The trans-Neptunian object (612533) 2002 XV93, about 500 km in diameter, has mysteriously developed a thin atmosphere (exosphere) in the Kuiper belt.
The atmosphere was detected using a combination of professional and amateur telescopes, with a surface pressure of 100-200 nanobars, millions of times thinner than Earth’s.
Possible causes include cryovolcanism or a recent impact, as such a thin atmosphere would otherwise dissipate within a thousand years.
The composition is unknown; it is speculated to be nitrogen with traces of methane and carbon monoxide, but JWST found no evidence of these ices on the surface.
Future observations of atmospheric density over years will help determine its origin: a decrease would suggest an impact, while constant density would indicate ongoing outgassing.
The research results were published in Nature Astronomy.