Plasma processes at comet 67P/Churyumov-Gerasimenko

Comet 67P

Outgassing from 67P. Credit: ESA/Rosetta/NavCam

IRF Uppsala contributes one of the instruments on board the Rosetta orbiter, a kind of weather station known as a Langmuir probe (LAP). Together with the other instruments in the Rosetta Plasma Consortium, we investigate the ionized component of the gas oozing out of the icy nucleus and how it interacts with the dust from the comet and the ever changing solar wind. At other comets, the environment is known to structure itself into several regions with different properties. From Rosetta, we are already learning that this picture is very simplified, as we follow how the comet environment changes with distance to the Sun.

Rosetta plasma consortium.

Rosetta plasma consortium instruments. Image: ESA/RPC

Rosetta is not like any other comet mission. Previous spacecraft have just flown by at high speed, at best catching a few shots, recording some waves and perhaps a few dust grains during a few minutes or (at best) hours. Rosetta will spend two years close to the nucleus, moving at relative speed to the nucleus of around a meter per second or even slower. This exploration at walking pace is something really unique not only for comets but for space science as a whole, allowing studies of complex plasma phenomena in a way that has never before been possible.

Plasma boundaries at a comet

Plasma boundaries at a comet. Image: NASA/JPL

Created by Michiko Morooka at

Last modified by Michiko Morooka at