Jupiter's Galilean satellite Io is one of the most remarkable objects in our Solar System. The
tidal heating Io undergoes through its orbital resonance with Europa and Ganymede has …

Since the Voyager mission flybys in 1979, we have known the moon Io to be both
volcanically active and the main source of plasma in the vast magnetosphere of Jupiter …

Jupiter's moon Io hosts extensive volcanism, driven by tidal heating. The isotopic
composition of Io's inventory of volatile chemical elements, including sulfur and chlorine …

We present a thermal observation of Callisto's leading hemisphere obtained using the
Atacama Large Millimeter/submillimeter Array at 0.87 mm (343 GHz). The angular resolution …

We present first results derived from the largest collection of contemporaneously recorded
Jovian sodium nebula and Io plasma torus in [S II] 6731 Å images assembled to date. The …

We present thermal observations of Ganymede from the Atacama Large Millimeter Array
(ALMA) in 2016–2019 at a spatial resolution of 300–900 km (0 farcs 1–0 farcs 2 angular …

We present best-fit values of porosity—and the corresponding effective thermal inertiae—
determined from three different depths in Europa's near-subsurface (∼ 1–20 cm). The …

Stable isotope fractionation of sulfur offers a window into Io's tidal heating history, which is
difficult to constrain because Io's dynamic atmosphere and high resurfacing rates leave it …

In the original plate-tectonic centric framework for Earth evolution as proposed in the 1960s,
the term 'subduction'was initially applied to the down thrusting of oceanic lithosphere below …

Decline and recovery timescales surrounding eclipse are indicative of the controlling
physical processes in Io's atmosphere. Recent studies have established that the majority of …