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Oxygen detected in the most distant galaxy ever found

Oxygen detected in the most distant galaxy ever found

CNN20-03-2025

Summary
Astronomers have discovered oxygen and heavy metals in galaxy JADES-GS-z14-0, the most distant galaxy ever found at 13.4 billion light-years away.
The presence of these elements suggests galaxies formed much faster than expected in the early universe.
Researchers described the unexpectedly mature galaxy as "like finding an adolescent where you would only expect babies," according to study author Sander Schouws.
The galaxy appears unusually large and bright and contains 10 times more heavy elements than expected.
Scientists are using both the James Webb Space Telescope and ALMA observatory to investigate whether the galaxy and its rapid evolution are unique. Astronomers have made the surprising discovery of oxygen and elements like heavy metals in the most distant known galaxy. The galaxy is 13.4 billion light-years away, meaning it formed in the early days of the universe.
Astronomers believe the big bang created the universe 13.8 billion years ago.
The unusually large, luminous distant galaxy, called JADES-GS-z14-0, was initially detected in January 2024 using the James Webb Space Telescope, which observes the universe in infrared light that's invisible to the human eye. The space observatory can effectively peer back in time to the beginning of a mysterious era called Cosmic Dawn, or the first few hundred million years after the big bang when the first galaxies were born, because it can observe light that has traveled for billions of years across space to Earth.
Light from JADES-GS-z14-0 has taken 13.4 billion years to reach our corner of the universe, so Webb and other observatories such as ALMA, or the Atacama Large Millimeter/submillimeter Array in Chile's Atacama Desert, are seeing the galaxy as it was when the universe was only about 300 million years old.
When astronomers used ALMA to follow up on Webb's initial observations, they were stunned to find the presence of oxygen and heavy metals because their presence suggests that galaxies formed more quickly than expected in the early days of the universe.
The results of the ALMA detections were published Thursday in separate studies in The Astrophysical Journal and Astronomy & Astrophysics.
'It is like finding an adolescent where you would only expect babies,' said Sander Schouws, lead author of The Astrophysical Journal study and a doctoral candidate at Leiden Observatory at Leiden University in the Netherlands, in a statement. 'The results show the galaxy has formed very rapidly and is also maturing rapidly, adding to a growing body of evidence that the formation of galaxies happens much faster than was expected.'
The fact that JADES-GS-z14-0 was laden with heavy elements is causing astronomers to question what some of the earliest galaxies were really like — as well as how many more they may find using Webb and ALMA.
A bright light leads to a surprise
Multiple aspects of JADES-GS-z14-0, including its large size and brightness, have proved to be unexpected. As Webb surveyed 700 distant galaxies, this one turned out to be the third brightest despite it being the farthest, Schouws said. But the oldest galaxies are expected to be smaller and dimmer because the universe was much smaller at the time.
'In general, galaxies this early in the universe are very different from the famous galaxies we know from the beautiful images of Hubble and JWST,' Schouws said in an email. 'They are a lot more compact, rich in gas and messy/disordered. The conditions are more extreme because a lot of stars are forming rapidly in a small volume.'
Galaxies typically begin from huge gas clouds that collapse and rotate, filling with young stars that are largely made of light elements such as helium and hydrogen. As stars evolve over time, they create heavier elements such as oxygen and metals, which disperse throughout the galaxy as stars explode at the end of their lifetime. In turn, the elements released by dying stars lead to the formation of more stars as well as the planets that orbit them.
But nothing about JADES-GS-z14-0 fits that model. Instead, the galaxy contains 10 times more heavy elements than expected, the study authors said.
'Such elements are produced by massive stars and the large amount of oxygen suggests that several generations of massive stars were already born and died,' said Dr.Stefano Carniani, assistant professor at the Scuola Normale Superiore of Pisa, Italy, and lead author of the Astronomy & Astrophysics study, in a statement. 'In conclusion (JADES-GS-z14-0) is more mature than expected and these results imply that the first generation of galaxies assembled their mass very quickly.'
Going the distance
Using ALMA also enabled the researchers to confirm the distance of the galaxy, originally measured using Webb, and refine their measurements. Together, both telescopes can be used to study the formation and evolution of the first galaxies, said Rychard Bouwens, associate professor at Leiden University and coauthor of the study in The Astrophysical Journal.
'I was really surprised by this clear detection of oxygen in JADES-GS-z14-0,' said Gergö Popping, a European Southern Observatory astronomer at the European ALMA Regional Centre, in a statement. Popping did not participate in either study.
'It suggests galaxies can form more rapidly after the Big Bang than had previously been thought. This result showcases the important role ALMA plays in unraveling the conditions under which the first galaxies in our Universe formed.'
While Webb can help identify extremely distant galaxies, ALMA can zoom in to study the gas and dust within them by detecting the far-infrared light they emit, Carniani said. Studying such galaxies can help shed light on the many remaining mysteries of Cosmic Dawn, such as what occurred shortly after the universe first began and the identities of the first celestial objects to appear.
The study authors believe the early galaxies may have formed more stars, and stars on a more massive scale, than expected, which would also affect the brightness of the galaxy overall.
'It's like burning candles: you can have candles with a wide wick that have a bright flame (massive stars) or you can have candles that burn slow and efficient (normal stars),' Schouws said.
But more observations are needed to understand exactly what the researchers are seeing, he said.
The team wants to determine whether the galaxy and its rapid evolution are truly unique, or if there are more like it in the early universe since a single celestial object is not enough to establish a new model of galaxy formation, Carniani said.

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Sign up for CNN's Wonder Theory science newsletter. Explore the universe with news on fascinating discoveries, scientific advancements and more. A tiny sign revealed in April seemed like it might change the universe as we know it. Astronomers had detected just a hint, a glimmer of two molecules swirling in the atmosphere of a distant planet called K2-18b — molecules that on Earth are produced only by living things. It was a tantalizing prospect: the most promising evidence yet of an extraterrestrial biosignature, or traces of life linked to biological activity. But only weeks later, new findings suggest the search must continue. 'It was exciting, but it immediately raised several red flags because that claim of a potential biosignature would be historic, but also the significance or the strength of the statistical evidence seemed to be too high for the data,' said Dr. Luis Welbanks, a postdoctoral research scholar at Arizona State University's School of Earth and Space Exploration. While the molecules identified on K2-18b by the April study — dimethyl sulfide, or DMS, and dimethyl disulfide, or DMDS — are associated largely with microbial organisms on our planet, scientists point out that the compounds can also form without the presence of life. Now, three teams of astronomers not involved with the research, including Welbanks, have assessed the models and data used in the original biosignature discovery and got very different results, which they have submitted for peer review. Meanwhile, the lead author of the April study, Nikku Madhusudhan, and his colleagues have conducted additional research that they say reinforces their previous finding about the planet. And it's likely that additional observations and research from multiple groups of scientists are on the horizon. The succession of research papers revolving around K2-18b offers a glimpse of the scientific process unfolding in real time. 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Meeting such a threshold will require many steps, Welbanks said, including repeated detections of the same molecule using multiple telescopes and ruling out potential nonbiological sources. While such evidence could be found in our lifetime, it is less likely to be a eureka moment and more a slow build requiring a consensus among astronomers, physicists, biologists and chemists. 'We have never reached that level of evidence in any of our studies,' Madhusudhan wrote in an email. 'We have only found evidence at or below 3-sigma in our two previous studies (Madhusudhan et al. 2023 and 2025). We refer to this as moderate evidence or hints but not a strong detection. I agree with (Luque and Zhang's) claim which is consistent with our study and we have discussed the need for stronger evidence extensively in our study and communications.' 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It's a window into the complexities and nuances of how researchers search for evidence of life beyond Earth — and shows why the burden of proof is so high and difficult to reach. Located 124 light-years from Earth, K2-18b is generally considered a worthy target to scour for signs of life. It is thought to be a Hycean world, a planet entirely covered in liquid water with a hydrogen-rich atmosphere, according to previous research led by Madhusudhan, a professor of astrophysics and exoplanetary science at the University of Cambridge's Institute of Astronomy. And as such, K2-18b has rapidly attracted attention as a potentially habitable place beyond our solar system. Convinced of K2-18b's promise, Madhusudhan and his Cambridge colleagues used observations of the planet by the largest space telescope in operation, the James Webb Space Telescope, to study the planet further. 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The most noticeable features from a gas like dimethyl sulfide stem from a bond of hydrogen and carbon molecules — a connection that can stretch and bend and absorb light at different wavelengths, making it hard to definitively detect one kind of molecule, Zhang said. 'The problem is basically every organic molecule has a carbon-hydrogen bond,' Zhang said. 'There's hundreds of millions of those molecules, and so these features are not unique. If you have perfect data, you can probably distinguish between different molecules. But if you don't have perfect data, a lot of molecules, especially organic molecules, look very similar, especially in the near-infrared.' Delving further into the paper, Luque and Zhang also noticed that the perceived temperature of the planet appeared to increase sharply from a range of about 250 Kelvin to 300 Kelvin (-9.67 F to 80.33 F or -23.15 C to 26.85 C) in research Madhusudhan published in 2023 to 422 Kelvin (299.93 F or 148.85 C) in the April study. 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But ethane does not signify life. Arizona State's Welbanks and his colleagues, including Dr. Matt Nixon, a postdoctoral researcher in the department of astronomy at the University of Maryland College Park, also found what they consider a fundamental problem with the April paper on K2-18b. The concern, Welbanks said, was with how Madhusudhan and his team created models to show which molecules might be in the planet's atmosphere. 'Each (molecule) is tested one at a time against the same minimal baseline, meaning every single model has an artificial advantage: It is the only explanation permitted,' Welbanks said. When Welbanks and his team conducted their own analysis, they expanded the model from Madhusudhan's study. '(Madhusudhan and his colleagues) didn't allow for any other chemical species that could potentially be producing these small signals or observations,' Nixon said. 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'Regardless of what any single author group says right now, we don't have a silver bullet. But that is exactly why this is exciting, because we know that we're the closest we have ever been (to finding a biosignature), and I think we may get it within our lifetime, but right now, we're not there. That is not a failure. We're testing bold ideas.'

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