Pressures in the hydrospheres of large ocean worlds extend to ranges exceeding those in
Earth deepest oceans. In this regime, dense water ices and other high-pressure phases …

The icy satellites of Jupiter and Saturn are perhaps the most promising places in the Solar
System regarding habitability. However, the potential habitable environments are hidden …

Geophysical measurements can reveal the structures and thermal states of icy ocean
worlds. The interior density, temperature, sound speed, and electrical conductivity thus …

Gibbs energy representations for ices II, III, V, and VI are reported. These were constructed
using new measurements of volumes at high pressure over a range of low temperatures …

Sodium chloride is expected to be found on many of the surfaces of icy moons like Europa
and Ganymede. However, spectral identification remains elusive as the known NaCl …

Electrolytes play an important role in the internal structure and dynamics of water-rich
satellites and potentially water-rich exoplanets. However, in planets, the presence of a large …

Prior analyses of oceanic magnetic induction within Jupiter's large icy moons have assumed
uniform electrical conductivity. However, the phase and amplitude responses of the induced …

Color centers are versatile systems that generate quantum light, sense magnetic fields and
produce spin‐photon entanglement. We review how these properties have pushed the limits …

Hydrogen bond symmetrisations in H-bonded systems triggered by pressure-induced
nuclear quantum effects (NQEs) is a long-known concept but experimental evidence in high …

We have studied the H 2 O ice VII–ice X phase transition at room temperature by performing
three quasicontinuous synchrotron time-resolved x-ray-diffraction experiments in a dynamic …