Constraints from Comets on the Formation and Volatile Acquisition of the Planets and Satellites

The first dedicated ice giants mission

The mysteries of the Uranus system can be unlocked through interdisciplinary exploration.

Theory meets experiment for elucidating the structure and stability of non-covalent complexes: water–amine interaction as a proof of concept

A joint experimental-theoretical spectroscopic investigation has focused on a better understanding of the nature of weak, non-covalent interactions in amine-water model systems.

Oxygen fractionation in dense molecular clouds

We have developed the first gas-grain chemical model for oxygen fractionation (also including sulphur fractionation) in dense molecular clouds, demonstrating that gas-phase chemistry generates variable oxygen fractionation levels, with a particularly strong effect for NO, SO, O2, and SO2. This large effect is due to the efficiency of the neutral 18O + NO, 18O + SO, and 18O + O2 exchange reactions. The modeling results were compared to new and existing observed isotopic ratios in a selection of cold cores. The good agreement between model and observations requires that the gas-phase abundance of neutral oxygen atoms is large in the observed regions. The S16O/S18O ratio is predicted to vary substantially over time showing that it can be used as a sensitive chemical proxy for matter evolution in dense molecular clouds.