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

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.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2025-09-15
DOI
https://doi.org/10.1093/mnras/staf1526
Primary Topic
Astro and Planetary Science
Type
article
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article

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

Rishav Garg, Yuk L. Yung, R. M. C. Lopes, Mario Damiano et al.
Monthly Notices of the Royal Astronomical Society
Astro and Planetary Science
article

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

Rishav Garg, Yuk L. Yung, R. M. C. Lopes, Mario Damiano, Carl Schmidt, Andrea Gebek, Luis Welbanks, Raissa Estrela, Moritz Meyer zu Westram, A. Oza, Anthony L. Piro, Renyu Hu, Yamila Miguel, Diana Powell, Armen Tokadjian, Amy Louca, Jeehyun Yang, Aaron Bello-Arufe, Raghav Chari, Pulkit Gupta, Yasuhiro Hasegawa, Athira Unni
article en

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.

Monthly Notices of the Royal Astronomical SocietyVol. 546(1)
Boston University (US), University of Bern (CH), Leiden University (NL), California Institute of Technology (US), Jet Propulsion Laboratory (US), University of California, Santa Cruz (US), University of California, Irvine (US), Ghent University (BE), Indian Institute of Management Indore (IN), University of Chicago (US), Gender Studies (CZ), Portola Pharmaceuticals (United States) (US), Carnegie Observatories (US), Space Research Organisation Netherlands (NL), Arizona State University (US), New York University (US), Indian Institute of Technology Indore (IN), University of Tennessee at Knoxville (US)
Openalex Percentile: Top 82%
Astro and Planetary Science
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