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Primary Investigator: H. Laakso,
FMI Helsinki. The permittivity changes with the abundance of polar molecules, i.e. especially water. Thus, the content and loss of water in the cometary surface material can be determined, which is assumed to vary at different distances to the sun, also with the comet's 'daytime'. This will help us to learn more of the chemical composition of the entire comet and it's behaviour in loosing his volatile material to open space. | ||||||||
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