[1]2015astro-ph.EPPreprint
Pits formation from volatile outgassing on 67P/Churyumov-Gerasimenko
O. Mousis, A. Guilbert-Lepoutre, B. Brugger & 8 others
What they foundThe active pits Rosetta saw could form when buried ice cages (clathrates) break down or amorphous ice crystallises at the depth of the pits.
Why it mattersIt links the comet's dramatic pits to processes inside its ice, either as sinkholes or after outbursts.
What they studied
Computer models of heat flowing into the subsurface of 67P's Seth region.
[2]2023astro-ph.EPPeer-reviewed
The ice composition close to the surface of comet 67P/Churyumov-Gerasimenko
Matthias Laeuter, Tobias Kramer, Martin Rubin & 1 other
What they foundThe team mapped where 14 gases, from water and CO₂ to methanol and ethanol, come off 67P's surface over the two-year mission.
Why it mattersLinking gas output to surface patches shows how the ice just below the surface is distributed.
What they studied
Rosetta ROSINA COPS and DFMS gas-density measurements, fitted onto the comet's shape model.
[3]2017astro-ph.EPPeer-reviewed
Aggregate dust particles at comet 67P/Churyumov-Gerasimenko
Mark S. Bentley, Roland Schmied, Thurid Mannel & 9 others
What they foundDust at 67P is made of aggregates of smaller, elongated grains.
Why it mattersThese are about as pristine as cometary dust gets, so they reveal how dust stuck together when planets were forming.
What they studied
In-place measurements by an instrument on the Rosetta orbiter that collected dust particles.