

Three station light curves of 2002 XV93’s stellar occultation on 10 January 2024. The flux points (points with error bars) observed at Kyoto (a), Kiso (b) and Fukushima stations (c) overlaid with the synthetic light curves (red lines, assuming a pure CH4 atmosphere and a best-fit surface pressure of 124 nanobars) are shown as a function of time. In panel c, the gray points are the flux points for the individual exposures, and the black points are those binned by a factor of 8. The vertical arrow represents the closest approach time to the shadow edge at Fukushima, at 13:12:50.818 UT. — astro-ph.EP
Trans-Neptunian objects (TNOs) in the outer Solar System are predominantly small, icy worlds long presumed to be atmosphereless except for the largest bodies.
Until now, Pluto has been unique among TNOs in exhibiting a substantial atmosphere (nitrogen with trace methane and carbon monoxide) at microbar pressure levels. All other known TNOs, including ~ 1000-km-sized bodies such as Eris, Haumea, Makemake, and Quaoar, have shown no detectable atmospheres in stellar occultation observations, with surface pressure upper limits of order 1-100 nanobars.
Here we report the first detection of an atmosphere around a TNO besides Pluto. A stellar occultation by the ~ 250-km-radius plutino (612533) 2002 XV93 on 10 January 2024 revealed a refractive signature, indicating the presence of a thin atmosphere.
The derived surface pressure is 100-200 nanobars, i.e. approximately a hundred times lower than Pluto’s and yet significantly above previous limits for other larger bodies. This discovery provides the first evidence that even a sub-1000-km TNO can retain an atmosphere, challenging current paradigms of volatile retention.
Our findings indicate that a fraction of distant icy minor planets can exhibit atmospheres possibly caused by ongoing cryovolcanic activity or a recent impact event of a small icy object.
Ko Arimatsu, Fumi Yoshida, Tsutomu Hayamizu, Satoshi Takita, Katsumasa Hosoi, Takafumi Ootsubo, Jun-ichi Watanabe
Comments: Original submitted version; 20 pages, 4 figures, 3 extended data figs. The revised and published version appears in Nature Astronomy under the title “Detection of an atmosphere on a trans-Neptunian object beyond Pluto”
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2605.02243 [astro-ph.EP] (or arXiv:2605.02243v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2605.02243
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Related DOI:
https://doi.org/10.1038/s41550-026-02846-1
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Submission history
From: Ko Arimatsu
[v1] Mon, 4 May 2026 05:35:46 UTC (10,180 KB)
https://arxiv.org/abs/2605.02243
Astrobiology, Astrogeology, Astrochemistry,






