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Turns Out The Most Distant Star Ever Discovered Is Not Actually A Star

This image from the NASA/ESA/CSA James Webb Space Telescope shows a massive galaxy cluster called WHL0137-08, and at the right, an inset of the most strongly magnified galaxy known in the Universe’s first billion years: the Sunrise Arc. Within that galaxy is the most distant star ever detected, first discovered by the NASA/ESA Hubble Space Telescope. Webb’s NIRCam (Near-Infrared Camera) instrument reveals the star, nicknamed Earendel, to be a massive B-type star more than twice as hot as our Sun, and about a million times more luminous. Stars of this mass often have companions. Astronomers did not expect Webb to reveal any companions of Earendel since they would be so close together and indistinguishable on the sky. However, based solely on the colours of Earendel detected by Webb, astronomers think they see hints of a cooler companion star. Webb’s NIRCam also shows other remarkable details in the Sunrise Arc. Features include both young star-forming regions and older established star clusters. On either side of the wrinkle of maximum magnification, which runs right through Earendel, these features are mirrored by the distortion of the gravitational lens. The region forming stars appears elongated, and is estimated to be less than 5 million years old. Smaller dots on either side of Earendel are two images of one older, more established star cluster, estimated to be 10 million years or older. Astronomers determined this star cluster is gravitationally bound and likely to persist until the present day. This shows us how the globular clusters in our own Milky Way might have looked when they formed 13 billion years ago. [Image description: The image is split in half vertically to create two images. In the left image, a black background is scattered with hundreds of small galaxies of different shapes, ranging in colour from white to yellow to red. Some galaxies, mostly the redder galaxies, are distorted, appearing to be stretched out or mirror imaged. Just a little bit above the centre, there is a bright source of light, a star, with 8 bright diffraction spikes extending out from it. The right image is a zoomed-in portion of the image at the left, showing a particularly long, red, thin line that stretches from 1 o’clock to 7 o’clock. There are several bright dots, some thicker than others, along this line, with one labelled as Earendel.]

When astronomers first spotted Earendel with the Hubble Space Telescope in 2022, it was hailed as the most distant star ever observed, located about 12.9 billion light years away. But new data from the James Webb Space Telescope is making scientists rethink that record-breaking discovery. Instead of being a single, massive star, Earendel might actually be a tightly packed cluster of stars.

The find was detailed in The Astrophysical Journal after Webb delivered higher-resolution spectra of the object. According to researchers, some of the light signatures looked more like those seen in ancient globular clusters than those of a lone star. That’s a big shift, because clusters behave very differently from individual stars when it comes to formation, brightness, and lifespan.

Image credits: NASA

When Earendel was first identified in the Sunrise Arc galaxy, scientists believed it represented a single, extraordinarily bright star that had formed less than a billion years after the Big Bang. If it were truly a star, it would have been an unprecedented window into the first stellar generations. But if it’s really a cluster, it still remains scientifically important—it would provide evidence that even in the earliest days of the universe, stars were already gathering into dense groups.

The challenge is that Earendel’s visibility relies on gravitational lensing, where the light is magnified by the gravity of an intervening galaxy cluster. This makes the object bright enough for telescopes to see, but it also distorts the image. Disentangling whether the light is from one star or many requires extremely careful modeling.

Astronomers are now looking for subtle variations that could reveal its true nature. For example, in a cluster, individual stars can cause microlensing events, where the brightness flickers slightly. Detecting those small changes could confirm that Earendel is more than one source. Researchers are also analyzing spectral fingerprints that might indicate a mix of stellar types rather than the uniform signal expected from a single giant star.

Even if the name “most distant star” no longer applies, the implications are still huge. Finding what could be a cluster at that distance means scientists can study the formation of compact stellar systems far earlier in cosmic history than previously thought. Webb’s precision has turned what once looked like a solitary beacon into something potentially more complex—and that complexity may end up teaching us even more about how the universe built its first structures.

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