SUBICE is a project of the University of Bern, the University of Applied Sciences and Arts, Western Switzerland (HES-SO), and Thales-Alenia Space Switzerland (TASCH).
The primary aim of SUBICE is to explore and establish experimental and numerical techniques for determining how water ice and refractory materials are physically connected within a cometary nucleus at scales of a centimetre or less. This is motivated, firstly, by a need to constrain how ices and refractory material combined in the planetesimal formation process in the early epochs of our Solar System, and secondly, by the need to understand specific measurements acquired by the Rosetta spacecraft at comet 67P/Churyumov-Gerasimenko that point to a complexity beyond that incorporated in current models.
SUBICE is supported through a MARVIS (Multidisciplinary Advanced Research Ventures in Space) programme of the Swiss Department for Business, Education, and Research (SBFI).