hi SBN Mission Support: Rosetta
SBN Small Bodies Mission Support

Rosetta Mission

The Rosetta Mission is the third cornerstone mission in ESA's Horizon 2000 program. The purpose of the mission is to rendezvous with the comet 67P/Churyumov-Gerasimenko 1, gather information on the comet as the spacecraft orbits it, and to land a package of instruments on the surface of the comet. Scientific objectives of the mission are to study the origin of comets, and the relationship between cometary and interstellar material.

The Rosetta spacecraft launched in March 2004 from Kourou, French Guiana. On its way to the comet it will fly by two asteroids, (2867) Steins on 5 September 2008 and (21) Lutetia on 10 July 2010. Rosetta will rendezvous with 67P/C-G 1 and gather data on the comet for 18 months.

The scheduled end of mission date is 2014.

The Rosetta Mission web site is maintained by the European Space Agency (ESA).

The SBN in cooperation with ESA will archive Earth-based observations of comet 67P/Churyumov-Gerasimenko 1.

Mission Home Page Instruments Mission Data Target Data

Orbiter Instruments

Instrument/Investigation Measuring Small Bodies Data
available below
Microwave Spectroscopy
(MIRO)
Abundance of major volatile species; isotope ratios

THERMAL-VACUUM TEST

COMMISSIONING

FIRST EARTH SWINGBY

COMET 9P/TEMPEL 1 & CRUISE 2

UV-Spectrometer
(ALICE)
Abundance of highly volatile molecular species, particularly including the noble gases Ar, Ne and He, and the molecules CO, CO2, and N2; the abundance of atoms H, C, N, O and S

COMMISSIONING 1 PHASE

Includes C/2002 T7 (LINEAR)

CRUISE 1 CHECKOUT PHASE

COMMISSIONING 2 PHASE

EARTH SWING-BY 1 PHASE

CRUISE 2 PHASE

Includes 9P/Tempel 1

MARS SWING-BY PHASE

Includes Jupiter and Io plasma torus

EARTH SWING-BY 2 PHASE

Rosetta Orbiter Plasma Consortium
(RPC)
IES Ions, electrons, dust particles, and electromagnetic fields around the cometary object

COMMISSIONING 1 PHASE

  • raw edited data

CRUISE 1 CHECKOUT PHASE

  • raw edited data

EARTH SWING-BY 1 PHASE

  • raw edited data

MARS SWING-BY PHASE

Includes Jupiter and Io plasma torus

  • raw edited data

Visible and Infrared Thermal Imaging Spectrometer
(VIRTIS)
Emission bands and warm dust  links
Optical, Spectroscopic, and Infrared Remote Imaging System
(OSIRIS)
Imaging of the the nucleus and the the dust and gas directly above the surface of the nucleus links
Rosetta Orbiter Spectrometer for Ion and Neutral Analysis
(ROSINA)
Neutral gas and ion mass links
Micro-Imaging Dust Analysis System
(MIDAS)
Grain morphology in the nanometer to micrometer range links
Grain Impact Analyser and Dust Accumulator
(GIADA)
Dust velocity and impact momentum links
Comet Nucleus Sounding Experiment By Radiowave Transmission
(CONSERT)
Nucleus tomography, permittivity, and absorption links
Radio Science
(RSI)
Cometary orbit; nucleus mass, bulk density and gravity coefficients; dust grain distribution and plasma content of the inner coma links
Cometary Secondary Ion Mass Analyzer
(COSIMA)
Chemical composition of elemental and molecular cometary particles links

Lander Instruments

Instrument/Investigation Measuring Small Bodies Data
available below
Stereo Pan Camera
(ÇIVA/ROLIS)
Morphology of the cometary object links
Methods of Determining and Understanding Light Elements from Unequivocal Stable Isotope Compositions
(MODULUS/Ptolemy)
Isotopic composition of the major volatiles links
Comet Nucleus Sounding Experiment By Radiowave Transmission
(CONSERT)
Nucleus tomography, permittivity, and absorption links
Alpha-Proton-X-ray Spectrometer
(APXS)
Elemental composition links
Cometary Sampling and Composition Experiment
(COSAC)
Elemental and molecular composition links
Surface Electrical, Seismic and Acoustic Monitoring Experiments
(SESAME)
Mechanic/elastic properties and permittivity of the cometary surface; dust impact and production rate links
RoLand Magnetic field investigation and Plasma monitor
(ROMAP)
Magnetic field components; interaction of cometary object with the solar wind links
Multi-Purpose Sensors For Surface and Sub-Surface Science
(MUPUS)
Physical properties and composition (elemental, isotopic, molecular and mineralogical) of the nucleus links
Drill and Sampling Device
(SD2)
This experiment is designed to carry out the drilling, sampling, and delivery of the cometary surface and subsurface material. The collected samples will be used by the other lander experiments COSAC, MODULUS/Ptolemy, and ÇIVA. links

Mission Data

Instrument/
Investigation
Description
Target Description of Available Data Data Link
No data available yet

Other Data Sets Targeting this Object

Target Target Type Other Data Sets Targeting this Object
(2867) Steins Asteroid  
(21) Lutetia Asteroid  
67P/Churyumoc-Gerasimenko 1 Comet