Abstract
Fluid inclusions entrapped in mineral cements and healed microfractures represent an important source of information on the ambient environment during mineral precipitation. This includes minerals precipitated in relatively low-temperature, surficial environments, which have been identified as targets for exploration for life on the Martian surface. As inclusion fluids are sealed from alteration, they preserve a record of the environment at a time when water was present. The most direct value of inclusions would be in biomolecular signatures in aqueous fluids, or physical remains of micro-organisms held in the fluids. High-resolution sensing techniques for organic molecules could analyse inclusion fluids released in situ on Mars or from returned samples.
Original language | English |
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Pages (from-to) | 395-398 |
Number of pages | 4 |
Journal | European Space Agency, (Special Publication) ESA SP |
Issue number | 518 |
Publication status | Published - 1 Sep 2002 |
Event | Proceedings of the Second European Workshop on Exo-Astrobiology - Graz, Austria Duration: 16 Sep 2002 → 19 Sep 2002 |