“…There are three different choices in this context, namely: (a) remote spectrometric analyses from spacecrafts with, for example, miniaturized X-ray spectrometers [20] or miniaturized mass spectrometers for the analysis of cosmic dust [21]; (b) analyses implemented by robots operating on the surface of other planets (e.g. to find traces of water in Mars [22], by using laser ionizationmass spectrometers [23]); or (c) monitoring of the inner and outer atmospheres of spacecrafts [ 24,25]. 3.…”