ESA title
The Cometary Secondary Ion Mass
Science & Exploration

Science from the Orbiter (2)

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ESA / Science & Exploration / Space Science / Rosetta

COSIMA (Cometary Secondary Ion Mass Analyser):Will analyse the characteristics of dust grains emitted by the comet, including their composition and whether they are organic or inorganic.

The Micro-Imaging Dust Analysis System
The Micro-Imaging Dust Analysis System

MIDAS (Micro-Imaging Dust Analysis System): Studies the dust environment around the asteroids and comet. It provides information on particle population, size, volume and shape.

The Comet Nucleus Sounding Experiment by Radiowave Transmission
The Comet Nucleus Sounding Experiment by Radiowave Transmission

CONSERT (Comet Nucleus Sounding Experiment by Radiowave Transmission): Probes the comet's interior by studying radio waves that are reflected and scattered by the nucleus.

The Grain Impact Analyser and Dust
The Grain Impact Analyser and Dust

GIADA (Grain Impact Analyser and Dust Accumulator):Measures the number,mass, momentum and velocity distribution of dust grains coming from the nucleus and from other directions (reflected by solar radiation pressure).

The Rosetta Plasma Consortium
The Rosetta Plasma Consortium

RPC (Rosetta Plasma Consortium): Five sensors measure the physical properties of the nucleus, examine the structure of the inner coma,monitor cometary activity, and study the comet's interaction with the solar wind.

RSI (Radio Science Investigation): Shifts in the spacecraft's radio signals are used to measure the mass, density and gravity of the nucleus, to define the comet's orbit, and to study the inner coma. RSI will also be used to measure the mass and density of Siwa, and to study the solar corona during the periods when the spacecraft, as seen from Earth, is passing behind the Sun.

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