Scientists have spotted a distant supernova unleashed by a collapsing star just 1 billion years after the birth of the universe.
The James Webb Space Telescope (JWST) captured images of the Type II supernova on Sept. 1 and Oct. 8, 2025.Dubbed “Eos,” after the Titan goddess of dawn in Greek mythology, the supernova will help scientists understand how stars and galaxies evolve over billions of years, researchers reported jan. 7 on the preprint server arXiv.
Deaths of the earliest stars
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SN Eos: A Distant Supernova Observed by the James Webb Space Telescope
SN Eos, a supernova observed at a redshift of approximately z=9.5, is among the most distant supernovae detected to date, providing insights into the early universe. Observations suggest it is indeed likely nearing the end of its brightness plateau, a characteristic phase in supernova evolution.
The discovery was made using the James Webb Space Telescope (JWST), which is designed to observe the universe at infrared wavelengths, allowing it to see objects too distant and faint for other telescopes.
as of January 20, 2026, no further peer-reviewed publications have superseded the initial findings regarding SN eos. ongoing observations are expected to refine our understanding of its properties.
Characteristics of SN Eos and its Implications for Early Star Populations
SN Eos appears to be a Type II supernova, resulting from the core collapse of a massive star. This type of supernova is expected to be common in the early universe, as it signals the death of massive, short-lived stars.
The supernova’s properties are being compared to models of Population III stars – the first generation of stars formed after the Big Bang – which are theorized to have been significantly more massive than stars formed later. Determining if Eos’s characteristics align with these models is crucial for understanding the early universe.
For example, the European Space Agency reported that JWST’s observations of Eos are helping scientists to understand the composition of the early universe and the processes that led to the formation of heavier elements.
The Role of JWST in Studying High-Redshift Supernovae
The James Webb Space Telescope is uniquely equipped to detect and study high-redshift supernovae like Eos. Redshift is a measure of how much the light from an object has been stretched due to the expansion of the universe; higher redshift corresponds to greater distance and earlier times in the universe’s history.
JWST’s infrared capabilities are essential because the light from distant objects is redshifted into the infrared part of the spectrum. Traditional optical telescopes are less effective at detecting this redshifted light.
In November 2023, Space.com reported that the discovery of SN eos was a “critical step” towards understanding the lives and deaths of the first stars, the origins of elements, and the assembly of early galaxies, directly aligning with JWST’s core mission objectives.
future Research and confirmation
Scientists emphasize the need for further observations of early supernovae to confirm whether SN Eos’s properties are representative of massive stars and supernovae in the early universe. A larger sample size will allow for more robust statistical analysis and a better understanding of the diversity of early stellar populations.
Ongoing and future JWST observations are planned to search for and characterize more distant supernovae, providing a more complete picture of star formation and evolution in the early universe.
The Space Telescope Science institute, which operates JWST, continues to release data and support research efforts aimed at unraveling the mysteries of the early universe, including the study of distant supernovae like SN Eos.
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