Rosetta instruments

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Rosetta orbiter showing narrow-angle and wide-angle cameras.
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Image courtesy NASA.

The Rosetta spacecraft has many instruments that it will use to measure various aspects of Comet Churyumov-Gerasimenko during its visit. This diagram shows the two cameras that make up the OSIRIS imaging system: the Narrow-Angle Camera (NAC) and the Wide-Angle Camera (WAC). The two cameras are shown in gray in the diagram.

The instruments on the Rosetta orbiter are described in detail in the table below. The instruments on the Rosetta lander are described on a separate page.


Instrument Purpose Principal investigator
ALICE - Ultraviolet Imaging Spectrometer Analyzes gases in comet's coma and tail Dr. Alan Stern, Southwest Research Institute, USA
CONSERT - Comet Nucleus Sounding Experiment by Radiowave Transmission Radio sounding, nucleus tomography - uses radio waves to probe comet's interior Prof. Wlodek Kofman, Ecole Nationale Superieure d'Ingenieurs, France
COSIMA - Cometary Secondary Ion Mass Analyser Dust mass spectrometer - chemical analysis of dust grains Dr. Jochen Kissel, Max-Planck-Institut für Extraterrestrische Physik, Germany
GIADA - Grain Impact Analyser and Dust Accumulator Dust velocity and impact measurement - number, masses, and velocities of dust grains coming from the comet Prof. Luigi Colangeli, Osservatorio Astronomico di Capodimonte, Italy
MIDAS - Micro-Imaging Dust Analysis System Micro-imaging dust analysis - physical analysis (size, shape, etc.) of dust grains Prof. Willi Riedler, Space Research Institute, Austria
MIRO - Microwave Instrument for the Rosetta Orbiter Microwave spectrometer - measures major gases and sub-surface temperature of the comet Dr. Samuel Gulkis, Jet Propulsion Laboratory, USA
OSIRIS - Optical, Spectroscopic, and Infrared Remote Imaging System Wide-angle and narrow-angle cameras Dr. Horst Uwe Keller, Max-Planck-Institut für Aeronomie, Germany
ROSINA - Rosetta Orbiter Spectrometer for Ion and Neutral Analysis Neutral gas and ion mass spectrometer - chemical analysis of comet's atmosphere Prof. Hans Balsiger, University of Bern, Switzerland
RPC - Rosetta Plasma Consortium Plasma measurements - 5 sensors measure physical properties of the nucleus, the structure of the coma, and the comet's interaction with the solar wind Dr. Rolf Boström, Swedish Inst. of Space Physics, Sweden
Dr. James Burch, Southwest Research Institute, USA
Prof. Karl-Heinz Glassmeier, Technische Universität, Germany
Prof. Rickard Lundin, Swedish Institute of Space Physics, Sweden
Dr. Jean-Gabriel Trotignon, LPCE/CNRS, France
RSI - Radio Science Investigation Spacecraft's radio signals are used to measure the mass & density of the nucleus and to define the comet's orbit. Dr. Martin Pätzold, Universität Köln, Germany
VIRTIS - Visible and Infrared Thermal Imaging Spectrometer Maps the temperature on the surface of the nucleus & identifies gases Dr. Angioletta Coradini, Istituto di Astrofisica Spaziale, Italy

Rosetta space mission

ESA's Rosetta home page

Rosetta instruments

Click for full size

Rosetta orbiter showing cameras.
Click on image for full size (23K JPEG)
Image courtesy NASA.

The Rosetta spacecraft has many instruments that it will use to measure Comet Churyumov-Gerasimenko during its visit. This diagram shows the two cameras that make up the OSIRIS imaging system: the Narrow-Angle Camera (NAC) and the Wide-Angle Camera (WAC). The two cameras are shown in gray in the diagram. The NAC takes pictures of objects when they are far away. The WAC takes pictures of objects when the spacecraft is very near them.

The instruments on the Rosetta orbiter are described in the table below. The instruments on the Rosetta lander are described on a separate page.


Instrument Purpose
ALICE Analyzes gases in comet's coma and tail
CONSERT Uses radio waves to probe comet's interior
COSIMA Chemical analysis of dust grains
GIADA Dust velocity and impact measurement - number, masses, and velocities of dust grains coming from the comet
MIDAS Micro-imaging dust analysis - physical analysis (size, shape, etc.) of dust grains
MIRO Measures major gases and sub-surface temperature of the comet
OSIRIS Wide-angle and narrow-angle cameras
ROSINA Chemical analysis of comet's atmosphere
RPC Plasma measurements - 5 sensors measure physical properties of the nucleus, the structure of the coma, and the comet's interaction with the solar wind
RSI Spacecraft's radio signals are used to measure the mass & density of the nucleus and to define the comet's orbit
VIRTIS Maps the temperature on the surface of the nucleus & identifies gases

Rosetta space mission

ESA's Rosetta home page

Rosetta instruments

Click for full size

Rosetta orbiter showing cameras.
Click on image for full size (23K JPEG)
Image courtesy NASA.

This picture shows two of the instruments on the Rosetta spacecraft. The instruments are colored gray in the picture. These instruments are two of the cameras on Rosetta. NAC is the Narrow-Angle Camera. It takes pictures of objects when they are far away. WAC is the Wide-Angle Camera. It takes pictures of objects when the spacecraft is very near them. Rosetta will use these instruments to study Comet Churyumov-Gerasimenko.

Rosetta has many other instruments. They are listed lower on this page. The instruments on the Rosetta lander are listed on another page.


Instruments What they do
ALICE, COSIMA, ROSINA Measure the kinds of chemicals the comet is made of
CONSERT Uses radio waves to "see" what the inside of the comet is like
GIADA Measures dust coming from comet
MIDAS, OSIRIS Cameras - take pictures
MIRO, VIRTIS Measure temperature
RPC, RSI Measure the comet's size, mass, and density

Rosetta space mission

ESA's Rosetta home page


Last modified January 21, 2004 by Randy Russell.
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