An Energetic Eruption With Associated SO 1.707 Micron Emissions at Io's Kanehekili Fluctus and a Brightening Event at Loki Patera Observed by JWST
Imke de Pater, E. Lellouch, D. F. Strobel, Katherine de Kleer, Thierry Fouchet, Michael H. Wong, Bryan J. Holler, John Stansberry, P. M. Fry, Michael E. Brown, D. Bockelée–Morvan, Samantha K. Trumbo, Leigh N. Fletcher, Matthew M. Hedman, Edward Molter, M. R. Showalter, Matthew S. Tiscareno, S. Cazaux, R. Hueso, Statia Luszcz‐Cook, Henrik Melin, Chris Moeckel, A. Mura, Glenn S. Orton, Lorenz Roth, Joachim Saur, F. Tosi
Abstract
Abstract We observed Io with the James Webb Space Telescope (JWST) while the satellite was in eclipse, and detected thermal emission from several volcanoes. The data were taken as part of our JWST‐ERS program #1373 on 15 November 2022. Kanehekili Fluctus was exceptionally bright, and Loki Patera had most likely entered a new brightening phase. Spectra were taken with NIRSpec/IFU at a resolving power R ≈ 2,700 between 1.65 and 5.3 µm. The spectra were matched by a combination of blackbody curves that showed that the highest temperature, ∼1,200 K, for Kanehekili Fluctus originated from an area ∼0.25 km 2 in size, and for Loki Patera this high temperature was confined to an area of ∼0.06 km 2 . Lower temperatures, down to 300 K, cover areas of ∼2,000 km 2 for Kanehekili Fluctus, and ∼5,000 km 2 for Loki Patera. We further detected the a 1 Δ ⇒ X 3 Σ − 1.707 µm rovibronic forbidden SO emission band complex over the southern hemisphere, which peaked at the location of Kanehekili Fluctus. This is the first time this emission has been seen above an active volcano, and suggests that the origin of such emissions is ejection of SO molecules directly from the vent in an excited state, after having been equilibrated at temperatures of ∼1,500 K below the surface, as was previously hypothesized.