NASA's Webb Hints at Possible Atmosphere Surrounding Rocky Exoplanet  

May 08, 2024 11:00AM (EDT)Release ID: 2024-102
Illustration of a rocky exoplanet and its star. The star is in the background at the lower left and appears somewhat, but not significantly, smaller in the sky than the planet. It has a bright orange-red glow, and appears to have an active surface. The planet is in the foreground to the upper right of the star. The left quarter of the planet (the side facing the star) is lit, while the rest is in shadow. The planet has hints of a rocky, partly molten surface beneath the haze of a thin atmosphere. The boundary between the day and night sides of the planet is fuzzy.

Summary

Gas bubbling up from a lava-covered surface on 55 Cancri e may feed an atmosphere rich in carbon dioxide or carbon monoxide. 

These days, detecting a planetary atmosphere tens or even hundreds of light-years from Earth might not sound like such a big deal. Scientists have found signs of atmosphere surrounding dozens of exoplanets over the past two decades. The catch is, all those planets have thick, hydrogen-dominated atmospheres that are relatively easy to study. The much thinner blankets of gas that almost certainly surround some small, rocky exoplanets have remained elusive.

Researchers think they may have finally caught a glimpse of a volatile-rich atmosphere surrounding a rocky planet. Light emitted by the hot, highly-irradiated exoplanet 55 Cancri e shows compelling evidence for an atmosphere, probably rich in carbon dioxide or carbon monoxide, which may be bubbling from a vast ocean of lava covering the planet’s surface.

The result is the best evidence to date for a rocky planet atmosphere outside our solar system.

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