Fluid inclusions are a common feature of minerals. When a mineral grows in the presence of a fluid phase, some of the fluid may be trapped as imperfections in the growing crystal to form fluid inclusions. Alternatively, tiny blebs of fluid can become trapped in healed fractures within a crystal. These inclusions normally range in size from <5 m to >100 m and are usually only visible in detail by microscopic study and in transparent minerals like quartz the inclusions visible in naked eye, but they are rare. Roedder (1984) and some other workers use the term fluid inclusion to describe only those inclusions, that have trapped a fluid and have remained in the fluid state during cooling to ambient temperatures. The broader and more modern approach that will be followed here is to use the term 'fluid inclusion' to refer to any inclusion that trapped a phase that was a fluid at the temperature and pressure of formation, regardless of the phase state of the inclusion as observed at laboratory conditions.
The minerals in which fluid inclusions can be observed are theoretically, all minerals deposited from the fluids. But there are certain minerals which will be opaque to the visible range of the light. Thus only minerals that are transparent to the visible range of light can be used to see the fluid inclusions. Mostly inclusions are studied in quartz, fluorite, halite, calcite, apatite, dolomite, sphalerite, barite, topaz and cassiterite and even in some are metamorphic minerals like garnet and cordierite.
Most ore minerals like sphalerite, cassiterite, wolframite and sulphide minerals like pyrite, molybdenite, stibnite are opaque under visible light, but actually they are transparent under near-infrared light. The use of infrared microscopy for microthermometric analyses of fluid inclusions in ore minerals was introduced by Campbell et al. (1984) and later subsequent studies were carried out by Campbell and Robinson-Cook (1987). Such studies of fluid inclusions in opaque ore minerals were used to obtain reliable information about depositional conditions of ore bearing fluids (Rosière and Rios, 2004; Ni, P. et al., 2008; 2015).