Astronomers Report Possible Thin Atmosphere on Kuiper Belt Object 2002 XV93 During Stellar Occultation
Astronomers detected an atmosphere on the plutino (612533) 2002 XV93, which measures less than 500 kilometres in diameter. The finding came from an occultation observed on 10 January 2024 that showed gradual dimming of starlight over 1.5 seconds. Researchers say the discovery challenges assumptions about small bodies in the outer solar system.
New ScientistAstronomers have detected a thin atmosphere on the trans-Neptunian object (612533) 2002 XV93, one of the smallest solar system bodies yet found with such a feature. The object, located in the Kuiper Belt, belongs to the class known as plutinos. These bodies share the same stable orbit as Pluto, completing three revolutions around the sun for every two made by Neptune.
On 10 January 2024, 2002 XV93 passed in front of a distant star, causing an occultation. Ko Arimatsu at Kyoto University and his colleagues observed the event from three locations in Japan. 5 seconds near the edge of the shadow.
“These gradual changes are best explained if the star’s light was bent by a very thin atmosphere around 2002 XV93,” says Arimatsu. The team estimates the surface pressure of this atmosphere at about 100 to 200 nanobars. That makes it roughly 5 million to 10 million times thinner than Earth’s atmosphere and about 50 to 100 times thinner than Pluto’s tenuous atmosphere.
“You could not breathe it, feel wind from it, or see anything like Earth’s sky,” says Arimatsu. ” Methane, nitrogen and carbon monoxide are the most plausible candidates for the atmosphere’s composition. The object (612533) 2002 XV93 has a diameter of less than 500 kilometres.
It was formally named after the date of its discovery nearly a quarter of a century ago. Possible causes for the atmosphere include volcanic activity, outgassing from the interior of 2002 XV93 or a cosmic collision. “This discovery challenges our conventional view of small worlds in the outer solar system,” says Arimatsu.
“Until now, clearly detectable atmospheres in the solar system were associated with planets, dwarf planets and some large satellites. ” Ben Montet at the University of New South Wales in Sydney, Australia, reacted to the findings by stating there is an atmosphere on 2002 XV93 and we don’t understand why.
“If you’re standing on the surface of this object, you’re not going to see a sky like [what] we have,” Montet said.
” @NewScientist reported that an artist’s impression shows the trans-Neptunian object (612533) 2002 XV93 blocking the light from a distant star. 1038/s41550-026-02846-1.
Key Facts
Story Timeline
3 events- 1990s
(612533) 2002 XV93 discovered and later formally named after its discovery date
1 source@NewScientist - 2024-01-10
2002 XV93 passed in front of a distant star causing an occultation observed from three sites in Japan
1 source@NewScientist - 2026-05-08
Nature Astronomy paper with DOI 10.1038/s41550-026-02846-1 published detailing thin atmosphere detection
1 source@NewScientist
Potential Impact
- 01
Challenges assumption that clearly detectable atmospheres require large bodies such as planets or dwarf planets
- 02
Raises questions about volatile gas supply mechanisms on small icy bodies in outer solar system
- 03
May prompt further occultation surveys of other small trans-Neptunian objects
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