- an "imaging system," i.e., a camera;
- radar calibrated to measure the thickness of the icy crust and the ocean underneath;
- sensitive magnetometers, also intended to study the crust
- a "mapping imaging spectrometer" to study the chemical composition of the surface
- a thermal imaging system to look for plumes of water erupting into space
- an ultraviolet spectrograph to do the same, and to study the chemical composition of the plumes
- a mass spectrometer to study the moon's extremely thin atmosphere;
- a dust analyzer to study the composition of small particles ejected from the surface
The idea behind most of these instruments is that if Europa is regularly ejecting plumes of water into space, we can study the composition of its ocean by sampling those plumes, without having to drill through miles of ice. Two approaches are planned: to study gases released by the plumes as they dissipate into space, by flying through them; and to examine the surface hoping that deposits have been left there by the plumes. The fantasy would be finding organic molecules in the plumes that point toward life under the surface. But even if the ocean is sterile, it is still an alien ocean of unknown chemistry, so knowing what is in it would be cool.
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