Work

Volcanic satellites tidally venting Na, K, and SO2 in optical and infrared light

Year: 2025
Type: article
Abstract: ABSTRACT Recent infrared spectroscopy from the James Webb Space Telescope (JWST) has spurred analyses of common volcanic gases such as carbon dioxide (CO$_2$), sulphur dioxide (SO$_2$), alongside alkali metals sodium (Na i) and potassium (K i) surrounding the hot Saturn WASP-39 b. We report more than an order-of-magnitude of variability in the density of neutral Na, K, and SO$_2$ between ground-based measurements and JWST, at distinct epochs, hinting at exogenic physical processes similar to those sourcing Io’s extended atmosphere and torus. Tidally heated volcanic satellite simulations sputtering gas into a cloud or toroid orbiting the planet are able to reproduce the probed line-of-sight column density variations. The estimated SO$_2$ flux is consistent with tidal gravitation predictions, with a Na/SO$_2$ ratio far smaller than Io’s. Although stable satellite orbits at this system are known to be ${<}$15.3 h, several high-resolution alkali Doppler shift observations are required to constrain a putative orbit. Due to the Roche limit interior to the planetary photosphere at ${\sim}$8 h, atmosphere–exosphere interactions are expected to be especially important in this system.
Language: English
Open Access status: gold
Estimated APC paid: $3,046
OpenAlex ID: W4414510301
FWCI: 0.452
Cites: 60
Cited by: 1
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