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A tiny trans-Neptunian object beyond Neptune, cataloged (612533) 2002 XV93, appears to be encircled by an ultra-thin atmosphere, according to a study led by Ko Arimatsu of Japan’s National Astronomical Observatory published in Nature Astronomy in May 2026.
Observers at three Japanese sites monitoring a January 10, 2024 stellar occultation recorded a gradual dimming of starlight — a refractive signature consistent with a gaseous envelope rather than a sharp occultation edge.
The putative atmosphere is extremely tenuous, roughly 5 million to 10 million times thinner than Earth’s atmosphere and an estimated 50–100 times thinner than Pluto’s.
Possible sources include recent cometary impact or active cryovolcanic outgassing, though alternative explanations such as rings were considered less consistent with the data.
Authors call for independent verification — particularly spectroscopic follow-up with facilities like NASA’s James Webb Space Telescope — to confirm composition and persistence.
Senior planetary scientists, including Alan Stern, have urged caution pending more observations.
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