Pittsburgh and Texas.

“This work makes a strong case for smaller galaxies to be the driving force behind reionizing the universe. While the number of energetic photons produced by these small galaxies may come as a shock to many, the cosmological implications are also profound.”

Reionization, which occurred some 500 to 900 million years after the Big Bang, marks a crucial period in the history of the universe. It represents the transformation of neutral hydrogen – which predominated the universe – into ionized gas and marks the end of the ‘Dark Ages’ in cosmic history.

Scientists have been arguing what drove the reionization of the universe for a long time. Confirmation of the hypothesis relating to low-mass galaxies has proven particularly difficult, given their low luminosity.

The study achieved this technological feat through the unique combination of JWST sensitivity and the gravitational lensing effect of the Abell 2744 cluster, making nearby galaxies act like cosmic magnifiers, distorting space and amplifying the light of background galaxies.

The team wants to extend this study to a larger scale, to confirm that this location is representative of the average distribution of galaxies in the universe.

“We have now entered uncharted territory with the JWST,” says Dr Nanayakkara. “This work opens up more exciting questions that we need to answer in our efforts to chart the evolutionary history of our beginnings."

-ENDS-

Dr Themiya Nanayakkara is available for interview.

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Nature
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Organisation/s: Swinburne University of Technology
Funder: H.A. and I.C. acknowledge support from CNES, focused on the JWST mission and the Programme National Cosmology and Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, co-funded by CEA and CNES. H.A. thanks the Cosmic Dawn Center (DAWN) for their support. DAWN is funded by the Danish National Research Foundation (grant no. 140). I.L. acknowledges support from the Australian Research Council through Future Fellowship FT220100798. P.D. acknowledges support from the NWO (grant no. 016.VIDI.189.162) (ODIN) and from the CO-FUND Rosalind Franklin programme of the European Commission and the University of Groningen. A.Z. acknowledges support from the US–Israel Binational Science Foundation (BSF) (grant no. 2020750), the US National Science Foundation (NSF) (grant no. 2109066) and the Ministry of Science and Technology, Israel. The work of C.C.W. is supported by NOIRLab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the NSF.
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