The key points:
The evidence remains indirect, but computer models support the hypothesis that heat from Pluto's interior melts nitrogen ice at the base of the glacier, where it collects in pressurized reservoirs before bursting to the surface .
A separate study led by Amanda Sickafoose (Planetary Science Institute), also published in August 2026 in The Planetary Science Journal, reports the first observed decline in Pluto's atmospheric pressure since its atmosphere was discovered in 1988 .
Scientists had predicted this freeze-out as early as 1996, but the 2026 study provides the first observational confirmation that the process has begun in earnest .
Taken together, the 2026 results paint a picture of a Pluto that is simultaneously losing its atmosphere as it cools while also maintaining geologic activity via subsurface reservoirs that occasionally release liquid nitrogen onto the surface. The dark streaks on Sputnik Planitia may be places where liquid nitrogen recently reached and flowed across the surface, while occultation data confirm that the atmosphere at higher altitudes has already begun to thin significantly .
Both findings were published in The Planetary Science Journal and drew on data collected years earlier — the New Horizons images from 2015 and occultation measurements spanning 2017–2023. The fact that such dramatic discoveries are still emerging from a single flyby and ground-based observations underscores how much Pluto continues to surprise us.
As one researcher put it, "Pluto never stops surprising us" — and the 2026 studies confirm that the dwarf planet remains one of the most dynamic and enigmatic worlds in our solar system.