Solar System Physics and Space Technology

IRF and the ESA Rosetta mission


(Picture: ESA)

The European Space Agency's Rosetta spacecraft will visit a comet called 67P/Churyomov-Gerasimenko, catching up with the comet in its elliptic orbit around the Sun in 2014 and following it closely for more than a year as it approaches the Sun. IRF participates with two instruments on board: an Ion Composition Analyser (ICA), provided by IRF in Kiruna, and a dual Langmuir probe (LAP), provided by IRF in Uppsala. These instruments concentrate on measuring the partly ionized gas and dust exhausted by the comet nuclei (about 4 km across) as it is heated by the Sun. The IRF instruments will be the first of their kind in long-time orbit around a comet. Previous missions, such as the ESA spacecraft Giotto to comets Halley and Grigg-Skjellerup, have only by-passed comets at great speed, while Rosetta will move around Churyomov-Gerasimenko with a speed on the order of a meter per minute, giving unprecedented measurement opportunities. Rosetta was launched from Kourou in French Guiana on 2 March 2004.


Launched: 2 March 2004
Destination: Comet 67P/Churyomov-Gerasimenko
IRF instruments:

RPC-ICA (Rosetta Plasma Consortium - Ion Composition Analyser, PI: Rickard Lundin)

RPC-LAP (Rosetta Plasma Consortium - Langmuir probe, PI: Anders Eriksson)

Contact: Scientific information: Dr Hans Nilsson, tel. +46-980-79127, hans.nilsson*irf.se (ICA); Dr Anders Eriksson, tel. +46-18-471 5945, aie@irfu.se (LAP)

Technical information (ICA): Herman Andersson, tel. +46-980-79034, herman.andersson@irf.se
Satellite page: Rosetta homepage at ESA

Press releases:

Links:


[IRF home] [SSPT home]

Updated by webmaster*irf.se, 2010-07-07